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  2. List of Solar System objects - Wikipedia

    en.wikipedia.org/wiki/List_of_Solar_System_objects

    The following is a list of Solar System objects by orbit, ordered by increasing distance from the Sun. Most named objects in this list have a diameter of 500 km or more. The Sun, a spectral class G2V main-sequence star; The inner Solar System and the terrestrial planets. 2021 PH27; Mercury. Mercury-crossing minor planets; Venus. Venus-crossing ...

  3. Astronomical naming conventions - Wikipedia

    en.wikipedia.org/wiki/Astronomical_naming...

    In the early days, only a very limited number of features could be seen on other Solar System bodies other than the Moon. Craters on the Moon could be observed with even some of the earliest telescopes, and 19th-century telescopes could make out some features on Mars. Jupiter had its famous Great Red Spot, also visible through early telescopes.

  4. Template:Solar System table - Wikipedia

    en.wikipedia.org/wiki/Template:Solar_System_table

    Afrikaans; Alemannisch; Anarâškielâ; Ænglisc; العربية; Aragonés; অসমীয়া; Asturianu; Avañe'ẽ; Azərbaycanca; Banjar; 閩南語 / Bân ...

  5. Category:Solar System templates - Wikipedia

    en.wikipedia.org/wiki/Category:Solar_System...

    [[Category:Solar System templates]] to the <includeonly> section at the bottom of that page. Otherwise, add <noinclude>[[Category:Solar System templates]]</noinclude> to the end of the template code, making sure it starts on the same line as the code's last character.

  6. List of Solar System objects by size - Wikipedia

    en.wikipedia.org/wiki/List_of_Solar_System...

    Parts-per-million chart of the relative mass distribution of the Solar System, each cubelet denoting 2 × 10 24 kg. This article includes a list of the most massive known objects of the Solar System and partial lists of smaller objects by observed mean radius. These lists can be sorted according to an object's radius and mass and, for the most ...

  7. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    The Solar System remains in a relatively stable, slowly evolving state by following isolated, gravitationally bound orbits around the Sun. [28] Although the Solar System has been fairly stable for billions of years, it is technically chaotic, and may eventually be disrupted. There is a small chance that another star will pass through the Solar ...