Live coverage: Veteran three-man crew docks with space station – Spaceflight Now


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Live coverage: Veteran three-man crew docks with space station
Spaceflight Now
The Soyuz MS-05 spacecraft has docked to the Poisk module of the space station, delivering Russian commander Sergey Ryazanskiy, NASA flight engineer Randy Bresnik and European Space Agency astronaut Paolo Nespoli to the complex after a six-hour, ...
ISS crew size increases to 6 with Soyuz MS-05 dockingSpaceFlight Insider
Soyuz rocket carries 3-man crew to space stationCBS News
Three-man crew reaches space station as US boosts researchReuters
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Live coverage: Veteran three-man crew docks with space station - Spaceflight Now

Musk: Falcon Heavy could fly as early as this fall – SpaceFlight Insider

Jason Rhian

July 30th, 2017

SpaceX Falcon Heavy lifts off from Kennedy Space Centers Launch Complex 39A. Image Credit: SpaceX

CAPE CANAVERAL, Fla. On an Instagram post, SpaceXs CEO and Founder has expressed less optimism than his companys fans about the success of the Heavy version of the first flight of his companys Falcon Heavy rocket. Elon Musks comments highlight his knowledge concerning the success rates that most launch vehicles encounter on their maiden flight, as well as the fact that the FH has 27 Merlin 1D engines in the rockets first stage alone.

According to Reuters Irene Klotz, that test flight was supposed to have flown in 2013 and Musk has noted numerous times that it is proving to be complex, even suggesting that it perhaps should have been called the Falcon 27 instead. Nevertheless, supporters of the company have attempted to argue that the Falcon Heavys first flight has not been delayed, that it has not flown because the launch vehicle lacked a paying customer, and the fact that the rockets first flight would need to be a test flight, as was the case with the Falcon 1 and Falcon 9.

When it does fly, the Falcon Heavy will be the most powerful rocket currently in operation (by a factor of two according to Space Coast Daily). However, at present, it is currently in the same classification as NASAs Space Launch System unproven.

The former Soviet Union had tried for three years (and four launches) to have their N1 rocket enable their lunar ambitions only to have each mission end in an explosion. Like the N1 (which had 30 NK-15 engines in its first stage), the Falcon Heavy has a large number of engines in its first stage.

Supporters of the Hawthorne, California-based companys innovative efforts have suggested that SLS should be canceled in favor of the Falcon Heavy often citing the rockets cost (possibly as low as $90 million per flight) and capabilities despite the fact that the rocket has never flown. Much like the Falcon 9, the expense of sending payloads to orbit is often the deciding factor for customers.

If SpaceX can bring the Falcon Heavy into service, it will eclipse the current highest capacity rocket currently in operation United Launch Alliances Delta IV Heavy. The Delta IV Heavy has one factor strongly in its favor a simpler design. Whereas the Falcon Heavy employs 27 engines in its first stage, the Delta Heavy has only oneAerojet Rocketdyne RS-68A engine in each of its three common booster cores.

However, should the Falcon Heavy enter into rotation at Cape Canaveral in Florida and Vandenberg Air Force Base in California, it will be a tough act to follow.

With the ability to send140,660 pounds (63,800kg) to orbit compared to the Delta Heavys 62,540 pounds (28,370kg), the Falcon Heavy will be able to send more to orbit and at a lower cost (estimates have placed the cost of the Falcon Heavy at $90 million compared to the Delta Heavys $375 million) than their competitor.

If everything continues to go as planned, the Falcon Heavy will be launched from SpaceXs facilities at Kennedy Space Centers Launch Complex 39A with the Falcon 9 lifting off from Cape Canaveral Air Force Stations Space Launch Complex 40.

Video courtesy of SpaceX

Tagged: Cape Canaveral Air Force Station Elon Musk Falcon Heavy Kennedy Space Center Lead Stories SpaceX

Jason Rhian spent several years honing his skills with internships at NASA, the National Space Society and other organizations. He has provided content for outlets such as: Aviation Week & Space Technology, Space.com, The Mars Society and Universe Today.

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Musk: Falcon Heavy could fly as early as this fall - SpaceFlight Insider

Anticipating upgraded spaceships, SpaceX builds final first-generation Dragon cargo craft – Spaceflight Now

File photo of a Dragon spacecraft at SpaceXs headquarters in Hawthorne, California. Credit: SpaceX

The Dragon supply ship set for liftoff from Florida next month was the last of SpaceXs first-generation cargo capsules off the production line, meaning future logistics deliveries to the International Space Station will fly on recycled spacecraft until a new Dragon variant is ready.

SpaceX launched a reused Dragon cargo craft on its last commercial supply shipment to the space station in June, and officials said then that the next Dragon mission now scheduled for launch next month will use a newly-manufactured capsule. Plans for subsequent resupply missions were still under review, NASA and SpaceX officials said at the time.

But a presentation to the NASA Advisory Councils human exploration and operations committee Monday by Sam Scimemi, director of the space station program at NASA Headquarters, suggested SpaceXs next Dragon spacecraft would be the last one to be built.

SpaceX clarified Friday that the company expects the upcoming automated logistics mission will be the last to fly with a newly-manufactured Dragon 1 spacecraft. SpaceX has a contract with NASA for 20 commercial resupply launches through 2019, followed by at least six more Dragon cargo missions through 2024 under a separate follow-on agreement.

NASA has also contracted with Orbital ATK and Sierra Nevada Corp. for the stations cargo needs.

Another iteration of the Dragon spaceship, with a different shape and other significant changes, is under development at SpaceX. NASA confirmed last week that the first unpiloted orbital demonstration flight of the Dragon 2, also known as the Crew Dragon in its human-rated configuration, would slip from late 2017 until at least February 2018.

A second test flight scheduled for June 2018 will carry two astronauts to the space station and back to Earth. NASA and SpaceX intend to have the Crew Dragon ready and certified for regular crew rotations to and from the orbiting research complex by the end of next year.

Meanwhile, a simpler version of the Dragon 2 capsule will also take over SpaceXs cargo delivery duties. Officials have not identified when the resupply runs will switch to the new spacecraft type, but the changeover could happen when SpaceX begins flying missions under its second cargo contract in late 2019 or early 2020, or sooner.

SpaceX chief executive Elon Musk said July 19 that there was little difference between the cost of a new Dragon capsule and the cost to refurbish the Dragon that launched to the space station June 3 and returned to Earth a month later.

The SpaceX internal accounting said that it cost us almost as much as building a Dragon 1 from scratch, but I expect our internal accounting wasnt counting certain things, Musk said at the International Space Station Research and Development Conference in Washington.

The Dragon that flew the last mission to the space station spent 34 days in orbit in 2014. Engineers replaced the ships heat shield and batteries, which were vulnerable to salt water damage when it splashed down in the Pacific Ocean.But the hull, thrusters, harnessing, propellant tanks, and some avionics boxes were original, officials said.

This had a lot of rework, Musk said. The next one, we think theres a decent shot of maybe being 50 percent of the cost of a new one.

SpaceX hopes to launch the its next supply ship on a Falcon 9 rocket from NASAs Kennedy Space Center in Florida as soon as Aug. 13 or 14, ahead of an Aug. 17 spacewalk by Russian cosmonauts that will release several small satellites from the space station. The deployments will prevent the Dragon cargo craft from approaching the space station for several days as a safety precaution until station managers have good tracking of the Russian satellites.

Technicians at Cape Canaveral will load more than 7,000 pounds (about 3,300 kilograms) of hardware, crew provisions and experiments into the Dragon spacecraft in the coming weeks, including a NASA-funded instrument to investigate the origins of cosmic rays.

If the SpaceX launch is not off the ground by the middle of August, it could be grounded several days until officials ensure the Russian satellites are well away from the station. Two other launches from Cape Canaveral in the second half of August an Atlas 5 flight set for around Aug. 20 and a Minotaur 4 rocket mission Aug. 25 could complicate SpaceXs scheduling in the event of a delay.

The mid-August launch will be the 12th time SpaceX has sent equipment and experiments to the space station since regular Dragon resupply flights began in October 2012. Counting two Dragon test flights in December 2010 and May 2012, the reused capsule that launched twice, and next months mission, SpaceX built 13 capsules based on the first-generation Dragon design.

After the upcoming cargo flight, SpaceXs next Dragon mission is scheduled for launch in November with a previously-flown capsule.

SpaceX will continue building unpressurized trunk modules for space station deliveries. Those sections, which hold solar panels and carry large external experiment payloads, are disposed at the end of each Dragon mission to burn up in the atmosphere.

Musk confirmed SpaceX will eventually use the Dragon 2 spacecraft for all crew and cargo missions to the space station.

The only thing cargo Dragon wont have is the launch escape system, Musk said, noting that the capsule will still be able to separate from a failing rocket. I think, most likely, even cargo Dragon 2 will be able to survive a booster anomaly. It will have everything the crew Dragon 2 has, except the (abort) thrusters, but I think, in most cases actually, it will be able to survive re-entry and keep the cargo safe.

Dragon 2 being used for both cargo and crew allows us to iterate with just a little more risk on the cargo version and prove it out before theres crew on-board, Musk said.

The SpaceX founder said the next-generation Dragon will not have the capability for propulsive returns to land as originally intended, instead returning to splashdowns at sea.

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Follow Stephen Clark on Twitter: @StephenClark1.

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Anticipating upgraded spaceships, SpaceX builds final first-generation Dragon cargo craft - Spaceflight Now

Soyuz rockets into space with three bound for station – Spaceflight Now

STORY WRITTEN FORCBS NEWS& USED WITH PERMISSION

A Russian Soyuz rocket blasted off from Kazakhstan Friday, boosting a three-man crew into orbit for a six-hour flight to the International Space Station.

The workhorse Soyuz rocket thundered to life at 11:41 a.m. EDT (GMT-4; 9:41 p.m. local time) and streaked away from the same pad at the Baikonur Cosmodrome that was used to launch Sputnik 60 years ago and Yuri Gagarin, the first man in space, in 1961.

Trailing a brilliant plume of exhaust visible for miles around in the clear early evening sky, the Soyuz booster climbed away directly into the plane of the space stations orbit, kicking off a six-hour rendezvous.

Live video from inside the Soyuz MS-05 spacecraft showed commander Sergey Ryazanskiy, flanked on his left by NASA flight engineer Randy Bresnik and on the right by Italian astronaut Paolo Nespoli, calmly monitoring cockpit displays as the spacecraft accelerated toward space.

Ryazanskiy, with a doctorate in biomedicine, is the first scientist-cosmonaut to serve as a Soyuz commander. He spent 166 days aboard the station in 2013-14 and commanded one of three international crews during a 500-day simulated Mars mission in 2009.

Bresnik, an F/A-18 pilot with more than 6,000 hours flying time in high-performance aircraft, spent 10 days in space as a shuttle crew member during a 2009 space station assembly mission. Nespoli, making his third spaceflight, has logged 174 days in orbit.

If all goes well, Ryazanskiy and Bresnik will oversee an automated four-orbit rendezvous with the space station, moving in for docking at the Earth-facing Rassvet module around 6 p.m.

After verifying a tight, airtight seal, hatches will be opened and the Soyuz crew will be welcomed aboard by Expedition 52 commander Fyodor Yurchikhin, flight engineer Jack Fischer and Peggy Whitson, NASAs most experienced astronaut.

Yurchikhin, Fischer and Whitson have had the station to themselves since June 2 when Soyuz MS-03 commander Oleg Novitskiy and European Space Agency astronaut Thomas Pesquet returned to Earth.

The expanded Expedition 52 crew will include four astronauts assigned to the U.S. segment of the station Fischer, Whitson, Bresnik and Nespoli and two in the Russian segment Yurchikhin and Ryazanskiy.

The station crew normally is evenly split between the Russians and the U.S. segment, which includes astronauts representing NASA, ESA, Japan and Canada. But the Russian space agency Roscosmos recently decided to reduce its crew complement to save money and that opened up additional Soyuz seats for USOS U.S. orbital segment astronauts.

With the arrival of the Soyuz MS-05 crew, an additional USOS crew member will be available to carry out research.

The big thing is were going to have four USOS crew members, and with over 330 possible experiments, of which 85 are new to the space station, theres a ton of science for us to do, Bresnik said in a pre-launch news conference.

And with that extra crew member, were going to have a lot more opportunity to not only do the science, were also going to have the opportunity to do repairs on the station. So we think the productivity of this huge laboratory will really go up quite a bit having a fourth crew member.

