Mercator

Controlled Mosaic of Phobos clxxx° West 57° -1 Stickney 120° 90° 60° 30° 0° West 57° Mp 50K 0/90 COMT, 2008 General Notes In 1877 Asaph Hall, an astronomer at the United States Naval Observatory, discovered the Martian moons Phobos and Deimos. Phobos, the larger of the ii moons, is orbiting with a mean distance of 9375 km to the center of Mars, recently in the gravitational field of the planet [1]. Since 2003 the Mars distil spacecraft explores the Martian System with different instruments. The orbiter carries the pushbroom electronic scanner High- fortitude Stereo Camera (HRSC) and its added imagination subsystem Super Resolution Channel (SRC) [2].

As HRSC is a push-broom scanning instrument with club CCD line detectors mounted (5184 px) in parallel on a focal plane, its unique feature is the ability to obtain nearsimultaneous imaging data at high resolution, with along-track triple stereo, four colour in and five different phase angles, avoiding any time-dependent variations of the observing -160 0 one hundred fifty° C -8 l u s -1600 t r i l l -2000 G u l l i v e r D 0 - 80 -120 0 r u n i o 30° 0 400 00 0 28 0 20 0° S We n d e l l t i c k n e y T o d d Limtoc 2000 1600 Sharpless -30° K e p 120 0 l DArrest 400 0 e r D -400 -800 -1200 -1600 -2000 -57° 180° West one hundred fifty° 120° 90° 60° 30° Scale 1: 50 000 0 1 Resolution on Map Image advocate Map 180° West 57° 57° 6 cl° 120° 90° 13 12 60° 30° 0° West 57° 180° West 57° 150° 120° 90° 60° 30° 0° West m/px 31 25 > 100 26 30° 30° 11 30° 10 1 30° 40 - 100 23 - 40 17 - 23 18 17 5 0° 7 8 2 16 -30° 21 0° 0° 13 - 17 11 - 13 8 - 11 0° -30° -30° -30° 30 9 24 14 15 29 23 22 -57° 150° 120° 90° 60° 30° 0° West 6 -8 < 6 -57° 180° West 150° 120° 90° 60° 30° 0° West -57° -57° 180° West 1 2 3 5 6 7 8 9... If you want to get a full essay, articulate it on our website: Orderessay

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