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Meteoroid-Induced Anomalies on SpacecraftMany programs/projects use a simple meteoroid environment based on Grun's 1985 paper or the old NASA space station spec in their design and risk assessments. These models, which are omni directional and mono-­velocity, bear little resemblance to the actual meteoroid environment, which is sun-fixed, very directional, and which has a complex speed distribution varying by source and particle size. As a result, the simple meteoroid models lead to estimates that underestimate the spacecraft/vehicle risk by a factor of 2 or more. In addition, programs often over-emphasize the risk posed by meteor showers, which typically account for less than ten percent of the meteoroid risk over the vehicle lifetime. Fueled by popular media, the emphasis on meteor showers (the risks from which can usually be mitigated operationally) can lead to ambivalence to the real risk driver, which is the sporadic background.
Document ID
20150016505
Acquisition Source
Marshall Space Flight Center
Document Type
Abstract
Authors
Cooke, William J.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 26, 2015
Publication Date
July 14, 2015
Subject Category
Space Sciences (General)
Report/Patent Number
M15-4640
Report Number: M15-4640
Meeting Information
Meeting: Stanford Meteor Environments and Effects Workshop
Location: Stanford, CA
Country: United States
Start Date: July 14, 2015
End Date: July 16, 2015
Sponsors: Stanford Univ.
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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