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Kepler-37

Line up comparing the Kepler-37 planets system to the moon and planets in our solar system.
Observation data Epoch J2000      Equinox J2000
Constellation	Lyra
Right ascension	18 56 14.28
Declination	44° 31′ 5.52″
Apparent magnitude (V)	9.710
Characteristics
Spectral type	G
Astrometry
Distance	215 ly (66 pc)
Details
Mass	0.803 ± 0.068 M☉
Radius	0.770 ± 0.026 R☉
Temperature	5417 ± 75 K
Metallicity	–0.32 ± 0.07 dex
Rotational velocity (v sin i)	1.1 ± 1.1 km/s
Age	6 Gyr
Other designations
KOI-245, KIC-8478994

Kepler-37 is a yellow dwarf, G-type star, located in the constellation Lyra, 215.2 light years from Earth. It is host to exoplanets Kepler-37b, Kepler-37c and Kepler-37d, all of which orbit very close to the star. Kepler-37 has a mass about 80.3 percent of the Sun's and a radius about 77 percent as large. It has a temperature similar to that of the Sun, but a bit cooler at 5,417 Kelvin. It has about half the metallicity of our Sun. With an age of roughly 6 billion years, it is slightly older than the Sun, but is still a main-sequence star. As of February 2013, Kepler-37 is the smallest star to be measured via asteroseismology. The asteroseismology work was paid for by White Dwarf, a crowd funded non-profit organization.

Planetary system

Kepler-37b is the closest planet to the Kepler-37. At the time of its discovery in February 2013, it was the smallest known exoplanet. At 3,865 kilometres (2,402 mi) in diameter, it is slightly larger than Earth's moon. It orbits Kepler-37 once every 13 Earth days at a distance of about 0.1 astronomical units (AU). Kepler-37b has a rocky surface and is believed to be too small and too close to its star to support water or maintain an atmosphere. Surface temperature is estimated at 700 Kelvin.

Kepler-37c is around three-quarters of the diameter of Earth and orbits approximately every 21 Earth days at a distance of just under 0.14 AU. Kepler-37d is about twice the diameter of Earth. It orbits in around 40 Earth days at a distance of nearly 0.21 AU. Neither is able to support water due to their close proximity to Kepler-37.

The periods of the three planets are close (within one per cent) to a 5:8:15 mean motion resonance relationship.

Discovery

The Kepler planets were discovered in September 2012 with the aid of transit events detected by the Kepler space telescope, and announced to the public in February 2013. Computer simulation was used to rule out other astronomical phenomenon mimicking planetary transit with probabilities of error <0.05% (3σ) for each potential planet. Additionally, simulation demonstrated that the proposed planetary configuration was stable. The exoplanets planets were considerably smaller than any previously detected, leading Science World Reports to state that a "a major technological improvement for the telescope" had been achieved.

Thomas Barclay, an astrophysicist on the Kepler space telescope team, said the discovery was "really good news" in the search for hospitable planets, a prime objective of the project, because it demonstrated the telescope was capable of detecting Earth-sized planets. However, he does not anticipate finding many planets as small as Kepler-37b due to the very small amount of light such planets obscure. According to NASA scientist Jack Lissauer, the discovery of Kelper-37b "suggests such little planets are common, and more planetary wonders await as we continue to gather and analyze additional data." Astronomer John Johnson of Caltech university said the discovery would have been "unimaginable" a few years ago and that the telescope had revolutionized astronomers' picture of the universe.

References

1. ^ "Kepler Host Star Characteristics". Archive for Space Telescopes. STSI. 2012-02-24. Retrieved 2013-02-21.
2. ^ "A sub-Mercury-sized exoplanet (Additional Information)" (PDF). Nature. 2013-02-20. Retrieved 2013-02-21.
3. ^ Barclay, T.; Rowe, J. F.; Lissauer, J. J.; Huber, D.; Fressin, F.; Howell, S. B.; Bryson, S. T.; Chaplin, W. J.; Désert, J.-M.; Lopez, E. D.; Marcy, G. W.; Mullally, F.; Ragozzine, D.; Torres, G.; Adams, E. R.; Agol, E.; Barrado, D.; Basu, S.; Bedding, T. R.; Buchhave, L. A.; Charbonneau, D.; Christiansen, J. L.; Christensen-Dalsgaard, J.; Ciardi, D.; Cochran, W. D.; Dupree, A. K.; Elsworth, Y.; Everett, M.; Fischer, D. A.; Ford, E. B.; Fortney, J. J.; Geary, J. C.; Haas, M. R.; Handberg, R.; Hekker, S.; Henze, C. E.; Horch, E.; Howard, A. W.; Hunter, R. C.; Isaacson, H.; Jenkins, J. M.; Karoff, C.; Kawaler, S. D.; Kjeldsen, H.; Klaus, T. C.; Latham, D. W.; Li, J.; Lillo-Box, J.; Lund, M. N.; Lundkvist, M.; Metcalfe, T. S.; Miglio, A.; Morris, R. L.; Quintana, E. V.; Stello, D.; Smith, J. C.; Still, M.; Thompson, S. E. (2013-02-20). "A sub-Mercury-sized exoplanet". Nature. doi:10.1038/nature11914. ISSN 0028-0836. Retrieved 2013-02-21.
4. ^ "NASA's Kepler Mission Discovers Tiny Planet System" (Press release). NASA. February 20, 2012. Retrieved February 21, 2012.
5. Phil Plait (February 20, 2013). "Astronomers Find the Tiniest Exoplanet Yet". Bad Astromony blog. Slate. {{cite news}}: Italic or bold markup not allowed in: |publisher= (help); Italic or bold markup not allowed in: |work= (help); Unknown parameter |access date= ignored (|access-date= suggested) (help)
6. ^ Catherine Griffin (February 21, 2013). "Tiniest Planet Yet Discovered by NASA Outside our Solar System". Science World Report. Retrieved February 21, 2013.
7. ^ Eryn Brown (February 21, 2013). "NASA, using Kepler space telescope, finds smallest planet yet". LA Times. Retrieved February 21, 2013.

Further reading

• Barclay, Thomas (2013). "A sub-Mercury-sized exoplanet". Nature. doi:10.1038/nature11914. ISSN 0028-0836. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help) (Supplementary information)

External links

• Table of confirmed planets at NASA, Kepler mission

• Planetary systems
• Planetary transit variables
• Lyra (constellation)
• G-type main sequence stars
• Kepler Objects of Interest