Mars Exploration Rover Mission: Home

Opportunity Mars Rover Preparing for Active Winter NASA's Opportunity Mars rover will soon drive to the southern side of a valley where a sunward tilt will help the solar-powered rover keep active through the Martian winter. Read News >> View Related Image >> Opportunity Rover's 7th Mars Winter to Include New Study Area NASA's Opportunity rover has resumed driving after Mars emerged from behind the sun. Plans call for the rover to examine sites in Marathon Valley during the upcoming winter. Read News >> Watch Related Video >> Mars Missions to Pause Commanding in June, Due to Sun Next month, Mars will swing almost directly behind the sun from Earth's perspective, and this celestial geometry will lead to diminished communications with spacecraft at Mars. >> Martian Reminder of a Pioneering Flight Names related to the first solo nonstop flight across the Atlantic have been informally assigned to a crater NASA's Opportunity Mars rover is studying. This false-color view of the "Spirit of St. Louis Crater" and the "Lindbergh Mound" inside it comes from Opportunity's panoramic camera. >> Rock Spire in 'Spirit of St. Louis Crater' on Mars An elongated crater called "Spirit of St. Louis," with a rock spire in it, dominates a recent scene from the panoramic camera (Pancam) on NASA's Mars Exploration Rover Opportunity. >> Mars Test Rover Joins Runners at Finish Line Runners at JPL cheer as a test model of NASA's Mars rover Opportunity does a ceremonial "crossing the finish line" after a relay marathon to celebrate the real rover surpassing the distance of a marathon race on Mars. >> Rover Amnesia Event Follows Latest Memory Reformatting The team operating NASA's Mars Exploration Rover Opportunity learned Thursday that the long-lived rover experienced a brief amnesia event related to its flash memory, the first since a reformatting of that nonvolatile type of memory a week earlier. >> NASA's Opportunity Mars Rover Passes Marathon Distance NASA's Mars Exploration Rover Opportunity completed its first Mars marathon Tuesday -- 26.219 miles (42.195 kilometers) with a finish time of roughly 11 years and two months. >> NASA Reformats Memory of Longest-Running Mars Rover After avoiding use of the rover's flash memory for three months, the team operating NASA's 11-year-old Mars Exploration Rover Opportunity has reformatted the vehicle's flash memory banks and resumed storing some data overnight for transmitting later. >> Rover Examining Odd Mars Rocks at Valley Overlook NASA's Mars Exploration Rover Opportunity is investigating unusual rocks before reformatting the rover's memory and continued driving toward "Marathon Valley." >> Opportunity Rover Nears Mars Marathon Feat In February 2015, NASA's Mars Exploration Rover Opportunity is approaching a cumulative driving distance on Mars equal to the length of a marathon race. This map shows the rover's position relative to where it could surpass that distance. >> Hilltop Panorama Marks Mars Rover's 11th Anniversary A panorama from one of the highest elevations that NASA's Mars Exploration Rover Opportunity has reached in its 11 years on Mars includes the U.S. flag at the summit. >> NASA Mars Rover Opportunity Climbs to High Point on Rim NASA's Mars Exploration Rover Opportunity, continuing to drive while engineers tackle a flash-memory issue, has reached a crater-rim high point on "Cape Tribulation." >> All Press Releases >> All Spotlights >>

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Mars Exploration Rover Mission: Home

NASA to deliver new findings on Mars’ atmosphere – CNN.com

Mars rover Curiosity

The rover drilled this dime-sized hole to collect a sample from a rock called "Buckskin" on July 30.

Mars rover Curiosity

This April 10 view from the navigation camera on Curiosity shows the terrain ahead of the rover as it makes its way west through a valley called "Artist's Drive."

Mars rover Curiosity

The Mars rover Curiosity does a test drill on a rock dubbed "Bonanza King" to determine whether it would be a good place to dig deeper and take a sample. But after the rock shifted, the test was stopped.

Mars rover Curiosity

Curiosity used the equivalent of a dust broom to sweep away reddish oxidized dust from the Bonanza King rock. The rover's team decided to ditch the site and drive Curiosity toward other destinations.

Mars rover Curiosity

Wheel tracks from Curiosity are seen on the sandy floor of a lowland area dubbed "Hidden Valley" in this image taken August 4.

Mars rover Curiosity

The rover recently encountered this iron meteorite, which NASA named Lebanon. This find is similar in shape and luster to iron meteorites found on Mars by the previous generation of rovers.

Mars rover Curiosity

Curiosity took this nighttime photo of a hole it drilled May 5 to collect soil samples. NASA said this image combines eight exposures taken after dark on May 13.

Mars rover Curiosity

An arm of Curiosity drills two holes into sandstone on May 5. The rock powder collected will be analyzed by the rover's onboard instruments.

Mars rover Curiosity

This view of the twilight sky and Martian horizon, taken by Curiosity, includes Earth as the brightest point of light in the night sky. Earth is a little left of center in the image, and our moon is just below Earth. A human observer with normal vision, if standing on Mars, could easily see Earth and the moon as two distinct, bright "evening stars."

Mars rover Curiosity

This mosaic of images from the Navigation Camera on Curiosity shows the terrain to the west from the rover's position on the 528th Martian day, or sol, of the mission on January 30. The images were taken right after Curiosity had arrived at the eastern edge of a location called "Dingo Gap."

Mars rover Curiosity

An illustration depicts the possible extent of an ancient lake inside Gale Crater, where the rover landed in August 2012. The $2.5 billion NASA mission set out to explore Gale Crater, which was thought to have once hosted flowing water. Curiosity found evidence of clay formations, or "mudstone," in the crater's Yellowknife Bay, scientists said in 2013. This clay may have held the key ingredients for life billions of years ago. It means a lake must have existed in the area.

Mars rover Curiosity

The Curiosity rover took this image of a rock formation informally dubbed "Darwin." Scientists had the rover stop in this region, called Waypoint 1, because it appeared to be a prime area to study the inner makeup and history of the floor of the Gale Crater. Analysis of Darwin may provide evidence of whether water played a role in the layering of rocks in this region.

Mars rover Curiosity

Curiosity began a trek toward Mount Sharp after spending more than six months in the "Glenelg" area. This image was taken on July 16, 2013, after the rover passed the 1-kilometer mark for the total distance covered since the start of the mission.

Mars rover Curiosity

The lower slopes of Mount Sharp are visible at the top of this image, taken on July 9, 2013. The turret of tools at the end of the rover's arm, including the rock-sampling drill in the lower left corner, can also be seen.

Mars rover Curiosity

This image, taken by the rover on July 8, 2013, shows the tracks left behind after the rover's first drive away from the "Glenelg" area.

Mars rover Curiosity

Curiosity drilled into a rock target called "Cumberland" on May 19, 2013, and it collected a powdered sample of material from the rock's interior. The sample will be compared to an earlier drilling at the "John Klein" site, which has a similar appearance and is about 9 feet away.

Mars rover Curiosity

Mars once had conditions favorable for microbial life, NASA scientists announced on March 12, 2013. One piece of evidence for that conclusion comes from this area of the Martian surface, nicknamed "Sheepbed." It shows veins of sediments that scientist believe were deposited under water and was an environment once hospitable to life.

Mars rover Curiosity

The rock on the left, called Wopmay, was discovered by the rover Opportunity, which arrived in 2004 on a different part of Mars. Iron-bearing sulfates indicate that this rock was once in acidic waters. On the right are rocks from Yellowknife Bay, where rover Curiosity was situated. These rocks are suggestive of water with a neutral pH, which is hospitable to life formation.

Mars rover Curiosity

Curiosity shows the first sample of powdered rock extracted by the rover's drill. The image was taken by Curiosity's mast camera on February 20, 2013.

Mars rover Curiosity

The rover drilled this hole, in a rock that's part of a flat outcrop researchers named "John Klein," during its first sample drilling on February 8, 2013.

Mars rover Curiosity

Curiosity's first set of nighttime photos include this image of Martian rock illuminated by ultraviolet lights. Curiosity used the camera on its robotic arm, the Mars Hand Lens Imager, to capture the images on January 22, 2013.

Mars rover Curiosity

Another nighttime image includes this rock called Sayunei in the Yellowknife Bay area of Mars' Gale Crater. Curiosity's front-left wheel had scraped the rock to inspect for fresh, dust-free materials in an area where drilling for rock would soon begin.

Mars rover Curiosity

Other night photos included this image of the calibration target for the Mars Hand Lens Imager camera at the end of the rover's robotic arm. For scale, a penny on the calibration target is three-fourths of an inch in diameter.

Mars rover Curiosity

A view of what NASA describes as "veined, flat-lying rock." It was selected as the first drilling site for the Mars rover.

Mars rover Curiosity

Curiosity used a dust-removal tool for the first time to clean this patch of rock on the Martian surface on January 6, 2013.

Mars rover Curiosity

The rover captured this mosaic of images of winding rocks known as the Snake River on December 20, 2012.

