Exoplanet

HD 330075 b

Orbiting HD 330075

Overview

HD 330075 b is an exoplanet orbiting the star HD 330075, discovered in 2004 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

152.56

Earth masses

0500 M⊕

Orbital Period

3.4

days

0.1d10,000d

Distance

45.3

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

152.56

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Stassun et al. 2017

Orbital Period

3.388+0.0000.000days

Semi-Major Axis

0.0400+0.00000.0000au

M sin(i) (Earth masses)

152.56+6.366.36

M sin(i) (Jupiter masses)

0.4800+0.02000.0200

Eccentricity

0.0000

Radial Velocity Semi-Amplitude

107.00+0.700.70m/s

Distance from Earth

45.3 pc (~148 ly)

Spectral Type

Unknown

Temperature

5000 K

Mass (Solar)

0.47 M☉

Radius (Solar)

0.84 R☉

Luminosity

Unknown

Planets in System

1

Stars in System

1

Coordinates (RA, Dec)

237.4055°, -49.9639°

Discovery Method

Radial Velocity

Discovery Year

2004

Data Sources

Source ID: HD 330075 b

System Context

HD 330075 b orbits HD 330075 and was reported in 2004 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 152.56 Earth masses (M sin i) and an orbital period of 3.39 days.

Catalog data places the system at about 45.3 parsecs from Earth 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 330075
HD 330075 b