Deuterium concentration in the early Solar System: hydrogen and oxygen isotope study

Nature ◽  
1979 ◽  
Vol 282 (5741) ◽  
pp. 785-789 ◽  
Author(s):  
F. Robert ◽  
L. Merlivat ◽  
M. Javoy
Keyword(s):  
Solar System ◽  
Oxygen Isotope ◽  
Early Solar System ◽  
Deuterium Concentration ◽  
Isotope Study ◽  
Hydrogen And Oxygen Isotope

Exchange Frequency of Oxygen Isotope Reservoirs in The Early Solar System

2008 ◽  
Author(s):  
S. Itoh ◽  
H. Yurimoto ◽  
Takuma Suda ◽  
Takaya Nozawa ◽  
Akira Ohnishi ◽  
...  
Keyword(s):  
Solar System ◽  
Oxygen Isotope ◽  
Early Solar System ◽  
Exchange Frequency

Extreme oxygen isotope ratios in the early Solar System

Nature ◽  
2005 ◽  
Vol 437 (7057) ◽  
pp. 385-388 ◽  
Author(s):  
Jérôme Aléon ◽  
François Robert ◽  
Jean Duprat ◽  
Sylvie Derenne
Keyword(s):  
Solar System ◽  
Oxygen Isotope ◽  
Isotope Ratios ◽  
Early Solar System ◽  
Oxygen Isotope Ratios

Laboratory and in-situ analysis of comet dust

1988 ◽  
Vol 46 ◽  
pp. 8-9
Author(s):  
D.E. Brownlee ◽  
A.L. Albee
Keyword(s):  
Electron Microscopy ◽  
Solar System ◽  
Laboratory Study ◽  
Isotopic Analysis ◽  
Building Blocks ◽  
Sem Analysis ◽  
Early Solar System ◽  
Cometary Material ◽  
Comet Dust

Comets are primitive, kilometer-sized bodies that formed in the outer regions of the solar system. Composed of ice and dust, comets are generally believed to be relic building blocks of the outer solar system that have been preserved at cryogenic temperatures since the formation of the Sun and planets. The analysis of cometary material is particularly important because the properties of cometary material provide direct information on the processes and environments that formed and influenced solid matter both in the early solar system and in the interstellar environments that preceded it.The first direct analyses of proven comet dust were made during the Soviet and European spacecraft encounters with Comet Halley in 1986. These missions carried time-of-flight mass spectrometers that measured mass spectra of individual micron and smaller particles. The Halley measurements were semi-quantitative but they showed that comet dust is a complex fine-grained mixture of silicates and organic material. A full understanding of comet dust will require detailed morphological, mineralogical, elemental and isotopic analysis at the finest possible scale. Electron microscopy and related microbeam techniques will play key roles in the analysis. The present and future of electron microscopy of comet samples involves laboratory study of micrometeorites collected in the stratosphere, in-situ SEM analysis of particles collected at a comet and laboratory study of samples collected from a comet and returned to the Earth for detailed study.

Preface: Evolution of the early solar system: Presolar cosmochemical fingerprints and the formation of watery rocky planets

2016 ◽  
Vol 50 (1) ◽  
pp. 1-2 ◽  
Author(s):  
Tomohiro Usui ◽  
Audrey Bouvier ◽  
Justin I. Simon ◽  
Noriko Kita
Keyword(s):  
Solar System ◽  
Early Solar System ◽  
Rocky Planets

A nearby neutron-star merger explains the actinide abundances in the early Solar System

Nature ◽  
2019 ◽  
Vol 569 (7754) ◽  
pp. 85-88 ◽  
Author(s):  
Imre Bartos ◽  
Szabolcs Marka
Keyword(s):  
Neutron Star ◽  
Solar System ◽  
Early Solar System

OSIRIS-REx at Bennu: Overcoming challenges to collect a sample of the early Solar System

2021 ◽  
pp. 163-194
Author(s):  
Dante S. Lauretta ◽  
Heather L. Enos ◽  
Anjani T. Polit ◽  
Heather L. Roper ◽  
Catherine W.V. Wolner
Keyword(s):  
Solar System ◽  
Early Solar System

Stable Hydrogen and Oxygen Isotope Composition of Waters from Mine Tailings in Different Climatic Environments

2007 ◽  
Vol 41 (6) ◽  
pp. 1870-1876 ◽  
Author(s):  
Jorge E. Spangenberg ◽  
Bernhard Dold ◽  
Marie-Louise Vogt ◽  
Hans-Rudolf Pfeifer
Keyword(s):  
Oxygen Isotope ◽  
Mine Tailings ◽  
Isotope Composition ◽  
Oxygen Isotope Composition ◽  
Hydrogen And Oxygen Isotope
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