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Stellar HostProfile

HAT-P-1

Unclassified star • 159.0 pc

Records

15

literature rows

Planets

1

system count

References

16

distinct source labels

TIC: TIC 346338552

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. 2007 • System source: TICv8

Temperature

5975 K

5718 to 6076

13 values • 8 distinct

Mass

1.12 Msun

1.12 to 1.15

9 values • 5 distinct

Radius

1.15 Rsun

1.04 to 1.30

11 values • 9 distinct

Age

3.60 Gyr

2.10 to 3.60

5 values • 3 distinct

Luminosity

0.18 log(Lsun)

0.17 to 0.22

5 values • 4 distinct

Distance

159.0 pc

single adopted value

15 values • 1 distinct

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 1.15 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HAT-P-1

1.15 R☉

System Layout

Known planets

1 planets linked to this host

HAT-P-1 b

Transit

◌

Discovery

2006

Period

4.47 days

Radius

14.78 R⊕

Mass

166.9 M⊕

Eq. Temp

1322 K

HAT-P-1 b: A Jupiter-Like Planet Orbiting a Sun-Like Star

HAT-P-1 is a star located 519 light-years away with a spectral type of G0 V. It hosts one known planet. The star is estimated to be 3.6 billion years old, with a mass of 1.12 solar masses and a radius of 1.15 solar radii. Its temperature is 5980 K. The star's reported mass and radius estimates are larger than the Sun's, and its reported temperature is hotter than the Sun's.

The planet HAT-P-1 b is classified as Jupiter-like, meaning its radius exceeds four times Earth's radius. It was discovered in 2006 via the transit method, in which a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. HAT-P-1 b has a mass of 167 Earth masses and a radius of 14.8 Earth radii. Its mean density is 0.284 g/cm³, which is 0.0516 times Earth's. The planet completes an orbit every 4.47 days. Its reported radius and mass estimates are both larger than Earth's.

Provenance

Underlying measurements and references

Evidence Summary

Rows

15

Stellar refs

15

System refs

1

Distancestable

15 values • 1 distinct

Parallaxstable

15 values • 1 distinct

Temperaturedisputed

13 values • 8 distinct

Massdisputed

9 values • 5 distinct

Radiusdisputed

11 values • 9 distinct

Agedisputed

5 values • 3 distinct

Luminositydisputed

5 values • 4 distinct

Surface Gravitydisputed

9 values • 8 distinct

Metallicitydisputed

9 values • 4 distinct

Spectral Typedisputed

3 values • 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
6000—————159.0Wakeford et al. 2013TICv8
59751.131.112.10——159.0Southworth 2010TICv8
59801.151.17———159.0Nikolov et al. 2014TICv8
—————F8159.0AGK 3 CatalogTICv8
5975—————159.0Yalçınkaya et al. 2024TICv8
6051.21.131.18—0.22—159.0TICv8TICv8
59751.121.153.600.18—159.0Bakos et al. 2007TICv8
5980—————159.0Turner et al. 2016TICv8
6051.2—1.18———159.0ExoFOPTICv8
60671.121.153.600.18G0 V159.0Ment et al. 2018TICv8
5718—1.30—0.21—159.0Gaia DR2TICv8
59801.131.142.70——159.0Bonomo et al. 2017TICv8
—1.131.11——G0 V159.0Johnson et al. 2008TICv8
59751.131.142.700.17—159.0Torres et al. 2008TICv8
60761.121.04———159.0Mortier et al. 2013TICv8