Milky Way's Supermassive Black Hole May Be a Neutrino Factory

November 17, 2014

Provided by Janet Anderson, NASA Marshall Space Flight Center and Megan Watzke, Chandra X-ray Center

The giant black hole at the center of the Milky Way may be producing mysterious particles called neutrinos. If confirmed, this would be the first time that scientists have traced neutrinos back to a black hole.

The evidence for this came from three NASA satellites that observe in X-ray light: the Chandra X-ray Observatory, the Swift gamma-ray mission, and the Nuclear Spectroscopic Telescope Array (NuSTAR).

Neutrinos are tiny particles that carry no charge and interact very weakly with electrons and protons. Unlike light or charged particles, neutrinos can emerge from deep within their cosmic sources and travel across the universe without being absorbed by intervening matter or, in the case of charged particles, deflected by magnetic fields.

The Earth is constantly bombarded with neutrinos from the sun. However, neutrinos from beyond the solar system can be millions or billions of times more energetic. Scientists have long been searching for the origin of ultra-high energy and very high-energy neutrinos.

Figuring out where high-energy neutrinos come from is one of the biggest problems in astrophysics today, said Yang Bai of the University of Wisconsin in Madison, who co-authored a study about these results published in Physical Review D. We now have the first evidence that an astronomical source the Milky Ways supermassive black hole may be producing these very energetic neutrinos.

Because neutrinos pass through material very easily, it is extremely difficult to build detectors that reveal exactly where the neutrino came from. The IceCube Neutrino Observatory, located under the South Pole, has detected 36 high-energy neutrinos since the facility became operational in 2010.

By pairing IceCubes capabilities with the data from the three X-ray telescopes, scientists were able to look for violent events in space that corresponded with the arrival of a high-energy neutrino here on Earth.

We checked to see what happened after Chandra witnessed the biggest outburst ever detected from Sagittarius A*, the Milky Ways supermassive black hole, said co-author Andrea Peterson, also of the University of Wisconsin. And less than three hours later, there was a neutrino detection at IceCube.

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Milky Way's Supermassive Black Hole May Be a Neutrino Factory

ICON Cleared For Next Development Phase

Image Caption: NASA's new ICON mission will study what causes variation in airglow such as the red glowing band seen in the atmosphere in this image from the International Space Station. Such emissions point to disturbances that can interfere with radio communications. Credit: NASA

Provided by Karen C. Fox, NASAs Goddard Space Flight Center

NASA has officially confirmed the Ionospheric Connection Explorer, or ICON, mission, clearing it to move forward into the development phase. ICON will explore a swath of Earths atmosphere where weather close to the ground impacts the dynamic space environment above in unexpected ways.

By studying this area where terrestrial weather meets space weather, ICON will help resolve long-standing mysteries about the behavior of our planets upper atmosphere, including what causes disruptions in this region, such as those that can significantly affect radio transmissions.

ICON addresses a national need to predict these kinds of disturbed conditions in space, said Thomas Immel, principal investigator for ICON at the University of California at Berkeley. These disturbances can cause radio communication to suddenly and unexpectedly drop out, which is a problem for ships, airplanes, the global positioning system, and the military.

To study the connection between these space weather disturbances and Earths weather, ICON will measure how motions in the lower atmosphere are transmitted into space. The lowest layer of the atmosphere the one we live in and where we experience weather is the troposphere. Above that is the stratosphere, the mesosphere, and the thermosphere. All of these are layers of the atmosphere made of neutral gas, which can move in reaction to the weather down closest to Earth.

The neutral particles in the mesosphere and higher up, however, exist side-by-side with a giant layer of charged particles stretching from 60 to 600 miles high, called the ionosphere. The charged particles are pushed around by the neutral gas, but are also pushed by electric and magnetic fields that course through the region. These forces are at work throughout the ionosphere, day and night.

ICON will fly at a height of some 360 miles and aim its instruments for a view of whats happening at the lowest reaches of space up to 250 miles providing the first ever comprehensive measurements of the region where the thermosphere and ionosphere overlap. Exploring this region will open up entirely new avenues of exploration, because traditionally the ionospheric disturbances at low latitudes were assumed to be primarily driven by the sun.

