Exoplanet

alf Tau b

Orbiting alf Tau

Overview

alf Tau b is an exoplanet orbiting the star alf Tau, discovered in 2015 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

2056.36

Earth masses

0500 M⊕

Orbital Period

629.0

days

0.1d10,000d

Distance

20.4

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

2056.36

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Hatzes et al. 2015

Orbital Period

628.960+0.9000.900days

Semi-Major Axis

1.4600+0.27000.2700au

M sin(i) (Earth masses)

2056.36+168.45168.45

M sin(i) (Jupiter masses)

6.4700+0.53000.5300

Eccentricity

0.1000+0.05000.0500

Epoch of Periastron

2451297.00+50.0050.00days(JD)

Argument of Periastron

287.0+29.029.0deg

Radial Velocity Semi-Amplitude

142.10+7.207.20m/s

Distance from Earth

20.4 pc (~67 ly)

Spectral Type

K5 III

Temperature

4055 K

Mass (Solar)

1.13 M☉

Radius (Solar)

45.10 R☉

Luminosity

Unknown

Planets in System

1

Stars in System

2

Coordinates (RA, Dec)

68.9802°, 16.5092°

Discovery Method

Radial Velocity

Discovery Year

2015

Data Sources

Source ID: alf Tau b

System Context

alf Tau b orbits alf Tau and was reported in 2015 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 2,056.36 Earth masses (M sin i) and an orbital period of 628.96 days.

Catalog data places the system at about 20.4 parsecs from Earth, a host star classified as K5 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 alf Tau