Quick
Search: 
 
advanced search
 GSW Home    GeoRef Home    My GSW Alerts    Contact GSW    About GSW    Journals List    Help 
Elements Don't get GSW? Talk to your librarian.
JOURNAL HOME HELP CONTACT PUBLISHER SUBSCRIBE ARCHIVE SEARCH TABLE OF CONTENTS

Elements; March 2005; v. 1; no. 2; p. 79-84; DOI: 10.2113/gselements.1.2.79
© 2005 Mineralogical Society of America
This Article
Right arrow Figures Only
Right arrow Full Text
Right arrow Full Text (PDF)
Right arrow Alert me when this article is cited
Right arrow Alert me if a correction is posted
Right arrow Citation Map
Services
Right arrow Email this article to a friend
Right arrow Related articles in Elements
Right arrow Similar articles in this journal
Right arrow Alert me to new issues of the journal
Right arrow Download to citation manager
Right arrow reprints & permissions
Citing Articles
Right arrow Citing Articles via HighWire
Right arrow Citing Articles via Google Scholar
Google Scholar
Right arrow Articles by Cartigny, P.
Right arrow Search for Related Content
GeoRef
Right arrow GeoRef Citation

Stable Isotopes and the Origin of Diamond

Pierre Cartigny1

1 Laboratoire de Géochimie des Isotopes Stables, Institut de Physique
du Globe de Paris, 4 place Jussieu, Paris Cédex 75251, France
E-mail: cartigny{at}ipgp.jussieu.fr

Most diamonds form in a relatively narrow depth interval of Earth's subcontinental mantle between 150 and 250 km. From carbon isotope analyses of diamond obtained in the 1970s, it was first proposed that eclogitic diamonds form from crustal carbon recycled into the mantle by subduction and that the more abundant peridotitic diamonds formed from mantle carbon. More recent stable isotope studies using nitrogen, oxygen, and sulfur, as well as carbon, combined with studies of mineral inclusions within diamonds, have strengthened arguments supporting and opposing the early proposal. The conflicting evidence is reconciled if mantle carbon is introduced via fluid into mantle eclogites and peridotites, some of which represent subducted oceanic crust.

KEYWORDS: diamond, stable isotopes, mantle, metasomatism


Related articles in Elements:

Diamonds
George E. Harlow and Rondi M. Davies
Elements 2005 1: 67-70. [Abstract] [Full Text]  



This article has been cited by other articles:


Home page
Mineral MagHome page
B. Harte, T. Taniguchi, and S. Chakraborty
Diffusion in diamond. II. High-pressure-temperature experiments
Mineralogical Magazine, August 4, 2009; 73(2): 201 - 204.
[Abstract] [Full Text] [PDF]


Home page
Eur J MineralHome page
G. Dorsam, A. Liebscher, B. Wunder, G. Franz, and M. Gottschalk
Crystal structure refinement of synthetic Ca0.43Sr0.57[SiO3]-walstromite and walstromite-fluid Ca-Sr distribution at upper-mantle conditions
European Journal of Mineralogy, August 1, 2009; 21(4): 705 - 714.
[Abstract] [Full Text] [PDF]


Home page
ELEMENTSHome page
L. A. Groat and B. M. Laurs
Gem Formation, Production, and Exploration: Why Gem Deposits Are Rare and What is Being Done to Find Them
Elements, June 1, 2009; 5(3): 153 - 158.
[Abstract] [Full Text] [PDF]


Home page
South African Journal of GeologyHome page
A.E. Moore
Type II diamonds: Flamboyant Megacrysts?
South African Journal of Geology, March 1, 2009; 112(1): 23 - 38.
[Abstract] [Full Text] [PDF]


Home page
Geological Society of America Special PapersHome page
Y. A. Litvin
High-pressure mineralogy of diamond genesis
Geological Society of America Special Papers, January 1, 2007; 421(0): 83 - 103.
[Abstract] [Full Text] [PDF]




JOURNAL HOME HELP CONTACT PUBLISHER SUBSCRIBE ARCHIVE SEARCH TABLE OF CONTENTS
Copyright © 2009 by Mineralogical Society of America