M
Martin Makuch
Researcher at University of Potsdam
Publications - 5
Citations - 395
Martin Makuch is an academic researcher from University of Potsdam. The author has contributed to research in topics: Cosmic dust & Enceladus. The author has an hindex of 4, co-authored 5 publications receiving 364 citations.
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Journal ArticleDOI
Cassini Dust Measurements at Enceladus and Implications for the Origin of the E Ring
Frank Spahn,Jürgen Schmidt,Nicole Albers,Marcel Hörning,Martin Makuch,Martin Seiß,Sascha Kempf,Ralf Srama,Valeri Dikarev,Valeri Dikarev,Stefan Helfert,Georg Moragas-Klostermeyer,Alexander V. Krivov,M. Sremcevic,Anthony J. Tuzzolino,Thanasis E. Economou,Eberhard Grün,Eberhard Grün +17 more
TL;DR: During Cassini's close flyby of Enceladus on 14 July 2005, the High Rate Detector of the Cosmic Dust Analyzer registered micron-sized dust particles enveloping this satellite; this asymmetric signature is consistent with a locally enhanced dust production in the south polar region of Encesladus.
Journal ArticleDOI
E ring dust sources: Implications from Cassini's dust measurements
Frank Spahn,Nicole Albers,Marcel Hörning,Sascha Kempf,Alexander V. Krivov,Martin Makuch,Jürgen Schmidt,Martin Seiß,M. Sremcevic +8 more
TL;DR: Spahn et al. as mentioned in this paper used the Enceladus flyby E11 data to identify the amount of dust produced in the impactor-ejecta process and to improve related modeling.
Journal ArticleDOI
Long-term dynamical evolution of dusty ejecta from Deimos
TL;DR: In this paper, the Poynting-Robertson drag (PR) was used to study the dynamics of the Deimos torus under the combined action of radiation pressure and Mars oblateness.
Journal ArticleDOI
Stochastic circumplanetary dynamics of rotating non-spherical dust particles
TL;DR: In this paper, a model of stochastic radiation pressure for rotating non-spherical particles was developed and applied to the circumplanetary dynamics of dust grains, and the model was compared with numerical simulations performed for the motion of the dusty ejecta from Deimos in orbit around Mars.
Stochastic circumplanetary Dynamics of rotating non-spherical Dust Particles
TL;DR: In this article, a model of stochastic radiation pressure for rotating non-spherical particles was developed and applied to the circumplanetary dynamics of dust grains, and the model was compared with numerical simulations performed for the motion of the dusty ejecta from Deimos in orbit around Mars.