Results 111 to 120 of about 441 (171)

Prebiotic organic compounds in samples of asteroid Bennu indicate heterogeneous aqueous alteration. [PDF]

open access: yesProc Natl Acad Sci U S A
Mojarro A   +6 more
europepmc   +1 more source

Actinide Elemental Ratios of Spent Nuclear Fuel Samples by Resonance Ionization Mass Spectrometry. [PDF]

open access: yesJ Am Soc Mass Spectrom
Raiwa M   +4 more
europepmc   +1 more source

Distribution of extraterrestrial nucleobases, other N-heterocycles, and their precursors in a sample from asteroid Bennu. [PDF]

open access: yesCommun Chem
Oba Y   +12 more
europepmc   +1 more source

Stability of the fcc phase in shocked nickel up to 332 GPa. [PDF]

open access: yesNat Commun
Pereira KA   +19 more
europepmc   +1 more source

Present-day thermal and water activity environment of the Mars Sample Return collection. [PDF]

open access: yesSci Rep
Zorzano MP   +26 more
europepmc   +1 more source

Cosmochemistry

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

An introduction to cosmochemistry

Geochimica et Cosmochimica Acta, 1995
This 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 ...
  +6 more sources

Extrasolar Cosmochemistry

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

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