Titlebook: Cosmochemistry; Proceedings of the S A. G. W. Cameron Conference proceedings 1973 D. Reidel Publishing Company, Dordrecht, Holland 1973 cos

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A Cosmochemical View of Cosmic Rays and Solar Particles,d solar matter. The composition of solar particles changes with energy and from flare to flare. A strong excess of heavy elements at energies below a few MeV/nuc decreases with energy, and at energies above ~15 MeV/nuc the composition of solar particles resembles that of galactic cosmic rays somewha

manifestation

MEET

Chemistry of the Solar Nebula,sses which took place in the primitive solar nebula. Chondrites thus are thought to contain a unique record of the physico-chemical conditions which prevailed at the time and place (asteroid belt) of their origin. Elemental abundance patterns are an important clue to the events and processes. Most e

Chronic

The Moon as a High Temperature Condensate,of the terrestrial planets and the Moon. An important factor is the variation of pressure and temperature with distance from the Sun, and in the case of the Moon and captured satellites of other planets, with distance from the median plane. Current estimates of the temperature and pressure in the so

ectropion

The Giant Planets, and Saturn because of the accuracy with which relevant equations of state are presently known. Current results are consistent with solar composition for Jupiter and perhaps also for Saturn. New theoretical techniques for calculating the gravitational multipole moments of rotating liquid planets may

事情

MAZE

一再困擾

美色花錢

,Introduction: ‘Trans-Scripts’,allic-lined stars); and (c) Population effects that may be related to the evolution of the Galaxy (correlation between stellar age and metal abundance, differences in details of heavy-element mixture in atmospheric composition of normal stars that have not reached an advanced evolutionary stage).

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