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Stellar HostProfile

Wolf 1061

M3.5 โ€ข 4.31 pc

Records

8

literature rows

Planets

3

system count

References

9

distinct source labels

TIC: TIC 413948621HIP: HIP 80824

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: Astudillo-Defru et al. 2017 โ€ข System source: TICv8

Temperature

3342 K

3268 to 3727.4

5 values โ€ข 5 distinct

Mass

0.29 Msun

0.25 to 0.32

4 values โ€ข 4 distinct

Radius

0.31 Rsun

0.31 to 0.34

3 values โ€ข 3 distinct

Luminosity

-1.99 log(Lsun)

-2.10 to -1.95

4 values โ€ข 4 distinct

Distance

4.31 pc

single adopted value

8 values โ€ข 1 distinct

Spectral Type

M3.5

Multiple classifications reported

M3.5 (2), M3.5V (1), M3/3.5 V (1)

Planets

3

Stable across source rows

3

Scale Comparison

Radius against the Sun

Current adopted radius: 0.31 Rโ˜‰ (circles scaled linearly by radius)

Sun

1.0 Rโ˜‰ baseline

Wolf 1061

0.31 Rโ˜‰

System Layout

Known planets

3 planets linked to this host

Wolf 1061 b

Radial Velocity

โ—Œ

Discovery

2015

Period

4.89 days

Radius

โ€”

Mass

1.91 MโŠ•

Eq. Temp

โ€”

Wolf 1061 c

Radial Velocity

โ—Œ

Discovery

2015

Period

17.87 days

Radius

โ€”

Mass

3.41 MโŠ•

Eq. Temp

โ€”

Wolf 1061 d

Radial Velocity

โ—Œ

Discovery

2015

Period

217.2 days

Radius

โ€”

Mass

7.70 MโŠ•

Eq. Temp

โ€”

Wolf 1061 and Its Three Known Planets

Wolf 1061 is a small, cool red dwarf of spectral type M3.5, lying 14 light-years from us. Its reported mass is 0.294 solar masses, and its reported radius is 0.307 solar radii. Both estimates are smaller than the Sun's. Its reported temperature is 3340 K, cooler than the Sun's. Three planets are known to orbit this star.

All three worlds were found in 2015 by the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period. Each has a minimum mass, meaning a lower bound on its true mass, and each minimum mass is larger than Earth's.

Wolf 1061 b has the smallest minimum mass of the three, 1.91 Earth masses. It completes one orbit in 4.89 days, the shortest year among these planets by reported estimates. Wolf 1061 c is the middle case, with a minimum mass of 3.41 Earth masses and a period of 17.9 days, the second-shortest year of the trio by reported estimates. Wolf 1061 d is the heaviest of the three and the slowest, with a minimum mass of 7.7 Earth masses and an orbital period of 217 days, the longest year among the listed planets by reported estimates.

Provenance

Underlying measurements and references

Evidence Summary

Rows

8

Stellar refs

8

System refs

1

Distancestable

8 values โ€ข 1 distinct

Parallaxstable

8 values โ€ข 1 distinct

Temperaturedisputed

5 values โ€ข 5 distinct

Massdisputed

4 values โ€ข 4 distinct

Radiusdisputed

3 values โ€ข 3 distinct

Luminositydisputed

4 values โ€ข 4 distinct

Surface Gravitystable

1 values โ€ข 1 distinct

Metallicitystable

1 values โ€ข 1 distinct

Spectral Typedisputed

4 values โ€ข 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
33090.300.32โ€”-1.95โ€”4.31TICv8TICv8
โ€”โ€”โ€”โ€”โ€”โ€”4.31Wright et al. 2004TICv8
33420.290.31โ€”-1.99M3.54.31Astudillo-Defru et al. 2017TICv8
32680.320.34โ€”-2M3.5V4.31Turnbull 2015TICv8
33930.25โ€”โ€”-2.10M3/3.5 V4.31Wright et al. 2016TICv8
3727.4โ€”โ€”โ€”โ€”โ€”4.31Gaia DR2TICv8
โ€”โ€”โ€”โ€”โ€”M3.54.31Hawley et al. 1996TICv8
โ€”โ€”โ€”โ€”โ€”โ€”4.31Nidever et al. 2002TICv8