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Stellar HostProfile

HIP 111909

K1 III • 88.08 pc

Records

2

literature rows

Planets

2

system count

References

3

distinct source labels

HIP: HIP 111909TIC: TIC 161173454

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

4891 K

4867 to 4891

2 values • 2 distinct

Mass

1.28 Msun

single adopted value

1 values • 1 distinct

Radius

4.53 Rsun

4.34 to 4.53

2 values • 2 distinct

Age

4.30 Gyr

single adopted value

1 values • 1 distinct

Luminosity

1.02 log(Lsun)

single adopted value

1 values • 1 distinct

Distance

88.08 pc

single adopted value

2 values • 1 distinct

Spectral Type

K1 III

Consistent across records

K1 III (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 4.53 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HIP 111909

4.53 R☉

System Layout

Known planets

2 planets linked to this host

HIP 111909 b

Radial Velocity

◌

Discovery

2025

Period

487.1 days

Radius

—

Mass

384.6 M⊕

Eq. Temp

—

HIP 111909 c

Radial Velocity

◌

Discovery

2025

Period

893.6 days

Radius

—

Mass

257.4 M⊕

Eq. Temp

—

Two Planets Orbiting HIP 111909

HIP 111909 is a K1 III star 287 light-years away with two known planets. The star is 4.3 billion years old and has 1.28 solar masses, 4.53 solar radii, and a temperature of 4890 K. Its reported mass and radius are larger than the Sun's, and its reported temperature is cooler than the Sun's.

HIP 111909 b was discovered in 2025 by radial velocity, a method that 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 385 Earth masses, a lower bound on its true mass, and an orbital period of 487 days. Its minimum mass is larger than Earth's and roughly 1.21 times Jupiter's mass. Among the listed planets, HIP 111909 b has the shortest year by reported estimates and the largest minimum mass.

HIP 111909 c was also discovered in 2025 by radial velocity. It has a minimum mass of 257 Earth masses, a lower bound on its true mass, and an orbital period of 894 days. Its minimum mass is larger than Earth's. Among the listed planets, HIP 111909 c has the longest year by reported estimates and the smallest 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

Agestable

1 values • 1 distinct

Luminositystable

1 values • 1 distinct

Surface Gravitystable

1 values • 1 distinct

Metallicitystable

1 values • 1 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
4867—4.34———88.08TICv8TICv8
48911.284.534.301.02K1 III88.08Jenkins et al. 2025TICv8