←Back to Stellar Hosts
Stellar HostProfile

HD 24040

Unclassified star • 46.62 pc

Records

15

literature rows

Planets

2

system count

References

16

distinct source labels

TIC: TIC 456863621HD: HD 24040HIP: HIP 17960

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: TICv8 • System source: TICv8

Temperature

5761 K

5761 to 5853

6 values • 6 distinct

Mass

1.03 Msun

1.03 to 1.22

9 values • 7 distinct

Radius

1.38 Rsun

1.26 to 1.39

5 values • 5 distinct

Luminosity

0.28 log(Lsun)

0.28 to 0.28

2 values • 2 distinct

Distance

46.62 pc

single adopted value

15 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.38 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 24040

1.38 R☉

System Layout

Known planets

2 planets linked to this host

HD 24040 b

Radial Velocity

◌

Discovery

2006

Period

3668 days

Radius

—

Mass

1226.8 M⊕

Eq. Temp

—

HD 24040 c

Radial Velocity

◌

Discovery

2021

Period

515.4 days

Radius

—

Mass

63.88 M⊕

Eq. Temp

—

HD 24040 and Its Two Known Planets

HD 24040 is a G-type dwarf star 152 light-years away. Its mass is 1.03 solar masses, its radius is 1.38 solar radii, and its temperature is 5760 K. The star's reported radius estimate is larger than the Sun's. Two planets are known to orbit it.

HD 24040 b was discovered in 2006 by the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion. Its minimum mass is 1230 Earth masses, which is roughly 3.86 times Jupiter's mass, and its orbital period is 3670 days. Among the listed planets, it has the longest year and the largest minimum mass.

HD 24040 c was discovered in 2021 by the radial velocity method. It has a minimum mass of 63.9 Earth masses and an orbital period of 515 days. Among the listed planets, it has the shortest year and the smallest minimum mass.

Provenance

Underlying measurements and references

Evidence Summary

Rows

15

Stellar refs

15

System refs

1

Distancestable

15 values • 1 distinct

Parallaxstable

15 values • 1 distinct

Temperaturedisputed

6 values • 6 distinct

Massdisputed

9 values • 7 distinct

Radiusdisputed

5 values • 5 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

6 values • 6 distinct

Metallicitydisputed

5 values • 5 distinct

Spectral Typedisputed

2 values • 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
——————46.62Valenti & Fischer 2005TICv8
58531.18———G0 V46.62Wright et al. 2007TICv8
—1.091.266.68——46.62Takeda et al. 2007TICv8
57611.031.38—0.28—46.62TICv8TICv8
58021.111.30———46.62Stassun et al. 2017TICv8
5805—1.36—0.28—46.62Gaia DR2TICv8
——————46.62Nordstrom et al. 2004TICv8
——————46.62Nidever et al. 2002TICv8
5776.51.101.39———46.62Rosenthal et al. 2021TICv8
—1.18————46.62Bryan et al. 2016TICv8
—————G046.62Cannon & Pickering 1918TICv8
——————46.62Wright et al. 2004TICv8
—1.18————46.62Boisse et al. 2012TICv8
58401.10————46.62Santos et al. 2013TICv8
—1.22————46.62An et al. 2025TICv8