Zobrazeno 1 - 10
of 894
pro vyhledávání: '"O. A. SCHAEFFER"'
Publikováno v:
Annals of the New York Academy of Sciences. 119:347-350
Autor:
Sahoo, R. N.1, Paul, M.1 paul@vms.huji.ac.il, Köster, U.2, Scott, R.3, Tessler, M.4, Zylstra, A.5, Avila, M. L.3, Dickerson, C.3, Jayatissa, H.3, Kohen, M.S.1, McLain, J.3, Pardo, R.C.3, Rehm, K. E.3, Tolstukhin, I.3, Vondrasek, R.3, Bailey, T.6, Callahan, L.6, Clark, A.6, Collon, P.6, Kashiv, Y.6
Publikováno v:
EPJ Web of Conferences. 5/26/2023, Vol. 284, p1-4. 4p.
Publikováno v:
Geophysical Research Letters. 5:219-222
Concentrations of argon-39 produced by cosmic rays in the metal in 30 meteorites are remarkably similar, but they are slightly higher than expected for the present solar-cycle-averaged flux of cosmic rays. This supports the idea suggested by Eddy (19
Autor:
O. A. Schaeffer, G. Heusser
Publikováno v:
Earth and Planetary Science Letters. 33:420-427
Cosmic-ray-produced 37 Ar ( t 1/2 = 35 days), and 39 Ar ( t 1/2 = 269 years) in the Fe-Ni phase of meteorites have been studied in connection with their implications for the radial gradient of cosmic ray particles. For the chondrite, Can˜on City, wh
Publikováno v:
Earth and Planetary Science Letters. 31:358-368
The crystallization ages of a suite of Apollo 17 basalts from four different stations have been measured using the Ar-39 to Ar-40 stepwise heating technique. The rocks analyzed include all principal petrographic types found at Apollo 17 landing site.
Publikováno v:
Planetary and Space Science. 29:1109-1118
The space erosion of stony meteorites has been determined to be 650μm 106y−1, while that of iron meteorites has been determined to be 22 μm 106y−1. The erosion rates are based on flux and size distributions of small particles in the solar syste
Autor:
William C. Burnett, O. A. Schaeffer
Publikováno v:
Estuarine and Coastal Marine Science. 11:605-611
In order to evaluate the influence of the ocean dumping of sewage sludge upon the organic carbon fraction of sediments of the New York Bight, a study of carbon isotopic variations in surface sediments from the area has been completed. On the basis of
Autor:
Liaquat Husain, O. A. Schaeffer
Publikováno v:
Geophysical Research Letters. 2:29-32
From a stepwise-heating experiment on neutron-irradiated samples of whole rock and a plagioclase separate, an Ar-40/Ar-39 age of 4.26 plus or minus 0.02 G.y. was determined for the Apollo 17 troctolite 76535. This rock is believed to have formed as a
Autor:
O. A. Schaeffer
Publikováno v:
Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences. 285:137-143
We have heard earlier in this Discussion Meeting that from the systematics of Sr and Pb isotopes in lunar samples, it is possible to ascertain that the Moon had a solid crust about 4.6 Ga ago, that is, very soon after the formation of the solar syste
Autor:
O A Schaeffer
Publikováno v:
Annual Review of Physical Chemistry. 13:151-170
A review is presented of the radioactive and stable nuclides produced in meteorites by cosmic rays. The question of constancy of cosmic rays in time and space is considered along with the exposure ages of meteorites. (D.L.C.)