Attendees enjoy space related activities prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

NASA Johnson Space Center Director Vanessa Wyche gives remarks prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

NASA Johnson Space Center Director Vanessa Wyche gives remarks prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

NASA TV producer of “The Color of Space” Jori Kates gives remarks prior to the screening of the documentary at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

Former NASA astronaut Susan Kilrain poses for a photograph with attendees prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

NASA TV producer of “The Color of Space” Jori Kates gives remarks prior to the screening of the documentary at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

Former NASA astronaut Leland Melvin gives remarks prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

NASA TV producer of “The Color of Space” Jori Kates gives remarks prior to the screening of the documentary at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

Popcorn awaits guests prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

Former NASA astronaut Leland Melvin shows some photographs from his previous flight experience prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

Former NASA astronaut Leland Melvin poses with attendees prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

NASA TV producer of “The Color of Space” Jori Kates gives remarks prior to the screening of the documentary at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

Former NASA astronaut Leland Melvin gives remarks prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

Former NASA astronaut Leland Melvin gives remarks prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

Children in attendance for the screening the NASA produced documentary “The Color of Space” draw on postcards that will be sent to space by Club for the Future on a Blue Origin New Shepard rocket at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

6-year old Armani Bonds draws on a postcard that will be sent to space by Club for the Future on a Blue Origin New Shepard rocket prior to he and his family screening the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

Attendees try on Oculus headsets and experience the International Space Station using virtual reality prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

NASA Johnson Space Center Director Vanessa Wyche speaks of NASA astronaut Jessica Watkins during her remarks prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

Attendees for the screening the NASA produced documentary “The Color of Space” get their photos taken with former NASA astronaut Alvin Drew, left, former astronaut Susan Kilrain, and NASA Johnson Space Center Director Vanessa Wyche, right, at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

9-year old Amara Bowman smiles as her father photographs her inside a Blue Origin New Shepard capsule mockup prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

NASA astronaut Stephanie Wilson, left, and former NASA astronauts Leland Melvin and Susan Kilrain pose for a photograph prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

Attendees line up to go inside a Blue Origin New Shepard capsule mockup prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

Former NASA astronaut Leland Melvin, left, and NASA astronaut Stephanie Wilson, pose for photograph with 6-year old Armani Bonds prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

6-year old Armani Bonds poses for a photograph as he exits a Blue Origin New Shepard capsule mockup prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

Attendees experience the inside of a Blue Origin New Shepard capsule mockup prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

NASA astronaut Stephanie Wilson talks with 7-year old Tre Rahaman, left, and 4-year old Amira Rahaman, along with their mother Nadia Rahaman of Silver Sping, Maryland prior to the screening of the NASA produced documentary “The Color of Space” at Howard University’s Cramton Auditorium in Washington, Saturday, June 18, 2022. Premiering on Juneteenth, the federal holiday commemorating the end of slavery in the United States, “The Color of Space” is an inspirational documentary that tells the stories of NASA’s Black astronauts determined to reach the stars. Photo Credit: (NASA/Bill Ingalls)

Astronomers using NASA's Hubble Space Telescope have assembled a comprehensive picture of the evolving universe – among the most colorful deep space images ever captured by the 24-year-old telescope. Researchers say the image, in new study called the Ultraviolet Coverage of the Hubble Ultra Deep Field, provides the missing link in star formation. The Hubble Ultra Deep Field 2014 image is a composite of separate exposures taken in 2003 to 2012 with Hubble's Advanced Camera for Surveys and Wide Field Camera 3. Credit: NASA/ESA Read more: <a href="http://1.usa.gov/1neD0se" rel="nofollow">1.usa.gov/1neD0se</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/NASAGoddardPix" 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>

Attendees watch “The Color of Space” during a screening of the documentary as part of the Department of Education’s HBCU Week Conference, Monday, Sept. 25, 2023, at the Hyatt Regency in Arlington, Va. Photo Credit: (NASA/Joel Kowsky)

Attendees watch “The Color of Space” during a screening of the documentary as part of the Department of Education’s HBCU Week Conference, Monday, Sept. 25, 2023, at the Hyatt Regency in Arlington, Va. Photo Credit: (NASA/Joel Kowsky)

This colorful view of Mercury was produced by using images from the color base map imaging campaign during MESSENGER's primary mission. These colors are not what Mercury would look like to the human eye, but rather the colors enhance the chemical, mineralogical, and physical differences between the rocks that make up Mercury's surface. This specific color combination places the second principle component in the red channel, the first principle component in the green channel, and the ratio of the 430 nm/1000 nm filters in the blue channel. The MESSENGER spacecraft is the first ever to orbit the planet Mercury, and the spacecraft's seven scientific instruments and radio science investigation are unraveling the history and evolution of the Solar System's innermost planet. During the first two years of orbital operations, MESSENGER acquired over 150,000 images and extensive other data sets. MESSENGER is capable of continuing orbital operations until early 2015. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington <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>

NASA’s Lisa Frazier introduces NASA TV producer of “The Color of Space” Jori Kates and NASA astronaut Alvin Drew before a screening of “The Color of Space” as part of the Department of Education’s HBCU Week Conference, Monday, Sept. 25, 2023, at the Hyatt Regency in Arlington, Va. Photo Credit: (NASA/Joel Kowsky)

NASA TV producer of “The Color of Space” Jori Kates, left, and NASA astronaut Alvin Drew answer questions before a screening of “The Color of Space” as part of the Department of Education’s HBCU Week Conference, Monday, Sept. 25, 2023, at the Hyatt Regency in Arlington, Va. Photo Credit: (NASA/Joel Kowsky)

NASA TV producer of “The Color of Space” Jori Kates, left, and NASA astronaut Alvin Drew answer questions before a screening of “The Color of Space” as part of the Department of Education’s HBCU Week Conference, Monday, Sept. 25, 2023, at the Hyatt Regency in Arlington, Va. Photo Credit: (NASA/Joel Kowsky)

NASA TV producer of “The Color of Space” Jori Kates, left, and NASA astronaut Alvin Drew answer questions before a screening of “The Color of Space” as part of the Department of Education’s HBCU Week Conference, Monday, Sept. 25, 2023, at the Hyatt Regency in Arlington, Va. Photo Credit: (NASA/Joel Kowsky)

NASA TV producer of “The Color of Space” Jori Kates, left, and NASA astronaut Alvin Drew answer questions before a screening of “The Color of Space” as part of the Department of Education’s HBCU Week Conference, Monday, Sept. 25, 2023, at the Hyatt Regency in Arlington, Va. Photo Credit: (NASA/Joel Kowsky)