Mars rover Curiosity

A view of the shallow depression known as "Yellowknife Bay," taken by the rover on December 12, 2012.

Mars rover Curiosity

The Mars rover Curiosity recorded this view from its left navigation camera after an 83-foot eastward drive on November 18, 2012. The view is toward "Yellowknife Bay" in the "Glenelg" area of Gale Crater.

Mars rover Curiosity

Three "bite marks" made by the rover's scoop can be seen in the soil on Mars surface on October 15, 2012.

Mars rover Curiosity

The robotic arm on NASA's Mars rover Curiosity delivered a sample of Martian soil to the rover's observation tray for the first time on October 16, 2012.

Mars rover Curiosity

This image shows part of the small pit or bite created when NASA's Mars rover Curiosity collected its second scoop of Martian soil on October 15, 2012. The rover team determined that the bright particle near the center of the image was native to Mars, and not debris from the rover's landing.

Mars rover Curiosity

This image shows what the rover team has determined to be a piece of debris from the spacecraft, possibly shed during the landing.

Mars rover Curiosity

The rover's scoop contains larger soil particles that were too big to filter through a sample-processing sieve. After a full-scoop sample had been vibrated over the sieve, this portion was returned to the scoop for inspection by the rover's mast camera.

Mars rover Curiosity

This 360-degree panorama shows the area where the rover will spend about three weeks collecting scoopfuls of soil for examination. The photo comprises images taken from the rover's navigation camera on October 5, 2012.

Mars rover Curiosity

An area of windblown sand and dust downhill from a cluster of dark rocks has been selected as the likely location for the first use of the scoop on the arm of NASA's Mars rover Curiosity.

Mars rover Curiosity

Curiosity cut a wheel scuff mark into a wind-formed ripple at the "Rocknest" site on October 3, 2012. This gave researchers a better opportunity to examine the particle-size distribution of the material forming the ripple.

Mars rover Curiosity

NASA's Curiosity rover found evidence for what scientists believe was an ancient, flowing stream on Mars at a few sites, including the rock outcrop pictured here. The key evidence for the ancient stream comes from the size and rounded shape of the gravel in and around the bedrock, according to the Jet Propulsion Laboratory/Caltech science team. The rounded shape leads the science team to conclude they were transported by a vigorous flow of water. The grains are too large to have been moved by wind.

Mars rover Curiosity

This photo is an up-close look at an outcrop that also shows evidence of flowing water, according to the JPL/Caltech science team. The outcrop's characteristics are consistent with rock that was formed by the deposition of water and is composed of many smaller rounded rocks cemented together. Water transport is the only process capable of producing the rounded shape of conglomerate rock of this size.

Mars rover Curiosity

Curiosity completed its longest drive to date on September 26, 2012. The rover moved about 160 feet east toward the area known as "Glenelg." As of that day the rover had moved about a quarter-mile from its landing site.

Mars rover Curiosity

This image shows the robotic arm of NASA's Mars rover Curiosity with the first rock touched by an instrument on the arm. The photo was taken by the rover's right navigation camera.

Mars rover Curiosity

This image combines photographs taken by the rover's Mars Hand Lens Imager at three distances from the first Martian rock that NASA's Curiosity rover touched with its arm. The images reveal that the target rock has a relatively smooth, gray surface with some glinty facets reflecting sunlight and reddish dust collecting in recesses in the rock.

Mars rover Curiosity

This rock will be the first target for Curiosity's contact instruments. Located on a turret at the end of the rover's arm, the contact instruments include the Alpha Particle X-Ray Spectrometer for reading a target's elemental composition and the Mars Hand Lens Imager for close-up imaging.

Mars rover Curiosity

Researchers used the Curiosity rover's mast camera to take a photo of the Alpha Particle X-Ray Spectrometer. The image was used to see whether it had been caked in dust during the landing.

Mars rover Curiosity

Researchers also used the mast camera to examine the Mars Hand Lens Imager on the rover to inspect its dust cover and check that its LED lights were functional. In this image, taken on September 7, 2012, the imager is in the center of the screen with its LED on. The main purpose of Curiosity's imager camera is to acquire close-up, high-resolution views of rocks and soil from the Martian surface.

Mars rover Curiosity

This is the open inlet where powdered rock and soil samples will be funneled down for analysis. The image is made up of eight photos taken on September 11, 2012, by the imager and is used to check that the instrument is operating correctly.

Mars rover Curiosity

This is the calibration target for the imager. This image, taken on September 9, 2012, shows that the surface of the calibration target is covered with a layor of dust as a result of the landing. The calibration target includes color references, a metric bar graphic, a penny for scale comparison, and a stair-step pattern for depth calibration.

Mars rover Curiosity

This view of the three left wheels of NASA's Mars rover Curiosity combines two images that were taken by the rover's Mars Hand Lens Imager on September 9, 2012, the 34th day of Curiosity's work on Mars. In the distance is the lower slope of Mount Sharp.

Mars rover Curiosity

This view of the lower front and underbelly areas of NASA's Mars rover Curiosity was taken by the rover's Mars Hand Lens Imager. Also visible are the hazard avoidance cameras on the front of the rover.

Mars rover Curiosity

The penny in this image is part of a camera calibration target on NASA's Mars rover Curiosity. The image was taken by the Mars Hand Lens Imager camera.

Mars rover Curiosity

The rover captured this mosiac of a rock feature called 'Snake River" on December 20, 2012.

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NASA to deliver new findings on Mars' atmosphere - CNN.com

Goddard Space Flight Center – Wikipedia, the free encyclopedia

The Goddard Space Flight Center (GSFC) is a major NASA space research laboratory established on May 1, 1959 as NASA's first space flight center.[1] GSFC employs approximately 10,000 civil servants and contractors, and is located approximately 6.5 miles (10.5km) northeast of Washington, D.C. in Greenbelt, Maryland, USA. GSFC, one of ten major NASA field centers, is named in recognition of Dr. Robert H. Goddard (18821945), the pioneer of modern rocket propulsion in the United States.

GSFC is the largest combined organization of scientists and engineers in the United States dedicated to increasing knowledge of the Earth, the Solar System, and the Universe via observations from space. GSFC is a major U.S. laboratory for developing and operating unmanned scientific spacecraft. GSFC conducts scientific investigation, development and operation of space systems, and development of related technologies. Goddard scientists can develop and support a mission, and Goddard engineers and technicians can design and build the spacecraft for that mission. Goddard scientist John C. Mather shared the 2006 Nobel Prize in Physics for his work on COBE.

GSFC also operates two spaceflight tracking and data acquisition networks (the Space Network and the Near Earth Network), develops and maintains advanced space and Earth science data information systems, and develops satellite systems for the National Oceanic and Atmospheric Administration (NOAA).

GSFC manages operations for many NASA and international missions including the Hubble Space Telescope (HST), the Explorer program, the Discovery Program, the Earth Observing System (EOS), INTEGRAL, MAVEN, OSIRIS-REx, the Solar and Heliospheric Observatory (SOHO), the Solar Dynamics Observatory (SDO), the Rossi X-ray Timing Explorer (RXTE) and Swift. Past missions managed by GSFC include the Compton Gamma Ray Observatory, SMM, COBE, IUE, and ROSAT. Typically, unmanned earth observation missions and observatories in Earth orbit are managed by GSFC,[citation needed] while unmanned planetary missions are managed by the Jet Propulsion Laboratory (JPL) in Pasadena, California.[citation needed]

Goddard is NASA's first, and oldest, space center. Its original charter was to perform five major functions on behalf of NASA: technology development and fabrication, planning, scientific research, technical operations, and project management. The center is organized into several directorates, each charged with one of these key functions.

Until May 1, 1959, NASA's presence in Greenbelt, Maryland was known as the Beltsville Space Center. It was then renamed the Goddard Space Flight Center (GSFC), after Dr. Robert H. Goddard. Its first 157 employees transferred from the United States Navy's Project Vanguard missile program, but continued their work at the Naval Research Laboratory in Washington, D.C., while the center was under construction.

Goddard Space Flight Center contributed to Project Mercury, America's first manned space flight program. The Center assumed a lead role for the project in its early days and managed the first 250 employees involved in the effort, who were stationed at Langley Research Center in Hampton, Virginia. However, the size and scope of Project Mercury soon prompted NASA to build a new Manned Spacecraft Center, now the Johnson Space Center, in Houston, Texas. Project Mercury's personnel and activities were transferred there in 1961.

Goddard Space Flight Center remained involved in the manned space flight program, providing computer support and radar tracking of flights through a worldwide network of ground stations called the Spacecraft Tracking and Data Acquisition Network (STDN). However, the Center focused primarily on designing unmanned satellites and spacecraft for scientific research missions. Goddard pioneered several fields of spacecraft development, including modular spacecraft design, which reduced costs and made it possible to repair satellites in orbit. Goddard's Solar Max satellite, launched in 1980, was repaired by astronauts on the Space Shuttle Challenger in 1984. The Hubble Space Telescope, launched in 1990, remains in service and continues to grow in capability thanks to its modular design and multiple servicing missions by the Space Shuttle.

