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Kepler-37b is an extrasolar planet (exoplanet) orbiting Kepler-37 in the constellation Lyra.[7] As of February 2013 it is the smallest planet discovered around a main-sequence star, with a radius slightly greater than that of the Moon and slightly smaller than that of Mercury. [8] The measurements do not constrain its mass, but masses above a few times that of the Moon give unphysically high densities.[5]

Kepler-37b
Artist's impression of Kepler-37b.
Discovery
Discovery siteKepler Space Observatory
Discovery dateFebruary 20, 2013[1]
Detection method
Transit (Kepler Mission)
Orbital characteristics
Semi-major axis
0.1003 AU (15,000,000 km)[2]
Eccentricity0.080+0.210
−0.080
Orbital period (sidereal)
13.367308[1] d
Inclination88.63[2]
StarKepler-37
Physical characteristics
Mean radius
0.354 (± 0.014) REarth
Mass0.01+5.99
−0.01[3][4][5][lower-alpha 1] MEarth
Temperature700 K (427 °C; 800 °F)[6]

    Characteristics


    A size comparison of the planets in the Kepler-37 system and objects in the Solar System
    A size comparison of the planets in the Kepler-37 system and objects in the Solar System

    Mass, radius and temperature


    Kepler-37b is a sub-Earth, an exoplanet with a radius and mass smaller than Earth. Its surface temperature is 700 K (427 °C; 800 °F). Because of this, it is not expected to have an atmosphere.[6] Its radius is approximately 0.35 REarth (about a diameter of 3,900 kilometres (2,400 mi)), larger than the Moon[9] (0.27 REarth), but a little smaller than Mercury (0.38 REarth). Due to its small size, it is very likely Kepler-37b is a rocky planet with a solid surface.[6] Furthermore, it is too hot to support liquid water on its surface.[6]


    Host star


    The planet orbits a (G-type) star similar to the Sun, named Kepler-37, orbited by a total of four planets. The star has a mass of 0.80 M☉ and a radius of 0.79 R☉. It has a temperature of 5417 K and is 5.66 billion years old. In comparison, the Sun is 4.6 billion years old[10] and has a temperature of 5778 K.[11]

    The star's apparent magnitude, or how bright it appears from Earth's perspective, is 9.71. Therefore, it is too dim to be seen with the naked eye.


    Orbit


    Kepler-37b orbits its parent star at a distance of about 15 million kilometers (9.3 million miles), with a period of roughly 13 days at a distance of 0.1 AU (compared to Mercury's distance from the Sun, which is about 0.38 AU).[8] The outer two planets in the system have orbital periods[1][2] within one percent of the 8:5 and 3:1 resonances with Kepler-37b's period.


    Discovery


    Kepler-37b, along with two other planets, Kepler-37c and Kepler-37d, were discovered by the Kepler space telescope, which observes stellar transits.[1][6] After observing transits of Kepler-37b, astronomers had to compare it with the size of the parent star.

    The size of the star was obtained using asteroseismology;[9] Kepler-37 is currently the smallest star to be studied using this process.[6] This allowed the size of Kepler-37b to be determined "with extreme accuracy".[6]

    To date, Kepler-37b is the smallest planet discovered around a main-sequence star[lower-alpha 2] outside the Solar System.[8] Detection of Kepler-37b was possible due to its short orbital period, relative brightness, and low activity of its host star, allowing brightness data to average out quickly.[12] The discovery of Kepler-37b has led Jack Lissauer, a scientist at NASA's Ames Research Center, to conjecture that "such little planets are common".[6]


    See also



    Notes


    1. Masses more than a few times that of the Moon result in unphysically high densities.
    2. The pulsar planet PSR B1257+12 A has a comparable mass. The actual size of PSR B1257+12 A is unknown, but is likely comparable to Kepler-37b.

