Exoplanet

HD 50499 b

Orbiting HD 50499

Overview

HD 50499 b is an exoplanet orbiting the star HD 50499, discovered in 2005 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

519.97

Earth masses

0500 M⊕

Orbital Period

2447.1

days

0.1d10,000d

Distance

46.3

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

519.97

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Barbato et al. 2018

Orbital Period

2447.100+21.92021.720days

Semi-Major Axis

3.8330+0.03050.0300au

M sin(i) (Earth masses)

519.97+5.405.40

M sin(i) (Jupiter masses)

1.6360+0.01700.0170

Eccentricity

0.2660+0.04400.0440

Epoch of Periastron

2456291.10+58.7057.60days(BJD)

Argument of Periastron

288.3+9.610.1deg

Radial Velocity Semi-Amplitude

21.99+1.081.02m/s

Distance from Earth

46.3 pc (~151 ly)

Spectral Type

Unknown

Temperature

6102 K

Mass (Solar)

1.25 M☉

Radius (Solar)

1.35 R☉

Luminosity

Unknown

Planets in System

2

Stars in System

1

Coordinates (RA, Dec)

103.0081°, -33.9153°

Discovery Method

Radial Velocity

Discovery Year

2005

Data Sources

Source ID: HD 50499 b

System Context

HD 50499 b orbits HD 50499 and was reported in 2005 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 519.97 Earth masses (M sin i) and an orbital period of 2,447.1 days.

Catalog data places the system at about 46.3 parsecs from Earth and 2 known planets in the system.

Host star

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

Open HD 50499

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