Melanie Moses, a professor of computer science at the University of New Mexico, presents a small replica of a Swarmie robot to Theresa Martinez, engagement manager of the Minority University Research and Education Program, during an awards ceremony at the Kennedy Space Center Visitor Complex in Florida on June 12, 2019. Swarmathon University Competition students and their mentors were at Kennedy to participate in a student/mentor panel, hear from speakers, get a behind-the-scenes tour of Kennedy Space Center, dine with an astronaut and receive awards. During Swarmathon University Challenge IV, students developed algorithms for robotic swarms that are robust and adaptable like the foraging strategies of ant colonies. The fourth and final Swarmathon was a combined virtual and physical competition, hosted by the University of New Mexico.
Swarmathon University Competition 2019 organizers, mentors, guest speakers and student teams gather for a group photo on June 11, 2019 at the Kennedy Space Center Visitor Complex in Florida. The University of New Mexico was the host for the physical competition held in May 2019. The student teams were at Kennedy to participate in a student/mentor panel, hear from speakers, get a behind-the-scenes tour of Kennedy Space Center, dine with an astronaut and receive awards during an awards ceremony. During Swarmathon University Challenge IV, students developed algorithms for robotic swarms that are robust and adaptable like the foraging strategies of ant colonies. The fourth and final Swarmathon was a combined virtual and physical competition.
Retired NASA astronaut John Blaha talks to Swarmathon University Challenge students and their mentors during a Dine with an Astronaut event at the Kennedy Space Center Visitor Complex in Florida on June 12, 2019. Students and mentors from some of the Swarmathon teams were at Kennedy to participate in a student/mentor panel, hear from speakers, get a behind-the-scenes tour of Kennedy Space Center, dine with an astronaut and receive awards. For the challenge, university students developed algorithms for robotic swarms that are robust and adaptable like the foraging strategies of ant colonies. The fourth and final Swarmathon challenge was a combined virtual and physical competition hosted by the University of New Mexico.
Retired NASA astronaut John Blaha talks to Swarmathon University Challenge students and their mentors during a Dine with an Astronaut event at the Kennedy Space Center Visitor Complex in Florida on June 12, 2019. Students and mentors from some of the Swarmathon teams were at Kennedy to participate in a student/mentor panel, hear from speakers, get a behind-the-scenes tour of Kennedy Space Center, dine with an astronaut and receive awards. For the challenge, university students developed algorithms for robotic swarms that are robust and adaptable like the foraging strategies of ant colonies. The fourth and final Swarmathon challenge was a combined virtual and physical competition hosted by the University of New Mexico.
During an awards ceremony on June 12, 2019 at the Kennedy Space Center Visitor Complex in Florida, mentors and volunteers from Kennedy received certificates of recognition for the NASA Swarmathon 2019 University Challenge. Second from right is Melanie Moses, a professor of computer science at the Swarmathon host location, University of New Mexico. At far right is Theresa Martinez, engagement manager of the Minority University Research and Education Program, managed at Kennedy. University students and their mentors were at Kennedy to participate in a student/mentor panel, hear from speakers, get a behind-the-scenes tour of Kennedy Space Center, dine with an astronaut and receive awards. During Swarmathon University Challenge IV, students developed algorithms for robotic swarms that are robust and adaptable like the foraging strategies of ant colonies. The fourth and final Swarmathon was a combined virtual and physical competition.
The Swarmathon team from the University of Puerto Rico at Arecibo received the Best Poster Award during the awards ceremony for NASA’s Swarmathon University Challenge IV, at the Kennedy Space Center Visitor Complex in Florida on June 12, 2019. Students and mentors from some of the Swarmathon teams were at Kennedy to participate in a student/mentor panel, hear from speakers, get a behind-the-scenes tour of Kennedy Space Center, dine with an astronaut and receive awards. For the challenge, university students developed algorithms for robotic swarms that are robust and adaptable like the foraging strategies of ant colonies. The fourth and final Swarmathon challenge was a combined virtual and physical competition. Fourth from right is Melanie Moses, a professor of computer science at the University of New Mexico, the host location for Swarmathon. Second from right is Theresa Martinez, engagement manager of the Minority University Research and Education Program, managed at Kennedy.
The University of New Mexico (UNM) faculty and students who administer the Swarmathon University Competition 2019 gather for a group photo on June 11, 2019 at the Kennedy Space Center Visitor Complex in Florida. Melanie Moses, faculty lead for Swarmathon and a professor of computer science at UNM, is second from left. Behind her is Theresa Martinez, Minority University Research and Education Program (MUREP) Science, Technology, Education and Math (STEM) engagement manager, at Kennedy Space Center. Swarmathon University Competition students and their mentors were at Kennedy to participate in a student/mentor panel, hear from speakers, get a behind-the-scenes tour of Kennedy Space Center, dine with an astronaut and receive awards. During Swarmathon University Challenge IV, students developed algorithms for robotic swarms that are robust and adaptable like the foraging strategies of ant colonies. The fourth and final Swarmathon was a combined virtual and physical competition, hosted by UNM.
The Swarmathon University Competition 2019 team members from the University of Maryland participate in activities at the Kennedy Space Center Visitor Complex in Florida on June 11, 2019. They are standing in front of a poster they created for the poster competition portion of Swarmathon. The University of New Mexico was the host for the physical competition held in May 2019. The student teams were at Kennedy to participate in a student/mentor panel, hear from speakers, get a behind-the-scenes tour of Kennedy Space Center, dine with an astronaut and receive awards during an awards ceremony. During Swarmathon University Challenge IV, students developed algorithms for robotic swarms that are robust and adaptable like the foraging strategies of ant colonies. The fourth and final Swarmathon was a combined virtual and physical competition.
The Swarmathon team from Cabrillo College received first place in NASA’s Swarmathon University Challenge IV, during a ceremony at the Kennedy Space Center Visitor Complex in Florida on June 12, 2019. Students and mentors from some of the Swarmathon teams were at Kennedy to participate in a student/mentor panel, hear from speakers, get a behind-the-scenes tour of Kennedy Space Center, dine with an astronaut and receive awards. For the challenge, university students developed algorithms for robotic swarms that are robust and adaptable like the foraging strategies of ant colonies. The fourth and final Swarmathon challenge was a combined virtual and physical competition. At far right is Melanie Moses, a professor of computer science at the University of New Mexico, the host location for Swarmathon. Third from left is Theresa Martinez, engagement manager of the Minority University Research and Education Program, managed at Kennedy.
