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HIP 41378
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Star HIP 41378

Yellow-White star HIP 41378 is located 346 light years away from the Sun. It is a single star of spectral class F8 D, that has 115 % of solar mass. There are multiple known exoplanets in this system.
Sun distance
346 light years
galaxy map

HIP 41378

Yellow-White star
Spectral class: F8 D

Location

Ascension iconRight ascension: 8h 26m 27.854s
Declination iconDeclination: 10° 4' 49.334'' (equatorial region)
Parallax iconParallax: 9.436
Distance iconSun distance: 345.651 ly | 106 pc

Basic characteristic

icon weight
Mass: 115 % M Sun | 1205 M Jupiter
radius icon
Size: 128 % R Sun | 12.7 R Jupiter
temperature iconTemperature: 6290 K | 1.09 T Sun

Photometry

Magnitude iconApparent magnitude (V): 8.9
Magnitude iconAbsolute magnitude (V): 3.8
5
10
15
20
25
30
35
K
2.1
H
1.6
J
1.2
Grp
0.8
I
0.8
G
0.6
V
0.5
Gbp
0.5
B
0.4
U
0.3
Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).

HIP 41378 system structure

 HIP 41378
HIP 41378 b n/a 2.9 R⊕ 15.6 days
HIP 41378 c n/a 2.9 R⊕ 15.6 days
HIP 41378 d n/a 4 R⊕ 278.4 days
HIP 41378 e n/a 5.5 R⊕ 131 days
HIP 41378 g
unconfirmed
 0.32 AU 7 M⊕ 62.1 days
HIP 41378 f 1.37 AU 12.1 M⊕ 9.2 R⊕ 542.1 days
More about HIP 41378
Star HIP 41378 is a main sequence star that fuses hydrogen atoms into helium. It is is approximately 28 % bigger than the Sun and temperature on its surface is around 6290 K (6017 °C), which is about 109 % of Sun's temperature.
       HIP 41378 can be found in northern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is easily observable from Northern America, Europe and Asia.
Other designations of this star
K2-93, EPIC 211311380, BD+10 1799, 2MASS J08262784+1004493, TIC 366443426, TYC 800-1325-1
External sources
icon study
The Dynamical History of HIP-41378 f -- Oblique Exorings Masquerading as a Puffy Planet
Scientific study, Accepted: 01. 10. 2024
icon study
HIP 41378 observed by CHEOPS: Where is planet d?
Scientific study, Accepted: 30. 05. 2024
icon study
Clouds and Clarity: Revisiting Atmospheric Feature Trends in Neptune-size Exoplanets
Scientific study, Accepted: 11. 10. 2023
icon study
Oblique rings from migrating exomoons: A possible origin for long-period exoplanets with enlarged radii
Scientific study, Accepted: 12. 06. 2023
tess icon
TESS database (TOI 4304.01)
Archive from the TESS mission
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