Heidelberg Dust Research Group
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Dusty Messengers: Dust particles in space carry information about
their birth at a remote site in space and time. By space measurements we
learn where dust comes from. From its state and composition we obtain
knowledge about the environment in and the processes by which the dust
was formed and by which it was altered on its way to us.
More information: Why dust?,
Kosmischer Staub, der Ursprung unserer Erde
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CDA Data:
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Latest Papers:
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Discriminating Contamination from Particle Components in Spectra of Cassini's Dust Detector CDA
Planetary and Space Science, (in press), (2009)
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Observation of Saturnian stream particles in the interplanetary space
Icarus, (in press), (2009)
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TandEM: Titan and Enceladus mission
Experimental Astronomy, 23, (2009)
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Sodium salts in E-ring ice grains from an ocean below the surface of Enceladus
Nature, 459, (2009)
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Laboratory calibration measurements of a piezoelectric lead zirconate titanate cosmic dust detector at low velocities
Advances in Space Research, 43, (2009)
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Characteristics of piezoelectric lead zirconate titanate multilayered detector bombarded with hypervelocity iron particles
Advances in Space Research, 43, (2009)
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Identification of Saturn's magnetospheric regions and associated plasma processes: Synopsis of Cassini observations during orbit insertion
Reviews of Geophysics, 46, (2008)
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Slow dust in Enceladus' plume from condensation and wall collisions in tiger stripe fractures
Nature, 451, (2008)
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Interpretation of high rate dust measurements with the Cassini dust detector CDA
Planetary and Space Science, 56, (2008)
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Characteristics of a dust trajectory sensor
Review of Scientific Instruments, 79, (2008)
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DuneXpress
Experimental Astronomy, 23, (2009)
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Sample return of interstellar matter (SARIM)
Experimental Astronomy, 23, (2009)
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The E-ring in the vicinity of Enceladus. II. Probing the moon's interior—The composition of E-ring particles
Icarus, 193, (2008)
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The E ring in the vicinity of Enceladus. I. Spatial distribution and properties of the ring particles
Icarus, 193, (2008)
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Measurement of temperature after hypervelocity collision of microparticles in the range from 10 to 40 km/s
Applied Physics Letters, 93, (2008)
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Interstellar Dust Inside and Outside the Heliosphere
Space Science Reviews, 153, (2008)
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The Dust Halo of Saturn's Largest Icy Moon, Rhea
Science, 319, (2008)
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Interstellar Dust in the Solar System
Space Science Review, 130, (2007)
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Interplanetary dust detected by the cassini CDA chemical analyser
Icarus, 190,643-654, (2007)
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The source of Saturn's G Ring
Science, 317,653-656, (2007)
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DuneXpress, in situ analysis of interstellar dust
Geochimica et Cosmochimica Acta, 71,A358, (2007)
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Cassini/Cosmic Dust Analyzer in situ dust measurements between Jupiter and Saturn
Journal of Geophysical Research-Space Physics, 112, (2007)
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The composition of Saturn's E ring
Monthly Notices of the Royal Astronomical Society, 377, (2007)
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Interstellar dust in the solar system
Space Science Reviews, 130, (2007)
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Large area mass analyzer instrument for the chemical analysis of interstellar dust particles
Review of Scientific Instruments, 78, (2007)
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COSIMA - High resolution time-of-flight secondary ion mass spectrometer for the analysis of cometary dust particles onboard Rosetta
Space Science Reviews, 128, (2007)
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Dust environment modelling of comet 67P/Churyumov-Gerasimenko
Space Science Reviews, 128, (2007)
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Rosetta Radio Science Investigations (RSI)
Space Science Reviews, 128, (2007)
Older publications
CDA publications
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