| 词条 | COROT-2 |
| 释义 |
| name = COROT-2 }}{{Starbox image | image = | caption = COROT-2 is a G7V class star somewhat less massive than the Sun (G2V) }}{{Starbox observe | epoch = J2000.0 | constell = Aquila | appmag_v = 12.57[1] | ra = {{RA|19|27|06.4945}}[2] | dec = {{DEC|+01|23|01.3576}}[2] }}{{Starbox character | class = G7V K0V (SIMBAD)[1] | appmag_1_passband = V | appmag_1 = ~12.577 | appmag_2_passband = I | appmag_2 = 11.49 ±0.03 | appmag_3_passband = J | appmag_3 = 10.5783 ±0.028 | appmag_4_passband = H | appmag_4 = 10.44 ±0.04 | appmag_5_passband = K | appmag_5 = 10.31 ±0.03 }}{{Starbox astrometry | radial_v = | prop_mo_ra = {{val|−3.409|0.084}}[2] | prop_mo_dec = {{val|−10.936|0.074}}[2] | parallax = 4.6608 | p_error = 0.0536 | parallax_footnote = [2] | absmag_v = }}{{Starbox detail | mass = 0.97 ±0.06 | temperature = 5625 ±120 | radius= 0.902 ±0.018 | metal = 0 ±0.1 | age = ? }}{{Starbox catalog | names = GSC 00465-01282, CoRoT-Exo-2, GSC2 N023200075, UCAC2 32263596, CoRoT 101206560, DENIS-P J192706.4+012301, 2MASS J19270649+0123013, USNO-B1.0 0913-00447544[1] }}{{Starbox reference | Simbad = GSC00465-01282 | EPE = CoRoT-2 }}{{Starbox end}}COROT-2 is a yellow dwarf main sequence star a little cooler than the Sun. This star is located approximately 700 light-years away in the constellation of Aquila. The apparent magnitude of this star is 12, 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.[1] It has a true physical companion, 2MASS J19270636+0122577, with a spectral type of K9, as earlier hypothesized by Alonso et al. (2008), making COROT-2 a wide binary system with at least one planet.[2] Planetary systemThis star is home to exoplanet COROT-2b discovered by the COROT Mission spacecraft using the transit method. COROT-2b (formerly known as COROT-Exo-2b[3]) is the second extrasolar planet to be detected by the French-led COROT mission, and orbits the star COROT-2 at a distance of 930 light years from Earth towards the constellation Aquila. Its discovery was announced on 20 December 2007.[4] After its discovery via the transit method, its mass was confirmed via the radial velocity method. The planet is a large hot Jupiter, about 1.43 times the radius of Jupiter and approximately 3.3 times as massive. Its huge size is due to the intense heating from its parent star, which causes the outer layers of its atmosphere to bloat. The extremely large radius of the planet indicates that COROT-2b is really hot, estimated to be around 1500 K, even hotter than would be expected given its location close to its parent star. This fact may be a sign of tidal heating due to interactions with another planet.[5] At Jupiter-like distances its radius would roughly be the same as Jupiter.[6] The complete phase curve of this planet has been observed.[7] COROT-2b orbits its star approximately once every 1.7 days, and orbits the star in a prograde direction close to the star's equator.[8] Its parent star is a G-type star, a bit cooler than the Sun but more active. It is located about 800 light-years from Earth. It takes 125 minutes to transit its star.[9] As of August 2008, the COROT-2b spin-orbit angle (that is, the angle between the equator of the star and the plane of the planet orbit) was calculated by Bouchy et al. by means of the Rossiter–McLaughlin effect[10] with a value of +7.2 ± 4.5 degrees.[8] {{OrbitboxPlanet begin}}{{OrbitboxPlanet| exoplanet = b | mass = 3.31 ±0.16 | period = 1.7429964 ±1.7e-06 | semimajor = 0.0281 ±0.0009 | eccentricity = 0 }}{{Orbitbox end}} See also
