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Stellar HostProfile

HD 35843

Unclassified star • 69.60 pc

Records

3

literature rows

Planets

2

system count

References

4

distinct source labels

HIP: HIP 25359HD: HD 35843TIC: TIC 7422496

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: Hesse et al. 2025 • System source: TICv8

Temperature

5666 K

5666 to 5744

3 values • 2 distinct

Mass

0.94 Msun

0.94 to 1.03

2 values • 2 distinct

Radius

0.90 Rsun

0.88 to 0.90

3 values • 2 distinct

Age

2.50 Gyr

single adopted value

1 values • 1 distinct

Luminosity

-0.12 log(Lsun)

-0.12 to -0.12

2 values • 2 distinct

Distance

69.60 pc

single adopted value

3 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.90 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 35843

0.90 R☉

System Layout

Known planets

2 planets linked to this host

HD 35843 b

Radial Velocity

◌

Discovery

2025

Period

9.90 days

Radius

—

Mass

5.84 M⊕

Eq. Temp

—

HD 35843 c

Transit

◌

Discovery

2025

Period

46.96 days

Radius

2.54 R⊕

Mass

11.32 M⊕

Eq. Temp

479 K

Planets Around HD 35843

HD 35843 is a star 227 light-years away with two known planets. The star is 2.5 billion years old, has 0.94 solar masses, and a radius of 0.897 solar radii. Its temperature is 5670 K, cooler than the Sun's, and its radius is smaller than the Sun's.

HD 35843 b was discovered in 2025 by the radial velocity method, which measures the wobble a planet's gravity induces in its star. It has a minimum mass of 5.84 Earth masses and an orbital period of 9.9 days, the shortest year among the listed planets. Its minimum mass is larger than Earth's.

HD 35843 c was also discovered in 2025, by the transit method, which detects the dip in starlight as a planet crosses its star. It is Neptune-like, with a mass of 11.3 Earth masses, a radius of 2.54 Earth radii, and an orbital period of 47 days, the longest among the listed planets. Its mass and radius are larger than Earth's, and its mean density is 3.81 g/cm³, 0.691 times 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

Agestable

1 values • 1 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

3 values • 2 distinct

Metallicitystable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
5744—0.88———69.60ExoFOPTICv8
57441.030.88—-0.12—69.60TICv8TICv8
56660.940.902.50-0.12—69.60Hesse et al. 2025TICv8