Ryazanskiy, who will join Yurchikhin for a spacewalk Aug. 17, said having only two Russian crew members aboard will require some Russian research to be carried out in their spare time, but he does not anticipate any problems.

We will be really busy because there will only be two of us, he said. I have a lot of science that is now going on the task list so some experiments will be done in my free time aboard the station. But overall, for life support and technical issues, two Russian crew members will be enough.

Yurchikhin, Fischer and Whitson are scheduled to return to Earth Sept. 3. They will be replaced 10 days later by Soyuz MS-06 commander Alexander Misurkin, NASA flight engineer Mark Vande Hei and astronaut Joe Acaba. It will be the second expedition with four USOS crew members.

Ryazanskiy, Bresnik and Nespoli will return to Earth Dec. 14. Between now and then, the overlapping station crews will carry out multiple spacewalks, help with the departure of one Soyuz, the arrival of another and unload four cargo ships, one Russian Progress, two SpaceX Dragons and one Orbital ATK Cygnus.

And throughout it all, the station crew will carry out a full slate of scientific research.

I am excited about having a full complement of people up here who can really utilize this amazing laboratory, Fischer said in a recent interview with CBS News.

This will be the first time where we have four USOS, were have three Americans and an Italian, Paolo, working on the U.S. segment on science. Four people. Thats crazy talk! Im super excited about how much science were going to be able to get done with all four people. So, overall, its awesome, I cannot wait for the discoveries that we make together.

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Soyuz rockets into space with three bound for station - Spaceflight Now

Musk aims for November debut of Falcon Heavy – Spaceflight Now

Artists concept of SpaceXs Falcon Heavy rocket in flight. Credit: SpaceX

SpaceX aims to launch the first Falcon Heavy rocket in November, company chief Elon Musk said Thursday, the latest in a series of schedule targets for the heavy-lift launchers delayed debut.

Musk shared the updated schedule on social media late Thursday, a week after hetempered expectations for the Falcon Heavys maiden flight in remarks at an industry conference in Washington.

A post on social media earlier this month from a passerby touring NASAs Kennedy Space Center in Florida apparently showed all three of the Falcon Heavys first stage boosters inside SpaceXs hangar near launch pad 39A, where the rocket will blast off on its inaugural flight.

The images are a sign of visible progress on the Falcon Heavy.

Attach mechanisms visible on the Falcon Heavys central core will connect two side-mounted boosters, each based on SpaceXs Falcon 9 rocket first stage.

The three rockets bolted together will generate 5.1 million pounds of thrust with 27 Merlin 1D main engines, making the Falcon Heavy the most powerful present-day launcher in the world once it flies.

The Falcon Heavy will weigh more than 3.1 million pounds (1.4 million kilograms) fully loaded with kerosene and liquid oxygen propellants and stand more than 229 feet (70 meters) tall.

The nice thing is when you fully optimize it, its about two-and-a-half times the payload capability of a Falcon 9, Musk said. Its well over 100,000 pounds to LEO (low Earth orbit) of payload capability, 50 tons. It can even get up a little higher than that if optimized.

If the demo mission gets off the ground successfully by the end of this year, two more Falcon Heavy flights are on the books in the first half of 2018, both from Florida. While the inaugural launch will not carry a customer payload, the Falcon Heavy missions next year will deploy satellites for commercial companies and the U.S. military.

Musk first announced plans for the Falcon Heavy in April 2011, when he suggested the huge rocket could make its first flight by the end of 2013. Those plans were delayed multiple times, and SpaceX officials said the company temporarily sidelined the Falcon Heavy project in the wake of a Falcon 9 launch failure in 2015.

The Falcon Heavy will be able to loft the worlds heaviest commercial communications satellites, the U.S. military largest national security spacecraft, and send the companys Dragon crew capsule on flights around the moon, according to Musk.

SpaceX also planned to launch Red Dragon capsules on one-way flights to land on Mars aboard Falcon Heavy rockets, but the Red Dragon program, at least in its current incarnation, is in doubt after a design change on the next-generation Dragon spacecraft to eliminate the ships propulsive landing capability.

The Falcon Heavy rockets development delays forced some customers to switch their satellites to SpaceX competitors. Two satellites owned by ViaSat and Inmarsat were originally slated to launch on Falcon Heavy rockets, but those telecom operators opted to swap their SpaceX rides for launches on European Ariane 5 rockets operated by Arianespace.

SpaceX aims to recover the Falcon Heavys two side boosters, which flew on Falcon 9 rocket flights last year and were modified with added nose cones, at a landing site at Cape Canaveral after the maiden launch. The company manufactured the center core new, giving it a strengthened structure, attach points, and other upgrades that make it different than a basic Falcon 9 booster.

Musk last week said the Falcon Heavy turned out to be more difficult than originally expected.

Theres a lot of risk associated with Falcon Heavy, a real good chance that that vehicle does not make it to orbit, Musk said, referring to the inaugural test launch. I want to make sure to set expectations accordingly. I hope it makes it far enough beyond the pad so that it does not cause pad damage. I would consider even that a win, to be honest.

Read our earlier story for more on Musks comments last week.

Repairs to SpaceXs launch pad 40 at Cape Canaveral in the aftermath of a rocket explosion there last year will help determine when the Falcon Heavy will take off for the first time. SpaceX plans to shift its Florida launch operations to pad 40 once it is available, allowing construction to resume at pad 39A to ready it for the Falcon Heavy.

In the meantime, all of SpaceXs Falcon 9 launches are departing from pad 39A, giving ground teams little time to modify the facility for the bigger booster.

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Follow Stephen Clark on Twitter: @StephenClark1.

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Musk aims for November debut of Falcon Heavy - Spaceflight Now

As dusk sets on NASA’s Cassini mission, Saturn still providing surprises – SpaceFlight Insider

Ocean McIntyre

July 28th, 2017

This false-color view from NASAs Cassini spacecraft gazes toward the rings beyond Saturns sunlit horizon, where a thin haze can be seen along the limb. Image & Caption Credit: NASA / JPL-Caltech / Space Science Institute

After twenty years in space and thirteen years directly observing Saturn and its system of hypnotic rings and moons, the Cassini spacecraft is continuing to tease out tantalizing data from the mysterious ringed beauty about every six days.

Currently in its sixteenth of twenty-two Grand Finale orbits that will culminate in the spacecrafts plunge into Saturns atmosphere on September 15, 2017, Cassini keeps sending back consistently stunning images as well as jaw dropping data.

Cassini is performing beautifully in the final leg of its long journey, said Earl Maize, Cassini Project Scientist at NASAs Jet Propulsion Laboratory (JPL), Pasadena, California. Its observations continue to surprise and delight as we squeeze out every last bit of science that we can get.

The Imaging Science Subsystem (ISS) was given priority to observe Titan for two periods, each lasting several hours, to view the atmosphere as well as the surface, and in hopes of observing formation and changes to clouds on Titan. In addition to the ISS, the Composite Infrared Spectrometer (CIRS) and the Visible and Infrared Mapping Spectrometer (VIMS) were active in this pursuit.

As Cassini approached and swooped past Saturn, the Ultraviolet Imaging Spectrograph (UVIS) observed both the northern and southern auroral zones, with the southern zone in darkness and the northern in sunlight, and a stunning image mosaic of this pass was made.

When Cassini began its Grand Finale orbits back in April 2017, one of the hopes of scientists studying the rings was to be able to closely observe the ring particles and measure their mass to get a better handle on their age and composition.

On 29 June, during the third of four of Cassinis close approaches to the innermost D-ring, Cassinis scientists and engineers decided to take a chance and turn the spacecraft so that the cosmic dust analyzer (CDA) instrument could directly sample the nanometer size particles. This strategic alignment allowed the spacecraft to be able to take a sample of some of the super fine particles as it passed just 3,040 miles (4,890 kilometers) from the inner edge of the D-ring while using the CDA.

Ring science researchers are excited to receive CDA results in coordination with some of the best high-resolution images ever received of the rings, including the C-ring with its bright bands and streaky textured appearance referred to as plateaus.

The central feature in this image, called Plateau P1, is found approximately 47,300 miles (76,200 kilometers) from Saturns center. It is situated amid some undulating structure that characterizes this region of the C ring. None of this structure is well understood. This image, especially the enhanced version (right), reveals three different textures with different kinds of structure. Images & Caption Credit: NASA / JPL-Caltech / Space Science Institute

Unlike geologic plateaus, Saturns ring plateaus arent necessarily higher in elevation, but rather they are an area of higher particle density which appears as brightness. When these regions are compared to the surrounding ring region, the non-plateau areas seem to lack any apparent structure whereas the plateaus are approximately five times denser.

The data we are seeing from Cassinis Grand Finale are every bit as exciting as we hoped, although we are still deep in the process of working out what they are telling us about Saturn and its rings, said Cassini Project Scientist Linda Spilker at JPL.

The new level of detail in the images combined with the results from the CDA data should shed some light on the questions of why and how they were created, and what the makes them different from other regions of the rings.

The central feature in this image, called Plateau P5, is found approximately 52,700 miles (84,800 kilometers) from Saturns center. It is situated amid some undulating structure that characterizes this region of the C ring. None of this structure is well understood. This image, especially the enhanced version (right), reveals that the plateau itself is shot through with elongated streaks. Images & Caption Credit: NASA / JPL-Caltech / Space Science Institute

It wasnt only the rings that received Cassinis attention. The ion and neutral mass spectrometer (INMS) was also able to take samples of the planets exosphere the atmospheres outermost layer just 1,750 miles (2,810 kilometers) above Saturns cloud tops. Cassinis imaging cameras were able to get some of the highest resolution images ever taken of Saturns clouds. These images include two new image mosaics and a movie sequence.

As interesting as all of that is, some of the most intriguing results have come from the gravitational and magnetic field data. When Saturn was first visited by the Voyager probes in 1980 and 1981, they noted that Saturns magnetic tilt was very well aligned with its axial tilt, which made calculating the exact length of a Saturnian sidereal day impossible. Its sidereal day is currently estimated at 10 hours, 47 minutes.

The Cassini spacecraft has been in orbit since 2004. Since that time, it has revolutionized our understanding of the ringed planet. Image Credit: James Vaughan / SpaceFlight Insider

When Cassini arrived 13 years ago, it found much the same thing, but the spacecraft had come prepared with far more sensitive equipment. Not only does Cassini have a more sensitive magnetometer (MAG), it has two the vector/scalar helium magnetometer located at the far end of the 36-foot (11-meter) boom, and the fluxgate magnetometer positioned half-way out along the boom.

Both instruments can measure strength and direction of magnetic fields, but they also have individual abilities as well. The vector/scalar helium magnetometer can also detect the strength of fields alone, whereas the fluxgate magnetometer can detect a range of strength three times greater than the vector/scalar magnetometer.

Why is this important? Because measuring and mapping the magnetic fields on a planet should give you an understanding of how those magnetic fields are generated. However, this is where things get a bit weird on Saturn.

Until now, we believed that electromagnetic fields in planets, called dynamos, were created and sustained by liquid metals surrounding and moving around a solid metal core deep inside of a planet. The greater the planets mass and more movement within the liquid core, the larger and stronger the magnetic field. Our understanding of how the liquid metal core spins is based on the difference in the axial rotation or the tilt of the planet as it spins or rotates in space.

The Earth has a 23.5-degree axial tilt, and Jupiter has an axial tilt of just 3.13 degrees. Saturn, on the other hand, has an axial tilt of less than 0.06 degrees, and that is only an estimate because its the lowest measurement the equipment is capable measuring down to.

The comparison of the gravitational field data and magnetic field data has come back with more than a small number of discrepancies from the expected models. These discrepancies suggest that there is something quite strange going on deep inside of the planet and that Saturns deep atmosphere could be masking how and where the internal magnetic field is being generated.

Everything that we believe thus far suggests that a planet with virtually no axial tilt, such as Saturn, would be incapable of sustaining a dynamo, let alone such a powerful dynamo as it possesses. Is there a link to the magnetic field generation somewhere in the deep narrow atmospheric lanes and zones? Is it generated by an as yet unidentified substance? Are Saturns thread-like convective cells contributing to it?

It will be interesting to see what researchers and scientists are able to piece together based on the data from these next (and last) seven passes. Once Cassini is lost after it plunges into Saturn on September 15, 2017, any additional data to answer these questions could take decades to obtain as there are no new missions currently being planned that extend beyond the orbit of Jupiter.