This colorful view of Mercury was produced by using images from the color base map imaging campaign during MESSENGER's primary mission. These colors are not what Mercury would look like to the human eye, but rather the colors enhance the chemical, mineralogical, and physical differences between the rocks that make up Mercury's surface. <b>To watch a movie of this colorful view of Mercury as a spinning globe go here: <a href="http://www.flickr.com/photos/gsfc/8497927473">www.flickr.com/photos/gsfc/8497927473</a></b> Young crater rays, extending radially from fresh impact craters, appear light blue or white. Medium- and dark-blue areas are a geologic unit of Mercury's crust known as the &quot;low-reflectance material&quot;, thought to be rich in a dark, opaque mineral. Tan areas are plains formed by eruption of highly fluid lavas. The giant Caloris basin is the large circular tan feature located just to the upper right of center of the image. The MESSENGER spacecraft is the first ever to orbit the planet Mercury, and the spacecraft's seven scientific instruments and radio science investigation are unraveling the history and evolution of the Solar System's innermost planet. Visit the Why Mercury? section of this website to learn more about the key science questions that the MESSENGER mission is addressing. During the one-year primary mission, MESSENGER acquired 88,746 images and extensive other data sets. MESSENGER is now in a yearlong extended mission, during which plans call for the acquisition of more than 80,000 additional images to support MESSENGER's science goals. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington <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 colorful view of Mercury was produced by using images from the color base map imaging campaign during MESSENGER's primary mission. These colors are not what Mercury would look like to the human eye, but rather the colors enhance the chemical, mineralogical, and physical differences between the rocks that make up Mercury's surface. Young crater rays, extending radially from fresh impact craters, appear light blue or white. Medium- and dark-blue areas are a geologic unit of Mercury's crust known as the &quot;low-reflectance material&quot;, thought to be rich in a dark, opaque mineral. Tan areas are plains formed by eruption of highly fluid lavas. The crater in the upper right whose rays stretch across the planet is Hokusai. <b>To watch a movie of this colorful view of Mercury as a spinning globe go here: <a href="http://www.flickr.com/photos/gsfc/8497927473">www.flickr.com/photos/gsfc/8497927473</a></b> Young crater rays, extending radially from fresh impact craters, appear light blue or white. Medium- and dark-blue areas are a geologic unit of Mercury's crust known as the &quot;low-reflectance material&quot;, thought to be rich in a dark, opaque mineral. Tan areas are plains formed by eruption of highly fluid lavas. The giant Caloris basin is the large circular tan feature located just to the upper right of center of the image. The MESSENGER spacecraft is the first ever to orbit the planet Mercury, and the spacecraft's seven scientific instruments and radio science investigation are unraveling the history and evolution of the Solar System's innermost planet. Visit the Why Mercury? section of this website to learn more about the key science questions that the MESSENGER mission is addressing. During the one-year primary mission, MESSENGER acquired 88,746 images and extensive other data sets. MESSENGER is now in a yearlong extended mission, during which plans call for the acquisition of more than 80,000 additional images to support MESSENGER's science goals. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington <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/NASAGoddardPix" 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>

As temperatures dropped and daylight began to shorten, autumn colors began to wash over the deciduous forests of North America. The Moderate Resolution Imaging Spectroradiometer (MODIS) aboard NASA’s Terra satellite captured this true-color image of the northeastern United States and Canada on September 27, 2014. Washes of orange, brown and yellow are brightest in the Upper Peninsula of Michigan, upstate New York, New Hampshire, Vermont, Maine, and southern Quebec and Ontario. Also, faint traces of phytoplankton blooms can be seen in the offshore waters of the Atlantic Ocean. The transition of autumn leaves from green, to glowing with colors, to browning and dropping to the ground, involve several complex interactions and reactions. However, length of sunlight and the temperature changes are dominant factors. Topography also plays a role, as does latitude. Temperature tends to drop faster at higher elevations and at higher latitudes, and day length shortens more quickly at higher latitudes. Color change tends to begin in the north and sweep southward, and change begins at mountain tops then moves into valleys. As explained by the U.S. Forest Service, certain species of trees produce certain colors. Oaks generally turn red, brown, or russet; hickories become golden bronze; aspen and yellow-poplar turn golden. Maples differ by species. Red maple turns brilliant scarlet; sugar maple, orange-red; and black maple, yellow. Leaves of some trees, such as elms, simply become brown. Credit: NASA/GSFC/Jeff Schmaltz/MODIS Land Rapid Response Team <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/NASAGoddardPix" 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>

NASA Hubble Space Telescope captured this sharpest view yet of the most famous of all planetary nebulae: the Ring Nebula M57. The colors are approximately true colors.

Space shuttle Enterprise is seen as the United States Marine Corp Drum and Bugle Corps and Color Guard march by at the Steven F. Udvar-Hazy Center Thursday, April 19, 2012 in Chantilly, Va. Enterprise was the first space shuttle orbiter, built for NASA to perform test flights in the atmosphere and was not capable of spaceflight. It has been on display at the Udvar-Hazy Center's Space Hangar since 2004. Enterprise will be transferred to the Intrepid Sea, Air and Space Museum in New York City. Photo Credit: (NASA/Carla Cioffi)

SL2-03-126 (June 1973) --- A color infrared photograph of the Los Angeles County and Kern County area, taken from the Skylab space station in Earth orbit during its first manned Skylab mission. The Mojave Desert occupies the northeast one-fourth of the photograph. Lake Isabella in the Sierra Nevada Mountains is the v-shaped body of water. The San Gabriel Mountains extend across the southern part of the picture. At lower center is the intersection of the San Andreas and Garlock faults. The San Joaquin Valley is in the center at the left edge. (The picture should be held with the heavy cloud cover at lower right corner so that north will be at top.) This picture was exposed by one of the six lenses of the Itek-furnished S190-A Multispectral Photographic Facility experiment in the Multiple Docking Adapter of the Skylab space station. Type 2443 film was used. Photo credit: NASA

This modern-looking "geoboard" adds a pop of color to the lab at Malin Space Science Systems in San Diego, California. With an array of colors and textures, this board looks like art, but it is an important tool for camera testing. Imaging the color samples and the rock and mineral specimens gives the camera team important references for when they are imaging rocks on Mars with Mastcam-Z. https://photojournal.jpl.nasa.gov/catalog/PIA24199

A rainbow of colors is captured in the center of a magnificent barred spiral galaxy, as witnessed by the three cameras of NASA Hubble Space Telescope.

