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Stellar HostProfile

HD 30177

Unclassified star • 55.59 pc

Records

16

literature rows

Planets

2

system count

References

17

distinct source labels

TIC: TIC 220408612HIP: HIP 21850HD: HD 30177

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

5595 K

5545.7 to 5680

10 values • 10 distinct

Mass

1.10 Msun

0.93 to 1.10

11 values • 9 distinct

Radius

1.04 Rsun

1.02 to 1.19

6 values • 6 distinct

Age

3.50 Gyr

2.52 to 14.20

6 values • 5 distinct

Luminosity

-0.02 log(Lsun)

-0.02 to 0.08

3 values • 3 distinct

Distance

55.59 pc

single adopted value

16 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.04 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 30177

1.04 R☉

System Layout

Known planets

2 planets linked to this host

HD 30177 b

Radial Velocity

◌

Discovery

2002

Period

2539 days

Radius

—

Mass

2622.1 M⊕

Eq. Temp

—

HD 30177 c

Radial Velocity

◌

Discovery

2016

Period

11320 days

Radius

—

Mass

1484.3 M⊕

Eq. Temp

—

HD 30177 and Its Two Known Planets

HD 30177 is a G8 V star 181 light-years away. It is a G-type main-sequence dwarf with 1.1 solar masses, 1.04 solar radii, and a temperature of 5600 K that is cooler than the Sun's. It is 3.5 billion years old, and two planets are known to orbit it.

Both planets were found by the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion. HD 30177 b was discovered in 2002 and has a mass of 2620 Earth masses, roughly 8.25 times Jupiter's mass and larger than Earth's. It completes one orbit every 2540 days. HD 30177 c was discovered in 2016 and has a mass of 1480 Earth masses, roughly 4.67 times Jupiter's mass and also larger than Earth's. Its orbital period is 11300 days. Among the listed planets, HD 30177 b has the shortest year and the largest reported mass, while HD 30177 c has the longest year and the smallest reported mass.

Provenance

Underlying measurements and references

Evidence Summary

Rows

16

Stellar refs

16

System refs

1

Distancestable

16 values • 1 distinct

Parallaxstable

16 values • 1 distinct

Temperaturedisputed

10 values • 10 distinct

Massdisputed

11 values • 9 distinct

Radiusdisputed

6 values • 6 distinct

Agedisputed

6 values • 5 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

9 values • 9 distinct

Metallicitydisputed

9 values • 6 distinct

Spectral Typedisputed

3 values • 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
55560.931.13———55.59Stassun et al. 2017TICv8
55951.101.043.50-0.02—55.59Ghezzi et al. 2010TICv8
—————G8 V55.59Michigan Catalog, Vol. 1TICv8
—0.951.1411.60——55.59Takeda et al. 2007TICv8
5601—————55.59Suárez-Andrés et al. 2016TICv8
——————55.59Valenti & Fischer 2005TICv8
—0.98————55.59Feng et al. 2022TICv8
55800.99—11.60——55.59Wittenmyer et al. 2017TICv8
55881.01————55.59Santos et al. 2004TICv8
—————G555.59Cannon & Pickering 1918TICv8
56071.051.022.52——55.59Barbato et al. 2018TICv8
—0.95—14.20——55.59Tinney et al. 2003TICv8
5576—1.18—0.08—55.59Gaia DR2TICv8
56800.98—3.55—G8 V55.59Peña et al. 2026TICv8
5545.70.981.19—0.08—55.59TICv8TICv8
55901————55.59Santos et al. 2003TICv8