Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-25T02:27:20.787Z Has data issue: false hasContentIssue false
  • English
  • Français

Influence of the magnetic field of stellar wind on hot jupiter’s envelopes

Published online by Cambridge University Press:  24 September 2020

Dmitry V. Bisikalo  and
Andrey G. Zhilkin Open the ORCID record for Andrey G. Zhilkin [Opens in a new window]
Dmitry V. Bisikalo
Affiliation:
Institute of Astronomy of the RAS, 48 Pyatnitskaya str., Moscow, Russia email: [email protected]
Andrey G. Zhilkin
Affiliation:
Institute of Astronomy of the RAS, 48 Pyatnitskaya str., Moscow, Russia email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Hot Jupiters have extended gaseous (ionospheric) envelopes, which extend far beyond the Roche lobe. The envelopes are loosely bound to the planet and, therefore, are strongly influenced by fluctuations of the stellar wind. We show that, since hot Jupiters are close to the parent stars, magnetic field of the stellar wind is an important factor defining the structure of their magnetospheres. For a typical hot Jupiter, velocity of the stellar wind plasma flow around the atmosphere is close to the Alfvén velocity. As a result stellar wind fluctuations, such as coronal mass ejections, can affect the conditions for the formation of a bow shock around a hot Jupiter. This effect can affect observational manifestations of hot Jupiters.

Keywords

MHDstars: windsstars: planetary systems
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S354: Solar and Stellar Magnetic Fields: Origins and Manifestations , June 2019 , pp. 268 - 279
Copyright
© International Astronomical Union 2020

References

Arakcheev, A.S., Zhilkin, A.G., Kaigorodov, P.V., et al. 2017, Astronomy Reports, 61, 932 CrossRefGoogle Scholar
Ben-Jaffel, L. 2007, ApJ, 671, L61 CrossRefGoogle Scholar
Ben-Jaffel, L., & Sona Hosseini, S. 2010, ApJ, 709, 1284 CrossRefGoogle Scholar
Bisikalo, D.V., Kaigorodov, P.V., Ionov, D.E., & Shematovich, V.I. 2013, Astronomy Reports, 57, 715 CrossRefGoogle Scholar
Bisikalo, D.V., Arakcheev, A.S., & Kaigorodov, P.V. 2017, Astronomy Reports, 61, 925 CrossRefGoogle Scholar
Bisikalo, D.V., Cherenkov, A.A., Shematovich, V.I., et al. 2018, Astronomy Reports, 62, 648 CrossRefGoogle Scholar
Bisikalo, D.V., & Cherenkov, A.A. 2016, Astronomy Reports, 60, 183 CrossRefGoogle Scholar
Charbonneau, D., Brown, T.M., Latham, D.W., & Mayor, M. 2000, ApJ, 529, L45 CrossRefGoogle Scholar
Cherenkov, A.A., Bisikalo, D.V., & Kaigorodov, P.V. 2014, Astronomy Reports, 58, 679 CrossRefGoogle Scholar
Cherenkov, A., Bisikalo, D., Fossati, L., Möstl, C. 2017, ApJ, 846, 31 CrossRefGoogle Scholar
Cherenkov, A.A., Bisikalo, D.V., & Kosovichev, A.G. 2018, MNRAS, 475, 605 CrossRefGoogle Scholar
Cherenkov, A.A., Shaikhislamov, I.F., Bisikalo, D.V., et al. 2019, Astronomy Reports, 63, 94 CrossRefGoogle Scholar
Farrell, W.M., Halekas, J.S., Killen, R.M., et al. 2012, J. Geophys. Res. (Planets), 117, E00K04Google Scholar
Ip, W.-H., Kopp, A., & Hu, J.H. 2004, ApJ, 602, L53 CrossRefGoogle Scholar
Kaigorodov, P.V., Ilyina, E.A., & Bisikalo, D.V. 2019, Astronomy Reports, 63, 365 CrossRefGoogle Scholar
Kislyakova, K.G., Holmström, M., Lammer, H., et al. 2014, Science, 346, 981 CrossRefGoogle Scholar
Li, S.-L., Miller, N., Lin, D.N.C., & Fortney, J.J. 2010, Nature, 463, 1054 CrossRefGoogle Scholar
Linsky, J.L., Yang, H., France, K. et al. 2010, ApJ, 717, 1291 CrossRefGoogle Scholar
Liu, Y.D., Richardson, J.D., Wang, C., & Luhmann, J.G. 2014, ApJ, 788, L28 CrossRefGoogle Scholar
Mayor, M., & Queloz, D. 1995, Nature, 378, 355 CrossRefGoogle Scholar
Möstl, C., Amla, K., Hall, J.R., et al. 2014, ApJ, 787, 119 CrossRefGoogle Scholar
Murray-Clay, R.A., Chiang, E.I., & Murray, N. 2009, ApJ, 693, 23 CrossRefGoogle Scholar
Owens, M.J., & Forsyth, R.J. 2013, Living Rev. Solar Phys., 10, 5 CrossRefGoogle Scholar
Parker, E.N. 1958, Astrophys. J., 128, 664 CrossRefGoogle Scholar
Roussev, I.I., Gombosi, T.I., Sokolov, I.V., et al. 2003, ApJ, 595, L57 CrossRefGoogle Scholar
Russell, C.T. 1993, Rep. Prog. Phys., 56, 687 CrossRefGoogle Scholar
Steinolfson, R.S., & Hundhausen, A.J. 1988, J. Geophys. Res., 93, 14269 CrossRefGoogle Scholar
Stevenson, D.J. 1983, Reports on Progress in Physics, 46, 555 CrossRefGoogle Scholar
Totten, T.L., Freeman, J.W., & Arya, S. 1995, J. Geophys. Res., 100, 13 CrossRefGoogle Scholar
Vidal-Madjar, A., Lecavelier des Etangs, A., Desert, J.-M., et al. 2003, Nature, 422, 143 CrossRefGoogle Scholar
Vidal-Madjar, A., Desert, J.-M., des Etangs, Lecavelier, et al. 2004, ApJ, 604, L69 CrossRefGoogle Scholar
Vidal-Madjar, A., Lecavelier des Etangs, A., Desert, J.-M., et al. 2008, ApJ, 676, L57 CrossRefGoogle Scholar
Weber, E.J., & Davis, L., Jr. 1967, ApJ, 148, 217 CrossRefGoogle Scholar
Withbroe, G.L. 1988, Astrophys. J., 325, 442 CrossRefGoogle Scholar
Zhilkin, A.G., & Bisikalo, D.V. 2019, Astronomy Reports, 63, 550 CrossRefGoogle Scholar
Zhilkin, A.G., Bisikalo, D.V., & Kaygorodov, P.V. 2020, Astronomy Reports, in press Google Scholar