Results 111 to 120 of about 441 (171)
Prebiotic organic compounds in samples of asteroid Bennu indicate heterogeneous aqueous alteration. [PDF]
Mojarro A +6 more
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Gamma activity concentrations of <sup>226</sup>Ra, <sup>232</sup>Th, <sup>40</sup>K, and health hazard assessments of granites from Wadi El-Nabi' mining area, Egyptian Nubian Shield. [PDF]
Shereif AS +5 more
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Actinide Elemental Ratios of Spent Nuclear Fuel Samples by Resonance Ionization Mass Spectrometry. [PDF]
Raiwa M +4 more
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Distribution of extraterrestrial nucleobases, other N-heterocycles, and their precursors in a sample from asteroid Bennu. [PDF]
Oba Y +12 more
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Stability of the fcc phase in shocked nickel up to 332 GPa. [PDF]
Pereira KA +19 more
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Present-day thermal and water activity environment of the Mars Sample Return collection. [PDF]
Zorzano MP +26 more
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Thirty Years of Astronomical Discovery With UKIRT, 2010
Cosmochemistry is a rapidly evolving field of planetary science and the second edition of this classic text reflects the exciting discoveries made over the past decade from new spacecraft missions. Topics covered include the synthesis of elements in stars, behaviour of elements and isotopes in the early solar nebula and planetary bodies, and ...
Bruce Fegley +2 more
exaly +3 more sources
Cosmochemistry is a rapidly evolving field of planetary science and the second edition of this classic text reflects the exciting discoveries made over the past decade from new spacecraft missions. Topics covered include the synthesis of elements in stars, behaviour of elements and isotopes in the early solar nebula and planetary bodies, and ...
Bruce Fegley +2 more
exaly +3 more sources
An introduction to cosmochemistry
Geochimica et Cosmochimica Acta, 1995This textbook describes the composition and evolution of material objects in the universe. The survey begins with a discussion of terrestrial materials and ends with the composition of quasars and distant galaxies. There are two main themes: chemical processes responsible for the abundances we observe, and nuclear processes in which the chemical ...
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Annual Review of Earth and Planetary Sciences, 2014
Evidence is now compelling that elements heavier than helium in many white dwarf atmospheres have accumulated by accretion from orbiting rocky bodies, often larger than 100 km in diameter, such as asteroids. Consequently, we now possess a powerful tool to measure the elemental constituents of extrasolar minor planets.
M. Jura, E.D. Young
openaire +1 more source
Evidence is now compelling that elements heavier than helium in many white dwarf atmospheres have accumulated by accretion from orbiting rocky bodies, often larger than 100 km in diameter, such as asteroids. Consequently, we now possess a powerful tool to measure the elemental constituents of extrasolar minor planets.
M. Jura, E.D. Young
openaire +1 more source

