Temperature
5143 K
4950.3 to 5388
←Back to Stellar Hosts
Stellar HostProfile
Kepler-1024
Unclassified star • 1087.4 pc
Records
13
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 137349536
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
0.81 Msun
0.81 to 0.93
Radius
0.78 Rsun
0.72 to 0.87
Age
5.25 Gyr
single adopted value
Distance
1087.4 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.78 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1024
0.78 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1024 b
Transit
◌
Discovery
2016
Period
66.42 days
Radius
3.91 R⊕
Mass
—
Eq. Temp
—
Kepler-1024: A Distant Star and Its Neptune-Like Planet
Kepler-1024 is a star located 3550 light-years away. It is 5.25 billion years old, has a mass of 0.81 solar masses, a radius of 0.78 solar radii, and a temperature of 5140 K. Its mass and radius are both smaller than the Sun's, and its temperature is cooler than the Sun's. One planet is known to orbit this host.
That planet is Kepler-1024 b, a Neptune-like world discovered in 2016 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 3.91 Earth radii, larger than Earth's, and its orbital period is 66.4 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
13
Stellar refs
13
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5186 | — | 0.74 | — | — | — | 1087.4 | Latham et al. 2005 | TICv8 |
| — | — | — | — | — | — | 1087.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5186 | — | 0.72 | — | — | — | 1087.4 | Q1-Q6 KOI Table | TICv8 |
| 5387 | 0.84 | 0.76 | — | — | — | 1087.4 | Q1-Q17 DR24 KOI Table | TICv8 |
| 4950.3 | — | 0.87 | — | -0.38 | — | 1087.4 | Gaia DR2 | TICv8 |
| 5383 | 0.85 | 0.76 | — | — | — | 1087.4 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5242.7 | 0.90 | 0.81 | — | -0.35 | — | 1087.4 | TICv8 | TICv8 |
| 5143 | 0.81 | 0.78 | 5.25 | — | — | 1087.4 | Morton et al. 2016 | TICv8 |
| 5186 | 0.93 | 0.74 | — | — | — | 1087.4 | Q1-Q8 KOI Table | TICv8 |
| 5387 | 0.84 | 0.76 | — | — | — | 1087.4 | Q1-Q12 KOI Table | TICv8 |
| 5388 | — | 0.81 | — | — | — | 1087.4 | Berger et al. 2018 | TICv8 |
| 5387 | 0.84 | 0.76 | — | — | — | 1087.4 | Q1-Q16 KOI Table | TICv8 |
| 5186 | 0.81 | 0.72 | — | — | — | 1087.4 | Batalha et al. 2013 | TICv8 |