Astronomy:HIP 41378

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Short description: Star in the constellation Cancer
HIP 41378
Observation data
Equinox J2000.0]] (ICRS)
Constellation Cancer
Right ascension  08h 26m 27.84909s[1]
Declination +10° 04′ 49.3342″[1]
Apparent magnitude (V) 8.92[2]
Characteristics
Evolutionary stage Main sequence[3]
Spectral type F8[4]
Astrometry
Radial velocity (Rv)50.42±0.37[5] km/s
Proper motion (μ) RA: −48.002±0.020[1] mas/yr
Dec.: 0.062±0.015[1] mas/yr
Parallax (π)9.4360 ± 0.0208[1] mas
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 a star located 346 light-years away in the constellation 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 about 6,251 K.

Planetary system

In 2016, the K2 Kepler mission discovered five planets around HIP 41378, with sizes ranging from 2 times the size of Earth to the size of Jupiter, out to about 1 AU for the outermost planet.[8] The semi-major axes were not known until K2 Haute-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) 		Mass Semimajor axis
(AU) 		Orbital period
(days) 		Eccentricity Inclination Radius
b 6.89 ± 0.88 M⊕ 0.1283 15.57208 ± 0.00002 0.07 ± 0.06 88.75 ± 0.13° 2.17 ± 0.28 R⊕
c 4.4 ± 1.1 M⊕ 0.2161 31.706038 ± 0.00006 0.04 88.477 ± 0.06° 2.727 ± 0.06 R⊕
g 7.0 ± 1.5 M⊕ 0.3227 ± 0.0036 62.06 ± 0.32 0.06 — —
d <4.6 M⊕ 0.88 ± 0.01 278.3618 ± 0.0005 0.06 ± 0.06 89.80 ± 0.02° 3.54 ± 0.06 R⊕
e 12 ± 5 M⊕ 1.06 ± 0.03 369 ± 10 0.14 ± 0.09 89.84 ± 0.07° 4.92 ± 0.09 R⊕
f 12 ± 3 M⊕ 1.37 ± 0.02 542.07975 ± 0.00014 0 89.971 ± 0.01° 9.2 ± 0.1 R⊕

See also

References

  1. ↑ 1.0 1.1 1.2 1.3 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  2. ↑ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P. et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics 355: L27. Bibcode: 2000A&A...355L..27H. 
  3. ↑ 3.0 3.1 3.2 Santerne, 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. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  6. ↑ 6.0 6.1 6.2 6.3 6.4 Petigura, Erik A.; Crossfield, Ian J. M.; Isaacson, Howard; Beichman, Charles A.; Christiansen, Jessie L.; Dressing, Courtney D.; Fulton, Benjamin J.; Howard, Andrew W. et al. (2018). "Planet Candidates from K2 Campaigns 5-8 and Follow-up Optical Spectroscopy". The Astronomical Journal 155 (1): 21. doi:10.3847/1538-3881/aa9b83. Bibcode: 2018AJ....155...21P. 
  7. ↑ "HIP 41378". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HIP+41378. 
  8. ↑ Andrew Vanderburg (2016). "Five Planets Transiting a Ninth Magnitude Star" (in en). The Astrophysical Journal 827 (1): L10. doi:10.3847/2041-8205/827/1/L10. Bibcode: 2016ApJ...827L..10V. 
  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?" (in en). Astronomy & Astrophysics 635: L8. doi:10.1051/0004-6361/202037618. ISSN 0004-6361. https://www.aanda.org/articles/aa/abs/2020/03/aa37618-20/aa37618-20.html. 
  10. ↑ exoplanet.eu Planet HIP 41378 g



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