Exoplanet

HD 134060 b

Orbiting HD 134060

Overview

HD 134060 b is an exoplanet orbiting the star HD 134060, discovered in 2019 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

10.10

Earth masses

0500 M⊕

Orbital Period

3.3

days

0.1d10,000d

Distance

24.0

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

10.10

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Udry et al. 2019

Orbital Period

3.270+0.0000.000days

Semi-Major Axis

0.0444+0.00130.0014au

M sin(i) (Earth masses)

10.10+0.790.75

M sin(i) (Jupiter masses)

0.0318+0.00250.0024

Eccentricity

0.4500+0.04000.0400

Epoch of Periastron

2455499.65+0.040.04days(BJD)

Argument of Periastron

-98.2+6.66.8deg

Radial Velocity Semi-Amplitude

4.61+0.220.22m/s

Distance from Earth

24.0 pc (~78 ly)

Spectral Type

G3 IV

Temperature

5966 K

Mass (Solar)

1.09 M☉

Radius (Solar)

Unknown

Luminosity

0.16 log L☉

Planets in System

2

Stars in System

1

Coordinates (RA, Dec)

227.6848°, -61.4224°

Discovery Method

Radial Velocity

Discovery Year

2019

Data Sources

Source ID: HD 134060 b

System Context

HD 134060 b orbits HD 134060 and was reported in 2019 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 10.1 Earth masses (M sin i) and an orbital period of 3.27 days.

Catalog data places the system at about 24 parsecs from Earth, a host star classified as G3 IV, 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 134060

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