For years people thought that energy coming in from above, through the solar wind or solar ultraviolet radiation, was the only cause of changes in the upper atmosphere, said Doug Rowland, mission scientist for ICON at NASAs Goddard Space Flight Center in Greenbelt, Maryland. But we now realize that atmospheric movements down below, closer to Earth, actually have a strong effect on whats happening above.

For example, recent images of the ionosphere in ultraviolet light have shown bright spots in two bands around the middle of Earth the brightness represents areas where the charged gas density is significantly higher. The spots also change over time in sync with daily cycles within the lower atmosphere, suggesting that they are directly linked to Earths weather.

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ICON Cleared For Next Development Phase

Space exploration – Wikipedia, the free encyclopedia

Space exploration is the ongoing discovery and exploration of celestial structures in outer space by means of continuously evolving and growing space technology. While the study of space is carried out mainly by astronomers with telescopes, the physical exploration of space is conducted both by unmanned robotic probes and human spaceflight.

While the observation of objects in space, known as astronomy, predates reliable recorded history, it was the development of large and relatively efficient rockets during the early 20th century that allowed physical space exploration to become a reality. Common rationales for exploring space include advancing scientific research, uniting different nations, ensuring the future survival of humanity and developing military and strategic advantages against other countries.

Space exploration has often been used as a proxy competition for geopolitical rivalries such as the Cold War. The early era of space exploration was driven by a "Space Race" between the Soviet Union and the United States, the launch of the first man-made object to orbit the Earth, the USSR's Sputnik 1, on 4 October 1957, and the first Moon landing by the American Apollo 11 craft on 20 July 1969 are often taken as landmarks for this initial period. The Soviet space program achieved many of the first milestones, including the first living being in orbit in 1957, the first human spaceflight (Yuri Gagarin aboard Vostok 1) in 1961, the first spacewalk (by Aleksei Leonov) on 18 March 1965, the first automatic landing on another celestial body in 1966, and the launch of the first space station (Salyut 1) in 1971.

After the first 20 years of exploration, focus shifted from one-off flights to renewable hardware, such as the Space Shuttle program, and from competition to cooperation as with the International Space Station (ISS).

With the substantial completion of the ISS[1] following STS-133 in March 2011, plans for space exploration by the USA remain in flux. Constellation, a Bush Administration program for a return to the Moon by 2020[2] was judged inadequately funded and unrealistic by an expert review panel reporting in 2009.[3] The Obama Administration proposed a revision of Constellation in 2010 to focus on the development of the capability for crewed missions beyond low earth orbit (LEO), envisioning extending the operation of the ISS beyond 2020, transferring the development of launch vehicles for human crews from NASA to the private sector, and developing technology to enable missions to beyond LEO, such as Earth/Moon L1, the Moon, Earth/Sun L2, near-earth asteroids, and Phobos or Mars orbit.[4] As of March 2011, the US Senate and House of Representatives are still working towards a compromise NASA funding bill, which will probably terminate Constellation and fund development of a heavy lift launch vehicle (HLLV).[5]

In the 2000s, the People's Republic of China initiated a successful manned spaceflight program, while the European Union, Japan, and India have also planned future manned space missions. China, Russia, Japan, and India have advocated manned missions to the Moon during the 21st century, while the European Union has advocated manned missions to both the Moon and Mars during the 21st century.

From the 1990s onwards, private interests began promoting space tourism and then private space exploration of the Moon (see Google Lunar X Prize).

The first steps of putting a man-made object into space were taken by German scientists during World War II while testing the V-2 rocket, which became the first man-made object in space on 3 October 1942 with the launching of the A-4. After the war, the U.S. used German scientists and their captured rockets in programs for both military and civilian research. The first scientific exploration from space was the cosmic radiation experiment launched by the U.S. on a V-2 rocket on 10 May 1946.[6] The first images of Earth taken from space followed the same year[7][8] while the first animal experiment saw fruit flies lifted into space in 1947, both also on modified V-2s launched by Americans. Starting in 1947, the Soviets, also with the help of German teams, launched sub-orbital V-2 rockets and their own variant, the R-1, including radiation and animal experiments on some flights. These suborbital experiments only allowed a very short time in space which limited their usefulness.