Today's image features a color view of the southern pole of Mercury. About midway down the image, the edge of the large Chao Meng-Fu crater, which lies almost directly on the south pole, can be seen poking out from the shadows. Surrounding Chao Meng-Fu are Roerich, Lovecraft, Hurley and L'Engle craters. This image was obtained as part of the 11-color south polar imaging campaign, through which scientists hope to be able to use the relative brightness of the surface in different colors to understand its composition. http://photojournal.jpl.nasa.gov/catalog/PIA19204

NASA Hubble Space Telescope snapped these images of the asteroid Vesta in preparation for the Dawn spacecraft visit in 2011. The images show the difference in brightness and color on the asteroid surface.

This false-color image from NASA Spitzer Space Telescope shows a dying star center surrounded by a cloud of glowing gas and dust.

A colorful image showing violent star formation triggered when two galaxies bumped into each other has been captured by NASA Hubble Space Telescope.

The false-color composite image of the Stephan’s Quintet galaxy cluster is made up of data from NASA Spitzer Space Telescope and a ground-based telescope in Spain.

These false-color image taken by NASA Spitzer Space Telescope shows the South Pillar region of the star-forming region called the Carina Nebula.

Looking like a colorful holiday card, a new image from NASA Hubble Space Telescope reveals a vibrant green and red nebula far from Earth.

This false-color infrared image from NASA Spitzer Space Telescope shows little dwarf galaxies forming in the tails of two larger galaxies that are colliding together.

This is a NASA Hubble Space Telescope color image of dwarf planet Ceres, the largest object in the asteroid belt. The contrast has been enhanced to reveal surface details.

This image was returned on Jan 14, 2005, by the European Space Agency Huygens probe during its successful descent to land on Titan. This colored view, following processing to add reflection spectra data, gives a better indication of the actual color.

NASA image acquired September 3, 2011 Dominici crater, the very bright crater to the top of this image, exhibits bright rays and contains hollows. This crater lies upon the peak ring of Homer Basin, a very degraded peak ring basin that has been filled by volcanism. This image contains several examples of craters that have excavated materials from depth that are spectrally distinct from the surface volcanic layers, providing windows into the subsurface. MESSENGER scientists are estimating the approximate depths of these spectrally distinct materials by applying knowledge of how impacts excavate material during the cratering process. The 1000, 750, and 430 nm bands of the Wide Angle Camera are displayed in red, green, and blue, respectively. This image was acquired as a high-resolution targeted observation. Targeted observations are images of a small area on Mercury's surface at resolutions much higher than the 250-meter/pixel (820 feet/pixel) morphology base map or the 1-kilometer/pixel (0.6 miles/pixel) color base map. It is not possible to cover all of Mercury's surface at this high resolution during MESSENGER's one-year mission, but several areas of high scientific interest are generally imaged in this mode each week. The MESSENGER spacecraft is the first ever to orbit the planet Mercury, and the spacecraft's seven scientific instruments and radio science investigation are unraveling the history and evolution of the Solar System's innermost planet. Visit the Why Mercury? section of this website to learn more about the key science questions that the MESSENGER mission is addressing. During the one-year primary mission, MDIS is scheduled to acquire more than 75,000 images in support of MESSENGER's science goals. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington <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://instagrid.me/nasagoddard/?vm=grid" rel="nofollow">Instagram</a></b>

This image from NASA's Spitzer Space Telescope shows the Tarantula Nebula in two wavelengths of infrared light, each represented by a different color. The red color at the heart of the nebula shows the presence of particularly hot gas emitting infrared light at a wavelength of 4.5 micrometers. The blue regions are dust composed of molecules called polycyclic aromatic hydrocarbons (PAHs), which are also found in ash from coal, wood and oil fires on Earth. Regions emitting both wavelengths appear white. https://photojournal.jpl.nasa.gov/catalog/PIA23646

Scientists produced new global maps of Jupiter using the Wide Field Camera 3 on NASA Hubble Space Telescope. One color map is shown here, projected onto a globe and as a flat image.

Tropical Cyclone Heat Potential TCHP field in the Gulf of Mexico during September 22, 2005. The path of Hurricane Rita is indicated with circles spaced every 3 hours with their size and color representing intensity see legend.

This false-color image from NASA Spitzer Space Telescope shows a distant galaxy yellow that houses a quasar, a super-massive black hole circled by a ring, or torus, of gas and dust.

Supernovae are the explosive deaths of the universe most massive stars. This false-color composite from NASA Spitzer Space Telescope and NASA Chandra X-ray Observatory shows the remnant of N132D, the wispy pink shell of gas at center.

This image from NASA Spitzer Space Telescope shows where the action is taking place in galaxy NGC 1291. The outer ring, colored red, is filled with new stars that are igniting and heating up dust that glows with infrared light.

This infrared image from NASA Spitzer Space Telescope shows the Helix nebula, a cosmic starlet often photographed by amateur astronomers for its vivid colors and eerie resemblance to a giant eye.

This new false-colored image from NASA Hubble, Chandra and Spitzer space telescopes shows a giant jet of particles that has been shot out from the vicinity of a type of supermassive black hole called a quasar.

This frame from an animation shows the motion of ice in Antarctica as measured by satellite data from various space agencies. The colors represent the speed of the ice flows in meters per year.

This image of the moon is from NASA Moon Mineralogy Mapper on the Indian Space Research Organization Chandrayaan-1 mission. It is a three-color composite of reflected near-infrared radiation from the sun.

NASA Spitzer, Hubble and Chandra space observatories teamed up to create this multi-wavelength, false-colored view of the M82 galaxy. The lively portrait celebrates Hubble weet sixteen birthday.

This image shows a series of color filters on the Color Filter Assembly for the Coronagraph Instrument on NASA's Nancy Grace Roman Space Telescope. Each filter blocks all but a specific color, or wavelength, of light. Many of the filters appear dark in this photo because they block all visible light – the range of wavelengths that are visible to the human eye – but are transparent to infrared light, which encompasses a range of wavelengths slightly longer than visible light. Most of the filters will be used by the instrument for calibration purposes, but there are scientific uses for some of the filters as well. The presence or absence of different wavelengths can reveal properties of exoplanets (planets around other stars) including their chemical composition and the presence of clouds high or low in their atmospheres. For example, cold gas giant planets with high clouds will appear redder, like Jupiter, compared to those without high clouds, like Neptune. https://photojournal.jpl.nasa.gov/catalog/PIA25436

This image shows an outflow of gas from a new star as it jets from a space object dubbed IRAS 21078+5211. The reddish blob in its center, as picked up by NASA Spitzer Space Telescope contrasts nicely with the clouds, colored green, that surround it.

