Exoplanet

HD 114729 b

Orbiting HD 114729

Overview

HD 114729 b is an exoplanet orbiting the star HD 114729, discovered in 2002 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

262.21

Earth masses

0500 M⊕

Orbital Period

1121.8

days

0.1d10,000d

Distance

37.8

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

262.21

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Barbato et al. 2018

Orbital Period

1121.790+3.5303.430days

Semi-Major Axis

2.0670+0.01000.0100au

M sin(i) (Earth masses)

262.21+2.222.22

M sin(i) (Jupiter masses)

0.8250+0.00700.0070

Eccentricity

0.0790+0.02900.0320

Epoch of Periastron

2454947.70+82.4082.80days(BJD)

Argument of Periastron

77.1+27.727.7deg

Radial Velocity Semi-Amplitude

16.91+0.530.52m/s

Distance from Earth

37.8 pc (~123 ly)

Spectral Type

Unknown

Temperature

5844 K

Mass (Solar)

0.94 M☉

Radius (Solar)

1.47 R☉

Luminosity

Unknown

Planets in System

1

Stars in System

2

Coordinates (RA, Dec)

198.1834°, -31.8747°

Discovery Method

Radial Velocity

Discovery Year

2002

Data Sources

Source ID: HD 114729 b

System Context

HD 114729 b orbits HD 114729 and was reported in 2002 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 262.21 Earth masses (M sin i) and an orbital period of 1,121.79 days.

Catalog data places the system at about 37.8 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 HD 114729