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Stellar HostProfile

Kepler-480

Unclassified star • 847.5 pc

Records

14

literature rows

Planets

1

system count

References

15

distinct source labels

TIC: TIC 27187218

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

6322 K

6231 to 6495

13 values • 8 distinct

Mass

1.20 Msun

1.19 to 1.25

8 values • 5 distinct

Radius

1.17 Rsun

0.87 to 1.44

13 values • 10 distinct

Age

2.34 Gyr

0.26 to 3.24

3 values • 3 distinct

Luminosity

0.47 log(Lsun)

0.46 to 0.48

2 values • 2 distinct

Distance

847.5 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-480 b

Transit

Discovery

2016

Period

4.92 days

Radius

2.78 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 • 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
62311.201.413.24847.5Fulton & Petigura 2018TICv8
62850.87847.5Latham et al. 2005TICv8
64951.191.17847.5Q1-Q12 KOI TableTICv8
847.5Q1-Q17 DR25 Supplemental KOI TableTICv8
62851.12847.5Batalha et al. 2013TICv8
64951.191.17847.5Q1-Q17 DR24 KOI TableTICv8
64851.201.140.26847.5Q1-Q8 KOI TableTICv8
6327.81.251.440.48847.5TICv8TICv8
62851.12847.5Q1-Q6 KOI TableTICv8
62361.221.38847.5Q1-Q17 DR25 KOI TableTICv8
63381.400.46847.5Gaia DR2TICv8
64951.191.17847.5Q1-Q16 KOI TableTICv8
62311.44847.5Berger et al. 2018TICv8
63221.251.342.34847.5Morton et al. 2016TICv8