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The interior structure of jupiter (consequences of pioneer 10 data) (Document No: 19750006616)
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Smoluchowski, R. |
| Copyright Year | 1974 |
| Description | Models of the Jovian interiors are based on theoretical equations of state of hydrogen and helium supported by a few experimental points and an observed parameter such as oblateness, gravitational coefficients, heat emission, and magnetic fields. The models fall into three categories: (1) those which assume a uniform and rather low H2/He ratio throughout the planet, (2) those in which this ratio is solar and thus higher and (3) those which take into account the lack of complete miscibility of the two elements in the condensed state. Recent values of the observed parameters obtained by Pioneer 10 permit improvements of the first two models but also pose new questions. In the first category of models the new data indicate that the amount of hydrogen has to be increased, while in the solar models which have a heavy core (made of SiO2, MgO, Fe and Ni), the abundance of hydrogen has to be decreased, both changes pointing in the direction of incomplete miscibility present in the third category of models. |
| File Size | 654913 |
| Page Count | 24 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19750006616 |
| Archival Resource Key | ark:/13960/t2n639r3g |
| Language | English |
| Publisher Date | 1974-01-01 |
| Access Restriction | Open |
| Subject Keyword | Lunar And Planetary Exploration Planetary Magnetic Fields Hydrogen Atmospheric Models Jupiter Atmosphere Gravitational Fields Heat Transmission Space Exploration Pioneer 10 Space Probe Helium Jupiter Planet Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
