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- W2288006475 abstract "The work performed in this research proposes to develop a dynamical evolution model of dust particles smaller than 0.1 mm, coming from the Main Belt, until they reach Mercury in order to obtain the micrometeoroid flux directly without any extrapolation. The results obtained by means of this model take issue with those given by Cintala in his article, that is the reference author in this field. In particular, the main results are that the Cintala flux, expressed in terms of mass is 407.8 times lower.This comparison yields that our model estimates a number of impacts smaller than Cintala, but a mass contribution much higher.The reason of this result is due to the fact that our numerical simulations give a number of impactshigher than Cintala for larger particles. This explains the major mass contribution" @default.
- W2288006475 created "2016-06-24" @default.
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- W2288006475 date "2009-02-02" @default.
- W2288006475 modified "2023-09-27" @default.
- W2288006475 title "Interplanetary dust analysis around Mercury and the interaction with the surface" @default.
- W2288006475 hasPublicationYear "2009" @default.
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