Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Aquila |
Right ascension | 19h 28m 13.2642s[1] |
Declination | +00° 07′ 18.6143″[1] |
Apparent magnitude (V) | 13.3 |
Characteristics | |
Spectral type | F3V[2] |
Apparent magnitude (B) | 13.85 ±0.44[2] |
Apparent magnitude (I) | 12.54 ±0.04[2] |
Apparent magnitude (J) | 11.94 ±0.03[2] |
Apparent magnitude (H) | 11.71 ±0.04[2] |
Apparent magnitude (K) | 11.62 ±0.03[2] |
Astrometry | |
Proper motion (μ) | RA: 3.493±0.084[1] mas/yr Dec.: −0.326±0.063<[1] mas/yr |
Parallax (π) | 1.2747 ± 0.0497 mas[1] |
Distance | 2,560 ± 100 ly (780 ± 30 pc) |
Details | |
Mass | 1.37 ±0.09 M☉ |
Radius | 1.56 ±0.09 R☉ |
Temperature | 6740 ±140 K |
Metallicity | -0.02 ±0.06 |
Age | 2 (−0.4+0.8)× 109 years |
Other designations | |
Database references | |
SIMBAD | data |
CoRoT-3 is a white-yellow dwarf main sequence star hotter than the Sun. This star is located approximately 2560 light-years away in the constellation of Aquila. The apparent magnitude of this star is 13, which means it is not visible to the naked eye but can be seen with a medium-sized amateur telescope on a clear dark night.[2]
Planetary system
This star is home to object designated CoRoT-3b. This object was discovered by the CoRoT Mission spacecraft using the transit method. Measurements made using the radial velocity method show that this object is probably a brown dwarf.[3]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 21.66 ±1 MJ | 0.057 ±0.003 | 4.2568 ±5e-06 | 0 | 85.9 ± 0.8° | 1.01 ± 0.07 RJ |
See also
References
- 1 2 3 4 5 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.
- 1 2 3 4 5 6 7 8 "GSC 00465-01645". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2009-04-27.
- ↑ Deleuil, M.; et al. (2008). "Transiting exoplanets from the CoRoT space mission. VI. CoRoT-Exo-3b: the first secure inhabitant of the brown-dwarf desert". Astronomy and Astrophysics. 491 (3): 889–897. arXiv:0810.0919. Bibcode:2008A&A...491..889D. doi:10.1051/0004-6361:200810625. S2CID 8944836.
External links
- "CoRot-3". Exoplanets. Archived from the original on 2016-03-03. Retrieved 2009-04-28.
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