Astronomy:CoRoT-7
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Monoceros[1] |
| Right ascension | 06h 43m 49.4688s[2] |
| Declination | −01° 03′ 46.817″[2] |
| Apparent magnitude (V) | 11.668[1] |
| Characteristics | |
| CoRoT-7A | |
| Spectral type | G9V[1] |
| CoRoT-7B | |
| Spectral type | M4V[3] |
| Astrometry | |
| Radial velocity (Rv) | +31.174 ± 0.0086[1] km/s |
| Proper motion (μ) | RA: 10.984[2] mas/yr Dec.: -0.040[2] mas/yr |
| Parallax (π) | 6.2676 ± 0.0139[2] mas |
| Distance | 520 ± 1 ly (159.6 ± 0.4 pc) |
| Absolute magnitude (MV) | 5.78[1] |
| Position (relative to CoRoT-7A)[3] | |
| Component | CoRoT-7B |
| Epoch of observation | 2021 |
| Angular distance | 75.7″ |
| Observed separation (projected) | 12160 AU |
| Details | |
| CoRoT-7A | |
| Mass | 0.91 ± 0.03[1] M☉ |
| Radius | 0.82 ± 0.04[1] R☉ |
| Surface gravity (log g) | 4.47 ± 0.10[1] cgs |
| Temperature | 5250 ± 60[1] K |
| Metallicity | [M/H] = 0.12 ± 0.06[1] |
| Rotation | ~23 days[4] |
| Rotational velocity (v sin i) | <3.5[1] km/s |
| Age | (1.2–2.3) × 109[1] years |
| CoRoT-7B | |
| Mass | 0.23[3] M☉ |
| Other designations | |
2MASS J06434947-0103468, TYC 4799-1733-1, GSC 04799-01733 | |
| CoRoT-7A: Gaia EDR3 3107267177757848576 | |
| CoRoT-7B: Gaia EDR3 3107267212116737792 | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
| Extrasolar Planets Encyclopaedia | data |
Coordinates: 
06h 43m 49.0s, −01° 03′ 46.0″
CoRoT-7 (TYC 4799-1733-1) is a binary star system.
Stellar components
CoRoT-7A
The primary, CoRoT-7A is a G-type main sequence star, slightly smaller, cooler, and younger than the Sun. It has an apparent magnitude of 11.67, fainter than Proxima Centauri (mag. 11.05), the nearest star to the Sun. This star is approximately 520 light-years away from the Solar System[2] in the constellation Monoceros (the Unicorn).[5]
CoRoT-7B
The comoving companion CoRoT-7B was discovered in 2021. It is a red dwarf star.[3]
Location and properties
The star is located in the LRa01 field of view of the CoRoT spacecraft. It is about 500 light years from Earth. According to the project website, this field is in the Monoceros constellation.[5] Published data[6] lists the stellar properties as being a G9V yellow dwarf with a temperature of 5250 K, a radius of about 82% of the Sun and a mass of about 91% of the Sun.[1] But other sources have listed it as a (K0V) orange dwarf.[7] The metallicity is 0.12 ± 0.06. The star is estimated to be about 150 parsecs away and with an age in the range 1.2 – 2.3 billion years, is younger than our own star which has an age of 4.6 billion years.[1] The rotation period of the star, inferred by the lightcurve obtained by CoRoT, is around 23 days.
Planetary system
The primary star is orbited by the super-Earth exoplanets CoRoT-7b and CoRoT-7c, both discovered in 2009.[4] A third planet CoRoT-7d, initially proposed in a 2010 study,[8] was confirmed in 2022.[9] The discovery of the inner planet was made using the transit method by the CoRoT program. CoRoT-7b is notable for its relatively small size, compared to other exoplanets known at the time.[10]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 6.056±0.653 M⊕ | 0.0172 ± 0.00029 | 0.853592±0.000000587 | 0 | 80.98±0.51° | 1.528±0.065 R⊕ |
| c | 13.289±0.689 M⊕ | 0.046 | 3.697±0.005 | 0 | — | — |
| d | 17.142±2.552 M⊕ | 0.08 | 8.966±1.546 | 0 | — | — |
Because of their closeness to their star, these exoplanets cannot be seen in a telescope; only their gravitational effect can be detected by the Doppler effect on the star's electromagnetic spectrum (radial velocity method), as well as transits of planet b. This star was reported to have stellar activity, making the confirmation process for CoRoT-7b more difficult. In fact, mass estimates are affected by large uncertainty due to stellar activity that perturbs the radial velocity measurements needed to "weigh" the planets.[4][11][12]
CoRoT-7d was first proposed by A. P. Hatzes et al in 2010 by the radial velocity method.[8] The existence of CoRoT-7d was disputed by a 2014 study, which concluded that the radial velocity signal was more likely to be an artifact of the stellar rotation.[12] However, a 2022 study provided strong evidence for the existence of this planet,[9] and it is now listed as a confirmed planet in the NASA Exoplanet Archive.[13] CoRoT-7d's mass is 17.1 times that of Earth, but its volume and diameter are unknown. One year on CoRoT-7d would be equivalent to 8.966 days on Earth.[9]
References
- ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 1.11 1.12 1.13 Léger, A et al. (2009). "Transiting exoplanets from the CoRoT space mission VIII. CoRoT-7b: the first Super-Earth with measured radius". Astronomy and Astrophysics 506 (1): 287–302. doi:10.1051/0004-6361/200911933. Bibcode: 2009A&A...506..287L. https://www.aanda.org/articles/aa/full_html/2009/40/aa11933-09/aa11933-09.html.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode: 2021A&A...649A...1G. Gaia EDR3 record for this source at VizieR.
