Temperature
6440 K
6037 to 6440
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Stellar HostProfile
CoRoT-11
F6 V • 655.0 pc
Records
8
literature rows
Planets
1
system count
References
9
distinct source labels
TIC: TIC 110178537
Approximate color
from effective temperature
Canonical Summary
Adopted host values from one source row
Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.
Stellar source: Gandolfi et al. 2010 • System source: TICv8
Mass
1.27 Msun
1.23 to 1.56
Radius
1.37 Rsun
1.33 to 1.59
Age
2 Gyr
single adopted value
Distance
655.0 pc
single adopted value
Spectral Type
F6 V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.37 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
CoRoT-11
1.37 R☉
System Layout
Known planets
1 planets linked to this host
CoRoT-11 b
Transit
◌
Discovery
2010
Period
2.99 days
Radius
16.03 R⊕
Mass
740.5 M⊕
Eq. Temp
1657 K
CoRoT-11 and Its Jupiter-Like Planet
CoRoT-11 is a star 2140 light-years away with a spectral type of F6 V, an F-type main-sequence dwarf. It is 2 billion years old and has a mass of 1.27 solar masses, a radius of 1.37 solar radii, and a temperature of 6440 K. Each of these reported estimates is larger or hotter than the corresponding value for the Sun. One planet orbits this host.
That planet is CoRoT-11 b, a Jupiter-like world discovered by transit in 2010. Its radius of 16 Earth radii is larger than Earth's, and its mass of 741 Earth masses is also larger than Earth's and roughly 2.33 times Jupiter's mass. Its mean density is 0.991 g/cm³, 0.18 times Earth's. CoRoT-11 b completes an orbit in 2.99 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
8
Stellar refs
8
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
Spectral Typestable
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 6440 | 1.27 | 1.37 | 2 | — | — | 655.0 | Bonomo et al. 2017 | TICv8 |
| 6440 | 1.26 | 1.37 | 2 | — | — | 655.0 | Southworth 2011 | TICv8 |
| — | 1.23 | 1.33 | 2 | — | — | 655.0 | Gandolfi et al. 2012 | TICv8 |
| 6343 | — | 1.59 | — | — | — | 655.0 | ExoFOP | TICv8 |
| 6343 | 1.56 | 1.36 | — | — | — | 655.0 | Tsantaki et al. 2014 | TICv8 |
| 6343 | 1.26 | 1.59 | — | 0.56 | — | 655.0 | TICv8 | TICv8 |
| 6440 | 1.27 | 1.37 | 2 | — | F6 V | 655.0 | Gandolfi et al. 2010 | TICv8 |
| 6037 | — | 1.41 | — | 0.38 | — | 655.0 | Gaia DR2 | TICv8 |