The composition of stony meteorites (V) some aspects of the composition of the basaltic achondrites
ISSN: |
0012-821X
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Source: |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
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Topics: |
Geosciences
Physics
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Type of Medium: |
Electronic Resource
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URL: |
_version_ | 1798290778245562368 |
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autor | Ahrens, L.H. Von Michaelis, H. |
autorsonst | Ahrens, L.H. Von Michaelis, H. |
book_url | http://linkinghub.elsevier.com/retrieve/pii/0012-821X(69)90172-1 |
datenlieferant | nat_lic_papers |
fussnote | Unique compositional features characterize the basaltic achondrites (eucrites and howardites), notably; remarkably uniform Si and almost uniform Fe contents; a constant Ca/Al ratio which is equivalent to that of the chondrites; an almost uniform Na/K ratio also similar in magnitude to that in the chondrites and a seemingy unusually well-developed inverse Ca (or Al)-Mg relationship. These compositional features suggest strongly that the basaltic achondrites could not have been formed by a process of magnetic differentiation and that physical processes played a dominant role. |
hauptsatz | hsatz_simple |
identnr | NLZ180732072 |
issn | 0012-821X |
journal_name | Earth and Planetary Science Letters |
materialart | 1 |
package_name | Elsevier |
publikationsort | Amsterdam |
publisher | Elsevier |
reference | 6 (1969), S. 304-308 |
search_space | articles |
shingle_author_1 | Ahrens, L.H. Von Michaelis, H. |
shingle_author_2 | Ahrens, L.H. Von Michaelis, H. |
shingle_author_3 | Ahrens, L.H. Von Michaelis, H. |
shingle_author_4 | Ahrens, L.H. Von Michaelis, H. |
shingle_catch_all_1 | Ahrens, L.H. Von Michaelis, H. The composition of stony meteorites (V) some aspects of the composition of the basaltic achondrites 0012-821X 0012821X Elsevier |
shingle_catch_all_2 | Ahrens, L.H. Von Michaelis, H. The composition of stony meteorites (V) some aspects of the composition of the basaltic achondrites 0012-821X 0012821X Elsevier |
shingle_catch_all_3 | Ahrens, L.H. Von Michaelis, H. The composition of stony meteorites (V) some aspects of the composition of the basaltic achondrites 0012-821X 0012821X Elsevier |
shingle_catch_all_4 | Ahrens, L.H. Von Michaelis, H. The composition of stony meteorites (V) some aspects of the composition of the basaltic achondrites 0012-821X 0012821X Elsevier |
shingle_title_1 | The composition of stony meteorites (V) some aspects of the composition of the basaltic achondrites |
shingle_title_2 | The composition of stony meteorites (V) some aspects of the composition of the basaltic achondrites |
shingle_title_3 | The composition of stony meteorites (V) some aspects of the composition of the basaltic achondrites |
shingle_title_4 | The composition of stony meteorites (V) some aspects of the composition of the basaltic achondrites |
sigel_instance_filter | dkfz geomar wilbert ipn albert fhp |
source_archive | Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
timestamp | 2024-05-06T08:22:08.112Z |
titel | The composition of stony meteorites (V) some aspects of the composition of the basaltic achondrites |
titel_suche | The composition of stony meteorites (V) some aspects of the composition of the basaltic achondrites Unique compositional features characterize the basaltic achondrites (eucrites and howardites), notably; remarkably uniform Si and almost uniform Fe contents; a constant Ca/Al ratio which is equivalent to that of the chondrites; an almost uniform Na/K ratio also similar in magnitude to that in the chondrites and a seemingy unusually well-developed inverse Ca (or Al)-Mg relationship. These compositional features suggest strongly that the basaltic achondrites could not have been formed by a process of magnetic differentiation and that physical processes played a dominant role. |
topic | TE-TZ U |
uid | nat_lic_papers_NLZ180732072 |