ReviewOrigins of life and evolution of the biosphere : the journal of the International Society for the Study of the Origin of Life1995
Dust in the Universe: implications for terrestrial prebiotic chemistry.
Review in Origins of life and evolution of the biosphere : the journal of the International Society for the Study of the Origin of Life, 1995. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 2 papers.
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The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.
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2 citing papers in PubMed, 13 citations in OpenAlex.
- Prebiotic synthesis of simple sugars by an interstellar formose reaction.Origins of life and evolution of the biosphere : the journal of the International Society for the Study of the Origin of Life · 2008Article
- Possible role of volcanic ash-gas clouds in the Earth's prebiotic chemistry.Origins of life and evolution of the biosphere : the journal of the International Society for the Study of the Origin of Life · 1996Review
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2 authors at 1 institution in 1 country.
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Abstract
In the present review we analyze the available literature on the distribution of dust in the Universe, methods of its observation and determination of the chemical composition, and the roles for terrestrial prebiotic chemistry. The most plausible natural sources of dust on the Earth in the prebiotic era are sedimentation of interplanetary dust, meteoritic and cometary impacts, volcanic eruptions, and soil microparticulates; the interplanetary medium being among the most powerful supplier of the dust matter. Two fundamental roles of dust particles for the origins of life are considered: (1) catalytic formation of prebiotic compounds; and (2) delivery of organic matter to the Earth by space dust particles. Due to the fact that there is only approximate information on the chemical composition and properties of interstellar, circumstellar, and major part of interplanetary dust, even the simulating experiments are difficult to perform. Until these gaps are filled, it seems reasonable to focus efforts of the scientists dealing with dust-driven catalytic formation of prebiotically important compounds on the volcanic and meteoritic/cometary impact environments.
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