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Stellar HostProfile

HD 75898

G0 • 78.05 pc

Records

9

literature rows

Planets

2

system count

References

10

distinct source labels

HD: HD 75898HIP: HIP 43674TIC: TIC 302580456

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: Ment et al. 2018 • System source: TICv8

Temperature

5963 K

5963 to 6137

7 values • 6 distinct

Mass

1.26 Msun

1.09 to 1.43

6 values • 6 distinct

Radius

1.58 Rsun

1.55 to 1.65

5 values • 5 distinct

Age

3.56 Gyr

3.20 to 3.80

3 values • 3 distinct

Luminosity

0.46 log(Lsun)

0.46 to 0.50

3 values • 3 distinct

Distance

78.05 pc

single adopted value

9 values • 1 distinct

Spectral Type

G0

Multiple classifications reported

G0 (2), F8 V (1), G0 V (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.58 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 75898

1.58 R☉

System Layout

Known planets

2 planets linked to this host

HD 75898 b

Radial Velocity

◌

Discovery

2007

Period

422.8 days

Radius

—

Mass

810.5 M⊕

Eq. Temp

—

HD 75898 c

Radial Velocity

◌

Discovery

2024

Period

6717 days

Radius

—

Mass

2698.4 M⊕

Eq. Temp

—

HD 75898 and Its Two Known Planets

HD 75898 is a star 255 light-years away with a spectral type of G0. It hosts two known planets. The star is estimated to be 3.56 billion years old, with a mass of 1.26 solar masses and a radius of 1.58 solar radii. Its temperature is 5960 K, and its reported mass, radius, and temperature are all larger or hotter than the Sun's.

HD 75898 b was discovered in 2007 by the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion. It has a minimum mass of 810 Earth masses, a lower bound on its true mass that is larger than Earth's and roughly 2.55 times Jupiter's mass. Its orbital period is 423 days, the shortest year among the listed planets.

HD 75898 c was discovered in 2024 by radial velocity. Its mass is 2700 Earth masses, larger than Earth's and roughly 8.49 times Jupiter's mass. Its orbital period is 6720 days, the longest year among the listed planets.

Provenance

Underlying measurements and references

Evidence Summary

Rows

9

Stellar refs

9

System refs

1

Distancestable

9 values • 1 distinct

Parallaxstable

9 values • 1 distinct

Temperaturedisputed

7 values • 6 distinct

Massdisputed

6 values • 6 distinct

Radiusdisputed

5 values • 5 distinct

Agedisputed

3 values • 3 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

5 values • 5 distinct

Metallicitydisputed

6 values • 5 distinct

Spectral Typedisputed

4 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
59631.261.583.560.46G078.05Ment et al. 2018TICv8
60211.281.603.80—G0 V78.05Robinson et al. 2007TICv8
61371.25————78.05Santos et al. 2013TICv8
60611.431.55———78.05Stassun et al. 2017TICv8
61221.29—3.20—F8 V78.05Ruggieri et al. 2024TICv8
——————78.05Nordstrom et al. 2004TICv8
6005.9—1.63—0.50—78.05Gaia DR2TICv8
—————G078.05Cannon & Pickering 1918TICv8
59631.091.65—0.49—78.05TICv8TICv8