The Cassini-Huygens mission is a cooperative project of NASA, European Space Agency (ESA), and the Italian Space Agency. NASAs Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the mission for NASAs Science Mission Directorate, Washington. JPL designed, developed, and assembled the Cassini orbiter.

The sounds and colorful spectrogram in this still image and video represent data collected by the Radio and Plasma Wave Science (RPWS) instrument on NASAs Cassini spacecraft, as it crossed through Saturns D ring on May 28, 2017. Image/Audio & Caption Credit: NASA / JPL-Caltech / University of Iowa

Tagged: Cassini Grand Finale Jet Propulsion Laboratory NASA Saturn The Range

A native of the Greater Los Angeles area, Ocean McIntyre's writing is focused primarily on science (STEM and STEAM) education and public outreach. McIntyre is a NASA/JPL Solar System Ambassador as well as holding memberships with The Planetary Society, Los Angeles Astronomical Society, and is a founding member of SafePlaceForSpace.org. McIntyre is currently studying astrophysics and planetary science with additional interests in astrobiology, cosmology and directed energy propulsion technology. With SpaceFlight Insider seeking to expand the amount of science articles it produces, McIntyre was a welcomed addition to our growing team.

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As dusk sets on NASA's Cassini mission, Saturn still providing surprises - SpaceFlight Insider

Go For Launch: Mercury Is A Historically Accurate VR Space Flight Simulator – UploadVR

As a guy that writes a lot about VR on the internet Ive seen and played my fair share of space flight games. From piloting massive ships as I explore the stars in Elite: Dangerous and engaging in epic multiplayer dogfights in EVE: Valkyrie, all the way down to some casual fun on the Gear VR with Anshar Wars 2 or even flying an X-Wing for the first time in the Star Wars Battlefront VR Mission, there is a ton of stuff to do in space if you have a VR headset. But what most of these things lack is a believable sense of realism.

I can hang out with friends aboard an Enterprise-caliber Starship in Star Trek: Bridge Crew, but thats entirely fiction. On the other end of the spectrum games like Go For Launch: Mercury are focused on 100% authentic, historically accurate, simulation.

Created by one amateur programmer named Joe Chisholm, Go For Launch: Mercury aims to be one of the most realistic space flight simulators ever made. Working with data from the NASA history office, the simulation accurately recreates Americas first manned space program down to the finest detail, writes Chisholm in an email to UploadVR. Every last nut, bolt, switch and lever functioning exactly as it did in the original Mercury Spacecraft.

The cockpits are fully interactive with HTC Vive and Oculus Touch motion controllers and you can even explore the cockpits themselves. Chisholm has been working on Go For Launch: Mercury for over two years now and is gearing up to launch the full experience later this year in September.

In the meantime, you can download and play a free demo on Steam, Oculus Home, or Viveport right now to get a taste of what hes building. What do you think of his simulation? Let us know down in the comments below!

Tagged with: flight sim, space flight

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Go For Launch: Mercury Is A Historically Accurate VR Space Flight Simulator - UploadVR

LISA Pathfinder mission terminated – SpaceFlight Insider

Laurel Kornfeld

July 27th, 2017

An artists impression of LISA Pathfinder in space. Image Credit: ESA/ATG medialab

The European Space Agencys (ESA) LISA Pathfinder, a probe that tested technologies for their capability to detect the ripples in space-time known as gravitational waves, has been shut down.

Over a period of 16 months, the spacecraft, a preliminary proof-of-mission project, tested technologies aimed at studying gravitational waves in a follow-up mission, the Laser Interferometer Space Antenna (LISA), scheduled for launch in 2034.

First proposed as part of Albert Einsteins theory of general relativity over a century ago, gravitational waves result from major space events, such as mergers of two black holes or supernova explosions.

Because only some types of gravitational waves can be detected by ground-based observatories, scientists had to create and launch a space-based observatory that would not be vulnerable to phenomena on Earth, such as seismic activity.

Were looking for the universe vibrating from these mergers, these big, big events, said LISA Pathfinder project scientist Paul McNamara in an ESA video about the mission. From the operations to the hardware to the development, its just been a wonderful mission.

Video courtesy of European Space Agency (ESA)

Two gold-platinum cubes, each with a weight of 4.3 pounds (2 kilograms) and a diameter of about 1.8 inches (4.6 centimeters), suspended inside LISA Pathfinder, served as its primary technology. A 1.5-inch (3.8-centimeter) laser measured the distances between the cubes to vary their positions, distance, and orientation.

During its period of operation, LISA Pathfinder had to be held steady to prevent its sensitive motion detector from being influenced by photons coming from the Sun. This was accomplished by thrusters that exerted tiny reactive forces to the probe, keeping it in a near-perfect gravitational orbit.

Keeping the spacecraft stable was so important that two separate systems, one designed by ESA and the other by NASA, were placed and used on board.

We were trying to hold it as stable as the width of a DNA helix. And we went down from there to the width of part of a DNA helix, explained John Ziemer of NASAs Jet Propulsion Laboratory (JPL) and systems lead for the NASA thruster system on the probe.

Known as the Space Technology 7 Disturbance Reduction System (ST7-DRS), the thruster system was developed by the company Busek Co. Inc. with assistance from JPL.

Algorithms developed by NASAs ST7 project were used in conjunction with ESAs commands and input from ESAs sensors to guide LISA Pathfinder during its U.S. operations phase.

While the spacecraft completed its primary mission in the fall of 2016, tests of various algorithms to stabilize it continued into March and April of this year.

The main goal for us was to show we can fly the spacecraft drag-free, Ziemer said. The main force on the spacecraft comes from the Sun, from photons with [an] extremely tiny force that can subtly move the spacecraft.

Engineers hope that the new steady thrusters could eventually replace reaction wheels, currently used to point and rotate spacecraft, on other probes, such as telescopes designed to hunt for exoplanets, he added.

Turned off on Tuesday, July 18, 2017, LISA Pathfinder will remain in a parking orbit, where it will coast while continuing to circle the Sun.Its 2034 successor will be composed of three separate spacecraft positioned in a triangle, with each one 1.55 million miles (2.5 million km) from its partners.

The three LISA probes will use technology much like LISA Pathfinders cubes and will detect gravitational waves by the minute distortion (only one trillionth of a meter) the waves exert on the distances between them.

This illustration shows ESAs (the European Space Agencys) LISA observatory, a multi-spacecraft mission to study gravitational waves expected to launch in 2034. In the mission concept, LISA consists of three spacecraft in a triangular formation spanning millions of kilometers. Test masses in spacecraft on each arm of the formation will be linked together by lasers to detect passing gravitational waves. Credits: Image AEI / Milde Marketing / Exozet; Caption NASA

Tagged: European Space Agency LISA Pathfinder The Range

Laurel Kornfeld is an amateur astronomer and freelance writer from Highland Park, NJ, who enjoys writing about astronomy and planetary science. She studied journalism at Douglass College, Rutgers University, and earned a Graduate Certificate of Science from Swinburne Universitys Astronomy Online program. Her writings have been published online in The Atlantic, Astronomy magazines guest blog section, the UK Space Conference, the 2009 IAU General Assembly newspaper, The Space Reporter, and newsletters of various astronomy clubs. She is a member of the Cranford, NJ-based Amateur Astronomers, Inc. Especially interested in the outer solar system, Laurel gave a brief presentation at the 2008 Great Planet Debate held at the Johns Hopkins University Applied Physics Lab in Laurel, MD.

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LISA Pathfinder mission terminated - SpaceFlight Insider

Launcher for next space station crew in position for liftoff Friday – Spaceflight Now

A Russian Soyuz rocket made a railroad journey Wednesday to its launch pad in Kazakhstan, two days before blastoff with a crew of three spaceflight veterans from the United States, Italy and Russia heading for the International Space Station.

The three-stage rocket departed an assembly building just after sunrise Wednesday on a special rail car for the journey to Launch Pad No. 1, the same mount from which Russian cosmonaut Yuri Gagarin launched on the first piloted space mission in April 1961.

A hydraulic lift raised the Soyuz vertical before swing arms moved into place around the rocket. The launch structure containing the Soyuz booster then rotated to align with the planned launch azimuth.

Fridays liftoff is scheduled for 1541 GMT (11:41 a.m. EDT; 9:41 p.m. Baikonur time). The three-man crew inside the Soyuz MS-05 capsule will head into orbit on a fast-track pursuit of the space station, with docking set for approximately 2200 GMT (6 p.m. EDT) with the research outposts Rassvet module.

Russian cosmonaut Sergey Ryazanskiy, 42, will occupy the Soyuz spacecrafts center seat during Fridays launch and docking. The Soyuz commander, a biochemist with a career in space medicine before his selection as a cosmonaut in 2003, is making his second trip to the space station after spending 166 days in orbit as a flight engineer on the Expedition 37 and 38 crews.

NASA astronaut Randy Bresnik will be the Soyuz MS-05 spaceships board engineer, assisting Ryazanskiy with cockpit duties during the six-hour voyage from liftoff to docking. The 49-year-old retired Marine Corps fighter pilot hails from Santa Monica, California, and logged nearly 11 days in orbit aboard the space shuttle Atlantis on a 2009 mission to the space station.

Bresnik will take command of the stations Expedition 53 crew in September.

European Space Agency flight engineer Paolo Nespoli has 174 days of space experience on two previous missions, including a flight on the shuttle Discovery in 2007 and a long-duration stay on the space station in 2010 and 2011. Nespoli, 60, is a native of Milan and was a special forces operator in the Italian Army before working on several European space projects as an engineer.

The trio will become part of the space stations Expedition 52 and 53 crews, joining commander Fyodor Yurchikhin and flight engineers Peggy Whitson and Jack Fischer on the orbiting complex. Yurchikhin, Whitson and Fischer are due to depart the station and return to Earth on Sept. 2, and three fresh crew members will launch on the next Soyuz spaceship from Baikonur on Sept. 12.

The space station has been flying with a three-person crew since early June, and Fridays docking will boost the outposts occupancy back to six.

Yurchikhin and Ryazanskiy will conduct a spacewalk Aug. 17 to deploy several small satellites and work outside the Russian segment of the station.

A SpaceX Dragon supply ship launched from NASAs Kennedy Space Center in Florida is expected to arrive at the complex the same week, but its liftoff will have to work around the scheduled Russian spacewalk. Station managers want to ensure the satellites released by the Russian spacewalkers are accurately tracked before committing the Dragon cargo freighter to approach the outpost, minimizing the chance for a collision with one of the small craft.

The Dragon capsule is currently set to launch around Aug. 14, but if it slips more than a day or two, the launch aboard a Falcon 9 rocket could be further delayed until officials are sure the small satellites are well away from the space station. A United Launch Alliance Atlas 5 rocket is also expected to launch the same week, potentially complicating bookings on the U.S. Air Forces Eastern Range, which is responsible for flight safety, communications and tracking support for all missions from Cape Canaveral.

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Launcher for next space station crew in position for liftoff Friday - Spaceflight Now

Commercial lunar mission signs up with Atlas 5 for launch – Spaceflight Now

Credit: Astrobotic illustration of lander

CAPE CANAVERAL In a commercial push to return to the Moon while celebrating the 50th anniversary of Apollo 11, Astrobotic Technology Inc. has contracted with United Launch Alliance to use an Atlas 5 rocket to send the Peregrine lander to the lunar surface in 2019.

Astrobotic is thrilled to select a ULA launch vehicle as the means to get Peregrine to the Moon, said John Thornton, CEO of Astrobotic. By launching with ULA, Astrobotic can rest assured our payload customers will ride on a proven launch vehicle with a solid track record of success. Together, our two organizations will honor the past and trail blaze the lunar future.

This initial Peregrine lunar lander will fly 77 pounds (35 kilograms) of customer payloads from six nations either above or below the spacecrafts deck, depending on specific needs.

The autonomous landing will use cameras, guidance computing and five Aerojet Rocketdyne-made hypergolic engines to set the lander down on four shock-absorbing legs.

It will stand 6 feet tall (1.8 meters) and have a diameter of 8 feet (2.5 meters).

Subsequent missions envision scaling up to payload masses of 585 pounds (265 kilograms). Markets range from scientific instruments to placing mementos on the Moon.

Technical credibility and signed deals remain key differentiators for Astrobotic as a lunar delivery company. Our customers and partners know that our 10 years of lunar lander development work has made us the world leader in this market, said Thornton.

The Pittsburgh-based Astrobotic aims to deliver payloads to the Moon for companies, governments, universities, non-profits and individuals.

