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  2. Mercury (planet) - Wikipedia

    en.wikipedia.org/wiki/Mercury_(planet)

    The probe successfully entered an elliptical orbit around the planet on March 18, 2011. The first orbital image of Mercury was obtained on March 29, 2011. The probe finished a one-year mapping mission, [202] and then entered a one-year extended mission into 2013.

  3. Astronomy on Mercury - Wikipedia

    en.wikipedia.org/wiki/Astronomy_on_Mercury

    This is due to the high eccentricity of Mercury's orbit around the Sun. [1] A 19th century depiction of the apparent size of the Sun as seen from the Solar System's planets (incl. 72 Feronia and the then most outlying known asteroid, here called Maximiliana and now called 65 Cybele).

  4. Tests of general relativity - Wikipedia

    en.wikipedia.org/wiki/Tests_of_general_relativity

    Transit of Mercury on November 8, 2006 with sunspots #921, 922, and 923 The perihelion precession of Mercury. Under Newtonian physics, an object in an (isolated) two-body system, consisting of the object orbiting a spherical mass, would trace out an ellipse with the center of mass of the system at a focus of the ellipse.

  5. Spacecraft beams back riveting photos after buzzing Mercury’s ...

    www.aol.com/spacecraft-beams-back-riveting...

    The maneuver put the spacecraft on course to enter orbit around Mercury late next year. The spacecraft holds two orbiters, one for Europe and the other for Japan, that will circle the planet's poles.

  6. Johannes Kepler thought he sketched Mercury orbiting ... - AOL

    www.aol.com/johannes-kepler-1607-sketches...

    Kepler mistakenly believed he had captured Mercury moving in orbit across the sun in May 1607, but he later retracted his report 11 years later and determined he had observed a sunspot group.

  7. Apparent retrograde motion - Wikipedia

    en.wikipedia.org/wiki/Apparent_retrograde_motion

    Mercury's elliptical orbit is farther from circular than that of any other planet in the Solar System, resulting in a substantially higher orbital speed near perihelion. As a result, at specific points on Mercury's surface an observer would be able to see the Sun rise part way, then reverse and set before rising again, all within the same ...

  8. Outline of Mercury (planet) - Wikipedia

    en.wikipedia.org/wiki/Outline_of_Mercury_(planet)

    Mercury – smallest and innermost planet in the Solar System. Its orbital period (about 88 Earth days) is less than any other planet in the Solar System. Seen from Earth, it appears to move around its orbit in about 116 days. It has no known natural satellites. It is named after the Roman deity Mercury, the messenger to the gods.

  9. Transit of Mercury - Wikipedia

    en.wikipedia.org/wiki/Transit_of_Mercury

    The orbit of the planet Mercury lies interior to that of the Earth, and thus it can come into an inferior conjunction with the Sun. When Mercury is near the node of its orbit, it passes through the orbital plane of the Earth. If an inferior conjunction occurs as Mercury is passing through its orbital node, the planet can be seen to pass across ...