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Stellar HostProfile

HATS-23

G V • 639.0 pc

Records

4

literature rows

Planets

1

system count

References

5

distinct source labels

TIC: TIC 7088246

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: Bento et al. 2017 • System source: TICv8

Temperature

5780 K

5532.3 to 5780

4 values • 3 distinct

Mass

1.12 Msun

1.03 to 1.12

2 values • 2 distinct

Radius

1.20 Rsun

1.05 to 1.20

4 values • 4 distinct

Age

4.20 Gyr

single adopted value

1 values • 1 distinct

Luminosity

0.16 log(Lsun)

6.26e-3 to 0.16

3 values • 3 distinct

Distance

639.0 pc

single adopted value

4 values • 1 distinct

Spectral Type

G V

Consistent across records

G V (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 1.20 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HATS-23

1.20 R☉

System Layout

Known planets

1 planets linked to this host

HATS-23 b

Transit

◌

Discovery

2017

Period

2.16 days

Radius

20.85 R⊕

Mass

467.2 M⊕

Eq. Temp

1654 K

HATS-23 b: A Jupiter-like World

HATS-23 is a G V star, a Sun-like main-sequence dwarf, located 2080 light-years away. Its reported mass is 1.12 solar masses and its radius is 1.2 solar radii, both larger than the Sun's. The star is 4.2 billion years old and has a temperature of 5780 K. One planet orbits this host.

That planet, HATS-23 b, was discovered in 2017 by the transit method, which detects the small dip in a star's brightness when a planet passes in front of it. The planet's radius is 20.8 Earth radii and its mass is 467 Earth masses; both values are larger than Earth's. Its mass is roughly 1.47 times Jupiter's mass. With a radius exceeding four times Earth's, HATS-23 b is classified as Jupiter-like. Its mean density is 0.284 g/cm³, 0.0516 times Earth's. HATS-23 b completes one orbit in 2.16 days.

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

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
57591.031.05—0.04—639.0TICv8TICv8
5780—1.20———639.0ExoFOPTICv8
5532.3—1.10—6.26e-3—639.0Gaia DR2TICv8
57801.121.204.200.16G V639.0Bento et al. 2017TICv8