We are thrilled that Astrobotic has selected ULA to launch the Peregrine Lander to the Moon, said ULA president and CEO, Tory Bruno. The Moon is the next great frontier, but in a different way than when Neil Armstrong landed there. Enabling technologies like those from Astrobotic will allow people to live and work in the space between here and the Moon and take advantage of all those resources in a way that is sustainable.

The Atlas 5 now has added six high-profile launches to its backlog in the past four months three commercial, two Air Force and one for NASA.

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Commercial lunar mission signs up with Atlas 5 for launch - Spaceflight Now

Orion STA undergoing pre-mission testing in Denver – NASASpaceflight.com

July 27, 2017 by Philip Sloss

With all the structural test articles (STA) of the Orion spacecraft at prime contractor Lockheed Martins Space Systems facility in the Denver area, work is underway to qualify the elements for the Exploration Mission-1 (EM-1) and Exploration Mission-2 (EM-2) missions to the Moon. Testing of different combinations of spacecraft hardware in support of EM-1 and EM-2 will continue into 2019. Current status:

This phase of testing will help characterize the dynamic response of the structures and verify that the design meets the required factor of safety.

The Crew Module STA is currently set up in a loads testing fixture in the Structural Test Lab at Lockheed Martin Space Systems Waterton facility in Littleton, Colorado. It was shipped from the Kennedy Space Center (KSC) in Florida on NASAs Super Guppy cargo aircraft in late April to Buckley Air Force Base near Denver.

The Service Module STA made the same Super Guppy flight a couple of months later after the Crew Module Adapter (CMA) and European Service Module (ESM) STAs were mated at Kennedy.

Weve done tests on two of them so far, Dan Qvale, Orion STA Assembly Test and Launch Operations Lead with Lockheed Martin, said during an interview with NASASpaceflight.com.

The crew module is actually in its second test, the first one was whats called proof pressure we went to 150% percent of the maximum expected internal pressure on the vehicle and validated that it structurally survived. That completed [at] Kennedy before we shipped it to Denver. Now that its here, were running qualification loads testing on the crew module primary and secondary structure.

The launch abort system has been assembled and were also in qualification load testing for it now, its having a test run. And then the service module is being set up for the next roughly one month. The spacecraft adapter cone is being installed, the outer walls on the CMA are going on, and then it will go into a modal test of just the service module. And that will begin about a month from now.

The launch abort system (LAS) STA was assembled with inert motors that simulate the weight and center of gravity of the units that will fly on EM-1 and EM-2.

Everything is on the LAS essentially except for the fact that its [an] inert motor. No antennas, but it has fillets, ogives, it has the MATA truss assembly (Motor Adapter Truss Assembly), [and] it has the inert motor. Structurally it has got all those components the ogives actually provide structural load path for the launch abort system as well.

Types of tests:

The STAs will go through different types of tests in the facilities at Waterton, including modal, loads, shock, and acoustic testing.

The tests are broken up into different types of tests and in many cases they are in multiple configurations, Qvale explained. A modal test is a way we take measurements of the vehicle, its dynamic response, and they use those to validate the numeric models that theyre using to simulate and obtain load data analytically.

They need these modal tests in order to measure the stiffness of the combined joints that connect all of the pieces together. And so you tend to run them in configurations your vehicle is going to be in.

In our case, the first one were going to run is the entire stacked vehicle SM (Service Module), CM, and Launch Abort System all connected so thats obviously a flight configuration on the launch pad and during ascent.

We run a modal test on just the CM alone, which is obviously a configuration it will be on reentry. We do a modal test on just the CM and SM, which is the flight configuration it would be in during the mission. We run one on the launch abort system connected to the crew module the LAV (Launch Abort Vehicle) they call it because that would be the configuration you would be in if you experienced an abort event.

So those tests are for the most part being run in order to validate models for all these different configurations that the vehicle will be in or could be in during a mission.

The second category of tests are loads tests.

Those very much fall into the category of one-time only [tests], Qvale added. What were trying to do is apply loads for the major events the vehicle experiences during the mission to simulate those.

You dont just want the vehicle to survive the maximum predicted event, you want some margin on that some assurances that it can survive and theres margin on top of that. And so what we do there is we try to go to 140% of what the maximum expected load is going to be. For example, right now were testing both the launch abort system and the crew module.

Qvale provided a breakdown of what they are trying to qualify/validate in the loads tests for the different elements, such as the all-important for crew safety Launch Abort System (LAS)

The LAS is basically getting two primary things validated, one is the ascent loads so the compression that happens on the vehicle while youre in nominal ascent. The other is abort loads, so qualification of loads that would be applied in the event that an abort actually happens and now instead of compressive loads you have large tension loads.

The crew module has a whole series of nine different events that were trying to simulate, so those include things like main parachute extraction. (Then) were running LAS load cases that represent the landing of the vehicle or the ascent of the vehicle. Weve already run cases where we simulate the jettison of the forward bay cover.

So its basically case-by-case cases where we take the hydraulic jacks, connect up to the vehicle, and then well apply a load thats intended to simulate what the flight-like the loads would be plus 40%. So as long as the design doesnt change on the vehicle, it has been qualified and theres no need to go revisit these.

As Qvale noted, the initial loads test on the CM articles was done at KSC. Both pressure vessels were proof tested to verify that they would hold pressure up to 140% of the maximum pressure load expected during flight. Qvale noted that the flight article, which is still at KSC being fully outfitted for the EM-1 flight, was pressurized to 140%; however, the STA was taken up to 150%.

The third type of tests are shock tests, to evaluate how well parts of the structure handle pyrotechnic events during flight.

[A] typical first flight vehicle would get protoqual shock tested, Qvale explained, which means you cant make the shock more severe, you cant say we did it plus margin. Its as severe as it ends up being. You cant add additional explosives to make it more severe, so instead what you do is you run it twice.

So the way that Orion is going to be protoqual-ing the shock environment (run it twice) is by number one doing it during the EM-1 mission and number two after EM-1 is recovered, were going in and running it a second time. All this needs to happen before we have a manned mission.

However, Qvale added that the program is starting shock testing on the STAs before EM-1. We dont want to wait until the EM-1 mission to start making sure that this will work properly, he said, so what the STA is doing is we are measuring the shock response on the vehicle from these events.

Were going in and say we have an avionics box [that is] near a shock source. Were putting accelerometers on it, and then were running the shock event and were measuring the response at that avionics box and were comparing that with the screening requirements that we gave the avionics box supplier to design and test the box too. And so this should validate that what we gave them to screen this hardware too is enveloped by the measurements that we just took.

So its essentially validation of the capability of the vehicle to survive shock and the combination of these measurements that were doing on the STA that will be compared with screening requirements that our EM-1 hardware was bought to and then ultimately validation by running the event during the mission and then running it a second time on the EM-1 vehicle post-mission.

The Waterton test facilities are used by Lockheed Martin on all the spacecraft they build and have been part of Orion testing since the early days of the spacecraft.

Both the test fixturing as well as the load control and data acquisition are incredibly specialized skills, and youre applying loads that basically take the vehicle to the limit of what its capable of most likely, Qvale explained. [It] doesnt matter if its Orion or another program, you tend to have the same objective there and its such a specialized area that essentially the Structures Test Lab does qualification loads testing for Lockheed Martin [Space Systems], period.

Space Systems brings them their hardware to run these sorts of tests because its impractical that youd have this expertise on a program, even if that program had hundreds of people on it.

At the time of the interview, Qvale noted that the Service Module was waiting for one of the next generation Global Positioning System (GPS) satellites to finish using a test facility before it could move in.

Test setup/configuration:

Structural test hardware for all the spacecraft elements is there to support the test campaign, with mass simulators for some of the larger moving parts, especially on the Service Module assembly.

We got the spacecraft adapter cone at the base, we have a flight-like OMS-E nozzle, we have a structural representation of the ESM so it has mass sims (simulators) instead of avionics boxes, Qvale explained.

On top of the ESM weve got the crew module adapter, so its made up of similar to the flight-like one it has all the longeron trusses, theyre called. The forward and the aft composite walls, the composite outer walls, mass simulators for all the avionics that goes in the avionics ring.

For the four solar arrays, we dont have any flight-like solar arrays theyre all mass simulators. And then for the SM fairings the SAJs (Spacecraft Adapter Jettisoned panels), theyre called theyre essentially flight like, they have the harnessing on them to run the pyro tests.

In addition, an Orion stage adapter STA also recently hitched a ride on the Super Guppy from the Marshall Space Flight Center in Alabama to Colorado. The stage adapter connects the full spacecraft stack to the launch vehicle upper stage.

Qvale explained that the tests are mostly focused on the spacecraft structure.

**Click here for 100s of Orion News Articles**

For the most part it is just the structural elements. The only electronics that we are putting on the vehicle are harnessing thats used to get to all the pyro-mechanisms, but instead of having an avionics box that fires the pyro-mechanisms we basically take test cables, mate up to the flight-like cables, and then use test equipment to fire the pyros. The only electronics per-se, is just the harnessing on the vehicle in order to run the shock tests. Everything else is structural.

One thing that is important is we want to have similar mass in the right locations on the vehicle to run a lot of these tests and so we have mass simulators that basically have the appropriate weight and the appropriate center of gravity so that when they get bolted onto the vehicle from a structural standpoint it looks like a flight vehicle.

Test campaign supports EM-1 and EM-2, runs into 2019:

Development of Orion was divided into three phases, with each culminating in the scheduled test flights: EFT-1, EM-1, and EM-2.

This round of testing in Colorado will support the two Exploration Mission test flights that first cover the major phases of flight to the Moon and back without a crew and then with a crew.

Right now the end of the campaign is [about the] middle of 2019, Qvale explained. One distinction here is that some of these tests are needed before EM-1 launches, but other tests are not needed until EM-2 launches. So the ones that are happening out in the 2019 time-frame are more the tests like of the LAV the crew module with the launch abort system. [Those tests are] trying to gather data in support of if we had either a pad or an ascent abort on EM-2.

Were predicting that all the prerequisites we need to complete before EM-1 launches are going to be completed by the beginning of November 2018, and thus far if you were to look at the start of the campaign, which we typically measure as the day that the crew module got delivered to Kennedy from MAF at this point, halfway through 2017 were essentially on schedule for all three vehicles.

The SM is on schedule, the launch abort system testing is on schedule and the CM is within two to three days of being on schedule.

Different hardware combinations will go through different tests at the Lockheed Martin facilities and the ordering of the test schedule was built based on multiple factors. In general the philosophy of how we ordered the tests, was number one we had to look at do any of these tests produce data that we need soon?, Qvale explained.

One of the first tests well run when we build the entire vehicle up the full stack is an acoustic test. And similar to what I told you about the shock test, this acoustic test is intended to be similar.

Its only intended to take measurements at specific locations and validate requirements that we are having [the] flight boxes screened to, so obviously it would be a really bad day to find out very late in the flow that we never designed and screened the boxes to the values that theyre going to experience. So for example [placing] a test like that early in the flow so that we can validate [the parameters] that all this hardware for EM-1 is getting designed and built around is a good plan.

Qvale added that the other part that determined the flow was that it takes a lot of time to build the vehicle.

For example, when we put the SM fairing on, thats on the order of twenty shifts of work to get it completed. You dont want to take them back off or youre going to have to go back through another twenty shifts worth of labor to reinstall them. So we ordered the flow so that if we build the vehicle one time, like we will be doing this Fall, we will knock out all the tests that need the vehicle in that configuration.

Theres an acoustic test thats stacked, theres a modal test thats stacked, and then we need to disassemble the vehicle to move it from one facility that has the acoustic chamber to another facility where were going to be running the loads testing. So rather than just dismantle the vehicle, we said lets just run the shock test for the launch abort system. Just run the test, blow the pyros, and thats what will separate the launch abort system and now thats how you take it apart.

So we tried to be smart about ordering things so that we got the maximum bang for the buck every time we had to assemble the vehicle.

There are plans to use at least some of the structural test articles after all the testing in Littleton is complete Qvale noted plans to use the crew module STA in a water impact test at NASAs Langley Research Center prior to the EM-2 flight. Given those future plans and the extensive testing that will be done during the test campaign, the health of the hardware will be closely monitored.

Lets go back to the loads test for example. The requirement may be that the vehicle needs to survive 140 percent [of] the limit load. In the case of the crew module, maybe survive means not rupture but it could be bent basically when youre done.

