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Stellar HostProfile

Kepler-531

Unclassified star • 252.8 pc

Records

14

literature rows

Planets

1

system count

References

15

distinct source labels

TIC: TIC 243272677

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

4883 K

4784.5 to 4935

13 values • 7 distinct

Mass

0.74 Msun

0.72 to 0.79

8 values • 5 distinct

Radius

0.75 Rsun

0.70 to 1.50

13 values • 9 distinct

Age

7.76 Gyr

2.75 to 9.30

3 values • 3 distinct

Luminosity

-0.57 log(Lsun)

-0.58 to -0.55

2 values • 2 distinct

Distance

252.8 pc

single adopted value

14 values • 1 distinct

Planets

1

Stable across source rows

1

System Layout

Known planets

1 planets linked to this host

Kepler-531 b

Transit

Discovery

2016

Period

29.88 days

Radius

Mass

Eq. Temp

Provenance

Underlying measurements and references

Evidence Summary

Rows

14

Stellar refs

14

System refs

1

Distancestable

14 values • 1 distinct

Parallaxstable

14 values • 1 distinct

Temperaturedisputed

13 values • 7 distinct

Massdisputed

8 values • 5 distinct

Radiusdisputed

13 values • 9 distinct

Agedisputed

3 values • 3 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

10 values • 5 distinct

Metallicitydisputed

8 values • 5 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
48830.720.75252.8Q1-Q16 KOI TableTICv8
48830.720.75252.8Q1-Q17 DR24 KOI TableTICv8
4784.50.770.77-0.55252.8TICv8TICv8
4924.80.70-0.58252.8Gaia DR2TICv8
49350.73252.8Berger et al. 2018TICv8
48690.71252.8Q1-Q6 KOI TableTICv8
49350.790.732.75252.8Fulton & Petigura 2018TICv8
48830.720.75252.8Q1-Q12 KOI TableTICv8
48830.720.75252.8Q1-Q17 DR25 KOI TableTICv8
48690.71252.8Batalha et al. 2013TICv8
48690.750.719.30252.8Q1-Q8 KOI TableTICv8
252.8Q1-Q17 DR25 Supplemental KOI TableTICv8
47941.50252.8Latham et al. 2005TICv8
48930.780.757.76252.8Morton et al. 2016TICv8