Temperature
5750 K
5443.8 to 5750
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Stellar HostProfile
Kepler-41
G2 V • 1093.1 pc
Records
19
literature rows
Planets
1
system count
References
20
distinct source labels
TIC: TIC 271042217
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: Bonomo et al. 2015 • System source: TICv8
Mass
1.15 Msun
0.90 to 1.15
Radius
1.29 Rsun
0.89 to 1.45
Age
4.40 Gyr
0.65 to 6.20
Distance
1093.1 pc
single adopted value
Spectral Type
G2 V
Multiple classifications reported
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.29 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-41
1.29 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-41 b
Transit
◌
Discovery
2011
Period
1.86 days
Radius
14.46 R⊕
Mass
178.0 M⊕
Eq. Temp
1790 K
Kepler-41 and Its Jupiter-Like Planet
Kepler-41 is a Sun-like G-type dwarf star located 3570 light-years away. The star is 4.4 billion years old and has a mass of 1.15 solar masses, a radius of 1.29 solar radii, and a temperature of 5750 K. Its reported mass and radius estimates are both larger than the Sun's. One planet orbits this host.
That planet, Kepler-41 b, is a Jupiter-like world discovered by the transit method in 2011. It has a mass of 178 Earth masses and a radius of 14.5 Earth radii, both larger than Earth's corresponding values. Its mean density is 0.324 g/cm³. Kepler-41 b completes an orbit in 1.86 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
19
Stellar refs
19
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
Spectral Typedisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5750 | 1.15 | 1.29 | 4.40 | — | — | 1093.1 | Bonomo et al. 2017 | TICv8 |
| 5750 | 1.15 | 1.29 | 4.40 | — | G2 V | 1093.1 | Bonomo et al. 2015 | TICv8 |
| 5651.8 | 1 | 1.41 | — | 0.26 | — | 1093.1 | TICv8 | TICv8 |
| 5585 | — | 0.94 | — | — | — | 1093.1 | Latham et al. 2005 | TICv8 |
| 5585 | — | 0.94 | — | — | — | 1093.1 | Q1-Q6 KOI Table | TICv8 |
| 5657 | 0.90 | 0.95 | — | — | — | 1093.1 | Q1-Q16 KOI Table | TICv8 |
| 5620 | 1.12 | 1.02 | — | — | — | 1093.1 | Esteves et al. 2015 | TICv8 |
| 5657 | 0.90 | 0.95 | — | — | — | 1093.1 | Q1-Q17 DR24 KOI Table | TICv8 |
| — | — | — | — | — | — | 1093.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5730 | 0.98 | 0.97 | 4.37 | — | — | 1093.1 | Morton et al. 2016 | TICv8 |
| 5443.8 | — | 1.45 | — | 0.22 | — | 1093.1 | Gaia DR2 | TICv8 |
| 5657 | 0.90 | 0.95 | — | — | — | 1093.1 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5651.8 | — | 1.41 | — | — | — | 1093.1 | ExoFOP | TICv8 |
| 5731 | 0.94 | 0.89 | 3.50 | — | — | 1093.1 | Q1-Q8 KOI Table | TICv8 |
| 5585 | — | 0.94 | — | — | — | 1093.1 | Batalha et al. 2013 | TICv8 |
| 5660 | 0.94 | 0.94 | 6.20 | — | — | 1093.1 | Southworth 2012 | TICv8 |
| 5620 | 1.12 | 1.02 | 0.65 | — | G6 V | 1093.1 | Santerne et al. 2011 | TICv8 |
| 5660 | — | 1.34 | — | — | — | 1093.1 | Berger et al. 2018 | TICv8 |
| 5657 | 0.90 | 0.95 | — | — | — | 1093.1 | Q1-Q12 KOI Table | TICv8 |