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Stellar HostProfile

TOI-1470

M1.5 V • 51.95 pc

Records

4

literature rows

Planets

2

system count

References

5

distinct source labels

TIC: TIC 284441182

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: González-Álvarez et al. 2023 • System source: TICv8

Temperature

3709 K

3399.8 to 3709

4 values • 3 distinct

Mass

0.47 Msun

0.47 to 0.49

2 values • 2 distinct

Radius

0.47 Rsun

0.47 to 0.49

4 values • 2 distinct

Age

1.30 Gyr

single adopted value

1 values • 1 distinct

Luminosity

-1.42 log(Lsun)

-1.43 to -1.42

2 values • 2 distinct

Distance

51.95 pc

single adopted value

4 values • 1 distinct

Spectral Type

M1.5 V

Consistent across records

M1.5 V (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.47 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-1470

0.47 R☉

System Layout

Known planets

2 planets linked to this host

TOI-1470 b

Transit

◌

Discovery

2023

Period

2.53 days

Radius

2.18 R⊕

Mass

7.32 M⊕

Eq. Temp

734 K

TOI-1470 c

Transit

◌

Discovery

2023

Period

18.09 days

Radius

2.47 R⊕

Mass

7.24 M⊕

Eq. Temp

373 K

TOI-1470: A Nearby Red Dwarf with Two Super-Earths

TOI-1470 is an M1.5 V star, a small, cool red dwarf, located 169 light-years from Earth. The star has a reported mass of 0.471 solar masses, a radius of 0.469 solar radii, and a temperature of 3710 K, all smaller or cooler than the corresponding values for the Sun. Its age is 1.3 billion years. Two planets have been found orbiting this star.

Both planets were discovered by transit in 2023. TOI-1470 b is a Super-Earth with a radius of 2.18 Earth radii and a mass of 7.32 Earth masses. Its orbital period is 2.53 days, the shortest among the listed planets. Among the listed planets, it also has the smallest radius and the largest reported mass. Its mean density is 3.89 g/cm³, 0.707 times Earth's.

TOI-1470 c is also a Super-Earth, with a radius of 2.47 Earth radii and a mass of 7.24 Earth masses. Its orbital period is 18.1 days, the longest among the listed planets. Among the listed planets, it has the largest radius and the smallest reported mass. Its mean density is 2.65 g/cm³, 0.48 times Earth's.

Both planets are larger and more massive than Earth. Their orbital periods demonstrate repeated transits, with TOI-1470 c completing one orbit in 18.1 days compared to 2.53 days for TOI-1470 b.

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

2 values • 2 distinct

Radiusdisputed

4 values • 2 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
3399.8—0.49———51.95Lafarga et al. 2026TICv8
37090.470.471.30-1.42M1.5 V51.95González-Álvarez et al. 2023TICv8
36240.490.49—-1.43—51.95TICv8TICv8
3624—0.49———51.95ExoFOPTICv8