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Stellar HostProfile

TOI-1266

M2 • 36.01 pc

Records

8

literature rows

Planets

3

system count

References

8

distinct source labels

TIC: TIC 467179528

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: Greklek-McKeon et al. 2025 • System source: TICv8

Temperature

3563 K

3563 to 3923.1

8 values • 5 distinct

Mass

0.44 Msun

0.43 to 0.45

5 values • 4 distinct

Radius

0.42 Rsun

0.42 to 0.44

7 values • 4 distinct

Age

4.60 Gyr

4.60 to 7.90

2 values • 2 distinct

Luminosity

-1.58 log(Lsun)

-1.58 to -1.53

4 values • 3 distinct

Distance

36.01 pc

single adopted value

8 values • 1 distinct

Spectral Type

M2

Multiple classifications reported

M2 (1), M2 V (1), M3 (1), M3 V (1)

Planets

3

Stable across source rows

3

Scale Comparison

Radius against the Sun

Current adopted radius: 0.42 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-1266

0.42 R☉

System Layout

Known planets

3 planets linked to this host

TOI-1266 b

Transit

◌

Discovery

2020

Period

10.89 days

Radius

2.52 R⊕

Mass

4.46 M⊕

Eq. Temp

415 K

TOI-1266 c

Transit

◌

Discovery

2020

Period

18.80 days

Radius

1.98 R⊕

Mass

3.17 M⊕

Eq. Temp

346 K

TOI-1266 d

Transit Timing Variations

◌

Discovery

2025

Period

32.51 days

Radius

—

Mass

3.68 M⊕

Eq. Temp

288 K

TOI-1266: A Cool Red Dwarf with Three Known Worlds

TOI-1266 is a red dwarf star of spectral type M2, sitting 117 light-years from us. It is a small, cool star: 0.437 solar masses and 0.423 solar radii, with a temperature of 3560 K, all below the Sun's corresponding values, and an age of 4.6 billion years. Three planets are known to orbit this star: TOI-1266 b and TOI-1266 c were both detected by the transit method, in which a planet passing in front of its star produces a small dip in observed brightness, and TOI-1266 d was detected through transit timing variations.

TOI-1266 b was announced in 2020. It is a Neptune-like planet with a radius of 2.52 Earth radii and a mass of 4.46 Earth masses, both larger than Earth's, and a mean density of 1.54 g/cm³, 0.279 times Earth's. It completes one orbit every 10.9 days, the shortest orbital period among the listed planets.

TOI-1266 c, also announced in 2020, is a Super-Earth with a radius of 1.98 Earth radii and a mass of 3.17 Earth masses, again both larger than Earth's. Its mean density is 2.25 g/cm³, 0.408 times Earth's, and it orbits once every 18.8 days, the second-shortest orbital period among the listed planets. It also has the smallest reported mass of the three.

TOI-1266 d was announced in 2025 after being found through transit timing variations, the slight shifts in the timing of the other planets' transits. It has a mass of 3.68 Earth masses, larger than Earth's and the second-smallest reported mass among the listed planets, and it orbits every 32.5 days, the longest orbital period among the listed planets.

The two 2020 discoveries orbit in 10.9 and 18.8 days, while the 2025 planet takes 32.5 days, giving the system a spread of orbital periods. TOI-1266 b's radius of 2.52 Earth radii is the largest of the trio, just above the Super-Earth limit and into Neptune-like territory. The star's mass of 0.437 solar masses and radius of 0.423 solar radii are both smaller than the Sun's, and its temperature of 3560 K is cooler. TOI-1266 d takes 32.5 days to complete one orbit.

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

7 values • 4 distinct

Agedisputed

2 values • 2 distinct

Luminositydisputed

4 values • 3 distinct

Surface Gravitydisputed

7 values • 4 distinct

Metallicitydisputed

4 values • 4 distinct

Spectral Typedisputed

4 values • 4 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
3923.1—————36.01Gaia DR2TICv8
35630.440.424.60-1.58M236.01Greklek-McKeon et al. 2025TICv8
35730.440.427.90-1.58M2 V36.01Stefánsson et al. 2020TICv8
3618—0.44———36.01ExoFOPTICv8
36000.450.42——M336.01Demory et al. 2020TICv8
36180.430.44—-1.54M3 V36.01Cloutier et al. 2024TICv8
36180.430.44—-1.53—36.01TICv8TICv8
3618—0.44———36.01ExoFOPTICv8