Exoplanet

iot Dra c

Orbiting iot Dra

Overview

iot Dra c is an exoplanet orbiting the star iot Dra, discovered in 2021 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

4958.12

Earth masses

0500 M⊕

Orbital Period

25000.0

days

0.1d10,000d

Distance

31.3

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

4958.12

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Hill et al. 2021

Orbital Period

25000.000+22000.00013000.000days

Semi-Major Axis

19.4000+10.00007.7000au

M sin(i) (Earth masses)

4958.12+4449.601620.92

M sin(i) (Jupiter masses)

15.6000+14.00005.1000

Eccentricity

0.4550+0.12000.0840

Epoch of Periastron

2476000.00+22000.0013000.00days(JD)

Argument of Periastron

62.0+262.032.0deg

Distance from Earth

31.3 pc (~102 ly)

Spectral Type

K2 III

Temperature

4504 K

Mass (Solar)

1.54 M☉

Radius (Solar)

11.79 R☉

Luminosity

1.72 log L☉

Planets in System

2

Stars in System

1

Coordinates (RA, Dec)

231.2323°, 58.9661°

Discovery Method

Radial Velocity

Discovery Year

2021

Data Sources

Source ID: iot Dra c

System Context

iot Dra c orbits iot Dra and was reported in 2021 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 4,958.12 Earth masses (M sin i) and an orbital period of 25,000 days.

Catalog data places the system at about 31.3 parsecs from Earth, a host star classified as K2 III, 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 iot Dra

More planets in this system