←Back to Stellar Hosts
Stellar HostProfile

HIP 74890

K1 III • 78.66 pc

Records

6

literature rows

Planets

1

system count

References

7

distinct source labels

HD: HD 135760HIP: HIP 74890TIC: TIC 148153804

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. 2025 • System source: TICv8

Temperature

4824 K

4824 to 4909

4 values • 3 distinct

Mass

1.31 Msun

1.31 to 1.74

2 values • 2 distinct

Radius

4.62 Rsun

4.45 to 5.77

4 values • 4 distinct

Age

4.41 Gyr

single adopted value

1 values • 1 distinct

Luminosity

1.02 log(Lsun)

1.02 to 1.21

3 values • 3 distinct

Distance

78.66 pc

single adopted value

6 values • 1 distinct

Spectral Type

K1 III

Multiple classifications reported

K1 III (2), K0 (1), K1 IIICNII (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 4.62 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HIP 74890

4.62 R☉

System Layout

Known planets

1 planets linked to this host

HIP 74890 b

Radial Velocity

◌

Discovery

2016

Period

822.3 days

Radius

—

Mass

762.8 M⊕

Eq. Temp

—

HIP 74890 and Its Planet

HIP 74890 is a K1 III star located 257 light-years away. It is 4.41 billion years old, with a mass of 1.31 solar masses, a radius of 4.62 solar radii, and a temperature of 4820 K. Its reported mass and radius estimates are larger than the Sun's, while its reported temperature is cooler than the Sun's. One planet is known to orbit this star.

That planet, HIP 74890 b, was discovered in 2016 through 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. HIP 74890 b has a minimum mass of 763 Earth masses, larger than Earth's and roughly 2.4 times Jupiter's mass. Its orbital period is 822 days.

Provenance

Underlying measurements and references

Evidence Summary

Rows

6

Stellar refs

6

System refs

1

Distancestable

6 values • 1 distinct

Parallaxstable

6 values • 1 distinct

Temperaturedisputed

4 values • 3 distinct

Massdisputed

2 values • 2 distinct

Radiusdisputed

4 values • 4 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

2 values • 2 distinct

Metallicitydisputed

3 values • 3 distinct

Spectral Typedisputed

4 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—————K1 IIICNII78.66Michigan Catalog, Vol. 2TICv8
4909—4.45———78.66TICv8TICv8
48241.314.624.411.02K1 III78.66Jenkins et al. 2025TICv8
4850—4.60—1.02—78.66Gaia DR2TICv8
48501.745.77—1.21K1 III78.66Jones et al. 2016TICv8
—————K078.66Cannon & Pickering 1918TICv8