Exoplanet

HD 3167 b

Orbiting HD 3167

Overview

HD 3167 b is an exoplanet orbiting the star HD 3167, discovered in 2016 using the Transit method. It is a Super-Earth world.

Key Measurements

Radius

1.60

Earth radii

015 R⊕

Mass

4.84

Earth masses

0500 M⊕

Orbital Period

1.0

days

0.1d10,000d

Distance

47.3

parsecs

Nearby10,000 pc

Equilibrium Temp

1781

K

150 K3,500 K

Radius (Earth radii)

1.60

Mass (Earth masses)

4.84

Measured

Equilibrium Temperature

1781 K

Parameter source: Coy et al. 2026

Orbital Period

0.960+0.0000.000days

Semi-Major Axis

0.0181+0.00030.0002au

Planet Mass (Earth masses)

4.84+0.270.25

Planet Mass (Jupiter masses)

0.0152+0.00080.0008

Eccentricity

0.0000

Argument of Periastron

90.0deg

Radial Velocity Semi-Amplitude

3.46+0.160.16m/s

Distance from Earth

47.3 pc (~154 ly)

Spectral Type

Unknown

Temperature

5338 K

Mass (Solar)

0.86 M☉

Radius (Solar)

0.87 R☉

Luminosity

-0.26 log L☉

Planets in System

4

Stars in System

1

Coordinates (RA, Dec)

8.7401°, 4.3807°

Discovery Method

Transit

Discovery Year

2016

Data Sources

Source ID: HD 3167 b

System Context

HD 3167 b orbits HD 3167 and was reported in 2016 and was detected with the Transit method.

Published measurements list a radius of 1.6 Earth radii, a mass of 4.84 Earth masses, an orbital period of 0.96 days, and an equilibrium temperature near 1,781 K.

Catalog data places the system at about 47.3 parsecs from Earth and 4 known planets in the system.

Host star

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

Open HD 3167

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