CoRoT-7c
{{short description|Extrasolar planet}}
{{Infobox planet
| name = CoRoT-7c
| image =
| caption = Artistic simulation of CoRoT-7c as a hot mini-Neptune.
| discoverer = Queloz et al.
| discovery_site = La Silla Observatory, Chile
| discovered = August 24, 2009
| discovery_method = Radial Velocity (HARPS)
| apsis = astron
| semimajor = {{convert|0.046|AU|km|abbr=on}}{{cite journal |author1=Queloz, D. |author2=Bouchy, F. |author3=Moutou, C. |author4=Hatzes, A. |author5=Hebrard, G. |author6=Alonso, R. |author7=Auvergne, M. |author8=Baglin, A. |author9=Barbieri, M. |author10=Barge, P. |author11=Benz, W. |author12=Bordé, P. |author13=Deeg, H. |author14=Deleuil, M. |author15=Dvorak, R. |author16=Erikson, A. |author17=Ferraz Mello, S. |author18=Fridlund, M. |author19=Gandolfi, D. |author20=Gillon, M. |author21=Guenther, E. |author22=Guillot, T. |author23=Jorda, L. |author24=Hartmann, M. |author25=Lammer, H. |author26=Léger, A. |author27=Llebaria, A. |author28=Lovis, C. |author29=Magain, P. |author30=Mayor, M. |author31=Mazeh, T. |author32=Ollivier, M. |author33=Pätzold, M. |author34=Pepe, F. |author35=Rauer, H. |author36=Rouan, D. |author37=Schneider, J. |author38=Segransan, D. |author39=Udry, S. |author40=Wuchterl, G. |name-list-style=amp |year=2009 |title=The CoRoT-7 planetary system: two orbiting Super-Earths |url=http://www.aanda.org/articles/aa/pdf/forth/aa13096-09.pdf |journal=Astronomy and Astrophysics |doi=10.1051/0004-6361/200913096 |volume=506 |issue=1 |pages=303–319 |bibcode=2009A&A...506..303Q |doi-access=free }} Also available from [http://exoplanet.eu/papers/corot7-RV.pdf exoplanet.eu] {{Webarchive|url=https://web.archive.org/web/20120111055444/http://exoplanet.eu/papers/corot7-RV.pdf |date=2012-01-11 }}
| eccentricity = 0
| period = 3.698 ± 0.003 d
| star = CoRoT-7
| mass = 13.289{{±|0.689}}{{Cite journal |last1=John |first1=Ancy Anna |last2=Collier Cameron |first2=Andrew |last3=Wilson |first3=Thomas G. |date=2022-09-01 |title=The impact of two non-transiting planets and stellar activity on mass determinations for the super-Earth CoRoT-7b |journal=Monthly Notices of the Royal Astronomical Society |volume=515 |issue=3 |pages=3975–3995 |doi=10.1093/mnras/stac1814 |doi-access=free |issn=0035-8711|arxiv=2206.14216 |bibcode=2022MNRAS.515.3975J }} {{Earth mass|sym=y|link=y}}
}}
CoRoT-7c is an extrasolar planet which orbits the G-type main sequence star CoRoT-7, located approximately 489 light years away in the constellation Monoceros. It is either a super-Earth or a Neptune-like planet, orbiting at 0.046 AU from the star, taking 3.7 days or 89 hours to make one round trip around the star.
Discovery
The discovery of the planet was announced in February 2009, during the First Corot Symposium. It was discovered during the follow-up started in order to confirm the existence of CoRoT-7b, a super-Earth uncovered by the CoRoT mission. However, unlike CoRoT-7b, it was not detected by the transit method from the CoRoT satellite, but only by the radial velocity method using HARPS from La Silla Observatory, Chile. A posteriori search of transits of CoRoT-7c in the lightcurve of the star CoRoT-7 yielded a negative result, confirming the planet is not transiting. As a consequence no radius measurement is available, and no density and structure models of the planet can be established.
