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  2. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    If the Sun–Neptune distance is scaled to 100 metres (330 ft), then the Sun would be about 3 cm (1.2 in) in diameter (roughly two-thirds the diameter of a golf ball), the giant planets would be all smaller than about 3 mm (0.12 in), and Earth's diameter along with that of the other terrestrial planets would be smaller than a flea (0.3 mm or 0. ...

  3. Extraterrestrial life - Wikipedia

    en.wikipedia.org/wiki/Extraterrestrial_life

    It is estimated that at least ten percent of all Sun-like stars have a system of planets, [40] i.e. there are 6.25 × 10 18 stars with planets orbiting them in the observable universe. Even if it is assumed that only one out of a billion of these stars has planets supporting life, there would be some 6.25 billion life-supporting planetary ...

  4. Superhabitable world - Wikipedia

    en.wikipedia.org/wiki/Superhabitable_world

    A superhabitable world is a hypothetical type of planet or moon that is better suited than Earth for the emergence and evolution of life. The concept was introduced in a 2014 paper by René Heller and John Armstrong, in which they criticized the language used in the search for habitable exoplanets and proposed clarifications. [ 2 ]

  5. Non-planetary abiogenesis - Wikipedia

    en.wikipedia.org/wiki/Non-planetary_abiogenesis

    The ability of information carriers to self-replicate faster than they disintegrate; The presence of free energy needed to constantly create order out of the disorder (i.e., to combat entropy) via self-replication; The authors proceed to argue that inside Sun-like stars objects that satisfy the above conditions can exist.

  6. Planets like Earth facing threat from stars blasting intense ...

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  7. List of unsolved problems in astronomy - Wikipedia

    en.wikipedia.org/wiki/List_of_unsolved_problems...

    A sample of 229 nearby "thick" disk stars has been used to investigate the existence of an age-metallicity relation in the Galactic thick disk and indicates that there is an age-metallicity relation present in the thick disk. [13] [14] Stellar ages from asteroseismology confirm the lack of any strong age-metallicity relation in the Galactic ...

  8. History of Solar System formation and evolution hypotheses

    en.wikipedia.org/wiki/History_of_Solar_System...

    Today, comets are known to be far too small to have created the Solar System in this way. [8] In 1755, Immanuel Kant speculated that observed nebulae could be regions of star and planet formation. In 1796, Laplace elaborated by arguing that the nebula collapsed into a star, and, as it did so, the remaining material gradually spun outward into a ...

  9. Planet-hosting star - Wikipedia

    en.wikipedia.org/wiki/Planet-hosting_star

    The authors of this study conclude that "stars are orbited by planets as a rule, rather than the exception". [2] In November 2013, it was announced that 22±8% of Sun-like [a] stars have an Earth-sized [b] planet in the habitable [c] zone. [9] [10] Regardless of the proportion of stars with planets, the total number of exoplanets must be very ...