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Open AccessJournal ArticleDOI

Stardust Interstellar Preliminary Examination II: Curating the interstellar dust collector, picokeystones, and sources of impact tracks

D. Frank, +68 more
- 01 Sep 2014 - 
- Vol. 49, Iss: 9, pp 1522-1547
TLDR
In this paper, the authors discuss the inherent difficulties that arise during "ground truth" characterization of the Stardust interstellar dust collector, and provide a detailed description of the sample preparation techniques developed to address the unique goals and restrictions of the Interstellar Preliminary Exam.
Abstract
We discuss the inherent difficulties that arise during "ground truth" characterization of the Stardust interstellar dust collector. The challenge of identifying contemporary interstellar dust impact tracks in aerogel is described within the context of background spacecraft secondaries and possible interplanetary dust particles and beta-meteoroids. In addition, the extraction of microscopic dust embedded in aerogel is technically challenging. Specifically, we provide a detailed description of the sample preparation techniques developed to address the unique goals and restrictions of the Interstellar Preliminary Exam. These sample preparation requirements and the scarcity of candidate interstellar impact tracks exacerbate the difficulties. We also illustrate the role of initial optical imaging with critically important examples, and summarize the overall processing of the collection to date.

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Citations
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Journal ArticleDOI

Evidence for interstellar origin of seven dust particles collected by the Stardust spacecraft

Andrew J. Westphal, +65 more
- 15 Aug 2014 - 
TL;DR: The Stardust Interstellar Dust Collector captured seven particles and returned to Earth for laboratory analysis have features consistent with an origin in the contemporary interstellar dust stream and more than 50 spacecraft debris particles were also identified as discussed by the authors.
Journal ArticleDOI

The Stardust Mission: Analyzing Samples from the Edge of the Solar System

TL;DR: In this article, the authors show that the cold regions of the early Solar System were not isolated and were not a refuge where interstellar materials could commonly survive, and that the rocky components in primitive asteroids and comets may differ because asteroid formation was dominated by local materials, whereas comets formed from mixed materials, many of which were transported from very distant locations.
Journal ArticleDOI

Stardust Interstellar Preliminary Examination X: Impact speeds and directions of interstellar grains on the Stardust dust collector

Veerle Sterken, +68 more
TL;DR: In this paper, the trajectories of ISD in the solar system and the distribution of the impact speeds, directions, and flux of the ISD particles on the Stardust Interstellar Dust Collector during the two collection periods of the mission were predicted.
Journal ArticleDOI

Concerns of Organic Contamination for Sample Return Space Missions

TL;DR: An overview of the successes and lessons learned with regards to the identification of indigenous organic matter of the returned samples vs terrestrial contamination is provided.
Journal ArticleDOI

Stardust Interstellar Preliminary Examination IV: Scanning transmission X-ray microscopy analyses of impact features in the Stardust Interstellar Dust Collector

Anna L. Butterworth, +69 more
TL;DR: In this paper, the authors report the quantitative characterization by synchrotron soft X-ray spectroscopy of 31 potential impact features in the aerogel capture medium of the Stardust Interstellar Dust Collector.
References
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Journal ArticleDOI

A unified representation of gas-phase element depletions in the interstellar medium*

TL;DR: In this paper, a study of gas-phase element abundances reported in the literature for 17 different elements sampled over 243 sight lines in the local part of our Galaxy reveals that the depletions into solid form (dust grains) are extremely well characterized by trends that employ only three kinds of parameters: an index that describes the overall level of depletion applicable to the gas in any particular sight line, and linear coefficients that describe how to derive each element's depletion from this sight-line parameter.
Journal ArticleDOI

A Unified Representation of Gas-Phase Element Depletions in the Interstellar Medium

TL;DR: In this article, a study of gas-phase element abundances reported in the literature for 17 different elements sampled over 243 sight lines in the local part of our Galaxy reveals that the depletions into solid form (dust grains) are extremely well characterized by trends that employ only three kinds of parameters: an index that describes the overall level of depletion applicable to the gas in any particular sight line, and linear coefficients that describe how to derive each element's depletion from this sight-line parameter.
Journal ArticleDOI

Cometary Origin of the Zodiacal Cloud and Carbonaceous Micrometeorites

TL;DR: In this article, a model based on the orbital properties and lifetimes of comets and asteroids, and on the dynamical evolution of dust after ejection was presented to predict the formation of the zodiacal cloud.
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