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Stellar HostProfile

K2-357

Unclassified star • 517.7 pc

Records

2

literature rows

Planets

1

system count

References

3

distinct source labels

TIC: TIC 293459761

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: Castro-González et al. 2022 • System source: TICv8

Temperature

5794 K

5664 to 5794

2 values • 2 distinct

Mass

0.98 Msun

0.98 to 1.01

2 values • 2 distinct

Radius

1 Rsun

0.96 to 1

2 values • 2 distinct

Distance

517.7 pc

single adopted value

2 values • 1 distinct

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 1 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

K2-357

1 R☉

System Layout

Known planets

1 planets linked to this host

K2-357 b

Transit

◌

Discovery

2021

Period

16.35 days

Radius

3.72 R⊕

Mass

—

Eq. Temp

735 K

K2-357 and Its Neptune-like Planet

K2-357 is a star 1,690 light-years away with one known planet. The host star has 0.98 solar masses and 1 solar radius, and a temperature of 5,790 K.

The planet K2-357 b was discovered in 2021 by the transit method. It is Neptune-like, with a radius of 3.72 Earth radii, and its reported radius estimate is larger than Earth's. It completes an orbit every 16.3 days.

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

Massdisputed

2 values • 2 distinct

Radiusdisputed

2 values • 2 distinct

Luminositystable

1 values • 1 distinct

Surface Gravitydisputed

2 values • 2 distinct

Metallicitystable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
56641.010.96—-0.07—517.7TICv8TICv8
57940.981———517.7Castro-González et al. 2022TICv8