Exoplanet

HATS-24 b

Orbiting HATS-24

Overview

HATS-24 b is an exoplanet orbiting the star HATS-24, discovered in 2017 using the Transit method. It is a Jupiter-sized world.

Key Measurements

Radius

15.64

Earth radii

015 R⊕

Mass

718.30

Earth masses

0500 M⊕

Orbital Period

1.3

days

0.1d10,000d

Distance

494.2

parsecs

Nearby10,000 pc

Equilibrium Temp

2166

K

150 K3,500 K

Radius (Earth radii)

15.64

Mass (Earth masses)

718.30

Measured

Equilibrium Temperature

2166 K

Parameter source: Oliveira et al. 2019

Orbital Period

1.348+0.000−0.000days

Semi-Major Axis

0.0238+0.0010−0.0010au

Planet Mass (Earth masses)

718.30+54.03−54.03

Planet Mass (Jupiter masses)

2.2600+0.1700−0.1700

Eccentricity

0.0000

Argument of Periastron

90.0deg

Distance from Earth

494.2 pc (~1612 ly)

Spectral Type

Unknown

Temperature

6125 K

Mass (Solar)

1.07 M☉

Radius (Solar)

1.12 R☉

Luminosity

0.19 log L☉

Planets in System

1

Stars in System

1

Coordinates (RA, Dec)

268.8907°, -61.7474°

Discovery Method

Transit

Discovery Year

2017

Data Sources
NASA Exoplanet Archive

Source ID: HATS-24 b

System Context

HATS-24 b orbits HATS-24 and was reported in 2017 and was detected with the Transit method.

Published measurements list a radius of 15.64 Earth radii, a mass of 718.3 Earth masses, an orbital period of 1.35 days, and an equilibrium temperature near 2,166 K.

Catalog data places the system at about 494.2 parsecs from Earth and 1 known planet in the system.

Host star

Explore the stellar record for this system to compare temperature, spectral type, and known planets.

Open HATS-24