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Stellar HostProfile

HATS-59

Unclassified star • 642.9 pc

Records

4

literature rows

Planets

2

system count

References

5

distinct source labels

TIC: TIC 437261733

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: Sarkis et al. 2018 • System source: TICv8

Temperature

5670 K

5459.3 to 5670

4 values • 3 distinct

Mass

1.04 Msun

1 to 1.04

2 values • 2 distinct

Radius

1.04 Rsun

1.04 to 1.12

4 values • 4 distinct

Age

4.30 Gyr

single adopted value

1 values • 1 distinct

Luminosity

-4.36e-3 log(Lsun)

-4.36e-3 to 0.04

3 values • 3 distinct

Distance

642.9 pc

single adopted value

4 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.04 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HATS-59

1.04 R☉

System Layout

Known planets

2 planets linked to this host

HATS-59 b

Transit

◌

Discovery

2018

Period

5.42 days

Radius

12.62 R⊕

Mass

256.2 M⊕

Eq. Temp

1128 K

HATS-59 c

Radial Velocity

◌

Discovery

2018

Period

1422 days

Radius

—

Mass

4036.4 M⊕

Eq. Temp

175.9 K

HATS-59 and Its Two Known Planets

HATS-59 is a star 2100 light-years away with two known planets. The host is 4.3 billion years old and has a mass of 1.04 solar masses and a radius of 1.04 solar radii. Its temperature of 5670 K is cooler than the Sun's. The planets were both discovered in 2018.

HATS-59 b is Jupiter-like and was found by the transit method, which detects the dip in starlight when a planet crosses in front of its star. It has a mass of 256 Earth masses and a radius of 12.6 Earth radii, both larger than Earth's corresponding values, and a mean density of 0.702 g/cm³, 0.127 times Earth's. Its orbital period is 5.42 days, the shortest among the listed planets.

HATS-59 c was found by the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion. Its minimum mass is 4040 Earth masses, roughly 12.7 times Jupiter's mass. Its orbital period is 1420 days, the longest among the listed planets.

Provenance

Underlying measurements and references

Evidence Summary

Rows

4

Stellar refs

4

System refs

1

Distancestable

4 values • 1 distinct

Parallaxstable

4 values • 1 distinct

Temperaturedisputed

4 values • 3 distinct

Massdisputed

2 values • 2 distinct

Radiusdisputed

4 values • 4 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

3 values • 3 distinct

Metallicitystable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
5652—1.10———642.9ExoFOPTICv8
56701.041.044.30-4.36e-3—642.9Sarkis et al. 2018TICv8
565211.10—0.04—642.9TICv8TICv8
5459.3—1.12—1.57e-3—642.9Gaia DR2TICv8