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Stellar HostProfile

TOI-5126

F V • 160.4 pc

Records

4

literature rows

Planets

2

system count

References

4

distinct source labels

TIC: TIC 27064468

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: Fairnington et al. 2024 • System source: TICv8

Temperature

6150 K

6150 to 6223

4 values • 2 distinct

Mass

1.24 Msun

1.20 to 1.24

2 values • 2 distinct

Radius

1.24 Rsun

1.24 to 1.24

4 values • 3 distinct

Age

0.80 Gyr

single adopted value

1 values • 1 distinct

Luminosity

0.30 log(Lsun)

0.30 to 0.32

2 values • 2 distinct

Distance

160.4 pc

single adopted value

4 values • 1 distinct

Spectral Type

F V

Consistent across records

F V (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.24 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-5126

1.24 R☉

System Layout

Known planets

2 planets linked to this host

TOI-5126 b

Transit

◌

Discovery

2023

Period

5.46 days

Radius

4.74 R⊕

Mass

—

Eq. Temp

1442 K

TOI-5126 c

Transit

◌

Discovery

2023

Period

17.90 days

Radius

3.86 R⊕

Mass

—

Eq. Temp

971 K

TOI-5126: An F-Type Star with Two Transiting Planets

TOI-5126 is a star 523 light-years away with a spectral type of F V, a main-sequence dwarf hotter and more massive than the Sun. Its mass is 1.24 solar masses and its radius is 1.24 solar radii, both larger than the Sun's, and its temperature of 6150 K is also hotter. Its age is 0.8 billion years. Two planets are known to orbit it.

Both planets were discovered in 2023 by the transit method, in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness. TOI-5126 b is a Jupiter-like planet with an orbital period of 5.46 days and a radius of 4.74 Earth radii, larger than Earth's. Among the listed planets, it has the shortest year and the largest radius. TOI-5126 c is a Neptune-like planet with an orbital period of 17.9 days and a radius of 3.86 Earth radii, also larger than Earth's. Among the listed planets, it has the longest year and the smallest 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

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

4 values • 3 distinct

Metallicitystable

1 values • 1 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
62231.201.24—0.32—160.4TICv8TICv8
6223—1.24———160.4ExoFOPTICv8
61501.241.240.800.30F V160.4Fairnington et al. 2024TICv8
6223—1.24———160.4ExoFOPTICv8