Computer Science
Scientific paper
Mar 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983natur.302..215g&link_type=abstract
Nature, vol. 302, Mar. 17, 1983, p. 215-218.
Computer Science
36
Abundance, Big Bang Cosmology, Deuterium, Helium, Jupiter Atmosphere, Saturn Atmosphere, Cosmochemistry, Helium Hydrogen Atmospheres, Planetary Composition, Planetary Evolution, Planets, Jupiter, Saturn, Helium, Deuterium, Abundance, Cosmology, Models, Nucleosynthesis, Data, Calculations, Comparisons, Voyager, Solar System, Iris, Infrared Radiometer Spectrometer, Pioneer 11, Theoretical Studies, Analysis, Origin, Formation
Scientific paper
The determination of relative abundances of helium and deuterium in Jupiter and Saturn provides estimates of the primordial abundances of these elements. The values so inferred can be compared with theoretical predictions of the standard model of the big-bang theory as a test of the model and suggest either that deuterium is more efficiently consumed in subsequent nucleosynthesis than hitherto assumed, or that the standard big-bang model should be revised in order for there to have been less production of primordial helium.
Gautier Daniel
Owen Theodore
No associations
LandOfFree
Cosmological implications of helium and deuterium abundances on Jupiter and Saturn does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Cosmological implications of helium and deuterium abundances on Jupiter and Saturn, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmological implications of helium and deuterium abundances on Jupiter and Saturn will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1470178