Today, the center remains involved in each of NASA's key programs. Goddard has developed more instruments for planetary exploration than any other organization, among them scientific instruments sent to every planet in the Solar System.[2] The Center's contribution to the Earth Science Enterprise includes several spacecraft in the Earth Observing System fleet as well as EOSDIS, a science data collection, processing, and distribution system. For the manned space flight program, Goddard develops tools for use by astronauts during extra-vehicular activity, and operates the Lunar Reconnaissance Orbiter, a spacecraft designed to study the Moon in preparation for future manned exploration.

Goddard's partly wooded campus is a few miles northeast of Washington, D.C. in Prince George's County. The center is on Greenbelt Road, which is Maryland Route 193. Baltimore, Annapolis, and NASA Headquarters in Washington are 3045 minutes away by highway. Greenbelt also has a train station with access to the Washington Metro system and the MARC commuter train's Camden line.

The Goddard Visitor Center is open to the public Tuesdays through Sundays, free of charge, and features displays of spacecraft and technologies developed there. The Hubble Space Telescope is represented by models and deep space imagery from recent missions. The center also features a Science On a Sphere projection system.

The center also features an Educator's Resource Center available for use by teachers and education volunteers such as Boy and Girl Scout leaders; and hosts special events during the year. As an example, in September 2008 the Center opened its gates for Goddard LaunchFest (see Goddard LaunchFest Site). The event, free to the public, included; robot competitions, tours of Goddard facilities hosted by NASA employees, and live entertainment on the Goddard grounds.

The High Bay Cleanroom located in building 29 is the world's largest ISO 7 cleanroom with 1.3 million cubic feet of space.[3] Vacuum chambers in adjacent buildings 10 and 7 can be chilled or heated to +/- 200C (392F). Adjacent building 15 houses the High Capacity Centrifuge which is capable of generating 30 G on up to a 2.5 tons load.[4]

The High Energy Astrophysics Science Archive Research Center (HEASARC) is NASA's designated center for the archiving and dissemination of high energy astronomy data and information. Information on X-ray and gamma-ray astronomy and related NASA mission archives are maintained for public information and science access.[5]

The Software Assurance Technology Center (SATC) is a NASA department founded in 1992 as part of their Systems Reliability and Safety Office at Goddard Space Flight Center. Its purpose was "to become a center of excellence in software assurance, dedicated to making measurable improvement in both the quality and reliability of software developed for NASA at GSFC". The Center has been the source of research papers on software metrics, assurance, and risk management.[6]

GSFC operates three facilities that are not located at the Greenbelt site. These facilities are:

GSFC is also responsible for the White Sands Complex, a set of two sites in Las Cruces, NM, but the site is owned by Johnson Space Center as part of the White Sands Test Facility.

Goddard Space Flight Center has a workforce of over 3,000 civil servant employees, 60% of which are engineers and scientists.[7] There are approximately 7,000 supporting contractors on site every day. It is one of the largest concentrations of the world's premiere space scientists and engineers. The Center is organized into 8 directorates, which includes Applied Engineering and Technology, Flight Projects, Science and Exploration, and Safety & Mission Assurance.[8]

Co-op students from universities in all 50 States can be found around the campus every season through the Cooperative Education Program.[9] During the summers, programs such as the Summer Institute in Engineering and Computer Applications (SIECA) and Excellence through Challenging Exploration and Leadership (EXCEL) provide internship opportunities to students from the US and territories such as Puerto Rico to learn and partake in challenging scientific and engineering work.

A fact sheet highlighting many of Goddard's previous missions are recorded on a 40th anniversary webpage [10]

Goddard has been involved in designing, building, and operating spacecraft since the days of Explorer 1, the nation's first artificial satellite. The list of these missions reflects a diverse set of scientific objectives and goals. The Landsat series of spacecraft has been studying the Earth's resources since the launch of the first mission in 1972. TIROS-1 launched in 1960 as the first success in a long series of weather satellites. The Spartan platform deployed from the space shuttle, allowing simple, low-cost 2-3 day missions. The second of NASA's Great Observatories, the Compton Gamma Ray Observatory, operated for nine years before re-entering the Earth's atmosphere in 2000. Another of Goddard's space science observatories, the Cosmic Background Explorer, provided unique scientific data about the early universe.[11]

Goddard currently supports the operation of dozens of spacecraft collecting scientific data. These missions include earth science projects like the Earth Observing System (EOS) that includes the Terra, Aqua, and Aura spacecraft flying alongside several projects from other Centers or other countries. Other major earth science projects that are currently operating include the Tropical Rainfall Measurement Mission TRMM, a mission that has provided data critical to hurricane predictions. Many Goddard projects support other organizations, such as the US Geological Survey on Landsat-7 and NOAA on the GOES spacecraft that provide weather predictions.

Other Goddard missions support a variety of space science disciplines. Goddard's most famous project is the Hubble Space Telescope, a unique science platform that has been breaking new ground in astronomy for nearly 20 years. Other missions such as the Wilkinson Microwave Anisotropy Probe WMAP study the structure and evolution of the universe. Other missions such as the Solar and Heliospheric Observatory (SOHO) are currently studying the Sun and how its behavior affects life on the Earth.[12]

The Goddard community continually works on numerous operations and projects that have launch dates ranging from the upcoming year to a decade down the road. These operations also vary in what scientists hope they will uncover.

Particularly noteworthy operations include: the James Webb Space Telescope which will try to study the history of the universe and Aquarius will measure the waters salinity in order to better understand the global cycling of water.[13]

Addressing Scientific Questions

NASA's missions (and therefore Goddards missions) address a broad range of scientific questions generally classified around four key areas: Earth sciences, astrophysics, heliophysics, and the solar system.[14] To simplify, Goddard studies Earth and Space.[15]

Within the Earth sciences area, Goddard plays a major role in research to advance our understanding of the Earth as an environmental system, looking at questions related to how the components of that environmental system have developed, how they interact and how they evolve. This is all important to enable scientists to understand the practical impacts of natural and human activities during the coming decades and centuries.

Within Space Sciences, Goddard has distinguished itself with the 2006 Nobel Physics Prize given to John Mather and the COBE mission. Beyond the COBE mission, Goddard studies how the universe formed, what it is made of, how its components interact, and how it evolves. The Center also contributes to research seeking to understand how stars and planetary systems form and evolve and studies the nature of the Suns interaction with its surroundings.

From Scientific Questions to Science Missions

Based on existing knowledge accumulated through previous missions, new science questions are articulated. Missions are developed in the same way an experiment would be developed using the scientific method. In this context, Goddard does not work as an independent entity but rather as one of the 10 NASA centers working together to find answers to these scientific questions.

Each mission starts with a set of scientific questions to be answered, a set of scientific requirements for the mission, which build on what has already been discovered by prior missions. Scientific requirements spell out the types data that will need to be collected. These scientific requirements are then transformed into mission concepts that start to specify the kind of spacecraft and scientific instruments need to be developed for these scientific questions to be answered.

Within Goddard, the Sciences and Exploration Directorate (SED) leads the center's scientific endeavors, including the development of technology related to scientific pursuits.

Collecting Data in Space Scientific Instruments

Some of the most important technological advances developed by Goddard (and NASA in general) come from the need to innovate with new scientific instruments in order to be able to observe or measure phenomena in space that have never been measured or observed before. Instrument names tend to be known by their initials. In some cases, the mission's name gives an indication of the type of instrument involved. For example, the James Webb Space Telescope is, as its name indicates, a telescope, but it includes a suite of four distinct scientific instruments: Mid Infrared Instrument (MIRI); Near Infrared Camera (NIRCam); Near Infrared Spectrograph (NIRSpec); Fine Guidance Sensor Tunable Filter Imager (FGS-TFI).[16] Scientists at Goddard work closely with the engineers to develop these instruments.

Typically, a mission consists of a spacecraft with an instrument suite (multiple instruments) on board. In some cases, the scientific requirements dictate the need for multiple spacecraft. For example, the Magnetospheric Multiscale Mission (MMS) will study reconnection, a 3-D process. In order to capture data about this complex 3-D process, a set of four spacecraft flying as a tetrahedron is being developed. Each spacecraft will carry an instrument suite consisting of four instruments. MMS is part of a larger program (Solar Terrestrial Probes) that studies the impact of the sun on the solar system.

