CoRoT-3

Star in the constellation of Aquila From Wikipedia, the free encyclopedia

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]

Quick facts Observation data Epoch J2000.0 Equinox J2000.0, Constellation ...
CoRoT-3
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
Evolutionary stage main sequence[2]
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: +3.528±0018[2] mas/yr
Dec.: −0.308±0.014<[2] mas/yr
Parallax (π)1.3118±0.0177 mas[2]
Distance2,490 ± 30 ly
(760 ± 10 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
SIMBADdata
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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.[5]

More information Companion (in order from star), Mass ...
The CoRoT-3 planetary system
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
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See also

References

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