CoRoT-1 b
Sign in to saveCoRoT-1b (previously named CoRoT-Exo-1b) is a transiting extrasolar planet approximately 2,630 light-years away in the constellation of Monoceros. The planet was discovered orbiting the yellow dwarf star CoRoT-1 in May 2007. The planet was the first discovery by the French-led CoRoT Mission.
Astronomical data · SIMBAD
- Object type
- Pl
- Distance
- 2,509 light-years
- Coordinates
- RA 102.0799° · Dec -3.1021°
via SIMBAD · CDS Strasbourg
Key facts
- Planet.period
- d
- Planet.name
- CoRoT-1b
- Planet.image
- Exoplanet Comparison CoRoT-1 b.png
- Planet.caption
- Size comparison of CoRoT-1b with Jupiter.
- Planet.discoverer
- Barge et al.
- Planet.discovery_site
- France
- Planet.discovered
- 3 May 2007
- Planet.discovery_method
- Transit
- Planet.apsis
- astron
- Planet.semimajor
- AU
- Planet.star
- CoRoT-1
- Planet.single_temperature
- 1,898±50
via Wikipedia infobox
Exoplanet data
- Host star
- CoRoT-1
- Discovered
- 2008
- Discovered by
- CoRoT
- Orbital period
- 1.51 days
- Radius
- 16.70 × Earth
- Mass
- 327.35 × Earth
- Equilibrium temp
- 1898 K
- Distance
- 787.91 pc
via NASA Exoplanet Archive
~2 min read
Encyclopedic overview
6 sectionsContents
- Discovery
- Characteristics
- Observation of phases
- See also
- References
- External links
CoRoT-1b (previously named CoRoT-Exo-1b) is a transiting extrasolar planet approximately 2,630 light-years away in the constellation of Monoceros. The planet was discovered orbiting the yellow dwarf star CoRoT-1 in May 2007. The planet was the first discovery by the French-led CoRoT Mission.
==Discovery== CoRoT-1b was identified as the best planetary candidate from the CoRoT spacecraft initial run from February 6 to April 2, 2007. Follow-up photometry with the Wise Observatorys 1.0 m telescope and at the Canada–France–Hawaii Telescope eliminated many of the possible false positives for the transit signal. 9 radial velocity measurements of CoRoT-1 were made at Haute-Provence Observatory in March–April and October 2007 with the SOPHIE échelle spectrograph. The radial velocity data matched the CoRoT light curve and supported the planetary nature of CoRoT-1b and eliminated other possibilities such as background stars, grazing eclipsing binaries, or a triple system.
Excerpted from Wikipedia’s “CoRoT-1 b” article, available under the CC BY-SA 4.0 licence.