Goddard's Scientific Collaborations

In many cases, Goddard works with partners (US Government agencies, aerospace industry, university-based research centers, other countries) that are responsible for developing the scientific instruments. In other cases, Goddard develops one or more of the instruments. The individual instruments are then integrated into an instrument suite which is then integrated with the spacecraft. In the case of MMS, for example, Southwest Research Institute (SwRI) is responsible for developing the scientific instruments and Goddard provides overall project management, mission systems engineering, the spacecraft, and mission operations.[17]

On the Lunar Reconnaissance Orbiter (LRO), six instruments have been developed by a range of partners. One of the instruments, the Lunar Orbiter Laser Altimeter (LOLA), was developed by Goddard. LOLA measures landing site slopes and lunar surface roughness in order to generate a 3-D map of the moon.[18]

The newest (as of October 2008) Mission to be managed by Goddard is MAVEN. MAVEN is the second mission within the Mars Scout Program that will explore the atmosphere of Mars in support of NASA's broader efforts to go to Mars. MAVEN will carry eight instruments to measure characteristics of Mars' atmospheric gases, upper atmosphere, solar wind, and ionosphere. Instrument development partners include the University of Colorado at Boulder, and the University of California, Berkeley. Goddard will contribute overall project management as well as two of the instruments, two magnetometers.

Managing Scientific Data

Once a mission is launched and reaches its destination, its instruments start collecting data. The data is transmitted back to earth where it needs to be analyzed and stored for future reference. Goddard manages large collections of scientific data resulting from past and ongoing missions.

The Earth Science Division hosts the Goddard Earth Science Data and Information Services Division (GES DISC).[19] It offers Earth science data, information, and services to research scientists, applications scientists, applications users, and students.

The National Space Science Data Center (NSSDC), created at Goddard in 1966, hosts a permanent archive of space science data, including a large collection of images from space.

Section 102(d) of the National Aeronautics and Space Act of 1958 calls for the establishment of long-range studies of the potential benefits to be gained from, the opportunities for, and the problems involved in the utilization of aeronautical and space activities for peaceful and scientific purposes. [20] Because of this mandate, the Technology Utilization Program was established in 1962 which required technologies to be brought down to Earth and commercialized in order to help the US economy and improve the quality of life.[21]

Documentation of these technologies that were spun off started in 1976 with Spinoff 1976.[22] Since then, NASA has produced a yearly publication of these spinoff technologies through the Innovative Partnerships Program Office.

Goddard Space Flight Center has made significant contributions to the US economy and quality of life with the technologies it has spun off. Here are some examples: Weather balloon technology has helped firefighters with its short-range radios; aluminized Mylar in satellites has made sports equipment more insulated; laser optics systems have transformed the camera industry and life detection missions on other planets help scientists find bacteria in contaminated food.[23]

The Goddard Space Flight Center maintains ties with local area communities through external volunteer and educational programs. Employees are encouraged to take part in mentoring programs and take on speaking roles at area schools. On Center, Goddard hosts regular colloquiums in engineering, leadership and science. These events are open to the general public, but attendees must sign up in advance to procure a visitors pass for access to the Centers main grounds. Passes can be obtained at the security office main gate on Greenbelt Road.

Goddard also hosts several different internship opportunities, including NASA DEVELOP at Goddard Space Flight Center.

Queen Elizabeth II of the United Kingdom and her husband Prince Philip, Duke of Edinburgh visited Goddard Space Flight Center on Tuesday, May 8, 2007. The tour of Goddard was near the end of the queen's visit to commemorate the 400th anniversary of the founding of Jamestown in Virginia. The queen spoke with crew aboard the International Space Station.[24]

Coordinates: 385949N 765054W / 38.99694N 76.84833W / 38.99694; -76.84833

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Goddard Space Flight Center - Wikipedia, the free encyclopedia

Welcome to the NSSDCA!

Welcome to the NASA Space Science Data Coordinated Archive, NASA's archive for space science mission data.

ESA's Gaia mission launched successfully on a Soyuz-Fregat rocket from Kourour, French Guiana at 09:12UT on 19December 2013. The mission is designed to measure the positions and velocity of roughly 1,000,000,000 stars as well as determine their temperature, composition, and other properties. More...

NASA's Wide-field Infrared Survey Explorer(WISE) satellite has released data from the first 57% of the sky surveyed during the mission. The satellite went into hibernation in early February2011, but its discoveries include 20 comets, more than 33,000 asteroids between Mars and Jupiter, and 133 near-Earth objects. More...

NASA's launch of the Interface Region Imaging Spectrograph (IRIS) spacecraft took place at 7:27p.m. on 27June 2013 (02:27UT, 28June) about 100miles from Vandenberg AFB. More...

Voyager 1 has encountered a region of spacecraft at the edge of our solar system that scientists believe is the last region the spacecraft will have to cross prior to entering interstellar space. More...

Five investigations have been selected as finalists for the next Discovery class missions. One or two will be chosen to fly as early as 2020. The finalists include two Venus missions, two asteroid missions, and an NEO mission. More...

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Welcome to the NSSDCA!

Project ATLANTA – Urban Heat Island Study

High Spatial Resolution Airborne Multispectral Thermal Infrared Data to Support Analysis and Modeling Tasks in EOS IDS Project ATLANTA

Dale A. Quattrochi (dale.quattrochi@msfc.nasa.gov), NASA, Global Hydrology and Climate Center, Huntsville, AL

Jeffrey C. Luvall (jeff.luvall@msfc.nasa.gov) , NASA, Global Hydrology and Climate Center, Huntsville, AL

Background

Project ATLANTA (ATlanta Land-use ANalysis: Temperature and Air-quality) as a newly-funded NASA EOS Interdisciplinary Science (IDS) investigation in 1996, seeks to observe, measure, model, and analyze how the rapid growth of the Atlanta, Georgia metropolitan area since the early 1970's has impacted the region's climate and air quality. The primary objectives for this research effort are: 1) To investigate and model the relationship between Atlanta urban growth, land cover change, and the development of the urban heat island phenomenon through time at nested spatial scales from local to regional; 2) To investigate and model the relationship between Atlanta urban growth and land cover change on air quality through time at nested spatial scales from local to regional; and 3) To model the overall effects of urban development on surface energy budget characteristics across the Atlanta urban landscape through time at nested spatial scales from local to regional. Our key goal is to derive a better scientific understanding of how land cover changes associated with urbanization in the Atlanta area, principally in transforming forest lands to urban land covers through time, has, and will, effect local and regional climate, surface energy flux, and air quality characteristics. Allied with this goal is the prospect that the results from this research can be applied by urban planners, environmental managers and other decision-makers, for determining how urbanization has impacted the climate and overall environment of the Atlanta area. It is our intent to make the results available from this investigation to help facilitate measures that can be applied to mitigate climatological or air quality degradation, or to design alternate measures to sustain or improve the overall urban environment in the future. Project ATLANTA is a multidisciplinary research endeavor and enlists the expertise of 8 investigators: Dale Quattrochi (PI) (NASA/Global Hydrology Center); Jeffrey Luvall (NASA/Global Hydrology and Climate Center); C.P. Lo (University of Georgia); Stanley Kidder (Colorado State University); Haider Taha (Lawrence Berkeley National Laboratory); Robert Bornstein (San Jose State University); Kevin Gallo (NOAA/NESDIS); and Robert Gillies (Utah State University).

Atlanta Urban Growth and Effects on Climate and Air Quality

In the last half of the 20th century, Atlanta, Georgia has risen as the premier commercial, industrial, and transportation urban area of the southeastern United States. The rapid growth of the Atlanta area, particularly within the last 25 years, has made Atlanta one of the fastest growing metropolitan areas in the United States. The population of the Atlanta metropolitan area increased 27% between 1970 and 1980, and 33% between 1980-1990 (Research Atlanta, Inc., 1993). Concomitant with this high rate of population growth, has been an explosive growth in retail, industrial, commercial, and transportation services within the Atlanta region. This has resulted in tremendous land cover change dynamics within the metropolitan region, wherein urbanization has consumed vast acreages of land adjacent to the city proper and has pushed the rural/urban fringe farther and farther away from the original Atlanta urban core. An enormous transition of land from forest and agriculture to urban land uses has occurred in the Atlanta area in the last 25 years, along with subsequent changes in the land-atmosphere energy balance relationships.

Air quality has degenerated over the Atlanta area, particularly in regard to elevations in ozone and emissions of volatile organic compounds (VOCs), as indicated by results from the Southern Oxidants Study (SOS) which has focused a major effort on measuring and quantifying the air quality over the Atlanta metropolitan region. SOS modeling simulations for Atlanta using U.S. Environmental Protection Agency (EPA) State Implementation Plan guidelines suggest that a 90% decrease in nitrogen oxide emissions, one of the key elements in ozone production, will be required to bring Atlanta into attainment with the present ozone standard (SOS, 1995).

