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Stellar HostProfile

GJ 504

G0Vs • 17.53 pc

Records

34

literature rows

Planets

1

system count

References

18

distinct source labels

TIC: TIC 397587084HD: HD 115383HIP: HIP 64792

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

6234 K

6029.2 to 6291

7 values • 6 distinct

Mass

1.29 Msun

1.12 to 1.29

5 values • 4 distinct

Radius

1.26 Rsun

1.26 to 1.35

5 values • 4 distinct

Age

1.40 Gyr

0.16 to 2.50

4 values • 4 distinct

Luminosity

0.36 log(Lsun)

0.33 to 0.36

4 values • 4 distinct

Distance

17.53 pc

single adopted value

34 values • 1 distinct

Spectral Type

G0Vs

Multiple classifications reported

G0 (1), G0 V (1), G0Vs (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 1.26 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

GJ 504

1.26 R☉

System Layout

Known planets

1 planets linked to this host

GJ 504 b

Imaging

◌

Discovery

2013

Period

—

Radius

—

Mass

1271.3 M⊕

Eq. Temp

510 K

GJ 504 and Its Planet

GJ 504 is a G-type main-sequence star 57.2 light-years away, with a spectral type of G0Vs. One planet is known to orbit it. The star is estimated to be 1.4 billion years old, with a mass of 1.29 solar masses and a radius of 1.26 solar radii. Its temperature is 6230 K, and its reported mass, radius, and temperature are all larger or hotter than the Sun's.

The known planet is GJ 504 b, discovered in 2013 by imaging. Its mass is 1270 Earth masses, which is roughly 4 times Jupiter's mass and larger than Earth's. No orbital period is reported for GJ 504 b.

Provenance

Underlying measurements and references

Evidence Summary

Rows

34

Stellar refs

17

System refs

1

Distancestable

34 values • 1 distinct

Parallaxstable

34 values • 1 distinct

Temperaturedisputed

7 values • 6 distinct

Massdisputed

5 values • 4 distinct

Radiusdisputed

5 values • 4 distinct

Agedisputed

4 values • 4 distinct

Luminositydisputed

4 values • 4 distinct

Surface Gravitydisputed

7 values • 6 distinct

Metallicitydisputed

6 values • 5 distinct

Spectral Typedisputed

3 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
6291—————17.53Swastik et al. 2021TICv8
6130—————17.53Maldonado et al. 2015TICv8
62341.291.261.400.36G0Vs17.53Turnbull 2015TICv8
——————17.53Valenti & Fischer 2005TICv8
——————17.53Duncan et al. 1991TICv8
——————17.53Duncan et al. 1991TICv8
——————17.53Duncan et al. 1991TICv8
——————17.53Duncan et al. 1991TICv8
——————17.53Duncan et al. 1991TICv8
——————17.53Duncan et al. 1991TICv8
——————17.53Duncan et al. 1991TICv8
——————17.53Duncan et al. 1991TICv8
62341.22—0.160.33G0 V17.53Kuzuhara et al. 2013TICv8
——————17.53Pizzolato et al. 2003TICv8
—1.291.260.76——17.53Takeda et al. 2007TICv8
——————17.53Duncan et al. 1991TICv8
——————17.53Duncan et al. 1991TICv8
——————17.53Nidever et al. 2002TICv8
6100—1.34—0.35—17.53Gaia DR2TICv8
——————17.53Duncan et al. 1991TICv8
——————17.53Wright et al. 2004TICv8
—————G017.53Cannon & Pickering 1918TICv8
6029.21.121.35—0.34—17.53TICv8TICv8
——————17.53Duncan et al. 1991TICv8
——————17.53Nordstrom et al. 2004TICv8
——————17.53Duncan et al. 1991TICv8
——————17.53Reiners & Schmitt 2003aTICv8
——————17.53Henry et al. 1996TICv8
——————17.53Duncan et al. 1991TICv8
——————17.53Duncan et al. 1991TICv8
——————17.53Duncan et al. 1991TICv8
62051.221.302.50——17.53D'Orazi et al. 2017TICv8
——————17.53Duncan et al. 1991TICv8
——————17.53Duncan et al. 1991TICv8