For our purposes that doesnt work because we cant destroy the vehicle we need to use it for the next year and a half. So during these tests, they monitor the health of the vehicle and if we believe were bumping up on the ultimate capability and we could damage it, then we curtail things and say OK, lets put completion of this test back on the shelf.

Well revisit it in a year and say were we close enough did we get to 138 percent and thats good enough? Or do we need to 140 percent and lets put the vehicle back in there and well bend things on it to verify that it doesnt rupture.

Thus far, every single test weve run has essentially gotten to the 140 percent limit load with no adverse effects. So I think well get the majority of these done the first time around and hopefully well end the campaign and the vehicle will have seen some extreme loading, but it will still be completely viable to go use for another mission.

Post EM-1 tests with returning Crew Module:

As noted earlier, the crew module that flies the EM-1 mission will also take part in gathering test data.

When we launch EM-1, the launch abort system isnt coming back, the service module not coming back, the fairings are not coming back the only thing were getting back is the crew module, Qvale said.

The first environmental test data set collected with the EM-1 crew module will occur as it flies the uncrewed mission to lunar orbit and then returns to Earth for entry, descent, and landing.

The reason most spacecraft go through environments testing is to verify that they work after theyre exposed to the environment, so thats acoustics and thermal and shock, he added. In the case of the EM-1 mission, theres one environment that its not going to experience and thats abort.

And so part of what well be doing with this post EM-1 flight testing is not only running the second shock test but exposing the vehicle to abort-level vibration and then validating that oh, by the way, all the mechanisms you need to survive and still operate after that did in fact work.

Part of our plan long term to validate the abort environment is well still have the STA service module and the STA launch abort system and the STA service module fairings. Were going to take all those things, assemble the vehicle with the EM-1 post-flight vehicle, and were going to go back and run these shock events a second time.

(Images: NASA, Lockheed Martin and L2 artist Nathan Koga The full gallery of Nathans (SpaceX Dragon to MCT, SLS, Commercial Crew and more) L2 images can be *found here*))

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Orion STA undergoing pre-mission testing in Denver - NASASpaceflight.com

Mars 160: 6-person crew arrives at arctic station – SpaceFlight Insider

Paul Knightly

July 22nd, 2017

Jonathan Clarke and Anastasiya Stepanova stand next to the Mars Society flag at the Flashline Mars Arctic Research Station. The second phase of the Mars 160 mission began its Mars mission simulation on July 20, 2017. Photo Credit: Mars Society

The second phase of the Mars Societys Mars 160 mission began at the end of June 2017 in the Canadian high arctic. A six-person crew is staying at the organizations Flashline Mars Arctic Research Station (FMARS) for several weeks. However, due to inclement weather, the crew was unable to make it to FMARS until July 17.

The six-person crew will be living under simulated Mars mission constraints for 30 days at FMARS located on the rim of the Haughton Impact Crater on Devon Island in Nunavut, Canada. The arctic mission represents the second half of Mars 160 after the first half concluded in December 2016 at the Mars Desert Research Station (MDRS) in Utah.

The primary goal of Mars 160 is to conduct two nearly identical field analog studies to determine how mission location impacts science return. As space agencies and organizations around the world are setting goals of sending humans to Mars, the metrics and methods used for crew selection and training on Earth increase in importance. Mars 160 also seeks to perform detailed field studies to answer questions about the geology and biology of these unique desert and high arctic environments.

The six-person Mars 160 crew arrives at the Flashline Mars Arctic Research Station on July 17, 2017. From left to right: Yusuke Marakami, Paul Knightly, Anastasiya Stepanova, Anushree Srivastava, Alexandre Mangeot, and Jonathan Clarke. Photo Credit: Mars Society

The location for FMARS was selected for its similarities to the surface of the Red Planet in terms of its analogous geology as well as its relative isolation. Situated on the rim of a well-preserved 39-million-year-old impact crater, periglacial processes near the arctic station are similar to those that have been observed on the Martian surface.

Daily temperatures during the arctic summer hover right around the freezing point of water, which would be considered a warm day at the Martian equator. Its remote location in the arctic has made it well-suited to test the effects of isolation on the 13 crews it has hosted over the last 17 years.

The Mars 160 arctic crew consists of six members representing six nationalities:

The second phase of Mars 160 is being coordinated by two principal investigators:

After performing a necessary refit of the station, the crew entered into simulation (or sim) conditions July 20. That, in part, requires crew members to wear simulated space suits while conducting field science activities. Additional simulation constraints placed on the crew will include limiting communications to the outside world.The Mars 160 mission is expected to run through the middle of August.

For more information and regular updates on the Mars 160 mission, visit http://mars160.marssociety.org/. Additionally, you can follow the mission on Twitter: @MDRSUpdates.

Paul Knightly is serving as a crew geologist for Mars 160 and is also writing for Spaceflight Insider.

Tagged: Flashline Mars Arctic Research Station Mars Mars 160 Mars Society The Range

Paul is currently a graduate student in Space and Planetary Sciences at the University of Akransas in Fayetteville. He grew up in the Kansas City area and developed an interest in space at a young age at the start of the twin Mars Exploration Rover missions in 2003. He began his studies in aerospace engineering before switching over to geology at Wichita State University where he earned a Bachelor of Science in 2013. After working as an environmental geologist for a civil engineering firm, he began his graduate studies in 2016 and is actively working towards a PhD that will focus on the surficial processes of Mars. He also participated in a 2-week simluation at The Mars Society's Mars Desert Research Station in 2014 and remains involved in analogue mission studies today. Paul has been interested in science outreach and communication over the years which in the past included maintaining a personal blog on space exploration from high school through his undergraduate career and in recent years he has given talks at schools and other organizations over the topics of geology and space. He is excited to bring his experience as a geologist and scientist to the Spaceflight Insider team writing primarily on space science topics.

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Mars 160: 6-person crew arrives at arctic station - SpaceFlight Insider

Videos: Atlas 5 rocket assembled to launch NASA’s TDRS-M bird … – Spaceflight Now

The United Launch Alliance Atlas 5 rocket that will boost NASAs latest communications relay satellite into space is targeting an Aug. 20 liftoff at 7:56 a.m. EDT (1156 GMT).

The Tracking and Data Relay satellite-M, or TDRS-M, will be carried aloft from Complex 41 at Cape Canaveral Air Force Station in Florida, reaching a customized high-perigee geosynchronous transfer orbit nearly two hours after launch.

The mission was delayed from Aug. 3 after a crane incident damaged the crafts Omni antenna in the cleanroom, requiring replacement.

The spacecraft will act like a relay station 22,300 miles above Earth to receive telemetry, voice, video and scientific data from lower orbiting platforms like the International Space Station and Hubble Space Telescope and beam the signals to a central ground hub.

The satellite will become the 12th TDRS placed in space since 1983 and extend the constellation well into the 2020s, providing near continuous connectivity to spacecraft that would otherwise be in range of ground stations 15 percent of each orbit.

The two stages of the Atlas 5 rocket arrived by sea on June 26, sailing into Port Canaveral from the manufacturing plant in Decatur, Alabama, aboard the Delta Mariner cargo ship.

On Wednesday, July 12, United Launch Alliance workers began stacking the launch vehicle, designated AV-074, by erecting the first stage aboard the mobile launch platform parked inside the VIF.

The combined interstage, Centaur upper stage and boattail of the fairing, all pre-integrated together off-site, was hoisted atop the first stage on July 13.

The 191-foot-tall rocket will be wheeled to the pad on Aug. 18 at 9 a.m.

Video courtesy of NASA-KSC TV

Arrival

First stage

Centaur

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Videos: Atlas 5 rocket assembled to launch NASA's TDRS-M bird ... - Spaceflight Now

Newly developed Nanotube Technology could revolutionize spaceflight – SpaceFlight Insider

Michael Cole

July 26th, 2017

A carbon nanotube Composite Overwrap Pressure Vessel (COPV) flew in May 2017 as part of the SubTec-7 mission using a 56-foot (17-meter) tall Black Brant IX rocket launched from NASAs Wallops Flight Facility in Virginia. Shown here is the SubTec7 payload undergoing final testing and evaluation at Wallops Flight Facility. Photo Credit: Berit Bland / NASA

A cold-gas thruster system, partially made from carbon nanotube material, was recently tested aboard a Black Brant IX suborbital sounding rocket, which was launchedon May 16, 2017, at 5:45 a.m. EDT (09:45 GMT) from NASAs Wallops Flight Facility in Virginia. Part of the thruster system was a Composite Overwrapped Pressure Vessel (COPV).

A Black Brant IX sounding rocket carrying SubTec-7 leaves the launch pad at NASAs Wallops Flight Facility. Photo Credit: Chris Perry / NASA

The COPV is an aluminum tank that is wrapped with a composite material to strengthen the tanks ability to hold a fluid or gas under pressure. In the recent test, the overwrap material was a newly developed carbon nanotube yarn that has 200 times the strength and five times the elasticity of steel.

We picked the COPV because the design properties require good tensile strength, Michael Meador, Program Element Manager for Lightweight Materials and Manufacturing at NASA Glenn Research Center in Cleveland, Ohio, told SpaceFlight Insider. But you could think about using these nanotube yarns in other structural components.

Meadors group did trade studies at NASAs Langley Research Center that looked at incorporating nanotube materials with lower structural densities into a cryotank for a notional launch vehicle.

Meador said: What we found out from those trade studies was that if you could reduce the density of the structural material by 25 percent or so, you could reduce the mass of the launch vehicle by 30 percent. So that is a real game-changer. We cant think about any other single technology that would have that much of an impact.

The nanotube fiber yarn used as the overwrap for the COPV in the test was manufactured by a company called Nanocomp Technologies, Inc., in Merrimack, New Hampshire. The company had developed it originally for use in lightweight data cables. Their initial emphasis was on the electrical properties of the yarn, so it was not very strong.

Since then, in collaboration with NASA, Nanocomp has modified their process for making this material. The yarn now has mechanical properties on a per weight basis that are comparable to or even a little bit better than carbon fiber.

Meador said: Our idea in this project was to work with Nanocomp to increase the tensile properties of the fiber, and [] develop techniques to incorporate this into composites.

Meadors project is part of the Game-Changing New Developments program at NASA. Developing a nanotube fiber that can reliably perform its function within the systems of a launch vehicle, while reducing the weight of that launch vehicle by 30 percent, is indeed a game-changer.

Game-changing program is all about maturing technologies and demonstrating them and their suitability for use in a NASA mission, Meador said. That usually involves making hardware, and it usually involves a flight test. We selected the COPV because the tensile properties of the fiber are particularly important for that component. And then we worked with Wallops to design an experiment where we could demonstrate the use of the COPV in a cold gas thruster system. We basically pressurized the COPV with argon and used it to make two maneuvers for the flight test. One was to wiggle the payload back and forth a little bit, and the second one was to spin the payload up prior to descent. They always do that to improve the aerodynamics.

The COPV on the sounding rocket test performed exactly as was expected. The payload was recovered, but Meador and his group have not received the COPV back yet. They intend to do some post-test analysis on it to see if the structural integrity has changed as a result of the flight test.

LEFT: A demonstration flight article is wound with carbon nanotube composites. RIGHT: COPV tank inside the sounding rocket. Photos Credit: NASA

This new carbon nanotube technology could potentially reduce the weight of a launch vehicle by 30 percent. But what, exactly, are carbon nanotubes?

First, one must understand that carbon nanotubes get their strength from the extremely strong bond between carbon atoms.

When you get down to a scale of 1 to 100 nanometers, conventional physics breaks down, and that gives rise to new phenomena, Meador explained. With carbon nanotubes, the aspect ratio, the length divided by the width of the tube, is quite large, and that means it makes a great reinforcement for things like plastics and other materials.

The nanotubes are made in a heated tube furnace by injecting a catalyst and a special mix of gases full of carbon atoms. What they generate is something that looks like black smoke. It is called a nanotube aerogel. That aerogel can be deposited onto a rotating drum to make a nonwoven fabric, or it can be grabbed and twisted and pulled onto a spindle to make a yarn out of it. The yarn is then further manipulated to make it into the material that was used to wrap around the pressure vessel in the recent test.

The nanotube yarn, then, is simply a million or so nanotubes with no binder between them. The yarn is all nanotube in the fiber. The only thing holding the fiber together are twists between the individual nanotubes interlocking between one another.

