Temperature
5409 K
5374 to 5409
←Back to Stellar Hosts
Stellar HostProfile
HD 154088
K1V • 18.27 pc
Records
12
literature rows
Planets
1
system count
References
13
distinct source labels
HD: HD 154088HIP: HIP 83541TIC: TIC 20856917
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: Turnbull 2015 • System source: TICv8
Mass
0.92 Msun
0.88 to 0.94
Radius
0.95 Rsun
0.95 to 0.98
Age
12.48 Gyr
8 to 12.48
Luminosity
-0.14 log(Lsun)
-0.16 to -0.13
Distance
18.27 pc
single adopted value
Spectral Type
K1V
Multiple classifications reported
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.95 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HD 154088
0.95 R☉
System Layout
Known planets
1 planets linked to this host
HD 154088 b
Radial Velocity
◌
Discovery
2021
Period
18.56 days
Radius
—
Mass
6.60 M⊕
Eq. Temp
—
HD 154088 and Its Planet
HD 154088 is a K1V star, a K-type main-sequence dwarf, located 59.6 light-years from Earth. It is older and somewhat less massive and smaller than the Sun: its age is 12.5 billion years, its mass is 0.92 solar masses, its radius is 0.95 solar radii, and its temperature is 5410 K. The star's reported mass and radius estimates are smaller than the Sun's, and its reported temperature is cooler than the Sun's.
One planet orbits this star. HD 154088 b was discovered in 2021 using the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion. The planet's minimum mass is 6.6 Earth masses, larger than Earth's, and its orbital period is 18.6 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
12
Stellar refs
12
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
Spectral Typedisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | G5 | 18.27 | Cannon & Pickering 1918 | TICv8 |
| — | 0.92 | 0.95 | 12.48 | — | — | 18.27 | Takeda et al. 2007 | TICv8 |
| 5409 | 0.92 | 0.95 | 12.48 | -0.14 | K1V | 18.27 | Turnbull 2015 | TICv8 |
| 5391.8 | 0.94 | 0.98 | — | -0.14 | — | 18.27 | TICv8 | TICv8 |
| 5374 | 0.91 | — | 8 | -0.13 | K0 IV-V | 18.27 | Unger et al. 2021 | TICv8 |
| — | — | — | — | — | — | 18.27 | Valenti & Fischer 2005 | TICv8 |
| 5374 | 0.88 | — | — | -0.16 | — | 18.27 | Sousa et al. 2008 | TICv8 |
| — | — | — | — | — | — | 18.27 | Henry et al. 1996 | TICv8 |
| — | — | — | — | — | — | 18.27 | Wright et al. 2004 | TICv8 |
| — | — | — | — | — | K1 V | 18.27 | Michigan Catalog, Vol. 3 | TICv8 |
| — | — | — | — | — | — | 18.27 | Nidever et al. 2002 | TICv8 |
| — | — | — | — | — | K0 IV-V | 18.27 | Gray et al. 2006 | TICv8 |