NMTSat is a student-built satellite built by undergraduate and graduates students primarily from New Mexico Tech. NMTSat is designed to operate five sensors in four experiments in space for 3 months of data collection. The experiments will provide data on earth’s magnetic field, high altitude plasma density, atmospheric weather measurements, and an optical beacon experiment. Approximately 50 students have contributed to NMTSat and its design not including the students and groups who have developed the science instruments. NMTSat CubeSat is providing the opportunity for these science experiments to be conducted on orbit and demonstrates the collaborative nature of the Educational Launch of Nano Satellite (ELaNa) Program at NASA. The instruments have been contributed by New Mexico Tech, Turabo University in Puerto Rico, Los Alamos National Laboratory, and Atmospheric and Space Technology Research Associates (ASTRA) in Boulder, CO. Dr. Anders M. Jorgensen, Associate Professor at New Mexico Tech is the PI and Dr. Hien Vo from Vietnamese-German University in Ho Chi Minh University in Vietnam is a Co-Investigator. NMTSat is funded by the New Mexico NASA EPSCoR program as well as New Mexico Tech.
NMTSat is a student-built satellite built by undergraduate and graduates students primarily from New Mexico Tech. NMTSat is designed to operate five sensors in four experiments in space for 3 months of data collection. The experiments will provide data on earth’s magnetic field, high altitude plasma density, atmospheric weather measurements, and an optical beacon experiment. Approximately 50 students have contributed to NMTSat and its design not including the students and groups who have developed the science instruments. NMTSat CubeSat is providing the opportunity for these science experiments to be conducted on orbit and demonstrates the collaborative nature of the Educational Launch of Nano Satellite (ELaNa) Program at NASA. The instruments have been contributed by New Mexico Tech, Turabo University in Puerto Rico, Los Alamos National Laboratory, and Atmospheric and Space Technology Research Associates (ASTRA) in Boulder, CO. Dr. Anders M. Jorgensen, Associate Professor at New Mexico Tech is the PI and Dr. Hien Vo from Vietnamese-German University in Ho Chi Minh University in Vietnam is a Co-Investigator. NMTSat is funded by the New Mexico NASA EPSCoR program as well as New Mexico Tech.
NMTSat is a student-built satellite built by undergraduate and graduates students primarily from New Mexico Tech. NMTSat is designed to operate five sensors in four experiments in space for 3 months of data collection. The experiments will provide data on earth’s magnetic field, high altitude plasma density, atmospheric weather measurements, and an optical beacon experiment. Approximately 50 students have contributed to NMTSat and its design not including the students and groups who have developed the science instruments. NMTSat CubeSat is providing the opportunity for these science experiments to be conducted on orbit and demonstrates the collaborative nature of the Educational Launch of Nano Satellite (ELaNa) Program at NASA. The instruments have been contributed by New Mexico Tech, Turabo University in Puerto Rico, Los Alamos National Laboratory, and Atmospheric and Space Technology Research Associates (ASTRA) in Boulder, CO. Dr. Anders M. Jorgensen, Associate Professor at New Mexico Tech is the PI and Dr. Hien Vo from Vietnamese-German University in Ho Chi Minh University in Vietnam is a Co-Investigator. NMTSat is funded by the New Mexico NASA EPSCoR program as well as New Mexico Tech.
Proteus DSA control room in Mojave, CA (L to R) Jean-Pierre Soucy; Amphitech International Software engineer Craig Bomben; NASA Dryden Test Pilot Pete Siebold; (with headset, at computer controls) Scaled Composites pilot Bob Roehm; New Mexico State University (NMSU) UAV Technical Analysis Application Center (TAAC) Chuck Coleman; Scaled Composites Pilot Kari Sortland; NMSU TAAC Russell Wolfe; Modern Technology Solutions, Inc. Scaled Composites' unique tandem-wing Proteus was the testbed for a series of UAV collision-avoidance flight demonstrations. An Amphitech 35GHz radar unit installed below Proteus' nose was the primary sensor for the Detect, See and Avoid tests.
KENNEDY SPACE CENTER, FLA. - Gregg Buckingham, University Affairs officer, External Relations and Business Development Directorate, addresses students of MESA, the New Mexico Mathematics, Engineering and Science Achievement Program. The students are visiting KSC, touring facilities and meeting with mentors. MESA students, high school seniors who hold grade-point averages of at least 3.2 and who tutor other students in math and science, have made the spring trip for the past 14 years. The MESA program has close ties to the NASA Training Project at the University of New Mexico.
KENNEDY SPACE CENTER, FLA. -- Gregg Buckingham, University Affairs officer, External Relations and Business Development Directorate, addresses students of MESA, the New Mexico Mathematics, Engineering and Science Achievement Program. The students are visiting KSC, touring facilities and meeting with mentors. MESA students, high school seniors who hold grade-point averages of at least 3.2 and who tutor other students in math and science, have made the spring trip for the past 14 years. The MESA program has close ties to the NASA Training Project at the University of New Mexico.
KENNEDY SPACE CENTER, FLA. - JoAnn Morgan, director, External Relations and Business Development, speaks to the students of MESA, the New Mexico Mathematics, Engineering and Science Achievement Program. The students are visiting KSC, touring facilities and meeting with mentors. MESA students, high school seniors who hold grade-point averages of at least 3.2 and who tutor other students in math and science, have made the spring trip for the past 14 years. The MESA program has close ties to the NASA Training Project at the University of New Mexico.
KENNEDY SPACE CENTER, FLA. - JoAnn Morgan, director, External Relations and Business Development, speaks to the students of MESA, the New Mexico Mathematics, Engineering and Science Achievement Program. The students are visiting KSC, touring facilities and meeting with mentors. MESA students, high school seniors who hold grade-point averages of at least 3.2 and who tutor other students in math and science, have made the spring trip for the past 14 years. The MESA program has close ties to the NASA Training Project at the University of New Mexico.
KENNEDY SPACE CENTER, FLA. - JoAnn Morgan, director, External Relations and Business Development, speaks to the students of MESA, the New Mexico Mathematics, Engineering and Science Achievement Program. The students are visiting KSC, touring facilities and meeting with mentors. MESA students, high school seniors who hold grade-point averages of at least 3.2 and who tutor other students in math and science, have made the spring trip for the past 14 years. The MESA program has close ties to the NASA Training Project at the University of New Mexico.
NASA Glenn researchers Jacki Houts, James Nessel and Michael Zemba perform a final inspection of the W/V-Band Terrestrial Link Experiment (WTLE) before it was transported to Albuquerque, New Mexico for testing. The experiment hardware includes a transmitter, which has been placed on the crest of the Sandia Mountains and a receiver (shown) placed at a research facility of the University of New Mexico. The wireless link spans 23km and will be used to study the effects of the atmosphere on high data-rate wireless communication links at 72 and 84 GHz. The goal of the experiment is to study these frequency bands for satellite communications.