The first successful orbital launch was of the Soviet unmanned Sputnik 1 ("Satellite 1") mission on 4 October 1957. The satellite weighed about 83kg (183lb), and is believed to have orbited Earth at a height of about 250km (160mi). It had two radio transmitters (20 and 40MHz), which emitted "beeps" that could be heard by radios around the globe. Analysis of the radio signals was used to gather information about the electron density of the ionosphere, while temperature and pressure data was encoded in the duration of radio beeps. The results indicated that the satellite was not punctured by a meteoroid. Sputnik 1 was launched by an R-7 rocket. It burned up upon re-entry on 3 January 1958.

This success led to an escalation of the American space program, which unsuccessfully attempted to launch a Vanguard satellite into orbit two months later. On 31 January 1958, the U.S. successfully orbited Explorer 1 on a Juno rocket. In the meantime, the Soviet dog Laika became the first animal in orbit on 3 November 1957.

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Space exploration - Wikipedia, the free encyclopedia

Pioneering Space Station Breakthroughs: NASA's EXPRESS Rack Reaches 100,000-Hour Milestone

November 12, 2014

Image Caption: NASA astronaut Steve Swanson grows vegetables on the International Space Station in the Veggie facility located in EXPRESS Rack 8 during Expedition 39. Credit: NASA

Provided by Bill Hubscher, International Space Station Program Science Office, NASAs Marshall Space Flight Center

Getting more from less is no clich aboard the International Space Station, its necessity. With six people living, working and conducting science in the space of a single-family house 240 miles above Earth, square footage is at a premium. NASAs EXPRESS Rack helps ensure theres room for research on the orbiting laboratory.

EXPRESS is a multipurpose rack system housing and supporting research. On Oct. 4, EXPRESS Rack 1 marked 100,000 hours of operation. There are eight EXPRESS racks on the station, each filled with multiple studies.

The versatility of EXPRESS is what makes it so valuable to NASA and scientists, said Tara Ruttley, associate program scientist for the space station at NASAs Johnson Space Center in Houston. Not only can it house experiments, but it also provides a customized environment for each, allowing proper working conditions for each investigation. It helps us learn more about living and working in space, which leads to new advances in science and medicine on Earth.

EXPRESS allows investigators to perform research across scientific disciplines by providing common structural interfaces, power, data, cooling, water and other items needed to conduct experiments in space. Since 2001, the racks have housed dozens of investigations leading to ground-breaking science discoveries, Earth benefits and technology innovations that are aiding future space travel.

Its rewarding to see our EXPRESS Rack reach this milestone and continue to play an integral part of space station research, said Annette Sledd, space station office manager at NASAs Marshall Space Flight Center in Huntsville, Alabama. The versatility of the racks to provide standard communication interfaces and utilities is key to their success and expanded use in support of station research, technology demonstrations and housing payload support equipment.

[ Watch the Video: ExPRESS Rack ]

Payloads flown in EXPRESS Racks range from Protein Crystal Growth experiments to the Advanced Astroculture (ADVASC) investigation to refrigerators and incubators, to name just a few examples. One investigation in the racks includes 20 mice and is part of the Rodent Research investigation. The fourth SpaceX cargo resupply service mission delivered the first rodent studies to the station. Studies on the space shuttle indicated rodents make good research models for physiological changes similar to those experienced by humans. The investigation will provide information about changes occurring during spaceflight and could lead to discoveries in basic biology and offer insight into human aging and disease on Earth.

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Pioneering Space Station Breakthroughs: NASA's EXPRESS Rack Reaches 100,000-Hour Milestone

Barrios Nimon presented Space Flight Awareness Trailblazer Award

PRESS RELEASE

Barrios Technologys Jessica Nimon was recently presented the coveted Space Flight Awareness Trailblazer Award. Nimon is the International Space Station (ISS) Research Communications Managing Editor on Barrios Mission and Program Integration (MAPI) contract. The award was presented to her in recognition of her leadership in the development and implementation of cross-center research communication products such as web stories, ISS Science blogs, and ISS science news features that engage stakeholders in the benefits of space station research.

Nimon has used her talents as both an exceptional writer and integrator to develop and implement new and innovative processes to coordinate ISS communication products across the various NASA centers and the Headquarters Public Affairs and Outreach (PAO) office. Her space station science web stories, blogs, and news features have been timely, relevant, interesting, amplifying ISS science messages. Sharing the benefits of ISS utilization to stakeholders such as the public, Congress, NASA management, and astronauts is a major goal for NASA. Nimon articles are used in such communication products as congressional packages, ISS scientific awards, astronaut training, and ISS science press conferences. Her ability to utilize social media has improved ISS research and technology web page views to over 500,000 per month, the@ISS_Research Twitter account which Nimon created and manages was nominated for a Twitter Shorty Award in Science (social media recognition for promoting science).