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. These false color images may reveal subtle variations of the surface not easily identified in a single band image. Today's false color image shows part of Nili Fossae. Nili Fossae is a collection of curved faults and down-dropped blocks of crust between the faults called graben. The graben lie northeast of the large volcano Syrtis Major and northwest of the ancient impact basin Isidis Planitia. The linear ridge in the center of the image is one side of a very large graben. When large amounts of pressure or tension are applied to rocks on timescales that are fast enough that the rock cannot respond by deforming, the rock breaks along faults. In the case of a graben, two parallel faults are formed by extension of the crust and the rock in between the faults drops downward into the space created by the extension. The THEMIS VIS camera is capable of capturing color images of the Martian surface using five different color filters. In this mode of operation, the spatial resolution and coverage of the image must be reduced to accommodate the additional data volume produced from using multiple filters. To make a color image, three of the five filter images (each in grayscale) are selected. Each is contrast enhanced and then converted to a red, green, or blue intensity image. These three images are then combined to produce a full color, single image. Because the THEMIS color filters don't span the full range of colors seen by the human eye, a color THEMIS image does not represent true color. Also, because each single-filter image is contrast enhanced before inclusion in the three-color image, the apparent color variation of the scene is exaggerated. Nevertheless, the color variation that does appear is representative of some change in color, however subtle, in the actual scene. Note that the long edges of THEMIS color images typically contain color artifacts that do not represent surface variation. Orbit Number: 85787 Latitude: 19.3564 Longitude: 73.5306 Instrument: VIS Captured: 2021-04-17 00:20 https://photojournal.jpl.nasa.gov/catalog/PIA25093

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. These false color images may reveal subtle variations of the surface not easily identified in a single band image. Today's false color image shows a small portion of Tempe Fossae. The linear features are tectonic graben. Graben are formed by extension of the crust and faulting. When large amounts of pressure or tension are applied to rocks on timescales that are fast enough that the rock cannot respond by deforming, the rock breaks along faults. In the case of a graben, two parallel faults are formed by extension of the crust and the rock in between the faults drops downward into the space created by the extension. The complete fossae system in almost 2000 km (1242 miles) long. The THEMIS VIS camera is capable of capturing color images of the Martian surface using five different color filters. In this mode of operation, the spatial resolution and coverage of the image must be reduced to accommodate the additional data volume produced from using multiple filters. To make a color image, three of the five filter images (each in grayscale) are selected. Each is contrast enhanced and then converted to a red, green, or blue intensity image. These three images are then combined to produce a full color, single image. Because the THEMIS color filters don't span the full range of colors seen by the human eye, a color THEMIS image does not represent true color. Also, because each single-filter image is contrast enhanced before inclusion in the three-color image, the apparent color variation of the scene is exaggerated. Nevertheless, the color variation that does appear is representative of some change in color, however subtle, in the actual scene. Note that the long edges of THEMIS color images typically contain color artifacts that do not represent surface variation. Orbit Number: 94065 Latitude: 46.5357 Longitude: 293.867 Instrument: VIS Captured: 2023-02-27 15:03 https://photojournal.jpl.nasa.gov/catalog/PIA26125

SL2-03-118 (June 1973) --- An infrared photograph of the San Francisco Bay, California area, taken from the Skylab 1/2 space station in Earth orbit. THE PICTURE SHOULD BE HELD WITH THE CLOUDS AND PACIFIC OCEAN ON THE LEFT. This photograph was taken by one of the six lenses of the Itek-furnished S190-A Multispectral Photographic Facility Experiment in the Multiple Docking Adapter of the space station. Type 2443 film was used. Note the thickly populated and highly developed area around the bay. Among the cities visible in this photograph are San Francisco, Oakland, Berkeley and San Jose. This view extends eastward to show a portion of the San Joaquin Valley. The S190-A experiment is part of the Skylab Earth Resources Experiment Package (EREP). Photo credit: NASA

SL2-03-200 (22 June 1973) --- The city of Phoenix, AZ (33.5N, 112.0W) can be seen in good detail in this color infrared scene. Situated among truck crop agriculture fields, the color infrared photo depicts the vegetated fields as shades of red making the agriculture stand out in this desert environment. To the east, Lake Theodore Roosevelt and dam can be easily seen. Photo credit: NASA

This trick that the planet is looking back at you is actually a Hubble treat: An eerie, close-up view of Jupiter, the biggest planet in our solar system. Hubble was monitoring changes in Jupiter’s immense Great Red Spot (GRS) storm on April 21, 2014, when the shadow of the Jovian moon, Ganymede, swept across the center of the storm. This gave the giant planet the uncanny appearance of having a pupil in the center of a 10,000 mile-diameter “eye.” For a moment, Jupiter “stared” back at Hubble like a one-eyed giant Cyclops. Credit: NASA, ESA, and A. Simon (Goddard Space Flight Center) <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/NASAGoddardPix" 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>

SL2-03-192 (22 June 1973) --- Lake Mead, Nevada, (36.0N, 114.5E) where the water from the Colorado River empties after it's 273 mile journey through the Grand Canyon of Arizona is the subject of this photo. Other features of interest are Hoover Dam on the south shore of Lake Mead where cheap hydroelectric power is secondary to the water resources made available in this northern desert region and the resort city of Las Vegas, just to the west of Lake Mead. In this harsh desert environment, color infrared photography readily penetrates haze, detects and portrays vegetation as shades of red. Photo credit: NASA

ISS040-E-007560 (5 June 2014) --- A colorful view of the interior of the Columbus laboratory of the International Space Station is featured in this image photographed by an Expedition 40 crew member on the station. The colored lighting is from the Veggie experiment in Columbus.

