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  2. File:Solar System planets, dual scale.jpg - Wikipedia

    en.wikipedia.org/wiki/File:Solar_System_planets...

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  3. List of directly imaged exoplanets - Wikipedia

    en.wikipedia.org/wiki/List_of_directly_imaged_e...

    Motion interpolation of seven images of the HR 8799 system taken from the W. M. Keck Observatory over seven years, featuring four exoplanets. This is a list of extrasolar planets that have been directly observed, sorted by observed separations. This method works best for young planets that emit infrared light and are far from the glare of the star.

  4. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    Solar system diagram by Emanuel Bowen in 1747, when neither Uranus, Neptune, nor the asteroid belts had yet been discovered. Orbits of planets are to scale, but the orbits of moons and the sizes of bodies are not. The term "Solar System" entered the English language by 1704, when John Locke used it to refer to the Sun, planets, and comets. [290]

  5. Not that I think an image lacking those objects would be better. I think the only reasonable solution would be to create an image of the Solar System that includes all known planets and dwarf planets, with the dwarf planets not on the ecliptic, and some representive sample of moons, undiscovered Kuiper belt objects, and comets.--

  6. File:Solar system.jpg - Wikipedia

    en.wikipedia.org/wiki/File:Solar_system.jpg

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  7. Family Portrait (MESSENGER) - Wikipedia

    en.wikipedia.org/wiki/Family_Portrait_(MESSENGER)

    The Solar System Family Portrait is an image of many of the Solar System's planets and moons acquired by MESSENGER during November 2010 from approximately the orbit of Mercury. The mosaic is intended to be complementary to the Voyager 1 ' s Family Portrait acquired from the outer edge of the Solar System on February 14, 1990. [1]

  8. Jupiter is the biggest planet in our solar system, according to NASA. Jupiter’s radius is over 11 times the equatorial radius of the Earth.

  9. Protoplanetary disk - Wikipedia

    en.wikipedia.org/wiki/Protoplanetary_disk

    [18] [19] The formation of planets and moons in geometrically thin, gas- and dust-rich disks is the reason why the planets are arranged in an ecliptic plane. Tens of millions of years after the formation of the Solar System, the inner few AU of the Solar System likely contained dozens of moon- to Mars-sized bodies that were accreting and ...