Temperature
5772 K
5700 to 5821
←Back to Stellar Hosts
Stellar HostProfile
HD 92788
Unclassified star • 34.65 pc
Records
19
literature rows
Planets
2
system count
References
20
distinct source labels
TIC: TIC 169248301HD: HD 92788HIP: HIP 52409
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: Ghezzi et al. 2010 • System source: TICv8
Mass
1.10 Msun
1.02 to 1.15
Radius
1.11 Rsun
1 to 1.16
Age
3.50 Gyr
1.16 to 3.50
Luminosity
0.09 log(Lsun)
0.02 to 0.10
Distance
34.65 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.11 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HD 92788
1.11 R☉
System Layout
Known planets
2 planets linked to this host
HD 92788 b
Radial Velocity
◌
Discovery
2000
Period
325.8 days
Radius
—
Mass
1195.0 M⊕
Eq. Temp
—
HD 92788 c
Radial Velocity
◌
Discovery
2019
Period
1.16e4 days
Radius
—
Mass
1166.4 M⊕
Eq. Temp
—
Two Planets Around the Sun-Like Star HD 92788
HD 92788 is a G-type main-sequence star 113 light-years away. Its spectral type is G5 V, and it is 3.5 billion years old. This host has two known planets. The star contains 1.1 solar masses, spans 1.11 solar radii, which is larger than the Sun's radius, and has a temperature of 5770 K.
The radial velocity method revealed both worlds. HD 92788 b was found in 2000. Its minimum mass is 1200 Earth masses, roughly 3.76 times Jupiter's mass, and it completes an orbit every 326 days, the shortest year among the listed planets. HD 92788 c was discovered in 2019, has a minimum mass of 1170 Earth masses, roughly 3.67 times Jupiter's mass, and takes 11600 days to orbit. It has both the longest year and the smallest minimum mass among the listed planets.
Provenance
Underlying measurements and references
Evidence Summary
Rows
19
Stellar refs
19
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 |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 34.65 | Nordstrom et al. 2004 | TICv8 |
| 5744 | 1.03 | — | — | 0.02 | — | 34.65 | Sousa et al. 2008 | TICv8 |
| 5738 | 1.15 | 1.11 | — | — | — | 34.65 | Stassun et al. 2017 | TICv8 |
| — | — | — | — | — | — | 34.65 | Valenti & Fischer 2005 | TICv8 |
| — | — | — | — | — | G6 V | 34.65 | Michigan Catalog, Vol. 5 | TICv8 |
| 5744 | 1.15 | 1.14 | 2.55 | — | G6 V | 34.65 | Rickman et al. 2019 | TICv8 |
| — | — | — | — | — | — | 34.65 | Nidever et al. 2002 | TICv8 |
| 5772 | 1.10 | 1.11 | 3.50 | 0.09 | — | 34.65 | Ghezzi et al. 2010 | TICv8 |
| 5821 | 1.12 | — | — | — | — | 34.65 | Santos et al. 2004 | TICv8 |
| 5821 | 1.10 | — | 2.10 | 0.02 | — | 34.65 | Mayor et al. 2004 | TICv8 |
| — | 1.08 | 1 | 1.16 | — | — | 34.65 | Takeda et al. 2007 | TICv8 |
| 5702.2 | 1.08 | 1.16 | — | — | — | 34.65 | Rosenthal et al. 2021 | TICv8 |
| 5700 | 1.02 | 1.15 | — | 0.10 | — | 34.65 | TICv8 | TICv8 |
| 5820 | 1.10 | — | — | — | — | 34.65 | Santos et al. 2003 | TICv8 |
| 5744 | 1.03 | — | — | — | — | 34.65 | Wittenmyer et al. 2019 | TICv8 |
| 5722 | — | 1.14 | — | 0.10 | — | 34.65 | Gaia DR2 | TICv8 |
| 5754 | 1.06 | 1.05 | — | — | G5 V | 34.65 | Fischer et al. 2001 | TICv8 |
| — | — | — | — | — | G5 | 34.65 | Cannon & Pickering 1918 | TICv8 |
| — | — | — | — | — | — | 34.65 | Wright et al. 2004 | TICv8 |