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Stellar HostProfile

HD 147873

G1 V • 109.1 pc

Records

7

literature rows

Planets

2

system count

References

8

distinct source labels

TIC: TIC 211080657HIP: HIP 80486HD: HD 147873

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: Jenkins et al. 2017 • System source: TICv8

Temperature

5972 K

5972 to 6169

3 values • 3 distinct

Mass

1.38 Msun

1.18 to 1.38

2 values • 2 distinct

Radius

2.29 Rsun

2.29 to 2.45

3 values • 3 distinct

Age

4 Gyr

single adopted value

1 values • 1 distinct

Luminosity

0.78 log(Lsun)

0.78 to 0.89

3 values • 3 distinct

Distance

109.1 pc

single adopted value

7 values • 1 distinct

Spectral Type

G1 V

Multiple classifications reported

G1 V (2), G0 (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 2.29 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 147873

2.29 R☉

System Layout

Known planets

2 planets linked to this host

HD 147873 b

Radial Velocity

◌

Discovery

2016

Period

116.6 days

Radius

—

Mass

1633.6 M⊕

Eq. Temp

—

HD 147873 c

Radial Velocity

◌

Discovery

2016

Period

491.5 days

Radius

—

Mass

731.0 M⊕

Eq. Temp

—

HD 147873 and Its Two Known Planets

HD 147873 is a G1 V star located 356 light-years away, and it is known to host two planets. The star is a main-sequence dwarf classified as Sun-like, with an age of 4 billion years, a mass of 1.38 solar masses, a radius of 2.29 solar radii, and a temperature of 5970 K. Its reported mass and radius estimates are both larger than the Sun's, and its reported temperature is hotter than the Sun's.

Both known planets were discovered in 2016 using the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion. HD 147873 b has a minimum mass of 1630 Earth masses, which is a lower bound on its true mass and roughly 5.14 times Jupiter's mass, and an orbital period of 117 days. HD 147873 c has a minimum mass of 731 Earth masses, also a lower bound and roughly 2.3 times Jupiter's mass, and an orbital period of 492 days. The minimum masses of both planets are larger than Earth's. Among the listed planets, HD 147873 b has the shortest year and the largest minimum mass, while HD 147873 c has the longest year and the smallest minimum mass.

Provenance

Underlying measurements and references

Evidence Summary

Rows

7

Stellar refs

7

System refs

1

Distancestable

7 values • 1 distinct

Parallaxstable

7 values • 1 distinct

Temperaturedisputed

3 values • 3 distinct

Massdisputed

2 values • 2 distinct

Radiusdisputed

3 values • 3 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

2 values • 2 distinct

Metallicitystable

1 values • 1 distinct

Spectral Typedisputed

3 values • 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
61691.182.45—0.89—109.1TICv8TICv8
——————109.1Nordstrom et al. 2004TICv8
—————G1 V109.1Michigan Catalog, Vol. 3TICv8
—————G0109.1Cannon & Pickering 1918TICv8
——————109.1Henry et al. 1996TICv8
6016.2—2.36—0.82—109.1Gaia DR2TICv8
59721.382.2940.78G1 V109.1Jenkins et al. 2017TICv8