The Venus of Willendorf made from Oolitic limestone.

The Venus of Willendorf made from Oolitic limestone.
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This view of Mars was captured by NASA's Odyssey orbiter using its Thermal Emission Imaging System, or THEMIS, camera. This image is a false color composite, made by combining three channels of infrared data that highlight water-ice clouds and dust in the atmosphere. This panorama was one of 10 captured on May 9, 2023, from an altitude of roughly 250 miles (400 kilometers) above the Martian surface - about the same altitude at which the International Space Station flies over Earth. The 10 panoramas of the Martian horizon were taken to capture a one-of-a-kind view of the Martian atmosphere as Odyssey circled the planet during its two-hour orbit. The reason why the view is so uncommon is because of the challenges involved in creating it. Engineers at NASA's Jet Propulsion Laboratory in Southern California (which leads the Odyssey mission) and Lockheed Martin Space (which built Odyssey and co-leads day-to-day operations) spent three months planning the observations. THEMIS' sensitivity to
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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 Chia Crater. Chia Crater is 92 km (57 miles) in diameter and is located in Xanthe Terra just east of Maja Valles. 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 ful
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This anaglyph from from NASA's Mars Exploration Rover Opportunity is of Victoria crater, looking north from 'Duck Bay' towards the dramatic promontory called 'Cape Verde.' 3D glasses are necessary to view this image.
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The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the floor of Melas Chasma.
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Valles Marineris
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This VIS image is located in Arabia Terra. 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. Orbit Number 61900 Latitude -8.73294 Longitude 352.802 Instrument VIS Captured 2015-11-27 14 36
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Albert Edler von Obermayer's 1899 silver gelatin photograph captures light forming stripe patterns, demonstrating photochemical reactions in a laboratory experiment.
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Full-Circle 'Bonestell' Panorama from Spirit
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This image shows part of Syria Planum
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NASA's Mars Exploration Rover captured this stereo, 360-degree view near the ridgeline of Endeavour Crater's western rim. The center is southeastward. You need 3D glasses to view this image.
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This image shows part of the south polar region
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Many constellations in the summer sky
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Today's VIS image shows part of the floor of Rutherford Crater. Blue tones in false color images are indicative of basaltic sand. Rutherford Crater is approximately 107 km (66 miles) in diameter. This crater is located in Arabia Terra. 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. Orbit Number 61900 Latitude 18.9562 Longitude 349.107 Instrument VIS Captured 2015-11-27 14 45
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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 the vast volcanic plains in the Tharsis region, in this case east of Pavonis Mons. The mottled appearance of the image is being caused by high altitude cloud cover. These clouds will be primarily composed of ice rather than dust. 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
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Three of Perseverance's Depot Locations. NASA's Perseverance Mars rover used its Mastcam-Z camera to take this image of the location where three of its 10 sample tubes will be deposited. 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/PIA25679
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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 cross section of Gale Crater, including the large layered deposit in the center of the crater. The Curiosity Rover is located on the floor of Gale Crater. Orbit Number 71162 Latitude -5.39778 Longitude 138.328 Instrument VIS Captured 2017-12-29 14 50
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This enhanced-color view of the eastern rim and floor of Victoria
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A Crater of Clues to Mars' Buried Past
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Image Number: 1746-29965202Rights ManagedCredit Line:World History Archive/Image Asset Management/SuperStockCollection:Image Asset ManagementStory:Mars Surface and Atmosphere ViewsContributor:World History ArchiveModel Release:NoProperty Release:NoResolution:2853×7351
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