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  2. Claimed moons of Earth - Wikipedia

    en.wikipedia.org/wiki/Claimed_moons_of_Earth

    This asteroid's orbit keeps it near the Earth, but not orbiting it in the usual sense. When analyzing its orbit from the perspective of different bodies, the presumed quasi-satellite does seem to have a more stable location near the Earth The orbit of 2020 CD 3 around the Earth. The white band is the orbit of the Moon.

  3. CoRoT-7b - Wikipedia

    en.wikipedia.org/wiki/CoRoT-7b

    The CoRoT team then published a second paper on CoRoT-7b's mass, [12] removing stellar activity through analysis only of radial velocity data for which multiple measurements were taken in a given night. The planet is weighed at 7.42 Earth masses, yielding an average density of 10.4 ± 1.8 g cm −3, far higher than the Earth's and similar to ...

  4. Rings of Earth - Wikipedia

    en.wikipedia.org/wiki/Rings_of_Earth

    The ring was first formally proposed after 21 impact craters from the meteor event were found to be located along a straight band around the Earth's equator. [10] [11] Andrew G. Tomkins, [9] Erin L. Martin [9] and Peter A. Cawood, [9] working with Monash University, released a study in September 2024 that gave evidence on the existence of the ...

  5. Ring system - Wikipedia

    en.wikipedia.org/wiki/Ring_system

    Some planetary rings are influenced by shepherd moons, small moons that orbit near the inner or outer edges of a ringlet or within gaps in the rings. The gravity of shepherd moons serves to maintain a sharply defined edge to the ring; material that drifts closer to the shepherd moon's orbit is either deflected back into the body of the ring ...

  6. List of natural satellites - Wikipedia

    en.wikipedia.org/wiki/List_of_natural_satellites

    Moons are classed into two separate categories according to their orbits: regular moons, which have prograde orbits (they orbit in the direction of their planets' rotation) and lie close to the plane of their equators, and irregular moons, whose orbits can be pro- or retrograde (against the direction of their planets' rotation) and often lie at ...

  7. List of objects at Lagrange points - Wikipedia

    en.wikipedia.org/wiki/List_of_objects_at...

    International Cometary Explorer, formerly the International Sun–Earth Explorer 3 (ISEE-3), diverted out of L 1 in 1983 for a comet rendezvous mission. Currently in heliocentric orbit . The Sun–Earth L 1 is also the point to which the Reboot ISEE-3 mission was attempting to return the craft as the first phase of a recovery mission (as of ...

  8. Satellite system (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Satellite_system_(astronomy)

    Gravitational accelerations at L 4. The Hill sphere is the region in which an astronomical body dominates the attraction of satellites. Of the Solar System planets, Neptune and Uranus have the largest Hill spheres, due to the lessened gravitational influence of the Sun at their far orbits, however all of the giant planets have Hill spheres in the vicinity of 100 million kilometres in radius.

  9. Natural satellite - Wikipedia

    en.wikipedia.org/wiki/Natural_satellite

    A planet usually has at least around 10,000 times the mass of any natural satellites that orbit it, with a correspondingly much larger diameter. [3] The Earth–Moon system is a unique exception in the Solar System; at 3,474 kilometres (2,158 miles) across, the Moon is 0.273 times the diameter of Earth and about 1 ⁄ 80 of its mass. [4]

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