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  2. Habitability of red dwarf systems - Wikipedia

    en.wikipedia.org/wiki/Habitability_of_red_dwarf...

    As red dwarf stars have an extended pre-main sequence phase, their eventual habitable zones would be for around 1 billion years in a zone where water was not liquid but rather in a gaseous state. Thus, terrestrial planets in the actual habitable zones, if provided with abundant surface water in their formation, would have been subject to a ...

  3. Habitable zone for complex life - Wikipedia

    en.wikipedia.org/wiki/Habitable_Zone_for_Complex...

    Dwarf stars (red dwarf/orange dwarf/brown dwarf/subdwarf) are not only unstable, but also emit low energy, so the habitable zone is very close to the star and planets become tidally locked on the timescales needed for the development of life. [17]

  4. LHS 1140 b - Wikipedia

    en.wikipedia.org/wiki/LHS_1140_b

    LHS 1140 b is an exoplanet orbiting within the conservative habitable zone of the red dwarf LHS 1140.Discovered in 2017 by the MEarth Project, [1] LHS 1140 b is about 5.6 times the mass of Earth and about 70% larger in radius, putting it within the super-Earth category of planets.

  5. Planetary habitability - Wikipedia

    en.wikipedia.org/wiki/Planetary_habitability

    Furthermore, this total amount of habitable zone will last longer, because red dwarf stars live for hundreds of billions of years or even longer on the main sequence. [98] However, combined with the above disadvantages, it is more likely that red dwarf stars would remain habitable longer to microbes, while the shorter-lived yellow dwarf stars ...

  6. Habitable zone - Wikipedia

    en.wikipedia.org/wiki/Habitable_zone

    K2-18b is an exoplanet 124 light-years away, orbiting in the habitable zone of the K2-18, a red dwarf. This planet is significant for water vapor found in its atmosphere; this was announced on September 17, 2019.

  7. Habitability of natural satellites - Wikipedia

    en.wikipedia.org/wiki/Habitability_of_natural...

    This is especially true of red dwarf systems, where comparatively high gravitational forces and low luminosities leave the habitable zone in an area where tidal locking would occur. If tidally locked, one rotation about the axis may take a long time relative to a planet (for example, ignoring the slight axial tilt of Earth's Moon and ...

  8. Planet in ‘habitable’ zone could have rare oceans and a ...

    www.aol.com/news/planet-habitable-zone-could...

    The James Webb Space Telescope investigated a giant planet, K2-18b, that could be an ocean world, according to NASA. The exoplanet lies 120 light-years away from Earth.

  9. Gliese 876 b - Wikipedia

    en.wikipedia.org/wiki/Gliese_876_b

    Gliese 876 b currently lies beyond the outer edge of the habitable zone but because Gliese 876 is a slowly evolving main-sequence red dwarf its habitable zone is very slowly moving outwards and will continue to do so for trillions of years.