Nimon joined the Barrios team in February of 2013. She holds a Masters in English from University of Dallas and a Bachelors in English and Photography from Sam Houston State University. Nimon has received other honors for her work on the MAPI contract including the NASA Group Achievement Award for The ISS Research Web and Social Media Team.

The SFA Trailblazer Award is presented to employees in the early stages of their career who demonstrate strong work ethic and creative, innovative thinking in support of human spaceflight. The SFA Program is a NASA-managed motivational and recognition program with invited representation from NASA and contractors having major responsibilities for human spaceflight mission success. SFAs goal is to ensure each and every employee involved in human space flight is aware of the importance of their role in promoting astronaut safety and mission success in the critical, challenging task of flying humans in the hostile environment of space by communicating and educating the Government/industry workforce about human space flight.

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Barrios Nimon presented Space Flight Awareness Trailblazer Award

Journey to space in Axe Apollo Space Academy (AASA) Program | Pirada Techavijit | TEDxChiangMai – Video


Journey to space in Axe Apollo Space Academy (AASA) Program | Pirada Techavijit | TEDxChiangMai
Mink won a competition to become Thailand #39;s first astronaut. This talk covers the first part of her story (preparations). She will be speaking at a future TEDxChiangMai event about her experience...

By: TEDx Talks

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Journey to space in Axe Apollo Space Academy (AASA) Program | Pirada Techavijit | TEDxChiangMai - Video

Mars MAVEN Orbiter Demonstrates Its Relay Prowess

November 11, 2014

Provided by Guy Webster/Jet Propulsion Laboratory and Nancy Neal Jones/Goddard Space Flight Center

The newest node in NASAs Mars telecommunications network a radio aboard the MAVEN orbiter custom-designed for data links with robots on the surface of Mars handled a copious 550 megabits during its first relay of real Mars data.

MAVENs Electra UHF radio received the transmission from NASAs Curiosity Mars rover on Nov. 6, using an adaptive data rate as the orbiter passed through the sky over the rover. The data that MAVEN relayed to NASAs Deep Space Network of large dish antennas on Earth included several images of terrain that Curiosity has been examining at the base of Mars Mount Sharp. The test also included relaying data to Curiosity from Earth via MAVEN.

MAVEN (for Mars Atmosphere and Volatile EvolutioN) entered orbit around Mars on Sept. 21. The orbiter is finishing a commissioning phase including calibration of its science instruments and fine tuning of its orbit before its prime science phase starts. MAVEN will investigate the upper atmosphere of Mars to provide understanding about processes that led to the loss of much of the original Martian atmosphere.

Two older NASA orbiters, Mars Odyssey and Mars Reconnaissance Orbiter, currently provide data relay for NASAs two active Mars rovers while also continuing to study Mars. Using relay via orbiters, compared with the rovers capability to transmit directly to Earth, greatly increases science data return from the Martian surface.

MAVEN will be available during its prime science mission to provide relay services if issues arise with the other orbiters, and it may routinely provide relay support during an anticipated extended mission.

The Electra design is also on UHF radios aboard Curiosity and Mars Reconnaissance Orbiter. It includes relay-enhancing features such as the ability to automatically adjust data rate to signal strength as the distance to the rover changes during the orbiters overflight. MAVENs orbit is more elongated than the orbits of either Mars Odyssey or Mars Reconnaissance Orbiter. During the Nov. 6 test, MAVENs distance from Curiosity ranged from about 680 miles to 2,300 miles (1,110 to 3,700 kilometers), farther than is typical in communication sessions between the Curiosity rover and the other orbiters.

MAVENs principal investigator is based at the University of Colorados Laboratory for Atmospheric and Space Physics, and NASAs Goddard Space Flight Center in Greenbelt, Maryland, manages the MAVEN project. NASAs Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, supplied and operates MAVENs Electra payload and provides Deep Space Network support for the mission.

For more information about the MAVEN mission, visit: http://www.nasa.gov/maven and http://lasp.colorado.edu/home/maven/. For more information about NASAs Mars Exploration Program, see: http://marsprogram.jpl.nasa.gov.

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Mars MAVEN Orbiter Demonstrates Its Relay Prowess