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Stellar HostProfile

K2-180

K2 V • 203.9 pc

Records

12

literature rows

Planets

1

system count

References

13

distinct source labels

TIC: TIC 366411016

Approximate color

from effective temperature

Canonical Summary

Adopted host values from all rows

Numeric fields use the median of non-null measurements. Disagreement stays visible through ranges, counts, and provenance.

Temperature

5358 K

5110 to 5375.5

9 values • 8 distinct

Mass

0.72 Msun

0.67 to 0.93

7 values • 6 distinct

Radius

0.69 Rsun

0.64 to 0.72

11 values • 9 distinct

Age

8.50 Gyr

7.50 to 9.50

2 values • 2 distinct

Luminosity

-0.44 log(Lsun)

-0.45 to -0.41

3 values • 3 distinct

Distance

203.9 pc

single adopted value

12 values • 1 distinct

Spectral Type

K2 V

Consistent across records

K2 V (1)

Planets

1

Stable across source rows

1

System Layout

Known planets

1 planets linked to this host

K2-180 b

Transit

Discovery

2018

Period

8.87 days

Radius

2.24 R⊕

Mass

11.44 M⊕

Eq. Temp

729 K

Provenance

Underlying measurements and references

Evidence Summary

Rows

12

Stellar refs

12

System refs

1

Distancestable

12 values • 1 distinct

Parallaxstable

12 values • 1 distinct

Temperaturedisputed

9 values • 8 distinct

Massdisputed

7 values • 6 distinct

Radiusdisputed

11 values • 9 distinct

Agedisputed

2 values • 2 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

8 values • 7 distinct

Metallicitydisputed

6 values • 6 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
53680.70203.9ExoFOPTICv8
51100.710.699.50K2 V203.9Korth et al. 2019TICv8
203.9Pope et al. 2016TICv8
53060.720.72203.9Castro-González et al. 2022TICv8
0.65203.9Petigura et al. 2018TICv8
53680.930.70-0.44203.9TICv8TICv8
0.69203.9Kruse et al. 2019TICv8
51660.670.64203.9Howard et al. 2025TICv8
53580.720.72203.9Livingston et al. 2018TICv8
53650.730.727.50-0.41203.9Thygesen et al. 2023TICv8
5375.50.69-0.45203.9Gaia DR2TICv8
52630.730.68203.9Mayo et al. 2018TICv8