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Stellar HostProfile

HD 1461

G5V • 23.45 pc

Records

17

literature rows

Planets

2

system count

References

18

distinct source labels

HD: HD 1461TIC: TIC 37748347HIP: HIP 1499

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

5765 K

5386 to 5765

9 values • 6 distinct

Mass

1.03 Msun

0.94 to 1.03

8 values • 6 distinct

Radius

1.11 Rsun

1.11 to 1.24

7 values • 5 distinct

Age

7.12 Gyr

7.12 to 13.80

3 values • 2 distinct

Luminosity

0.11 log(Lsun)

0.07 to 0.11

6 values • 5 distinct

Distance

23.45 pc

single adopted value

17 values • 1 distinct

Spectral Type

G5V

Multiple classifications reported

G3 V (2), G0 (1), G0 V (1), G5 V (1), G5V (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.11 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 1461

1.11 R☉

System Layout

Known planets

2 planets linked to this host

HD 1461 b

Radial Velocity

◌

Discovery

2010

Period

5.77 days

Radius

—

Mass

6.44 M⊕

Eq. Temp

—

HD 1461 c

Radial Velocity

◌

Discovery

2015

Period

13.51 days

Radius

—

Mass

5.59 M⊕

Eq. Temp

—

HD 1461 and Its Two Known Planets

HD 1461 is a G5V star 76.5 light-years from Earth. A G-type dwarf is Sun-like, and this one is estimated to be 7.12 billion years old, with a mass of 1.03 solar masses and a radius of 1.11 solar radii. Its temperature is 5770 K. Both planets orbit this star, and both were found by the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion.

The two planets are HD 1461 b and HD 1461 c. HD 1461 b was discovered in 2010, and HD 1461 c in 2015. HD 1461 b has a minimum mass of 6.44 Earth masses and an orbital period of 5.77 days. HD 1461 c has a minimum mass of 5.59 Earth masses and an orbital period of 13.5 days. Among the listed planets, HD 1461 b has the shortest year by reported estimates and the largest minimum mass, while HD 1461 c has the longest year and the smallest minimum mass.

Provenance

Underlying measurements and references

Evidence Summary

Rows

17

Stellar refs

17

System refs

1

Distancestable

17 values • 1 distinct

Parallaxstable

17 values • 1 distinct

Temperaturedisputed

9 values • 6 distinct

Massdisputed

8 values • 6 distinct

Radiusdisputed

7 values • 5 distinct

Agedisputed

3 values • 2 distinct

Luminositydisputed

6 values • 5 distinct

Surface Gravitydisputed

7 values • 5 distinct

Metallicitydisputed

7 values • 4 distinct

Spectral Typedisputed

6 values • 5 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
——————23.45Wright et al. 2004TICv8
57651.031.117.120.11G5V23.45Turnbull 2015TICv8
5764.5—1.12—0.10—23.45Gaia DR2TICv8
—————G3 V23.45Gray et al. 2003TICv8
57651.02——0.07—23.45Sousa et al. 2008TICv8
53860.941.2413.800.07G3 V23.45von Braun et al. 2014TICv8
——————23.45Nidever et al. 2002TICv8
—————G5 V23.45Michigan Catalog, Vol. 5TICv8
5755—————23.45Maldonado et al. 2015TICv8
——————23.45Nordstrom et al. 2004TICv8
—1.031.117.12——23.45Takeda et al. 2007TICv8
57391.031.13—0.10—23.45TICv8TICv8
—————G023.45Cannon & Pickering 1918TICv8
57651.02———G0 V23.45Díaz et al. 2016TICv8
57651.021.11—0.07—23.45Rivera et al. 2010TICv8
——————23.45Valenti & Fischer 2005TICv8
5695.21.031.15———23.45Rosenthal et al. 2021TICv8