A Swarmathon University Competition 2019 team presents their poster to a panel of judges at the Kennedy Space Center Visitor Complex in Florida on June 11, 2019. Swarmathon students and their mentors were at Kennedy to participate in a student/mentor panel, hear from speakers, get a behind-the-scenes tour of Kennedy Space Center, dine with an astronaut and receive awards during an awards ceremony. During Swarmathon University Challenge IV, students developed algorithms for robotic swarms that are robust and adaptable like the foraging strategies of ant colonies. The fourth and final Swarmathon was a combined virtual and physical competition, hosted by UNM.
The Swarmathon team from the University of Houston Clearlake and San Jacinto College received the Mission to Mars award for their achievements in the NASA Swarmathon University Challenge for 2019. They are at the Kennedy Space Center Visitor Complex on June 12, 2019. Students and mentors from some of the Swarmathon teams were at Kennedy to participate in a student/mentor panel, hear from speakers, get a behind-the-scenes tour of Kennedy Space Center, dine with an astronaut and receive awards. During Swarmathon University Challenge IV, students developed algorithms for robotic swarms that are robust and adaptable like the foraging strategies of ant colonies. The fourth and final Swarmathon challenge was a combined virtual and physical competition.
This narrated animation shows NASA's Perseverance rover on Mars and how the rover's SuperCam laser instrument works. SuperCam is led by Los Alamos National Laboratory in New Mexico, where the instrument's Body Unit was developed. That part of the instrument includes several spectrometers, control electronics and software. The Mast Unit was developed and built by several laboratories of the CNRS (French research center) and French universities under the contracting authority of CNES (French space agency). Calibration targets on the rover deck are provided by Spain's University of Valladolid. Animation available at https://photojournal.jpl.nasa.gov/catalog/PIA24426
NASA is looking to biological techniques that are millions of years old to help it develop new materials and technologies for the 21st century. Sponsored by NASA, Jeffrey Brinker of the University of New Mexico is studying how multiple elements can assemble themselves into a composite material that is clear, tough, and impermeable. His research is based on the model of how an abalone builds the nacre, also called mother-of-pearl, inside its shell. The mollusk layers bricks of calcium carbonate (the main ingredient in classroom chalk) and mortar of biopolymer to form a new material (top and bottom left) that is twice as hard and 1,000 times as tough as either of the original building materials.
NASA is looking to biological techniques that are millions of years old to help it develop new materials and technologies for the 21st century. Sponsored by NASA, Jeffrey Brinker of the University of New Mexico is studying how multiple elements can assemble themselves into a composite material that is clear, tough, and impermeable. His research is based on the model of how an abalone builds the nacre, also called mother-of-pearl, inside its shell. Strong thin coatings, or lamellae, in Brinker's research are formed when objects are dip-coated. Evaporation drives the self-assembly of molecular aggregates (micelles) of surfactant, soluble silica, and organic monomers and their further self-organization into layered organic and inorganic assemblies.
2010/119 - 04/29 at 16 :48 UTC Oil slick in the Gulf of Mexico (Input Direct Broadcast data courtesy Direct Readout Lab, NASA/GSFC) Satellite: Terra NASA/GSFC/Jeff Schmaltz/MODIS Land Rapid Response Team To learn more about MODIS go to: <a href="http://rapidfire.sci.gsfc.nasa.gov/gallery/?latest" rel="nofollow">rapidfire.sci.gsfc.nasa.gov/gallery/?latest</a> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> is home to the nation's largest organization of combined scientists, engineers and technologists that build spacecraft, instruments and new technology to study the Earth, the sun, our solar system, and the universe.
ISS011-E-08410 (9 June 2005) --- Las Cruces, New Mexico is featured in this image photographed by an Expedition 11 crewmember on the International Space Station. The city of Las Cruces is located within the Rio Grande Rift, a large geological feature that extends from Colorado southward into Mexico. According to NASA geologists, rifting usually heralds the breakup of continental landmasses, such as the separation of South America and Africa to form the southern Atlantic Ocean during the Mesozoic Era. The Rift is marked by a series of depressions (known as graben) caused by the subsidence of crustal blocks between parallel faults as the continental crust is pulled apart by tectonic forces. These graben are frequently marked by uplifted rocks along bounding faults — the striking Organ Mountains to the east of Las Cruces are one such uplifted fault block. While separation of the continental crust is no longer occurring, the Rio Grande Rift is still considered active as evidenced by frequent low-intensity earthquakes and hot springs to the north of Las Cruces. The modern city of Las Cruces — the seat of Doña Ana County and home to New Mexico State University — is undergoing rapid urban expansion due to influx of new residents attracted to the climate and landscape. The current urban area (gray to white region at image center) contrasts sharply with agricultural lands (dark green and grey brown) located along the Rio Grande River and the surrounding desert valley floor to the northeast and southwest (brown, blue gray and tan areas).
CAPE CANAVERAL, Fla. – Inside the Prototype Laboratory at NASA's Kennedy Space Center in Florida, Evan Williams, left, an Education intern from the University of Central Florida, and Anthony Bharrat, NASA avionics lead, prepare the experiment container for NASA's Exposing Microorganisms in the Stratosphere, or E-MIST, experiment. The container was designed and built at Kennedy. The 80-pound structure features four doors that rotate to expose up to 10 microbial samples each for a predetermined period of time in the Earth's stratosphere. The E-MIST experiment will launch on the exterior of a giant scientific balloon gondola at about 8 a.m. MST on Aug. 24 from Ft. Sumner, New Mexico. It will soar 125,000 feet above the Earth during a 5-hour journey over the desert to understand how spore-forming bacteria, commonly found in spacecraft assembly facilities can survive. Photo credit: NASA/Kim Shiflett
NASA image acquired Sept 6, 2010 at 16 :45 UTC Tropical Storm Hermine (10L) in the Gulf of Mexico Satellite: Terra Credit: NASA/GSFC/Jeff Schmaltz/MODIS Land Rapid Response Team To learn more go to: <a href="http://www.nasa.gov/mission_pages/hurricanes/archives/2010/h2010_Hermine.html" rel="nofollow">www.nasa.gov/mission_pages/hurricanes/archives/2010/h2010...</a> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> is home to the nation's largest organization of combined scientists, engineers and technologists that build spacecraft, instruments and new technology to study the Earth, the sun, our solar system, and the universe. <b>Follow us on <a href="http://twitter.com/NASA_GoddardPix" rel="nofollow">Twitter</a></b> <b>Join us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b>
CAPE CANAVERAL, Fla. – Inside the Prototype Laboratory at NASA's Kennedy Space Center in Florida, Evan Williams, an Education intern from the University of Central Florida, prepares the experiment container for NASA's Exposing Microorganisms in the Stratosphere, or E-MIST, experiment. The container was designed and built at Kennedy. The 80-pound structure features four doors that rotate to expose up to 10 microbial samples each for a predetermined period of time in the Earth's stratosphere. The E-MIST experiment will launch on the exterior of a giant scientific balloon gondola at about 8 a.m. MST on Aug. 24 from Ft. Sumner, New Mexico. It will soar 125,000 feet above the Earth during a 5-hour journey over the desert to understand how spore-forming bacteria, commonly found in spacecraft assembly facilities can survive. Photo credit: NASA/Kim Shiflett
2010/119 - 04/29 at 16 :48 UTC Oil slick in the Gulf of Mexico To see a full view of this image go to: <a href="http://www.flickr.com/photos/gsfc/4563296541/">www.flickr.com/photos/gsfc/4563296541/</a> (Input Direct Broadcast data courtesy Direct Readout Lab, NASA/GSFC) Satellite: Terra NASA/GSFC/Jeff Schmaltz/MODIS Land Rapid Response Team To learn more about MODIS go to: <a href="http://rapidfire.sci.gsfc.nasa.gov/gallery/?latest" rel="nofollow">rapidfire.sci.gsfc.nasa.gov/gallery/?latest</a> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> is home to the nation's largest organization of combined scientists, engineers and technologists that build spacecraft, instruments and new technology to study the Earth, the sun, our solar system, and the universe.
