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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.

Astronomical data · SIMBAD

Object type
Pl
Distance
2,509 light-years
Coordinates
RA 102.0799° · Dec -3.1021°
View on SIMBAD →

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 sections
Contents
  • 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.