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Stellar HostProfile

TOI-1685

M3.0 V • 37.62 pc

Records

8

literature rows

Planets

1

system count

References

9

distinct source labels

TIC: TIC 28900646

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: Bluhm et al. 2021 • System source: TICv8

Temperature

3434 K

3434 to 3575

6 values • 5 distinct

Mass

0.49 Msun

0.45 to 0.49

6 values • 5 distinct

Radius

0.49 Rsun

0.46 to 0.49

7 values • 5 distinct

Age

1.30 Gyr

1 to 1.40

3 values • 3 distinct

Luminosity

-1.52 log(Lsun)

-1.57 to -1.52

4 values • 4 distinct

Distance

37.62 pc

single adopted value

8 values • 1 distinct

Spectral Type

M3.0 V

Multiple classifications reported

M2.5 V (2), M2.65 V (1), M3 V (1), M3.0 V (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 0.49 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-1685

0.49 R☉

System Layout

Known planets

1 planets linked to this host

TOI-1685 b

Transit

◌

Discovery

2021

Period

0.67 days

Radius

1.42 R⊕

Mass

3.07 M⊕

Eq. Temp

1000 K

TOI-1685 and Its Earth-Sized Planet

TOI-1685 is an M3.0 V star, a small, cool red dwarf, located 123 light-years away. Its measured mass is 0.495 solar masses, its radius is 0.492 solar radii, and its temperature is 3430 K, all smaller or cooler than the Sun's corresponding values. The star is estimated to be 1.3 billion years old. One planet is known to orbit this host.

That planet, TOI-1685 b, was found by the transit method in 2021, when it passed in front of its star and produced a small dip in observed brightness. It has a radius of 1.42 Earth radii, placing it in the Earth-like size class, and a mass of 3.07 Earth masses, both larger than Earth's. Its mean density is 5.9 g/cm³, 1.07 times Earth's.

TOI-1685 b completes an orbit in just 0.669 days, giving it one of the shortest orbital periods known among planets detected around cool dwarf stars.

Provenance

Underlying measurements and references

Evidence Summary

Rows

8

Stellar refs

8

System refs

1

Distancestable

8 values • 1 distinct

Parallaxstable

8 values • 1 distinct

Temperaturedisputed

6 values • 5 distinct

Massdisputed

6 values • 5 distinct

Radiusdisputed

7 values • 5 distinct

Agedisputed

3 values • 3 distinct

Luminositydisputed

4 values • 4 distinct

Surface Gravitydisputed

5 values • 4 distinct

Metallicitydisputed

4 values • 4 distinct

Spectral Typedisputed

5 values • 4 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
35750.450.461-1.52M2.65 V37.62Burt et al. 2024TICv8
3457—0.46———37.62ExoFOPTICv8
34610.460.46—-1.57—37.62Hirano et al. 2021TICv8
—————M2.5 V37.62Luque et al. 2025TICv8
—0.450.46——M2.5 V37.62Fisher et al. 2026TICv8
34570.460.46—-1.56—37.62TICv8TICv8
34340.490.491.30-1.52M3.0 V37.62Bluhm et al. 2021TICv8
34700.470.461.40—M3 V37.62Egger et al. 2025TICv8