The Planetary Entry Systems Synthesis Tool: A conceptual design and analysis tool for EDL systems
Abstract
Conceptual design of entry, descent, and landing (EDL) systems requires models over several disciplines as well as knowledge regarding the interactions between these disciplines. To ease the conceptual development of an EDL mission segment and to explore the mission design space, the Planetary Entry Systems Synthesis Tool (PESST) was created. The PESST framework estimates the performance and mass of an entry system using user-defined geometry, aerodynamics, flight mechanics, terminal descent guidance, thermal response and mass estimation models. Trade studies can be performed by parameter sweeps to gain an understanding of the design space for conceptual studies. Several standard atmospheres are available, and either a user-defined or GRAM atmospheric model may be used. In its present form, PESST may be applied to entry studies for Earth, Mars and Venus missions. This framework is broadly applicable to the conceptual study of EDL systems. A detailed presentation of the PESST tool and each discipline model is provided along with comparisons to historical entry missions for Earth, Mars and Venus. The PESST framework for system level sizing and synthesis allows for the impact of technologies such as inflatable aerodynamic decelerators and guided terminal descent propulsion to be examined at the mission design level. Closing conceptual designs about these major discipline analyses models the effects of design changes on entry mass, peak deceleration, propellant mass, payload mass, and other mission level design constraints.
Additional Information
The authors would like to thank the Jet Propulsion Laboratory and the Charles Stark Draper Laboratory for their sponsorship of the new PESST framework. The work of Michael J. Grant and Bradley A. Steinfeldt of the SSDL was invaluable towards the incorporation of guidance algorithms into the current framework. The authors remain greatly appreciative of the time provided by Mike Tauber for conversations on radiative heating. Finally, the authors also wish to thank Patrick J. Smith for his work in implementing a very flexible parametric study capability.Attached Files
Accepted Version - IEEE-2010-1331.pdf
Files
IEEE-2010-1331.pdf
Additional details
Identifiers
- Eprint ID
- 119982
- Resolver ID
- CaltechAUTHORS:20230314-222595000.13
Related works
- Describes
- 10.1109/AERO.2010.5447017 (DOI)
Funding
- JPL
- Charles Stark Draper Laboratory
Dates
- Created
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2023-03-17Created from EPrint's datestamp field
- Updated
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2023-03-17Created from EPrint's last_modified field