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Stellar HostProfile

TOI-1130

K7 • 58.26 pc

Records

8

literature rows

Planets

2

system count

References

8

distinct source labels

TIC: TIC 254113311

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: Huang et al. 2020 • System source: TICv8

Temperature

4250 K

4236 to 4360

8 values • 5 distinct

Mass

0.68 Msun

0.66 to 0.74

5 values • 4 distinct

Radius

0.69 Rsun

0.69 to 0.74

8 values • 6 distinct

Age

8.20 Gyr

4.10 to 8.20

4 values • 3 distinct

Luminosity

-0.85 log(Lsun)

-0.85 to -0.80

3 values • 3 distinct

Distance

58.26 pc

single adopted value

8 values • 1 distinct

Spectral Type

K7

Multiple classifications reported

K6-K7 (1), K7 (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.69 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-1130

0.69 R☉

System Layout

Known planets

2 planets linked to this host

TOI-1130 b

Transit

◌

Discovery

2020

Period

4.07 days

Radius

3.66 R⊕

Mass

19.80 M⊕

Eq. Temp

825 K

TOI-1130 c

Transit

◌

Discovery

2020

Period

8.35 days

Radius

13 R⊕

Mass

336 M⊕

Eq. Temp

650 K

TOI-1130: A Cool Star With Two Transiting Planets

TOI-1130 is a K7 star located 190 light-years away. Its mass is 0.684 solar masses, its radius is 0.687 solar radii, its temperature is 4250 K, and its age is 8.2 billion years. Both reported measurements place it below the Sun in mass and radius, and at 4250 K it is cooler than the Sun. The star hosts two known planets, both discovered by transit in 2020.

TOI-1130 b is a Neptune-like planet with an orbital period of 4.07 days, a radius of 3.66 Earth radii, and a mass of 19.8 Earth masses. Its radius is larger than Earth's, as is its mass, and its mean density is 2.23 g/cm³, 0.404 times Earth's. Among the listed planets, TOI-1130 b has the shortest year, the smallest radius, and the smallest reported mass.

TOI-1130 c is a Jupiter-like planet with an orbital period of 8.35 days, a radius of 13 Earth radii, and a mass of 336 Earth masses. Its radius is larger than Earth's, and its mass is larger than Earth's as well, at roughly 1.06 times Jupiter's mass. Its mean density is 0.843 g/cm³, 0.153 times Earth's. Among the listed planets, TOI-1130 c has the longest year, the largest radius, and the largest reported mass.

Provenance

Underlying measurements and references

Evidence Summary

Rows

8

Stellar refs

7

System refs

1

Distancestable

8 values • 1 distinct

Parallaxstable

8 values • 1 distinct

Temperaturedisputed

8 values • 5 distinct

Massdisputed

5 values • 4 distinct

Radiusdisputed

8 values • 6 distinct

Agedisputed

4 values • 3 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

7 values • 5 distinct

Metallicitydisputed

4 values • 3 distinct

Spectral Typedisputed

2 values • 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
42360.660.74—-0.80—58.26TICv8TICv8
43600.740.705.40——58.26Borsato et al. 2024TICv8
43500.710.694.10—K6-K758.26Korth et al. 2023TICv8
4236—0.74———58.26ExoFOPTICv8
4236—0.74———58.26ExoFOPTICv8
42500.680.698.20-0.85K758.26Huang et al. 2020TICv8
4341.4—0.69—-0.82—58.26Gaia DR2TICv8
42500.680.698.20——58.26Knudstrup et al. 2024TICv8