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Large Vehicle Lunar Landing Surface Interaction and In-Situ Resource Based Risk Mitigation: Landing & Launch PadsA key capability required for the exploration of planetary bodies is the ability to land on the surface. Previous work performed by NASA and other institutions has primarily focused on landing small spacecraft on planetary surfaces and the associated small-to-medium thrusters required for the soft landing. In the case of human exploration—particularly the establishment of long duration exploration and habitation outposts—the ability to land large landers, such as the SpaceX Starship, is necessary. These larger landing systems require the use of more powerful engines, with higher engine exhaust temperatures and higher landing loads. Understanding the excavation of material by the engines, as well as the potential for the landing legs to sink into the subsurface, is key in ensuring reliable and safe landings. A further improvement in landing reliability can be achieved by constructing landing / launch pads, especially with in-situ resources. Some material excavation by the plume is inevitable, leaving at least a portion of the surface scoured and uneven under the lander and ejecting regolith particles and rocks at very high velocities. One possible solution would be to robotically build landing / launch pads (ideally autonomously) at the destination using in-situ materials. In this case, the first one or few landers will need to land on unimproved surfaces at higher risk; however, they would bring the required equipment to build the landing pads with mostly local resources, thus increasing the reliability of safe landing for subsequent larger landers. A number of methods to build in-situ landing and launch pads have already been developed. These methods include no, or some, addition of required binder additives to the local regolith material, different processing approaches and result in varying landing pad strengths. A sub-scale rocket engine plume, was used to simulate some of the conditions of a landing on the Moon to assess the effectiveness of various materials for an in-situ built landing pad, The GO2/GCH4rocket engine fired on a 1m2area coupons of representative pad materials. The results will allow continued development towards materials that satisfy the landing pad properties required for the effective risk reduction and increased reliability for landing people and equipment on the lunar surface. This work contained two parts: (1) computer modeling of a large rocket engine plume interacting with regolith on the Moon, using the Granular Gas Flow Solver (GGFS) provided by CFD Research Corporation as well as other computational fluid dynamics codes (CFD) such as Loci/CHEM. (2) Developing landing/launch pad materials that could be used for in-situ construction on the lunar surface in the future, to mitigate the calculated effects of a large vehicle rocket engine landing and launching on the Moon.
Document ID
20210022503
Acquisition Source
Kennedy Space Center
Document Type
Conference Paper
Authors
Robert P Mueller
(Kennedy Space Center Merritt Island, Florida, United States)
Nathan J Gelino
(Kennedy Space Center Merritt Island, Florida, United States)
Laurent Sibille
(Southeastern Universities Research Association Washington D.C., District of Columbia, United States)
Kyle L Dixon
(Kennedy Space Center Merritt Island, Florida, United States)
Bruce T Vu
(Kennedy Space Center Merritt Island, Florida, United States)
Matthew Kuhns
(Masten Space Systems)
Date Acquired
October 6, 2021
Subject Category
Spacecraft Propulsion And Power
Fluid Mechanics And Thermodynamics
Meeting Information
Meeting: AIAA ASCEND Conference
Location: Las Vegas, NV
Country: US
Start Date: November 15, 2021
End Date: November 17, 2021
Sponsors: American Institute of Aeronautics and Astronautics
Funding Number(s)
OTHER: SW 0001
Distribution Limits
Public
Copyright
Public Use Permitted.
Technical Review
NASA Peer Committee
Keywords
Lunar
Landing / Launch Pad
ISRU
Regolith
Rocket Engine
Plume Surface Impingement
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