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CoRoT-3

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]

CoRoT-3
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]
Distance2,560 ± 100 ly
(780 ± 30 pc)
Details
Mass1.37 ±0.09 M
Radius1.56 ±0.09 R
Temperature6740 ±140 K
Metallicity-0.02 ±0.06
Age2 (−0.4+0.8)× 109 years
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[2]
Database references
SIMBADdata
Extrasolar Planets
Encyclopaedia
data

Planetary system Edit

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]

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

See also Edit

References Edit

  1. ^ a b c d e 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.
  2. ^ a b c d e f g h "GSC 00465-01645". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2009-04-27.
  3. ^ 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 Edit

  • . Exoplanets. Archived from the original on 2016-03-03. Retrieved 2009-04-28.


corot, white, yellow, dwarf, main, sequence, star, hotter, than, this, star, located, approximately, 2560, light, years, away, constellation, aquila, apparent, magnitude, this, star, which, means, visible, naked, seen, with, medium, sized, amateur, telescope, . 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 CoRoT 3 Observation dataEpoch J2000 0 Equinox J2000 0Constellation AquilaRight ascension 19h 28m 13 2642s 1 Declination 00 07 18 6143 1 Apparent magnitude V 13 3CharacteristicsSpectral 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 AstrometryProper motion m RA 3 493 0 084 1 mas yr Dec 0 326 0 063 lt 1 mas yrParallax p 1 2747 0 0497 mas 1 Distance2 560 100 ly 780 30 pc DetailsMass1 37 0 09 M Radius1 56 0 09 R Temperature6740 140 KMetallicity 0 02 0 06Age2 0 4 0 8 109 yearsOther designationsGSC 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 2 Database referencesSIMBADdataExtrasolar PlanetsEncyclopaediadata Contents 1 Planetary system 2 See also 3 References 4 External linksPlanetary system EditThis 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 The CoRoT 3 planetary system Companion in order from star Mass Semimajor axis AU Orbital period days Eccentricity Inclination Radiusb 21 66 1 MJ 0 057 0 003 4 2568 5e 06 0 85 9 0 8 1 01 0 07 RJSee also EditList of extrasolar planetsReferences Edit a b c d e Brown A G A et al Gaia collaboration August 2018 Gaia Data Release 2 Summary of the contents and survey properties Astronomy amp Astrophysics 616 A1 arXiv 1804 09365 Bibcode 2018A amp A 616A 1G doi 10 1051 0004 6361 201833051 Gaia DR2 record for this source at VizieR a b c d e f g h GSC 00465 01645 SIMBAD Centre de donnees 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 amp A 491 889D doi 10 1051 0004 6361 200810625 S2CID 8944836 External links Edit CoRot 3 Exoplanets Archived from the original on 2016 03 03 Retrieved 2009 04 28 Retrieved from https en wikipedia org w index php title CoRoT 3 amp oldid 1116409940, wikipedia, wiki, book, books, library,

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