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Stellar HostProfile

HD 94890

K0 III • 61.70 pc

Records

2

literature rows

Planets

2

system count

References

3

distinct source labels

TIC: TIC 158543228HD: HD 94890HIP: HIP 53502

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: Fontanet et al. 2025 • System source: TICv8

Temperature

4867 K

4865.8 to 4867

2 values • 2 distinct

Mass

1.74 Msun

single adopted value

1 values • 1 distinct

Radius

10.71 Rsun

10.71 to 10.91

2 values • 2 distinct

Luminosity

1.76 log(Lsun)

single adopted value

1 values • 1 distinct

Distance

61.70 pc

single adopted value

2 values • 1 distinct

Spectral Type

K0 III

Consistent across records

K0 III (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 10.71 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 94890

10.71 R☉

System Layout

Known planets

2 planets linked to this host

HD 94890 b

Radial Velocity

◌

Discovery

2025

Period

824.6 days

Radius

—

Mass

677.0 M⊕

Eq. Temp

—

HD 94890 c

Radial Velocity

◌

Discovery

2025

Period

2492.2 days

Radius

—

Mass

2831.9 M⊕

Eq. Temp

—

HD 94890 and Its Two Known Planets

HD 94890 is a K0 III star located 201 light-years away. Its reported mass is 1.74 solar masses, its reported radius is 10.7 solar radii, and its reported temperature is 4870 K. The star’s mass and radius are larger than the Sun’s, while its temperature is cooler. Two planets are known to orbit this host.

HD 94890 b was discovered in 2025 by the radial velocity method, which measures the wobble a planet’s gravity induces in its star’s motion; repeated wobbles reveal the planet and its orbital period. The planet has a minimum mass of 677 Earth masses, larger than Earth’s and roughly 2.13 times Jupiter’s mass. Its orbital period is 825 days, the shortest year among the listed planets.

HD 94890 c was also discovered in 2025 by radial velocity. It has a minimum mass of 2830 Earth masses, larger than Earth’s and roughly 8.91 times Jupiter’s mass. Its orbital period is 2490 days, the longest year among the listed planets. Among the listed planets, HD 94890 b has the smallest minimum mass and HD 94890 c has the largest minimum mass.

Provenance

Underlying measurements and references

Evidence Summary

Rows

2

Stellar refs

2

System refs

1

Distancestable

2 values • 1 distinct

Parallaxstable

2 values • 1 distinct

Temperaturedisputed

2 values • 2 distinct

Massstable

1 values • 1 distinct

Radiusdisputed

2 values • 2 distinct

Luminositystable

1 values • 1 distinct

Surface Gravitystable

1 values • 1 distinct

Metallicitydisputed

2 values • 2 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
48671.7410.71—1.76K0 III61.70Fontanet et al. 2025TICv8
4865.8—10.91———61.70TICv8TICv8