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Stellar HostProfile

Kepler-556

Unclassified star • 674.6 pc

Records

14

literature rows

Planets

1

system count

References

15

distinct source labels

TIC: TIC 122449752

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

5732 K

5550 to 5957

13 values • 8 distinct

Mass

1.00 Msun

0.89 to 1.03

8 values • 6 distinct

Radius

0.94 Rsun

0.91 to 1.00

13 values • 10 distinct

Age

4.17 Gyr

1 to 4.27

3 values • 3 distinct

Luminosity

-0.07 log(Lsun)

-0.10 to -0.05

2 values • 2 distinct

Distance

674.6 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-556 b

Transit

Discovery

2016

Period

11.72 days

Radius

2.07 R⊕

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 • 6 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
55500.890.95674.6Q1-Q17 DR25 KOI TableTICv8
5618.30.991.00-0.05674.6TICv8TICv8
57320.94674.6Latham et al. 2005TICv8
57320.91674.6Q1-Q6 KOI TableTICv8
674.6Q1-Q17 DR25 Supplemental KOI TableTICv8
5570.30.96-0.10674.6Gaia DR2TICv8
57320.91674.6Batalha et al. 2013TICv8
574010.984.17674.6Morton et al. 2016TICv8
59571.030.94674.6Q1-Q16 KOI TableTICv8
59571.030.94674.6Q1-Q12 KOI TableTICv8
59571.030.94674.6Q1-Q17 DR24 KOI TableTICv8
56410.920.914.27674.6Fulton & Petigura 2018TICv8
59341.010.921674.6Q1-Q8 KOI TableTICv8
56410.92674.6Berger et al. 2018TICv8