    References


    1. Barclay, T.; Rowe, J. F.; Lissauer, J. J.; Huber, D.; Fressin, F.; Howell, S. B.; Bryson, S. T.; Chaplin, W. J.; Désert, J. M. (2013-02-20). "A sub-Mercury-sized exoplanet". Nature. 494 (7438): 452–4. arXiv:1305.5587. Bibcode:2013Natur.494..452B. doi:10.1038/nature11914. ISSN 0028-0836. PMID 23426260. S2CID 205232792.
    2. "Kepler-37 System". kepler.nasa.gov. Archived from the original on May 16, 2013. Retrieved February 21, 2013.
    3. Johnson, Michele (31 March 2015). "Kepler and K2 Missions". nasa.gov. Archived from the original on 18 December 2014. Retrieved 5 October 2017.
    4. "The Extrasolar Planet Encyclopaedia — Kepler-37b". Archived from the original on 2014-02-09. Retrieved 2014-03-03.
    5. Marcy, Geoffrey W.; Isaacson, Howard; Howard, Andrew W.; Rowe, Jason F.; Jenkins, Jon M.; Bryson, Stephen T.; Latham, David W.; Howell, Steve B.; Gautier, Thomas N.; Batalha, Natalie M.; Rogers, Leslie; Ciardi, David; Fischer, Debra A.; Gilliland, Ronald L.; Kjeldsen, Hans; Christensen-Dalsgaard, Jørgen; Huber, Daniel; Chaplin, William J.; Basu, Sarbani; Buchhave, Lars A.; Quinn, Samuel N.; Borucki, William J.; Koch, David G.; Hunter, Roger; Caldwell, Douglas A.; Van Cleve, Jeffrey; Kolbl, Rea; Weiss, Lauren M.; Petigura, Erik; et al. (2014). "Masses, Radii, and Orbits of Smallkeplerplanets: The Transition from Gaseous to Rocky Planets". The Astrophysical Journal Supplement Series. 210 (2): 20. arXiv:1401.4195. Bibcode:2014ApJS..210...20M. doi:10.1088/0067-0049/210/2/20. S2CID 10760418.
    6. "NASA's Kepler Mission Discovers Tiny Planet System". NASA. February 20, 2013. Retrieved February 21, 2013.
    7. "Smallest Alien Planet Kepler-37b Explained (Infographic)". space.com. 20 February 2013. Retrieved 5 October 2017.
    8. "Tiniest Planet Yet Discovered by NASA Outside our Solar System". scienceworldreport.com. February 21, 2013. Retrieved February 21, 2013.
    9. "Astronomers Find the Tiniest Exoplanet Yet". Slate. February 20, 2013. Retrieved February 21, 2013.
    10. Fraser Cain (16 September 2008). "How Old is the Sun?". Universe Today. Retrieved 19 February 2011.
    11. Fraser Cain (15 September 2008). "Temperature of the Sun". Universe Today. Retrieved 19 February 2011.
    12. "Small Planets Confirm Kepler's Capabilities". www.centauri-dreams.org. Retrieved 5 October 2017.
    Records
    Preceded by Least massive exoplanet[citation needed]
    2013—2015    		 Succeeded by
    Preceded by
    Kepler-42 d
    		 Smallest-radius exoplanet
    2013—2015    		 Succeeded by


    На других языках

    [de] Kepler-37b

    Kepler-37b ist ein extrasolarer Planet, der im Sternbild Lyra den Stern Kepler-37 begleitet.[5] Er ist der bisher kleinste Exoplanet (Stand:2013), der einen Hauptreihen-Stern umläuft. Sein Radius (und wohl auch seine Masse) sind nur geringfügig größer als die des irdischen Mondes.
    - [en] Kepler-37b

    [ru] Kepler-37 b

    Kepler-37 b — экзопланета, обращающаяся вокруг звезды Kepler-37 в созвездии Лиры. Планета находится на расстоянии около 210 световых лет от Солнца. На момент открытия была самой маленькой из известных экзопланет, её радиус лишь немногим превышает радиус Луны[3][4].


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