What is it about?

Spacecrafts designed to enter, descend and land on planets are usually characterized by a blunt frontal geometry to withstand the high heating. This geometry leads to recirculating, turbulent flows on the rear portion of the vehicle, which can lead to unexpected oscillations and high roll rates, potentially compromising the mission. This work aims to characterize these instabilities in the context of novel deployable vehicles designed for Mars missions.

Featured Image

Read the Original

This page is a summary of: Mach, Reynolds, and Strouhal Number Effects on Deployable Aeroshell Pitch Dynamics, Journal of Spacecraft and Rockets, March 2025, American Institute of Aeronautics and Astronautics (AIAA),
DOI: 10.2514/1.a36126.
You can read the full text:

Read

Contributors

The following have contributed to this page