This image from NASA's Mars Reconnaissance Orbiter shows one of two spots that likely appeared in connection with the Oct. 19, 2016, arrival of ESA's Schiaparelli test lander.

This image from NASA's Mars Reconnaissance Orbiter shows one of two spots that likely appeared in connection with the Oct. 19, 2016, arrival of ESA's Schiaparelli test lander.
SuperStock offers millions of photos, videos, and stock assets to creatives around the world. This image of This image from NASA's Mars Reconnaissance Orbiter shows one of two spots that likely appeared in connection with the Oct. 19, 2016, arrival of ESA's Schiaparelli test lander. by Piemags/PL Photography Limited is available for licensing today.

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This image was obtained by NASA's Cassini radar instrument during a flyby on Oct. 28, 2005. Equatorial Pass (Trailing hemisphere, Central Adiri, Central Belet, Huygens Landing Site, Antillia Faculae).
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Bright strands in Saturn's ever changing F ring emerge from the planet's shadow. The F ring usually has a single bright core, about 50 kilometers (31 miles) across, but the section of the ring seen here appears to have a second bright strand
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This image is from a set of mosaic images from NASA's Cassini spacecraft showing three fan-like structures in Saturn's tenuous F ring. Such fans suggest the existence of additional objects in the F ring.
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Fluorescent minerals emit visible light when exposed to ultraviolet light
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This image was acquired by NASA's Mars Reconnaissance Orbiter to complete a stereo pair over sinuous ridges in Argyre Planitia, but dust clouds kicked up, obscuring most of the surface.
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Encke's Moon
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Saturn's shadow sweeps across the rings in a view captured on Nov. 5, 2006 by NASA's Cassini spacecraft. In the bottom half of the image, the countless icy particles that make up the rings bask in full daylight. In the top half, they move through Saturn's shadow. On the right side of the image, the planet's night side, dimly lit by reflected ringshine, can be seen through gaps in the darkened rings. This view is a mosaic of four visible light images taken with Cassini's narrow-angle camera at a distance of approximately 932,000 miles (1.5 million kilometers) from Saturn. The Cassini spacecraft ended its mission on Sept. 15, 2017.
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P-29506BW Range 1.12 million kilometers (690,000 miles) This high-resolution image of the epsilon ring of Uranus is a clear-filter picture from Voyager's narrow-angle camera and has a resolution of about 10 km (6 mi). The epsilon ring, approx. 100 km (60 mi) wide at this location, clearly shows a structural variation. Visible here are a broad, bright outer component about 40 km (25 mi) wide; a darker, middle region of comparable width; and a narrow, bright inner strip about 15 km (9 mi) wide. The epsilon-ring structure seen by Voyager is similiar to that observed from the ground with stellar-occultation techniques. This frame represents the first Voyager image that resolves these features within the epsilon ring. The occasional fuzzy splotches on the outer and innerparts of the ring are artifacts left by the removal of reseau marks (used for making measurements on the image).
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Image Number: 6145-45118953Royalty FreeCredit Line:Piemags/PL Photography Limited/SuperStockCollection:PL Photography LimitedStory:Astrophysical Imaging and ExperimentationContributor:PiemagsModel Release:NoProperty Release:NoResolution:1400×788
Mars
Mars Reconnaissance Orbiter (MRO)|