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Stellar HostProfile

Kepler-886

Unclassified star • 711.3 pc

Records

14

literature rows

Planets

1

system count

References

15

distinct source labels

TIC: TIC 158215023

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

6122 K

5810 to 6352

13 values • 8 distinct

Mass

1.03 Msun

0.91 to 1.15

8 values • 5 distinct

Radius

1.04 Rsun

0.98 to 1.26

13 values • 10 distinct

Age

3.39 Gyr

0.76 to 6.76

3 values • 3 distinct

Luminosity

0.04 log(Lsun)

0.03 to 0.04

2 values • 2 distinct

Distance

711.3 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-886 b

Transit

Discovery

2016

Period

6.24 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

8 values • 5 distinct

Radiusdisputed

13 values • 10 distinct

Agedisputed

3 values • 3 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

10 values • 6 distinct

Metallicitydisputed

8 values • 6 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
711.3Q1-Q17 DR25 Supplemental KOI TableTICv8
63521.151.100.76711.3Q1-Q8 KOI TableTICv8
63341.031.04711.3Q1-Q16 KOI TableTICv8
60981.101.163.39711.3Morton et al. 2016TICv8
61221.07711.3Latham et al. 2005TICv8
58570.910.986.76711.3Fulton & Petigura 2018TICv8
5922.20.990.03711.3Gaia DR2TICv8
63341.031.04711.3Q1-Q12 KOI TableTICv8
5815.21.051.030.04711.3TICv8TICv8
58101.031.26711.3Q1-Q17 DR25 KOI TableTICv8
61221.04711.3Q1-Q6 KOI TableTICv8
63341.031.04711.3Q1-Q17 DR24 KOI TableTICv8
58570.99711.3Berger et al. 2018TICv8
61221.04711.3Batalha et al. 2013TICv8