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. These false color images may reveal subtle variations of the surface not easily identified in a single band image. Today's false color image shows part of Terra Sirenum. The linear features at the bottom of the image are tectonic features called graben. These graben are part of Sirenum Fossae. Graben are formed by extension of the crust and faulting. When large amounts of pressure or tension are applied to rocks on timescales that are fast enough that the rock cannot respond by deforming, the rock breaks along faults. In the case of a graben, two parallel faults are formed by extension of the crust and the rock in between the faults drops downward into the space created by the extension.The graben in this image are trending from north-northeast to south-southwest. Because the faults defining the graben are formed perpendicular to the direction of the applied stress, we know that extensional forces were pulling the crust apart in the west-northwest/east-southeast direction. The Sirenum Fossae graben are 2735km (1700 miles) long. The THEMIS VIS camera is capable of capturing color images of the Martian surface using five different color filters. In this mode of operation, the spatial resolution and coverage of the image must be reduced to accommodate the additional data volume produced from using multiple filters. To make a color image, three of the five filter images (each in grayscale) are selected. Each is contrast enhanced and then converted to a red, green, or blue intensity image. These three images are then combined to produce a full color, single image. Because the THEMIS color filters don't span the full range of colors seen by the human eye, a color THEMIS image does not represent true color. Also, because each single-filter image is contrast enhanced before inclusion in the three-color image, the apparent color variation of the scene is exaggerated. Nevertheless, the color variation that does appear is representative of some change in color, however subtle, in the actual scene. Note that the long edges of THEMIS color images typically contain color artifacts that do not represent surface variation. Orbit Number: 91704 Latitude: -32.2019 Longitude: 203.852 Instrument: VIS Captured: 2022-08-17 04:19 https://photojournal.jpl.nasa.gov/catalog/PIA26084

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. These false color images may reveal subtle variations of the surface not easily identified in a single band image. Today's false color image shows part of Sirenum Fossae. The linear depressions in this VIS image are tectonic graben. Graben are formed by extension of the crust and faulting. When large amounts of pressure or tension are applied to rocks on timescales that are fast enough that the rock cannot respond by deforming, the rock breaks along faults. In the case of a graben, two parallel faults are formed by extension of the crust and the rock in between the faults drops downward into the space created by the extension. Several graben are visible in this THEMIS VIS image, trending from north-northeast to south-southwest. Because the faults defining the graben are formed perpendicular to the direction of the applied stress, we know that extensional forces were pulling the crust apart in the west-northwest/east-southeast direction. The Sirenum Fossae graben are 2735km (1700 miles) long. The THEMIS VIS camera is capable of capturing color images of the Martian surface using five different color filters. In this mode of operation, the spatial resolution and coverage of the image must be reduced to accommodate the additional data volume produced from using multiple filters. To make a color image, three of the five filter images (each in grayscale) are selected. Each is contrast enhanced and then converted to a red, green, or blue intensity image. These three images are then combined to produce a full color, single image. Because the THEMIS color filters don't span the full range of colors seen by the human eye, a color THEMIS image does not represent true color. Also, because each single-filter image is contrast enhanced before inclusion in the three-color image, the apparent color variation of the scene is exaggerated. Nevertheless, the color variation that does appear is representative of some change in color, however subtle, in the actual scene. Note that the long edges of THEMIS color images typically contain color artifacts that do not represent surface variation. Orbit Number: 92540 Latitude: -32.6048 Longitude: 205.563 Instrument: VIS Captured: 2022-10-25 00:23 https://photojournal.jpl.nasa.gov/catalog/PIA26122

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. These false color images may reveal subtle variations of the surface not easily identified in a single band image. Today's false color image shows part of Terra Sirenum. The linear features at the top of the image are tectonic features called graben. These graben are part of Sirenum Fossae. Graben are formed by extension of the crust and faulting. When large amounts of pressure or tension are applied to rocks on timescales that are fast enough that the rock cannot respond by deforming, the rock breaks along faults. In the case of a graben, two parallel faults are formed by extension of the crust and the rock in between the faults drops downward into the space created by the extension.The graben in this image are trending from north-northeast to south-southwest. Because the faults defining the graben are formed perpendicular to the direction of the applied stress, we know that extensional forces were pulling the crust apart in the west-northwest/east-southeast direction. The Sirenum Fossae graben are 2735km (1700 miles) long. The THEMIS VIS camera is capable of capturing color images of the Martian surface using five different color filters. In this mode of operation, the spatial resolution and coverage of the image must be reduced to accommodate the additional data volume produced from using multiple filters. To make a color image, three of the five filter images (each in grayscale) are selected. Each is contrast enhanced and then converted to a red, green, or blue intensity image. These three images are then combined to produce a full color, single image. Because the THEMIS color filters don't span the full range of colors seen by the human eye, a color THEMIS image does not represent true color. Also, because each single-filter image is contrast enhanced before inclusion in the three-color image, the apparent color variation of the scene is exaggerated. Nevertheless, the color variation that does appear is representative of some change in color, however subtle, in the actual scene. Note that the long edges of THEMIS color images typically contain color artifacts that do not represent surface variation. Orbit Number: 91654 Latitude: -33.0364 Longitude: 206.174 Instrument: VIS Captured: 2022-08-13 01:31 https://photojournal.jpl.nasa.gov/catalog/PIA26083

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. These false color images may reveal subtle variations of the surface not easily identified in a single band image. Today's false color image shows part of Sirenum Fossae. The linear depressions in this VIS image are tectonic graben. Graben are formed by extension of the crust and faulting. When large amounts of pressure or tension are applied to rocks on timescales that are fast enough that the rock cannot respond by deforming, the rock breaks along faults. In the case of a graben, two parallel faults are formed by extension of the crust and the rock in between the faults drops downward into the space created by the extension. Several graben are visible in this THEMIS VIS image, trending from north-northeast to south-southwest. Because the faults defining the graben are formed parallel to the direction of the applied stress, we know that extensional forces were pulling the crust apart in the west-northwest/east-southeast direction. The Sirenum Fossae graben are 2735km (1700 miles) long. The THEMIS VIS camera is capable of capturing color images of the Martian surface using five different color filters. In this mode of operation, the spatial resolution and coverage of the image must be reduced to accommodate the additional data volume produced from using multiple filters. To make a color image, three of the five filter images (each in grayscale) are selected. Each is contrast enhanced and then converted to a red, green, or blue intensity image. These three images are then combined to produce a full color, single image. Because the THEMIS color filters don't span the full range of colors seen by the human eye, a color THEMIS image does not represent true color. Also, because each single-filter image is contrast enhanced before inclusion in the three-color image, the apparent color variation of the scene is exaggerated. Nevertheless, the color variation that does appear is representative of some change in color, however subtle, in the actual scene. Note that the long edges of THEMIS color images typically contain color artifacts that do not represent surface variation. Orbit Number: 84903 Latitude: -30.8518 Longitude: 208.42 Instrument: VIS Captured: 2021-02-03 04:32 https://photojournal.jpl.nasa.gov/catalog/PIA25007

