Titlebook: Comets and the Origin of Life; Proceedings of the F Cyril Ponnamperuma Conference proceedings 1981 D. Reidel Publishing Company, Dordrecht,

amateur

書目名稱Comets and the Origin of Life影響因子(影響力)




書目名稱Comets and the Origin of Life影響因子(影響力)學(xué)科排名




書目名稱Comets and the Origin of Life網(wǎng)絡(luò)公開度




書目名稱Comets and the Origin of Life網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Comets and the Origin of Life被引頻次




書目名稱Comets and the Origin of Life被引頻次學(xué)科排名




書目名稱Comets and the Origin of Life年度引用




書目名稱Comets and the Origin of Life年度引用學(xué)科排名




書目名稱Comets and the Origin of Life讀者反饋




書目名稱Comets and the Origin of Life讀者反饋學(xué)科排名

ornithology

Comet Nucleus: Some Characteristics and a Hypothesis on Origin and Structure,mets. These points will be followed by presentation of the problem of cosmic ray irradiation of comets in the long time they survive in the Oort Cloud. A more detailed discussion of this phenomenon, including an experimental investigation of ice irradiation by 1 MV proton, will be given by Marla Moo

Landlocked

Ultraviolet Spectroscopy of Comets,l as several simple molecules made from these species have their strong resonance transitions in the ultraviolet region of the spectrum. However, due to the opacity of the atmosphere to ultraviolet, these observations must be made from space, and it was not until 1970 that the extensive HI Lyman α e

dictator

entitle

Interplanetary Dust - Its Physical Nature and Entry into the Atmosphere of Terrestrial Planets,k, fine grained material similar to carbonaceous chondrites but different from known meteorites in mineralogy and structure. If the analyzed samples are typical interplanetary particles then they are probably cometary materials similar to the vast numbers of cometary particles which have continuousl

悄悄移動(dòng)

悄悄移動(dòng)

Chemical Kinetics IM the Coma,are described and correlated to distance in the coma above the nucleus and to heliocentric distance of the comet. Two classes for the composition of comets are considered based on their place of origin: in the environs of the giant planets or in a companion fragment of the presolar nebula. Compariso

RENIN

Oration

,Chemical Evolution of Interstellar Dust — A Source of Prebiotic Material ?, cloud collapse (early pre-solar nebula) of complex non-volatile molecular mixtures of oxygen, carbon and nitrogen with hydrogen in addition to such volatile combinations as H.O, CO, etc. These constituents may be presumed to be the predominant constituents of a comet which accreted out of the inter

defile