HIP 65426 b / Najsakopajk
HIP 65426 b is on the lower left of the image, with the circle representing what Neptune's orbit would look like around the star HIP 65426, represented by a small cross.
Discovery[1]
Discovered bySPHERE consortium[2]
Discovery date6 July 2017
Direct imaging
Designations
Najsakopajk[3]
Orbital characteristics
87+108
−31 au[4]
Inclination100+15
−6 deg[4]
Physical characteristics
Mean radius
Atmospheric model:
0.92±0.04 RJ[4]
Evolutionary model:
1.45±0.03 RJ[4]
Mass7.1±1.1 MJ[4]
4.07±0.19 dex
TemperatureAtmospheric model:
1667+25
−24 K[4]

1560±100 K[5]

Evolutionary model:
1282+26
−31 K[4]

    HIP 65426 b, formally named Najsakopajk,[3] is a super-Jupiter exoplanet orbiting the star HIP 65426. It was discovered on 6 July 2017 by the SPHERE consortium using the Spectro-Polarimetric High-Contrast Exoplanet Research (SPHERE) instrument belonging to the European Southern Observatory (ESO).[6][7] It is 385 light-years from Earth.[8] It is the first planet discovered by ESO's SPHERE instrument.[9]

    Nomenclature

    In August 2022, this planet and its host star were included among 20 systems to be named by the third NameExoWorlds project.[10] The approved names, proposed by a team from Mexico, were announced in June 2023. HIP 65426 b is named Najsakopajk and its host star is named Matza, after Zoque words for "Mother Earth" and "star".[3]

    Overview

    The exoplanet HIP 65426 b orbits its host star HIP 65426, an A2V star with apparent magnitude 7.01 and a mass of 1.96±0.04 M☉.[11] This planetary system is located in the constellation Centaurus. The planet is around 14 million years old. However, it is not associated with a debris disk, despite its young age,[7][8] causing it to not fit current models for planetary formation.[12] It is around 92 AU from its parent star, with a possible dusty atmosphere.[13] It was discovered as part of the SHINE program, which aimed to find planetary systems around 600 new stars.[1]

    In September 2022, HIP 65426 b became the first exoplanet directly observed by the James Webb Space Telescope.[14]

    Planetary atmosphere

    The spectrum taken in 2020 has indicated that HIP 65426 b is carbon-poor and oxygen-rich compared to Solar System gas giants.[5]

    Spectral analysis of data from the James Webb Space Telescope revealed strong evidence of silicate clouds containing enstatite with no evidence of a dusty atmosphere.[15]

    James Webb Space Telescope observation

    In August 2022, a pre-print of the James Webb Space Telescope (JWST) observations was published. The JWST direct imaging observations between 2-16 μm of HIP 65426 b tightly constrained its bolometric luminosity to , which provides a robust mass constraint of 7.1±1.1 MJ. The atmospheric fitting of both temperature and radius are in disagreement with evolutionary models. The team also constrained the semi-major axis and the inclination of the planet, but the new JWST astrometry of the planet did not significantly improve the orbit of the planet, especially the eccentricity remains unconstrained.[4]

    HIP 65426 b is the first exoplanet to be imaged by JWST and the first exoplanet to be detected beyond 5 μm. The observations demonstrate that the James Webb Space Telescope will exceed its nominal predicted performance by a factor of 10 and that it will be able to image 0.3 MJ planets at 100 au for main-sequence stars, Neptune and Uranus-mass objects at 100-200 au for M-dwarfs and Saturn-mass objects at 10 au for M-dwarfs. For α Cen A JWST might be able to push the limit to a 5 R🜨 planet at 0.5 to 2.5 au.[4]

    HIP 65426 star map
    HIP 65426 b viewed by the James Webb Space Telescope (August 2022)

