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Stellar HostProfile

HD 155918

G2V • 27.56 pc

Records

8

literature rows

Planets

2

system count

References

9

distinct source labels

HD: HD 155918TIC: TIC 311649327HIP: HIP 84988

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: Turnbull 2015 • System source: TICv8

Temperature

5752 K

5752 to 5771.8

2 values • 2 distinct

Mass

1.63 Msun

1.03 to 1.63

3 values • 2 distinct

Radius

1.07 Rsun

1.02 to 1.07

2 values • 2 distinct

Age

12.30 Gyr

single adopted value

1 values • 1 distinct

Luminosity

0.05 log(Lsun)

0.02 to 0.05

2 values • 2 distinct

Distance

27.56 pc

single adopted value

8 values • 1 distinct

Spectral Type

G2V

Multiple classifications reported

G0 (1), G2 V (1), G2 V Fe-1.0 CH-0.6 (1), G2V (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.07 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 155918

1.07 R☉

System Layout

Known planets

2 planets linked to this host

HD 155918 b

Radial Velocity

◌

Discovery

2022

Period

1.88 days

Radius

—

Mass

7.63 M⊕

Eq. Temp

—

HD 155918 c

Radial Velocity

◌

Discovery

2022

Period

1.72e4 days

Radius

—

Mass

1878.0 M⊕

Eq. Temp

—

HD 155918 and Its Two Known Planets

HD 155918 is a G2V star 89.9 light-years away, with a reported age of 12.3 billion years, a mass of 1.63 solar masses, a radius of 1.07 solar radii, and a temperature of 5750 K. Two planets have been reported around it.

HD 155918 b was discovered in 2022 by the radial velocity method. Its minimum mass is 7.63 Earth masses, and its orbital period is 1.88 days - the shortest year among the listed planets.

HD 155918 c was also discovered in 2022 by radial velocity. Its mass is 1880 Earth masses, and it takes 17200 days to complete one orbit, the longest among the listed planets. The star's mass and radius estimates are larger than the Sun's, and its temperature is cooler than the Sun's.

Provenance

Underlying measurements and references

Evidence Summary

Rows

8

Stellar refs

8

System refs

1

Distancestable

8 values • 1 distinct

Parallaxstable

8 values • 1 distinct

Temperaturedisputed

2 values • 2 distinct

Massdisputed

3 values • 2 distinct

Radiusdisputed

2 values • 2 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

2 values • 2 distinct

Metallicitydisputed

2 values • 2 distinct

Spectral Typedisputed

4 values • 4 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—————G2 V27.56Michigan Catalog, Vol. 1TICv8
5771.81.031.02—0.02—27.56TICv8TICv8
——————27.56Valenti & Fischer 2005TICv8
——————27.56Nordstrom et al. 2004TICv8
57521.631.0712.300.05G2V27.56Turnbull 2015TICv8
—1.03————27.56Feng et al. 2022TICv8
—————G027.56Cannon & Pickering 1918TICv8
—————G2 V Fe-1.0 CH-0.627.56Gray et al. 2006TICv8