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Stellar HostProfile

TOI-2095

M2.5 V • 41.92 pc

Records

5

literature rows

Planets

2

system count

References

5

distinct source labels

TIC: TIC 235678745

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: Murgas et al. 2023 • System source: TICv8

Temperature

3759 K

3662 to 3759

5 values • 3 distinct

Mass

0.44 Msun

0.44 to 0.47

3 values • 3 distinct

Radius

0.44 Rsun

0.44 to 0.46

5 values • 3 distinct

Age

1 Gyr

single adopted value

1 values • 1 distinct

Luminosity

-1.46 log(Lsun)

-1.48 to -1.42

3 values • 3 distinct

Distance

41.92 pc

single adopted value

5 values • 1 distinct

Spectral Type

M2.5 V

Multiple classifications reported

M0.5-1.0 V (1), M2.5 V (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.44 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-2095

0.44 R☉

System Layout

Known planets

2 planets linked to this host

TOI-2095 b

Transit

◌

Discovery

2023

Period

17.66 days

Radius

1.25 R⊕

Mass

4.10 M⊕

Eq. Temp

347 K

TOI-2095 c

Transit

◌

Discovery

2023

Period

28.17 days

Radius

1.33 R⊕

Mass

7.40 M⊕

Eq. Temp

297 K

TOI-2095 and Its Two Planets

TOI-2095 is an M2.5 V star, a small, cool red dwarf, located 137 light-years away. Its reported lower age limit is 1 billion years, and it has a mass of 0.44 solar masses and a radius of 0.44 solar radii, both smaller than the Sun's. Its temperature of 3760 K is cooler than the Sun's. Two planets orbit this host.

Both planets were discovered by transit in 2023. TOI-2095 b is an Earth-like planet with a radius of 1.25 Earth radii, a reported upper mass limit of 4.1 Earth masses, and an orbital period of 17.7 days. TOI-2095 c is also Earth-like, with a radius of 1.33 Earth radii, a reported upper mass limit of 7.4 Earth masses, and an orbital period of 28.2 days. Both radii are larger than Earth's.

Provenance

Underlying measurements and references

Evidence Summary

Rows

5

Stellar refs

4

System refs

1

Distancestable

5 values • 1 distinct

Parallaxstable

5 values • 1 distinct

Temperaturedisputed

5 values • 3 distinct

Massdisputed

3 values • 3 distinct

Radiusdisputed

5 values • 3 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

4 values • 2 distinct

Metallicitydisputed

2 values • 2 distinct

Spectral Typedisputed

2 values • 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
36620.470.45—-1.48M0.5-1.0 V41.92Quintana et al. 2023TICv8
37460.460.46—-1.42—41.92TICv8TICv8
3746—0.46———41.92ExoFOPTICv8
37590.440.441-1.46M2.5 V41.92Murgas et al. 2023TICv8
3746—0.46———41.92ExoFOPTICv8