Other major molecules observed in Saturns atmosphere are methane and ammonia, which are two to sevener times more abundant relative to hydrogen than in the Sun. Hydrogen sulfide and water are also suspect to be drive home in the deeper atmosphere but have not yet been detected. Minor molecules that have been detected spectroscopically from existence include phosphine, carbon monoxide, and germane. Such molecules would not be present in detectable amounts in a hydrogen-rich atmosphere in chemical equilibrium.
They may be products of reactions at high closet and temperature in Saturns deep atmosphere, well below the plain clouds, that have been transported to visible atmospheric regions by convective motions. A come in of other nonequilibrium hydrocarbons are observed in Saturns stratosphere: acetylene, ethane, and, possibly, propane and methyl group acetylene. All of the latter may be produced by photochemical effects from solar ultraviolet radiation or, at higher(prenominal) latitudes, by ener formic electrons precipitating from Saturns radiation belts.
Astronomers on Earth have analyzed the refraction (bending) of starlight and radio waves from spacecraft passing through Saturns atmosphere to gain training on atmospheric temperature over depths corresponding to pressures of...If you want to get a full essay, order it on our website: Ordercustompaper.com
If you want to get a full essay, wisit our page: write my paper
No comments:
Post a Comment