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  2. Water on terrestrial planets of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Water_on_terrestrial...

    The current Venusian atmosphere has only ~200 mg/kg H 2 O(g) in its atmosphere and the pressure and temperature regime makes water unstable on its surface. Nevertheless, assuming that early Venus's H 2 O had a ratio between deuterium (heavy hydrogen, 2H) and hydrogen (1H) similar to Earth's Vienna Standard Mean Ocean Water of 1.6×10 −4, [7] the current D/H ratio in the Venusian atmosphere ...

  3. Extraterrestrial liquid water - Wikipedia

    en.wikipedia.org/wiki/Extraterrestrial_liquid_water

    Extraterrestrial liquid water is water in its liquid state that naturally occurs outside Earth.It is a subject of wide interest because it is recognized as one of the key prerequisites for life as we know it and is thus surmised to be essential for extraterrestrial life.

  4. Lists of planets - Wikipedia

    en.wikipedia.org/wiki/Lists_of_planets

    The best available theory of planet formation is the nebular hypothesis, which posits that an interstellar cloud collapses out of a nebula to create a young protostar orbited by a protoplanetary disk. There are eight planets within the Solar System; planets outside of the solar system are also known as exoplanets.

  5. List of planet types - Wikipedia

    en.wikipedia.org/wiki/List_of_planet_types

    A planet in the Solar System beyond the asteroid belt, and hence refers to the gas giants. Jupiter, Saturn, Uranus and Neptune Pulsar planet: A planet that orbits a pulsar or a rapidly rotating neutron star. PSR B1257+12 A, B and C: Rogue planet: Also known as an interstellar planet. A planet that is not bound to any star, stellar remnant or ...

  6. Another point for life on Mars: Signs of liquid water ... - AOL

    www.aol.com/another-point-life-mars-signs...

    Scientists discovered evidence of a reservoir of liquid water seven to 13 miles below the Martian surface, lingering in the pores of the planet's crust. They believe there's enough to cover the ...

  7. Planet - Wikipedia

    en.wikipedia.org/wiki/Planet

    The period of one revolution of a planet's orbit is known as its sidereal period or year. [62] A planet's year depends on its distance from its star; the farther a planet is from its star, the longer the distance it must travel and the slower its speed, since it is less affected by its star's gravity.

  8. List of extrasolar candidates for liquid water - Wikipedia

    en.wikipedia.org/wiki/List_of_extrasolar...

    Solid bodies condensing from the disk should have liquid water, if they are the right distance from the star, have solid surfaces and atmospheres. [11] Toliman: Star has some potential for a planet with liquid water if super dense planet with high gravity and atmospheric pressure is found orbiting it (none have to date). [12] GD 61

  9. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    Earth (0.98–1.02 AU) [D 6] is the only place in the universe where life and surface liquid water are known to exist. [102] Earth's atmosphere contains 78% nitrogen and 21% oxygen, which is the result of the presence of life. [103] [104] The planet has a complex climate and weather system, with conditions differing drastically between climate ...