Project ATLANTA Science Approach

The scientific approach we are using in relating land cover changes with modifications in the local and regional climate and in air quality, is predicated on the analysis of remote sensing data in conjunction with in situ data (e.g., meteorological measurements) that are employed to initialize local and regional-level numerical models of land-atmosphere interactions. Remote sensing data form the basis for quantifying how land covers have changed within the Atlanta metropolitan area through time from the mid-1970's, when Atlanta's dramatic growth began in earnest, to the present. These remotely sensed data will be used to provide input to numerical models that relate land cover change through time with surface energy flux and meteorological parameters to derive temporal models of how land cover changes have impacted both the climatology and the air quality over the Atlanta region. Current remote sensing data (i.e., data obtained during 1997) will be used to calibrate the models and as baseline data for extending the models to predict how prospective future land cover changes will effect the local and regional climate and air quality over the Atlanta-north Georgia region. Additionally, remote sensing data will be used as an indirect modeling method to describe urbanization and deforestation parameters that can be used to assess, as well as predict, the effects of land use changes on the local microclimate.

In concert with the remote sensing-based analysis and modeling of land cover changes is an extensive numerically-based modeling effort to better understand the cause-and-effect relationships between urbanization and trends in climatology and air quality. Sophisticated numerical meteorological models can complement extensive field monitoring projects and help improve our understanding of these relationships and the evolution of the urban climate on a location-specific basis. Measured data alone cannot resolve the relationships between the many causes of urban heat islands/urban climates and observations. For example, measured data cannot directly attribute a certain fraction of temperature rise to a certain modification in land use patterns, change in energy consumption, or release of anthropogenic heat into the atmosphere. These are aspects that numerical modeling can help resolve. Similarly, monitored air quality data cannot be used to establish a direct cause-and-effect relationship between emission sources, activities, or urbanization and observed air quality (e.g., smog). In this sense, photochemical models can be used in testing the sensitivity of ozone concentrations to changes in various land-use components, emission modifications and control, or other strategies. Thus, we are incorporating an assessment of land cover/land use change as measured from remote sensing data, with temporal numerical modeling simulations to better understand the effects that the growth of Atlanta has had on local and regional climate characteristics and air quality.

ATLAS Data: Role and Characteristics

To augment the quantitative measurements of land cover change and land surface thermal characteristics derived from satellite data (i.e, Landsat MSS and TM data for assessment of land cover change; Landsat TM thermal, and AVHRR and GOES data for land surface thermal characteristics), we are employing high spatial resolution airborne multispectral thermal data to provide detailed measurements of thermal energy fluxes that occur for specific surfaces (e.g., pavements, buildings) across the Atlanta urban landscape, and the changes in thermal energy response for these surfaces between day and night. This information is critical to resolving the underlying surface responses that lead to development of local and regional-scale urban climate processes, such as the urban heat island phenomenon and related characteristics. (Quattrochi and Ridd, 1994, 1997). These aircraft data will also be used to develop a functional classification of the thermal attributes of the Atlanta metropolitan area to better understand the energy budget linkages between the urban surface and the boundary layer atmosphere. This will be performed using the Thermal Response Number (TRN) (Luvall and Holbo, 1989; Luvall, 1997) which is expressed as

Where Rn is total net radiation and T change in surface temperature for time period t1 to t2.

Because urban landscapes are very complex in composition, the partitioning of energy budget terms depends on surface type. In natural landscapes, the partitioning is dependent on canopy biomass, leaf area index, aerodynamic roughness, and moisture status, all of which are influenced by the development stage of the ecosystem. In urban landscapes, however, the distribution of artificial or altered surfaces substantially modifies the surface energy budget. Thus, one key component of Project ATLANTA is to measure and model surface energy responses in both space and time, to better understand the processes-responses of urban climate and air quality interactions across the Atlanta metropolitan area.

The airborne sensor used to acquire high spatial resolution multispectral thermal infrared data over Atlanta is the Advanced Thermal and Land Applications Sensor (ATLAS), which is flown onboard a Lear 23 jet aircraft operated by the NASA Stennis Space Center. The ATLAS is a 15-channel multispectral scanner that basically incorporates the bandwidths of the Landsat TM (along with several additional channels) and 6 thermal IR channels similar to that available on the airborne Thermal Infrared Multispectral Scanner (TIMS) sensor (Table 1). Of particular importance to the Atlanta study is the multispectral thermal IR capability of the ATLAS instrument. ATLAS thermal IR data, collected at a very high spatial resolution, have been used to study urban surface energy responses in a previous study over the Huntsville, Alabama metropolitan area with excellent results (Lo et al., 1997).

ATLAS Data Collection

ATLAS data were collected over a 48 x 48 km2 area, centered on the Atlanta Central Business District (CBD) on May 11 and 12, 1997. An early May data acquisition window was selected to facilitate the collection of ATLAS data during the spring when vegetation canopy was filled out, surface temperatures were high enough to permit substantial heating of the urban landscape, and there was a high probability that cool fronts would still be moving through the Atlanta area to permit clear skies, as opposed to later in the spring or summer when increased cloud cover or convective storms become limiting factors in obtaining aircraft data. ATLAS data were collected at a 10m pixel spatial resolution during the daytime, between approximately 11:00 a.m. and 3:00 p.m. local time (Eastern Daylight Time) to capture the highest incidence of solar radiation across the city landscape around solar noon. ATLAS 10m data were also obtained the following morning (May 12) between 2:00-4:00 a.m. local time (Eastern Daylight Time) to measure the Atlanta urban surface during the coolest time of the diurnal energy cycle. Eleven flight lines were required to cover the 48 x 48 km2 area at a 10m spatial resolution. To permit the derivation of TRN values, all 11 daytime flight lines were flown and then repeated later at about a 2 hour interval. Nighttime overflights were not repeated because of the relative invariance in thermal energy fluxes at night which obviated the need to calculate TRNs.

Sky conditions at the time of the daytime overflights were mostly clear with some cirrus clouds present. The Lear jet aircraft flew at an altitude of 5,063m above mean terrain to achieve a 10m pixel resolution which was well below the cirrus clouds. Cirrus clouds covered the entire Atlanta metropolitan area during the night flights. The presence of cirrus cloud cover at night did, to some extent, dampen the cooling effect of thermal energy release to a clear sky, but air temperatures were still sufficiently cool to provide ample difference with daytime heating. Maximum air temperatures during the daytime overflights were approximately 25oC, while air temperature during the nighttime flights was around 10oC. Sample surface temperatures for tree-shaded grass, tree canopy, and asphalt in full sunlight recorded with a hand-held infrared thermometer (8-14 lm) during the afternoon were 28oC, 21oC, and 50oC, respectively. Daytime temperatures for a commercial building roof comprised of rock/membrane coating ranged from 49oC to 52oC. This illustrates that although air temperatures were cooler than optimal for development of the urban heat island effect, there was still significant heating by artificial urban surfaces to permit good contrast with nighttime cooling.

Atmospheric radiance must be accounted for in order to obtain calibrated surface temperatures. Although the ATLAS thermal channels fall within the atmospheric window for atmospheric longwave transmittance (8.0-13.0 m), the maximum transmittance is only about 80%. The amount of atmospheric radiance in the atmospheric window is mostly dependent on the atmospheric water vapor content, although there is an ozone absorption band around 9.5 m. To assist in obtaining accurate thermal surface energy response measurements from the ATLAS data, radiosonde launches were made concurrently with both the daytime and nighttime overflights. The atmospheric profiles obtained from these radiosonde data are then incorporated into the MODTRAN3 model for calculation of atmospheric radiance (Berk et al., 1989). The output from MODTRAN3 is combined with calibrated ATLAS spectral response curves and blackbody information recorded during the flight, using the Earth Resources Laboratory Applications Software (ELAS) module TRADE (Thermal Radiant Temperature) (Graham et al., 1986), to produce a look-up table for pixel temperatures as a function of ATLAS values (Anderson, 1992).

One pyranometer and one pyrgeometer were also stationed on a rooftop within one of aircraft flight lines for use in measuring incoming shortwave and longwave radiation within the study area. Additionally, two shadowband radiometers were placed in strategic locations within the flight path for use in measuring shortwave visible radiation for determining visibility parameters for input into MODTRAN3. The output from MODTRAN3 is combined with calibrated ATLAS spectral response curves and onboard calibration lamp information recorded during the flight in TRADE to produce calibrated at-sensor radiance for the visible wavelengths.