CAPE CANAVERAL, Fla. – Inside the Prototype Laboratory at NASA's Kennedy Space Center in Florida, Prital Thakrar, left, design lead and student engineer trainee from the University of Florida in Gainesville, Anthony Bharrat, NASA avionics lead, and Evan Williams, an Education intern from the University of Central Florida, prepare the experiment container for NASA's Exposing Microorganisms in the Stratosphere, or E-MIST, experiment. The container was designed and built at Kennedy. The 80-pound structure features four doors that rotate to expose up to 10 microbial samples each for a predetermined period of time in the Earth's stratosphere. The E-MIST experiment will launch on the exterior of a giant scientific balloon gondola at about 8 a.m. MST on Aug. 24 from Ft. Sumner, New Mexico. It will soar 125,000 feet above the Earth during a 5-hour journey over the desert to understand how spore-forming bacteria, commonly found in spacecraft assembly facilities can survive. Photo credit: NASA/Kim Shiflett
CAPE CANAVERAL, Fla. – Inside the Prototype Laboratory at NASA's Kennedy Space Center in Florida, Prital Thakrar, left, design lead and student engineer trainee from the University of Florida in Gainesville, Anthony Bharrat, NASA avionics lead, and Evan Williams, an Education intern from the University of Central Florida, prepare the experiment container for NASA's Exposing Microorganisms in the Stratosphere, or E-MIST, experiment. The container was designed and built at Kennedy. The 80-pound structure features four doors that rotate to expose up to 10 microbial samples each for a predetermined period of time in the Earth's stratosphere. The E-MIST experiment will launch on the exterior of a giant scientific balloon gondola at about 8 a.m. MST on Aug. 24 from Ft. Sumner, New Mexico. It will soar 125,000 feet above the Earth during a 5-hour journey over the desert to understand how spore-forming bacteria, commonly found in spacecraft assembly facilities can survive. Photo credit: NASA/Kim Shiflett
Caption: In this composite image, visible-light observations by NASA’s Hubble Space Telescope are combined with infrared data from the ground-based Large Binocular Telescope in Arizona to assemble a dramatic view of the well-known Ring Nebula. Credit: NASA, ESA, C.R. Robert O’Dell (Vanderbilt University), G.J. Ferland (University of Kentucky), W.J. Henney and M. Peimbert (National Autonomous University of Mexico) Credit for Large Binocular Telescope data: David Thompson (University of Arizona) ---- The Ring Nebula's distinctive shape makes it a popular illustration for astronomy books. But new observations by NASA's Hubble Space Telescope of the glowing gas shroud around an old, dying, sun-like star reveal a new twist. "The nebula is not like a bagel, but rather, it's like a jelly doughnut, because it's filled with material in the middle," said C. Robert O'Dell of Vanderbilt University in Nashville, Tenn. He leads a research team that used Hubble and several ground-based telescopes to obtain the best view yet of the iconic nebula. The images show a more complex structure than astronomers once thought and have allowed them to construct the most precise 3-D model of the nebula. "With Hubble's detail, we see a completely different shape than what's been thought about historically for this classic nebula," O'Dell said. "The new Hubble observations show the nebula in much clearer detail, and we see things are not as simple as we previously thought." The Ring Nebula is about 2,000 light-years from Earth and measures roughly 1 light-year across. Located in the constellation Lyra, the nebula is a popular target for amateur astronomers. Read more: <a href="http://1.usa.gov/14VAOMk" rel="nofollow">1.usa.gov/14VAOMk</a> <b><a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a></b> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. <b>Follow us on <a href="http://twitter.com/NASA_GoddardPix" rel="nofollow">Twitter</a></b> <b>Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b> <b>Find us on <a href="http://instagram.com/nasagoddard?vm=grid" rel="nofollow">Instagram</a></b>
This photograph shows the Compton Gamma-Ray Observatory (GRO) being deployed by the Remote Manipulator System (RMS) arm aboard the Space Shuttle Atlantis during the STS-37 mission in April 1991. The GRO reentered Earth atmosphere and ended its successful mission in June 2000. For nearly 9 years, the GRO Burst and Transient Source Experiment (BATSE), designed and built by the Marshall Space Flight Center (MSFC), kept an unblinking watch on the universe to alert scientists to the invisible, mysterious gamma-ray bursts that had puzzled them for decades. By studying gamma-rays from objects like black holes, pulsars, quasars, neutron stars, and other exotic objects, scientists could discover clues to the birth, evolution, and death of stars, galaxies, and the universe. The gamma-ray instrument was one of four major science instruments aboard the Compton. It consisted of eight detectors, or modules, located at each corner of the rectangular satellite to simultaneously scan the entire universe for bursts of gamma-rays ranging in duration from fractions of a second to minutes. In January 1999, the instrument, via the Internet, cued a computer-controlled telescope at Las Alamos National Laboratory in Los Alamos, New Mexico, within 20 seconds of registering a burst. With this capability, the gamma-ray experiment came to serve as a gamma-ray burst alert for the Hubble Space Telescope, the Chandra X-Ray Observatory, and major gound-based observatories around the world. Thirty-seven universities, observatories, and NASA centers in 19 states, and 11 more institutions in Europe and Russia, participated in the BATSE science program.
