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  2. List of potentially habitable exoplanets - Wikipedia

    en.wikipedia.org/wiki/List_of_potentially...

    KOI-1686.01 was also considered a potentially habitable exoplanet after its detection in 2011, until proven a false positive by NASA in 2015. [ 72] Several other KOIs, like Kepler-577b and Kepler-1649b, were considered potentially habitable prior to confirmation, but with new data are no longer considered habitable.

  3. List of Solar System objects by size - Wikipedia

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

    Relative masses of the Solar planets. Jupiter at 71% of the total and Saturn at 21% dominate the system. Relative masses of the solid bodies of the Solar System. Earth at 48% and Venus at 39% dominate. Bodies less massive than Pluto are not visible at this scale. Relative masses of the rounded moons of the Solar System.

  4. List of exoplanets discovered by the Kepler space telescope

    en.wikipedia.org/wiki/List_of_exoplanets...

    On February 26, 2014, NASA announced the discovery of 715 newly verified exoplanets around 305 stars by the Kepler Space Telescope. The exoplanets were found using a statistical technique called "verification by multiplicity". 95% of the discovered exoplanets were smaller than Neptune and four, including Kepler-296f, were less than 2 1/2 the ...

  5. Habitable zone - Wikipedia

    en.wikipedia.org/wiki/Habitable_zone

    The planet has 6.9 Earth masses and 1.8–2.4 Earth radii, and with its close orbit receives 40 percent more stellar radiation than Earth, leading to surface temperatures of about 60° C. HD 40307 g, a candidate planet tentatively discovered in November 2012, is in the circumstellar habitable zone of HD 40307.

  6. Planetary habitability - Wikipedia

    en.wikipedia.org/wiki/Planetary_habitability

    Planetary habitability is the measure of a planet 's or a natural satellite 's potential to develop and maintain environments hospitable to life. [1] Life may be generated directly on a planet or satellite endogenously or be transferred to it from another body, through a hypothetical process known as panspermia. [2]

  7. Venus - Wikipedia

    en.wikipedia.org/wiki/Venus

    The predicted values for the moment of inertia based on planetary models suggest a core radius of 2,900–3,450 km. [73] This is in line with the first observation-based estimate of 3,500 km. [75] The principal difference between the two planets is the lack of evidence for plate tectonics on Venus, possibly because its crust is too strong to ...

  8. List of gravitationally rounded objects of the Solar System

    en.wikipedia.org/wiki/List_of_gravitationally...

    Vesta (radius 262.7 ± 0.1 km), the second-largest asteroid, appears to have a differentiated interior and therefore likely was once a dwarf planet, but it is no longer very round today. [74] Pallas (radius 255.5 ± 2 km ), the third-largest asteroid, appears never to have completed differentiation and likewise has an irregular shape.

  9. List of exoplanet extremes - Wikipedia

    en.wikipedia.org/wiki/List_of_exoplanet_extremes

    The stars R126 and R66 in the Large Magellanic Cloud have radius of 78 R ☉ and 131 R ☉ [81] and have dust discs but no planets have been detected yet. Smallest stellar radius (main sequence star) TRAPPIST-1 planets TRAPPIST-1: 0.1192 ± 0.0013 R ☉ [82] VB 10 (0.102 R ☉) [83] has a disproven planet candidate. Smallest stellar radius ...