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Eberhard Grün

Researcher at Max Planck Society

Publications -  414
Citations -  17010

Eberhard Grün is an academic researcher from Max Planck Society. The author has contributed to research in topics: Cosmic dust & Interplanetary dust cloud. The author has an hindex of 68, co-authored 414 publications receiving 15918 citations. Previous affiliations of Eberhard Grün include University of Hawaii & University of Colorado Boulder.

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Collisional balance of the meteoritic complex

TL;DR: In this article, a detailed analysis of the effects of mutual collisions (i.e., destruction of meteoroids and production of fragment particles) and of radiation pressure has been performed which yielded a new picture of the balance of the meteoritic complex.
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Composition of comet Halley dust particles from Giotto observations

TL;DR: The mass spectra of cometary dust particles measured by the PIA dust particle analyzer aboard the Giotto spacecraft showed some unexpected and striking features as mentioned in this paper, such as small particles below 10 to the -14th g are much more abundant than anticipated by models.
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Discovery of Jovian dust streams and interstellar grains by the Ulysses spacecraft

TL;DR: Within 1 AU from Jupiter, the Ulysses spacecraft during the flyby on February 8, 1992 recorded periodic bursts of submicron dust particles with durations ranging from several hours to two days and occurring at about monthly intervals.
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Dust measurements in the coma of comet 67P/Churyumov-Gerasimenko inbound to the Sun

Alessandra Rotundi, +90 more
- 23 Jan 2015 - 
TL;DR: In this article, the GIADA (Grain Impact Analyser and Dust Accumulator) experiment on the European Space Agency's Rosetta spacecraft orbiting comet 67P/Churyumov-Gerasimenko was used to detect 35 outflowing grains of mass 10−10 to 10−7 kilograms.
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Cassini Dust Measurements at Enceladus and Implications for the Origin of the E Ring

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.