Back to Stellar Hosts
Stellar HostProfile

Kepler-846

Unclassified star • 1127.1 pc

Records

13

literature rows

Planets

1

system count

References

14

distinct source labels

TIC: TIC 399911496

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

5677 K

5375 to 5787

12 values • 7 distinct

Mass

0.94 Msun

0.93 to 0.97

7 values • 5 distinct

Radius

0.85 Rsun

0.63 to 0.91

12 values • 9 distinct

Age

2.39 Gyr

0.40 to 4.37

2 values • 2 distinct

Luminosity

-0.22 log(Lsun)

-0.22 to -0.22

2 values • 2 distinct

Distance

1127.1 pc

single adopted value

13 values • 1 distinct

Planets

1

Stable across source rows

1

System Layout

Known planets

1 planets linked to this host

Kepler-846 b

Transit

Discovery

2016

Period

19.81 days

Radius

2.20 R⊕

Mass

Eq. Temp

629 K

Provenance

Underlying measurements and references

Evidence Summary

Rows

13

Stellar refs

13

System refs

1

Distancestable

13 values • 1 distinct

Parallaxstable

13 values • 1 distinct

Temperaturedisputed

12 values • 7 distinct

Massdisputed

7 values • 5 distinct

Radiusdisputed

12 values • 9 distinct

Agedisputed

2 values • 2 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
53750.89-0.221127.1Gaia DR2TICv8
57750.930.841127.1Q1-Q17 DR25 KOI TableTICv8
55600.791127.1Batalha et al. 2013TICv8
57870.940.851127.1Q1-Q12 KOI TableTICv8
54940.960.86-0.221127.1TICv8TICv8
57810.970.860.401127.1Q1-Q8 KOI TableTICv8
55600.631127.1Latham et al. 2005TICv8
55790.940.914.371127.1Morton et al. 2016TICv8
57870.940.851127.1Q1-Q16 KOI TableTICv8
1127.1Q1-Q17 DR25 Supplemental KOI TableTICv8
55600.791127.1Q1-Q6 KOI TableTICv8
57870.940.851127.1Q1-Q17 DR24 KOI TableTICv8
57810.831127.1Berger et al. 2018TICv8