New Insights into the Carrier Phase(s) of Extraterrestrial He-3 in Geologically Old Sediments

DSpace/Manakin Repository

New Insights into the Carrier Phase(s) of Extraterrestrial He-3 in Geologically Old Sediments

Citable link to this page

. . . . . .

Title: New Insights into the Carrier Phase(s) of Extraterrestrial He-3 in Geologically Old Sediments
Author: Farley, Ken; Mukhopadhyay, Sujoy

Note: Order does not necessarily reflect citation order of authors.

Citation: Mukhopadhyay, Sujoy, and Ken A. Farley. 2006. New insights into the carrier phase(s) of extraterrestrial He-3 in geologically old sediments. Geochimica et Cosmochimica Acta 70(19): 5061-5073.
Access Status: At the direction of the depositing author this work is not currently accessible through DASH.
Full Text & Related Files:
Abstract: To better understand the composition, characteristics of helium diffusion, and size distribution of interplanetary dust particles (IDPs) responsible for the long-term retention of extraterrestrial 3He, we carried out leaching, stepped heating, and sieving experiments on pelagic clays that varied in age from 0.5 Ma to similar to 90 Myr. The leaching experiments suggest that the host phase(s) of 3He in geologically old sediments are neither organic matter nor refractory phases, such as diamond, graphite, Al2O3, and SiC, but are consistent with extraterrestrial silicates, Fe-Ni sulfides, and possibly magnetite. Stepped heating experiments demonstrate that the 3He release profiles from the magnetic and non-magnetic components of the pelagic clays are remarkably similar. Because helium diffusion is likely to be controlled by mineral chemistry and structure, the stepped heating results suggest a single carrier that may be magnetite, or more probably a phase associated with magnetite. Furthermore, the stepped outgassing experiments indicate that about 20% of the 3He will be lost through diffusion at seafloor temperatures after 50 Myrs, while sedimentary rocks exposed on the Earth's surface for the same amount of time would lose up to 60%. The absolute magnitude of the 3 He loss is, however, likely to depend upon the 3He concentration profile within the IDPs, which is not well known. Contrary to previous suggestions that micrometeorites in the size range of 50-100 mu m in diameter are responsible for the extraterrestrial 3He in geologically old sediments [Stuart, F.M., Harrop, P.J., Knott, S., Turner, G., 1999. Laser extraction of helium isotopes from Antarctic micrometeorites: source of He and implications for the flux of extraterrestrial 3He flux to earth. Geochim. Cosmochim. Acta 63,2653-2665 ], our sieving experiment demonstrates that at most 20% of the 3He is carried by particles greater than 50 mu m in diameter. The size-distribution of the 3He-bearing particles implies that extraterrestrial 3He in sediments record the IDP flux rather than the micrometeorite flux.
Published Version: http://dx.doi.org/10.1016/j.gca.2006.06.1566
Other Sources: http://www.people.fas.harvard.edu/%7emukhop/Carrierphase.pdf
Citable link to this page: http://nrs.harvard.edu/urn-3:HUL.InstRepos:3224736

Show full Dublin Core record

This item appears in the following Collection(s)

  • FAS Scholarly Articles [7106]
    Peer reviewed scholarly articles from the Faculty of Arts and Sciences of Harvard University
 
 

Search DASH


Advanced Search
 
 

Submitters