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Stellar HostProfile

TOI-6692

Unclassified star • 312.9 pc

Records

3

literature rows

Planets

1

system count

References

4

distinct source labels

TIC: TIC 324609409

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: Bieryla et al. 2026 • System source: TICv8

Temperature

5890 K

5890 to 6047

3 values • 2 distinct

Mass

1.05 Msun

1.05 to 1.12

2 values • 2 distinct

Radius

1.39 Rsun

1.37 to 1.39

3 values • 2 distinct

Age

7.80 Gyr

single adopted value

1 values • 1 distinct

Luminosity

0.32 log(Lsun)

0.32 to 0.35

2 values • 2 distinct

Distance

312.9 pc

single adopted value

3 values • 1 distinct

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 1.39 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-6692

1.39 R☉

System Layout

Known planets

1 planets linked to this host

TOI-6692 b

Transit

◌

Discovery

2026

Period

131.1 days

Radius

11.68 R⊕

Mass

197.1 M⊕

Eq. Temp

467 K

TOI-6692 b: A Jupiter-like World Orbiting a Star

TOI-6692 is a star 1020 light-years away with a radius of 1.39 solar radii, a mass of 1.05 solar masses, and a temperature of 5890 K. Its age is 7.8 billion years. The star's reported radius estimate is larger than the Sun's. One planet is known to orbit this host.

That planet, TOI-6692 b, is a Jupiter-like world discovered by the transit method in 2026. During a transit, a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. The planet's radius is 11.7 Earth radii, and its reported radius estimate is larger than Earth's. Jupiter-like planets exceed 4 times Earth's radius. Its mass of 197 Earth masses makes its reported mass estimate larger than Earth's. Its mean density is 0.681 g/cm³, 0.124 times Earth's. Its orbital period is 131 days, the time it takes to complete one orbit.

Provenance

Underlying measurements and references

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Evidence Summary

Rows

3

Stellar refs

3

System refs

1

Distancestable

3 values • 1 distinct

Parallaxstable

3 values • 1 distinct

Temperaturedisputed

3 values • 2 distinct

Massdisputed

2 values • 2 distinct

Radiusdisputed

3 values • 2 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

3 values • 2 distinct

Metallicitystable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
58901.051.397.800.32—312.9Bieryla et al. 2026TICv8
6047—1.37———312.9ExoFOPTICv8
60471.121.37—0.35—312.9TICv8TICv8