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  2. List of Solar System objects by size - Wikipedia

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

    The size of solid bodies does not include an object's atmosphere. For example, Titan looks bigger than Ganymede, but its solid body is smaller. For the giant planets , the "radius" is defined as the distance from the center at which the atmosphere reaches 1 bar of atmospheric pressure.

  3. Astronomical object - Wikipedia

    en.wikipedia.org/wiki/Astronomical_object

    Each star follows an evolutionary track across this diagram. If this track takes the star through a region containing an intrinsic variable type, then its physical properties can cause it to become a variable star. An example of this is the instability strip, a region of the H-R diagram that includes Delta Scuti, RR Lyrae and Cepheid variables. [7]

  4. Fossorial - Wikipedia

    en.wikipedia.org/wiki/Fossorial

    A fossorial animal (from Latin fossor 'digger') is one that is adapted to digging and which lives primarily (but not solely) underground. Examples of fossorial vertebrates are badgers , naked mole-rats , meerkats , armadillos , wombats , and mole salamanders . [ 1 ]

  5. File : Diameters of terrestrial bodies of the solar system ...

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

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  6. Wikipedia:Featured picture candidates/Size of planets and stars

    en.wikipedia.org/.../Size_of_planets_and_stars

    Original - An illustration of the comparative sizes of planets and stars. Starting with the planet Mercury at the top left we follow a growing sequence of planets and then a growing sequence of stars until we reach the second largest known star VV Cephei in the bottom right. Reason It's a mind-blowing sequence.

  7. File:Star-sizes.jpg - Wikipedia

    en.wikipedia.org/wiki/File:Star-sizes.jpg

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  8. Habitability of F-type main-sequence star systems - Wikipedia

    en.wikipedia.org/wiki/Habitability_of_F-type...

    Indeed, F0 stars (7,400 K, 1.6 M ☉︎, 1.7 R ☉︎, ~7 L ☉︎) are considered by many scientists as the hottest and most massive stars capable of supporting habitable planets. A planet orbiting an F-type star at the Earth boundary within the HZ would receive 2.5 (F9 star) to 7.1 (F0 star) times the UV that Earth gets from the sun. [1]

  9. Habitable zone - Wikipedia

    en.wikipedia.org/wiki/Habitable_zone

    Of these, Kepler-186f is closest in size to Earth with 1.2 times Earth's radius, and it is located towards the outer edge of the habitable zone around its red dwarf star. Among nearest terrestrial exoplanet candidates, Tau Ceti e is 11.9 light-years away. It is in the inner edge of its planetary system's habitable zone, giving it an estimated ...

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