Stardust Interstellar Preliminary Examination IV: Scanning transmission X-ray microscopy analyses of impact features in the Stardust Interstellar Dust Collector - Université Claude Bernard Lyon 1 Access content directly
Journal Articles Meteoritics and Planetary Science Year : 2014

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

Hugues Leroux
  • Function : Author
Ariel Leonard
  • Function : Author
Robert Lettieri
  • Function : Author
William Marchant
  • Function : Author
Larry R. Nittler
  • Function : Author
Ryan Ogliore
  • Function : Author
Wei Ja Ong
  • Function : Author
Frank Postberg
  • Function : Author
Mark C. Price
  • Function : Author
Scott A. Sandford
  • Function : Author
Juan-Angel Sans Tresseras
  • Function : Author
Sylvia Schmitz
  • Function : Author
Tom Schoonjans
  • Function : Author
Geert Silversmit
  • Function : Author
Alexandre S. Simionovici
  • Function : Author
Vicente A. Sole
  • Function : Author
Ralf Srama
  • Function : Author
Frank J. Stadermann
  • Function : Author
Thomas Stephan
  • Function : Author
Veerle J. Sterken
  • Function : Author
Rhonda M. Stroud
  • Function : Author
Steven Sutton
  • Function : Author
Mario Trieloff
  • Function : Author
Peter Tsou
  • Function : Author
Akira Tsuchiyama
  • Function : Author
Bart Vekemans
  • Function : Author
Laszlo Vincze
  • Function : Author
Joshua von Korff
  • Function : Author
Naomi Wordsworth
  • Function : Author
Daniel Zevin
  • Function : Author
Michael E. Zolensky
  • Function : Author
Anna L. Butterworth
  • Function : Author
Andrew J. Westphal
  • Function : Author
Tolek Tyliszczak
  • Function : Author
Zack Gainsforth
  • Function : Author
Julien Stodolna
  • Function : Author
David R. Frank
  • Function : Author
Carlton Allen
  • Function : Author
David Anderson
Asna Ansari
  • Function : Author
Sasa Bajt
  • Function : Author
Ron K. Bastien
  • Function : Author
Nabil Bassim
  • Function : Author
Hans A. Bechtel
  • Function : Author
Janet Borg
  • Function : Author
Frank E. Brenker
  • Function : Author
John Bridges
  • Function : Author
Donald E. Brownlee
  • Function : Author
Mark Burchell
  • Function : Author
Manfred Burghammer
  • Function : Author
Hitesh Changela
  • Function : Author
Peter Cloetens
  • Function : Author
Andrew M. Davis
  • Function : Author
Ryan Doll
  • Function : Author
Christine Floss
  • Function : Author
George Flynn
  • Function : Author
Eberhard Gruen
  • Function : Author
Philipp R. Heck
  • Function : Author
Jon K. Hillier
  • Function : Author
Peter Hoppe
  • Function : Author
Bruce Hudson
  • Function : Author
Joachim Huth
  • Function : Author
Brit Hvide
  • Function : Author
Anton Kearsley
  • Function : Author
Ashley J. King
  • Function : Author
Barry Lai
  • Function : Author
Jan Leitner
  • Function : Author

Abstract

We 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. Samples were analyzed in aerogel by acquiring high spatial resolution maps and high energy-resolution spectra of major rock-forming elements Mg, Al, Si, Fe, and others. We developed diagnostic screening tests to reject spacecraft secondary ejecta and terrestrial contaminants from further consideration as interstellar dust candidates. The results support an extraterrestrial origin for three interstellar candidates: I1043,1,30 (Orion) is a 3 pg particle with Mg-spinel, forsterite, and an iron-bearing phase. I1047,1,34 (Hylabrook) is a 4 pg particle comprising an olivine core surrounded by low-density, amorphous Mg-silicate and amorphous Fe, Cr, and Mn phases. I1003,1,40 (Sorok) has the track morphology of a high-speed impact, but contains no detectable residue that is convincingly distinguishable from the background aerogel. Twenty-two samples with an anthropogenic origin were rejected, including four secondary ejecta from impacts on the Stardust spacecraft aft solar panels, nine ejecta from secondary impacts on the Stardust Sample Return Capsule, and nine contaminants lacking evidence of an impact. Other samples in the collection included I1029,1,6, which contained surviving solar system impactor material. Four samples remained ambiguous: I1006,2,18, I1044,2,32, and I1092,2,38 were too dense for analysis, and we did not detect an intact projectile in I1044,3,33. We detected no radiation effects from the synchrotron soft X-ray analyses; however, we recorded the effects of synchrotron hard X-ray radiation on I1043,1,30 and I1047,1,34.

Dates and versions

hal-02351072 , version 1 (06-11-2019)

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Cite

Laurence Lemelle, Hugues Leroux, Ariel Leonard, Robert Lettieri, William Marchant, et al.. Stardust Interstellar Preliminary Examination IV: Scanning transmission X-ray microscopy analyses of impact features in the Stardust Interstellar Dust Collector. Meteoritics and Planetary Science, 2014, 49 (9, SI), pp.1562--1593. ⟨10.1111/maps.12220⟩. ⟨hal-02351072⟩
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