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Stellar HostProfile

TOI-5713

M3.5+/-0.5 • 40.87 pc

Records

3

literature rows

Planets

1

system count

References

4

distinct source labels

TIC: TIC 219041246

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: Ghachoui et al. 2024 • System source: TICv8

Temperature

3225 K

3225 to 3271

3 values • 2 distinct

Mass

0.27 Msun

0.27 to 0.27

2 values • 2 distinct

Radius

0.30 Rsun

0.29 to 0.30

3 values • 2 distinct

Age

4.50 Gyr

single adopted value

1 values • 1 distinct

Luminosity

-2.06 log(Lsun)

-2.06 to -2.05

2 values • 2 distinct

Distance

40.87 pc

single adopted value

3 values • 1 distinct

Spectral Type

M3.5+/-0.5

Consistent across records

M3.5+/-0.5 (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 0.30 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-5713

0.30 R☉

System Layout

Known planets

1 planets linked to this host

TOI-5713 b

Transit

◌

Discovery

2024

Period

10.44 days

Radius

1.77 R⊕

Mass

—

Eq. Temp

347.2 K

TOI-5713 and Its Super-Earth

TOI-5713 is an M-type dwarf, a small, cool red star 133 light-years away. Its spectral type is M3.5+/-0.5, with a temperature of 3230 K, making it cooler than the Sun. The star's reported mass estimate is 0.265 solar masses and its reported radius estimate is 0.299 solar radii, both smaller than the Sun's. Its age carries a reported upper limit of 4.5 billion years. One planet is known to orbit this host.

That planet is TOI-5713 b, a Super-Earth discovered by the transit method in 2024. A transit occurs when a planet crosses in front of its star from our viewpoint, dimming the star's light slightly and helping establish the planet's orbital period. TOI-5713 b completes one orbit in 10.4 days and has a radius of 1.77 Earth radii, larger than Earth's. The planet's radius places it in the Super-Earth class.

Provenance

Underlying measurements and references

Download JSONDownload CSV

Evidence Summary

Rows

3

Stellar refs

3

System refs

1

Distancestable

3 values • 1 distinct

Parallaxstable

3 values • 1 distinct

Temperaturedisputed

3 values • 2 distinct

Massdisputed

2 values • 2 distinct

Radiusdisputed

3 values • 2 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

3 values • 2 distinct

Metallicitystable

1 values • 1 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
32250.270.304.50-2.06M3.5+/-0.540.87Ghachoui et al. 2024TICv8
32710.270.29—-2.05—40.87TICv8TICv8
3271—0.29———40.87ExoFOPTICv8