Magellan - Balch crater mgn c130n279 1
Författare/Upphovsman:
Magellan Team (NASA - Jet Propulsion Laboratory)
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Källa:
Upplösning:
800 x 800 Pixel (797100 Bytes)
Beskrivning:
Magellan radar image of Balch Crater, Venus, originally designated Somerville Crater. This crater is one of the few examples of tectonically modified craters seen on Venus. The absence of such craters indicates a possible cessation of tectonic deformation on Venus at some point in history. Balch is located at 30° N, 283° W in Devana Chasma, Central Beta Regio. The crater was originally 37 kilometres in diameter. North is up. (Magellan C1-MIDR 30N279;1,framelet 30)
Location & Time Information Date/Time (UT): N/A Distance/Range (km): 479.4 Central Latitude/Longitude (deg): +29.95/279.43 Orbit(s): 1859-1969 Imaging Information Area or Feature Type: Crater, Rift Instrument: Synthetic Aperture Radar Instrument Resolution (pixels): 240 x 240, 8 bit Instrument Field of View (deg): 2.1 x 2.5 Filter: N/A Illumination Incidence Angle (deg): 39.1-44.4 Phase Angle (deg): 0 Instrument Look Direction: Left Surface Emission Angle (deg): 39.1-44.4 Ordering Information CD-ROM Volume: MG_0043 NASA Image ID number: C1-30N279;1 Other Image ID number: P-38741 NSSDC Data Set ID (Photo): 89-033B-01O NSSDC Data Set ID (CD): 89-033B-01C Other ID: N/A
Licens:
Public domain
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