Exoplanet

TOI-1288 c

Orbiting TOI-1288

Overview

TOI-1288 c is an exoplanet orbiting the star TOI-1288, discovered in 2022 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

85.70

Earth masses

0500 M⊕

Orbital Period

416.0

days

0.1d10,000d

Distance

114.9

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

85.70

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Polanski et al. 2024

Orbital Period

416.000+12.00012.000days

Semi-Major Axis

1.0700+0.03000.0300au

M sin(i) (Earth masses)

85.70+12.1011.70

M sin(i) (Jupiter masses)

0.2696+0.03810.0368

Eccentricity

0.0000

Argument of Periastron

90.0deg

Radial Velocity Semi-Amplitude

7.54+0.990.99m/s

Distance from Earth

114.9 pc (~375 ly)

Spectral Type

Unknown

Temperature

5388 K

Mass (Solar)

0.96 M☉

Radius (Solar)

0.96 R☉

Luminosity

-0.15 log L☉

Planets in System

2

Stars in System

1

Coordinates (RA, Dec)

313.1670°, 65.6088°

Discovery Method

Radial Velocity

Discovery Year

2022

Data Sources

Source ID: TOI-1288 c

System Context

TOI-1288 c orbits TOI-1288 and was reported in 2022 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 85.7 Earth masses (M sin i) and an orbital period of 416 days.

Catalog data places the system at about 114.9 parsecs from Earth 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 TOI-1288

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