Temperature
6761 K
6680 to 6915
Unclassified star • 601.3 pc
Records
17
literature rows
Planets
2
system count
References
14
distinct source labels
Approximate color
from effective temperature
Canonical Summary
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
Temperature
6761 K
6680 to 6915
Mass
1.46 Msun
1.35 to 1.71
Radius
1.74 Rsun
1.38 to 2.60
Age
1.66 Gyr
1.41 to 1.66
Distance
601.3 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 1.74 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-880
1.74 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2016
Period
7.71 days
Radius
2.66 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2023
Period
11.81 days
Radius
2.87 R⊕
Mass
—
Eq. Temp
1407 K
Kepler-880 is a star 1960 light-years away with two known planets. The host is 1.46 solar masses, 1.74 solar radii, and a temperature of 6760 K, all larger or hotter than the Sun, with an age of 1.66 billion years.
Both planets were found by the transit method, which detects the small dip in a star's brightness when a planet crosses in front of it. Kepler-880 b, discovered in 2016, is Neptune-like, with a radius of 2.66 Earth radii and an orbital period of 7.71 days. Kepler-880 c, discovered in 2023, is also Neptune-like, with a radius of 2.87 Earth radii and an orbital period of 11.8 days.
Among the listed planets, Kepler-880 b has the shortest year and the smallest radius by reported estimates, while Kepler-880 c has the longest year and the largest radius. Because a Neptune-like class extends to four times Earth's radius, both planets fit that size range.
Provenance
Evidence Summary
Rows
17
Stellar refs
13
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 6869.0 | — | 1.49 | — | 0.65 | — | 601.3 | Gaia DR2 | TICv8 |
| 6905 | 1.35 | 1.46 | 1.41 | — | — | 601.3 | Q1-Q8 KOI Table | TICv8 |
| 6680 | — | 1.38 | — | — | — | 601.3 | Latham et al. 2005 | TICv8 |
| 6900 | 1.71 | 2.60 | — | — | — | 601.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6680 | — | 1.47 | — | — | — | 601.3 | Q1-Q6 KOI Table | TICv8 |
| 6915 | 1.39 | 1.45 | — | — | — | 601.3 | Q1-Q16 KOI Table | TICv8 |
| 6819 | 1.47 | 1.54 | — | 0.67 | — | 601.3 | TICv8 | TICv8 |
| 6900 | 1.71 | 2.60 | — | — | — | 601.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6680 | — | 1.47 | — | — | — | 601.3 | Batalha et al. 2013 | TICv8 |
| — | — | — | — | — | — | 601.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| — | — | — | — | — | — | 601.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6915 | 1.39 | 1.45 | — | — | — | 601.3 | Q1-Q12 KOI Table | TICv8 |
| 6907 | — | 1.55 | — | — | — | 601.3 | Berger et al. 2018 | TICv8 |
| 6761 | 1.46 | 1.74 | 1.66 | — | — | 601.3 | Morton et al. 2016 | TICv8 |
| 6915 | 1.39 | 1.45 | — | — | — | 601.3 | Q1-Q12 KOI Table | TICv8 |
| 6915 | 1.39 | 1.45 | — | — | — | 601.3 | Q1-Q16 KOI Table | TICv8 |
| 6915 | 1.39 | 1.45 | — | — | — | 601.3 | Q1-Q17 DR24 KOI Table | TICv8 |