Exoplanet

HD 104985 b

Orbiting HD 104985

Overview

HD 104985 b is an exoplanet orbiting the star HD 104985, discovered in 2003 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

1766.81

Earth masses

0500 M⊕

Orbital Period

199.7

days

0.1d10,000d

Distance

100.6

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

1766.81

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Teng et al. 2023

Orbital Period

199.680+0.0900.070days

Semi-Major Axis

0.7150+0.00000.0000au

M sin(i) (Earth masses)

1766.81+34.9638.78

M sin(i) (Jupiter masses)

5.5590+0.11000.1220

Eccentricity

0.0470+0.01500.0280

Epoch of Periastron

2455083.50+17.7016.10days(JD)

Argument of Periastron

133.8+33.328.0deg

Radial Velocity Semi-Amplitude

169.06+3.333.74m/s

Distance from Earth

100.6 pc (~328 ly)

Spectral Type

G9 III

Temperature

4738 K

Mass (Solar)

1.22 M☉

Radius (Solar)

11.12 R☉

Luminosity

1.77 log L☉

Planets in System

1

Stars in System

1

Coordinates (RA, Dec)

181.3158°, 76.9053°

Discovery Method

Radial Velocity

Discovery Year

2003

Data Sources

Source ID: HD 104985 b

System Context

HD 104985 b orbits HD 104985 and was reported in 2003 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 1,766.81 Earth masses (M sin i) and an orbital period of 199.68 days.

Catalog data places the system at about 100.6 parsecs from Earth, a host star classified as G9 III, and 1 known planet in the system.

Host star

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

Open HD 104985