We got interested in this technology initially in 2000, Emilie Siochi, Research Materials Engineer at NASAs Langley Research Center in Hampton, Virginia, told SpaceFlight Insider. The reason is we thought there were data showing that the mechanical properties of carbon nanotubes far exceed those that are typically used for structural applications in aerospace. Especially for space exploration, we care about mass reduction. The initial analysis of how much mass we could save in large structures like launch vehicles [was] based on what we knew about the properties of carbon nanotubes at that time.

LEFT: Shown here is a Composite Overwrapped Pressure Vessel, or COPV, in a test setup. The aluminum vessel was pressurized to test the overwrapped carbon nanotube yarns ability to strengthen or reinforce the vessel against the internal pressure forces. A number of these burst-tests were conducted to prepare the newly developed carbon nanotube yarn and the COPV for its launch test aboard a sounding rocket launched from NASA Wallops. Photo Credit: NASA Glenn Research Center. RIGHT: A spool of the newly developed carbon nanotube yarn developed in collaboration with NASA by Nanocomp Technologies, Inc. in Merrimack, New Hampshire.Photo Credit: Nanocomp Technologies, Inc.

Siochi and others at Langley did a series of analyses on how much the mechanical properties of the nanotubes would have to be improved in order to use them in spaceflight applications. The analysis told them the nanotube fibers would have to be doubled in strength.

We spent many years trying to work with carbon nanotubes in the form that was available, Siochi said. This changed in 2004 when Nanocomp started making carbon nanotubes not in powder form but in large sheets. These sheets are now in a form that is very similar to what we can use for carbon fiber composites. We started working with them around 2010 because we were evaluating their material for our applications.

The early versions of the carbon nanotube yarn, if looked at under a microscope, would show gaps between the individual nanotubes within the yarn.

They (Nanocomp) have changed the process, and modified the chemicals they use to make the yarn, Meador said. They also did some post-processing techniques on them. To look at a cross section of the current yarn under a microscope, it looks more like a fiber. It is very consolidated and the gaps arent there anymore.

Like any new technology, it takes time to gain acceptance of the technology as reliable for its designed tasks. Further development and testing on the carbon nanotube yarn will determine that acceptance.

There are more improvements that can be made to get the strength up, Meador said. Nanocomp is working on that, and we are continuing to collaborate with them.

Tagged: carbon nanotubes Nanocomp Technologies NASA The Range

Michael Cole is a life-long space flight enthusiast and author of some 36 educational books on space flight and astronomy for Enslow Publishers. He lives in Findlay, Ohio, not far from Neil Armstrongs birthplace of Wapakoneta. His interest in space, and his background in journalism and public relations suit him for his focus on research and development activities at NASA Glenn Research Center, and its Plum Brook Station testing facility, both in northeastern Ohio. Cole reached out to SpaceFlight Insider and asked to join SFI as the first member of the organizations Team Glenn.

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Newly developed Nanotube Technology could revolutionize spaceflight - SpaceFlight Insider

First-ever laser communications terminal to be tested on the Moon – SpaceFlight Insider

Tomasz Nowakowski

July 25th, 2017

Astrobotics Peregrine Lander will deliver a laser communications terminal built by ATLAS to the Moon. Image Credit: Astrobotic

ATLAS Space Operations Inc., a company specializing in cloud-based satellite management and control services, has announced that it will test the first-ever laser communications terminal on the lunar surface. The company has recently signed a contract with Astrobotic Technology Inc., which could see their system fly to the Moon in late 2019.

The terminal, under development by ATLAS, is expected to establish the worlds first laser communication link from the lunar surface. This could mark a significant breakthrough in terms of laser communications for planetary missions.

It is hoped this new system could serve to revolutionize deep space communications. Photo Credit: Mark Usciak / SpaceFlight Insider

Our main goal is to demonstrate the viability of a commercial laser communications capability from the lunar surface. This is a stepping-stone to establishing a permanent infrastructure in support of future lunar activity, Dan Carey, Director of Marketing at ATLAS Space Operations, told SpaceFlight Insider.

The terminal, which will be sent to the Moon on board Astrobotics Peregrine Lander, will carry out first the crucial tests for the development of this potentially ground-breaking technology. This hardware is intended to be a baseline for ATLAS future interplanetary communications technology. Carey noted that the tests on lunar surface will allow us to learn the hard lessons closer to home, on the Moon, before venturing beyond.

By sending its payload to the Moon ATLAS also aims to provide a platform for the public to access a virtual lunar experience. With this technology and lunar capability, the company would be able to provide the rest of humanity an experience that previously has been reserved for an elite class of explorers.

Organizations like NASA and MIT/Lincoln Labs are the ones who have developed the revolutionary technology. ATLAS is taking that technology and commercializing it for the advancement of human interest in space. Our company was founded on the ideal of making space accessible to all, Carey said.

The laser communications terminal is expected to weigh less than 22 pounds (10 kilograms) and will consume less than 60 W for up to 1.0 Gbps of data transfer to Earth. The ground segment of this system will be comprised of Earth Observation Stations, part of the International Laser Ranging Service adapted for this mission, and other commercially-available ground terminal technology previously used for laser communications.

For ATLAS management, the partnership with Astrobotic is considered to be key to showcase its capabilities. Moreover, both companies share the same vision of space exploration and look forward to a long-lasting collaboration.

Astrobotic is progressive and forward thinking. Our companies share a common goal in advancing human interest in lunar and interplanetary exploration. We aim to make the heavens more available and affordable than ever before to all who have similar interests, Carey concluded.

Tagged: Astrobotic Atlas Moon Peregrine lander The Range

Tomasz Nowakowski is the owner of Astro Watch, one of the premier astronomy and science-related blogs on the internet. Nowakowski reached out to SpaceFlight Insider in an effort to have the two space-related websites collaborate. Nowakowski's generous offer was gratefully received with the two organizations now working to better relay important developments as they pertain to space exploration.

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New Horizons team obtains wealth of data from 2014 MU69 occultation – SpaceFlight Insider

Laurel Kornfeld

July 24th, 2017

A 2014 MU69 occultation campaign telescope. Photo Credit: NASA / JHU-APL / SwRI

NASAs New Horizons team captured crucial data on Kuiper Belt Object (KBO) 2014 MU69 the spacecrafts second target during a third organized observation of the KBO occulting a star on Monday, July 17, 2017.

Mission scientists traveled to a remote area in Argentina to catch MU69 pass in front of a star after analysis of observations made with the Hubble Space Telescope and the Gaia satellite determined the location where the KBO would cast a shadow on Earths surface.

Now you see it, now you dont: NASAs New Horizons team trained mobile telescopes on an unnamed star (center) from rural Argentina on July 17, 2017. A Kuiper Belt object 4.1 billion miles from Earth known as 2014 MU69 briefly blocked the light from the background star, in whats called an occultation. The time difference between frames is 200 milliseconds (0.2 seconds). This data helps scientists to better measure the shape, size, and environment around the object; the New Horizons spacecraft will fly by this ancient relic of Solar System formation on Jan. 1, 2019. Animation & Caption Credit: NASA / JHU-APL / SwRI

Led by Marc Buie of the Southwest Research Institute (SwRI), more than 60 scientists braved cold weather and high winds, setting up a line of 24 portable telescopes in Chubut and Santa Cruz, Argentina.

They received support and logistical assistance from Argentinian government officials, scientists, and members of the public, including a two-hour closure of a highway to prevent headlights from impeding the observation.

Located 4.1 billion miles (6.6 billion km) from Earth and one billion miles (1.6 billion km) beyond Pluto, MU69 blocked the light of a bright background star for just 0.2 seconds, but that was enough for at least five observation teams to capture the event.

It was the most historic occultation on the face of the Earth, said NASA director of planetary science Jim Green, who called the team to congratulate them. You pulled it off and made it happen.

Mission co-investigator Amanda Zangari was the first to detect the signature of the 1425 miles (2240 kilometers) wide KBO, which the spacecraft will fly by on January 1, 2019.

MU69 will then be the most distant object to be visited by a spacecraft.

The July 17 event was the last of three stellar occultations by the KBO. The other two occurred on June 3 and July 10. Mission scientists traveled to Argentina and South Africa to observe the June 3 event, then flew above the clouds in NASAs Stratospheric Observatory for Infrared Astronomy (SOFIA) aircraft over the Pacific Ocean from New Zealand for the second one in an effort to study the KBOs environment.

That study centered on detection of any potential hazards near MU69 that could pose a threat to New Horizons.

While it will take scientists weeks to analyze all the data collected during the occultations, that data will play a key role in helping them discover its size, shape, orbit, and environment.

MU69 was detected in 2014 by the Hubble Space Telescope as part of the New Horizons teams search for a second flyby target after Pluto, but it was too remote for any constraint on its size and shape.

Buie praised the Argentinian community of Comodoro Rivadavia for assisting the team by turning off street lights and even parking trucks to act as windbreakers.

The local people were a major team player, he emphasized. He specifically thanked Argentinas National Commission on Space Activities and the Argentinian people for their assistance, noting the effort is an example of space exploration bringing out the best in everyone.

Principal Investigator Alan Stern said: This effort, spanning six months, three spacecraft, 24 portable ground-based telescopes, and NASAs SOFIA airborne observatory was the most challenging stellar occultation in the history of astronomy, but we did it. We spied the shape and size of 2014 MU69 for the first time, a Kuiper Belt scientific treasure we will explore just over 17 months from now.

LEFT: Marc Buie, New Horizons occultation campaign lead, holds up five fingers to represent the number of mobile telescopes in Argentina initially thought to have detected the fleeting shadow of 2014 MU69. The New Horizons spacecraft will fly by the ancient Kuiper Belt object on Jan. 1, 2019. RIGHT: New Horizons Co-Investigator Amanda Zangari was the first occultation campaign scientist to see the telltale signature of MU69 while analyzing data from July 17, saying, We nailed it spectacularly. Credits: NASA / JHU-APL / SwRI / Adriana Ocampo

A video depicting preparations for the July 17 occultation is available for viewing here, and reports on all three occultation observations can be viewed here.

Tagged: KBO 2014 MU69 New Horizons The Range

Laurel Kornfeld is an amateur astronomer and freelance writer from Highland Park, NJ, who enjoys writing about astronomy and planetary science. She studied journalism at Douglass College, Rutgers University, and earned a Graduate Certificate of Science from Swinburne Universitys Astronomy Online program. Her writings have been published online in The Atlantic, Astronomy magazines guest blog section, the UK Space Conference, the 2009 IAU General Assembly newspaper, The Space Reporter, and newsletters of various astronomy clubs. She is a member of the Cranford, NJ-based Amateur Astronomers, Inc. Especially interested in the outer solar system, Laurel gave a brief presentation at the 2008 Great Planet Debate held at the Johns Hopkins University Applied Physics Lab in Laurel, MD.

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New Horizons team obtains wealth of data from 2014 MU69 occultation - SpaceFlight Insider

Our SpaceFlight Heritage: The Shuttle replacement that never was – SpaceFlight Insider

Christopher Paul

July 22nd, 2017

In this artists depiction, NASAs Shuttle C spacecraft opens its payload bay doors. Image Credit: Nathan Koga / SpaceFlight Insider

When the Space Shuttle was first proposed it was meant to be all things to all users, a replacement for all U.S. launch vehicles. All the expendable launchers, Atlas, Titan, and Delta would retire and the shuttle would be responsible for all U.S. launches from its three pads, LC-39A / B at Kennedy Space Center, and SLC-6 at Vandenberg Air Force Base.

The shuttles launch rate was expected to be 100 launches a year. Enormous amounts of money would be saved through the Shuttles reusability.

Unfortunately, this plan fell apart. The shuttle never came close to its predicted launch rate. Officials in the Air Force doubted that a human-rated system would ever save money. However, after the Challenger (STS-51L) disaster, the military almost totally abandoned the shuttle and restored the expendable systems it had nearly abandoned, for its part, as noted by Astronautix, NASA thought the shuttle would only fly about 14 times per year after 1986 (a number of annual flights the agency never came close to reaching).

What was more, the space station that NASA wanted to build was slowly growing in mass. Two modules had already become too heavy for the agencys fleet of orbiters to launch.In the face of these problems, a solution was sought. Shuttle-C was one of the answers proposed.

A NASA Shuttle-C vehicle roars to orbit in this artists depiction. Image Credit: Nathan Koga / SpaceFlight Insider

Shuttle-C was designed as a pure cargo launcher, able to launch much more cargo than the Space Shuttle itself. Since the shuttle was intended to return to Earth with its crew, it necessitated an aerodynamic form, heat shielding for that form, and a crew cabin as well as all of the prerequisites to allow astronauts to live on orbit. Shuttle-C would be an expendable vehicle, enabling much larger cargoes to be delivered to orbit.

