Temperature
6086 K
5838 to 6229
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Stellar HostProfile
Kepler-1755
Unclassified star • 982.4 pc
Records
16
literature rows
Planets
1
system count
References
11
distinct source labels
TIC: TIC 239225129
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: Q1-Q12 KOI Table • System source: TICv8
Mass
1.00 Msun
1.00 to 1.20
Radius
0.92 Rsun
0.88 to 1.18
Distance
982.4 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.92 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1755
0.92 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1755 b
Transit
◌
Discovery
2021
Period
24.81 days
Radius
5.92 R⊕
Mass
—
Eq. Temp
—
Kepler-1755 and Its Jupiter-Like Planet
Kepler-1755 is a star 3200 light-years away with one known planet. The host star has a mass of 1 solar masses, a radius of 0.921 solar radii, and a temperature of 6090 K, which is hotter than the Sun's.
The planet Kepler-1755 b is Jupiter-like, meaning its radius exceeds 4 times Earth's radius. It was 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; repeated dips help establish orbital periods. Kepler-1755 b has an orbital period of 24.8 days and a radius of 5.92 Earth radii, larger than Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
16
Stellar refs
10
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositystable
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5838 | — | 0.89 | — | — | — | 982.4 | Latham et al. 2005 | TICv8 |
| 5838 | — | 0.88 | — | — | — | 982.4 | Batalha et al. 2013 | TICv8 |
| — | — | — | — | — | — | 982.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6086 | 1.00 | 0.92 | — | — | — | 982.4 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6086 | 1.00 | 0.92 | — | — | — | 982.4 | Q1-Q16 KOI Table | TICv8 |
| 6086 | 1.00 | 0.92 | — | — | — | 982.4 | Q1-Q12 KOI Table | TICv8 |
| 5838 | — | 0.88 | — | — | — | 982.4 | Q1-Q6 KOI Table | TICv8 |
| 6106 | 1.07 | 0.98 | 0.30 | — | — | 982.4 | Q1-Q8 KOI Table | TICv8 |
| 6086 | 1.00 | 0.92 | — | — | — | 982.4 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6086 | 1.00 | 0.92 | — | — | — | 982.4 | Q1-Q16 KOI Table | TICv8 |
| 6086 | 1.00 | 0.92 | — | — | — | 982.4 | Q1-Q12 KOI Table | TICv8 |
| 6086 | 1.00 | 0.92 | — | — | — | 982.4 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6229 | 1.20 | 1.18 | — | 0.27 | — | 982.4 | TICv8 | TICv8 |
| 6106 | 1.07 | 0.98 | 0.30 | — | — | 982.4 | Q1-Q8 KOI Table | TICv8 |
| — | — | — | — | — | — | 982.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6086 | 1.00 | 0.92 | — | — | — | 982.4 | Q1-Q17 DR24 KOI Table | TICv8 |