Temperature
6088 K
6020 to 6161
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Stellar HostProfile
Kepler-1725
Unclassified star • 558.7 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 377908774
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: Fulton & Petigura 2018 • System source: TICv8
Mass
1.11 Msun
1.05 to 1.18
Radius
1.10 Rsun
1.03 to 1.13
Age
1.66 Gyr
0.89 to 1.66
Distance
558.7 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.10 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
Kepler-1725
1.10 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1725 b
Transit
◌
Discovery
2021
Period
16.72 days
Radius
2.81 R⊕
Mass
—
Eq. Temp
—
Kepler-1725 and Its Neptune-Like Planet
Kepler-1725 is a star 1820 light-years away with an age of 1.66 billion years. Its mass is 1.11 solar masses, its radius is 1.1 solar radii, and its temperature is 6090 K. The star's reported mass and radius estimates are larger than the Sun's, and its reported temperature is hotter than the Sun's. One planet orbits this host.
That planet is Kepler-1725 b, a Neptune-like world discovered by transit in 2021. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Kepler-1725 b has an orbital period of 16.7 days, the time it takes to complete one orbit. Its radius is 2.81 Earth radii, larger than Earth's. In size classification, a Neptune-like planet reaches 4 times Earth's radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
11
Stellar refs
11
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositystable
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 6108 | 1.13 | 1.03 | — | — | — | 558.7 | Q1-Q16 KOI Table | TICv8 |
| 6129 | — | 1.13 | — | — | — | 558.7 | Q1-Q6 KOI Table | TICv8 |
| 6088 | 1.11 | 1.10 | 1.66 | — | — | 558.7 | Fulton & Petigura 2018 | TICv8 |
| 6129 | — | 1.13 | — | — | — | 558.7 | Batalha et al. 2013 | TICv8 |
| 6161 | 1.17 | 1.10 | — | 0.20 | — | 558.7 | TICv8 | TICv8 |
| 6129 | 1.18 | 1.13 | 0.89 | — | — | 558.7 | Q1-Q8 KOI Table | TICv8 |
| — | — | — | — | — | — | 558.7 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6020 | 1.05 | 1.08 | — | — | — | 558.7 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6108 | 1.13 | 1.03 | — | — | — | 558.7 | Q1-Q12 KOI Table | TICv8 |
| 6065 | — | 1.07 | — | — | — | 558.7 | Latham et al. 2005 | TICv8 |
| 6108 | 1.13 | 1.03 | — | — | — | 558.7 | Q1-Q17 DR24 KOI Table | TICv8 |