Deep mantle origin of kimberlite magmas revealed by neon isotopes

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

5

Geochemistry: Composition Of The Mantle, Geochemistry: Intra-Plate Processes (3615, 8415), Geochemistry: Mantle Processes (3621), Geochemistry: Radiogenic Isotope Geochemistry, Geochemistry: Stable Isotope Geochemistry (0454, 4870)

Scientific paper

We measured noble gases in olivines extracted from alteration-free samples of the Udachnaya-East kimberlite pipe, eastern Siberia. Neon isotope ratios indicate that the kimberlite has a less nucleogenic Ne signature than a typical mid-ocean ridge basalt (MORB) source, which is consistent with the less radiogenic 40Ar/36Ar ratio compared to MORB and subcontinental lithospheric mantle (SCLM) sources. Based on He-Ne systematics, the 3He/4He ratio of the plume source of the Udachnaya kimberlite pipe would be higher than 15 RA with the dominant He signature of the magma acquired by assimilation of SCLM and/or crustal material during magma ascent. Our results indicate that the source of the Udachnaya kimberlite has similar noble gas characteristics to those of ocean island basalts (OIBs). Its origin is therefore deeper than that of the MORB source mantle, and probably is the same as the OIB-source mantle.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Deep mantle origin of kimberlite magmas revealed by neon isotopes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Deep mantle origin of kimberlite magmas revealed by neon isotopes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Deep mantle origin of kimberlite magmas revealed by neon isotopes will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1780762

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.