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Stellar HostProfile

TOI-5143

K V • 181.4 pc

Records

4

literature rows

Planets

1

system count

References

4

distinct source labels

TIC: TIC 281837575

Approximate color

from effective temperature

Canonical Summary

Adopted host values from one source row

Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.

Stellar source: Radzom et al. 2025 • System source: TICv8

Temperature

5183 K

5183 to 5296.4

4 values • 2 distinct

Mass

0.86 Msun

0.86 to 0.91

2 values • 2 distinct

Radius

0.85 Rsun

0.85 to 0.85

4 values • 2 distinct

Age

7.40 Gyr

single adopted value

1 values • 1 distinct

Distance

181.4 pc

single adopted value

4 values • 1 distinct

Spectral Type

K V

Consistent across records

K V (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 0.85 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-5143

0.85 R☉

System Layout

Known planets

1 planets linked to this host

TOI-5143 c

Transit

◌

Discovery

2025

Period

5.21 days

Radius

16.25 R⊕

Mass

—

Eq. Temp

—

TOI-5143 c: A Jupiter-Like World Around a Cool Dwarf

TOI-5143 is a K V star, a main-sequence dwarf cooler and redder than the Sun, located 592 light-years away. Its reported mass is 0.864 solar masses and its radius is 0.852 solar radii, both smaller than the Sun's corresponding values. The star's temperature is 5180 K, cooler than the Sun's, and its age is 7.4 billion years. One planet is known to orbit this host.

That planet is TOI-5143 c, a Jupiter-like world discovered by the transit method in 2025. It completes an orbit in 5.21 days and has a reported radius of 16.3 Earth radii. This radius is larger than Earth's, and it exceeds four times Earth's radius, the threshold for the Jupiter-like size class. Its mass has not been reported, so no mass comparison can be drawn. The transit method detects the small dip in a star's observed brightness as a planet passes in front of it from our viewpoint, and repeated dips help establish the planet's orbital period of 5.21 days.

Provenance

Underlying measurements and references

Evidence Summary

Rows

4

Stellar refs

3

System refs

1

Distancestable

4 values • 1 distinct

Parallaxstable

4 values • 1 distinct

Temperaturedisputed

4 values • 2 distinct

Massdisputed

2 values • 2 distinct

Radiusdisputed

4 values • 2 distinct

Agestable

1 values • 1 distinct

Luminositystable

1 values • 1 distinct

Surface Gravitydisputed

4 values • 2 distinct

Metallicitydisputed

2 values • 2 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
51830.860.857.40—K V181.4Radzom et al. 2025TICv8
5296.4—0.85———181.4ExoFOPTICv8
5296.40.910.85—-0.29—181.4TICv8TICv8
5296.4—0.85———181.4ExoFOPTICv8