ATLAS Data: Some Examples

Approximately 5 Gb of raw (unprocessed) ATLAS data were collected during the May 11-12 aircraft overflights. In addition to the digital ATLAS data, color infrared aerial photography at 1:32,000 scale was obtained during daytime mission. Figure 1 illustrates daytime thermal (channel 13 - 9.60-10.2 m) ATLAS data collected over the Atlanta CBD area. Figure 2 provides an example of ATLAS data (channel 13) acquired during the night over the Atlanta CBD. Both images are oriented with north at the top. Excluding the effects of the highly variable emissivites of urban building materials, an empirical observation of the images presented in Figures 1 and 2 illustrates the wide range of thermal energy responses present across the Atlanta city landscape, as well as the detail that can be discerned from the 10m data. The Georgia Dome, an enclosed football stadium, appears as the large square-shaped structure due west of the Atlanta city center. Interstate highways 75/85 which traverse in a north-south direction around the city center, are seen as a dark "ribbon" on the day data (Figure 1) just to the east of downtown Atlanta. Just south of the city center, is the junction of Interstate Highways 75/85 and 20. Shadows from tall buildings located in the Atlanta city center can also be observed on the daytime data. In Figure 1, the intense thermal energy responses from buildings, pavements and other surfaces typical of the urban landscape, as well as the heterogeneous distribution of these responses, stand in significant contrast to the relative "flatness" of Atlanta thermal landscape at night (Figure 2). Also, the damping effect that the urban forest has on upwelling thermal energy responses is evident, particularly in the upper right side of the daytime image where residential tree canopy is extensive. In Figure 2, there is still evidence, even in the very early morning, of elevated thermal energy responses from buildings and other surfaces in the Atlanta CBD and from streets and highways. It appears that thermal energy responses for vegetation across the image are relatively uniform at night, regardless of vegetative type (e.g., grass, trees).

ATLAS Data Analysis: The Next Steps

From the images in Figures 1 and 2, it is apparent that high resolution ATLAS data offer a unique opportunity to measure, analyze and model the state and dynamics of thermal energy responses across the Atlanta metropolitan landscape. In addition to deriving energy balance measurements for day and night, and TRN values for specific urban surfaces to better understand the thermal characteristics that drive the development of the urban heat island phenomena and the overall Atlanta urban climate, these multispectral ATLAS data also exist as database record of current land cover/land use conditions for the Atlanta metropolitan area. Along with the extensive meteorological data available via a network of mesonet stations that are currently operating across the Atlanta area, the ATLAS data will be used to initialize and calibrate the meteorological and air quality models that will be run for the time period when the airborne data were collected. Moreover, one of the key facets from Project ATLANTA is to work with local planning agencies, such as the Atlanta Regional Commission (ARC), to model how the continued growth of Atlanta will impact the climate and air quality of the north Georgia region. The ARC is currently developing a 20-year growth plan for a 10 county area around Atlanta. Using the ATLAS data obtained in May, 1997 as a baseline for land cover/land use, our objective is to perform some "prospective" modeling on how meteorological conditions and air quality will change, predicated on the ARC's 20-year plan. By doing so, we hope to provide the ARC and other planning or decision-making bodies, with model output that can be used to modify or revise growth plans for the Atlanta metropolitan area, and to help mitigate or ameliorate the expansion of the urban heat island effect or the further deterioration in air quality.

References

Anderson, J. E., 1992. Determination of water surface temperature based on the use of thermal infrared multispectral scanner data. Geocarto International 3:3-8.

Berk, A., L. S. Bernstein, and D. C. Robertson., 1989: Modtran: A Moderate Resolution Model for Lowtran 7. U.S. Air Force Geophysics Laboratory, Environmental Research Papers GL-TR-89-0122, Hanscom Air Force Base, MA, 37 pp.

Graham, M.H., B.G. Junkin, M.T. Kalcic, R.W. Pearson and B.R. Seyfarth, 1986. ELAS - Earth resources laboratory applications software. Revised Jan.1986. NASA/NSTL/ERL Report No. 183.

Lo, C.P., D.A. Quattrochi, and J.C. Luvall, 1997. Application of high-resolution thermal infrared remote sensing and GIS to assess the urban heat island effect. International Journal of Remote Sensing 18:287-304.

Luvall, J.C., and H. R. Holbo, 1989: Measurements of short-term thermal responses of coniferous forest canopies using thermal scanner data. Remote Sensing of Environment, 27, 1-10.

Luvall, J.C., 1997. The use of remotely sensed surface temperatures from an aircraft-based thermal infrared multispectral scanner (TIMS) to estimate the spatial and temporal variability of latent heat fluxes and thermal response numbers from a white pine (Pinus strobus L.) plantation. In Scale in Remote Sensing and GIS, D.A. Quattrochi and M.F. Goodchild, eds. CRC/Lewis Publishers, Boca Raton, FL, pp.169-185.

Quattrochi, D.A. and M.K. Ridd, 1994. Measurement and analysis of thermal energy responses from discrete urban surfaces using remote sensing data. International Journal of Remote Sensing 15:1991-2022.

Quattrochi, D.A. and M.K. Ridd, 1997. Analysis of vegetation within a semi-arid urban environment using high spatial resolution airborne thermal infrared remote sensing data. Atmospheric Environment (In press).

Research Atlanta, Inc., 1993: The Dynamics of Change: An Analysis of Growth in Metropolitan Atlanta over the Past Two Decades. Policy Research Center, Georgia State University, Atlanta.

SOS, 1995. The State of the Southern Oxidants Study: Policy-Relevant Findings in Ozone Pollution Research 1988-1994. Southern Oxidants Study: Raleigh, NC, 94 pp.

Figure Captions

Figure 1. ATLAS daytime thermal image (channel 13 -- 9.60-10.2 m) of the Atlanta central business district area. These data have not been geometrically or atmospherically corrected.

Figure 2. ATLAS nighttime thermal image (channel 13 -- 9.60-10.2 m) of the Atlanta central business district area. These data have not been geometrically or atmospherically corrected.

Global Hydrology and Climate Center

Responsible Official: Dr. Steven J. Goodman (steven.goodman@nasa.gov) Page Curator: Paul J. Meyer (paul.meyer@msfc.nasa.gov)

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Project ATLANTA - Urban Heat Island Study

Space Center Houston – Visit Houston Texas

Space Center Houston, the official visitors center for NASA's Johnson Space Center, is the only place on earth where guests can embark on an out-of-this-world journey through human adventures in space.

Space Center Houston features a multitude of permanent exhibits, attractions and theaters. In addition, the venue presents an array of traveling exhibits and events created exclusively by Space Center Houston's creative exhibit team.

NEW: The space shuttle replica Independence is now on display at Space Center Houston. The 122-foot, 130,000-pound wooden replica is being restored so the public can go inside the capsule and it's NASA 747 carrier aircraft as part of a behind-the-scenes look at life inside a space shuttle, an experience only available at Space Center Houston. The exhibit is currently under construction and will be open to the public January 23, 2016. Guests can currently see the outside of the replica, which is positioned in front of the Space Center building.

Both the shuttle and carrier will feature interior exhibits featuring the flight deck and cockpit of the shuttle, astronaut living quarters mid-deck, history on the development of the shuttle program, and how the carrier aircraft docks with shuttles. Visitors walking through the payload bay will even get to see a recently returned artifact from STS-49, a space satellite rescue mission.

Independence Plaza will be the worlds first and only shuttle/carrier replica open to the public when it debuts January 23. The exhibit is the largest project Space Center Houston has taken on since it was founded in 1992. Along with original artifacts and history, the complex will offer educational workshops and problem-solving activities for those interested in science, mathematics, and engineering careers. At the final leg, guests will see a film covering the history of space shuttle program as well as a special tribute to the crew members of the Challenger and Columbia missions.

Visitors to Space Center Houston can experience the monumental exhibit at no extra charge as part of museum general admission. Timed ticketing will ensure that a manageable number of guests can access the shuttles smaller space at different intervals.

Permanent Exhibits Blast Off Blast-Off is an unparalleled multi-media sensory experience. Visitors encounter a dramatic high-definition audio/video extravaganza culminating in a dynamic space shuttle blast off.

Living in Space Living in Space is a hands-on exhibit where guests can test their skills at landing the shuttle or retrieving a satellite through interactive computer simulators. A Mission Briefing Officer receives help from an audience participant in a live presentation showing how astronauts handle daily activities like showering, sleeping and preparing meals in space.

The NASA Tram Tour With this behind-the-scenes journey through NASA's Johnson Space Center, you may visit the Historic Mission Control Center, the Space Vehicle Mockup Facility or the current Mission Control Center. Before returning to Space Center Houston, you can visit the "all new" Saturn V Complex at Rocket Park. Occasionally, the tour may visit other facilities, such as the Sonny Carter Training Facility or Neutral Buoyancy Laboratory. You may even get to see astronauts training for upcoming missions.

The Astronaut Gallery This unparalleled exhibit features spacesuits dating back to the first American trip to space and a wall that contains portraits and crew photos of every U.S. astronaut who has flown in space.

Mission Status Mission briefing officers provide live updates on current space flights and astronaut training activities. Guests can listen to communications between Mission Control and astronaut crews aboard the space shuttle. A live video shows a behind-the-scenes view of activities in the Johnson Space Center and a satellite link of a shuttle launch via Kennedy Space Center of Florida.

The Martian Matrix Four stories of out-of-this-world fun for kids, Pepsi's Martian Matrix is an action-packed play area with a space theme. Slides, swings and foam ball battles are just a few of the featured activities.

Kids Space Place Interactive stations and themed areas give children a chance to explore and investigate the different aspects of space exploration. Jumping on the Moon, manning the space shuttle, building a rocket and flying in space are all a part of the growing exhibit.

