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Jürgen Schmidt

Researcher at University of Oulu

Publications -  80
Citations -  3148

Jürgen Schmidt is an academic researcher from University of Oulu. The author has contributed to research in topics: Enceladus & Population. The author has an hindex of 23, co-authored 78 publications receiving 2780 citations. Previous affiliations of Jürgen Schmidt include Braunschweig University of Technology & University of Colorado Boulder.

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Sodium salts in E-ring ice grains from an ocean below the surface of Enceladus

TL;DR: The identification of a population of E-ring grains that are rich in sodium salts, which can arise only if the plumes originate from liquid water, and the abundance of various salt components in these particles exhibit a compelling similarity to the predicted composition of a subsurface Enceladus ocean in contact with its rock core.
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A salt-water reservoir as the source of a compositionally stratified plume on Enceladus

TL;DR: Whereas previous Cassini observations were compatible with a variety of plume formation mechanisms, these data eliminate or severely constrain non-liquid models and strongly imply that a salt-water reservoir with a large evaporating surface provides nearly all of the matter in the plume.
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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.
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A permanent, asymmetric dust cloud around the Moon

TL;DR: Observations of a permanent, asymmetric dust cloud around the Moon, caused by impacts of high-speed cometary dust particles on eccentric orbits, as opposed to particles of asteroidal origin following near-circular paths striking the Moon at lower speeds are reported.
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Slow dust in Enceladus' plume from condensation and wall collisions in tiger stripe fractures.

TL;DR: It is shown that repeated wall collisions of grains, with re-acceleration by the gas, induce an effective friction, offering a natural explanation for the reduced grain velocity, and suggests liquid water below Enceladus’ south pole.