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Stellar HostProfile

Kepler-33

Unclassified star • 1209.2 pc

Records

46

literature rows

Planets

5

system count

References

19

distinct source labels

TIC: TIC 158935283

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: Lissauer et al. 2012 • System source: TICv8

Temperature

5904 K

5823.7 to 6018

38 values • 6 distinct

Mass

1.29 Msun

1.07 to 1.29

33 values • 7 distinct

Radius

1.82 Rsun

1.29 to 1.82

40 values • 9 distinct

Age

4.27 Gyr

4.24 to 4.79

8 values • 4 distinct

Luminosity

0.56 log(Lsun)

0.49 to 0.56

3 values • 3 distinct

Distance

1209.2 pc

single adopted value

46 values • 1 distinct

Planets

5

Stable across source rows

5

Scale Comparison

Radius against the Sun

Current adopted radius: 1.82 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

Kepler-33

1.82 R☉

System Layout

Known planets

5 planets linked to this host

◌

Discovery

2011

Period

5.67 days

Radius

1.74 R⊕

Mass

—

Eq. Temp

—

◌

Discovery

2011

Period

13.18 days

Radius

3.20 R⊕

Mass

—

Eq. Temp

—

◌

Discovery

2011

Period

21.78 days

Radius

5.35 R⊕

Mass

—

Eq. Temp

—

◌

Discovery

2011

Period

31.78 days

Radius

4.02 R⊕

Mass

—

Eq. Temp

—

◌

Discovery

2011

Period

41.03 days

Radius

4.46 R⊕

Mass

—

Eq. Temp

—

Kepler-33 and Its Five Planets

Kepler-33 is a star located 3940 light-years away. It is 4.27 billion years old, has a mass of 1.29 solar masses, and a radius of 1.82 solar radii. Its reported mass and radius estimates are larger than the Sun’s, and its temperature of 5900 K is hotter than the Sun’s. Five planets are known to orbit this host.

All five planets were discovered by transit in 2011. Kepler-33 b is a Super-Earth with a radius of 1.74 Earth radii and an orbital period of 5.67 days. Kepler-33 c is Neptune-like, with a radius of 3.2 Earth radii and an orbital period of 13.2 days. Kepler-33 d is Jupiter-like, with a radius of 5.35 Earth radii and an orbital period of 21.8 days. Kepler-33 e is also Jupiter-like, with a radius of 4.02 Earth radii and an orbital period of 31.8 days. Kepler-33 f is likewise Jupiter-like, with a radius of 4.46 Earth radii and an orbital period of 41 days.

Each planet’s reported radius estimate is larger than Earth’s. Among the listed planets, Kepler-33 b has the shortest year by reported estimates and the smallest radius. Kepler-33 f has the longest year and the second-largest radius. Kepler-33 c has the second-shortest year and the second-smallest radius, while Kepler-33 d has the largest radius. Kepler-33 e has the second-longest year by reported estimates.

Provenance

Underlying measurements and references

Evidence Summary

Rows

46

Stellar refs

18

System refs

1

Distancestable

46 values • 1 distinct

Parallaxstable

46 values • 1 distinct

Temperaturedisputed

38 values • 6 distinct

Massdisputed

33 values • 7 distinct

Radiusdisputed

40 values • 9 distinct

Agedisputed

8 values • 4 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

35 values • 6 distinct

Metallicitydisputed

25 values • 6 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
59001.101.69———1209.2Q1-Q17 DR25 KOI TableTICv8
5904—1.82———1209.2Q1-Q6 KOI TableTICv8
59001.101.69———1209.2Q1-Q17 DR25 KOI TableTICv8
5823.7—1.72—0.49—1209.2Gaia DR2TICv8
59001.101.69———1209.2Q1-Q17 DR25 KOI TableTICv8
59041.291.824.270.56—1209.2Lissauer et al. 2012TICv8
—1.101.69———1209.2Hadden et al. 2014TICv8
59041.291.824.24——1209.2Q1-Q8 KOI TableTICv8
59001.101.69———1209.2Q1-Q16 KOI TableTICv8
5904—1.82———1209.2Q1-Q6 KOI TableTICv8
59001.101.69———1209.2Q1-Q12 KOI TableTICv8
5933—1.29———1209.2Latham et al. 2005TICv8
59041.291.824.24——1209.2Q1-Q8 KOI TableTICv8
59001.101.69———1209.2Q1-Q12 KOI TableTICv8
59001.101.69———1209.2Q1-Q17 DR24 KOI TableTICv8
59001.101.69———1209.2Q1-Q16 KOI TableTICv8
59001.101.69———1209.2Q1-Q17 DR25 KOI TableTICv8
59041.291.824.24——1209.2Q1-Q8 KOI TableTICv8
59041.291.82———1209.2Batalha et al. 2013TICv8
——————1209.2Q1-Q17 DR25 Supplemental KOI TableTICv8
59001.101.69———1209.2Q1-Q17 DR24 KOI TableTICv8
60181.181.524.37——1209.2Morton et al. 2016TICv8
5904—1.82———1209.2Q1-Q6 KOI TableTICv8
——————1209.2Q1-Q17 DR25 Supplemental KOI TableTICv8
59001.101.69———1209.2Q1-Q16 KOI TableTICv8
5904—1.82———1209.2Q1-Q6 KOI TableTICv8
59001.101.69———1209.2Q1-Q17 DR24 KOI TableTICv8
59001.101.69———1209.2Q1-Q16 KOI TableTICv8
5904—1.82———1209.2Q1-Q6 KOI TableTICv8
——————1209.2Q1-Q17 DR25 Supplemental KOI TableTICv8
59001.101.69———1209.2Q1-Q17 DR25 KOI TableTICv8
—1.10————1209.2Hadden & Lithwick 2017TICv8
59041.291.824.24——1209.2Q1-Q8 KOI TableTICv8
59041.071.71—0.51—1209.2TICv8TICv8
59001.101.69———1209.2Q1-Q16 KOI TableTICv8
——————1209.2Q1-Q17 DR25 Supplemental KOI TableTICv8
59001.101.69———1209.2Q1-Q12 KOI TableTICv8
59001.101.69———1209.2Q1-Q12 KOI TableTICv8
59001.101.69———1209.2Q1-Q17 DR24 KOI TableTICv8
——————1209.2Q1-Q17 DR25 Supplemental KOI TableTICv8
5947—1.66———1209.2Berger et al. 2018TICv8
59001.101.69———1209.2Q1-Q12 KOI TableTICv8
59001.101.69———1209.2Q1-Q17 DR24 KOI TableTICv8
—1.101.69———1209.2Hadden & Lithwick 2016TICv8
59471.211.614.79——1209.2Fulton & Petigura 2018TICv8
59041.291.824.24——1209.2Q1-Q8 KOI TableTICv8