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XO-4

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(Redirected from Koit (star)) Star in the constellation Lynx Not to be confused with the OLPC XO-4 from the One Laptop per Child (OLPC) initiative or the Martin XO-4.
XO-4 / Koit
Observation data
Epoch J2000      Equinox J2000
Constellation Lynx
Right ascension 07 21 33.1602
Declination +58° 16′ 05.110″
Apparent magnitude (V) 10.674 ± 0.019
Characteristics
Spectral type F5V
Apparent magnitude (B) 11.240 ± 0.029
Apparent magnitude (V) 10.674 ± 0.019
Apparent magnitude (J) 9.667 ± 0.021
Apparent magnitude (H) 9.476 ± 0.022
Apparent magnitude (K) 9.406 ± 0.023
Astrometry
Proper motion (μ) RA: −17.008(12) mas/yr
Dec.: 5.463(12) mas/yr
Parallax (π)3.7812 ± 0.0156 mas
Distance863 ± 4 ly
(264 ± 1 pc)
Details
Mass1.32 ± 0.02 M
Radius1.56 ± 0.05 R
Temperature6397 ± 70 K
Metallicity -0.04 ± 0.03 dex
Age2.1 ± 0.6 Gyr
Other designations
Koit, TYC 3793-1994-1, GSC 03793-01994, 2MASS J07213317+5816051
Database references
SIMBADdata

XO-4 is a star located approximately 863 light-years away from Earth in the Lynx constellation. It has a magnitude of about 11 and cannot be seen with the naked eye but is visible through a small telescope. A search for a binary companion star using adaptive optics at MMT Observatory was negative.

The star XO-4 is named Koit. The name was selected in the NameExoWorlds campaign by Estonia, during the 100th anniversary of the IAU. Koit is Estonian for dawn, and was named for a character in a folk tale written by Friedrich Robert Faehlmann.

Planetary system

One known exoplanet, XO-4b, which is classified as a hot jupiter, orbits XO-4. This exoplanet was discovered in 2008 by the XO Telescope project using the transit method. It has been named Hämarik, meaning dusk, and referring to a character from the same Faehlmann story featuring Koit.

The XO-4 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b / Hämarik 1.72 ± 0.20 MJ 0.0552 ± 0.0003 4.1250823 ± 0.0000039 0(assumed)

Notes

  1. eccentricity approximately equal to zero is expected theoretically and is consistent with the radial velocities and secondary eclipses timing

References

  1. Roman, Nancy G. (1987). "Identification of a Constellation From a Position". Publications of the Astronomical Society of the Pacific. 99 (617): 695–699. Bibcode:1987PASP...99..695R. doi:10.1086/132034. Vizier query form
  2. ^ Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  3. ^ McCullough, P. R.; et al. (2008). "XO-4b: An Extrasolar Planet Transiting an F5V Star". arXiv:0805.2921 .
  4. ^ Cutri; et al. (2003). "2MASS===07213317+5816051". 2MASS All-Sky Catalog of Point Sources. Retrieved 2012-02-25.
  5. "SIMBAD query result: TYC 3793-1994-1 -- Star". Centre de Données astronomiques de Strasbourg. Retrieved 2009-04-26.
  6. Adams, E. R.; et al. (2013). "Adaptive Optics Images. II. 12 Kepler Objects of Interest and 15 Confirmed Transiting Planets". The Astronomical Journal. 146 (1). 9. arXiv:1305.6548. Bibcode:2013AJ....146....9A. doi:10.1088/0004-6256/146/1/9. S2CID 119117620.
  7. "Approved names". NameExoworlds. Retrieved 2020-01-02.
  8. "International Astronomical Union | IAU". www.iau.org. Retrieved 2020-01-02.
  9. "Estonia has been assigned its own star and planet". Estonian World. 20 January 2020. Retrieved 2020-01-20.
  10. "Estonia has been assigned its own star and planet". Estonian World. 20 January 2020. Retrieved 2020-01-20.
  11. Narita, Norio; et al. (2010). "The Rossiter-McLaughlin Effect of the Transiting Exoplanet XO-4b". Publications of the Astronomical Society of Japan. 62 (6): L61 – L65. arXiv:1008.3803. Bibcode:2010PASJ...62L..61N. doi:10.1093/pasj/62.6.l61. S2CID 2967944.
  12. ^ Todorov, Kamen O.; et al. (2012). "Warm Spitzer Observations of Three Hot Exoplanets: XO-4b, HAT-P-6b, and HAT-P-8b". The Astrophysical Journal. 746 (1). 111. arXiv:1111.5858. Bibcode:2012ApJ...746..111T. doi:10.1088/0004-637X/746/1/111. S2CID 119200344.

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