Kepler-737b

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Kepler-737b
Discovery
Discovered by HARPS, Kepler space telescope
Discovery dateMay 10, 2016
Transit
Designations
KOI-947.01, KIC 9710326 b, Gaia DR2 2126820324123177472 b
Orbital characteristics
0.1422 AU
29.5992 days
Star Kepler-737
Physical characteristics
Mean radius
1.96 R🜨
Mass ~4.5 MEarth
Mean density
~3.3 g/cm3
Temperature 298 K (25 °C; 77 °F)

    Kepler-737b is a super-Earth exoplanet 669 light years away. [1] There is a chance it could be on the inner edge of the habitable zone. [2]

    Contents

    Physical properties

    Mass, radius and temperature

    Kepler-737b is an exoplanet with 1.96 R🜨 (0.175 RJ). Its mass is unknown, but is estimated at 4.5 MEarth based on a mass-radius relationship. [1] [3] [4] If the 4.5-earth mass estimate is correct, this gives the planet an approximate density of 3.3 times that of water, giving it the possibility of being a mini-Neptune or, more favorable to habitability, a water world. Due to its stellar flux 121% that of Venus, it may be a smaller version of GJ 1214b, a classic superpressured water world. The planet's equilibrium temperature is 298 K (25 °C).

    Star

    The star's designations include Kepler-737 and KOI-947. [2] It is an early M-star. The mass is 0.51 solar masses and its radius is 0.48 times that of the Sun. [2] [5] The temperature of the star is 3813 K and its metallicity is -0.24, significantly lower than the Sun's. [2] The host star's age is 3.89 billion years, 680 million years younger than the Sun. [6]

    Orbit

    Kepler-737b orbits its star once every 28.5992 days. [2] It may be within the inner part of the habitable zone, depending on the habitable zone model used. The conservative model/models place it over 1 Earth flux level outside of the habitable zone, but some very optimistic models place it inside the far inner section of the extended habitable zone. If it is not a mini-Neptune, then it might have a small chance of being habitable. It would be substantially hotter than Earth, due to its stellar flux 2.297 times that of Earth, [3] greater than that of Venus, [7] and resulting equilibrium temperature of 298 K (25 °C; 77 °F). [1]

    Discovery

    Kepler-737b is a confirmed exoplanet that was found by Kepler using the transit method. [2] It was confirmed on May 10, [2] 2016. [1]

    Nomenclature

    Kepler-737b is also known as KOI-947.01, KIC 9710326 b, and Gaia DR2 2126820324123177472 b. [2] KOI means "Kepler Object of Interest" and KIC means "Kepler Input Catalog". Gaia is a Europe an satellite that was launched on December 19, 2013. [8]

    Habitability

    With a stellar flux 2.297 times that of Earth, [3] greater than that of Venus, [7] Kepler-737b is unlikely to be habitable. However, Kepler-737b is considered to be in the habitable zone by the Open Exoplanet Catalogue, [2] based on an extremely optimistic habitable zone model that also places Venus in the habitable zone. [9] Due to its equilibrium temp. of 298 K, with and earth-like GE it would be about sixty degrees Celsius, and with twice its GE, ninety degrees. It is likely tidally locked due to its short orbit; a tidally locked planet would have one side facing the star permanently while the other would be in constant darkness. [10] If Kepler-737b has little or no atmosphere, this could make one side too hot to live on, and the other too cold. However, there may be a "sweet spot" in between the two, where liquid water can exist. This spot would be the planet's terminator line. Kepler-737b may instead have atmospheric circulation that would distribute the heat around the planet, potentially making a large portion of it habitable, [11] although given its stellar flux the most likely scenario is that the planet's surface is too hot to be habitable. Water on Kepler-737b's surface could also distribute heat. [12]

    Kepler-737b's density is unknown, so it could either be a rocky super-Earth or a mini-Neptune. The fact that the planet is quite likely to have no magnetic field[ citation needed ] could spark adaptations to the relatively high radiation level, such as a thick shell of a substance that could repel the radiation or tardigrade-like DNA. In most earthly creatures, DNA is damaged permanently, but with tardigrades, DNA is repairable after being damaged by deadly radiation. [13]

