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Stellar HostProfile

HAT-P-13

G4 • 246.8 pc

Records

13

literature rows

Planets

2

system count

References

14

distinct source labels

TIC: TIC 20096620

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: Bakos et al. 2009 • System source: TICv8

Temperature

5653 K

5579.3 to 5720

8 values • 3 distinct

Mass

1.22 Msun

1.02 to 1.32

7 values • 4 distinct

Radius

1.56 Rsun

1.56 to 1.91

7 values • 4 distinct

Age

5 Gyr

3.50 to 6.59

4 values • 3 distinct

Luminosity

0.35 log(Lsun)

0.35 to 0.51

3 values • 3 distinct

Distance

246.8 pc

single adopted value

13 values • 1 distinct

Spectral Type

G4

Consistent across records

G4 (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.56 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HAT-P-13

1.56 R☉

System Layout

Known planets

2 planets linked to this host

HAT-P-13 b

Transit

◌

Discovery

2009

Period

2.92 days

Radius

14.26 R⊕

Mass

270.5 M⊕

Eq. Temp

—

HAT-P-13 c

Radial Velocity

◌

Discovery

2009

Period

446.3 days

Radius

—

Mass

4538.4 M⊕

Eq. Temp

—

HAT-P-13 and Its Two Known Planets

HAT-P-13 is a star located 805 light-years away with a spectral type of G4. It has an age of 5 billion years, a mass of 1.22 solar masses, and a radius of 1.56 solar radii. Its reported temperature is 5650 K, cooler than the Sun's, while its mass and radius estimates are both larger than the Sun's. Two planets are known to orbit this host.

HAT-P-13 b is a Jupiter-like planet discovered by the transit method in 2009. Its radius is 14.3 Earth radii, larger than Earth's, and its mass is 270 Earth masses, also larger than Earth's. Its mean density is 0.514 g/cm³, 0.0933 times Earth's. It completes an orbit in 2.92 days, the shortest year among the listed planets by reported estimates.

HAT-P-13 c was discovered by radial velocity in 2009, the same year as its companion. Radial velocity measures the wobble a planet's gravity induces in its star's motion. Its minimum mass is 4540 Earth masses, larger than Earth's and roughly 14.3 times Jupiter's mass. It orbits in 446 days, the longest year among the listed planets by reported estimates.

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

8 values • 3 distinct

Massdisputed

7 values • 4 distinct

Radiusdisputed

7 values • 4 distinct

Agedisputed

4 values • 3 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

6 values • 4 distinct

Metallicitydisputed

7 values • 3 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—1.321.763.50——246.8Southworth et al. 2012TICv8
—1.321.76———246.8Buhler et al. 2016TICv8
5653—————246.8Turner et al. 2016TICv8
5653—————246.8Yalçınkaya et al. 2024TICv8
—1.21—6.59——246.8Maxted et al. 2015TICv8
57201.021.83—0.51—246.8TICv8TICv8
5720—1.83———246.8ExoFOPTICv8
—1.32————246.8Knutson et al. 2014TICv8
56531.221.5650.35G4246.8Bakos et al. 2009TICv8
——————246.8Winn et al. 2010TICv8
5579.3—1.91—0.50—246.8Gaia DR2TICv8
56531.221.565——246.8Bonomo et al. 2017TICv8
5653—————246.8Sada & Ramón-Fox 2016TICv8