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Gary R. Huss

Researcher at University of Hawaii at Manoa

Publications -  240
Citations -  8713

Gary R. Huss is an academic researcher from University of Hawaii at Manoa. The author has contributed to research in topics: Chondrite & Chondrule. The author has an hindex of 51, co-authored 228 publications receiving 8012 citations. Previous affiliations of Gary R. Huss include University of New Mexico & University of Southern California.

Papers
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Presolar diamond, sic, and graphite in primitive chondrites : abundances as a function of meteorite class and petrologic type

Gary R. Huss, +1 more
- 01 Jan 1995 - 
TL;DR: In this article, diamond and SiC were found in unmetamorphosed members of all seven chondrite classes and evidence for graphite was found in Orgued (CI) and LL3.1 chondrites.
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Noble gases in presolar diamonds I: Three distinct components and their implications for diamond origins

Gary R. Huss, +2 more
- 01 Nov 1994 - 
TL;DR: In this article, three distinct noble gas components are present in diamonds, HL, P3, and P6, each of which is found to consist of five noble gases, and they were measured using stepped pyrolysis.
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Evidence for Widespread 26Al in the Solar Nebula and Constraints for Nebula Time Scales

Sara S. Russell, +4 more
- 09 Aug 1996 - 
TL;DR: The absence of 26Mg* from the decay of 26Al in Al-rich objects from unequilibrated ordinary chondrites indicates that the lifetime of the solar nebula over which CAIs and chondrules formed extended over ∼5 million years.
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The matrices of unequilibrated ordinary chondrites: Implications for the origin and history of chondrites

Gary R. Huss, +2 more
- 01 Jan 1981 - 
TL;DR: The fine-grained, opaque, silicate matrix of type 3 unequilibrated chondrites was examined by optical microscopy, an electron microprobe, and a scanning electron microscope as mentioned in this paper.
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Origin and chronology of chondritic components: A review

Alexander N. Krot, +16 more
- 01 Sep 2009 - 
TL;DR: In this article, the x-wind model vs. the shock-wave model of the origin of chondritic components and irradiation vs. stellar origin of short-lived radionuclides are compared.