Exoplanet

TOI-1669 b

Orbiting TOI-1669

Overview

TOI-1669 b is an exoplanet orbiting the star TOI-1669, discovered in 2023 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

191.00

Earth masses

0500 M⊕

Orbital Period

500.0

days

0.1d10,000d

Distance

111.3

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

191.00

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Polanski et al. 2024

Orbital Period

500.000+13.00013.000days

Semi-Major Axis

1.2700+0.03000.0300au

M sin(i) (Earth masses)

191.00+25.0024.00

M sin(i) (Jupiter masses)

0.6010+0.07870.0755

Eccentricity

0.0000

Argument of Periastron

90.0deg

Radial Velocity Semi-Amplitude

15.50+1.801.80m/s

Distance from Earth

111.3 pc (~363 ly)

Spectral Type

Unknown

Temperature

5497 K

Mass (Solar)

0.99 M☉

Radius (Solar)

1.06 R☉

Luminosity

-0.04 log L☉

Planets in System

2

Stars in System

1

Coordinates (RA, Dec)

45.9565°, 83.5874°

Discovery Method

Radial Velocity

Discovery Year

2023

Data Sources

Source ID: TOI-1669 b

System Context

TOI-1669 b orbits TOI-1669 and was reported in 2023 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 191 Earth masses (M sin i) and an orbital period of 500 days.

Catalog data places the system at about 111.3 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-1669

More planets in this system