This photograph shows the Compton Gamma-Ray Observatory being released from the Remote Manipulator System (RMS) arm aboard the Space Shuttle Atlantis during the STS-35 mission in April 1991. The GRO reentered the Earth's atmosphere and ended its successful mission in June 2000. For nearly 9 years, GRO's Burst and Transient Source Experiment (BATSE), designed and built by the Marshall Space Flight Center, kept an unblinking watch on the universe to alert scientist to the invisible, mysterious gamma-ray bursts that had puzzled them for decades. By studying gamma-rays from objects like black holes, pulsars, quasars, neutron stars, and other exotic objects, scientists could discover clues to the birth, evolution, and death of star, galaxies, and the universe. The gamma-ray instrument was one of four major science instruments aboard the Compton. It consisted of eight detectors, or modules, located at each corner of the rectangular satellite to simultaneously scan the entire universe for bursts of gamma-rays ranging in duration from fractions of a second to minutes. In January 1999, the instrument, via the Internet, cued a computer-controlled telescope at Las Alamos National Laboratory in Los Alamos, New Mexico, within 20 seconds of registering a burst. With this capability, the gamma-ray experiment came to serve as a gamma-ray burst alert for the Hubble Space Telescope, the Chandra X-Ray Observatory, and major gound-based observatories around the world. Thirty-seven universities, observatories, and NASA centers in 19 states, and 11 more institutions in Europe and Russia, participated in BATSE's science program.
CAPE CANAVERAL, Fla. – Inside the Prototype Laboratory at NASA's Kennedy Space Center in Florida, Evan Williams, left, an Education intern from the University of Central Florida, and Anthony Bharrat, NASA avionics lead, prepare the experiment container for NASA's Exposing Microorganisms in the Stratosphere, or E-MIST, experiment. In the background is David J. Smith, Ph.D., NASA E-MIST principal investigator. The container was designed and built at Kennedy. The 80-pound structure features four doors that rotate to expose up to 10 microbial samples each for a predetermined period of time in the Earth's stratosphere. The E-MIST experiment will launch on the exterior of a giant scientific balloon gondola at about 8 a.m. MST on Aug. 24 from Ft. Sumner, New Mexico. It will soar 125,000 feet above the Earth during a 5-hour journey over the desert to understand how spore-forming bacteria, commonly found in spacecraft assembly facilities can survive. Photo credit: NASA/Kim Shiflett
Release date: July 1, 2008 This image is a composite of visible (or optical), radio, and X-ray data of the full shell of the supernova remnant from SN 1006. The radio data show much of the extent that the X-ray image shows. In contrast, only a small linear filament in the northwest corner of the shell is visible in the optical data. The object has an angular size of roughly 30 arcminutes (0.5 degree, or about the size of the full moon), and a physical size of 60 light-years (18 parsecs) based on its distance of nearly 7,000 light-years. The small green box along the bright filament at the top of the image corresponds to the dimensions of the Hubble release image. The optical data was obtained at the University of Michigan's 0.9-meter Curtis Schmidt telescope at the National Science Foundation's Cerro Tololo Inter-American Observatory (CTIO) near La Serena, Chile. H-alpha, continuum-subtracted data were provided by F. Winkler (Middlebury COllege) et al. The X-ray data were acquired from the Chandra X-ray Observatory's AXAF CCD Imaging Spectrometer (ACIS) at 0.5-3keV, and were provided by J. Hughes (Rutgers University) et al. The radio data, supplied by K. Dyer (NRAO, Socorro) et al., were a composite from the National Radio Astronomy Observatory's Very Large Array (NRAO/VLA) in Socorro, New Mexico, along with the Green Bank Telescope (GBT) in Green Bank, West Virginia. Data of the supernova remnant were blended on a visible-light stellar background created using the Digitized Sky Survey's Anglo-Australian Observatory (AAO2) blue and red plates. Photo Credit: NASA, ESA, and Z. Levay (STScI) Science Credit: Radio: NRAO/AUI/NSF GBT+VLA 1.4 GHz mosaic (Dyer, Maddalena and Cornwell, NRAO); X-ray: NASA/CXC/Rutgers/G. Cassam-Chenai and J. Hughes et al.; Optical: F.Winkler/Middlebury College and NOAO/AURA/NSF; and DSS To learn more about the Hubble Space Telescope go here: <a href="http://www.nasa.gov/mission_pages/hubble/main/index.html" rel="nofollow">www.nasa.gov/mission_pages/hubble/main/index.html</a> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> is home to the nation's largest organization of combined scientists, engineers and technologists that build spacecraft, instruments and new technology to study the Earth, the sun, our solar system, and the universe. <b>Follow us on <a href="http://twitter.com/NASAGoddardPix" rel="nofollow">Twitter</a></b> <b>Join us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a><b> </b></b>
This composite image of the "Delta Scarp" in Mars' Jezero Crater was generated using data from two imagers aboard NASA's Perseverance rover. Taken by the rover's Mastcam-Z, the bottom image shows both the base and plateau of the escarpment. The inset above, created from a mosaic of five Remote Microscopic Imager (RMI) pictures, zooms in on a 377-foot-wide (115-meter-wide) portion of the scarp, allowing closer inspection of some of its intriguing geologic features. Part of the rover's SuperCam instrument, the RMI is able to spot an object the size of a softball from nearly a mile away, allowing scientists to take images of details from a long distance. It also provides fine details of nearby targets zapped by SuperCam's laser. SuperCam is led by Los Alamos National Laboratory in New Mexico, where the instrument's Body Unit was developed. That part of the instrument includes several spectrometers, control electronics and software. The Mast Unit was developed and built by several laboratories of the CNRS (French National Centre for Scientific Research) and French universities under the contracting authority of CNES. Arizona State University in Tempe leads the operations of the Mastcam-Z instrument, working in collaboration with Malin Space Science Systems in San Diego. A key objective for Perseverance's mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet's geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith (broken rock and dust). Subsequent NASA missions, in cooperation with ESA (European Space Agency), would send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis. The Mars 2020 Perseverance mission is part of NASA's Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet. https://photojournal.jpl.nasa.gov/catalog/PIA24684
Proteus and an F/A-18 Hornet from NASA's Dryden Flight Research Center are seen here in flight over Las Cruces, New Mexico.
Scaled Composites' Doug Shane examines the screen of his ground control station during tests in New Mexico. Shane used this configuration as the ground control station to remotely pilot the Proteus aircraft during a NASA sponsored series of tests.
Proteus aircraft low-level flyby at Las Cruces Airport.
Proteus aircraft over Las Cruces International Airport in New Mexico.
