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Stellar HostProfile

HD 48265

G5 IV/V • 90.54 pc

Records

12

literature rows

Planets

2

system count

References

13

distinct source labels

HD: HD 48265HIP: HIP 31895TIC: TIC 255781806

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: Jenkins et al. 2017 • System source: TICv8

Temperature

5650 K

5650 to 5805

7 values • 7 distinct

Mass

1.28 Msun

0.93 to 1.38

7 values • 7 distinct

Radius

2.05 Rsun

1.82 to 2.14

5 values • 5 distinct

Age

5 Gyr

0.16 to 5

4 values • 4 distinct

Luminosity

0.58 log(Lsun)

0.51 to 0.64

4 values • 4 distinct

Distance

90.54 pc

single adopted value

12 values • 1 distinct

Spectral Type

G5 IV/V

Multiple classifications reported

G5 IV/V (3), G5 (1), G5 V (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 2.05 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 48265

2.05 R☉

System Layout

Known planets

2 planets linked to this host

HD 48265 b

Radial Velocity

◌

Discovery

2008

Period

778.5 days

Radius

—

Mass

484.7 M⊕

Eq. Temp

—

HD 48265 c

Radial Velocity

◌

Discovery

2026

Period

10418 days

Radius

—

Mass

1414.3 M⊕

Eq. Temp

—

HD 48265 and Its Two Known Planets

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

Underlying measurements and references

Evidence Summary

Rows

12

Stellar refs

12

System refs

1

Distancestable

12 values • 1 distinct

Parallaxstable

12 values • 1 distinct

Temperaturedisputed

7 values • 7 distinct

Massdisputed

7 values • 7 distinct

Radiusdisputed

5 values • 5 distinct

Agedisputed

4 values • 4 distinct

Luminositydisputed

4 values • 4 distinct

Surface Gravitydisputed

6 values • 6 distinct

Metallicitydisputed

7 values • 6 distinct

Spectral Typedisputed

5 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
57331.311.904.20——90.54Barbato et al. 2018TICv8
———0.16——90.54Sanz-Forcada et al. 2010TICv8
—————G590.54Cannon & Pickering 1918TICv8
57891.221.824.560.51—90.54Jofré et al. 2015TICv8
5784.71.042.06—0.63—90.54TICv8TICv8
56501.282.0550.58G5 IV/V90.54Jenkins et al. 2017TICv8
57981.21————90.54Mortier et al. 2013TICv8
—————G5 IV/V90.54Michigan Catalog, Vol. 2TICv8
—0.93———G5 V90.54Minniti et al. 2009TICv8
5695—2.14—0.64—90.54Gaia DR2TICv8
58051.38———G5 IV/V90.54Wu et al. 2026TICv8
——————90.54Nordstrom et al. 2004TICv8