用户名: 密码: 验证码:
Venus’ radar-bright highlands: Different signatures and materials on Ovda Regio and on Maxwell Montes
详细信息    查看全文
文摘

An enduring puzzle about Venus is why its highlands are bright in reflected radar (i.e., have surfaces of high apparent permittivity).

On equatorial highlands, the pattern or radar reflectance is consistent with the presence of a ferro-electric substance, confirming earlier work.

The ferroelectric substance on the equatorial highlands is likely chlorapatite, formed by reaction between igneous fluorapatite and HCl in the Venus atmosphere.

On the highlands of Maxwell Montes, the pattern of radar reflectance is consistent with presence of a semiconductor substance formed in chemical reaction between the atmosphere and the surface, not a ferro-electric like chlorapatite.

The radar difference between the equatorial highlands and Maxwell Montes apparently represents significant differences either in bedrock type or in atmosphere composition & temperature.

© 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