Exoplanet

HD 21693 c

Orbiting HD 21693

Overview

HD 21693 c is an exoplanet orbiting the star HD 21693, discovered in 2019 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

17.37

Earth masses

0500 M⊕

Orbital Period

53.7

days

0.1d10,000d

Distance

33.3

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

17.37

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Udry et al. 2019

Orbital Period

53.736+0.0310.031days

Semi-Major Axis

0.2586+0.01030.0113au

M sin(i) (Earth masses)

17.37+1.771.79

M sin(i) (Jupiter masses)

0.0547+0.00560.0056

Eccentricity

0.0700+0.06000.0500

Epoch of Periastron

2455528.41+7.088.18days(BJD)

Argument of Periastron

-17.3+47.555.4deg

Radial Velocity Semi-Amplitude

3.44+0.200.20m/s

Distance from Earth

33.3 pc (~108 ly)

Spectral Type

G8 V

Temperature

5430 K

Mass (Solar)

0.80 M☉

Radius (Solar)

Unknown

Luminosity

-0.21 log L☉

Planets in System

2

Stars in System

1

Coordinates (RA, Dec)

51.8040°, -58.3233°

Discovery Method

Radial Velocity

Discovery Year

2019

Data Sources

Source ID: HD 21693 c

System Context

HD 21693 c orbits HD 21693 and was reported in 2019 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 17.37 Earth masses (M sin i) and an orbital period of 53.74 days.

Catalog data places the system at about 33.3 parsecs from Earth, a host star classified as G8 V, 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 21693

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