Temperature
5933 K
5806 to 5933
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Stellar HostProfile
Kepler-464
Unclassified star • 667.6 pc
Records
14
literature rows
Planets
1
system count
References
15
distinct source labels
TIC: TIC 27239696
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
1.21 Msun
1.06 to 1.26
Radius
1.59 Rsun
1.01 to 1.69
Age
4.90 Gyr
3.80 to 4.90
Distance
667.6 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.59 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-464
1.59 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-464 b
Transit
◌
Discovery
2016
Period
7.26 days
Radius
3.30 R⊕
Mass
—
Eq. Temp
—
Kepler-464 and Its Neptune-Like Planet
Kepler-464 is a star 2180 light-years away with one known planet. The host star is estimated to be 4.9 billion years old and has a mass of 1.21 solar masses, a radius of 1.59 solar radii, and a temperature of 5930 K. Its reported mass, radius, and temperature estimates are each larger or hotter than the Sun's corresponding values.
The planet Kepler-464 b was discovered by transit in 2016. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Repeated dips help establish orbital periods. Kepler-464 b completes an orbit every 7.26 days and has a radius of 3.3 Earth radii, larger than Earth's. Its Neptune-like class places it within the radius range of that size category, which extends to 4 times Earth's radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
14
Stellar refs
14
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 |
|---|---|---|---|---|---|---|---|---|
| 5919 | — | 1.27 | — | — | — | 667.6 | Q1-Q6 KOI Table | TICv8 |
| 5919 | 1.16 | 1.27 | 3.80 | — | — | 667.6 | Q1-Q8 KOI Table | TICv8 |
| 5873.7 | 1.06 | 1.69 | — | 0.48 | — | 667.6 | TICv8 | TICv8 |
| 5862 | 1.20 | 1.59 | — | — | — | 667.6 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5919 | — | 1.27 | — | — | — | 667.6 | Batalha et al. 2013 | TICv8 |
| 5933 | 1.21 | 1.59 | 4.90 | — | — | 667.6 | Morton et al. 2016 | TICv8 |
| 5920 | — | 1.62 | — | — | — | 667.6 | Berger et al. 2018 | TICv8 |
| 5862 | 1.20 | 1.59 | — | — | — | 667.6 | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | 667.6 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5920 | 1.26 | 1.60 | 4.07 | — | — | 667.6 | Fulton & Petigura 2018 | TICv8 |
| 5806 | — | 1.69 | — | 0.47 | — | 667.6 | Gaia DR2 | TICv8 |
| 5858 | 1.13 | 1.55 | — | — | — | 667.6 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5816 | — | 1.01 | — | — | — | 667.6 | Latham et al. 2005 | TICv8 |
| 5862 | 1.20 | 1.59 | — | — | — | 667.6 | Q1-Q16 KOI Table | TICv8 |