Multiple nitrogen isotopic components coexisting in ureilites
Abstract— Nitrogen and noble gas isotopic compositions and C abundance of ureilites were analyzed using a stepwise combustion technique. Four Antarctic ureilites, ALHA77257, Asuka 881931, Yamato 791538 and Yamato 790981 were analyzed. Multiple N isotopic components were observed in these ureilites....
Published in: | Meteoritics & Planetary Science |
---|---|
Main Authors: | , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
Wiley
1998
|
Subjects: | |
Online Access: | http://dx.doi.org/10.1111/j.1945-5100.1998.tb01692.x https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1111%2Fj.1945-5100.1998.tb01692.x https://onlinelibrary.wiley.com/doi/pdf/10.1111/j.1945-5100.1998.tb01692.x |
id |
crwiley:10.1111/j.1945-5100.1998.tb01692.x |
---|---|
record_format |
openpolar |
spelling |
crwiley:10.1111/j.1945-5100.1998.tb01692.x 2024-09-15T17:48:30+00:00 Multiple nitrogen isotopic components coexisting in ureilites YAMAMOTO, TOMOKO HASHIZUME, KO MATSUDA, JUN‐ICHI KASE, TOMOHIKO 1998 http://dx.doi.org/10.1111/j.1945-5100.1998.tb01692.x https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1111%2Fj.1945-5100.1998.tb01692.x https://onlinelibrary.wiley.com/doi/pdf/10.1111/j.1945-5100.1998.tb01692.x en eng Wiley http://onlinelibrary.wiley.com/termsAndConditions#vor Meteoritics & Planetary Science volume 33, issue 4, page 857-870 ISSN 1086-9379 1945-5100 journal-article 1998 crwiley https://doi.org/10.1111/j.1945-5100.1998.tb01692.x 2024-08-22T04:17:46Z Abstract— Nitrogen and noble gas isotopic compositions and C abundance of ureilites were analyzed using a stepwise combustion technique. Four Antarctic ureilites, ALHA77257, Asuka 881931, Yamato 791538 and Yamato 790981 were analyzed. Multiple N isotopic components were observed in these ureilites. The δ 15 N values of these N components ranged from +160 to −120%. The minimum δ 15 N values of typically −120% were observed at combustion temperatures at 700–900 °C where large amounts of C were released. A heavy N component was observed in only two ureilites, ALHA77257 and Asuka 881931. Silicate‐enriched fractions and C‐concentrated fractions were prepared for these two ureilites. We conclude that both the light N and the heavy N are trapped in the carbonaceous vein minerals. The lack of correction between the N/C ratio and the 36 Ar/C ratio suggests that the primary carrier phase of the light N does not correspond to that of the planetary noble gases. We consider that the isotopically heavy N, which was observed in this study, is related to the heavy N observed among polymict ureilites. Small amounts (<0.5 ppm) of light N with the minimum δ 15 N value of −120% were observed among the silicate fractions at the highest combustion temperature of 1200 °C, although the exact carrier phase of this light N is not known. We consider that the currently observed ureilites were produced by injection of several volatile‐rich objects into volatile‐poor ureilitic silicates. Article in Journal/Newspaper Antarc* Antarctic Wiley Online Library Meteoritics & Planetary Science 33 4 857 870 |
institution |
Open Polar |
collection |
Wiley Online Library |
op_collection_id |
crwiley |
language |
English |
description |
Abstract— Nitrogen and noble gas isotopic compositions and C abundance of ureilites were analyzed using a stepwise combustion technique. Four Antarctic ureilites, ALHA77257, Asuka 881931, Yamato 791538 and Yamato 790981 were analyzed. Multiple N isotopic components were observed in these ureilites. The δ 15 N values of these N components ranged from +160 to −120%. The minimum δ 15 N values of typically −120% were observed at combustion temperatures at 700–900 °C where large amounts of C were released. A heavy N component was observed in only two ureilites, ALHA77257 and Asuka 881931. Silicate‐enriched fractions and C‐concentrated fractions were prepared for these two ureilites. We conclude that both the light N and the heavy N are trapped in the carbonaceous vein minerals. The lack of correction between the N/C ratio and the 36 Ar/C ratio suggests that the primary carrier phase of the light N does not correspond to that of the planetary noble gases. We consider that the isotopically heavy N, which was observed in this study, is related to the heavy N observed among polymict ureilites. Small amounts (<0.5 ppm) of light N with the minimum δ 15 N value of −120% were observed among the silicate fractions at the highest combustion temperature of 1200 °C, although the exact carrier phase of this light N is not known. We consider that the currently observed ureilites were produced by injection of several volatile‐rich objects into volatile‐poor ureilitic silicates. |
format |
Article in Journal/Newspaper |
author |
YAMAMOTO, TOMOKO HASHIZUME, KO MATSUDA, JUN‐ICHI KASE, TOMOHIKO |
spellingShingle |
YAMAMOTO, TOMOKO HASHIZUME, KO MATSUDA, JUN‐ICHI KASE, TOMOHIKO Multiple nitrogen isotopic components coexisting in ureilites |
author_facet |
YAMAMOTO, TOMOKO HASHIZUME, KO MATSUDA, JUN‐ICHI KASE, TOMOHIKO |
author_sort |
YAMAMOTO, TOMOKO |
title |
Multiple nitrogen isotopic components coexisting in ureilites |
title_short |
Multiple nitrogen isotopic components coexisting in ureilites |
title_full |
Multiple nitrogen isotopic components coexisting in ureilites |
title_fullStr |
Multiple nitrogen isotopic components coexisting in ureilites |
title_full_unstemmed |
Multiple nitrogen isotopic components coexisting in ureilites |
title_sort |
multiple nitrogen isotopic components coexisting in ureilites |
publisher |
Wiley |
publishDate |
1998 |
url |
http://dx.doi.org/10.1111/j.1945-5100.1998.tb01692.x https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1111%2Fj.1945-5100.1998.tb01692.x https://onlinelibrary.wiley.com/doi/pdf/10.1111/j.1945-5100.1998.tb01692.x |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_source |
Meteoritics & Planetary Science volume 33, issue 4, page 857-870 ISSN 1086-9379 1945-5100 |
op_rights |
http://onlinelibrary.wiley.com/termsAndConditions#vor |
op_doi |
https://doi.org/10.1111/j.1945-5100.1998.tb01692.x |
container_title |
Meteoritics & Planetary Science |
container_volume |
33 |
container_issue |
4 |
container_start_page |
857 |
op_container_end_page |
870 |
_version_ |
1810289790847811584 |