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Title: EARLY UV INGRESS IN WASP-12b: MEASURING PLANETARY MAGNETIC FIELDS

Abstract

Recently, Fossati et al. observed that the UV transit of WASP-12b showed an early ingress compared with the optical transit. We suggest that the resulting early ingress is caused by a bow shock ahead of the planetary orbital motion. In this Letter, we investigate the conditions that might lead to the formation of such a bow shock. We consider two scenarios: (1) the stellar magnetic field is strong enough to confine the hot coronal plasma out to the planetary orbit and (2) the stellar magnetic field is unable to confine the plasma, which escapes in a wind. In both cases, a shock capable of compressing plasma to the observed densities will form around the planet for plasma temperatures T {approx_lt} (4-5) x 10{sup 6} K. In the confined case, the shock always forms directly ahead of the planet, but in the wind case the shock orientation depends on the wind speed and hence on the plasma temperature. For higher wind temperatures, the shock forms closer to the line of centers between the planet and the star. We conclude that shock formation leading to an observable early UV ingress is likely to be a common feature of transiting systems and maymore » prove to be a useful tool in setting limits on planetary magnetic field strengths B{sub p} . In the case of WASP-12b, we derive an upper limit of about B{sub p} = 24 G.« less

Authors:
; ;  [1]
  1. School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, KY16 9SS (United Kingdom)
Publication Date:
OSTI Identifier:
21452740
Resource Type:
Journal Article
Journal Name:
Astrophysical Journal Letters
Additional Journal Information:
Journal Volume: 722; Journal Issue: 2; Other Information: DOI: 10.1088/2041-8205/722/2/L168; Journal ID: ISSN 2041-8205
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ELECTRON TEMPERATURE; ION TEMPERATURE; MAGNETIC FIELDS; PLANETS; PLASMA; SATELLITES; SHOCK WAVES; STARS

Citation Formats

Vidotto, A A, Jardine, M, and Helling, Ch. EARLY UV INGRESS IN WASP-12b: MEASURING PLANETARY MAGNETIC FIELDS. United States: N. p., 2010. Web. doi:10.1088/2041-8205/722/2/L168.
Vidotto, A A, Jardine, M, & Helling, Ch. EARLY UV INGRESS IN WASP-12b: MEASURING PLANETARY MAGNETIC FIELDS. United States. https://doi.org/10.1088/2041-8205/722/2/L168
Vidotto, A A, Jardine, M, and Helling, Ch. 2010. "EARLY UV INGRESS IN WASP-12b: MEASURING PLANETARY MAGNETIC FIELDS". United States. https://doi.org/10.1088/2041-8205/722/2/L168.
@article{osti_21452740,
title = {EARLY UV INGRESS IN WASP-12b: MEASURING PLANETARY MAGNETIC FIELDS},
author = {Vidotto, A A and Jardine, M and Helling, Ch},
abstractNote = {Recently, Fossati et al. observed that the UV transit of WASP-12b showed an early ingress compared with the optical transit. We suggest that the resulting early ingress is caused by a bow shock ahead of the planetary orbital motion. In this Letter, we investigate the conditions that might lead to the formation of such a bow shock. We consider two scenarios: (1) the stellar magnetic field is strong enough to confine the hot coronal plasma out to the planetary orbit and (2) the stellar magnetic field is unable to confine the plasma, which escapes in a wind. In both cases, a shock capable of compressing plasma to the observed densities will form around the planet for plasma temperatures T {approx_lt} (4-5) x 10{sup 6} K. In the confined case, the shock always forms directly ahead of the planet, but in the wind case the shock orientation depends on the wind speed and hence on the plasma temperature. For higher wind temperatures, the shock forms closer to the line of centers between the planet and the star. We conclude that shock formation leading to an observable early UV ingress is likely to be a common feature of transiting systems and may prove to be a useful tool in setting limits on planetary magnetic field strengths B{sub p} . In the case of WASP-12b, we derive an upper limit of about B{sub p} = 24 G.},
doi = {10.1088/2041-8205/722/2/L168},
url = {https://www.osti.gov/biblio/21452740}, journal = {Astrophysical Journal Letters},
issn = {2041-8205},
number = 2,
volume = 722,
place = {United States},
year = {Wed Oct 20 00:00:00 EDT 2010},
month = {Wed Oct 20 00:00:00 EDT 2010}
}