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Stellar HostProfile

HIP 41378

Unclassified star • 106.3 pc

Records

12

literature rows

Planets

6

system count

References

12

distinct source labels

TIC: TIC 366443426HIP: HIP 41378

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: Becker et al. 2019 • System source: TICv8

Temperature

6199 K

6169 to 6371

9 values • 6 distinct

Mass

1.14 Msun

1.14 to 1.26

6 values • 6 distinct

Radius

1.35 Rsun

1.27 to 1.40

11 values • 10 distinct

Age

4.28 Gyr

1.80 to 4.28

2 values • 2 distinct

Distance

106.3 pc

single adopted value

12 values • 1 distinct

Planets

6

Stable across source rows

6

Scale Comparison

Radius against the Sun

Current adopted radius: 1.35 R☉ • circles scaled linearly by radius

Sun

1.0 R☉ baseline

HIP 41378

1.35 R☉

System Layout

Known planets

6 planets linked to this host

Discovery

2016

Period

15.57 days

Radius

2.42 R⊕

Mass

9.06 M⊕

Eq. Temp

970.7 K

Discovery

2016

Period

31.71 days

Radius

2.50 R⊕

Mass

6.53 M⊕

Eq. Temp

765.9 K

Discovery

2016

Period

278.4 days

Radius

3.54 R⊕

Mass

4.60 M⊕

Eq. Temp

367 K

Discovery

2016

Period

369 days

Radius

4.92 R⊕

Mass

12 M⊕

Eq. Temp

335 K

Discovery

2016

Period

542.1 days

Radius

Mass

Eq. Temp

HIP 41378 g

Radial Velocity

Discovery

2025

Period

64.07 days

Radius

Mass

6.81 M⊕

Eq. Temp

Planets of HIP 41378

HIP 41378 is a star 347 light-years away with six planets. The star is an F6 type with an age of 4.28 billion years, a mass of 1.14 solar masses, a radius of 1.35 solar radii, and a temperature of 6200 K. Its reported mass and radius estimates are larger than the Sun's, and its reported temperature is hotter than the Sun's.

HIP 41378 b, c, and d are Neptune-like planets, each with a radius and mass larger than Earth's. HIP 41378 b has a mass of 6.9 Earth masses, a radius of 2.64 Earth radii, and an orbital period of 15.6 days. HIP 41378 c has a mass of 5.97 Earth masses, a radius of 2.74 Earth radii, and an orbital period of 31.7 days. HIP 41378 d has a mass of 6.53 Earth masses, a radius of 3.65 Earth radii, and an orbital period of 278 days.

HIP 41378 e and f are Jupiter-like planets, both with a radius and mass larger than Earth's. HIP 41378 e has a mass of 7.62 Earth masses, a radius of 5.19 Earth radii, and an orbital period of 393 days. HIP 41378 f has a mass of 25 Earth masses, a radius of 9.47 Earth radii, and an orbital period of 542 days.

HIP 41378 g was discovered by radial velocity and has a minimum mass of 5.75 Earth masses and an orbital period of 63.2 days. Among the listed planets, HIP 41378 b has the shortest year at 15.6 days, HIP 41378 c has the second-shortest at 31.7 days, HIP 41378 e has the second-longest at 393 days, and HIP 41378 f has the longest at 542 days.

Provenance

Underlying measurements and references

Evidence Summary

Rows

12

Stellar refs

11

System refs

1

Distancestable

12 values • 1 distinct

Parallaxstable

12 values • 1 distinct

Temperaturedisputed

9 values • 6 distinct

Massdisputed

6 values • 6 distinct

Radiusdisputed

11 values • 10 distinct

Agedisputed

2 values • 2 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

7 values • 5 distinct

Metallicitydisputed

5 values • 4 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
6352.31.31106.3ExoFOPTICv8
6352.31.261.310.40106.3TICv8TICv8
6352.31.31106.3ExoFOPTICv8
1.30106.3Grouffal et al. 2025TICv8
63711.251.311.80106.3Leonardi et al. 2025TICv8
61991.141.354.28106.3Becker et al. 2019TICv8
62261.171.34106.3Berardo et al. 2019TICv8
F6106.3Luo et al. 2018TICv8
61991.151.40106.3Vanderburg et al. 2016TICv8
1.28106.3Grouffal et al. 2022TICv8
63201.161.27106.3Howard et al. 2025TICv8
61691.380.40106.3Gaia DR2TICv8