Temperature
5650 K
5650 to 5805
G5 IV/V • 90.54 pc
Records
12
literature rows
Planets
2
system count
References
13
distinct source labels
Approximate color
from effective temperature
Canonical Summary
Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.
Stellar source: Jenkins et al. 2017 • System source: TICv8
Temperature
5650 K
5650 to 5805
Mass
1.28 Msun
0.93 to 1.38
Radius
2.05 Rsun
1.82 to 2.14
Age
5 Gyr
0.16 to 5
Luminosity
0.58 log(Lsun)
0.51 to 0.64
Distance
90.54 pc
single adopted value
Spectral Type
G5 IV/V
Multiple classifications reported
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 2.05 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HD 48265
2.05 R☉
System Layout
2 planets linked to this host
Radial Velocity
Discovery
2008
Period
778.5 days
Radius
—
Mass
484.7 M⊕
Eq. Temp
—
Radial Velocity
Discovery
2026
Period
10418 days
Radius
—
Mass
1414.3 M⊕
Eq. Temp
—
HD 48265 is a G-type star 295 light-years away, and two planets have been reported around it. The star is classified as G5 IV/V, with an age of 5 billion years, a mass of 1.28 solar masses, and a radius of 2.05 solar radii. Its temperature is 5650 K. Its reported mass and radius are larger than the Sun's, while its reported temperature is cooler.
HD 48265 b was discovered in 2008 by the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion. Its minimum mass is 485 Earth masses, a lower bound on its true mass, and it is roughly 1.53 times Jupiter's mass. It completes an orbit in 779 days, the shortest year among the listed planets.
HD 48265 c was also found by radial velocity, with a discovery year of 2026. Its reported mass is 1410 Earth masses, roughly 4.45 times Jupiter's mass, and it orbits in 10400 days, the longest year among the listed planets.
Provenance
Evidence Summary
Rows
12
Stellar refs
12
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5733 | 1.31 | 1.90 | 4.20 | — | — | 90.54 | Barbato et al. 2018 | TICv8 |
| — | — | — | 0.16 | — | — | 90.54 | Sanz-Forcada et al. 2010 | TICv8 |
| — | — | — | — | — | G5 | 90.54 | Cannon & Pickering 1918 | TICv8 |
| 5789 | 1.22 | 1.82 | 4.56 | 0.51 | — | 90.54 | Jofré et al. 2015 | TICv8 |
| 5784.7 | 1.04 | 2.06 | — | 0.63 | — | 90.54 | TICv8 | TICv8 |
| 5650 | 1.28 | 2.05 | 5 | 0.58 | G5 IV/V | 90.54 | Jenkins et al. 2017 | TICv8 |
| 5798 | 1.21 | — | — | — | — | 90.54 | Mortier et al. 2013 | TICv8 |
| — | — | — | — | — | G5 IV/V | 90.54 | Michigan Catalog, Vol. 2 | TICv8 |
| — | 0.93 | — | — | — | G5 V | 90.54 | Minniti et al. 2009 | TICv8 |
| 5695 | — | 2.14 | — | 0.64 | — | 90.54 | Gaia DR2 | TICv8 |
| 5805 | 1.38 | — | — | — | G5 IV/V | 90.54 | Wu et al. 2026 | TICv8 |
| — | — | — | — | — | — | 90.54 | Nordstrom et al. 2004 | TICv8 |