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Stellar HostProfile

TOI-6008

M5.0 • 23.10 pc

Records

3

literature rows

Planets

1

system count

References

4

distinct source labels

TIC: TIC 286201103

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: Barkaoui et al. 2024 • System source: TICv8

Temperature

3075 K

3075 to 3098

3 values • 2 distinct

Mass

0.23 Msun

0.20 to 0.23

2 values • 2 distinct

Radius

0.24 Rsun

0.24 to 0.24

3 values • 2 distinct

Age

3 Gyr

single adopted value

1 values • 1 distinct

Luminosity

-2.33 log(Lsun)

-2.34 to -2.33

2 values • 2 distinct

Distance

23.10 pc

single adopted value

3 values • 1 distinct

Spectral Type

M5.0

Consistent across records

M5.0 (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 0.24 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-6008

0.24 R☉

System Layout

Known planets

1 planets linked to this host

TOI-6008 b

Transit

◌

Discovery

2024

Period

0.86 days

Radius

1.03 R⊕

Mass

4 M⊕

Eq. Temp

707 K

TOI-6008 b: A Close-In Earth-Sized World

TOI-6008 is an M5.0 star located 75.3 light-years away. As an M-type dwarf, it is a small, cool red star, and its reported mass estimate is 0.23 solar masses, smaller than the Sun's. Its reported radius estimate is 0.242 solar radii, also smaller than the Sun's, and its reported temperature is 3080 K, cooler than the Sun's. The star's age is given as a reported lower limit of 3 billion years. One planet is known to orbit this host.

That planet is TOI-6008 b, an Earth-like planet discovered in 2024 by the transit method. Its radius is 1.03 Earth radii, placing it within the Earth-like size class, which spans planets up to 1.5 times Earth's radius. Its mass is a reported upper limit of 4 Earth masses, and its orbital period is just 0.857 days. The transit method detects such worlds when they pass in front of their star from our viewpoint, causing a small dip in observed brightness; repeated dips help establish orbital periods.

Provenance

Underlying measurements and references

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
3098—0.24———23.10ExoFOPTICv8
30750.230.243-2.33M5.023.10Barkaoui et al. 2024TICv8
30980.200.24—-2.34—23.10TICv8TICv8