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      NASA’s Meteoroid Engineering Model 3 and Its Ability to Replicate Spacecraft Impact Rates

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          Abstract

          Meteoroids pose one of the largest risks to spacecraft outside of low Earth orbit. To correctly predict the rate at which meteoroids impact and damage spacecraft, environment models must describe the mass, directionality, velocity, and density distributions of meteoroids. NASA’s Meteoroid Engineering Model (MEM) is one such model; MEM 3 is an updated version of the code that better captures the correlation between directionality and velocity and incorporates a bulk density distribution. This paper describes MEM 3 and compares its predictions with the rate of large particle impacts seen on the Long Duration Exposure Facility and the Pegasus II and III satellites.

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          Collisional balance of the meteoritic complex

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            A direct measurement of the terrestrial mass accretion rate of cosmic dust.

            The mass of extraterrestrial material accreted by the Earth as submillimeter particles has not previously been measured with a single direct and precise technique that samples the particle sizes representing most of that mass. The flux of meteoroids in the mass range 10(-9) to 10(-4) grams has now been determined from an examination of hypervelocity impact craters on the space-facing end of the Long Duration Exposure Facility satellite. The meteoroid mass distribution peaks near 1.5 x 10(-5) grams (200 micrometers in diameter), and the small particle mass accretion rate is (40 +/- 20) x 106 kilograms per year, higher than previous estimates but in good agreement with total terrestrial mass accretion rates found by geochemical methods. This mass input is comparable with or greater than the average contribution from extraterrestrial bodies in the 1-centimeter to 10-kilometer size range.
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              DYNAMICAL MODEL FOR THE ZODIACAL CLOUD AND SPORADIC METEORS

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                Author and article information

                Journal
                jsr
                Journal of Spacecraft and Rockets
                J. Spacecraft
                American Institute of Aeronautics and Astronautics
                1533-6794
                18 November 2019
                January–February 2020
                : 57
                : 1
                : 160-176
                Affiliations
                NASA Marshall Space Flight Center , Huntsville, Alabama 35812
                ERC, Inc. , Huntsville, Alabama 35812
                Qualis Corporation , Huntsville, Alabama 35812
                Author notes
                [*]

                Aerospace Technologist, Planetary Studies, NASA Meteoroid Environment Office, MSFC EV44.

                [†]

                Instrumentation Specialist, Jacobs Space Exploration Group, NASA Meteoroid Environment Office, MSFC EV44.

                [‡]

                Astronomer, Jacobs Space Exploration Group, NASA Meteoroid Environment Office, MSFC EV44.

                Article
                A34561 A34561
                10.2514/1.A34561
                8e2cc483-bc02-48d0-b071-607a0b27e09d
                This material is declared a work of the U.S. Government and is not subject to copyright protection in the United States. All requests for copying and permission to reprint should be submitted to CCC at www.copyright.com; employ the eISSN 1533-6794 to initiate your request. See also AIAA Rights and Permissions www.aiaa.org/randp.
                History
                : 4 June 2019
                : 11 September 2019
                : 12 September 2019
                Page count
                Figures: 26, Tables: 2
                Funding
                Funded by: Marshall Space Flight Centerhttp://dx.doi.org/10.13039/100006197
                Award ID: 80MSFC18C0011
                Categories
                Full-Length Papers

                Engineering,Physics,Mechanical engineering,Space Physics
                Engineering, Physics, Mechanical engineering, Space Physics

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