Estimates of Flight Regimes in the Venus Atmosphere
ResearchPublished 1963
ResearchPublished 1963
A study of the aerodynamic flight regions that may be encountered during entry into the atmosphere of Venus, and an estimate of the gross aerodynamic behavior of objects entering that atmosphere. It is found that the best evidence available does not permit an estimate of a single likely model atmosphere suitable for aerodynamic use. Substantial differences in flight regions, particularly in the troposphere, must be considered. Depending on the models used, the continuum flight region is entered at altitudes between about 150 and 80 km above the visible cloud layer. In view of this uncertainty in the structure of the Venus atmosphere, a more detailed analysis of flow problems in shock layers, boundary layers, etc., would be premature. The flight regime limits given, however, may provide design criteria for probes approaching the planet or possibly those reaching the cloud layer itself.
This publication is part of the RAND research memorandum series. The research memorandum series, a product of RAND from 1948 to 1973, included working papers meant to report current results of RAND research to appropriate audiences.
This document and trademark(s) contained herein are protected by law. This representation of RAND intellectual property is provided for noncommercial use only. Unauthorized posting of this publication online is prohibited; linking directly to this product page is encouraged. Permission is required from RAND to reproduce, or reuse in another form, any of its research documents for commercial purposes. For information on reprint and reuse permissions, please visit www.rand.org/pubs/permissions.
RAND is a nonprofit institution that helps improve policy and decisionmaking through research and analysis. RAND's publications do not necessarily reflect the opinions of its research clients and sponsors.