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Stellar HostProfile

TOI-2096

M4 • 48.48 pc

Records

4

literature rows

Planets

2

system count

References

4

distinct source labels

TIC: TIC 142748283

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: Pozuelos et al. 2023 • System source: TICv8

Temperature

3300 K

3285 to 3300

4 values • 2 distinct

Mass

0.23 Msun

0.22 to 0.23

2 values • 2 distinct

Radius

0.23 Rsun

0.23 to 0.25

4 values • 2 distinct

Age

4 Gyr

single adopted value

1 values • 1 distinct

Luminosity

-2.23 log(Lsun)

-2.23 to -2.19

2 values • 2 distinct

Distance

48.48 pc

single adopted value

4 values • 1 distinct

Spectral Type

M4

Consistent across records

M4 (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.23 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-2096

0.23 R☉

System Layout

Known planets

2 planets linked to this host

TOI-2096 b

Transit

◌

Discovery

2023

Period

3.12 days

Radius

1.24 R⊕

Mass

—

Eq. Temp

445 K

TOI-2096 c

Transit

◌

Discovery

2023

Period

6.39 days

Radius

1.91 R⊕

Mass

—

Eq. Temp

349 K

Planets Around the Red Dwarf TOI-2096

TOI-2096 is a small, cool red dwarf of spectral type M4, located 158 light-years away. Its reported mass is 0.231 solar masses and its reported radius is 0.235 solar radii, both smaller than the Sun's, and its reported temperature of 3300 K is cooler than the Sun's. Its age carries a reported lower limit of 4 billion years. Two planets are known to orbit this host.

Both planets were discovered by transit in 2023, the method in which a planet crosses in front of its star and produces a small dip in observed brightness. TOI-2096 b is an Earth-like planet with a reported radius of 1.24 Earth radii, larger than Earth's, and an orbital period of 3.12 days. TOI-2096 c is a Super-Earth with a reported radius of 1.91 Earth radii, also larger than Earth's, and an orbital period of 6.39 days. Among the listed planets, TOI-2096 b has the shortest year and the smallest radius by reported estimates, while TOI-2096 c has the longest year and the largest radius.

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

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

4 values • 2 distinct

Metallicitystable

1 values • 1 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
32850.220.25—-2.19—48.48TICv8TICv8
33000.230.234-2.23M448.48Pozuelos et al. 2023TICv8
3285—0.25———48.48ExoFOPTICv8
3285—0.25———48.48ExoFOPTICv8