Proteus in flight over mountains near Las Cruces, New Mexico.
The Proteus aircraft and NASA Dryden's T-34 in flight over Las Cruces, New Mexico.
Scaled Composites' Proteus aircraft and an F/A-18 Hornet from NASA's Dryden Flight Research Center during a low-level flyby at Las Cruces Airport in New Mexico.
The Proteus high-altitude aircraft at Sunset
NASA's Perseverance Mars rover captured this doughnut-shaped rock in Jezero Crater from about 328 feet (100 meters) away using its Remote Microscopic Imager (RMI), part of the SuperCam instrument, on June 22, 2023, the 832nd Martian day, or sol, of the mission. Oddly shaped rocks aren't uncommon, either on Earth or Mars; they're often formed over eons as winds sandblast rock faces. This particular rock may have formed after a smaller rock (or multiple rocks) eroded near its center. That left behind a cavity that was later enlarged by the wind. Figure A shows the same rock in its broader context, when it was first spotted by the rover's Mastcam-Z instrument from about 1,312 feet (400 meters away) on April 15, 2023, the 765th Martian day, or sol, of the mission. SuperCam is led by Los Alamos National Laboratory in New Mexico, where the instrument's body unit was developed. That part of the instrument includes several spectrometers as well as control electronics and software. The mast unit, including RMI, was developed and built by several laboratories of the CNRS (the French research center) and French universities under the contracting authority of Centre National d'Études Spatiales (CNES), the French space agency. Arizona State University leads the operations of the Mastcam-Z instrument, working in collaboration with Malin Space Science Systems in San Diego, on the design, fabrication, testing, and operation of the cameras, and in collaboration with the Niels Bohr Institute of the University of Copenhagen on the design, fabrication, and testing of the calibration targets. A key objective for Perseverance's mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet's geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith (broken rock and dust). Subsequent NASA missions, in cooperation with ESA (European Space Agency), would send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis. The Mars 2020 Perseverance mission is part of NASA's Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet. https://photojournal.jpl.nasa.gov/catalog/PIA25916
This enhanced-color close-up of a rock target called "Cine" was captured by the SuperCam instrument aboard NASA's Perseverance Mars rover on Sept. 17, 2021, the 206th Martian day, or sol, of rover's mission. SuperCam’s Remote Microscopic Imager took two images that were later combined to form this close-up. The target is 92 inches (2 meters) away, seen from the rover's mast. The image shows a rock layer made up of tightly packed millimeter-size gray, angular grains, or crystals. The image on the right shows a detail of the grain/crystal texture. The composition of this rock target was investigated with SuperCam's laser and spectrometer, along with the Mastcam-Z camera. Using these instruments, scientists can study the chemical composition of rocks from a distance. Analysis of "Cine" showed that it is rich in the mineral olivine. After the image was taken, the mission’s science team debated whether the rock is igneous (volcanic) or consists of fine sedimentary grains of igneous material that were cemented together in a watery environment. SuperCam is led by Los Alamos National Laboratory in New Mexico, where the instrument's body unit was developed. That part of the instrument includes several spectrometers as well as control electronics and software. The mast unit, including the Remote Microscopic Imager used for these images, was developed and built by several laboratories of the CNRS (the French research center) and French universities under the contracting authority of Centre National d'Etudes Spatiales (CNES), the French space agency. A key objective for Perseverance's mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet's geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith (broken rock and dust). Subsequent NASA missions, in cooperation with ESA (European Space Agency), would send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis. The Mars 2020 Perseverance mission is part of NASA's Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet. https://photojournal.jpl.nasa.gov/catalog/PIA24936
Composed of five images, this mosaic of the Jezero Crater's "Delta Scarp" was taken on March 17, 2021, by the Remote Microscopic Imager (RMI) camera aboard NASA's Perseverance rover from 1.4 miles (2.25 kilometers) away. Scientists believe the 377-foot-wide (115-meter-wide) escarpment is a portion of the remnants of a fan-shaped deposit of sediments that resulted from the confluence between an ancient river and an ancient lake. An annotated version of the same image (Figure 1) reveals location of a conglomerate (rock composed of coarse-grained pebbles mixed with sand) and examples of crossbedding (tilted layers of sedimentary rock that can result from water passing over a loose bed of sediment). Part of the SuperCam instrument, the RMI is able to spot an object the size of a softball from nearly a mile away, allowing scientists to take images of details from a long distance. It also provides fine details of nearby targets zapped by SuperCam's laser. SuperCam is led by Los Alamos National Laboratory in New Mexico, where the instrument's Body Unit was developed. That part of the instrument includes several spectrometers as well as control electronics and software. The Mast Unit was developed and built by several laboratories of the CNRS (the French research center) and French universities under the contracting authority of CNES (the French space agency). A key objective for Perseverance's mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet's geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith (broken rock and dust). Subsequent NASA missions, in cooperation with ESA (European Space Agency), would send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis. The Mars 2020 Perseverance mission is part of NASA's Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet. https://photojournal.jpl.nasa.gov/catalog/PIA24683
NASA's Perseverance rover took these zoomed-in images of a layered outcrop (just below center of image) nicknamed "Artuby" on June 17, 2021 (the 116th sol, or Martian Day, of its mission), from a little more than a third of a mile (615 meters) away. This mosaic is made up of three images taken by the Remote Microscopic Imager (RMI), part of the rover's SuperCam instrument. Each circular image has a field of view of 37.73 feet (11.50 meters) at this distance. The images were combined using an algorithm that weights the image centers. The outcrop shows evidence of being formed in an ancient lake. The feature is in the 'Verdon' quadrangle of Mars' Jezero Crater, south of the landing site. Artuby is the name of a river in southern France. Perseverance has been exploring the floor of Jezero Crater since it landed on Feb. 18, 2021. SuperCam is led by Los Alamos National Laboratory in New Mexico, where the instrument's Body Unit was developed. That part of the instrument includes several spectrometers as well as control electronics and software. The Mast Unit, including the RMI used for these images, was developed and built by several laboratories of the CNRS (the French research center) and French universities under the contracting authority of Centre National d'Etudes Spatiales (CNES, the French space agency). A key objective for Perseverance's mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet's geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith (broken rock and dust). Subsequent NASA missions, in cooperation with ESA (European Space Agency), would send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis. The Mars 2020 Perseverance mission is part of NASA's Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet. https://photojournal.jpl.nasa.gov/catalog/PIA24747