The configuration that NASA settled into for Shuttle-C involved an unmodified External Tank and Reusable Solid Rocket Boosters, with a cylindrical cargo container attached to the Shuttles boattail engine housing. Two Space Shuttle Main Engines (SSMEs) would be mounted on the boattail, along with the Shuttles Orbital Maneuvering System.

While SSMEs are expensive and were designed to be reusable, they had a limited life span. NASA usually planned for a maximum of ten flights for each SSME. If Shuttle-C was only launched with engines that already had 9 flights under their belts, no money would be lost in expending them.

NASA also thought about making Shuttle-Cs avionics reusable. By replacing the aerodynamic nose cone over the cylindrical cargo carrier with a Mercury-style reentry vehicle, the avionics could be returned to Earth after launch and reused. NASA studied this system and released a technical report to document this study, entitled, Preliminary design of the Shuttle-C avionics recovery system.

Other versions of Shuttle-C were envisioned, both by internal NASA documents and Martin-Marietta studies. Many included an in-line launch vehicle, with SSMEs mounted under a modified External Tank, and included the option for upper stages. However, NASA disliked these versions, since they required modifications to the External Tank. NASA desired a system that would be a drop-in replacement for their orbiters for cargo-only launches.

Shuttle-C never came into existence. Despite NASAs desire for a heavy-lift cargo launch vehicle, the fusion of Space Station Freedom and Russias Mir-2 station into the International Space Station changed much of the shuttle-station centered planning at NASA.

However, Shuttle-C nearly got another chance at life when NASA started plans to send their fleet of orbiters off on their next mission, as monuments in museums and tourist destinations.

One option presented to the Augustine Committees study of shuttle replacement options in 2009 was Shuttle-C. The proposal was essentially to mount the Orion capsule and its Launch Escape System on top of the Shuttle-C cargo carrier. This would allow both crew and cargo launches to the ISS, and the Shuttle-C cargo carrier had room for both a Delta Cryogenic Second Stage derived upper stage, a J-2X powered Earth Departure Stage as well as additional cargo. This version of Shuttle-C would have mounted three SSMEs and have no additional Orbital Maneuvering System. The proposal suggested an initial cargo-only launch in 2013, and a first crew launch in 2014 after the Shuttles expected retirement in 2010-2011.

Shuttle-C was an often-discussed option, both in and outside of the space agency, though it never came to anything. It might also be considered a symptom of the Shuttle systems success.

However, the independent value of the Shuttle-C system itself is difficult to evaluate in the shadow of NASAs now-retired fleet of shuttle orbiters. It does seem clear in hindsight that a dedicated cargo heavy-lift vehicle would have been a powerful supplement to the orbiter fleet, perhaps enabling a crewed mission to the Moon, or heavier and more-capable robotic missions to other planets, including possibly a dedicated Europa orbiter akin to the Europa Clipper mission now scheduled for an SLS launch.

Regardless of Shuttle-Cs utility or value, NASA is subject to many forces that influence its decision-making, perhaps most potently the whims of elected officials. In the past 13 years, presidents and congresses have come and gone and NASAs directive has been altered several times with many of its programs and efforts rising and falling. Shuttle-C would was joined by other cancelled initiatives, such as Venturestar and Constellation and will, doubtlessly, as new political winds blow in and out of Washington, be joined by others.

Video courtesy of NASA STI

Tagged: NASA Shuttle-C Space Shuttle Main Engine The Range

Christopher Paul has had a lifelong interest in spaceflight. He began writing about his interest in the Florida Tech Crimson. His primary areas of interest are in historical space systems and present and past planetary exploration missions. He lives in Kissimmee, Florida, and also enjoys cooking and photography. Paul saw his first Space Shuttle launch in 2005 when he moved to central Florida to attend classes at the Florida Institute of Technology, studying space science, and has closely followed the space program since. Paul is especially interested in the renewed effort to land crewed missions on the Moon and to establish a permanent human presence there. He has covered several launches from NASA's Kennedy Space Center and Cape Canaveral for space blogs before joining SpaceFlight Insider in mid-2017.

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Our SpaceFlight Heritage: The Shuttle replacement that never was - SpaceFlight Insider

Opportunity rover peers into ‘Perseverance Valley’ Spaceflight Now – Spaceflight Now

Toward the right side of this scene is a broad notch in the crest of the western rim of Endeavour Crater. Wheel tracks in that area were left by NASAs Mars Exploration Rover Opportunity as it observed Perseverance Valley from above in the spring of 2017. The valley is a major destination for the rovers extended mission. It descends out of sight on the inner slope of the rim, extending down and eastward from that notch. Credit: NASA/JPL-Caltech/Cornell/Arizona State Univ.

NASAs Opportunity rover, now showing nearly 28 miles (45 kilometers) on its odometer since landing on Mars, recorded a panoramic view last month of its next scientific destination, a valley that may have been carved by water, an icy or muddy debris flow, or ancient Martian winds.

Imagery experts stitched together this view from a series of images taken by Opportunitys panoramic camera from June 7 to June 19, according to NASA. The panorama covers three-quarters of a full-circle view.

The rover collected images for the panorama while engineers analyzed a stall on the robots left-front wheel steering actuator.

The wheel was pointed outward more than 30 degrees,prompting the team to call the resulting vista Pancams Sprained Ankle panorama, NASA said in a press release.

Engineers were able to get the wheel pointed straight ahead to resume driving, but Opportunity now uses the steering capability of only its two rear wheels, NASA said. The right-front steering actuator failed in 2006.

Opportunitys tracks lead into notch to the right of an outcrop dubbed Cape Tribulation, and scientists think the dip may have been a spillway through which water, ice or wind flowed into the bed of Endeavour Crater, an expansive 14-mile-wide (22-kilometer) depression the rover has explored for nearly six years.

The mobile robot landed on Mars in January 2004 and studied several smaller craters to find evidence that Mars was once habitable. Opportunity arrived at the rim of Endeavour Crater in 2011 after a cross-country journey from its original landing site, outliving its original three-month design life more than 50 times.

The floor of Endeavour Crater stretches toward the horizon in this panorama.

The wheel tracks visible in the image were created as Opportunity drove to the edge of the crater to look into Perseverance Valley, which lies on the inner slope of the crater rim just beyond the notch. Three-dimensional stereo images will help controllers plot Opportunitys drive into the valley, which sits at a slope of 15 to 17 degrees and extends the length of two football fields, based on observations from orbit.

It is a tantalizing scene, said Ray Arvidson, Opportunitys deputy principal investigator from Washington University in St. Louis. You can see what appear to be channels lined by boulders, and the putative spillway at the top of Perseverance Valley. We have not ruled out any of the possibilities of water, ice or wind being responsible.

The rover is now parked in the upper reaches of the valley.

Opportunity will drive deeper into Perseverance Valley next month once engineers re-establish full communications with the rover. Signals between Earth and spacecraft at Mars are currently blocked as the red planet travels behind the sun, but the rover is collecting a new panorama from its current location.

The valley is the prime target for this phase of Opportunitys mission, which NASA approved last year through at least September 2018. Scientists want to know what created the valley, which is the first such fluid-carved feature to ever be visited by a rover on Mars.

Opportunity will also take measurements of the rocks inside Endeavour Crater to compare their composition to the material on the plains outside the crater, officials said.

Email the author.

Follow Stephen Clark on Twitter: @StephenClark1.

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Study teams comb through NASA’s wish list for new telescope – Spaceflight Now

This artists rendition shows a possible design of a potential successor to the Hubble Space Telescope. This conceptual mission, called the Advanced Telescope Large-Aperture Space Telescope (ATLAST), is similar in approach to one of several observatories currently under study by astronomers. Credit: NASA

Scientists outlining four concepts for a powerful new space telescope that could launch in the 2030s this week said improvements in optics, detectors and access to huge new rockets like NASAs Space Launch System could revolutionize the way astronomers observe potentially habitable planets, black holes, and the earliest galaxies in the universe.

It is likely NASA will only be able to afford one of the four proposed flagship observatories, and the space agency will take the advice of an independent review by the National Research Council in 2020 on which type of telescope should receive highest priority.

NASA launched studies last year to look into the scientific benefits, costs and technical challenges of four astronomy missions:

Four teams will produce interim reports on the four mission concepts by the end of this year, then publish their final reports in 2019 as a resource for scientists on the next astrophysics decadal survey panel in 2020, which will rank priorities for future NASA astronomy missions.

The studies will offer only a roadmap for NASAs next leap in astronomy, and officials say any telescope that does reach the launch pad in the 2030s will likely look much different from the concepts currently under investigation. Tough decisions on engineering constraints and cost caps remain ahead, but NASA it needs to start preparing now given the long life cycles of such missions.

The space agency typically follows the decadal surveys advice.

The two last decadal surveys prioritized infrared astronomy. A report from the National Research Council in 2001 led to the approval of the James Webb Space Telescope, which is due for launch next year, and the 2010 decadal survey recommended NASA pursue a mission which became the Wide-Field Infrared Survey Telescope, or WFIRST, scheduled for liftoff in the mid-2020s.

NASA expects to have funding for another advanced flagship-class, multibillion-dollar great observatory to launch some time in the 2030s, once the agency puts behind major spending on JWST and WFIRST.

Astronomers expect breakthroughs with any route prioritized in the next decadal survey.Cost estimates on each of the four mission concepts will come later to help inform the decadal surveys decisions.

The LUVOIR mission concept would be a true successor to Hubble, covering much the same range of wavelengths as NASAs most famous long-lived orbiting telescope. The mission outline is similar in capability to the High Definition Space Telescope, a super-Hubble proposed by astronomers in 2015, and the Advanced Technology Large-Aperture Space Telescope, known by the apt acronym ATLAST.

With LUVOIR, we would be able to study in much greater detail how galaxies assemble their stars, said Debra Fischer, a professor of astronomy at Yale University who co-chairs the LUVOIR study team. The killer app for LUVOIR is actually being able to coronagraph and image pale blue dots around some of the nearest stars, and then once we have those images, to be able to take spectra of them.

Instruments on a mission like LUVOIR could look for signs of water vapor, oxygen, methane and other gases in alien atmospheres that might be habitable, Fischer said in a presentation Thursday to NASAs Astrophysics Advisory Committee.

The size of an observatory like LUVOIR hinges on the volume of launchers that might be available in the 2030s. A primary mirror with multiple segments, similar to the design of JWST, would be folded up for liftoff.

Commercial rockets like United Launch Alliances Delta 4-Heavy and SpaceXs Falcon Heavy come with standard fairings around 5 meters (16 feet) in diameter, while NASAs more costly but more powerful Space Launch System could accommodate payloads as wide as 8.4 meters (28 feet) by the late 2020s.

The dimensions of a telescope like LUVOIR are bracketed by the capabilities of the Delta, Falcon and SLS rocket options, although the Delta 4 rocket is likely to be retired in favor of ULAs next-generation Vulcan booster by the time such a mission is ready for liftoff.

Another rocket that might give future telescopes rides into space is the New Glenn, a methane-powered booster in development by Blue Origin, the space company founded by Amazon.coms Jeff Bezos. The privately-operated New Glenn could make its debut launch by 2020, and it can loft payloads as wide as 7 meters (23 feet).

A rule-of-thumb for deployable telescopes is that a 9 or 10-meter (30-33 foot) primary mirror could tuck inside standard Delta 4-Heavy or Falcon Heavy fairings. The Space Launch Systems nose cone could fit a 16-meter (52-foot) multi-segment mirror folded up origami-style.

None of the proposals under study would need in-space assembly by astronauts, but Fischer said robotic or human servicing might be possible for a mission like LUVOIR.

Fischer identified launch vehicle limitations as one of the top technological risks for the LUVOIR concept, which would likely be sent to an observation post at the L2 Lagrange point a million miles (1.5 million kilometers) from Earth in the direction away from the sun. Other question marks include the readiness of ultraviolet mirror coatings, infrared detector technology, and ultra-stable opto-mechanical systems, Fischer said.

While LUVOIR would be a general purpose observatory best geared for large-scale galactic, dark matter and statistical exoplanet surveys, the smaller HabEx concept would emphasize exoplanet research, focusing on a few nearby stars known to host potentially habitable worlds.

Rather than statistical-based as LUVOIR is, were more exploration-based, said Scott Gaudi, a professor of astronomy at Ohio State University who co-chairs the HabEx study. We want to study nearby planetary systems and just figure out what theyre like.

