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Solar eclipses on Mars

From Wikipedia, the free encyclopedia

Annular eclipse of the Sun by Phobos (Curiosity, August 20, 2013)
Annular eclipse of the Sun by Phobos (Curiosity, August 20, 2013)
Eclipse of the Sun by Phobos, the larger of the two moons of Mars, in real time (Curiosity, August 20, 2013)

The two moons of Mars, Phobos and Deimos, are much smaller than the Moon, greatly reducing the frequency of solar eclipses on that planet.[1][2] Neither moon's apparent diameter is large enough to cover the disk of the sun, and therefore they are annular solar eclipses and can also be considered transits.

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Eclipses caused by Phobos

Transit of Phobos (Opportunity, March 2004)
Transit of Phobos (Opportunity, March 2004)

Due to the small size of Phobos (about 20 by 25 km (12 by 16 mi)) and its rapid orbital motion, an observer on the surface of Mars would never experience a solar eclipse for longer than about thirty seconds. Phobos also takes only 7 hours 39 minutes to orbit Mars, while a Martian day is 24 hours 37 minutes long, meaning that Phobos can create two eclipses per Martian day. These are annular eclipses, because Phobos is not quite large enough or close enough to Mars to create a total solar eclipse.

Transits caused by Deimos

Deimos is too small (about 15 by 10 km (9.3 by 6.2 mi)) and too far from Mars to cause an eclipse. The best an observer on Mars would see is a small spot crossing the Sun's disc.

View from Earth

Both moons are too small to cast a shadow on Mars that can be seen from Earth. However, shortly after the first artificial satellites were placed in orbit around Mars, the shadow of Phobos was seen in pictures transmitted to Earth. One of these photos was from the NASA rover Opportunity.


  1. ^ "See a solar eclipse from Mars". NBC News. 10 March 2004. Retrieved 22 August 2017.
  2. ^ "JPL News --  NASA Rovers Watching Solar Eclipses by Mars Moons". Retrieved 22 August 2017.

External links

This page was last edited on 17 November 2019, at 04:47
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