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Stellar HostProfile

HD 15906

K V • 45.56 pc

Records

3

literature rows

Planets

2

system count

References

4

distinct source labels

HD: HD 15906TIC: TIC 4646810

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: Tuson et al. 2023 • System source: TICv8

Temperature

4757 K

4757 to 4884

3 values • 2 distinct

Mass

0.79 Msun

0.79 to 0.80

2 values • 2 distinct

Radius

0.76 Rsun

0.74 to 0.76

3 values • 2 distinct

Luminosity

-0.57 log(Lsun)

-0.57 to -0.55

2 values • 2 distinct

Distance

45.56 pc

single adopted value

3 values • 1 distinct

Spectral Type

K V

Consistent across records

K V (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.76 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 15906

0.76 R☉

System Layout

Known planets

2 planets linked to this host

HD 15906 b

Transit

◌

Discovery

2023

Period

10.92 days

Radius

2.24 R⊕

Mass

—

Eq. Temp

668 K

HD 15906 c

Transit

◌

Discovery

2023

Period

21.58 days

Radius

2.93 R⊕

Mass

—

Eq. Temp

532 K

HD 15906 and Its Two Planets

HD 15906 is a K V star 149 light-years away. Its spectral type places it among the cooler, redder K-class stars, and the trailing V marks it as a main-sequence dwarf. Astronomers report its mass at 0.79 solar masses, its radius at 0.762 solar radii, and its temperature at 4760 K, making it less massive, smaller, and cooler than the Sun. Two planets are known to orbit this host.

Both planets were discovered by transit in 2023, the method in which a planet crosses in front of its star from our viewpoint and causes a small dip in observed brightness. HD 15906 b is a Super-Earth with a radius of 2.24 Earth radii and an orbital period of 10.9 days. HD 15906 c is Neptune-like, with a radius of 2.93 Earth radii and an orbital period of 21.6 days. The two are respectively the smallest and largest among the listed planets by radius, and their years are the shortest and longest among the listed planets by reported estimates. Both radii exceed Earth's.

Provenance

Underlying measurements and references

Evidence Summary

Rows

3

Stellar refs

3

System refs

1

Distancestable

3 values • 1 distinct

Parallaxstable

3 values • 1 distinct

Temperaturedisputed

3 values • 2 distinct

Massdisputed

2 values • 2 distinct

Radiusdisputed

3 values • 2 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

3 values • 2 distinct

Metallicitydisputed

2 values • 2 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
48840.800.74—-0.55—45.56TICv8TICv8
47570.790.76—-0.57K V45.56Tuson et al. 2023TICv8
4884—0.74———45.56ExoFOPTICv8