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Stellar HostProfile

HD 45184

G2V • 21.95 pc

Records

16

literature rows

Planets

2

system count

References

17

distinct source labels

HD: HD 45184TIC: TIC 49831913HIP: HIP 30503

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

5810 K

5810 to 5869

7 values • 6 distinct

Mass

1.01 Msun

1.01 to 1.06

6 values • 6 distinct

Radius

1.08 Rsun

1.05 to 1.08

5 values • 4 distinct

Age

6.80 Gyr

single adopted value

2 values • 1 distinct

Luminosity

0.08 log(Lsun)

0.05 to 0.08

5 values • 5 distinct

Distance

21.95 pc

single adopted value

16 values • 1 distinct

Spectral Type

G2V

Multiple classifications reported

G1.5 V (2), G0 (1), G2 V (1), G2V (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.08 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 45184

1.08 R☉

System Layout

Known planets

2 planets linked to this host

HD 45184 b

Radial Velocity

◌

Discovery

2019

Period

5.89 days

Radius

—

Mass

12.19 M⊕

Eq. Temp

—

HD 45184 c

Radial Velocity

◌

Discovery

2019

Period

13.14 days

Radius

—

Mass

8.81 M⊕

Eq. Temp

—

HD 45184: A Sun-Like Star With Two Known Planets

HD 45184 is a G2V star, a Sun-like spectral type, located 71.6 light-years away. Its measured mass is 1.01 solar masses, and its radius is 1.08 solar radii. The star's reported temperature is 5810 K, hotter than the Sun's, and its age is 6.8 billion years. Two planets are known to orbit this host.

Both planets were discovered in 2019 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 45184 b has a minimum mass of 12.2 Earth masses and an orbital period of 5.89 days, giving it the shortest year among the listed planets. HD 45184 c has a minimum mass of 8.81 Earth masses and an orbital period of 13.1 days, the longest year among the listed planets. A minimum mass is a lower bound on a planet's true mass, and both planets' minimum masses are larger than Earth's. Among the listed planets, HD 45184 c has the smallest minimum mass and HD 45184 b has the largest.

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

7 values • 6 distinct

Massdisputed

6 values • 6 distinct

Radiusdisputed

5 values • 4 distinct

Agestable

2 values • 1 distinct

Luminositydisputed

5 values • 5 distinct

Surface Gravitydisputed

7 values • 5 distinct

Metallicitydisputed

6 values • 4 distinct

Spectral Typedisputed

5 values • 4 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
——————21.95Wright et al. 2004TICv8
5840—————21.95Maldonado et al. 2015TICv8
—1.011.086.80——21.95Takeda et al. 2007TICv8
——————21.95Nordstrom et al. 2004TICv8
58541.061.05—0.07—21.95TICv8TICv8
——————21.95Nidever et al. 2002TICv8
58101.011.086.800.08G2V21.95Turnbull 2015TICv8
—————G2 V21.95Michigan Catalog, Vol. 3TICv8
——————21.95Valenti & Fischer 2005TICv8
——————21.95Henry et al. 1996TICv8
5820.11.011.08———21.95Rosenthal et al. 2021TICv8
58691.03——0.05G1.5 V21.95Udry et al. 2019TICv8
—————G1.5 V21.95Gray et al. 2006TICv8
—————G021.95Cannon & Pickering 1918TICv8
5862—1.05—0.07—21.95Gaia DR2TICv8
58691.03——0.05—21.95Sousa et al. 2008TICv8