External links
- "CoRot-3". Exoplanets. Archived from the original on 2016-03-03. Retrieved 2009-04-28.
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Aquila [1] |
| Right ascension | 19h 28m 13.2642s [2] |
| Declination | +00° 07′ 18.614″ [2] |
| Apparent magnitude (V) | 13.3 [3] |
| Characteristics | |
| Spectral type | F3V [4] |
| Apparent magnitude (B) | 13.85 ±0.44 [4] |
| Apparent magnitude (I) | 12.54 ±0.04 [4] |
| Apparent magnitude (J) | 11.94 ±0.03 [4] |
| Apparent magnitude (H) | 11.71 ±0.04 [4] |
| Apparent magnitude (K) | 11.62 ±0.03 [4] |
| Astrometry | |
| Proper motion (μ) | RA: 3.493±0.084 [2] mas/yr Dec.: −0.326±0.063< [2] mas/yr |
| Parallax (π) | 1.2747±0.0497 mas [2] |
| Distance | 2,560 ± 100 ly (780 ± 30 pc) |
| Other designations | |
| GSC 00465-01645, DENIS-P J192813.2+000718, 2MASS J19281326+0007185, USNO-A2.0 0900-15209129, CoRoT-Exo-3, GSC2.3 N1MO000645, UCAC2 31931545, USNO-B1.0 0901-00488457 [4] | |
| 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. [4]
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. [5]
| 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 |
