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Kepler-10

Coordinates: Sky map 19h 02m 43s, +50° 14′ 28.7″
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Kepler-10

An artist's depiction of the Kepler-10 system. Kepler-10c is in the foreground.
Observation data
Epoch J2000      Equinox J2000
Constellation Draco
Right ascension 19h 02m 43.0612s[1]
Declination +50° 14′ 28.701″[1]
Apparent magnitude (V) 11.157[2]
Astrometry
Proper motion (μ) RA: −18.394±0.045[1] mas/yr
Dec.: 41.448±0.046[1] mas/yr
Parallax (π)5.3618 ± 0.0233 mas[1]
Distance608 ± 3 ly
(186.5 ± 0.8 pc)
Characteristics
Spectral type G[3]
Details
Mass0.910 ± 0.021[2] M☉
Radius1.065 ± 0.009[2] R☉
Temperature5708 ± 28[2] K
Age10.6+1.5
−1.3[2] Gyr
Other designations
KOI-72, KIC 11904151, GSC 03549-00354, 2MASS J19024305+5014286[4]
Database references
SIMBADdata
KICdata

Kepler-10, formerly known as KOI-72, is a Sun-like star in the constellation of Draco that lies 187 parsecs (608 light years) from Earth. Kepler-10 was targeted by NASA's Kepler spacecraft, as it was seen as the first star identified by the Kepler mission that could be a possible host to a small, transiting exoplanet.[5] The star is slightly less massive, slightly larger, and slightly cooler than the Sun; at an estimated 10.4 billion years in age, Kepler-10 is almost 2.6 times the age of the Sun. Kepler-10 is host to a planetary system made up of at least two planets. Kepler-10b, the first undeniably rocky planet,[5] was discovered in its orbit after eight months of observation and announced on January 10, 2011. The planet orbits its star closely, completing an orbit every 0.8 days,[6] and has a density similar to that of iron.[5] The second planet, Kepler-10c, was confirmed on May 23, 2011, based on follow-up observations by the Spitzer Space Telescope. The data shows it has an orbital period of 42.3 days and has a radius more than double that of Earth, but a higher density, making it the largest and most massive rocky planet discovered as of June 2014.[2][7][8]

Nomenclature and history

Kepler-10 was named because it was the tenth planetary system observed by the Kepler spacecraft, a NASA satellite designed to search for Earth-like planets that transit, or cross in front of, their host stars with respect to Earth. The transit slightly dims the host star; this periodic dimming effect is then noted by Kepler.[9] After eight months of observation ranging from May 2009 to January 2010, the Kepler team established Kepler-10b as the first rocky exoplanet discovered by the Kepler satellite. Kepler-10 was the first Kepler-targeted star suspected of having a small planet in orbit. Because of that, verifying Kepler's discovery was prioritized by telescopes at the W.M. Keck Observatory in Hawaii. The discovery was successfully verified.[5] Although there had been many potentially rocky exoplanets discovered in the past, Kepler-10b was the first definitively rocky planet to have been discovered.[10]

The discovery of Kepler-10b was announced to the public at a winter meeting of the American Astronomical Society on January 10, 2011 in Seattle.[10] On May 23, 2011, the existence of Kepler-10c was confirmed at the 218th AAS meeting in Boston.[11]

Characteristics

Kepler-10 is a G-type star, like the Sun. With a mass of 0.895 (± 0.06) Msun and a radius of 1.056 (± 0.021) Rsun, the star is approximately 10% smaller than and 5% wider than the Sun. The metallicity of Kepler-10, as measured in [Fe/H] (the amount of iron in the star), is -0.15 (± 0.04); this means that Kepler-10 is about 70% as metal-rich as the Sun. Metallicity tends to play a large role in the formation of planets, determining if they form, and what kind of planet they will form.[12] In addition, Kepler-10 is estimated to be 11.9 billion years old and to have an effective temperature of 5627 (± 44) K;[3] To compare, the Sun is younger and hotter, with an age of 4.6 billion years[13] and an effective temperature of 5778 K.[14]

Kepler-10 is located at a distance of 173 (± 27) parsecs from the Earth, which equates to approximately 564 light years. Also, Kepler-10's apparent magnitude, or brightness as seen from Earth, is 10.96; it therefore cannot be seen with the naked eye.[3]

An artist's impression of planet Kepler-10b.

