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Stellar HostProfile

KOI-351

Unclassified star • 848.3 pc

Records

49

literature rows

Planets

8

system count

References

19

distinct source labels

TIC: TIC 267667295

Approximate color

from effective temperature

Canonical Summary

Adopted host values from one source row

Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.

Stellar source: TICv8 • System source: TICv8

Temperature

6031.1 K

5970 to 6330

40 values • 8 distinct

Mass

1.12 Msun

0.97 to 1.24

35 values • 7 distinct

Radius

1.25 Rsun

0.94 to 1.29

40 values • 10 distinct

Luminosity

0.27 log(Lsun)

0.25 to 0.27

2 values • 2 distinct

Distance

848.3 pc

single adopted value

49 values • 1 distinct

Planets

8

Stable across source rows

8

Scale Comparison

Radius against the Sun

Current adopted radius: 1.25 R☉ • circles scaled linearly by radius

Sun

1.0 R☉ baseline

KOI-351

1.25 R☉

System Layout

Known planets

8 planets linked to this host

KOI-351 b

Transit

Discovery

2013

Period

7.01 days

Radius

1.31 R⊕

Mass

Eq. Temp

KOI-351 c

Transit

Discovery

2013

Period

8.72 days

Radius

1.19 R⊕

Mass

Eq. Temp

KOI-351 d

Transit

Discovery

2013

Period

59.74 days

Radius

2.87 R⊕

Mass

Eq. Temp

KOI-351 e

Transit

Discovery

2013

Period

91.94 days

Radius

2.66 R⊕

Mass

Eq. Temp

KOI-351 f

Transit

Discovery

2013

Period

124.9 days

Radius

2.88 R⊕

Mass

Eq. Temp

KOI-351 g

Transit

Discovery

2013

Period

210.7 days

Radius

Mass

15 M⊕

Eq. Temp

KOI-351 h

Transit

Discovery

2013

Period

331.6 days

Radius

Mass

203 M⊕

Eq. Temp

Discovery

2017

Period

14.45 days

Radius

1.32 R⊕

Mass

Eq. Temp

709 K

KOI-351 and Its Eight Worlds

KOI-351 is a star 2770 light-years away with a mass of 1.12 solar masses, a radius of 1.25 solar radii, and a temperature of 6030 K. Its mass and radius are larger than the Sun's, and its temperature is hotter than the Sun's. Eight planets are known to orbit it, all discovered by transit, the dimming of starlight as a planet crosses the star's face.

The two planets with the shortest orbital periods are Earth-like in size. KOI-351 b orbits every 7.01 days with a radius of 1.31 Earth radii, and KOI-351 c orbits every 8.72 days with a radius of 1.19 Earth radii. Both are larger than Earth, and among the listed planets b has the shortest year while c has the second-shortest. Kepler-90 i, also Earth-like, orbits every 14.4 days with a radius of 1.32 Earth radii, larger than Earth's.

Three Neptune-like planets follow. KOI-351 d orbits every 59.7 days with a radius of 2.87 Earth radii, KOI-351 e every 91.9 days with a radius of 2.66 Earth radii, and KOI-351 f every 125 days with a radius of 2.88 Earth radii. Each is larger than Earth.

The two planets with measured masses are among those with the longest orbital periods. KOI-351 g, with a mass of 15 Earth masses, orbits every 211 days, and KOI-351 h, with a mass of 203 Earth masses, orbits every 332 days. Both are more massive than Earth, and h has the longest year among the listed planets while g has the second-longest.

Provenance

Underlying measurements and references

Evidence Summary

Rows

49

Stellar refs

18

System refs

1

Distancestable

49 values • 1 distinct

Parallaxstable

49 values • 1 distinct

Temperaturedisputed

40 values • 8 distinct

Massdisputed

35 values • 7 distinct

Radiusdisputed

40 values • 10 distinct

Agedisputed

7 values • 2 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

36 values • 8 distinct

Metallicitydisputed

28 values • 6 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
848.3Q1-Q17 DR25 Supplemental KOI TableTICv8
848.3Q1-Q17 DR25 Supplemental KOI TableTICv8
60801.201.20848.3Santerne et al. 2016TICv8
61031.02848.3Q1-Q6 KOI TableTICv8
1.24848.3Shaw et al. 2025TICv8
60151.21848.3Berger et al. 2018TICv8
63301.141.070.53848.3Q1-Q8 KOI TableTICv8
6031.11.121.250.27848.3TICv8TICv8
62380.971.05848.3Q1-Q16 KOI TableTICv8
848.3Q1-Q17 DR25 Supplemental KOI TableTICv8
60151.111.193.55848.3Fulton & Petigura 2018TICv8
63301.141.070.53848.3Q1-Q8 KOI TableTICv8
848.3Q1-Q17 DR25 Supplemental KOI TableTICv8
59701.091.20848.3Q1-Q17 DR25 KOI TableTICv8
848.3Q1-Q17 DR25 Supplemental KOI TableTICv8
61031.02848.3Q1-Q6 KOI TableTICv8
62380.971.05848.3Q1-Q12 KOI TableTICv8
62380.971.05848.3Q1-Q12 KOI TableTICv8
59701.091.20848.3Q1-Q17 DR25 KOI TableTICv8
60151.121.29848.3Shallue & Vanderburg 2018TICv8
61031.02848.3Batalha et al. 2013TICv8
63301.141.070.53848.3Q1-Q8 KOI TableTICv8
61030.94848.3Latham et al. 2005TICv8
62380.971.05848.3Q1-Q12 KOI TableTICv8
848.3Q1-Q17 DR25 Supplemental KOI TableTICv8
63301.141.070.53848.3Q1-Q8 KOI TableTICv8
62380.971.05848.3Q1-Q12 KOI TableTICv8
59701.091.20848.3Q1-Q17 DR25 KOI TableTICv8
59701.091.20848.3Q1-Q17 DR25 KOI TableTICv8
62380.971.05848.3Q1-Q17 DR24 KOI TableTICv8
62380.971.05848.3Q1-Q16 KOI TableTICv8
63301.141.070.53848.3Q1-Q8 KOI TableTICv8
59701.091.20848.3Q1-Q17 DR25 KOI TableTICv8
60801.201.20848.3Cabrera et al. 2014TICv8
61031.02848.3Q1-Q6 KOI TableTICv8
62380.971.05848.3Q1-Q16 KOI TableTICv8
59701.091.20848.3Q1-Q17 DR25 KOI TableTICv8
63301.141.070.53848.3Q1-Q8 KOI TableTICv8
848.3Q1-Q17 DR25 Supplemental KOI TableTICv8
62380.971.05848.3Q1-Q12 KOI TableTICv8
62380.971.05848.3Q1-Q16 KOI TableTICv8
62380.971.05848.3Q1-Q16 KOI TableTICv8
62380.971.05848.3Q1-Q12 KOI TableTICv8
59871.240.25848.3Gaia DR2TICv8
62380.971.05848.3Q1-Q16 KOI TableTICv8
62380.971.05848.3Q1-Q16 KOI TableTICv8
62380.971.05848.3Q1-Q12 KOI TableTICv8
59701.091.20848.3Q1-Q17 DR25 KOI TableTICv8
1.11848.3Weiss et al. 2024TICv8