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  2. Quasi-satellite - Wikipedia

    en.wikipedia.org/wiki/Quasi-satellite

    A quasi-satellite's orbit around the Sun takes the same time as the planet's, but has a different eccentricity (usually greater), as shown in the diagram. When viewed from the perspective of the planet by an observer facing the Sun, the quasi-satellite will appear to travel in an oblong retrograde loop around the planet. (See Analemma § Of ...

  3. File:Quasi-satellite diagram.svg - Wikipedia

    en.wikipedia.org/wiki/File:Quasi-satellite...

    Quasi-satellite diagram.png; Cuasi-satélite (diagrama).png; Quasi-satellite diagramme.png; SVG development . The SVG code is . This diagram was created with a text ...

  4. List of natural satellites - Wikipedia

    en.wikipedia.org/wiki/List_of_natural_satellites

    (See Other moons of Earth and Quasi-satellite.) Mars has two known moons , Phobos and Deimos ("fear" and "dread", after attendants of Ares , the Greek god of war, equivalent to the Roman Mars). Searches for more satellites have been unsuccessful, putting the maximum radius of any other satellites at 90 m (100 yd).

  5. Co-orbital configuration - Wikipedia

    en.wikipedia.org/wiki/Co-orbital_configuration

    Low-eccentricity quasi-satellite orbits are highly unstable, but for moderate to high eccentricities such orbits can be stable. [2] From a co-rotating perspective the quasi-satellite appears to orbit the primary like a retrograde satellite , although at distances so large that it is not gravitationally bound to it. [ 2 ]

  6. Claimed moons of Earth - Wikipedia

    en.wikipedia.org/wiki/Claimed_moons_of_Earth

    The orbit of a satellite of Earth fundamentally depends on the gravity of the Earth–Moon system, whereas the orbit of a co-orbiting object would negligibly change if Earth and the Moon were suddenly removed because a quasi-satellite is orbiting the Sun on an Earth-like orbit in the vicinity of Earth.

  7. Quasi-Zenith Satellite System - Wikipedia

    en.wikipedia.org/wiki/Quasi-Zenith_Satellite_System

    Quasi-Zenith satellite orbit QZSS animation, the "Quasi-Zenith/tundra orbit" plot is clearly visible.The Quasi-Zenith Satellite System (QZSS) (Japanese: 準天頂衛星システム, Hepburn: juntenchō eisei shisutemu), also known as Michibiki (みちびき, "guidance"), is a four-satellite regional satellite navigation system and a satellite-based augmentation system developed by the Japanese ...

  8. 524522 Zoozve - Wikipedia

    en.wikipedia.org/wiki/524522_Zoozve

    524522 Zoozve (/ ˈ z uː z v eɪ / ⓘ; provisional designation 2002 VE 68) is a sub-kilometer sized asteroid and temporary quasi-satellite of Venus. [5] Discovered in 2002, it was the first such object to be discovered around a major planet in the Solar System.

  9. QZS-1R - Wikipedia

    en.wikipedia.org/wiki/QZS-1R

    QZS-1R replaced the QZS-1 (Michibiki-1) satellite launched in September 2010. QZS-1 had a design life of ten years. QZS-1 had a design life of ten years. As QZS-1 was an experimental satellite, it did not broadcast the MADOCA (Multi-GNSS Advanced Demonstration tool for Orbit and Clock Analysis) signal, which can be used for centimeter-order ...

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