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Stellar HostProfile

Kepler-1104

Unclassified star • 530.7 pc

Records

14

literature rows

Planets

1

system count

References

15

distinct source labels

TIC: TIC 27186509

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

6387 K

6216 to 6470

13 values • 8 distinct

Mass

1.22 Msun

1.18 to 1.33

9 values • 7 distinct

Radius

1.27 Rsun

1.20 to 1.47

13 values • 10 distinct

Age

2.04 Gyr

1.66 to 2.32

3 values • 3 distinct

Luminosity

0.50 log(Lsun)

0.49 to 0.51

2 values • 2 distinct

Distance

530.7 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-1104 b

Transit

Discovery

2016

Period

5.04 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 • 6 distinct

Metallicitydisputed

8 values • 6 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
63871.311.38530.7Q1-Q17 DR25 KOI TableTICv8
64521.221.20530.7Q1-Q17 DR24 KOI TableTICv8
64521.221.20530.7Q1-Q12 KOI TableTICv8
63321.470.49530.7Gaia DR2TICv8
6461.81.311.440.51530.7TICv8TICv8
64521.221.20530.7Q1-Q16 KOI TableTICv8
62161.25530.7Q1-Q6 KOI TableTICv8
63861.47530.7Berger et al. 2018TICv8
62161.22530.7Latham et al. 2005TICv8
64701.181.272.32530.7Q1-Q8 KOI TableTICv8
62161.211.25530.7Batalha et al. 2013TICv8
63861.331.451.66530.7Fulton & Petigura 2018TICv8
530.7Q1-Q17 DR25 Supplemental KOI TableTICv8
64171.301.412.04530.7Morton et al. 2016TICv8