These images from the Chemistry and Camera (ChemCam) instrument on NASA's Curiosity Mars rover indicate similarly dark material, but with very different chemistries, in mineral veins at "Garden City." Each of the side-by-side circular images covers an area about 2 inches (5 centimeters) in diameter. The images were taken by ChemCam's Remote Micro-Imager. Researchers used ChemCam's laser, telescope and spectrometers to examine the chemistry of material in these veins. While both of these veins are dark, their chemistries are very different, indicating that they were formed by different fluids. One common aspect of the chemistry in the dark material is an iron content higher than nearby bedrock. Thus the dark appearance may be result of similar iron content. The dark maerial in the vein on the left is enriched in calcium and contains calcium fluorine. The dark material in the vein on the right is enriched in magnesium, but not in calcium or calcium fluorine. Thus, the veins were formed by different fluids that deposited minerals in rock fractures. The Remote Micro-Imager took the image on the left on March 27, 2015, during the 938th Martian day, or sol, of Curiosity's work on Mars. The next day, it took the image on the right. A broader view of the prominent mineral veins at Garden City is at PIA19161. ChemCam is one of 10 instruments in Curiosity's science payload. The U.S. Department of Energy's Los Alamos National Laboratory, in Los Alamos, New Mexico, developed ChemCam in partnership with scientists and engineers funded by the French national space agency (CNES), the University of Toulouse and the French national research agency (CNRS). More information about ChemCam is available at http://www.msl-chemcam.com. http://photojournal.jpl.nasa.gov/catalog/PIA19924
This 2015 diagram shows components of the investigations payload for NASA's Mars 2020 rover mission. Mars 2020 will re-use the basic engineering of NASA's Mars Science Laboratory to send a different rover to Mars, with new objectives and instruments, launching in 2020. The rover will carry seven instruments to conduct its science and exploration technology investigations. They are: Mastcam-Z, an advanced camera system with panoramic and stereoscopic imaging capability and the ability to zoom. The instrument also will determine mineralogy of the Martian surface and assist with rover operations. The principal investigator is James Bell, Arizona State University in Tempe. SuperCam, an instrument that can provide imaging, chemical composition analysis, and mineralogy. The instrument will also be able to detect the presence of organic compounds in rocks and regolith from a distance. The principal investigator is Roger Wiens, Los Alamos National Laboratory, Los Alamos, New Mexico. This instrument also has a significant contribution from the Centre National d'Etudes Spatiales, Institut de Recherche en Astrophysique et Planétologie (CNES/IRAP) France. Planetary Instrument for X-ray Lithochemistry (PIXL), an X-ray fluorescence spectrometer that will also contain an imager with high resolution to determine the fine-scale elemental composition of Martian surface materials. PIXL will provide capabilities that permit more detailed detection and analysis of chemical elements than ever before. The principal investigator is Abigail Allwood, NASA's Jet Propulsion Laboratory, Pasadena, California. Scanning Habitable Environments with Raman & Luminescence for Organics and Chemicals (SHERLOC), a spectrometer that will provide fine-scale imaging and uses an ultraviolet (UV) laser to determine fine-scale mineralogy and detect organic compounds. SHERLOC will be the first UV Raman spectrometer to fly to the surface of Mars and will provide complementary measurements with other instruments in the payload. SHERLOC includes a high-resolution color camera for microscopic imaging of Mars' surface. The principal investigator is Luther Beegle, JPL. The Mars Oxygen ISRU Experiment (MOXIE), an exploration technology investigation that will produce oxygen from Martian atmospheric carbon dioxide. The principal investigator is Michael Hecht, Massachusetts Institute of Technology, Cambridge, Massachusetts. Mars Environmental Dynamics Analyzer (MEDA), a set of sensors that will provide measurements of temperature, wind speed and direction, pressure, relative humidity and dust size and shape. The principal investigator is Jose Rodriguez-Manfredi, Centro de Astrobiologia, Instituto Nacional de Tecnica Aeroespacial, Spain. The Radar Imager for Mars' Subsurface Experiment (RIMFAX), a ground-penetrating radar that will provide centimeter-scale resolution of the geologic structure of the subsurface. The principal investigator is Svein-Erik Hamran, the Norwegian Defence Research Establishment, Norway. http://photojournal.jpl.nasa.gov/catalog/PIA19672
How Warm is Mars?
The Remote Microscopic Imager (RMI) camera aboard NASA's Perseverance Mars rover took these zoomed-in images of the Ingenuity Mars Helicopter and one of its rotor blades on Feb. 24, 2024, the 1,072nd Martian day, or sol, of the mission. The mosaic shows the helicopter at right, standing at an angle near the apex of a sand ripple. About 49 feet (15 meters) to the west of the helicopter's location (just left of center in the image), a large portion of one of the helicopter's rotor blades lies on the surface. The Ingenuity team is considering a theory that the blade detached after the rotorcraft impacted the Martian surface at the conclusion of the helicopter's 72nd and final flight on Jan. 18, 2024. This mosaic is made up of seven images taken by the RMI, which is part of the rover's SuperCam instrument. At the time these images were taken, the distance between the rover and helicopter was about 1,365 feet (415 meters). Each circular image has a field of view of 26 feet (7.8 meters) at this distance. Able to spot a softball from nearly a mile away, the RMI allows scientists to take images of details from a long distance. It also provides fine details of nearby targets zapped by SuperCam's laser. SuperCam is led by Los Alamos National Laboratory in New Mexico, where the instrument's body unit was developed. The mast unit, including the RMI used for these images, was developed and built by several laboratories of the CNRS (the French research center) and French universities under the contracting authority of Centre National d'Études Spatiales (CNES), the French space agency. A key objective for Perseverance's mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet's geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith (broken rock and dust). Subsequent NASA missions, in cooperation with ESA (European Space Agency), would send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis. The Mars 2020 Perseverance mission is part of NASA's Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet. https://photojournal.jpl.nasa.gov/catalog/PIA26238
On May 18, 2022, NASA's Perseverance Mars rover used an artificial intelligence software called Autonomous Exploration for Gathering Increased Science (AEGIS) to select and target the rock seen in close-up here. It's one of two rocks that the AI for the first time helped Perseverance study without direction from the mission's team back on Earth. AEGIS was developed by NASA's Jet Propulsion Laboratory in Southern California – which also built Perseverance – to collect data on rocks and other Martian features that the rover discovers while driving. AEGIS is used in conjunction with Perseverance's SuperCam laser instrument, directing the laser to zap certain features that scientists have commanded the rover to look for. SuperCam used its Remote Micro-Imager (RMI) camera to take two images of this target, which were stitched together into the main picture seen here. The rock target, which was about 16 feet (5 meters) away from the rover, is named "AEGIS_0442B," referring to the Martian day, or sol, it was targeted (Sol 442) and that it was the second rock ("B") targeted by AEGIS on that sol. The red crosshairs seen across the rock target indicate each place AEGIS directed the laser to zap. SuperCam is led by Los Alamos National Laboratory in New Mexico, where the instrument's body unit was developed. That part of the instrument includes several spectrometers as well as control electronics and software. The mast unit, including RMI, was developed and built by several laboratories of the CNRS (the French research center) and French universities under the contracting authority of Centre National d'Études Spatiales (CNES), the French space agency. A key objective for Perseverance's mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet's geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith (broken rock and dust). Subsequent NASA missions, in cooperation with ESA (European Space Agency), would send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis. The Mars 2020 Perseverance mission is part of NASA's Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet. https://photojournal.jpl.nasa.gov/catalog/PIA25289