HabEx could probe up to a dozen potentially Earth-like planets around stars in the suns neighborhood, Gaudi said Thursday.

Our goal is to detect and characterize a handful of potentially habitable planets, and then search for signs of habitability and biosignatures on those planets, he said.

A mission based on the HabEx concept could perhaps distinguish between analogs of Venus, Earth and Mars, which all lie within the suns habitable zone, a region where liquid water could persist on a planets surface under the right conditions. But only Earth has an environment ripe for life.

Gaudi said his team will present at least two HabEx mission concepts to the decadal survey panel, one with a single-piece 4-meter (13-meter) primary mirror with nearly twice the collecting area of Hubble, and another with a 6.5-meter (21-foot) segmented mirror comparable to JWSTs.

HabEx will need help resolving the faint light coming from exoplanets, which can be more than a billion times dimmer than the light coming from their host stars.

One option is to launch a separate starshade, a petal-shaped spacecraft tens of meters (up to 100 feet) wide that would keep formation via laser navigation tens of thousands of miles from a telescope such as HabEx. The idea is to block bright starlight, revealing planets lurking nearby.

A tiny coronagraph embedded inside the telescope could also help detectors register exoplanets, allowing instruments to break up the light into spectra like a prism, telling scientists about the chemicals and gases in their atmospheres.

No space telescope has ever flown with a starshade, and coronagraphs aboard current-era observatories like Hubble and JWST are unable to see planets close to their stars, where temperatures might be favorable for life. The WFIRST mission might carry a coronagraph that works in concert with deformable mirrors and ultra-low-noise cameras, yielding views of potentially habitable worlds, but HabEx would have much better sensitivity thanks to a bigger mirror.

Two other concepts under scrutiny would scan the infrared and X-ray universe.

The Origins Space Telescope will probe the births of stars and planets in the Milky Way galaxy, trace the evolution of galaxies throughout cosmic history, seeing through thick envelopes of dust to study regions invisible to other telescopes.

Building on discoveries expected from JWST and WFIRST both infrared observatories the Origins Space Telescope would be sensitive to lower-energy far-infrared light, a part of the spectrum that reveals some of the coldest parts of the universe.

Beyond JWST, we will still have questions, said Asantha Cooray, a professor at the University of California, Irvine, and co-chair of the Origins Space Telescope study. We will not how those stars came to be. We want to know and we want to understand what mechanics produce what stars.

The far-infrared telescope could be as big as 9 meters (30 feet) in diameter, Cooray said Thursday, a size limit set by the volumes of Delta and Falcon rocket fairings.

The Origins Space Telescope could image pockets of tenuous gas and dust in the interstellar medium, the area between stars. Clumps of cold matter glow in far-infrared light.

We still do not have a probe for the interstellar medium, and thats where the Origins Space Telescope comes in, Cooray said.

He said the infrared observatory would also make observations of exoplanets like LUVOIR and HabEx, and potentially detect biosignatures.

Our science case is broad and covers a wide range of topics, Cooray said. Our aim is to provide a factor of maybe between 5,000 and 10,000 improvement in sensitivity relative to the best we had with (ESAs) Herschel. Thats a large number.

Cooray said a mission based on the Origins Space Telescope approach would have have a factor of 30 better sensitivity than JWST, not just because of its size but because mechanical coolers would chill the observatorys detectors below 5 Kelvin (minus 450 degrees Fahrenheit), just above absolute zero. That will make the future telescope capable of seeing frigid parts of the universe.

We are not trying to take images and improve a little bit, he said. We are really talking about revolutionary astronomy with the Origins Space Telescope.

Astronomers scoping the next potential X-ray telescope are working on the Lynx mission concept.

Billed as a machine for looking back in time to the first billion years after the Big Bang, the Lynx observatory would seek to find the universes first black holes and galaxies. Theories currently govern astronomers understanding of this era, when light from the first stars could escape through an absorbing haze of hydrogen left over from the Big Bang, but Lynx could add hard data to the equation.

We have decided what kind of observatory Lynx should be, how big that observatory should be, said Alexey Vikhlinin, astrophysicist at the Harvard-Smithsonian Center of Astrophysics and co-chair of the Lynx study. We have identified plans for the X-ray optics. We are in the process of making a decision on the (proposed) instrument suite.

Vikhlinin said Thursday the Lynx team has identified the drivers of galaxy formation and the dawn of black holes as two key pillars of the would-be mission.

Lynx would also map the distribution of matter in the cosmic web, the voids, clusters and filaments that tie together the universe. Another target would be the halos of material surrounding galaxies brightest star-filled regions, which astronomers believe plays an important role in a galaxys birth.

Scientists say the Lynx mission would offer a leap in sensitivity two orders of magnitude over Chandra, which launched in 1999, and the planned European-led Athena X-ray telescope due for liftoff in 2028.

But big advances in technology are required to make a mission like Lynx a reality.Vikhlinin said high-resolution lightweight X-ray optics is the area of most concern for us.

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Study teams comb through NASA's wish list for new telescope - Spaceflight Now

On Atlantis’ anniversary, USA’s future space fleet closing in on maiden flights – NASASpaceflight.com

July 21, 2017 by Chris Bergin

The long-awaited return of American astronauts launching on US spacecraft, a capability last seen when Atlantis closed out the Shuttle Program in 2011, is set to return next year. Along with new crew transporters, the Space Shuttles legacy will be honored by the return of a lifting body vehicle, as Dream Chaser makes progress towards her role for uncrewed ISS resupply efforts. Commercial Spacecraft:

Two spacecraft are in a race to launch Americans to the International Space Station (ISS), a capability that has been exclusively conducted by the Russians with a hefty price tag via their Soyuz spacecraft following the 2011 retirement of the Space Shuttle fleet.

The Space Shuttle programs storied 30+ year flight history came to an emotional conclusion six years ago today whenAtlantis dropped from thepre-dawn darkness into the lights illuminating runway 15 at the Kennedy Space Center.

When Atlantis wheels came to a stop just before 5:58am on 21 July 2011, the conclusion of the Shuttle programresulted in a planned crew launch capability gap for the U.S., though few at the time believed the gapwouldlast more than a few years.

Originally, a transition period using the Orion spacecraft in an opening role of launching crew to the ISShad been considered before the demise of the Constellation Program (CxP) created an uncertain future for Orion.

When the SLS program architecture was announced in September 2011, Orion was re-revealed as an exclusivelyBeyond Earth Orbit (BEO) vehicle.

Notably, this change of call sign for Orions future missions was part of a further transition towards handing over Low Earth Orbit (LEO) to the commercial sector, a partnership between NASA and the space launch industry that resulted in the agency contracting out its LEO obligations to commercial companies, all with NASA oversight.

The commercialization of LEO, focused on a supply line to the ISS, began by complementing existing resupply vehicles, such as Russias Progress, Japans HTV and ESAs ATV spacecraft. Joining the resupply team were Orbital ATKs Cygnus and SpaceXs Dragon cargo spacecraft.

Although both vehicles have suffered from a launch vehicle-related failure, the Commercial Resupply Services (CRS) program has proven its worth, paving the way for a second phase, known as CRS2, to continue to provide commercial supply runs into the 2020s.

CRS2 expands the number of flights on the manifest for Cygnus and cargo Dragon whilst also welcoming Dream Chaser to the uncrewed fleet.

A fan favorite in the space flight community, Dream Chaser was one of the main contenders to launch American astronauts to the Station during the Commercial Crew competitionphase.

That crew version of the spacecraft is still technically within NASAs thoughts, as she completes the CCiCAP (Commercial Crew Integrated Capability) element of a NASA contract that was part of the Agencys Commercial Crew Program (CCP) aspirations.

Despite variouslevels of international interest, the crewed version of Dream Chaser faces an uncertain future. However, her new version an uncrewed cargo variant has a lot to look forward to.

As recently noted by SNC, Dream Chaser is currently undergoing a second roundof testing at the Dryden Flight Research Center in California, mirroring the tests conducted in 2013 that resulted in a successful set of milestones, only to be ruined by one of her landing gear gear that was salvaged from a fighter jet failing to deploy during landingthe resulted in the vehicle crashing off the side of the runway.

The spacecraft, a repaired and modified Engineering Test Article (ETA), is currently moving through tow tests ahead of Captive Carry tests and on a date yet to be decided this fall a replay of her free flight and landing that will hopefully conclude the test program with a safe rollout on Edwards Air Force Base runway 22L.

SNC is building two cargo Dream Chasers, each able to fly a total of 30 times over a 10 year lifetime. They, as expected, will be launched by United Launch Alliances Atlas V rocket, with a contract that confirms the partnership signed just this week.

ULA is pleased to partner with Sierra Nevada Corporation to launch its Dream Chaser cargo system to the International Space Station in less than three years, said Gary Wentz, ULA vice president of Human and Commercial Systems, speaking about the deal for the first two launches. We recognize the importance of on time and reliable transportation of crew and cargo to Station and are honored the Atlas V was selected to continue to launch cargo resupply missions for NASA.

Dream Chasers partnership with Atlas V goes back as far as the SpaceDev days, which first provided a fascinating glimpse of the lifting body spacecraft perched on top of the Atlas Vs Centaur upper stage.

The latest version of Dream Chaser is more streamlined and fits inside the large Atlas V fairing. The first launch is expected to take place in 2020.

SNC recognizes the proven reliability of the Atlas V rocket and its availability and schedule performance makes it the right choice for the first two flights of the Dream Chaser, added Mark Sirangelo, corporate vice president of SNCs Space Systems business area.

ULA is an important player in the market and we appreciate their history and continued contributions to space flights and are pleased to support the aerospace community in Colorado and Alabama.

Along with Dream Chasers often-touted dissimilar redundancy by way of being a different type of spacecraft when compared to her capsule based colleagues she will add to NASAs downmass capability, a required element that only Dragon is currently capable of achieving for the CRS program.

This downmass capability which includes time-sensitive science payloads will be returned directly to land, with Dream Chaser utilizing her design by landing on a runway, allowing for quick access to critical experiments.

While Orbital ATKs Cygnus can only look forward to a destructive re-entry at the conclusion of her mission, SpaceXs Dragon returns to a Pacific Ocean splashdown before being shipped back to the Port of Los Angeles and then eventually to Texas for a full mission debrief.

Interestingly, land and sea returns will now be the forward pathfor NASAs two CCP partners, SpaceX and Boeing.

SpaceXs Dragon 2 is nowconfirmed to be returning only to a splashdown in the Pacific, after an anticipatedtransition to a propulsive land landing capability via her SuperDraco thrusters was deleted.

Elon Musk confirmed while noting the related impact on the now-cancelled Red Dragon that propulsive landings are too challenging for the interim, which means Dragon 2 will be heading for water landings via parachutes.

Notably, Dragon 2 was always going to use parachutes, albeit just on the opening crew missions, before transitioning to apropulsive landing.

Regardless of landing style, as previously reported, the first launch of SpaceXs newDragon 2 on an uncrewed demonstration mission to the ISS has now officially slipped into 2018, with the SpX Demo-1 mission now set for February of next year, followed by SpX Demo-2, this time with a crew, in June.

Dragon 2s rival, Boeings Starliner had no plans for propulsive landings, but will interestingly return to land to conclude her crew missions thanks to an invention called airbags, as one Boeing employee cheekily referenced when comparing his spacecraft to other returning vehicles.

Starliner will return under parachutes before inflating itsairbag system at the base of the capsule to allow for a soft touchdown at the landing site. This capability has already been tested during Starliners development program.

The spacecraft like Dream Chaser has partnered with ULA forAtlas V launches en route to the Station.

The first Starliner launch known as the Orbital Flight Test (OFT) is now set to take place in June ahead of a crewed version of themission (the Crewed Flight Test CFT) currently scheduled just two months later in August.

All four missions will be heavily reviewed after each flight prior to NASA working a certification process that will green light the spacecraft for official NASA crew rotation missions.

While Soyuz continues to be contracted for the interim, including an overlap during this initial period as a back-up in case of problems with the commercial vehicles, the ultimate aim is to focus NASA money on American vehicles, as opposed to paying for seats on Soyuz.

(Images: Boeing, SNC, SpaceX, NASA, andL2 artist Nathan Koga The full gallery of Nathans (Starliner to SpaceX Dragon to MCT, SLS, Commercial Crew and more) L2 images can be *found here*)

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On Atlantis' anniversary, USA's future space fleet closing in on maiden flights - NASASpaceflight.com