Datoteka:Eastern Tharsis and Noctis Labyrinthus.png

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Original caption

Viking 1 Orbiter color mosaic of the eastern Tharsis region on Mars. At left, from top to bottom, are the three 25 km high volcanic shields, Ascraeus Mons, Pavonis Mons, and Arsia Mons. The shield at upper right is Tharsis Tholus. The canyon system at lower right is Noctis Labyrinthus, the westernmost extension of Valles Marineris. The smooth area at bottom center is Syria Planum. The distance between the calderas of Ascraeus and Pavonis Mons is 800 km. North is up. The images used to produce this mosaic were taken during orbit 1334 on 22 February 1980. (Viking 1 Orbiter MG01N104-334S0)

Location & Time Information

  • Date/Time (UT): 1980-02-22 T 11:00
  • Distance/Range (km): N/A
  • Central Latitude/Longitude (deg): +01.,104.
  • Orbit(s): 1,334

Imaging Information

  • Area or Feature Type: volcano, valley
  • Instrument: Visual Imaging Subsystem
  • Instrument Resolution (pixels): 1056 x 1182, 7 bit
  • Instrument Field of View (deg): 1.54 x 1.69
  • Filter: N/A
  • Illumination Incidence Angle (deg): N/A
  • Phase Angle (deg): N/A
  • Instrument Look Direction: N/A
  • Surface Emission Angle (deg): N/A

Source

This image or video was catalogued by Jet Propulsion Laboratory of the United States National Aeronautics and Space Administration (NASA) under Photo ID: PIA02987.

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Licencija

Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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sadašnja15:49, 26. listopada 2005.Minijatura za inačicu od 15:49, 26. listopada 2005.1.024 × 1.024 (1,46 MB)Ævar Arnfjörð Bjarmason== Original caption== Viking 1 Orbiter color mosaic of the eastern Tharsis region on Mars. At left, from top to bottom, are the three 25 km high volcanic shields, Ascraeus Mons, Pavonis Mons, and Arsia Mons. The shield at upper right is Tharsis Tholus. Th

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