Print Email Facebook Twitter Asteroid Muon Tomography Title Asteroid Muon Tomography: A feasibility study on using galactic cosmic rays to map small Solar System body interiors. Author Reichert, Jules (TU Delft Aerospace Engineering) Contributor Menicucci, A. (mentor) Degree granting institution Delft University of Technology Programme Aerospace Engineering Date 2021-01-15 Abstract Asteroids and comets are thought to be the primordial remnants of our early Solar System, their interior structure and composition providing a snapshot of this turbulent era of planet formation. Thus far, everything we know of the internals of these small Solar System bodies has been inferred from surface observations and meteorite mineralogy. Evidence suggests however that their surface characteristics might not be representative of their interior features, due to effects like granular convection and space weathering. One proposed method to directly measure these features makes use of the already present galactic cosmic ray flux. Muons are created in collisions between the asteroid surface and these cosmic rays, their properties altered by the type and quantity of material traversed. By measuring the muon flux exiting the surface, the interior can be reconstructed. This thesis surveys the feasibility of muon tomography in space, with model creation and particle passage simulations. Subject muontomographyasteroidinteriorGeant4 To reference this document use: http://resolver.tudelft.nl/uuid:409c0c23-f012-400c-93c2-d780d56ed6f0 Part of collection Student theses Document type master thesis Rights © 2021 Jules Reichert Files PDF Asteroid_Muon_Tomography_ ... ichert.pdf 35.44 MB Close viewer /islandora/object/uuid:409c0c23-f012-400c-93c2-d780d56ed6f0/datastream/OBJ/view