Exoplanet

HD 224018 b

Orbiting HD 224018

Overview

HD 224018 b is an exoplanet orbiting the star HD 224018, discovered in 2025 using the Radial Velocity method. It is a Earth-sized world.

Key Measurements

Radius

0.91

Earth radii

015 R⊕

Mass

4.10

Earth masses

0500 M⊕

Orbital Period

10.6

days

0.1d10,000d

Distance

105.5

parsecs

Nearby10,000 pc

Equilibrium Temp

968

K

150 K3,500 K

Radius (Earth radii)

0.91

Mass (Earth masses)

4.10

Measured

Equilibrium Temperature

968 K

Parameter source: Damasso et al. 2025

Orbital Period

10.641+0.0030.003days

Semi-Major Axis

0.0952+0.00200.0020au

Planet Mass (Earth masses)

4.10+0.800.80

Planet Mass (Jupiter masses)

0.0129+0.00250.0025

Eccentricity

0.0600+0.07000.0400

Argument of Periastron

190.0+69.086.0deg

Radial Velocity Semi-Amplitude

1.19+0.220.22m/s

Distance from Earth

105.5 pc (~344 ly)

Spectral Type

G V

Temperature

5784 K

Mass (Solar)

1.01 M☉

Radius (Solar)

1.15 R☉

Luminosity

0.12 log L☉

Planets in System

3

Stars in System

1

Coordinates (RA, Dec)

358.6390°, -4.7233°

Discovery Method

Radial Velocity

Discovery Year

2025

Data Sources

Source ID: HD 224018 b

System Context

HD 224018 b orbits HD 224018 and was reported in 2025 and was detected with the Radial Velocity method.

Published measurements list a radius of 0.91 Earth radii, a mass of 4.1 Earth masses, an orbital period of 10.64 days, and an equilibrium temperature near 968 K.

Catalog data places the system at about 105.5 parsecs from Earth, a host star classified as G V, and 3 known planets in the system.

Host star

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

Open HD 224018

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