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Stellar HostProfile

HD 181433

Unclassified star • 26.88 pc

Records

15

literature rows

Planets

3

system count

References

15

distinct source labels

TIC: TIC 410399074HD: HD 181433HIP: HIP 95467

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: Ghezzi et al. 2010 • System source: TICv8

Temperature

4915 K

4843.4 to 4962

8 values • 6 distinct

Mass

0.90 Msun

0.63 to 0.90

10 values • 9 distinct

Radius

0.78 Rsun

0.78 to 0.85

5 values • 5 distinct

Age

2 Gyr

2 to 6.70

2 values • 2 distinct

Luminosity

-0.50 log(Lsun)

-0.51 to -0.44

7 values • 6 distinct

Distance

26.88 pc

single adopted value

15 values • 1 distinct

Planets

3

Stable across source rows

3

Scale Comparison

Radius against the Sun

Current adopted radius: 0.78 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 181433

0.78 R☉

System Layout

Known planets

3 planets linked to this host

HD 181433 b

Radial Velocity

◌

Discovery

2008

Period

9.37 days

Radius

—

Mass

7.22 M⊕

Eq. Temp

—

HD 181433 c

Radial Velocity

◌

Discovery

2008

Period

1018.5 days

Radius

—

Mass

235.5 M⊕

Eq. Temp

—

HD 181433 d

Radial Velocity

◌

Discovery

2008

Period

6896.1 days

Radius

—

Mass

206.9 M⊕

Eq. Temp

—

HD 181433: A K-Type Star and Its Three Worlds

HD 181433 is a K2IV/V star located 87.7 light-years away. This star has three known planets. The star is roughly 2 billion years old, with a mass of 0.9 solar masses, a radius of 0.78 solar radii, and a temperature of 4920 K. Its reported radius is smaller than the Sun's, and its temperature is cooler than the Sun's.

All three planets were discovered in 2008 using the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period.

HD 181433 b has a minimum mass of 7.22 Earth masses and an orbital period of 9.37 days. Among the listed planets, it has the shortest year and the smallest minimum mass.

HD 181433 c has a minimum mass of 236 Earth masses and an orbital period of 1020 days. Among the listed planets, it has the second-shortest year and the largest minimum mass.

HD 181433 d has a minimum mass of 207 Earth masses and an orbital period of 6900 days. Among the listed planets, it has the longest year and the second-smallest minimum mass.

Each planet's minimum mass is larger than Earth's. A minimum mass is a lower bound on a planet's true mass, differing from an ordinary mass estimate.

Provenance

Underlying measurements and references

Evidence Summary

Rows

15

Stellar refs

14

System refs

1

Distancestable

15 values • 1 distinct

Parallaxstable

15 values • 1 distinct

Temperaturedisputed

8 values • 6 distinct

Massdisputed

10 values • 9 distinct

Radiusdisputed

5 values • 5 distinct

Agedisputed

2 values • 2 distinct

Luminositydisputed

7 values • 6 distinct

Surface Gravitydisputed

7 values • 5 distinct

Metallicitydisputed

6 values • 4 distinct

Spectral Typedisputed

5 values • 5 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—————K3 III-IV26.88Gray et al. 2006TICv8
—————K2 IV/V26.88Michigan Catalog, Vol. 1TICv8
49000.770.83—-0.44K2IV/V26.88Turnbull 2015TICv8
49620.78——-0.51K3 IV26.88Bouchy et al. 2009TICv8
——————26.88Nordstrom et al. 2004TICv8
49620.78——-0.51—26.88Sousa et al. 2008TICv8
49150.900.782-0.50—26.88Ghezzi et al. 2010TICv8
—0.86————26.88Standing et al. 2026TICv8
—0.87————26.88An et al. 2025TICv8
—————K226.88Cannon & Pickering 1918TICv8
4843.4—0.85—-0.45—26.88Gaia DR2TICv8
—0.87————26.88An et al. 2025TICv8
49180.630.79———26.88Stassun et al. 2017TICv8
4929.60.810.81—-0.46—26.88TICv8TICv8
49620.78—6.70-0.51—26.88Horner et al. 2019TICv8