    There is a reduced chance of intelligent life on Kepler-737b due to the fair chance that it is a water world, with no dry land.[ citation needed ] It is likely substantially hotter than Earth, due to its stellar flux 2.297 times that of Earth [3] and resulting equilibrium temperature of 298 K (25 °C; 77 °F). [14] If ice caps exist, then they would likely be much smaller than Earth's, due to the temperature as well as to the possibility that Kepler-737b has more carbon dioxide in its atmosphere than Earth. [lower-alpha 1] It would have accreted the carbon dioxide by gravity or because water worlds are likely to have a lot of carbon dioxide in their atmospheres.[ citation needed ] More carbon dioxide in an atmosphere equalizes the temperature.

    See also

    Notes

    1. ↑ Does not include all possible factors.

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    References

    1. 1 2 3 4 "Exoplanet-catalog – Exoplanet Exploration: Planets Beyond our Solar System Kepler-737 b".
    2. 1 2 3 4 5 6 7 8 9 "Open Exoplanet Catalogue - Kepler-737 b". www.openexoplanetcatalogue.com. Retrieved May 11, 2021.
    3. 1 2 3 4 "Planetary Systems Composite Data". NASA Exoplanet Archive . Retrieved January 16, 2022.
    4. ↑ "About the Planetary Systems Composite Parameters Table". NASA Exoplanet Archive . Retrieved January 16, 2022. If the Planetary Systems table does not have a value for the planetary radius, mass or density or a stellar luminosity, these values are calculated. See How the Archive Calculates Values in the Planetary Systems Composite Parameters Table for a detailed explanation.
    5. ↑ "Kepler 737 Star Facts (Type, Distance, Colour, Radius, Location, Exoplanets & more)". www.universeguide.com. April 27, 2019. Retrieved February 20, 2022.
    6. ↑ "The Extrasolar Planet Encyclopaedia — Kepler-737 b". Extrasolar Planets Encyclopaedia . Retrieved May 11, 2021.
    7. 1 2 HEC HZ hpcf.upr.edu
    8. ↑ "Gaia | Description & Facts". Encyclopedia Britannica. Retrieved May 24, 2021.
    9. ↑ "Open Exoplanet Catalogue - Venus". www.openexoplanetcatalogue.com. Retrieved January 16, 2022.
    10. ↑ "Tidally locked exoplanets may be more common than previously thought". UW News. Retrieved May 18, 2021.
    11. ↑ Hammond, Mark; Lewis, Neil T. (March 30, 2021). "The rotational and divergent components of atmospheric circulation on tidally locked planets". Proceedings of the National Academy of Sciences. 118 (13): e2022705118. arXiv: 2102.11760 . Bibcode:2021PNAS..11822705H. doi: 10.1073/pnas.2022705118 . ISSN   0027-8424. PMC   8020661 . PMID   33753500.
    12. ↑ Sutter, Paul (March 8, 2021). "Can super-rotating oceans cool off extreme exoplanets?". Space.com. Retrieved May 18, 2021.
    13. ↑ "Are tardigrades really aliens? | A World Unseen: the diversity of life". u.osu.edu. Retrieved May 11, 2021.
    14. ↑ Guo, Xueying; Ballard, Sarah; Dragomir, Diana; Werner, Michael; Livingston, John; Gorjian, Varoujan (July 2019). "Temperate Super-Earths/Mini-Neptunes around M/K Dwarfs Consist of Two Populations Distinguished by Kepler and Spitzer Transit Depth Variations". The Astrophysical Journal. 880 (1): 64. arXiv: 1804.00071 . Bibcode:2019ApJ...880...64G. doi: 10.3847/1538-4357/ab24be . ISSN   0004-637X. S2CID   119288494.
    15. ↑ "GJ 832c: Habitable Super-Earth or Super-Venus?". Drew Ex Machina. June 27, 2014. Retrieved May 21, 2022.
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