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  2. Astronomy on Mars - Wikipedia

    en.wikipedia.org/wiki/Astronomy_on_Mars

    Phobos orbits so fast (with a period of just under one third of a sol) that it rises in the west and sets in the east, and does so twice per sol; Deimos on the other hand rises in the east and sets in the west, but orbits only a few hours slower than a Martian sol, so it spends about two and a half sols above the horizon at a time.

  3. Orbit of Mars - Wikipedia

    en.wikipedia.org/wiki/Orbit_of_Mars

    Mars comes closer to Earth more than any other planet save Venus at its nearest—56 million km is the closest distance between Mars and Earth, whereas the closest Venus comes to Earth is 40 million km. Mars comes closest to Earth every other year, around the time of its opposition, when Earth is sweeping between the Sun and Mars. Extra-close ...

  4. List of quadrangles on Mars - Wikipedia

    en.wikipedia.org/wiki/List_of_quadrangles_on_Mars

    The maps below were produced by the Mars Global Surveyor ' s Mars Orbiter Laser Altimeter; redder colors indicate higher elevations.The maps of the equatorial quadrangles use a Mercator projection, while those of the mid-latitude quadrangles use a Lambert conformal conic projection, and the maps of the polar quadrangles use a polar stereographic projection.

  5. Areography - Wikipedia

    en.wikipedia.org/wiki/Areography

    Mars has two permanent polar ice caps, the northern one located at Planum Boreum and the southern one at Planum Australe. The difference between Mars's highest and lowest points is nearly 30 km (from the top of Olympus Mons at an altitude of 21.2 km to Badwater Crater [1] at the bottom of the Hellas impact basin at an altitude of 8.2 km below ...

  6. Areostationary orbit - Wikipedia

    en.wikipedia.org/wiki/Areostationary_orbit

    Several factors make placing a spacecraft into an areostationary orbit more difficult than a geostationary orbit. Since the areostationary orbit lies between Mars's two natural satellites, Phobos (semi-major axis: 9,376 km) and Deimos (semi-major axis: 23,463 km), any satellites in the orbit will suffer increased orbital station keeping costs due to unwanted orbital resonance effects.

  7. South (Martian crater) - Wikipedia

    en.wikipedia.org/wiki/South_(Martian_crater)

    South is an impact crater in the Mare Australe quadrangle of Mars, located at 76.9°S latitude and 21.9°E longitude. It measures 101.84 kilometres (63.28 mi) in diameter, and was named after British astronomer Sir James South (1785–1867).

  8. NASA's Mars Rover Mission to Bring Samples Home Is at Risk - AOL

    www.aol.com/news/nasas-mars-rover-mission-bring...

    An exploding budget and an unraveling schedule spell disappointment for NASA's mission to learn more about Mars's history.

  9. Candor Chasma - Wikipedia

    en.wikipedia.org/wiki/Candor_Chasma

    The climate of Mars may have been such in the past that water ran on its surface. It has been known for some time that Mars undergoes many large changes in its tilt or obliquity because its two small moons lack the gravity to stabilize it, as the Moon stabilizes Earth; at times the tilt of Mars has even been greater than 80 degrees [ 3 ] [ 4 ]