Seismic Detectability of a Subsurface Ocean on Europa
详细信息    查看全文
文摘
A seismometer placed on Jupiter's moon Europa can use passive monitoring to determine the presence or absence of a possible liquid water ocean beneath Europa's surface ice and estimates of the thickness of the ice shell itself. Using probable seismic velocities for Europa's ice it is demonstrated that surface waves propagating in the frequency band of 0.1 to 0.5 Hz (wave periods of 2 to 10 s) can discriminate ice shells varying from 5 to 20 km in thickness. Miniature, light-weight seismometers with appropriate sensitivities are available.

© 2004-2018 中国地质图书馆版权所有 京ICP备05064691号 京公网安备11010802017129号

地址:北京市海淀区学院路29号 邮编:100083

电话:办公室:(+86 10)66554848;文献借阅、咨询服务、科技查新:66554700