Starship Gallery On Human Destiny is shown in the Starship Gallery, which highlights great moments in space exploration. The gallery contains artifacts and hardware from the Mercury program through Apollo-Soyuz, including a special Lunar Vault. The New Explorers video wall shares the visions of today's NASA engineers and scientists.

Greater Houston Convention and Visitors Bureau - Member

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Space Center Houston - Visit Houston Texas

Near-Earth Object Program

Earth Flyby of 'Space Peanut' Captured in New Video (1999 JD6) July 31, 2015

NASA scientists have used two giant, Earth-based radio telescopes to bounce radar signals off a passing asteroid and produce images of the peanut-shaped body as it approached close to Earth this past weekend. The images show the rotation of the asteroid, named 1999 JD6, which made its closest approach on July 24 at 9:55 p.m. PDT (12:55 a.m. EDT on July 25) at a distance of about 4.5 million miles (7.2 million kilometers, or about 19 times the distance from Earth to the moon).

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Asteroid Icarus will safely pass by Earth at more than 21 times the distance of Earth to the moon on June 16. To put it another way, Icarus, one of the first near-Earth asteroids ever discovered (1949), will approach no closer than five million miles away (eight million kilometers).

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An asteroid, designated 1999 FN53, will safely pass more than 26 times the distance of Earth to the moon on May 14. To put it another way, at its closest point, the asteroid will get no closer than 6.3 million miles away (10 million kilometers). It will not get closer than that for well over 100 years. And even then, (119 years from now) it will be so far away it will not affect our planet in any way, shape or form. 1999 FN53 is approximately 3,000 feet (1 kilometer) across.

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NASA announced more details on its plan for its Asteroid Redirect Mission (ARM), which in the mid-2020s will test a number of new capabilities needed for future human expeditions to deep space, including to Mars. NASA also announced it has increased the detection of near-Earth asteroids by 65 percent since launching its asteroid initiative three years ago. For ARM, a robotic spacecraft will capture a boulder from the surface of a near-Earth asteroid and move it into a stable orbit around the moon for exploration by astronauts, all in support of advancing the nation's journey to Mars.

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On January 18, 2015 - a little over four years since the NHATS assessments began - the 1332nd NHATS-compliant asteroid was identified, doubling the number of known accessible NEAs.

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Scientists working with NASA's 230-foot-wide (70-meter) Deep Space Network antenna at Goldstone, California, have released the first radar images of asteroid 2004 BL86. The images show the asteroid, which made its closest approach today (Jan. 26, 2015) at 8:19 a.m. PST (11:19 a.m. EST) at a distance of about 745,000 miles (1.2 million kilometers, or 3.1 times the distance from Earth to the moon), has its own small moon.

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Updated Animation (January 30, 2015)

New orbital chart and star charts are now available.

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An asteroid, designated 2004 BL86, will safely pass about three times the distance of Earth to the moon on January 26. From its reflected brightness, astronomers estimate that the asteroid is about a third of a mile (0.5 kilometers) in size. The flyby of 2004 BL86 will be the closest by any known space rock this large until asteroid 1999 AN10 flies past Earth in 2027.

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Some recent press reports have suggested that an asteroid designated 2014 UR116 represents an impact threat to the Earth. The asteroid does not represent a threat because it's orbital path does not pass sufficiently close to the Earth's orbit.

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Small asteroids near Earth, with sizes of only about a meter, hit the atmosphere and disintegrate with surprising frequency - around every other week, new data show.

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Small meteorite impact reported in Nicaragua is unrelated to Asteroid 2014 RC. 2014 RC has a rotation rate of 15.8 seconds - the fastest rotating asteroid ever observed.

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A small asteroid, designated 2014 RC, will safely pass very close to the Earth on Sunday, 7 September 2014. From its brightness, astronomers estimate that the asteroid is about 20 meters (60 feet) in size

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Agency officials announced on Thursday, June 19, recent progress to identify candidate asteroids for its Asteroid Redirect Mission (ARM), increase public participation in the search for asteroids, and advance the mission's design.

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NASA scientists using Earth-based radar have produced sharp views of a recently discovered asteroid 2014 HQ124 as it slid silently past our planet. The new views are some of the most detailed radar images of a near-Earth asteroid ever obtained.

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A large newfound asteroid - 2014 HQ124 - will safely pass Earth on June 8 from a distance of about 777,000 miles (1.25 million kilometers), more than three times farther away than our moon.

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NASA is sponsoring a series of virtual seminars on the properties of Near Earth Asteroids (NEAs) and what is being done to learn more about the hazards and the opportunities they may pose for us here on Earth.

Seminars Link

Recent observations have removed from NASA's asteroid impact hazard list the near-Earth object (NEO) known to pose the most significant risk of Earth impact over the next 100 years.

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An asteroid about 25 feet (8 meters) across will safely pass Earth at about 1:21 p.m. PST (4:21 p.m. EST) today, March 6, approaching us six times closer than the moon.

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As happens about 20 times a year with current detection capabilities, a known asteroid will safely pass Earth Wednesday closer than the distance from Earth to the moon.

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Radar images of asteroid 2006 DP14 reveal it is a peanut-shaped space rock.

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As the next step in advancing NASA's asteroid initiative, the agency will host an Opportunities Forum March 26, 2014 at NASA Headquarters in Washington.

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NASA is developing an Asteroid Redirect Mission (ARM) -- a first-ever mission to identify, capture and redirect an asteroid to a safe orbit of Earth's moon for future exploration by astronauts in the 2020s.

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NASA's Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE) spacecraft has spotted a never-before-seen asteroid -- its first such discovery since coming out of hibernation last year.

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Several sources confirm that the first discovered asteroid of 2014, designated 2014 AA, entered the Earth's atmosphere late January 1 EST over the mid-Atlantic Ocean.

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The first asteroid discovered in 2014 has entered Earth's atmosphere on January 2nd over the ocean off the coast of West Africa.

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Two surprisingly large Near-Earth Asteroids have been discovered in just the last week or so, as well as a third moderately large asteroid which surprisingly has also gone undetected until now, even though it can pass close enough to the Earth to be classified as "potentially hazardous".

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Near-Earth Object Program

NASA/JPL Solar System Simulator

Targets and Date Show me the Solar System the Sun Mercury Venus Earth ...the Moon Mars ...Phobos ...Deimos Jupiter ...Io ...Europa ...Ganymede ...Callisto Saturn ...Mimas ...Enceladus ...Tethys ...Dione ...Rhea ...Titan ...Hyperion ...Iapetus ...Phoebe Uranus ...Ariel ...Umbriel ...Titania ...Oberon ...Miranda Neptune ...Triton ...Nereid Pluto ...Charon Dawn Messenger Mars Science Laboratory Spitzer (SIRTF) Rosetta Mars Orbiter Mission Juno Cassini New Horizons Voyager 1 Voyager 2 Pioneer 10 Pioneer 11 Phoenix Ulysses 1 Ceres 4 Vesta as seen from above below the Sun Mercury Venus Earth ...the Moon Mars ...Phobos ...Deimos Jupiter ...Io ...Europa ...Ganymede ...Callisto Saturn ...Mimas ...Enceladus ...Tethys ...Dione ...Rhea ...Titan ...Hyperion ...Iapetus ...Phoebe Uranus ...Ariel ...Umbriel ...Titania ...Oberon ...Miranda Neptune ...Triton ...Nereid Pluto ...Charon Dawn Messenger Mars Science Laboratory Spitzer (SIRTF) Rosetta Mars Orbiter Mission Juno Cassini New Horizons Voyager 1 Voyager 2 Pioneer 10 Pioneer 11 Phoenix Ulysses 1 Ceres 4 Vesta On Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 in the year 1990 1991 1992 1993 1994 1995 1996 1997 1998 1999 2000 2001 2002 2003 2004 2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 2016 2017 2018 2019 2020 2021 2022 2023 2024 2025 at 00 01 02 03 04 05 06 07 08 09 10 11 12 13 14 15 16 17 18 19 20 21 22 23 :00 :05 :10 :15 :20 :25 :30 :35 :40 :45 :50 :55 UTC Field of View (choose one) I want a field of view of 120 90 60 45 30 20 10 5 2 1 0.5 0.2 0.1 0.05 0.02 0.01 0.005 0.002 0.001 0.0005 0.0002 0.0001 degree(s) I want the body to take up 100 90 80 70 60 50 40 30 20 10 5 2 1 percent of the image width Options (choose any) -orbits -extra brightness -show all spacecraft

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NASA/JPL Solar System Simulator

Universal Electro Systems Company TVX Unregistered Nonprofit Official Nasa Venezuela – Video


Universal Electro Systems Company TVX Unregistered Nonprofit Official Nasa Venezuela
Sistemas Electro Universal Tvx Empresa No Registrada Sin Fines De Lucro Logo Oficial Nasa Venezuela Operador Alexis Jos Morillo Anlisis de los primitivos humanos el amor por el dinero...

