Circumplanetary dust dynamics
application to Martian dust tori and Enceladus dust plumes
dc.contributor.author | Makuch, Martin | |
dc.date.accessioned | 2010-10-12T18:23:18Z | |
dc.date.available | 2010-10-12T18:23:18Z | |
dc.date.issued | 2007 | |
dc.identifier.uri | http://hdl.handle.net/11858/00-1735-0000-0001-30DD-5 | |
dc.description.abstract | Our Solar system contains a large amount of dust, containing valuable information about our close cosmic environment. If created in a planet's system, the particles stay predominantly in its vicinity and can form extended dust envelopes, tori or rings around them. A fascinating example of these complexes are Saturnian rings containing a wide range of particles sizes from house-size objects in the main rings up to micron-sized grains constituting the E ring. Other example are ring systems in general, containing a large fraction of dust or also the putative dust-tori surrounding the planet Mars. The dynamical life'' of such circumplanetary dust populations is the main subject of our study... | |
dc.format.extent | 115, 10 Bl. | |
dc.format.mimetype | application/pdf | |
dc.language.iso | eng | |
dc.publisher | Univ. Potsdam | |
dc.rights.uri | http://e-docs.geo-leo.de/rights | |
dc.subject.ddc | 523 | |
dc.subject.gok | TGL 800 | |
dc.title | Circumplanetary dust dynamics | |
dc.title.alternative | application to Martian dust tori and Enceladus dust plumes | |
dc.type | monograph | |
dc.subject.gokverbal | Interplanetarer Staub {Astronomie} | |
dc.identifier.doi | 10.23689/fidgeo-87 | |
dc.identifier.ppn | 53871493X | |
dc.type.version | publishedVersion | |
dc.relation.collection | Astronomie, Astrophysik, Weltraumforschung | |
dc.description.type | thesis |