<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-04-13T10:00:22Z</responseDate><request verb="GetRecord" identifier="oai:www.recercat.cat:2117/11559" metadataPrefix="oai_dc">https://recercat.cat/oai/request</request><GetRecord><record><header><identifier>oai:recercat.cat:2117/11559</identifier><datestamp>2025-07-17T00:31:27Z</datestamp><setSpec>com_2072_1033</setSpec><setSpec>col_2072_452950</setSpec></header><metadata><oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
   <dc:title>Low-energy impact dynamics in the Earth – Moon system</dc:title>
   <dc:creator>Masdemont Soler, Josep</dc:creator>
   <dc:creator>Gómez Muntané, Gerard</dc:creator>
   <dc:creator>Alessi, Elisa Maria</dc:creator>
   <dc:contributor>Universitat Politècnica de Catalunya. Departament de Matemàtica Aplicada I</dc:contributor>
   <dc:contributor>Universitat Politècnica de Catalunya. EGSA - Equacions Diferencials, Geometria, Sistemes Dinàmics i de Control, i Aplicacions</dc:contributor>
   <dc:subject>Àrees temàtiques de la UPC::Matemàtiques i estadística</dc:subject>
   <dc:subject>Lunar craters</dc:subject>
   <dc:subject>Invariant manifolds</dc:subject>
   <dc:subject>Lluna</dc:subject>
   <dc:subject>Cràters de meteorits</dc:subject>
   <dc:subject>Varietats (Matemàtica)</dc:subject>
   <dc:description>Most of the craters on the surface of the Moon were created by the collision of minor&#xd;
bodies of the Solar System, in particular asteroids coming from the Main Belt as a consequence&#xd;
of different types of resonance. Our aim is to investigate the dynamics of such asteroids, paying&#xd;
special attention on the hyperbolic invariant manifolds associated with the equilibrium point&#xd;
L2 of the Earth – Moon system within the framework of the Circular Restricted Three – Body&#xd;
Problem. We analyze how different distributions of initial conditions for transit trajectories and&#xd;
the value considered for the relative Earth – Moon distance can vary the probability of a lunar&#xd;
impact. Then, we add the gravitational effect of the Sun by means of the Bicircular Restricted&#xd;
Four – Body Problem, showing that the initial phase associated with the Sun and the ratio&#xd;
between the Earth – Moon – Sun distance and the Earth – Moon one can affect the collision&#xd;
pattern in terms of lunar longitude and latitude.</dc:description>
   <dc:description>Postprint (published version)</dc:description>
   <dc:date>2010</dc:date>
   <dc:type>Conference report</dc:type>
   <dc:identifier>Masdemont, J.J.; Gómez Muntané, G.; Alessi, E. M. Low-energy impact dynamics in the Earth – Moon system. A: Conference on Nonlinear Science and Complexity. "3rd Conference on Nonlinear Science and Complexity NCS10". Ankara: 2010.</dc:identifier>
   <dc:identifier>https://hdl.handle.net/2117/11559</dc:identifier>
   <dc:language>eng</dc:language>
   <dc:relation>http://nsc10.cankaya.edu.tr/proceedings/PAPERS/Symp5-Celestial%20Mechanics%20and%20Dynamical%20Astronomy%20Methods%20and%20Applications/Paper50.pdf</dc:relation>
   <dc:rights>http://creativecommons.org/licenses/by-nc-nd/3.0/es/</dc:rights>
   <dc:rights>Open Access</dc:rights>
   <dc:rights>Attribution-NonCommercial-NoDerivs 3.0 Spain</dc:rights>
   <dc:format>1 p.</dc:format>
   <dc:format>application/pdf</dc:format>
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