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  2. Frost line (astrophysics) - Wikipedia

    en.wikipedia.org/wiki/Frost_line_(astrophysics)

    In astronomy or planetary science, the frost line, also known as the snow line or ice line, is the minimum distance from the central protostar of a solar nebula where the temperature is low enough for volatile compounds such as water, ammonia, methane, carbon dioxide and carbon monoxide to condense into solid grains, which will allow their accretion into planetesimals.

  3. Asteroidal water - Wikipedia

    en.wikipedia.org/wiki/Asteroidal_water

    The "snow line" of the Solar System lies outside of the main asteroid belt, and the majority of water is expected in minor planets (e.g. Kuiper belt objects (KBOs) and Centaurs). Nevertheless, a significant amount of water is also found inside the snow line, including in near-earth objects (NEOs).

  4. List of Solar System objects most distant from the Sun

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

    One particularly distant body is 90377 Sedna, which was discovered in November 2003.It has an extremely eccentric orbit that takes it to an aphelion of 937 AU. [2] It takes over 10,000 years to orbit, and during the next 50 years it will slowly move closer to the Sun as it comes to perihelion at a distance of 76 AU from the Sun. [3] Sedna is the largest known sednoid, a class of objects that ...

  5. Solar System belts - Wikipedia

    en.wikipedia.org/wiki/Solar_System_belts

    [6] [7] The Grand tack hypothesis is a model of the unique placement of the giant planets and the Solar System belts. [3] [4] [8] Most giant planets found outside our Solar System, exoplanets, are inside the snow line, and are called Hot Jupiters. [5] [9] Thus in normal planetary systems giant planets form beyond snow line and then migrated ...

  6. V883 Orionis - Wikipedia

    en.wikipedia.org/wiki/V883_Orionis

    V883 Orionis is a protostar in the constellation of Orion.It is associated with IC 430 (Haro 13A), a peculiar Hα object surveyed by Guillermo Haro in 1952. [4] It is assumed to be a member of the Orion Nebula cluster at 414 ± 7 pc.

  7. Dust astronomy - Wikipedia

    en.wikipedia.org/wiki/Dust_astronomy

    Dust astronomy is a subfield of astronomy that uses the information contained in individual cosmic dust particles ranging from their dynamical state to its isotopic, elemental, molecular, and mineralogical composition in order to obtain information on the astronomical objects occurring in outer space.

  8. Five planets will line up in the skies above WA state. Here’s ...

    www.aol.com/news/five-planets-line-skies-above...

    The planets of the solar system all move around the same orbital plane, according to National Geographic, so when several planets are on the same side of the sun as Earth, it looks as if they’re ...

  9. LHS 3844 b - Wikipedia

    en.wikipedia.org/wiki/LHS_3844_b

    In order to explain the lack of atmosphere, it has been proposed that the planet was formed interior to the star system's snow-line, because if it formed beyond the snow-line it would have carried volatiles, on the surface and in a thick atmosphere, that according to models on atmospheric loss should have been enough to sustain an atmosphere to ...