- ↑ 3.0 3.1 3.2 3.3 Fontanive, Clémence; Daniella Bardalez Gagliuffi (2021), "The Census of Exoplanets in Visual Binaries: population trends from a volume-limited Gaia DR2 and literature search", Frontiers in Astronomy and Space Sciences 8: 16, doi:10.3389/fspas.2021.625250, Bibcode: 2021FrASS...8...16F
- ↑ 4.0 4.1 4.2 4.3 Queloz, D. et al. (2009). "The CoRoT-7 planetary system: two orbiting Super-Earths". Astronomy and Astrophysics 506 (1): 303. doi:10.1051/0004-6361/200913096. Bibcode: 2009A&A...506..303Q. http://www.aanda.org/articles/aa/pdf/forth/aa13096-09.pdf. Also available from exoplanet.eu
- ↑ 5.0 5.1 Rouan (February 3, 2009). "CoRoT-exo-7b Has CoRoT discovered the first transiting Super-Earth around a main sequence star?". CoRoT Symposium—Paris. Archived from the original on July 20, 2011. https://web.archive.org/web/20110720154622/http://www.colloquium.eu/congres/09COROT/docs/slides/03mardi/11h/d_rouan/alancer.pdf. Retrieved 2009-07-05.
- ↑ Bruntt; Deleuil; Fridlund; Alonso; Bouchy; Hatzes; Mayor; Moutou et al. (2010). "Improved stellar parameters of CoRoT-7". Astronomy and Astrophysics 519: A51. doi:10.1051/0004-6361/201014143. Bibcode: 2010A&A...519A..51B.
- ↑ Jean Schneider. "Star : CoRoT-7". Extrasolar Planets Encyclopaedia. http://exoplanet.eu/star.php?st=CoRoT-7. Retrieved 2009-12-26.
- ↑ 8.0 8.1 Hatzes; Dvorak; Wuchterl; Guterman; Hartmann; Fridlund; Gandolfi; Guenther et al. (2010). "An Investigation into the Radial Velocity Variations of CoRoT-7". Astronomy and Astrophysics 520: A93. doi:10.1051/0004-6361/201014795. Bibcode: 2010A&A...520A..93H.
- ↑ 9.0 9.1 9.2 9.3 Anna John, Ancy; Collier Cameron, Andrew; Wilson, Thomas G. (2022), "The impact of two non-transiting planets and stellar activity on mass determinations for the super-Earth CoRoT-7b", Monthly Notices of the Royal Astronomical Society 515 (3): 3975–3995, doi:10.1093/mnras/stac1814
- ↑ "Super-Earth found! The smallest transiting extrasolar planet ever discovered". Paris Observatory. February 2009. Archived from the original on 2009-09-23. https://web.archive.org/web/20090923014043/http://www.obspm.fr/actual/nouvelle/feb09/exo7.en.shtml. Retrieved 2009-02-04.
- ↑ "CoRoT-Exo-7b: Confirming the first transiting rocky planet". http://ssc.spitzer.caltech.edu/warmmission/scheduling/approvedprograms/ddt/534.txt. Retrieved 2010-08-23.
- ↑ 12.0 12.1 Haywood, R. D. (September 2014). "Planets and stellar activity: hide and seek in the CoRoT-7 system". Monthly Notices of the Royal Astronomical Society 443 (3): 2517–2531. doi:10.1093/mnras/stu1320. Bibcode: 2014MNRAS.443.2517H.
- ↑ "CoRoT-7". https://exoplanetarchive.ipac.caltech.edu/overview/CoRoT-7. Retrieved 31 July 2022.
External links
- Schilling, Govert (2009-02-03). "CoRoT Finds the Smallest Exoplanet Yet". Sky & Telescope. http://www.skyandtelescope.com/news/38820797.html. Retrieved 2009-02-04.
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