Exoplanet

HD 75784 c

Orbiting HD 75784

Overview

HD 75784 c is an exoplanet orbiting the star HD 75784, discovered in 2018 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

1792.56

Earth masses

0500 M⊕

Orbital Period

7900.0

days

0.1d10,000d

Distance

85.4

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

1792.56

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Luhn et al. 2019

Orbital Period

7900.000+2000.0002000.000days

Semi-Major Axis

8.4000+1.40001.4000au

M sin(i) (Earth masses)

1792.56+228.84228.84

M sin(i) (Jupiter masses)

5.6400+0.72000.7200

Eccentricity

0.4890+0.09200.0920

Epoch of Periastron

2431200.00+5900.005900.00days(JD)

Argument of Periastron

325.0+12.012.0deg

Radial Velocity Semi-Amplitude

56.50+5.205.20m/s

Distance from Earth

85.4 pc (~279 ly)

Spectral Type

Unknown

Temperature

4867 K

Mass (Solar)

1.26 M☉

Radius (Solar)

3.40 R☉

Luminosity

Unknown

Planets in System

2

Stars in System

1

Coordinates (RA, Dec)

133.0992°, 13.2331°

Discovery Method

Radial Velocity

Discovery Year

2018

Data Sources

Source ID: HD 75784 c

System Context

HD 75784 c orbits HD 75784 and was reported in 2018 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 1,792.56 Earth masses (M sin i) and an orbital period of 7,900 days.

Catalog data places the system at about 85.4 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 75784

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