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

More planets in this system

HD 21693 c