Planetary system

Per the usual exoplanet nomenclature, the first planet discovered to be orbiting Kepler-10 is called Kepler-10b. Announced in 2011, it was the first rocky planet identified outside the Solar system. The planet has a mass that is 3.33±0.49 times that of Earth's and a radius that is 1.47+0.03
−0.02 times that of Earth.[2] The planet orbits Kepler-10 at a distance of 0.01684 AU every 0.8375 days; this can be compared to the orbit and orbital period of planet Mercury, which circles the Sun at a distance of 0.3871 AU every 87.97 days.[15] Because the planet orbits so closely to its star, its eccentricity is virtually zero. It, thus, has an extremely circular orbit.[6]

Kepler-10c[7] was also discovered by NASA's Kepler Mission,[16] the second exoplanet found to orbit Kepler-10. Radial-velocity measurements of the body suggest that it has a mass of 17.2±1.9 Earth masses and a radius of 2.35 Earth radii, making it the largest known rocky planet as of 2014. Kepler-10c would orbit Kepler-10 at a distance of 0.24 AU every 45.29 days.[2]

Kepler-10d was discovered in 2017 and still has not been confirmed. It would orbit its parent star at a distance of 0.366 AU every 102±1 days. [17]

The Kepler-10 planetary system[6]
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
(days) 		Eccentricity Inclination Radius
b 3.33±0.49 M🜨 0.01684 0.837495 0 84.8+3.2
−3.9° 		1.47+0.03
−0.02 R🜨
c 7.37+1.32
−1.19[18] M🜨 		0.2410 45.29485 0 89.59+0.25
−0.43° 		2.35+0.09
−0.04 R🜨
d (unconfirmed) 5.7+1.9
−1.7 M🜨 		0.366 102 ± 1 ? ?° ? R🜨
Kepler-10 System.

See also

References

  1. ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. ^ a b c d e f g h Dumusque, Xavier; Bonomo, Aldo S.; Haywood, Raphaëlle D.; Malavolta, Luca; Ségransan, Damien; Buchhave, Lars A.; Cameron, Andrew Collier; Latham, David W.; Molinari, Emilio; Pepe, Francesco; Udry, Stéphane; Charbonneau, David; Cosentino, Rosario; Dressing, Courtney D.; Figueira, Pedro; et al. (2014). "The Kepler-10 Planetary System Revisited by Harps-N: A Hot Rocky World and a Solid Neptune-Mass Planet". The Astrophysical Journal. 789 (2): 154. arXiv:1405.7881. Bibcode:2014ApJ...789..154D. doi:10.1088/0004-637X/789/2/154. S2CID 53475787.
  3. ^ a b c "Notes for star Kepler-10". Extrasolar Planets Encyclopaedia. 2011. Archived from the original on 21 January 2011. Retrieved 13 March 2011.
  4. ^ "Kepler-10". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2011-02-01.
  5. ^ a b c d Perrotto, Trent J.; Hoover, Rachel (10 January 2011). "NASA'S Kepler Mission Discovers Its First Rocky Planet". Ames Research Center. NASA. Retrieved 13 March 2011.
  6. ^ a b c "Summary Table of Kepler Discoveries". NASA. 2011. Retrieved 13 March 2011.
  7. ^ a b Fressin, François; et al. (2011). "Kepler-10c, A 2.2-Earth Radius Transiting Planet In A Multiple System". The Astrophysical Journal Supplement Series. 197 (1). 5. arXiv:1105.4647. Bibcode:2011ApJS..197....5F. doi:10.1088/0067-0049/197/1/5.
  8. ^ Clavin, Whitney (June 2, 2014). "Astronomers Confounded By Massive Rocky World". NASA. Retrieved June 3, 2014.
  9. ^ "Mission overview". Kepler and K2. NASA. Retrieved 9 August 2020.
  10. ^ a b Richard A. Lovett (10 January 2011). "NASA Finds Smallest Earthlike Planet Outside Solar System". National Geographic Society. Retrieved 13 March 2011.
  11. ^ "Kepler Spacecraft Shows That Smaller Planets Abound". Scientific American. 2011. Retrieved 2011-05-26.
  12. ^ Henry Bortman (12 October 2004). "Extrasolar Planets: A Matter of Metallicity". Space Daily. Retrieved 13 March 2011.
  13. ^ Fraser Cain (16 September 2008). "How Old is the Sun?". Universe Today. Retrieved 13 March 2011.
  14. ^ Ed Grayzeck. "Sun Fact Sheet". Goddard Space Flight Center. NASA. Retrieved 13 March 2011.
  15. ^ David Williams (17 November 2010). "Mercury Fact Sheet". Goddard Space Flight Center. NASA. Retrieved 27 February 2011.
  16. ^ "NASA'S Kepler Mission Discovers Its First Rocky Planet". NASA. 2011-01-10. Retrieved 2011-01-10.
  17. ^ "Three planets in the Kepler-10 system" (in Russian).
  18. ^ Rajpaul, V.; Buchhave, L. A.; Aigrain, S. (2017). "Pinning down the mass of Kepler-10c: The importance of sampling and model comparison". Monthly Notices of the Royal Astronomical Society. 471 (1): L125. arXiv:1707.06192. Bibcode:2017MNRAS.471L.125R. doi:10.1093/mnrasl/slx116. S2CID 119243418.{{cite journal}}: CS1 maint: unflagged free DOI (link)


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