Final reports of the Stardust Interstellar Preliminary Examination. (22nd August 2014)
- Record Type:
- Journal Article
- Title:
- Final reports of the Stardust Interstellar Preliminary Examination. (22nd August 2014)
- Main Title:
- Final reports of the Stardust Interstellar Preliminary Examination
- Authors:
- Westphal, Andrew J.
Bechtel, Hans A.
Brenker, Frank E.
Butterworth, Anna L.
Flynn, George
Frank, David R.
Gainsforth, Zack
Hillier, Jon K.
Postberg, Frank
Simionovici, Alexandre S.
Sterken, Veerle J.
Stroud, Rhonda M.
Allen, Carlton
Anderson, David
Ansari, Asna
Bajt, Saša
Bastien, Ron K.
Bassim, Nabil
Borg, Janet
Bridges, John
Brownlee, Donald E.
Burchell, Mark
Burghammer, Manfred
Changela, Hitesh
Cloetens, Peter
Davis, Andrew M.
Doll, Ryan
Floss, Christine
Grün, Eberhard
Heck, Philipp R.
Hoppe, Peter
Hudson, Bruce
Huth, Joachim
Hvide, Brit
Kearsley, Anton
King, Ashley J.
Lai, Barry
Leitner, Jan
Lemelle, Laurence
Leroux, Hugues
Leonard, Ariel
Lettieri, Robert
Marchant, William
Nittler, Larry R.
Ogliore, Ryan
Ong, Wei Ja
Price, Mark C.
Sandford, Scott A.
Tresseras, Juan‐Angel Sans
Schmitz, Sylvia
Schoonjans, Tom
Silversmit, Geert
Solé, Vicente A.
Srama, Ralf
Stadermann, Frank
Stephan, Thomas
Stodolna, Julien
Sutton, Steven
Trieloff, Mario
Tsou, Peter
Tsuchiyama, Akira
Tyliszczak, Tolek
Vekemans, Bart
Vincze, Laszlo
Von Korff, Joshua
Wordsworth, Naomi
Zevin, Daniel
Zolensky, Michael E.
>30, 000 Stardust@home dusters
… (more) - Abstract:
- <abstract abstract-type="main" id="maps12221-abs-0001"> <title>Abstract</title> <p>With the discovery of bona fide extraterrestrial materials in the Stardust Interstellar Dust Collector, NASA now has a fundamentally new returned sample collection, after the Apollo, Antarctic meteorite, Cosmic Dust, Genesis, Stardust Cometary, Hayabusa, and Exposed Space Hardware samples. Here, and in companion papers in this volume, we present the results from the Preliminary Examination of this collection, the Stardust Interstellar Preliminary Examination (ISPE). We found extraterrestrial materials in two tracks in aerogel whose trajectories and morphology are consistent with an origin in the interstellar dust stream, and in residues in four impacts in the aluminum foil collectors. While the preponderance of evidence, described in detail in companion papers in this volume, points toward an interstellar origin for some of these particles, alternative origins have not yet been eliminated, and definitive tests through isotopic analyses were not allowed under the terms of the ISPE. In this summary, we answer the central questions of the ISPE: How many tracks in the collector are consistent in their morphology and trajectory with interstellar particles? How many of these potential tracks are consistent with real interstellar particles, based on chemical analysis? Conversely, what fraction of candidates are consistent with either a secondary or interplanetary origin? What is the mass distribution<abstract abstract-type="main" id="maps12221-abs-0001"> <title>Abstract</title> <p>With the discovery of bona fide extraterrestrial materials in the Stardust Interstellar Dust Collector, NASA now has a fundamentally new returned sample collection, after the Apollo, Antarctic meteorite, Cosmic Dust, Genesis, Stardust Cometary, Hayabusa, and Exposed Space Hardware samples. Here, and in companion papers in this volume, we present the results from the Preliminary Examination of this collection, the Stardust Interstellar Preliminary Examination (ISPE). We found extraterrestrial materials in two tracks in aerogel whose trajectories and morphology are consistent with an origin in the interstellar dust stream, and in residues in four impacts in the aluminum foil collectors. While the preponderance of evidence, described in detail in companion papers in this volume, points toward an interstellar origin for some of these particles, alternative origins have not yet been eliminated, and definitive tests through isotopic analyses were not allowed under the terms of the ISPE. In this summary, we answer the central questions of the ISPE: How many tracks in the collector are consistent in their morphology and trajectory with interstellar particles? How many of these potential tracks are consistent with real interstellar particles, based on chemical analysis? Conversely, what fraction of candidates are consistent with either a secondary or interplanetary origin? What is the mass distribution of these particles, and what is their state? Are they particulate or diffuse? Is there any crystalline material? How many detectable impact craters (&gt;100 nm) are there in the foils, and what is their size distribution? How many of these craters have analyzable residue that is consistent with extraterrestrial material? And finally, can craters from secondaries be recognized through crater morphology (e.g., ellipticity)?</p> </abstract> … (more)
- Is Part Of:
- Meteoritics & planetary science. Volume 49:Number 9(2014:Sep.)
- Journal:
- Meteoritics & planetary science
- Issue:
- Volume 49:Number 9(2014:Sep.)
- Issue Display:
- Volume 49, Issue 9 (2014)
- Year:
- 2014
- Volume:
- 49
- Issue:
- 9
- Issue Sort Value:
- 2014-0049-0009-0000
- Page Start:
- 1720
- Page End:
- 1733
- Publication Date:
- 2014-08-22
- Subjects:
- Meteorites -- Periodicals
Planetology -- Periodicals
523.4 - Journal URLs:
- http://onlinelibrary.wiley.com/journal/10.1111/(ISSN)1945-5100 ↗
http://www.uark.edu/%7Emeteor/ ↗
http://www.uark.edu/meteor/ ↗
http://adsabs.harvard.edu/tocservice.html ↗
http://onlinelibrary.wiley.com/ ↗ - DOI:
- 10.1111/maps.12221 ↗
- Languages:
- English
- ISSNs:
- 1086-9379
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 5703.350000
British Library DSC - BLDSS-3PM
British Library STI - ELD Digital store - Ingest File:
- 3595.xml