TY  - JOUR
AU  - Sterken, Veerle J.
AU  - Westphal, Andrew J.
AU  - Altobelli, Nicolas
AU  - Grün, Eberhard
AU  - Hillier, Jon K.
AU  - Postberg, Frank
AU  - Srama, Ralf
AU  - Allen, Carlton
AU  - Anderson, David
AU  - Ansari, Asna
AU  - Bajt, Saša
AU  - Bastien, Ron S.
AU  - Bassim, Nabil
AU  - Bechtel, Hans A.
AU  - Borg, Janet
AU  - Brenker, Frank E.
AU  - Bridges, John
AU  - Brownlee, Donald E.
AU  - Burchell, Mark
AU  - Burghammer, Manfred
AU  - Butterworth, Anna L.
AU  - Changela, Hitesh
AU  - Cloetens, Peter
AU  - Davis, Andrew M.
AU  - Doll, Ryan
AU  - Floss, Christine
AU  - Flynn, George
AU  - Frank, David
AU  - Gainsforth, Zack
AU  - Heck, Philipp R.
AU  - Hoppe, Peter
AU  - Hudson, Bruce
AU  - Huth, Joachim
AU  - Hvide, Brit
AU  - Kearsley, Anton
AU  - King, Ashley J.
AU  - Lai, Barry
AU  - Leitner, Jan
AU  - Lemelle, Laurence
AU  - Leroux, Hugues
AU  - Leonard, Ariel
AU  - Lettieri, Robert
AU  - Marchant, William
AU  - Nittler, Larry R.
AU  - Ogliore, Ryan
AU  - Ong, Wei Ja
AU  - Price, Mark C.
AU  - Sandford, S. A.
AU  - Tresseras, Juan-Angel Sans
AU  - Schmitz, Sylvia
AU  - Schoonjans, Tom
AU  - Silversmit, Geert
AU  - Simionovici, Alexandre
AU  - Solé, Vicente A.
AU  - Stephan, Thomas
AU  - Stodolna, Julien
AU  - Stroud, Rhonda M.
AU  - Sutton, Steven
AU  - Trieloff, Mario
AU  - Tsou, Peter
AU  - Tsuchiyama, Akira
AU  - Tyliszczak, Tolek
AU  - Vekemans, Bart
AU  - Vincze, Laszlo
AU  - Korff, Joshua Von
AU  - Wordsworth, Naomi
AU  - Zevin, Daniel
AU  - Zolensky, Michael E.
TI  - Stardust Interstellar Preliminary Examination X: Impact Speeds and Directions of Interstellar Grains on the Stardust Dust Collector
JO  - Meteoritics & planetary science
VL  - 49
IS  - 9
SN  - 1086-9379
CY  - Hoboken, NJ
PB  - Wiley-Blackwell
M1  - PUBDB-2015-01250
SP  - 1680 - 1697
PY  - 2014
N1  - (c) The Meteoritical Society. Post referee full text in progress.
AB  - On the basis of an interstellar dust model compatible with Ulysses and Galileo observations, we calculate and predict the trajectories of interstellar dust (ISD) in the solar system and the distribution of the impact speeds, directions, and flux of ISD particles on the Stardust Interstellar Dust Collector during the two collection periods of the mission. We find that the expected impact velocities are generally low (<10 km s<sup>−1</sup>) for particles with the ratio of the solar radiation pressure force to the solar gravitational force β > 1, and that some of the particles will impact on the cometary side of the collector. If we assume astronomical silicates for particle material and a density of 2 g cm<sup>−3</sup>, and use the Ulysses measurements and the ISD trajectory simulations, we conclude that the total number of (detectable) captured ISD particles may be on the order of 50. In companion papers in this volume, we report the discovery of three interstellar dust candidates in the Stardust aerogel tiles. The impact directions and speeds of these candidates are consistent with those calculated from our ISD propagation model, within the uncertainties of the model and of the observations.
LB  - PUB:(DE-HGF)16
UR  - <Go to ISI:>//WOS:000342912100010
DO  - DOI:10.1111/maps.12219
UR  - https://bib-pubdb1.desy.de/record/207267
ER  -