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Stellar HostProfile

51 Peg

G5V • 15.46 pc

Records

35

literature rows

Planets

1

system count

References

23

distinct source labels

HD: HD 217014HIP: HIP 113357TIC: TIC 139298196

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

5787 K

5758 to 5830

9 values • 9 distinct

Mass

1.05 Msun

1.03 to 1.12

8 values • 7 distinct

Radius

1.15 Rsun

1.15 to 1.29

8 values • 7 distinct

Age

6.76 Gyr

4 to 15

5 values • 4 distinct

Luminosity

0.16 log(Lsun)

0.14 to 0.16

3 values • 3 distinct

Distance

15.46 pc

single adopted value

35 values • 1 distinct

Spectral Type

G5V

Multiple classifications reported

G0 (1), G2 V+ (1), G2.5 IV (1), G3 V (1), G5V (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 1.15 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

51 Peg

1.15 R☉

System Layout

Known planets

1 planets linked to this host

51 Peg b

Radial Velocity

◌

Discovery

1995

Period

4.23 days

Radius

—

Mass

193.9 M⊕

Eq. Temp

—

51 Peg and Its Planet

51 Peg is a G5V star 50.4 light-years away. It has one known planet. The star is 6.76 billion years old, with a mass of 1.05 solar masses, a radius of 1.15 solar radii, and a temperature of 5790 K. Its mass and radius are larger than the Sun's, and it is hotter than the Sun.

The planet 51 Peg b was discovered in 1995 by the radial velocity method, which detects the wobble a planet's gravity induces in its star. It has a mass of 194 Earth masses, larger than Earth's, and orbits in 4.23 days.

Provenance

Underlying measurements and references

Evidence Summary

Rows

35

Stellar refs

22

System refs

1

Distancestable

35 values • 1 distinct

Parallaxstable

35 values • 1 distinct

Temperaturedisputed

9 values • 9 distinct

Massdisputed

8 values • 7 distinct

Radiusdisputed

8 values • 7 distinct

Agedisputed

5 values • 4 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

8 values • 7 distinct

Metallicitydisputed

7 values • 4 distinct

Spectral Typedisputed

5 values • 5 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—1.04————15.46Martins et al. 2015TICv8
5773—1.2910——15.46Mayor & Queloz 1995TICv8
—————G2 V+15.46Gray et al. 2006TICv8
5830—1.16—0.15—15.46Gaia DR2TICv8
5786—————15.46Maldonado et al. 2015TICv8
——————15.46Nordstrom et al. 2004TICv8
—————G015.46Cannon & Pickering 1918TICv8
57931.121.204—G2.5 IV15.46Fuhrmann et al. 1997TICv8
——————15.46Duncan et al. 1991TICv8
58051.04————15.46Santos et al. 2003TICv8
——————15.46Duncan et al. 1991TICv8
——————15.46Nidever et al. 2002TICv8
5760.81.071.19———15.46Rosenthal et al. 2021TICv8
———15——15.46Sanz-Forcada et al. 2010TICv8
——————15.46Duncan et al. 1991TICv8
——————15.46Henry et al. 1996TICv8
——————15.46Duncan et al. 1991TICv8
57581.031.18—0.14—15.46TICv8TICv8
57871.051.156.760.16G5V15.46Turnbull 2015TICv8
——————15.46Naef et al. 2004TICv8
——————15.46Wright et al. 2004TICv8
——————15.46Duncan et al. 1991TICv8
——————15.46Duncan et al. 1991TICv8
57611.071.19———15.46Cont et al. 2026TICv8
——————15.46Duncan et al. 1991TICv8
——————15.46Duncan et al. 1991TICv8
——————15.46Duncan et al. 1991TICv8
——————15.46Duncan et al. 1991TICv8
—1.051.156.76——15.46Takeda et al. 2007TICv8
——————15.46Duncan et al. 1991TICv8
——————15.46Valenti & Fischer 2005TICv8
——————15.46Duncan et al. 1991TICv8
——————15.46Duncan et al. 1991TICv8
——————15.46Duncan et al. 1991TICv8
—————G3 V15.46Gray et al. 2003TICv8