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  2. Transit of Phobos from Mars - Wikipedia

    en.wikipedia.org/wiki/Transit_of_Phobos_from_Mars

    During a transit, Phobos can be seen from Mars as a large black disc rapidly moving across the face of the Sun. At the same time, the shadow ( antumbra ) of Phobos moves across the Martian surface. The event could also be regarded as a particularly quick and shallow annular solar eclipse by Phobos.

  3. Solar eclipses on Mars - Wikipedia

    en.wikipedia.org/wiki/Solar_eclipses_on_Mars

    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. The highest resolution, highest frame rate video of a ...

  4. List of films featuring eclipses - Wikipedia

    en.wikipedia.org/wiki/List_of_films_featuring...

    The Eclipse, or the Courtship of the Sun and Moon: 1907: The French silent film shows a solar eclipse resulting from a consummation between the Sun and the Moon. [5] [6] [2] [8] [4] Fantasia: 1940: In one of the segments of the American animated film, a solar eclipse takes place after dinosaurs go extinct, and the landscape is changed into a ...

  5. Transit of Deimos from Mars - Wikipedia

    en.wikipedia.org/wiki/Transit_of_Deimos_from_Mars

    A transit of Deimos across the Sun as seen from Mars occurs when Deimos passes directly between the Sun and a point on the surface of Mars, obscuring a small part of the Sun's disc for an observer on Mars. During a transit, Deimos can be seen from Mars as a small dark spot rapidly moving across the Sun's face. [1] [2]

  6. Phobos (moon) - Wikipedia

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

    Phobos is named after the Greek god of fear and panic, who is the son of Ares (Mars) and twin brother of Deimos. Phobos is a small, irregularly shaped object with a mean radius of 11 km (7 mi). It orbits 6,000 km (3,700 mi) from the Martian surface, closer to its primary body than any other known natural satellite to a planet.

  7. Eclipse - Wikipedia

    en.wikipedia.org/wiki/Eclipse

    This is an accepted version of this page This is the latest accepted revision, reviewed on 12 November 2024. Astronomical event where one body is hidden by another For other uses, see Eclipse (disambiguation). "Total eclipse" redirects here. For other uses, see Total eclipse (disambiguation). Totality during the 1999 solar eclipse. Solar prominences can be seen along the limb (in red) as well ...

  8. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    Thus, the Sun occupies 0.00001% (1 part in 10 7) of the volume of a sphere with a radius the size of Earth's orbit, whereas Earth's volume is roughly 1 millionth (10 −6) that of the Sun. Jupiter, the largest planet, is 5.2 AU from the Sun and has a radius of 71,000 km (0.00047 AU; 44,000 mi), whereas the most distant planet, Neptune, is 30 AU ...

  9. Solar eclipse - Wikipedia

    en.wikipedia.org/wiki/Solar_eclipse

    A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby obscuring the view of the Sun from a small part of Earth, totally or partially.Such an alignment occurs approximately every six months, during the eclipse season in its new moon phase, when the Moon's orbital plane is closest to the plane of Earth's orbit. [1]