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

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