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. These false color images may reveal subtle variations of the surface not easily identified in a single band image. Today's false color image shows part of Sirenum Fossae. The linear depressions in this VIS image are tectonic graben. Graben are formed by extension of the crust and faulting. When large amounts of pressure or tension are applied to rocks on timescales that are fast enough that the rock cannot respond by deforming, the rock breaks along faults. In the case of a graben, two parallel faults are formed by extension of the crust and the rock in between the faults drops downward into the space created by the extension. Several graben are visible in this THEMIS VIS image, trending from north-northeast to south-southwest. Because the faults defining the graben are formed parallel to the direction of the applied stress, we know that extensional forces were pulling the crust apart in the west-northwest/east-southeast direction. The Sirenum Fossae graben are 2735km (1700 miles) long. The THEMIS VIS camera is capable of capturing color images of the Martian surface using five different color filters. In this mode of operation, the spatial resolution and coverage of the image must be reduced to accommodate the additional data volume produced from using multiple filters. To make a color image, three of the five filter images (each in grayscale) are selected. Each is contrast enhanced and then converted to a red, green, or blue intensity image. These three images are then combined to produce a full color, single image. Because the THEMIS color filters don't span the full range of colors seen by the human eye, a color THEMIS image does not represent true color. Also, because each single-filter image is contrast enhanced before inclusion in the three-color image, the apparent color variation of the scene is exaggerated. Nevertheless, the color variation that does appear is representative of some change in color, however subtle, in the actual scene. Note that the long edges of THEMIS color images typically contain color artifacts that do not represent surface variation. Orbit Number: 84379 Latitude: -32.7134 Longitude: 204.562 Instrument: VIS Captured: 2020-12-22 01:06 https://photojournal.jpl.nasa.gov/catalog/PIA25004

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. These false color images may reveal subtle variations of the surface not easily identified in a single band image. Today's false color image shows part of Sirenum Fossae. The linear depressions in this VIS image are tectonic graben. Graben are formed by extension of the crust and faulting. When large amounts of pressure or tension are applied to rocks on timescales that are fast enough that the rock cannot respond by deforming, the rock breaks along faults. In the case of a graben, two parallel faults are formed by extension of the crust and the rock in between the faults drops downward into the space created by the extension. Several graben are visible in this THEMIS VIS image, trending from north-northeast to south-southwest. Because the faults defining the graben are formed parallel to the direction of the applied stress, we know that extensional forces were pulling the crust apart in the west-northwest/east-southeast direction. The Sirenum Fossae graben are 2735km (1700 miles) long. The THEMIS VIS camera is capable of capturing color images of the Martian surface using five different color filters. In this mode of operation, the spatial resolution and coverage of the image must be reduced to accommodate the additional data volume produced from using multiple filters. To make a color image, three of the five filter images (each in grayscale) are selected. Each is contrast enhanced and then converted to a red, green, or blue intensity image. These three images are then combined to produce a full color, single image. Because the THEMIS color filters don't span the full range of colors seen by the human eye, a color THEMIS image does not represent true color. Also, because each single-filter image is contrast enhanced before inclusion in the three-color image, the apparent color variation of the scene is exaggerated. Nevertheless, the color variation that does appear is representative of some change in color, however subtle, in the actual scene. Note that the long edges of THEMIS color images typically contain color artifacts that do not represent surface variation. Orbit Number: 83755 Latitude: -32.1324 Longitude: 205.871 Instrument: VIS Captured: 2020-10-31 16:02 https://photojournal.jpl.nasa.gov/catalog/PIA25001

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. These false color images may reveal subtle variations of the surface not easily identified in a single band image. Today's false color image shows part of Sirenum Fossae. The linear depressions in this VIS image are tectonic graben. Graben are formed by extension of the crust and faulting. When large amounts of pressure or tension are applied to rocks on timescales that are fast enough that the rock cannot respond by deforming, the rock breaks along faults. In the case of a graben, two parallel faults are formed by extension of the crust and the rock in between the faults drops downward into the space created by the extension. Several graben are visible in this THEMIS VIS image, trending from north-northeast to south-southwest. Because the faults defining the graben are formed parallel to the direction of the applied stress, we know that extensional forces were pulling the crust apart in the west-northwest/east-southeast direction. The Sirenum Fossae graben are 2735km (1700 miles) long. The THEMIS VIS camera is capable of capturing color images of the Martian surface using five different color filters. In this mode of operation, the spatial resolution and coverage of the image must be reduced to accommodate the additional data volume produced from using multiple filters. To make a color image, three of the five filter images (each in grayscale) are selected. Each is contrast enhanced and then converted to a red, green, or blue intensity image. These three images are then combined to produce a full color, single image. Because the THEMIS color filters don't span the full range of colors seen by the human eye, a color THEMIS image does not represent true color. Also, because each single-filter image is contrast enhanced before inclusion in the three-color image, the apparent color variation of the scene is exaggerated. Nevertheless, the color variation that does appear is representative of some change in color, however subtle, in the actual scene. Note that the long edges of THEMIS color images typically contain color artifacts that do not represent surface variation. Orbit Number: 84841 Latitude: -35.7019 Longitude: 196.266 Instrument: VIS Captured: 2021-01-29 02:03 https://photojournal.jpl.nasa.gov/catalog/PIA25005

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. These false color images may reveal subtle variations of the surface not easily identified in a single band image. Today's false color image shows part of Sirenum Fossae. The linear depressions in this VIS image are tectonic graben. Graben are formed by extension of the crust and faulting. When large amounts of pressure or tension are applied to rocks on timescales that are fast enough that the rock cannot respond by deforming, the rock breaks along faults. In the case of a graben, two parallel faults are formed by extension of the crust and the rock in between the faults drops downward into the space created by the extension. Several graben are visible in this THEMIS VIS image, trending from north-northeast to south-southwest. Because the faults defining the graben are formed perpendicular to the direction of the applied stress, we know that extensional forces were pulling the crust apart in the west-northwest/east-southeast direction. The Sirenum Fossae graben are 2735km (1700 miles) long. The THEMIS VIS camera is capable of capturing color images of the Martian surface using five different color filters. In this mode of operation, the spatial resolution and coverage of the image must be reduced to accommodate the additional data volume produced from using multiple filters. To make a color image, three of the five filter images (each in grayscale) are selected. Each is contrast enhanced and then converted to a red, green, or blue intensity image. These three images are then combined to produce a full color, single image. Because the THEMIS color filters don't span the full range of colors seen by the human eye, a color THEMIS image does not represent true color. Also, because each single-filter image is contrast enhanced before inclusion in the three-color image, the apparent color variation of the scene is exaggerated. Nevertheless, the color variation that does appear is representative of some change in color, however subtle, in the actual scene. Note that the long edges of THEMIS color images typically contain color artifacts that do not represent surface variation. Orbit Number: 92203 Latitude: -31.0389 Longitude: 208.065 Instrument: VIS Captured: 2022-09-27 06:25 https://photojournal.jpl.nasa.gov/catalog/PIA26087

