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Stellar HostProfile

TOI-1839

Unclassified star • 116.1 pc

Records

3

literature rows

Planets

2

system count

References

4

distinct source labels

TIC: TIC 381714186

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: TICv8 • System source: TICv8

Temperature

5382.7 K

5315.9 to 5382.7

3 values • 2 distinct

Mass

0.93 Msun

single adopted value

1 values • 1 distinct

Radius

0.85 Rsun

single adopted value

3 values • 1 distinct

Luminosity

-0.26 log(Lsun)

single adopted value

1 values • 1 distinct

Distance

116.1 pc

single adopted value

3 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.85 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-1839

0.85 R☉

System Layout

Known planets

2 planets linked to this host

TOI-1839 b

Transit

◌

Discovery

2026

Period

1.42 days

Radius

2.22 R⊕

Mass

—

Eq. Temp

—

TOI-1839 c

Transit

◌

Discovery

2026

Period

4.02 days

Radius

2.41 R⊕

Mass

—

Eq. Temp

—

TOI-1839: A Nearby Star with Two Super-Earths

TOI-1839 is a star located 379 light-years away. It has 0.934 solar masses, a radius of 0.848 solar radii, and a temperature of 5380 K. Its reported radius is smaller than the Sun's, and its reported temperature is cooler than the Sun's. Two planets are known to orbit this star, both discovered by transit in 2026.

TOI-1839 b and TOI-1839 c are both classified as Super-Earths, a size class that reaches 2.5 times Earth's radius. TOI-1839 b has a radius of 2.22 Earth radii and an orbital period of 1.42 days. TOI-1839 c has a radius of 2.41 Earth radii and an orbital period of 4.02 days. Each planet's reported radius is larger than Earth's. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness, and repeated dips help establish orbital periods.

Among the listed planets, TOI-1839 b has the shortest year, at 1.42 days, and the smallest radius, at 2.22 Earth radii. TOI-1839 c has the longest year, at 4.02 days, and the largest radius, at 2.41 Earth radii.

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 • 2 distinct

Massstable

1 values • 1 distinct

Radiusstable

3 values • 1 distinct

Luminositystable

1 values • 1 distinct

Surface Gravitydisputed

3 values • 2 distinct

Metallicitystable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
5382.70.930.85—-0.26—116.1TICv8TICv8
5315.9—0.85———116.1Lafarga et al. 2026TICv8
5382.7—0.85———116.1ExoFOPTICv8