    See also

    References

    1. 1 2 Chauvin, G.; Desidera, S.; Lagrange, A. -M.; Vigan, A.; Gratton, R.; Langlois, M.; Bonnefoy, M.; Beuzit, J. -L.; Feldt, M.; Mouillet, D.; Meyer, M.; Cheetham, A.; Biller, B.; Boccaletti, A.; d'Orazi, V.; Galicher, R.; Hagelberg, J.; Maire, A. -L.; Mesa, D.; Olofsson, J.; Samland, M.; Schmidt, T. O. B.; Sissa, E.; Bonavita, M.; Charnay, B.; Cudel, M.; Daemgen, S.; Delorme, P.; Janin-Potiron, P.; et al. (2017). "Discovery of a warm, dusty giant planet around HIP 65426". Astronomy and Astrophysics. 605: L9. arXiv:1707.01413. Bibcode:2017A&A...605L...9C. doi:10.1051/0004-6361/201731152. S2CID 102344893.
    2. ↑ "Odd planetary system around fast-spinning star doesn't quite fit existing models of planet formation". www.sphere.osug.fr. Retrieved 2017-07-06.
    3. 1 2 3 "2022 Approved Names". nameexoworlds.iau.org. IAU. Retrieved 7 June 2023.
    4. 1 2 3 4 5 6 7 8 9 Carter, Aarynn L.; Hinkley, Sasha; Kammerer, Jens; Skemer, Andrew; Biller, Beth A.; Leisenring, Jarron M.; Millar-Blanchaer, Maxwell A.; Petrus, Simon; Stone, Jordan M.; Ward-Duong, Kimberly; Wang, Jason J.; Girard, Julien H.; Hines, Dean C.; Perrin, Marshall D.; Pueyo, Laurent (2023-07-06). "The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems I: High Contrast Imaging of the Exoplanet HIP 65426 b from 2-16 μm". The Astrophysical Journal Letters. 951 (1): L20. arXiv:2208.14990. Bibcode:2023ApJ...951L..20C. doi:10.3847/2041-8213/acd93e.
    5. 1 2 Petrus, S.; Bonnefoy, M.; Chauvin, G.; Charnay, B.; Marleau, G.-D.; Gratton, R.; Lagrange, A.-M.; Rameau, J.; Mordasini, C.; Nowak, M.; Delorme, P.; Boccaletti, A.; Carlotti, A.; Houllé, M.; Vigan, A.; Allard, F.; Desidera, S.; d'Orazi, V.; Hoeijmakers, H. J.; Wyttenbach, A.; Lavie, B. (2021), "Medium-resolution spectrum of the exoplanet HIP 65426 B", Astronomy & Astrophysics, 648: A59, arXiv:2012.02798, Bibcode:2021A&A...648A..59P, doi:10.1051/0004-6361/202038914, S2CID 227347064
    6. ↑ "Scientists have found a planet that means everything they thought about planets isn't true". The Independent. 2017-07-08. Retrieved 2019-08-02.
    7. 1 2 "Astronomers Directly Image Super-Jupiter around HIP 65426 | Astronomy | Sci-News.com". Breaking Science News | Sci-News.com. Retrieved 2019-08-02.
    8. 1 2 "Holiday Special: Eight nights of Exoplanet Light". Exoplanet Exploration: Planets Beyond our Solar System. NASA. Retrieved 2019-08-03.
    9. ↑ "ESO's SPHERE Unveils its First Exoplanet". www.eso.org. Retrieved 2017-07-07.
    10. ↑ "List of ExoWorlds 2022". nameexoworlds.iau.org. IAU. 8 August 2022. Retrieved 27 August 2022.
    11. ↑ "The Extrasolar Planet Encyclopaedia — HIP 65426 b". Extrasolar Planets Encyclopaedia. Paris Observatory.
    12. ↑ "Odd planetary system around fast-spinning star doesn't quite fit existing models of planet formation". phys.org. Retrieved 2019-08-03.
    13. ↑ Johnson-Groh, Mara; July 12, 2017 (12 July 2017). "New exoplanet challenges formation models". Astronomy.com. Retrieved 2019-08-03.{{cite web}}: CS1 maint: numeric names: authors list (link)
    14. ↑ Fisher, Alise (2022-09-01). "NASA's Webb Takes Its First-Ever Direct Image of Distant World". NASA Blogs. NASA. Retrieved 2022-09-01.
    15. ↑ Wang 王, Ji 吉 (2023-11-01). "Spectral Retrieval with JWST Photometric data: a Case Study for HIP 65426 b". The Astronomical Journal. 166 (5): 203. arXiv:2310.00089. Bibcode:2023AJ....166..203W. doi:10.3847/1538-3881/acfca0. ISSN 0004-6256.
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