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Stellar HostProfile

TOI-375

Unclassified star • 396.2 pc

Records

3

literature rows

Planets

3

system count

References

4

distinct source labels

TIC: TIC 280097543

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: Reinarz et al. 2026 • System source: TICv8

Temperature

5259.9 K

5001.6 to 5259.9

3 values • 3 distinct

Mass

1.44 Msun

single adopted value

1 values • 1 distinct

Radius

2.90 Rsun

2.90 to 3.27

3 values • 2 distinct

Age

2.94 Gyr

single adopted value

1 values • 1 distinct

Luminosity

0.76 log(Lsun)

single adopted value

1 values • 1 distinct

Distance

396.2 pc

single adopted value

3 values • 1 distinct

Planets

3

Stable across source rows

3

Scale Comparison

Radius against the Sun

Current adopted radius: 2.90 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-375

2.90 R☉

System Layout

Known planets

3 planets linked to this host

TOI-375 b

Transit

◌

Discovery

2026

Period

9.45 days

Radius

10.77 R⊕

Mass

236.8 M⊕

Eq. Temp

1373 K

TOI-375 c

Radial Velocity

◌

Discovery

2026

Period

115.5 days

Radius

—

Mass

669.3 M⊕

Eq. Temp

596 K

TOI-375 d

Radial Velocity

◌

Discovery

2026

Period

297.9 days

Radius

—

Mass

445.6 M⊕

Eq. Temp

434 K

TOI-375 and Its Three Worlds

TOI-375 is a star located 1290 light-years away. It is 2.94 billion years old, has 1.44 solar masses, and spans 2.9 solar radii. Its temperature is 5260 K, making it cooler than the Sun. Both its mass and radius estimates are larger than the Sun's. Three planets orbit this host: TOI-375 b, TOI-375 c, and TOI-375 d.

TOI-375 b was discovered by the transit method in 2026, when the planet passed in front of its star from our viewpoint and caused a small dip in brightness. It is a Jupiter-like planet, with a radius of 10.8 Earth radii and a mass of 237 Earth masses. Both its radius and mass estimates are larger than Earth's, and its mean density is 1.04 g/cm³, 0.189 times Earth's. It completes an orbit in 9.45 days, the shortest year among the listed planets.

TOI-375 c was found by the radial velocity method in 2026, which measures the wobble a planet's gravity induces in its star's motion. Its minimum mass is 669 Earth masses, roughly 2.11 times Jupiter's mass and larger than Earth's, and it orbits every 116 days, the second-shortest year among the listed planets. TOI-375 d was also discovered by radial velocity in 2026. Its minimum mass is 446 Earth masses, roughly 1.4 times Jupiter's mass and larger than Earth's, and it completes an orbit in 298 days, the longest year among the listed planets.

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 • 3 distinct

Massstable

1 values • 1 distinct

Radiusdisputed

3 values • 2 distinct

Agestable

1 values • 1 distinct

Luminositystable

1 values • 1 distinct

Surface Gravitystable

1 values • 1 distinct

Metallicitydisputed

2 values • 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
5001.6—3.27———396.2ExoFOPTICv8
5259.91.442.902.940.76—396.2Reinarz et al. 2026TICv8
5001.6—3.27———396.2TICv8TICv8