Abstract
We considered the effect of the wind on the entry of meteorites into the venusian atmosphere by solving the entry equations involving a term related with the wind drag. We found that the wind affects only the entry of iron meteorites with masses less than 109 kg and stone meteorites with masses less than 1011 kg. Since meteorites that produce craters on Venus have masses exceeding these limits we conclude that the effect of the wind is negligible in the processes of craterization of the surface of Venus.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
