Exoplanet

HD 33142 c

Orbiting HD 33142

Overview

HD 33142 c is an exoplanet orbiting the star HD 33142, discovered in 2016 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

282.87

Earth masses

0500 M⊕

Orbital Period

810.2

days

0.1d10,000d

Distance

121.4

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

282.87

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Trifonov et al. 2022

Orbital Period

810.200+3.8004.200days

Semi-Major Axis

1.9550+0.01600.0120au

M sin(i) (Earth masses)

282.87+19.0715.89

M sin(i) (Jupiter masses)

0.8900+0.06000.0500

Eccentricity

0.0810+0.05500.0470

Argument of Periastron

52.0+71.057.0deg

Radial Velocity Semi-Amplitude

14.70+0.900.90m/s

Distance from Earth

121.4 pc (~396 ly)

Spectral Type

K0 III

Temperature

5025 K

Mass (Solar)

1.52 M☉

Radius (Solar)

4.17 R☉

Luminosity

1.00 log L☉

Planets in System

3

Stars in System

1

Coordinates (RA, Dec)

76.8981°, -13.9863°

Discovery Method

Radial Velocity

Discovery Year

2016

Data Sources

Source ID: HD 33142 c

System Context

HD 33142 c orbits HD 33142 and was reported in 2016 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 282.87 Earth masses (M sin i) and an orbital period of 810.2 days.

Catalog data places the system at about 121.4 parsecs from Earth, a host star classified as K0 III, 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 33142

More planets in this system

HD 33142 c