Temperature
6273 K
6035 to 6407
←Back to Stellar Hosts
Stellar HostProfile
Kepler-410 A
Unclassified star • 147.5 pc
Records
16
literature rows
Planets
1
system count
References
17
distinct source labels
TIC: TIC 164458714HD: HD 175289
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: Van Eylen et al. 2014 • System source: TICv8
Mass
1.21 Msun
1.17 to 1.30
Radius
1.35 Rsun
1.34 to 1.51
Age
2.76 Gyr
2.76 to 3.40
Luminosity
0.43 log(Lsun)
0.43 to 0.46
Distance
147.5 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.35 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-410 A
1.35 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-410 A b
Transit
◌
Discovery
2013
Period
17.83 days
Radius
2.84 R⊕
Mass
—
Eq. Temp
—
Kepler-410 A and Its Neptune-Like Planet
Kepler-410 A is a star 481 light-years away with a mass of 1.21 solar masses and a radius of 1.35 solar radii. Its reported mass and radius estimates are larger than the Sun's, and its temperature of 6270 K is hotter than the Sun's. The star is 2.76 billion years old. One planet is known to orbit this host.
That planet, Kepler-410 A b, is Neptune-like. It was discovered in 2013 by the transit method, in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness. Its radius is 2.84 Earth radii, larger than Earth's, and it completes an orbit every 17.8 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
16
Stellar refs
16
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 147.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6304 | 1.24 | 1.43 | — | 0.46 | — | 147.5 | TICv8 | TICv8 |
| 6375 | 1.30 | 1.41 | — | — | — | 147.5 | Tsantaki et al. 2014 | TICv8 |
| 6341 | 1.22 | 1.35 | 2.82 | — | — | 147.5 | Morton et al. 2016 | TICv8 |
| 6325 | 1.24 | 1.36 | — | — | — | 147.5 | Q1-Q16 KOI Table | TICv8 |
| 6325 | 1.24 | 1.36 | — | — | — | 147.5 | Q1-Q12 KOI Table | TICv8 |
| 6170 | — | 1.36 | — | — | — | 147.5 | Batalha et al. 2013 | TICv8 |
| 6170 | — | 1.36 | — | — | — | 147.5 | Q1-Q6 KOI Table | TICv8 |
| 6273 | 1.21 | 1.35 | 2.76 | 0.43 | — | 147.5 | Van Eylen et al. 2014 | TICv8 |
| 6407 | 1.21 | 1.34 | — | — | — | 147.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6306 | — | 1.51 | — | — | — | 147.5 | Berger et al. 2018 | TICv8 |
| 6170 | 1.17 | 1.36 | 3.40 | — | — | 147.5 | Q1-Q8 KOI Table | TICv8 |
| 6035 | — | 1.37 | — | — | — | 147.5 | Latham et al. 2005 | TICv8 |
| 6304 | — | 1.43 | — | — | — | 147.5 | ExoFOP | TICv8 |
| 6325 | 1.24 | 1.36 | — | — | — | 147.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6374.7 | — | 1.38 | — | 0.45 | — | 147.5 | Gaia DR2 | TICv8 |