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  2. Moons of Mars - Wikipedia

    en.wikipedia.org/wiki/Moons_of_Mars

    [7] [34] Both moons have very circular orbits which lie almost exactly in Mars's equatorial plane, and hence a capture origin requires a mechanism for circularizing the initially highly eccentric orbit, and adjusting its inclination into the equatorial plane, most probably by a combination of atmospheric drag and tidal forces, [35] although it ...

  3. Phobos (moon) - Wikipedia

    en.wikipedia.org/wiki/Phobos_(moon)

    Phobos has been photographed in close-up by several spacecraft whose primary mission has been to photograph Mars. The first was Mariner 7 in 1969, followed by Mariner 9 in 1971, Viking 1 in 1977, Phobos 2 in 1989 [ 75 ] Mars Global Surveyor in 1998 and 2003, Mars Express in 2004, 2008, 2010 [ 76 ] and 2019, and Mars Reconnaissance Orbiter in ...

  4. Deimos (moon) - Wikipedia

    en.wikipedia.org/wiki/Deimos_(moon)

    Curiosity's view of the Mars moons: Phobos passing in front of Deimos in real-time (video-gif, 1 August 2013) As seen from Mars, Deimos would have an angular diameter of no more than 2.5 minutes (sixty minutes make one degree), one twelfth of the width of the Moon as seen from Earth, and would therefore appear almost star-like to the naked eye ...

  5. Mars’s moons don’t get much credit. But they’re small, lifeless, and weird little things. Here’s everything you should know about them.

  6. Orbit of Mars - Wikipedia

    en.wikipedia.org/wiki/Orbit_of_Mars

    Extra-close oppositions of Mars happen every 15 to 17 years, when we pass between Mars and the Sun around the time of its perihelion (closest point to the Sun in orbit). The minimum distance between Earth and Mars has been declining over the years, and in 2003 the minimum distance was 55.76 million km, nearer than any such encounter in almost ...

  7. List of natural satellites - Wikipedia

    en.wikipedia.org/wiki/List_of_natural_satellites

    Mercury, the smallest and innermost planet, has no moons, or at least none that can be detected to a diameter of 1.6 km (1.0 mi). [2] For a very short time in 1974, Mercury was thought to have a moon. Venus also has no moons, [3] though reports of a moon around Venus have circulated since the 17th century.

  8. Mars' 2 weird moons began as 1 large moon, study suggests - AOL

    www.aol.com/mars-2-weird-moons-began-235538365.html

    Mars may have had a single moon before something smashed into it, tearing it asunder into the two moons we see today. In a study published Monday in Nature, scientists explained how they used the ...

  9. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    [120] [121] Mars has a highly differentiated internal structure, and lost its magnetosphere 4 billion years ago. [122] [123] Mars has two tiny moons: [124] Phobos is Mars's inner moon. It is a small, irregularly shaped object with a mean radius of 11 km (7 mi). Its surface is very unreflective and dominated by impact craters.