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Stellar HostProfile

TOI-1386

G5V • 146.9 pc

Records

4

literature rows

Planets

2

system count

References

5

distinct source labels

TIC: TIC 343019899

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: Hill et al. 2024 • System source: TICv8

Temperature

5793 K

5735 to 5793

4 values • 3 distinct

Mass

1.04 Msun

1.03 to 1.04

3 values • 3 distinct

Radius

1.01 Rsun

1.01 to 1.03

4 values • 4 distinct

Age

3.30 Gyr

3.20 to 3.30

2 values • 2 distinct

Luminosity

0.02 log(Lsun)

0.01 to 0.03

3 values • 3 distinct

Distance

146.9 pc

single adopted value

4 values • 1 distinct

Spectral Type

G5V

Consistent across records

G5V (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.01 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-1386

1.01 R☉

System Layout

Known planets

2 planets linked to this host

TOI-1386 b

Transit

◌

Discovery

2024

Period

25.84 days

Radius

6.22 R⊕

Mass

45.80 M⊕

Eq. Temp

615.0 K

TOI-1386 c

Radial Velocity

◌

Discovery

2024

Period

232 days

Radius

—

Mass

75.20 M⊕

Eq. Temp

—

TOI-1386 and Its Two Known Planets

TOI-1386 is a Sun-like star with a spectral type of G5V. It lies 479 light-years away and has a mass of 1.04 solar masses, a radius of 1.01 solar radii, a temperature of 5790 K, and an age of 3.3 billion years. Two planets are known to orbit this star.

TOI-1386 b is a Jupiter-like planet discovered by the transit method in 2024. Its radius is 6.22 Earth radii, which is larger than Earth's. Its mass is 45.8 Earth masses, also larger than Earth's, and its mean density is 1.05 g/cm³, 0.191 times Earth's. Among the listed planets, it has the shortest year by reported estimates, at 25.8 days.

TOI-1386 c was discovered by the radial velocity method in 2024. This technique measures the wobble a planet's gravity induces in its star's motion, and repeated wobbles reveal the planet and its orbital period. Its minimum mass is 75.2 Earth masses, meaning its true mass is at least this value, and is larger than Earth's. Its orbital period is 232 days, the longest year among the listed planets by reported estimates.

Provenance

Underlying measurements and references

Evidence Summary

Rows

4

Stellar refs

4

System refs

1

Distancestable

4 values • 1 distinct

Parallaxstable

4 values • 1 distinct

Temperaturedisputed

4 values • 3 distinct

Massdisputed

3 values • 3 distinct

Radiusdisputed

4 values • 4 distinct

Agedisputed

2 values • 2 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

4 values • 4 distinct

Metallicitydisputed

2 values • 2 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
57931.041.013.300.02G5V146.9Hill et al. 2024TICv8
5769—1.03———146.9ExoFOPTICv8
57691.031.03—0.03—146.9TICv8TICv8
57351.041.023.200.01—146.9MacDougall et al. 2023TICv8