Temperature
6087 K
5719 to 6087
←Back to Stellar Hosts
Stellar HostProfile
Kepler-1485
Unclassified star • 615.7 pc
Records
16
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 273690208
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: Morton et al. 2016 • System source: TICv8
Mass
1.11 Msun
1.06 to 1.11
Radius
1.12 Rsun
1.09 to 1.31
Age
2.51 Gyr
2.51 to 5.25
Distance
615.7 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.12 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1485
1.12 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1485 b
Transit
◌
Discovery
2016
Period
19.92 days
Radius
1.47 R⊕
Mass
—
Eq. Temp
—
Kepler-1485 and Its Earth-like Planet
Kepler-1485 is a star 2010 light-years away with one known planet. The host star is 2.51 billion years old and has a mass of 1.11 solar masses, a radius of 1.12 solar radii, and a temperature of 6090 K. Its reported mass and radius estimates are larger than the Sun's, and its reported temperature is hotter than the Sun's.
The planet Kepler-1485 b was discovered in 2016 by the transit method, which identifies a planet when it passes in front of its star from our viewpoint and causes a small dip in observed brightness; repeated dips help establish orbital periods. Kepler-1485 b is classified as Earth-like, a size class for planets within 1.5 times Earth's radius. It has an orbital period of 19.9 days and a radius of 1.47 Earth radii, and its reported radius estimate is larger than Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
16
Stellar refs
11
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 |
|---|---|---|---|---|---|---|---|---|
| 6053 | 1.07 | 1.09 | — | — | — | 615.7 | Q1-Q12 KOI Table | TICv8 |
| 6053 | 1.07 | 1.09 | — | — | — | 615.7 | Q1-Q16 KOI Table | TICv8 |
| 6087 | 1.11 | 1.12 | 2.51 | — | — | 615.7 | Morton et al. 2016 | TICv8 |
| 5980 | 1.07 | 1.25 | 5.25 | — | — | 615.7 | Fulton & Petigura 2018 | TICv8 |
| 6053 | 1.07 | 1.09 | — | — | — | 615.7 | Q1-Q16 KOI Table | TICv8 |
| — | — | — | — | — | — | 615.7 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5719 | — | 1.31 | — | — | — | 615.7 | Latham et al. 2005 | TICv8 |
| 5980 | — | 1.26 | — | — | — | 615.7 | Berger et al. 2018 | TICv8 |
| 6053 | 1.07 | 1.09 | — | — | — | 615.7 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6053 | 1.07 | 1.09 | — | — | — | 615.7 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6047 | 1.06 | 1.09 | — | — | — | 615.7 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5719 | — | 1.28 | — | 0.20 | — | 615.7 | Gaia DR2 | TICv8 |
| 6053 | 1.07 | 1.09 | — | — | — | 615.7 | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | 615.7 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6047 | 1.06 | 1.09 | — | — | — | 615.7 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5993 | 1.10 | 1.28 | — | 0.28 | — | 615.7 | TICv8 | TICv8 |