References1. ^1 2 3 {{cite simbad | title =GSC 00465-01282 | accessdate=2009-04-27 }} [11]2. ^{{cite journal | title=The extended chromosphere of CoRoT-2A: Discovery and analysis of the chromospheric Rossiter-McLaughlin effect | author=S. Czesla | author2=S. Schröter | author3=U. Wolter | author4=C. von Essen | author5=K. F. Huber | author6=J. H. M. M. Schmitt | author7=D. E. Reichart | author8=J. P. Moore | journal=Astronomy and Astrophysics | volume=539 | pages=A150 | date=March 2012 | doi=10.1051/0004-6361/201118042 |bibcode = 2012A&A...539A.150C }} 3. ^{{cite mailing list|url=http://listes.obs.ujf-grenoble.fr/wws/arc/exoplanets/2009-03/msg00003.html|title=Change in CoRoT planets names|author=Schneider, J.|date=10 March 2009|accessdate=2009-03-19|mailinglist=Exoplanets|deadurl=yes|archiveurl=https://archive.is/20100118162658/http://listes.obs.ujf-grenoble.fr/wws/arc/exoplanets/2009-03/msg00003.html|archivedate=18 January 2010|df=}} 4. ^{{cite web | title = COROT surprises a year after launch | url = http://www.esa.int/SPECIALS/COROT/SEMF0C2MDAF_0.html | accessdate = 2007-12-21}} 5. ^{{cite web | title = CoRoT-exo-2 c? | url = http://oklo.org/?p=262 | accessdate = 2007-12-21}} 6. ^{{cite journal | title=Planetesimals to Brown Dwarfs: What is a Planet? | date=20 August 2006 | pages=193–216 | author1=Gibor Basri | volume=34 | author2=Brown | doi=10.1146/annurev.earth.34.031405.125058 | journal=Annu. Rev. Earth Planet. Sci. | arxiv=astro-ph/0608417 |bibcode = 2006AREPS..34..193B }} 7. ^{{cite journal | bibcode = 2011sptz.prop80044C | title=Phase Variations, Transits and Eclipses of the Misfit CoRoT-2b | journal=Spitzer Proposal | year=2011 | authors=Cowan, Nicolas; Deming, Drake; Gillon, Michael; Knutson, Heather; Madhusudhan, Nikku; Rauscher, Emily;}} 8. ^1 {{Cite journal | last1 = Bouchy | first1 = F. | last2 = Queloz | first2 = D. | last3 = Deleuil | first3 = M. | last4 = Loeillet | first4 = B. | last5 = Hatzes | first5 = A. P. | last6 = Aigrain | first6 = S. | last7 = Alonso | first7 = R. | last8 = Auvergne | first8 = M. | last9 = Baglin | first9 = A. | last10 = Barge | first10 = P. | last11 = Benz | first11 = W. | last12 = Bordé | first12 = P. | last13 = Deeg | first13 = H. J. | last14 = De La Reza | first14 = R. | last15 = Dvorak | first15 = R. | last16 = Erikson | first16 = A. | last17 = Fridlund | first17 = M. | last18 = Gondoin | first18 = P. | last19 = Guillot | first19 = T. | last20 = Hébrard | first20 = G. | last21 = Jorda | first21 = L. | last22 = Lammer | first22 = H. | last23 = Léger | first23 = A. | last24 = Llebaria | first24 = A. | last25 = Magain | first25 = P. | last26 = Mayor | first26 = M. | last27 = Moutou | first28 = M. | first29 = M. | last30 = Pepe | first30 = F. | last28 = Ollivier | last29 = Pätzold | first27 = C. | title = Transiting exoplanets from the CoRoT space mission | doi = 10.1051/0004-6361:200809433 | journal = Astronomy and Astrophysics | volume = 482 | issue = 3 | pages = L25 | year = 2008 | pmid = | pmc = | displayauthors = 29 |arxiv = 0803.3209 |bibcode = 2008A&A...482L..25B }} 9. ^{{cite web |title=Predicted Transit Epochs: CoRoTExo2 b |publisher=TransitSearch (Oklo Corporation) |url=http://207.111.201.70/transitsearch/dynamiccontent/CoRoTExo2b.transits.txt |accessdate=2009-07-15 }}{{dead link|date=July 2017 |bot=InternetArchiveBot |fix-attempted=yes }} 10. ^{{Cite journal| title= Measuring accurate transit parameters | journal=Proceedings of the International Astronomical Union | volume=4 | pages=99 | author=Joshua N. Winn | arxiv=0807.4929 |year=2008 | doi= 10.1017/S174392130802629X}} 11. ^1 2 3 4 5 {{Cite Gaia DR2|4287820848378092672}} }} External links
| url=http://media4.obspm.fr/exoplanets/base/etoile.php?nom=CoRot-2 | title=CoRot-2 | work=Exoplanets | accessdate=2009-04-28}}{{Sky|19|27|06.5|+|01|23|01.5|930}}{{Stars of Aquila}} 4 : G-type main-sequence stars|Planetary systems|Planetary transit variables|Aquila (constellation) |
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