←Back to Stellar Hosts
Stellar HostProfile

K2-331

Unclassified star • 211.4 pc

Records

3

literature rows

Planets

2

system count

References

4

distinct source labels

TIC: TIC 46296576

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: de Leon et al. 2021 • System source: TICv8

Temperature

5994 K

5797 to 6010

3 values • 3 distinct

Mass

1.10 Msun

1.04 to 1.10

2 values • 2 distinct

Radius

1.06 Rsun

1.04 to 1.06

3 values • 3 distinct

Distance

211.4 pc

single adopted value

3 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.06 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

K2-331

1.06 R☉

System Layout

Known planets

2 planets linked to this host

K2-331 b

Transit

◌

Discovery

2021

Period

9.40 days

Radius

1.79 R⊕

Mass

—

Eq. Temp

909 K

K2-331 c

Transit

◌

Discovery

2021

Period

23.00 days

Radius

2.72 R⊕

Mass

—

Eq. Temp

673 K

K2-331: A Distant Star With Two Known Planets

K2-331 is a star located 690 light-years away. It has 1.1 solar masses, a radius of 1.06 solar radii, and a temperature of 5990 K, making it larger, wider, and hotter than the Sun by reported estimates. Two planets are known to orbit this host.

K2-331 b is a Super-Earth discovered by transit in 2021. It completes an orbit in 9.4 days and has a radius of 1.79 Earth radii, larger than Earth's. Its year is the shortest among the listed planets, and its radius is the smallest.

K2-331 c is a Neptune-like planet, also found by transit in 2021. Its orbital period is 23 days, and its radius is 2.72 Earth radii, larger than Earth's. Among the listed planets, it has the longest year and the largest radius.

A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Repeated dips help establish orbital periods.

Provenance

Underlying measurements and references

Evidence Summary

Rows

3

Stellar refs

3

System refs

1

Distancestable

3 values • 1 distinct

Parallaxstable

3 values • 1 distinct

Temperaturedisputed

3 values • 3 distinct

Massdisputed

2 values • 2 distinct

Radiusdisputed

3 values • 3 distinct

Luminositystable

1 values • 1 distinct

Surface Gravitydisputed

3 values • 3 distinct

Metallicitystable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
59941.101.06———211.4de Leon et al. 2021TICv8
57971.041.06—0.06—211.4TICv8TICv8
6010—1.04———211.4Yu et al. 2018TICv8