Characteristics
Like CoRoT-7b, the mass of CoRoT-7c is weakly constrained, since the radial velocity data is noisy due to the presence of stellar activity. Published mass measurements range from 8.4 Earth masses to 13.5 Earth masses,{{Cite journal | arxiv=1011.2144 | author1=Ferraz-Mello | author2=Tadeu dos Santos | author3=Beauge | author4=Michtchenko | author5=Rodriguez | title=On planetary mass determination in the case of super-Earths orbiting active stars. The case of the CoRoT-7 system | year=2010 | doi=10.1051/0004-6361/201016059 | volume=531 | journal=Astronomy | page=A161 | bibcode=2011A&A...531A.161F| s2cid=55422304 }} passing through 12.4 Earth masses{{Cite journal | arxiv=1006.5476 | author1=Hatzes | author2=Dvorak | author3=Wuchterl | author4=Guterman | author5=Hartmann | author6=Fridlund | author7=Gandolfi | author8=Guenther | author9=Paetzold | title=An Investigation into the Radial Velocity Variations of CoRoT-7 | year=2010 | doi=10.1051/0004-6361/201014795 | volume=520 | journal=Astronomy and Astrophysics | page=A93 | bibcode=2010A&A...520A..93H| s2cid=38803450 }} and 13.1 Earth masses.{{Cite journal | last1 = Léger | first1 = A. | last2 = Grasset | first2 = O. | last3 = Fegley | first3 = B. | last4 = Codron | first4 = F. | last5 = Albarede | first5 = A. F. | last6 = Barge | first6 = P. | last7 = Barnes | first7 = R. | last8 = Cance | first8 = P. | last9 = Carpy | first9 = S. | last10 = Catalano | first10 = F. | last11 = Cavarroc | first11 = C. | last12 = Demangeon | first12 = O. | last13 = Ferraz-Mello | first13 = S. | last14 = Gabor | first14 = P. | last15 = Grießmeier | first15 = J. -M. | last16 = Leibacher | first16 = J. | last17 = Libourel | first17 = G. | last18 = Maurin | first18 = A. -S. | last19 = Raymond | first19 = S. N. | last20 = Rouan | first20 = D. | last21 = Samuel | first21 = B. | last22 = Schaefer | first22 = L. | last23 = Schneider | first23 = J. | last24 = Schuller | first24 = P. A. | last25 = Selsis | first25 = F. | last26 = Sotin | first26 = C. | title = The extreme physical properties of the CoRoT-7b super-Earth | doi = 10.1016/j.icarus.2011.02.004 | journal = Icarus | volume = 213 | issue = 1 | pages = 1 | year = 2011 |arxiv = 1102.1629 |bibcode = 2011Icar..213....1L | s2cid = 55348462 }} This mass range encompasses the Super-Earths to Neptunes transition, so the nature of CoRoT-7c, either a rocky planet or an ice giant, remains unclear. However, if the larger mass estimates are correct, CoRoT-7c is probably a hot Uranus-like planet. Chances are high that planet's rotation is tidally locked to the orbital period, with one side of the planet always facing the star CoRoT-7 and the other one in permanent darkness.
A third planet, CoRoT-7d, is present in the system. Strong mutual gravitational forces could be exchanged between these planets, leading to powerful tidal forces.
Doubts about existence
A published study{{Cite journal | arxiv=1008.3859 | author1=Frederic Pont | author2=Suzanne Aigrain | author3=Shay Zucker | title=Re-assessing the radial-velocity evidence for planets around CoRoT-7 | year=2010 | doi=10.1111/j.1365-2966.2010.17823.x | volume=411 | issue=3 | journal=Monthly Notices of the Royal Astronomical Society | pages=1953–1962 | doi-access=free | bibcode=2011MNRAS.411.1953P| s2cid=118544414 }} cast doubt on CoRoT-7c's existence, arguing that the combined presence of stellar activity and additional errors on HARPS radial velocity measurements preclude a meaningful search for additional companions besides CoRoT-7b. However, all the other studies seem to confirm the planet's existence: the signal in the HARPS data of CoRoT-7c is detected in analysis of different type, does not seem to be correlated with stellar activity and is stronger than the signal associated with the confirmed CoRoT-7b. The remarkable stability and precision showed by the HARPS spectrograph{{cite web | url=http://www.eso.org/public/news/eso0308/ | title="First Light" for HARPS at la Silla - Advanced Planet-Hunting Spectrograph Passes First Tests with Flying Colours}} also speaks in favour of the detection. The status of CoRoT-7c seems very well confirmed.
References
{{Reflist}}
{{CoRoT-7}}
{{DEFAULTSORT:Corot-7c}}
Category:Exoplanets discovered in 2009