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Stellar HostProfile

Kepler-1258

Unclassified star • 717.6 pc

Records

14

literature rows

Planets

1

system count

References

15

distinct source labels

TIC: TIC 279918915

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

5825 K

5627 to 6069

13 values • 8 distinct

Mass

1.01 Msun

0.83 to 1.12

9 values • 7 distinct

Radius

0.96 Rsun

0.83 to 1.66

13 values • 10 distinct

Age

3.89 Gyr

0.40 to 13.49

3 values • 3 distinct

Luminosity

0.09 log(Lsun)

0.09 to 0.09

2 values • 2 distinct

Distance

717.6 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-1258 b

Transit

Discovery

2016

Period

0.98 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 • 8 distinct

Massdisputed

9 values • 7 distinct

Radiusdisputed

13 values • 10 distinct

Agedisputed

3 values • 3 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

10 values • 7 distinct

Metallicitydisputed

8 values • 6 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
717.6Q1-Q17 DR25 Supplemental KOI TableTICv8
56270.831.1013.49717.6Fulton & Petigura 2018TICv8
58251.121.66717.6Q1-Q17 DR25 KOI TableTICv8
60601.010.93717.6Q1-Q12 KOI TableTICv8
581810.89717.6Batalha et al. 2013TICv8
56271.12717.6Berger et al. 2018TICv8
60691.060.960.40717.6Q1-Q8 KOI TableTICv8
60601.010.93717.6Q1-Q16 KOI TableTICv8
60601.010.93717.6Q1-Q17 DR24 KOI TableTICv8
58180.83717.6Latham et al. 2005TICv8
5830.51.080.09717.6Gaia DR2TICv8
5761.01.031.120.09717.6TICv8TICv8
58180.89717.6Q1-Q6 KOI TableTICv8
58390.990.993.89717.6Morton et al. 2016TICv8