Exoplanet

tau Cet f

Orbiting tau Cet

Overview

tau Cet f is an exoplanet orbiting the star tau Cet, discovered in 2017 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

3.93

Earth masses

0500 M⊕

Orbital Period

636.1

days

0.1d10,000d

Distance

3.6

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

3.93

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Feng et al. 2017

Orbital Period

636.130+11.70047.690days

Semi-Major Axis

1.3340+0.01700.0440au

M sin(i) (Earth masses)

3.93+1.051.37

M sin(i) (Jupiter masses)

0.0124+0.00330.0043

Eccentricity

0.1600+0.07000.1600

Argument of Periastron

119.8+41.370.5deg

Radial Velocity Semi-Amplitude

0.35+0.100.12m/s

Distance from Earth

3.6 pc (~12 ly)

Spectral Type

Unknown

Temperature

Unknown

Mass (Solar)

0.78 M☉

Radius (Solar)

Unknown

Luminosity

Unknown

Planets in System

3

Stars in System

1

Coordinates (RA, Dec)

26.0093°, -15.9338°

Discovery Method

Radial Velocity

Discovery Year

2017

Data Sources

Source ID: tau Cet f

System Context

tau Cet f orbits tau Cet and was reported in 2017 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 3.93 Earth masses (M sin i) and an orbital period of 636.13 days.

Catalog data places the system at about 3.6 parsecs from Earth 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 tau Cet

More planets in this system