Constraints on Neon and Argon Isotopic Fractionation in Solar Wind

Author:

Meshik Alex12345,Mabry Jennifer12345,Hohenberg Charles12345,Marrocchi Yves12345,Pravdivtseva Olga12345,Burnett Donald12345,Olinger Chad12345,Wiens Roger12345,Reisenfeld Dan12345,Allton Judith12345,McNamara Karen12345,Stansbery Eileen12345,Jurewicz Amy J. G.12345

Affiliation:

1. Physics Department, Washington University, St. Louis, MO 63130, USA.

2. Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.

3. Neutron Science and Technology, MS H803, Los Alamos National Laboratory, Los Alamos, NM 87545, USA.

4. Space Science and Applications, MS D466, Los Alamos National Laboratory, Los Alamos, NM 87545, USA.

5. Physics and Astronomy Department, University of Montana, SC 121, 32 Campus Drive, MS 1080, Missoula, MT 59812, USA.

Abstract

To evaluate the isotopic composition of the solar nebula from which the planets formed, the relation between isotopes measured in the solar wind and on the Sun's surface needs to be known. The Genesis Discovery mission returned independent samples of three types of solar wind produced by different solar processes that provide a check on possible isotopic variations, or fractionation, between the solar-wind and solar-surface material. At a high level of precision, we observed no significant inter-regime differences in 20 Ne/ 22 Ne or 36 Ar/ 38 Ar values. For 20 Ne/ 22 Ne, the difference between low- and high-speed wind components is 0.24 ± 0.37%; for 36 Ar/ 38 Ar, it is 0.11 ± 0.26%. Our measured 36 Ar/ 38 Ar ratio in the solar wind of 5.501 ± 0.005 is 3.42 ± 0.09% higher than that of the terrestrial atmosphere, which may reflect atmospheric losses early in Earth's history.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference30 articles.

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3. Interstellar Chemistry Recorded in Organic Matter from Primitive Meteorites

4. R. Wieler, H. Busemann, I. Franchi, in Meteorites and the Early Solar System II, D. S. Lauretta, H. McSween Jr., Eds. (Univ. of Arizona, Tucson, AZ, 2006), part vi, pp. 499–521.

5. Nuclear-energy generation in the interior of the Sun has produced significant elemental and isotopic changes but matter is not exchanged between the inner and outer regions so with a few exceptions the composition of the solar surface has remained unchanged since the beginning of the solar system.

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