These two false-color images of the Manaus region of Brazil in South America were acquired by the Spaceborne Imaging Radar-C and X-band Synthetic Aperture Radar on board the space shuttle Endeavour. The image at left was acquired on April 12, 1994, and the image at right was acquired on October 3, 1994. The area shown is approximately 8 kilometers by 40 kilometers (5 miles by 25 miles). The two large rivers in this image, the Rio Negro (at top) and the Rio Solimoes (at bottom), combine at Manaus (west of the image) to form the Amazon River. The image is centered at about 3 degrees south latitude and 61 degrees west longitude. North is toward the top left of the images. The false colors were created by displaying three L-band polarization channels: red areas correspond to high backscatter, horizontally transmitted and received, while green areas correspond to high backscatter, horizontally transmitted and vertically received. Blue areas show low returns at vertical transmit/receive polarization; hence the bright blue colors of the smooth river surfaces can be seen. Using this color scheme, green areas in the image are heavily forested, while blue areas are either cleared forest or open water. The yellow and red areas are flooded forest or floating meadows. The extent of the flooding is much greater in the April image than in the October image and appears to follow the 10-meter (33-foot) annual rise and fall of the Amazon River. The flooded forest is a vital habitat for fish, and floating meadows are an important source of atmospheric methane. These images demonstrate the capability of SIR-C/X-SAR to study important environmental changes that are impossible to see with optical sensors over regions such as the Amazon, where frequent cloud cover and dense forest canopies block monitoring of flooding. Field studies by boat, on foot and in low-flying aircraft by the University of California at Santa Barbara, in collaboration with Brazil's Instituto Nacional de Pesguisas Estaciais, during the first and second flights of the SIR-C/X-SAR system have validated the interpretation of the radar images. http://photojournal.jpl.nasa.gov/catalog/PIA01735

The Patrick Air Force Base color guard presents the colors during the playing of the national anthem during this year's Day of Remembrance ceremony at the Kennedy Space Center Visitor Complex. Each year spaceport employees and guests join others throughout NASA honoring the contributions of astronauts who have perished in the conquest of space.

In visible light, the bulk of our Milky Way galaxy stars are eclipsed behind thick clouds of galactic dust and gas. But to the infrared eyes of NASA Spitzer Space Telescope, distant stars and dust clouds shine with unparalleled clarity and color.

This color composite C-band and L-band image of the Kilauea volcano on the Big Island of Hawaii was acquired by NASA Spaceborne Imaging Radar-C/X-band Synthetic Aperture Radar SIR-C/X-SAR flying on space shuttle Endeavour.

Something appears to be peering through a shiny red mask, in this new false-colored image from NASA Spitzer Space Telescope. The mysterious blue eyes are actually starlight from the cores of two merging galaxies, called NGC 2207 and IC 2163.

This image, taken by NASA Hubble Space Telescope, shows the colorful last hurrah of a star like our Sun. The star is ending its life by casting off its outer layers of gas, which formed a cocoon around the star remaining core.

This false-color L-band image of the Manaus region of Brazil was acquired by NASA Spaceborne Imaging Radar-C and X-Band Synthetic Aperture Radar SIR-C/X-SAR aboard the space shuttle Endeavour on orbit 46 of the mission.

Our Milky Way galaxy is ablaze with dust in this new all-sky map from Planck, a European Space Agency mission with important NASA contributions. The towers of fiery colors are actually dust in the galaxy and beyond that has been polarized.

This is a color Hubble Space Telescope (HST) heritage image of supernova remnant N49, a neighboring galaxy, that was taken with Hubble's Wide Field Planetary Camera 2. Color filters were used to sample light emitted by sulfur, oxygen, and hydrogen. The color image was superimposed on a black and white image of stars in the same field also taken with Hubble. Resembling a fireworks display, these delicate filaments are actually sheets of debris from a stellar explosion.

ISS048e056981 (0813/2016) --- Sparkling aurora colors of magenta and green color the sky's while the International Space Station orbits above the planet every 90 minutes. SpaceX’s Dragon resupply vehicle is seen docked to the Earth-facing port of the Harmony module.

A tray holding 39 sample tubes headed to Mars is installed into the Perseverance rover on May 21, 2020, in a clean room at NASA's Kennedy Space Center in Florida during final installation for launch. Each tube is enveloped in its own gold-colored titanium sheath that protects it until the sample handling arm within the rover retrieves it to begin the process of collecting a sample of Martian rock or regolith (dust and crushed rock). In total, the rover carries 43 sample tubes. https://photojournal.jpl.nasa.gov/catalog/PIA24305

NASA's Curiosity Mars rover recorded this view of the sun setting at the close of the mission's 956th Martian day, or sol (April 15, 2015), from the rover's location in Gale Crater. This was the first sunset observed in color by Curiosity. The image comes from the left-eye camera of the rover's Mast Camera (Mastcam). The color has been calibrated and white-balanced to remove camera artifacts. Mastcam sees color very similarly to what human eyes see, although it is actually a little less sensitive to blue than people are. Dust in the Martian atmosphere has fine particles that permit blue light to penetrate the atmosphere more efficiently than longer-wavelength colors. That causes the blue colors in the mixed light coming from the sun to stay closer to sun's part of the sky, compared to the wider scattering of yellow and red colors. The effect is most pronounced near sunset, when light from the sun passes through a longer path in the atmosphere than it does at mid-day. Malin Space Science Systems, San Diego, built and operates the rover's Mastcam. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology, Pasadena, manages the Mars Science Laboratory Project for NASA's Science Mission Directorate, Washington. JPL designed and built the project's Curiosity rover. http://photojournal.jpl.nasa.gov/catalog/PIA19400

This image from NASA's Spitzer Space Telescope shows the Tarantula Nebula in three wavelengths of infrared light, each represented by a different color. The magenta-colored regions are dust composed of molecules called polycyclic aromatic hydrocarbons (PAHs), which are also found in ash from coal, wood and oil fires on Earth. PAHs emit in multiple wavelengths. The PAHs emit in multiple wavelengths, so the magenta color is a combination of red (corresponding to an infrared wavelength of 8 micrometers) and blue (3.6 micrometers). The green color in this image shows the presence of particularly hot gas emitting infrared light at a wavelength of 4.5 micrometers. The stars in the image are mostly a combination of green and blue. White hues indicate regions that radiate in all three wavelengths. https://photojournal.jpl.nasa.gov/catalog/PIA23647

A recent Hubble Space Telescope (HST) view reveals Uranus surrounded by its 4 major rings and 10 of its 17 known satellites. This false color image was generated by Erich Karoschka using data taken with Hubble's Near Infrared Camera and Multi-Object Spectrometer. The HST recently found about 20 clouds. The colors in the image indicate altitude. The green and blue regions show where the atmosphere is clear and can be penetrated by sunlight. In yellow and grey regions, the sunlight reflects from a higher haze or cloud layer. The orange and red colors indicate very high clouds, such as cirrus clouds on Earth.

