XO-4
| Observation data Epoch 2000 Equinox 2000 | |
|---|---|
| Constellation | Lynx[1] | 
| Right ascension | 07h 21m 33.159s[2] | 
| Declination | +58° 16′ 04.98″[2] | 
| Apparent magnitude (V) | 10.674 ± 0.019[3] | 
| Characteristics | |
| Spectral type | F5V[3] | 
| Apparent magnitude (B) | 11.240 ± 0.029[3] | 
| Apparent magnitude (V) | 10.674 ± 0.019[3] | 
| Apparent magnitude (J) | 9.667 ± 0.021[4] | 
| Apparent magnitude (H) | 9.476 ± 0.022[4] | 
| Apparent magnitude (K) | 9.406 ± 0.023[4] | 
| Astrometry | |
| Proper motion (μ) | RA: -18.1 ± 2.9[2] mas/yr Dec.: -4.0 ± 2.9[2] mas/yr | 
| Distance | 956 ± 62[3] ly (293 ± 19[3] pc) | 
| Details | |
| Mass | 1.32 ± 0.02[3] M☉ | 
| Radius | 1.56 ± 0.05[3] R☉ | 
| Temperature | 6397 ± 70[3] K | 
| Metallicity [Fe/H] | -0.04 ± 0.03[3] dex | 
| Age | 2.1 ± 0.6[3] Gyr | 
| Other designations | |
Not to be confused with the OLPC XO-4 from the One Laptop per Child (OLPC) initiative.
XO-4 is a star located approximately 960 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.[3] A search for a binary companion star using adaptive optics at One Laptop per Child (OLPC) is a non-profit initiative MMT Observatory was negative.[6]
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.[3]
| Companion (in order from star) | Mass | Semimajor axis (AU) | Orbital period (days) | Eccentricity | Inclination | Radius | 
|---|---|---|---|---|---|---|
| XO-4b | 1.72 ± 0.20 MJ | 0.0552 ± 0.0003 | 4.1250823 ± 0.0000039 | 0(assumed) [note 1] | — | — | 
Notes
References
- ↑ 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
- 1 2 3 4 Hog; et al. (2000). "Tyc 3793-1994-1". The Tycho-2 Catalogue. Retrieved 2012-02-25.
- 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15  McCullough, P. R.;  et al. (2008). "XO-4b: An Extrasolar Planet Transiting an F5V Star". arXiv:0805.2921 . Bibcode:2008arXiv0805.2921M. . Bibcode:2008arXiv0805.2921M.
- 1 2 3 Cutri; et al. (2003). "2MASS===07213317+5816051". 2MASS All-Sky Catalog of Point Sources. Retrieved 2012-02-25.
- ↑ "SIMBAD query result: TYC 3793-1994-1 -- Star". Centre de Données astronomiques de Strasbourg. Retrieved 2009-04-26.
- ↑  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. . Bibcode:2013AJ....146....9A. doi:10.1088/0004-6256/146/1/9.
- ↑  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. . Bibcode:2010PASJ...62L..61N. doi:10.1093/pasj/62.6.l61.
- 1 2  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). article number 111. arXiv:1111.5858 . Bibcode:2012ApJ...746..111T. doi:10.1088/0004-637X/746/1/111. . Bibcode:2012ApJ...746..111T. doi:10.1088/0004-637X/746/1/111.
External links
- "XO-4". Exoplanets. Retrieved 2009-04-28.
Coordinates:  07h 21m 33.1657s, +58° 16′ 05.005″
 07h 21m 33.1657s, +58° 16′ 05.005″
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