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HIP 41378

From Wikipedia, the free encyclopedia
Star in the constellation Cancer
HIP 41378
Observation data
Epoch J2000      Equinox J2000
ConstellationCancer
Right ascension08h 26m 27.84909s[1]
Declination+10° 04′ 49.3342″[1]
Apparent magnitude (V)8.92[2]
Characteristics
Evolutionary stageMain sequence[3]
Spectral typeF8[4]
Astrometry
Radial velocity (Rv)50.42±0.37[5] km/s
Proper motion (μ)RA: −48.002±0.020mas/yr[1]
Dec.: 0.062±0.015mas/yr[1]
Parallax (π)9.4360±0.0208 mas[1]
Distance345.7 ± 0.8 ly
(106.0 ± 0.2 pc)
Details
Mass1.15+0.06
−0.05
[6] M
Radius1.25+0.16
−0.11
[6] R
Surface gravity (log g)4.28 cgs
Temperature6,251[6] K
Metallicity [Fe/H]0.00[6] dex
Rotational velocity (v sin i)5.7[6] km/s
Other designations
BD+10°1799,HIP 41378,PPM 125260,YZ 10 3402, AG+10 1097,EPIC 211311380[7]
Database references
SIMBADdata

HIP 41378 is astar located 346light-years away in theconstellation of Cancer. The star has an apparent magnitude of 8.92. This F-type main sequence dwarf has a mass of 1.15 M and a radius of 1.25 R. It has a surface temperature of about6,251 K.

Planetary system

[edit]

In 2016, theK2 Kepler mission discovered five planets around HIP 41378, with sizes ranging from 2 times the size of Earth to the size ofJupiter, out to about 1 AU for the outermost planet.[8] The semi-major axes were not known until K2Haute-Provence Observatory radial velocity data was obtained in 2019. Also, a sixth non-transiting planet, HIP 41378 g, was discovered, along with speculation that additional planets may exist between HIP 41378 g and HIP 41378 d. The planet HIP 41378 f was also found to likely have optically-thick rings or a highly extended atmosphere.[3][9]

The HIP 41378 planetary system[3][10]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b6.89 ± 0.88 M🜨0.128315.57208 ± 0.000020.07 ± 0.0688.75 ± 0.13°2.17 ± 0.28 R🜨
c4.4 ± 1.1 M🜨0.216131.706038 ± 0.000060.0488.477 ± 0.06°2.727 ± 0.06 R🜨
g7.0 ± 1.5 M🜨0.3227 ± 0.003662.06 ± 0.320.06
d<4.6 M🜨0.88 ± 0.01278.3618 ± 0.00050.06 ± 0.0689.80 ± 0.02°3.54 ± 0.06 R🜨
e12 ± 5 M🜨1.06 ± 0.03369 ± 100.14 ± 0.0989.84 ± 0.07°4.92 ± 0.09 R🜨
f12 ± 3 M🜨1.37 ± 0.02542.07975 ± 0.00014089.971 ± 0.01°9.2 ± 0.1 R🜨

See also

[edit]

References

[edit]
  1. ^abcdVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  2. ^Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".Astronomy and Astrophysics.355: L27.Bibcode:2000A&A...355L..27H.
  3. ^abcSanterne, A.; Malavolta, L.; Kosiarek, M. R.; Dai, F.; Dressing, C. D.; Dumusque, X.; Hara, N. C.; Lopez, T. A.; Mortier, A.; Vanderburg, A.; Adibekyan, V.; Armstrong, D. J.; Barrado, D.; Barros, S. C. C.; Bayliss, D.; Berardo, D.; Boisse, I.; Bonomo, A. S.; Bouchy, F.; Brown, D. J. A.; Buchhave, L. A.; Butler, R. P.; Collier Cameron, A.; Cosentino, R.; Crane, J. D.; Crossfield, I. J. M.; Damasso, M.; Deleuil, M. R.; Delgado Mena, E.; et al. (2019). "An extremely low-density and temperate giant exoplanet".arXiv:1911.07355 [astro-ph.EP].
  4. ^Hill, Sarah J.; Schilt, Jan (1952). "Photographic magnitudes of 55700 stars in the zones 10 deg to 20 deg and 30 deg to 50 deg".Contributions from the Rutherford Observatory of Columbia University New York.32: 1.Bibcode:1952CoRut..32....1H.
  5. ^Brown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source atVizieR.
  6. ^abcdePetigura, Erik A.; Crossfield, Ian J. M.; Isaacson, Howard; Beichman, Charles A.; Christiansen, Jessie L.; Dressing, Courtney D.; Fulton, Benjamin J.; Howard, Andrew W.; Kosiarek, Molly R.; Lépine, Sébastien; Schlieder, Joshua E.; Sinukoff, Evan; Yee, Samuel W. (2018)."Planet Candidates from K2 Campaigns 5-8 and Follow-up Optical Spectroscopy".The Astronomical Journal.155 (1): 21.arXiv:1711.06377.Bibcode:2018AJ....155...21P.doi:10.3847/1538-3881/aa9b83.S2CID 55674757.
  7. ^"HIP 41378".SIMBAD.Centre de données astronomiques de Strasbourg.
  8. ^Andrew Vanderburg; et al. (2016)."Five Planets Transiting a Ninth Magnitude Star".The Astrophysical Journal.827 (1): L10.arXiv:1606.08441.Bibcode:2016ApJ...827L..10V.doi:10.3847/2041-8205/827/1/L10.S2CID 8794583.
  9. ^Akinsanmi, B.; Santos, N. C.; Faria, J. P.; Oshagh, M.; Barros, S. C. C.; Santerne, A.; Charnoz, S. (2020-03-01)."Can planetary rings explain the extremely low density of HIP 41378 𝑓?".Astronomy & Astrophysics.635: L8.arXiv:2002.11422.doi:10.1051/0004-6361/202037618.ISSN 0004-6361.
  10. ^exoplanet.eu Planet HIP 41378 g
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