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Largest available format 2860 × 1957 px 0 MB
Dimension [pixels] Dimension in 300dpi [mm] File size [MB] Online Purchase
Large 2860 × 1957 px 242 × 166 mm 191 KB
Medium 1024 × 701 px 87 × 59 mm 100 KB

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PIX4624886

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Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. The largest satellite, Titan, projects its shadow on the planet and three satellites are visible on the left: Mimas and its shadow are discernable on Titan's left, just above the rings, on its left, above the rings, Dione is clearly visible, and on the left, the Enceladus satellite. Several of Saturn's moons transiting the face of the gas giant planet. This is a rare event because the rings are tilted edge on to Earth every 15 years. This frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow are below, at left, slightly above the rings. To the far left off the disk, Dione, the brightest of the icy moons in this view - and Enceladus, fainter and farther to the left - can easily be seen just above the rings. This picture was taken with Hubble's Wide Field Planetary Camera 2 on February 24, 2009, when Saturn was at a distance of roughly 775 million miles (1.25 billion kilometers) from Earth. Hubble can see details as small as 190 miles (300 km) across on Saturn

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Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. The largest satellite, Titan, projects its shadow on the planet and three satellites are visible on the left: Mimas and its shadow are discernable on Titan's left, just above the rings, on its left, above the rings, Dione is clearly visible, and on the left, the Enceladus satellite. Several of Saturn's moons transiting the face of the gas giant planet. This is a rare event because the rings are tilted edge on to Earth every 15 years. This frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow are below, at left, slightly above the rings. To the far left off the disk, Dione, the brightest of the icy moons in this view - and Enceladus, fainter and farther to the left - can easily be seen just above the rings. This picture was taken with Hubble's Wide Field Planetary Camera 2 on February 24, 2009, when Saturn was at a distance of roughly 775 million miles (1.25 billion kilometers) from Earth. Hubble can see details as small as 190 miles (300 km) across on Saturn

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Photo © NASA/ESA/Hubble Heritage team/Novapix / Bridgeman Images

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Largest available format 2860 × 1957 px 0 MB
Dimension [pixels] Dimension in 300dpi [mm] File size [MB] Online Purchase
Large 2860 × 1957 px 242 × 166 mm 191 KB
Medium 1024 × 701 px 87 × 59 mm 100 KB

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