We present a methodology to determine the thickness and material properties of the icy crust of Europa, a satellite of Jupiter. Instruments proposed for NASA’s Europa Multiple Flyby mission may be insufficient to adequately measure the ice’s thickness. We propose a complementary experiment in which vibration of the Europan surface is induced by an artificial impact. Optical vibrometry techniques, such as 2-D digital image correlation and vibration magnification are considered for detecting the displacement field at a sub-pixel level. We make use of COMSOL Multiphysics, which simulates wave motions via the finite element method. Dispersion curves of elastic waves and the wavenumber filtering are used to estimate the thickness and properties of the extraterrestrial ice.
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April 01 2016
Preliminary study of extraterrestrial optical vibrometry for an impactor mission to Europa
Thomas Campbell;
Thomas Campbell
Mech. Eng., The Catholic Univ. of America, 620 Michigan Ave. NE., Washington, DC 20064, 96campbellt@cua.edu
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John Brewer;
John Brewer
Mech. Eng., The Catholic Univ. of America, 620 Michigan Ave. NE., Washington, DC 20064, 96campbellt@cua.edu
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Masataka Okutsu;
Masataka Okutsu
Mech. Eng., The Catholic Univ. of America, 620 Michigan Ave. NE., Washington, DC 20064, 96campbellt@cua.edu
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Diego Turo;
Diego Turo
Mech. Eng., The Catholic Univ. of America, 620 Michigan Ave. NE., Washington, DC 20064, 96campbellt@cua.edu
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Joseph Vignola
Joseph Vignola
Mech. Eng., The Catholic Univ. of America, 620 Michigan Ave. NE., Washington, DC 20064, 96campbellt@cua.edu
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J. Acoust. Soc. Am. 139, 2077 (2016)
Citation
Thomas Campbell, John Brewer, Masataka Okutsu, Diego Turo, Joseph Vignola; Preliminary study of extraterrestrial optical vibrometry for an impactor mission to Europa. J. Acoust. Soc. Am. 1 April 2016; 139 (4_Supplement): 2077. https://doi.org/10.1121/1.4950162
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