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Stellar HostProfile

HD 177830

Unclassified star • 62.77 pc

Records

15

literature rows

Planets

2

system count

References

16

distinct source labels

TIC: TIC 265052133HD: HD 177830HIP: HIP 93746

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: Jofré et al. 2015 • System source: TICv8

Temperature

5058 K

4744.9 to 5058

9 values • 9 distinct

Mass

1.37 Msun

1.03 to 1.91

7 values • 7 distinct

Radius

2.81 Rsun

2.62 to 3.58

7 values • 6 distinct

Age

3.46 Gyr

3.24 to 4.40

3 values • 3 distinct

Luminosity

0.60 log(Lsun)

0.60 to 0.77

3 values • 3 distinct

Distance

62.77 pc

single adopted value

15 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 2.81 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 177830

2.81 R☉

System Layout

Known planets

2 planets linked to this host

HD 177830 b

Radial Velocity

◌

Discovery

1999

Period

410.1 days

Radius

—

Mass

537.1 M⊕

Eq. Temp

—

HD 177830 c

Radial Velocity

◌

Discovery

2010

Period

110.9 days

Radius

—

Mass

47.67 M⊕

Eq. Temp

—

HD 177830 and Its Two Known Planets

HD 177830 is a K0 star located 205 light-years away. Its reported mass is 1.37 solar masses and its reported radius is 2.81 solar radii, both larger than the Sun's corresponding values. The star's reported temperature of 5060 K is cooler than the Sun's, and its age is given as 3.46 billion years. Two planets have been found around this star.

HD 177830 b was discovered in 1999 by the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion. The planet's minimum mass is 537 Earth masses and its orbital period is 410 days; among the listed planets, it has the longest year. That minimum mass is larger than Earth's and is roughly 1.69 times Jupiter's mass.

HD 177830 c was discovered in 2010, also by radial velocity. Its minimum mass is 47.7 Earth masses and its orbital period is 111 days; among the listed planets, it has the shortest year and the smallest minimum mass. Its minimum mass is likewise larger than Earth's, while the minimum mass of HD 177830 b remains the largest among the listed planets.

A minimum mass is a lower bound on a planet's true mass, so these figures represent how light each world could be rather than its exact mass.

Provenance

Underlying measurements and references

Evidence Summary

Rows

15

Stellar refs

15

System refs

1

Distancestable

15 values • 1 distinct

Parallaxstable

15 values • 1 distinct

Temperaturedisputed

9 values • 9 distinct

Massdisputed

7 values • 7 distinct

Radiusdisputed

7 values • 6 distinct

Agedisputed

3 values • 3 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

8 values • 8 distinct

Metallicitydisputed

8 values • 8 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
49491.472.624.400.69—62.77Meschiari et al. 2011TICv8
——————62.77Valenti & Fischer 2005TICv8
48401.03————62.77Santos et al. 2003TICv8
49011.703.26———62.77Stassun et al. 2017TICv8
——————62.77Duncan et al. 1991TICv8
—————K062.77Cannon & Pickering 1918TICv8
4923.8—3.31———62.77TICv8TICv8
4847.5—3.45—0.77—62.77Gaia DR2TICv8
——————62.77Nidever et al. 2002TICv8
4804—————62.77Santos et al. 2004TICv8
——————62.77Wright et al. 2004TICv8
50581.372.813.460.60—62.77Jofré et al. 2015TICv8
47521.17————62.77Mortier et al. 2013TICv8
—1.912.623.24——62.77Takeda et al. 2007TICv8
4744.91.323.58———62.77Rosenthal et al. 2021TICv8