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Stellar HostProfile

TOI-1453

Unclassified star • 78.74 pc

Records

4

literature rows

Planets

2

system count

References

4

distinct source labels

TIC: TIC 198390247

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: Stalport et al. 2025 • System source: TICv8

Temperature

4975 K

4920 to 4975

4 values • 2 distinct

Mass

0.71 Msun

0.71 to 0.81

2 values • 2 distinct

Radius

0.72 Rsun

0.71 to 0.72

4 values • 3 distinct

Age

12 Gyr

single adopted value

1 values • 1 distinct

Distance

78.74 pc

single adopted value

4 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.72 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-1453

0.72 R☉

System Layout

Known planets

2 planets linked to this host

TOI-1453 b

Transit

◌

Discovery

2025

Period

4.31 days

Radius

1.17 R⊕

Mass

2.32 M⊕

Eq. Temp

944.2 K

TOI-1453 c

Transit

◌

Discovery

2025

Period

6.59 days

Radius

2.22 R⊕

Mass

2.95 M⊕

Eq. Temp

819.8 K

TOI-1453 and Its Two Planets

TOI-1453 is a star 257 light-years from Earth with two known planets. The star is 12 billion years old, has a mass of 0.715 solar masses, a radius of 0.72 solar radii, and a temperature of 4980 K. Its mass, radius, and temperature are all smaller or cooler than the Sun's.

Both planets were discovered by transit in 2025. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness.

TOI-1453 b is classified as Earth-like. It has an orbital period of 4.31 days, a radius of 1.17 Earth radii, and a reported upper limit mass of 2.32 Earth masses. Its radius is larger than Earth's. Among the listed planets, it has the shortest year and the smallest radius.

TOI-1453 c is classified as a Super-Earth. It has an orbital period of 6.59 days, a mass of 2.95 Earth masses, and a radius of 2.22 Earth radii. Its mass and radius are both larger than Earth's, and its mean density is 1.48 g/cm³, which is 0.268 times Earth's. Among the listed planets, it 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 • 3 distinct

Agestable

1 values • 1 distinct

Luminositystable

1 values • 1 distinct

Surface Gravitydisputed

4 values • 3 distinct

Metallicitystable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
49750.710.7212——78.74Stalport et al. 2025TICv8
4920—0.71———78.74ExoFOPTICv8
4920—0.71———78.74ExoFOPTICv8
49200.810.71—-0.58—78.74TICv8TICv8