Exoplanet

HD 31527 b

Orbiting HD 31527

Overview

HD 31527 b is an exoplanet orbiting the star HD 31527, discovered in 2019 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

10.47

Earth masses

0500 M⊕

Orbital Period

16.6

days

0.1d10,000d

Distance

38.4

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

10.47

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Udry et al. 2019

Orbital Period

16.553+0.0030.004days

Semi-Major Axis

0.1254+0.00410.0045au

M sin(i) (Earth masses)

10.47+0.890.87

M sin(i) (Jupiter masses)

0.0329+0.00280.0028

Eccentricity

0.1000+0.05000.0500

Epoch of Periastron

2455499.55+1.311.58days(BJD)

Argument of Periastron

41.1+29.534.4deg

Radial Velocity Semi-Amplitude

2.72+0.130.13m/s

Distance from Earth

38.4 pc (~125 ly)

Spectral Type

G2 V

Temperature

5898 K

Mass (Solar)

0.96 M☉

Radius (Solar)

Unknown

Luminosity

0.08 log L☉

Planets in System

3

Stars in System

1

Coordinates (RA, Dec)

73.9096°, -23.2413°

Discovery Method

Radial Velocity

Discovery Year

2019

Data Sources

Source ID: HD 31527 b

System Context

HD 31527 b orbits HD 31527 and was reported in 2019 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 10.47 Earth masses (M sin i) and an orbital period of 16.55 days.

Catalog data places the system at about 38.4 parsecs from Earth, a host star classified as G2 V, and 3 known planets in the system.

Host star

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

Open HD 31527

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