Temperature
5500 K
5281 to 5506
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Stellar HostProfile
Kepler-1722
Unclassified star โข 772.3 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
TIC: TIC 360023124
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 โข System source: TICv8
Mass
0.86 Msun
0.86 to 0.94
Radius
0.80 Rsun
0.76 to 0.94
Distance
772.3 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.80 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
Kepler-1722
0.80 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1722 b
Transit
โ
Discovery
2021
Period
9.18 days
Radius
2.87 Rโ
Mass
โ
Eq. Temp
โ
Kepler-1722 b: A Neptune-like World in a Distant System
Kepler-1722 is a star located 2520 light-years away, with a reported mass of 0.859 solar masses - smaller than the Sun's - and a radius of 0.795 solar radii. Its reported temperature of 5500 K is cooler than the Sun's. One planet is known to orbit this host.
That planet, Kepler-1722 b, was discovered in 2021 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. Repeated dips help establish orbital periods. Kepler-1722 b completes an orbit every 9.18 days and has a reported radius of 2.87 Earth radii, larger than Earth's. This places it in the Neptune-like size class, which extends to 4 times Earth's radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
10
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 |
|---|---|---|---|---|---|---|---|---|
| 5406 | 0.94 | 0.94 | โ | -0.17 | โ | 772.3 | TICv8 | TICv8 |
| 5500 | 0.86 | 0.80 | โ | โ | โ | 772.3 | Q1-Q16 KOI Table | TICv8 |
| 5281 | โ | 0.83 | โ | โ | โ | 772.3 | Latham et al. 2005 | TICv8 |
| 5281 | โ | 0.76 | โ | โ | โ | 772.3 | Q1-Q6 KOI Table | TICv8 |
| 5500 | 0.86 | 0.80 | โ | โ | โ | 772.3 | Q1-Q12 KOI Table | TICv8 |
| 5506 | 0.90 | 0.80 | 1.40 | โ | โ | 772.3 | Q1-Q8 KOI Table | TICv8 |
| 5500 | 0.86 | 0.80 | โ | โ | โ | 772.3 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5281 | โ | 0.76 | โ | โ | โ | 772.3 | Batalha et al. 2013 | TICv8 |
| โ | โ | โ | โ | โ | โ | 772.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5506 | 0.88 | 0.79 | โ | โ | โ | 772.3 | Q1-Q17 DR25 KOI Table | TICv8 |