NASA's Perseverance Mars rover used its abrasion tool to grind down the rock surface at this target, nicknamed "Bellegarde," on Aug. 29, 2021, the 188th Martian day, or sol, of the mission. The abraded patch is 0.4 inches (5 centimeters) in diameter. The mission has nicknamed the rock itself "Rochette" and acquired its first two core samples from it. The rover abrades rocks using a tool on its robotic arm before drilling them in order to clear away dust and weathering rinds, allowing other instruments to study the rocks and determine if scientists want to grab a sample of them. This close-up image was produced by Perseverance's SuperCam instrument in natural color, as it would appear under daytime lighting conditions. Besides imagery, SuperCam has a rock-vaporizing laser and spectrometer. By studying a rock's vapor after each laser zap, scientists can study the chemical composition of rocks from a distance. Perseverance landed in Mars' Jezero Crater on Feb. 18, 2021, and has been exploring the floor of the crater since. At the time these images were taken, Perseverance was in an area nicknamed the "Crater Floor Fractured Rough" area. SuperCam is led by Los Alamos National Laboratory in New Mexico, where the instrument's Body Unit was developed. That part of the instrument includes several spectrometers as well as control electronics and software. The Mast Unit, including the Remote Microscopic Imager used for these images, was developed and built by several laboratories of the CNRS (the French research center) and French universities under the contracting authority of Centre National d'Etudes Spatiales (CNES, the French space agency). A key objective for Perseverance's mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet's geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith (broken rock and dust). Subsequent NASA missions, in cooperation with ESA (European Space Agency), would send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis. The Mars 2020 Perseverance mission is part of NASA's Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet. https://photojournal.jpl.nasa.gov/catalog/PIA24768
This composite image, made from four taken by the SuperCam instrument aboard NASA's Perseverance rover on August 8, 2021, shows the hole in a Martian rock where the rover attempted to collect its first sample; the small pits within it were created by laser zaps from SuperCam during subsequent efforts to analyze the rock's composition. The rover science team has nicknamed the drill hole "Roubion." The team believes that because of this rock's unusual composition, the process of extracting a core created a significant pile of tailings (or cuttings) around the coring hole. Eight pits produced by 30 laser shots each are seen in two columns inside the drill hole. The SuperCam team's analysis suggests that the top six pits penetrated the compacted mound of tailings around the hole, while the bottom two pits in the hole interrogated material below the rock surface. Two additional laser pits can be seen in the tailings at the near side of the hole. Two vertical ridges inside the hole – one on each side of the laser pits – were produced as the drill was removed, prior to laser analysis. Some bright mineral grains can be seen as glints in the tailings and in the drill hole. A few clumps or larger pieces of material are seen at the top of the tailings pile just to the left of the hole. The SuperCam images were taken from a distance of 7.32 feet (2.23 meters). A scale bar is included in this image. Perseverance landed in Mars' Jezero Crater on February 18, 2021, and has been exploring the floor of the crater since. At the time these images were taken, Perseverance was in an area nicknamed the "Crater Floor Fractured Rough" area. SuperCam is led by Los Alamos National Laboratory in New Mexico, where the instrument's Body Unit was developed. That part of the instrument includes several spectrometers as well as control electronics and software. The Mast Unit, including the Remote Microscopic Imager used for these images, was developed and built by several laboratories of the CNRS (the French research center) and French universities under the contracting authority of Centre National d'Etudes Spatiales (CNES, the French space agency). A key objective for Perseverance's mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet's geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith (broken rock and dust). Subsequent NASA missions, in cooperation with ESA (European Space Agency), would send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis. The Mars 2020 Perseverance mission is part of NASA's Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet. Movie available at https://photojournal.jpl.nasa.gov/catalog/PIA24749
NASA image acquired June 26, 2010 As of June 27, 2010, the entire gulf-facing beachfront of several barrier islands in eastern Mississippi (offshore of Pascagoula) had received a designation of at least “lightly oiled” by the interagency Shoreline Cleanup Assessment Team that is responding to the disaster in the Gulf of Mexico. A few small stretches of Petit Bois Island had been labeled heavily or moderately oiled. (To view this image without a description go to: This high-resolution image shows Petit Bois Island (top right) and the eastern end of Horn Island (top left) on June 26. In general, oil-covered waters are silvery and cleaner waters are blue-gray. This pattern is especially consistent farther from the islands. The intensely bright patches of water directly offshore of the barrier islands, however, may be from a combination of factors, including sediment and organic material, coastal currents and surf, and oil. The islands provide a sense of scale for the ribbons of oil swirling into the area from the south. Petit Bois Island is about 10 kilometers (6 miles) long. It is one of seven barrier islands that, along with some mainland areas of Mississippi and Florida, make up the Gulf Islands National Seashore. According to the National Park Service Gulf Islands National Seashore Website, all the islands remained open to the public as of June 28, 2010, and clean-up crews were on hand to respond to any oil coming ashore. The large version of this image, which was captured by the Advanced Land Imager on NASA’s Earth Observing-1 (EO-1) satellite, shows a larger area, including the Mississippi Sound and parts of mainland Mississippi. Although oil has been observed in the Sound, it is unlikely that all the bright patches of water in that area are thickly oil-covered. Differences in brightness in coastal area waters may be due to other factors, including freshwater runoff, strong currents, and water depth and clarity. NASA Earth Observatory image created by Jesse Allen and Robert Simmon, using EO-1 ALI data provided courtesy of the NASA EO-1 team. Caption by Rebecca Lindsey. Instrument: EO-1 - ALI To see more images go to: <a href="http://earthobservatory.nasa.gov/" rel="nofollow">earthobservatory.nasa.gov/</a> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> is home to the nation's largest organization of combined scientists, engineers and technologists that build spacecraft, instruments and new technology to study the Earth, the sun, our solar system, and the universe.
This map shows the distribution of water in the stratosphere of Jupiter as measured with the Herschel space observatory. White and cyan indicate highest concentration of water, and blue indicates lesser amounts.