By: Alexis Morillo

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Universal Electro Systems Company TVX Unregistered Nonprofit Official Nasa Venezuela - Video

NASA julia Belechak Course Video Assignmt News packages for Students’ Live Newscast – Video


NASA julia Belechak Course Video Assignmt News packages for Students #39; Live Newscast
This NASA video was part of the JMA 449 Newsroom Operations Class where each student, each week, is required to produce News packages for their Live Newscast. Student Julia Belechak ...

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NASA to Celebrate MESSENGER Mission Prior to Surface Impact of Mercury

NASA will hold a media and public event at 1 p.m. EDT on Thursday, April 16, to share scientific findings and technical accomplishments of the agencys MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft.

After more than 10 years in space, the highly successful mission will come to an end when it is expected to collide into Mercury at a speed of more than 8,750 miles per hour (3.91 km/sec) near the end of this month.

The event will take place in the NASA Headquarters' James E. Webb Auditorium, 300 E Street, S.W., Washington, and will be carried live on NASA Television and the agencys website.

Launched in August 2004, MESSENGER traveled 4.9 billion miles (7.9 billion kilometers) - a journey that included 15 trips around the sun and flybys of Earth once, Venus twice, and Mercury three times - before it was inserted into orbit around its target planet in March 2011. The spacecraft's cameras and other sophisticated, high-technology instruments have collected unprecedented images and made other observations. Mission managers are preparing to impact Mercury surface in the next couple weeks.

Participants will include:

James Green, director, Planetary Science Division, NASA Headquarters, Washington

Sean Solomon, MESSENGER principal investigator; director, Columbia University's Lamont-Doherty Earth Observatory, Palisades, New York

Helene Winters, MESSENGER project manager, Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland

Daniel OShaughnessy, MESSENGER systems engineer, Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland

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NASA to Celebrate MESSENGER Mission Prior to Surface Impact of Mercury

NASA catches Tropical Cyclone Solo dissipating

IMAGE:On April 13, the MODIS instrument aboard NASA's Aqua satellite captured this visible-light image of Solo's elongated remnants. The bulk of clouds were southeast of the barely discernable center.... view more

Tropical Cyclone Solo was dissipating over the Southwestern Pacific Ocean when NASA's Aqua satellite passed overhead on April 13, 2015.

On April 11 Tropical Cyclone Solo spawned warnings in New Caledonia as it passed by. By April 12, the warnings were dropped and wind shear had taken its toll on the storm weakening it.

On April 12 at 0300 UTC (April 11 at 11 p.m. EDT), the Joint Typhoon Warning Center (JTWC) issued their final bulletin on Solo. At that time it was 116 nautical miles north of Noumea, New Caledonia near 20.2 south latitude and 165.7 east longitude. Solo had maximum sustained winds near 35 knots (40 mph/64 kph) and weakening. Solo was moving to the east-southeast at 18 knots (20.7 mph/33.3 kph).

As Solo continued in an east-southeasterly direction and passed New Caledonia, strong vertical wind shear weakened the storm to a remnant low pressure area. NASA's Aqua satellite passed over Solo's remnants on April 13 and the MODIS (Moderate Resolution Imaging Spectroradiometer) instrument aboard captured a visible-light image of it. The MODIS image revealed that the remnants had become an elongated system with the bulk of clouds pushed southeast of the barely discernable center. Solo continued to dissipate under the strong vertical wind shear.

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NASA catches Tropical Cyclone Solo dissipating

NASA Invites ESA to Attempt Europa Landing

If there's one place in the solar system where were likely to find extraterrestrial life, its Europa. The Jovian moon is covered in ice, almost certainly has liquid water oceans underneath, and tidal forces from Jupiter drivegeologic activity to keepeverything warm.

Considering that finding aliens (even if theyre just microbes)would be (or will be) one of the most profound discoveries that anyone has ever made, ever, its a little weird that weve managed to send a few dozen spacecraft to Mars, and not a single one to Europa. NASA has had Europa missions scrapped over and over by budget cuts, but it now looks as though the agency will be putting a Europa Clipper mission together starting later this year. NASA wont be incorporating a lander into the Clipper, but they've asked the European Space Agency if theyre interested in sending one along for the ride.We could be looking at the very first Europa landing attempt.

NASAsEuropa Clipper would launch in the early2020s and head straight for Jupiter, spending about eight years in transit. On arrival, rather than try to orbit Europa, the Clipper would loop into a fancy orbit around Jupiter that it would swing it past Europa as many as 45 times, giving us an excellent look at the moon (from altitudes as low as 25 kilometers)over the course of several years, or until Jupiter's radiation fries the Clipper to a crisp.

Since NASA doesnt have the budget for the fancy life-detecting roboticlander/submarine that we all want, they've asked ESA if the agency wants to sendits lander along for the ride. NASA might be a little wary of sending a lander if they're fans of Arthur C. Clarke (and Im sure they are), but besides budgetary constraints, ESA also already has some experience dropping probes onto the moons of gas giants.

Ten years ago, ESAs Cassini spacecraft launched a small probe called Huygens toward Titan, one of the moons of Saturn. Even though Huygens wasnt really intended to be a lander,but more of an atmospheric probe, it managed to survive entry into Titans atmosphere, descent, and a touchdown on the surface, where it continued to send back data for an hour and a half, despite an expected design life of just a few minutes.

Specifically, NASA has asked ESA to consider a surface lander or even a surface penetrator for the Europa mission. For its part, ESA seems open to the idea, especially since theyre already planning to launch their ownJUpiter ICy moons Explorer (JUICE) mission to study Europa, Ganymede, and Callisto in 2022.

The next step is for ESA to decide whether it wants to be involved in the Clipper mission, and if so, what exactly its involvement will consist of. NASA expects to make some sort of announcement regarding the science payload of the Europa Clipper within the next few weeks, and final instrument selection will (hopefully) happen by next year.

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NASA Invites ESA to Attempt Europa Landing

NASA-funded Study Explains Saturn's Epic Tantrums

The long-standing mystery of why Saturn seethes with enormous storms every 30 years may have been solved by scientists working with data from NASA's Cassini mission. The tempests, which can grow into bright bands that encircle the entire planet, are on a natural timer that is reset by each subsequent storm, the researchers report.

In 140 years of telescope observations, great storms have erupted on Saturn six times. Cassini and observers on Earth tracked the most recent of these storms from December 2010 to August 2011. During that time, the storm exploded through the clouds, eventually winding its way around Saturn.

In a paper published online today in the journal Nature Geoscience, scientists describe the effect they believe is responsible for the periodic outbursts. The basic idea is that water vapor is heavier than the hydrogen and helium that make up the bulk of Saturn's atmosphere, so once each giant storm dumps its huge mass of rain, the air within the clouds is left lighter than the atmosphere below. For a time, this situation shuts off the process of convection -- in which warm, moist air rises, and cool, dense air sinks -- that creates new clouds and storms.

"For decades after one of these storms, the warm air in Saturn's deep atmosphere is too wet, and too dense, to rise," said Cheng Li, a graduate student at the California Institute of Technology in Pasadena, who led the study. "The air above has to cool off, radiating its heat to space, before its density is greater than that of the hot, wet air below. This cooling process takes about 30 years, and then come the storms."

Li thinks the episodic nature of the storms indicates Saturn's deep atmosphere contains more water, relative to the other atmospheric constituents, than Jupiter. The researchers suggest Saturn's extra-wet interior might explain why the planet has such epic tantrums, whereas Jupiter does not. If Saturn's deep atmosphere were drier, scientists would expect continuous, smaller storms, as observed on Jupiter, Li said. Instead, Saturn's outbursts are episodic and quite explosive.

Other observations by ground and space-based telescopes have hinted at a wet interior for Saturn. "Previous studies using spectroscopy have shown that Saturn's interior is enriched in methane and other volatiles, by two or three times, compared to Jupiter. From there, it's a short leap to expect that Saturn is also rich in oxygen, which is also a volatile and a big part of every H2O molecule," said Andrew Ingersoll, a member of the Cassini science team, also at Caltech, who co-authored the paper with Li. Volatiles are elements and chemical compounds that change from solid to liquid or gas at relatively low temperatures.

Scientists are interested in understanding the amount of oxygen and other volatile ingredients in Saturn and Jupiter. These ingredients provide important clues about the formation of the two planets -- which are thought to have formed before all the others -- and conditions in the early solar system.

The Cassini-Huygens mission is a cooperative project of NASA, ESA (European Space Agency) and the Italian Space Agency. JPL, a division of Caltech, manages the mission for NASA's Science Mission Directorate in Washington.

For previous news and images related to Saturn's giant storm: http://go.nasa.gov/1H89e3p

For more information about Cassini, visit: http://www.nasa.gov/cassini http://saturn.jpl.nasa.gov

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NASA-funded Study Explains Saturn's Epic Tantrums