Zobrazeno 1 - 10
of 25
pro vyhledávání: '"I. S. Sanders"'
Publikováno v:
Meteoritics & Planetary Science. 52:690-708
Ureilite meteorites are abundant, carbon-rich, primitive achondrites made of coarse-grained, equilibrated olivine and pyroxene (usually pigeonite). They probably sample the baked, heterogeneous, melt-depleted mantle of a large, once-chondritic parent
Whole rock Δ(17)O and nucleosynthetic isotopic variations for chromium, titanium, nickel, and molybdenum in meteorites define two isotopically distinct populations: carbonaceous chondrites (CCs) and some achondrites, pallasites, and irons in one and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8a3ed1daf5afe1f841e7d11ec94f2744
https://europepmc.org/articles/PMC6398615/
https://europepmc.org/articles/PMC6398615/
Autor:
I. S. Sanders
Publikováno v:
A revised correlation of Pre-Cambrian rocks in the British Isles ISBN: 9781897799116
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2837afc5153f559bd037ae5622d6b22a
https://doi.org/10.1144/sr22.7
https://doi.org/10.1144/sr22.7
Autor:
I. S. Sanders, Edward Scott
Publikováno v:
Meteoritics & Planetary Science. 47:2170-2192
– We investigate the hypothesis that many chondrules are frozen droplets of spray from impact plumes launched when thin-shelled, largely molten planetesimals collided at low speed during accretion. This scenario, here dubbed “splashing,” stems
Publikováno v:
Geochimica et Cosmochimica Acta. 73:5835-5853
A few eucrites have anomalous oxygen isotopic compositions. To help understand their origin and identify additional samples, we have analyzed the oxygen isotopic compositions of 18 eucrites and four diogenites. Except for five eucrites, these meteori
Autor:
I. S. Sanders, Edward Scott
Publikováno v:
Geochimica et Cosmochimica Acta. 73:5137-5149
An excellent 53 Mn– 53 Cr isochron for bulk CI, CM, CO, CV, CB, and ungrouped C3 chondrites seems to suggest that each carbonaceous chondrite group acquired its Mn/Cr ratio 4568 ± 1 Myr ago. This age is indistinguishable from the age of Ca–Al-ri
Autor:
I. S. Sanders, Phonsie J. Hevey
Publikováno v:
Meteoritics & Planetary Science. 41:95-106
The melting of planetesimals heated by 26 Al has been modelled using a new finite difference method that incorporates convection. As an example, we consider a planetesimal with a radius of 64 km, which accretes instantaneously at t = 0.75 Myr (after
Publikováno v:
Nature. 420:156-159
There have recently been various reports of weak ferromagnetism in graphite (1,2) and synthetic carbon materials (3) such as rhombohedral C60 (4), as well as a theoretical prediction of a ferromagnetic instability in graphene sheets (5). With very sm
Autor:
D. H. Doff, I. S. Sanders
Publikováno v:
Mineralogical Magazine. 55:167-172
Deep azure-blue beryl is reported from veins in Upper Devonian conglomerate from southeast Ireland. Microprobe analysis, Mössbauer spectroscopy and loss on ignition suggest an unusual chemistry with an exceptionally high degree of substitution of Fe