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Stellar HostProfile

Kepler-674

Unclassified star • 342.3 pc

Records

14

literature rows

Planets

1

system count

References

15

distinct source labels

TIC: TIC 48528770

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

4082 K

3741 to 4215

12 values • 7 distinct

Mass

0.58 Msun

0.47 to 0.65

7 values • 5 distinct

Radius

0.56 Rsun

0.45 to 0.76

12 values • 9 distinct

Age

3.97 Gyr

3.31 to 13.90

3 values • 3 distinct

Luminosity

-0.89 log(Lsun)

-0.91 to -0.88

2 values • 2 distinct

Distance

342.3 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-674 b

Transit

Discovery

2016

Period

2.24 days

Radius

1.32 R⊕

Mass

Eq. Temp

685 K

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

12 values • 7 distinct

Massdisputed

7 values • 5 distinct

Radiusdisputed

12 values • 9 distinct

Agedisputed

3 values • 3 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

10 values • 7 distinct

Metallicitydisputed

6 values • 4 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
41350.650.69-0.91342.3TICv8TICv8
37410.470.45342.3Q1-Q16 KOI TableTICv8
37410.470.45342.3Q1-Q17 DR24 KOI TableTICv8
40820.54342.3Q1-Q6 KOI TableTICv8
41490.66342.3Berger et al. 2018TICv8
40820.61342.3Latham et al. 2005TICv8
3996.30.76-0.88342.3Gaia DR2TICv8
37410.470.45342.3Q1-Q12 KOI TableTICv8
42150.580.5513.90342.3Q1-Q8 KOI TableTICv8
41490.580.56342.3Q1-Q17 DR25 KOI TableTICv8
342.3Q1-Q17 DR25 Supplemental KOI TableTICv8
40820.54342.3Batalha et al. 2013TICv8
3.97342.3Gaidos et al. 2024TICv8
41920.600.573.31342.3Morton et al. 2016TICv8