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Stellar HostProfile

HD 105618

Unclassified star • 70.08 pc

Records

2

literature rows

Planets

2

system count

References

3

distinct source labels

TIC: TIC 397519199HD: HD 105618

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

5671 K

single adopted value

1 values • 1 distinct

Mass

1.01 Msun

single adopted value

2 values • 1 distinct

Radius

1.27 Rsun

single adopted value

1 values • 1 distinct

Luminosity

0.18 log(Lsun)

single adopted value

1 values • 1 distinct

Distance

70.08 pc

single adopted value

2 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.27 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 105618

1.27 R☉

System Layout

Known planets

2 planets linked to this host

HD 105618 b

Radial Velocity

◌

Discovery

2022

Period

10.02 days

Radius

—

Mass

25.43 M⊕

Eq. Temp

—

HD 105618 c

Radial Velocity

◌

Discovery

2022

Period

7.71e4 days

Radius

—

Mass

8419.6 M⊕

Eq. Temp

—

HD 105618 and Its Two Known Planets

HD 105618 is a star located 229 light-years away. It has 1.01 solar masses, a radius of 1.27 solar radii, and a temperature of 5670 K. Its reported radius estimate is larger than the Sun's, and its reported temperature is cooler than the Sun's. Two planets are known to orbit this host.

HD 105618 b was discovered in 2022 by the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion. It has a minimum mass of 25.4 Earth masses and an orbital period of 10 days, the shortest year among the listed planets by reported estimates. Its minimum mass is larger than Earth's.

HD 105618 c was also discovered in 2022 by radial velocity. Its reported mass estimate is 8420 Earth masses, roughly 26.5 times Jupiter's mass, and larger than Earth's. Its orbital period is 77100 days, the longest year among the listed planets by reported estimates.

Provenance

Underlying measurements and references

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Evidence Summary

Rows

2

Stellar refs

2

System refs

1

Distancestable

2 values • 1 distinct

Parallaxstable

2 values • 1 distinct

Temperaturestable

1 values • 1 distinct

Massstable

2 values • 1 distinct

Radiusstable

1 values • 1 distinct

Luminositystable

1 values • 1 distinct

Surface Gravitystable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
56711.011.27—0.18—70.08TICv8TICv8
—1.01————70.08Feng et al. 2022TICv8