KENNEDY SPACE CENTER, FLA. -- A tri-colored heron stands sentry in the marshes around KSC. It has slate blue feathers on most of its body except for a white chest and belly and a rust-colored neck. It has long yellow legs, a white stripe that runs up its neck and long pointed yellow bill. The bill turns blue during breeding season.The heron is one of 310 species of birds that inhabit the Merritt Island National Wildlife Refuge, which shares a boundary with KSC. The marshes and open water of the refuge also provide wintering areas for 23 species of migratory waterfowl, as well as a year-round home for great egrets, wood storks, cormorants, brown pelicans and other species of marsh and shore birds.

**This image was taken at 3:38 a.m. EDT on July 13, one day before New Horizons’ closest approach to Pluto.** New Horizons has obtained impressive new images of Pluto and its large moon Charon that highlight their compositional diversity. These are not actual color images of Pluto and Charon—they are shown here in exaggerated colors that make it easy to note the differences in surface material and features on each planetary body. The images were obtained using three of the color filters of the “Ralph” instrument on July 13 at 3:38 am EDT. New Horizons has seven science instruments on board the spacecraft—including “Ralph” and “Alice”, whose names are a throwback to the “Honeymooners,” a popular 1950s sitcom. “These images show that Pluto and Charon are truly complex worlds. There's a whole lot going on here,” said New Horizons co-investigator Will Grundy, Lowell Observatory, Flagstaff, Arizona. “Our surface composition team is working as fast as we can to identify the substances in different regions on Pluto and unravel the processes that put them where they are.” The color data helps scientists understand the molecular make-up of ices on the surfaces of Pluto and Charon, as well as the age of geologic features such as craters. They can also tell us about surface changes caused by space “weather,” such as radiation. The new color images reveal that the “heart” of Pluto actually consists of two remarkably different-colored regions. In the false-color image, the heart consists of a western lobe shaped like an ice cream cone that appears peach color in this image. A mottled area on the right (east) side looks bluish. A mid-latitude band appears in shades ranging from pale blue through red. Even within the northern polar cap, in the upper part of the image, various shades of yellow-orange indicate subtle compositional differences. This image was obtained using three of the color filters of the Ralph instrument on July 13 at 3:38 am EDT and received on the ground on at 12:25 pm. Charon is Just as Colorful The surface of Charon is viewed using the same exaggerated color. The red on the dark northern polar cap of Charon is attributed to hydrocarbon and other molecules, a class of chemical compounds called tholins. The mottled colors at lower latitudes point to the diversity of terrains on Charon. This image was obtained using three of the color filters of the Ralph instrument on July 13 at 3:38 am EDT and received on the ground on at 12:25 pm. “We make these color images to highlight the variety of surface environments present in the Pluto system,” said Dennis Reuter, co-investigator with the New Horizons Composition Team. “They show us in an intuitive way that there is much still to learn from the data coming down.” Due to the three-billion-mile distance to Pluto, data takes 4 ½ hours to come to Earth, even at the speed of light. It will take 16 months for all of New Horizons’ science data to be received, and the treasure trove from this mission will be studied for decades to come. Image Caption: Pluto and Charon in False Color Show Compositional Diversity This July 13, 2015, image of Pluto and Charon is presented in false colors to make differences in surface material and features easy to see. It was obtained by the Ralph instrument on NASA's New Horizons spacecraft, using three filters to obtain color information, which is exaggerated in the image. These are not the actual colors of Pluto and Charon, and the apparent distance between the two bodies has been reduced for this side-by-side view. The image reveals that the bright heart-shaped region of Pluto includes areas that differ in color characteristics. The western lobe, shaped like an ice-cream cone, appears peach color in this image. A mottled area on the right (east) appears bluish. Even within Pluto's northern polar cap, in the upper part of the image, various shades of yellow-orange indicate subtle compositional differences. The surface of Charon is viewed using the same exaggerated color. The red on the dark northern polar cap of Charon is attributed to hydrocarbon materials including a class of chemical compounds called tholins. The mottled colors at lower latitudes point to the diversity of terrains on Charon. --- At 7:49 AM EDT on Tuesday, July 14 New Horizons sped past Pluto at 30,800 miles per hour (49,600 kilometers per hour), with a suite of seven science instruments. As planned, New Horizons went incommunicado as it hurtled through the Pluto-Charon system busily gathering data. The New Horizons team will breathe a sigh of relief when New Horizons “phones home” at approximately 9:02 p.m. EDT on July 14. The mission to the icy dwarf planet completes the initial reconnaissance of the solar system. Stay in touch with the New Horizons mission with #PlutoFlyby and on Facebook at: <a href="https://www.facebook.com/new.horizons1" rel="nofollow">www.facebook.com/new.horizons1</a>

STS039-88-054 (28 April-6 May 1991) --- The dense urban development of the New York City metropolitan area in downstate New York, Long Island and New Jersey shows up as gray and white on this color Infrared photograph. The scene was taken on a remarkably clear spring day. Almost all the major man-made structures of the area are obvious, including ship traffic in and out of New York Harbor, the piers, all of the bridges spanning the area rivers and connecting Manhattan Island with New Jersey, the Bronx, Brooklyn and Queens, the three major airports (Newark, La Guardia and JFK), the New York State thruway, as well as Shea Stadium and Yankee Stadium. The reds and pinks are vegetated areas. Central Park clearly shows up on Manhattan, as do the string of parks along the cliffs (formed by the Palisades sill) along the west side of the Hudson north of the George Washington Bridge.

STS039-87-012 (28 April-6 May 1991) --- A handheld 70mm camera onboard the Space Shuttle Discovery exposed this infrared frame showing oil fires near the Kuwait coast as well as south-bound oil slicks in the Gulf. Pools of oil on the land are recognized as white objects near the burning wells.