Exoplanet

HD 158259 e

Orbiting HD 158259

Overview

HD 158259 e is an exoplanet orbiting the star HD 158259, discovered in 2020 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

6.08

Earth masses

0500 M⊕

Orbital Period

8.0

days

0.1d10,000d

Distance

27.0

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

Minimum Mass, M sin(i) (Earth masses)

6.08

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Hara et al. 2020

Orbital Period

7.951+0.0020.002days

M sin(i) (Earth masses)

6.08+0.941.03

M sin(i) (Jupiter masses)

0.0191+0.00300.0032

Radial Velocity Semi-Amplitude

1.86+0.260.29m/s

Distance from Earth

27.0 pc (~88 ly)

Spectral Type

G0

Temperature

Unknown

Mass (Solar)

1.08 M☉

Radius (Solar)

1.21 R☉

Luminosity

Unknown

Planets in System

5

Stars in System

1

Coordinates (RA, Dec)

261.3496°, 52.7905°

Discovery Method

Radial Velocity

Discovery Year

2020

Data Sources

Source ID: HD 158259 e

System Context

HD 158259 e orbits HD 158259 and was reported in 2020 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 6.08 Earth masses (M sin i) and an orbital period of 7.95 days.

Catalog data places the system at about 27 parsecs from Earth, a host star classified as G0, and 5 known planets in the system.

Host star

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

Open HD 158259