Planet HIP 41378 f
| Name | HIP 41378 f | ||
| Planet Status | Confirmed | ||
| Discovered in | 2016 | ||
| Mass | 0.038 (± 0.009) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 1.37 (± 0.02) AU | |
|
| Orbital Period | 542.07975 (± 0.00014) day | |
+ |
| Eccentricity | 0.004 ( -0.003 +0.009 ) | |
|
| ω | — | ||
| Tperi | — | ||
| Radius | 0.821 (± 0.009) RJ | |
+ |
| Inclination | 89.97 (± 0.01) deg | |
|
| Update | 2023-03-28 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | — | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2457186.91451 (± 0.00032) JD | |
|
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | 0.227 (± 0.089) | |
|
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | 335.0 (± 4.0) K | |
|
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
HIP 41378| Name | HIP 41378 | ||
| Distance | 116.0 (± 18.0) pc | |
|
| Spectral type | |||
| Apparent magnitude V | 8.9 | ||
| Mass | 1.15 (± 0.064) MSun | |
|
| Age | — | ||
| Effective temperature | 6199.0 (± 50.0) K | |
|
| Radius | 1.4 (± 0.19) RSun | |
|
| Metallicity [Fe/H] | -0.11 (± 0.08) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 08:26:28.0 | ||
| Dec2000 | +10:04:49 | ||
| Alternate Names | |||
| Planetary system | 5 planets |
Observability Predictor 
Remarks
27 Feb 2020:Akinsamni et al. (2020) suggest there is a ring around the planet, with an inclination of 25 +3/-4 deg. and a position angle 95 +16/-17 deg., leading to a planetary radius of 3.7 +0.3/-0.2 REarth.
Related publications
Stability and detectability of exomoons orbiting HIP 41378 f, a temperate Jovian planet with an anomalously low apparent density
2023
HARADA C., DRESSING C., ALAM M., KIRK J., LOPEZ-MORALES M. et al.
Astron. J., submitted
arxiv
The First Near-Infrared Transmission Spectrum of HIP 41378 f, a Low-Mass Temperate Jovian World in a Multi-Planet System
2022
ALAM M., KIRK J., DRESSING C., LOPEZ-MORALES M., OHNO K. et al.
ApJ. Letters, 927, L5
paper arxiv
A Multi-Planet System's Sole Super-Puff: Exploring Allowable Physical Parameters for the Cold Super-Puff HIP 41378 f
2022
BELKOVSKI M., BECKER J., HOWE A., MALSKY I. & BATYGIN K.
Astron. J., 163, 277
paper arxiv
A transit timing variation observed for the long-period extremely low density exoplanet HIP 41378 f
2021
BRYANT E., BAYLISS D., SANTERNE A., WHEATLEY P., NASCIMBENI V. et al.
MNRAS Letters, 504, L45
paper arxiv
Can planetary rings explain the extremely low density of HIP 41378f?
2020
AKINSANMI B., SANTOS N., FARIA J., OSHAGH M., BARROS S. et al.
Astron. & Astrophys., 635, L8
paper arxiv
A Discrete Set of Possible Transit Ephemerides for Two Long Period Gas Giants Orbiting HIP 41378
2019
BECKER J., VANDERBURG A., RODRIGUEZ J., OMOHUNDRO M., ADAMS F. et al.
Astron. J., 157, 19
paper arxiv
An extremely low-density and temperate giant exoplanet
2019
SANTERNE A., KOSIAREK M., DAI F., DRESSING C., DUMUSQUE X. et al.
Nature Astronomy, submitted
arxiv
Revisiting the HIP41378 system with K2 and Spitzer
2018
BERARDO D., CROSSFIELD I., WERNER M., PETIGURA E.
Astron. J., submitted
arxiv
Five Planets Transiting a Ninth Magnitude Star
2016
VANDERBURG A., BECKER J., KRISTIANSEN M., BIERYLA A., DUEV D. et al.
ApJ Letters, 827, L10
arxiv
paper
ADS
