Abstract
The finding of /sup 36/A excess on Venus by the mass-spectroscopic measurement of the Venus Pioneer appears to endorse the more rapid accretion theory of Venus than the Earth and the secondary origin of the terrestrial atmosphere.
Shimizu, M
[1]
- Tokyo Univ. (Japan). Inst. of Space and Aeronautical Science
Citation Formats
Shimizu, M.
Implications of /sup 36/A excess on Venus.
Netherlands: N. p.,
1979.
Web.
doi:10.1007/BF00907582.
Shimizu, M.
Implications of /sup 36/A excess on Venus.
Netherlands.
https://doi.org/10.1007/BF00907582
Shimizu, M.
1979.
"Implications of /sup 36/A excess on Venus."
Netherlands.
https://doi.org/10.1007/BF00907582.
@misc{etde_5755537,
title = {Implications of /sup 36/A excess on Venus}
author = {Shimizu, M}
abstractNote = {The finding of /sup 36/A excess on Venus by the mass-spectroscopic measurement of the Venus Pioneer appears to endorse the more rapid accretion theory of Venus than the Earth and the secondary origin of the terrestrial atmosphere.}
doi = {10.1007/BF00907582}
journal = []
volume = {20:3}
journal type = {AC}
place = {Netherlands}
year = {1979}
month = {May}
}
title = {Implications of /sup 36/A excess on Venus}
author = {Shimizu, M}
abstractNote = {The finding of /sup 36/A excess on Venus by the mass-spectroscopic measurement of the Venus Pioneer appears to endorse the more rapid accretion theory of Venus than the Earth and the secondary origin of the terrestrial atmosphere.}
doi = {10.1007/BF00907582}
journal = []
volume = {20:3}
journal type = {AC}
place = {Netherlands}
year = {1979}
month = {May}
}