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The differences are not due to the vertical extent of the clouds but due to different origins and chemical composition of the clouds on Earth and Venus.
To figure out the chemical composition of the clouds, they studied the spectrum of light from a background quasar that had traveled through the gas on its way to the telescope.
More information on the molecular composition of the clouds would help make a stronger case, says Carlberg: A predominance of pristine hydrogen and helium gas would buttress the new theory by suggesting that the cloud was formed in the big bang, while the presence of heavier elements would indicate that the material was derived from stars.
The images allowed the researchers to analyze the structure, height, thickness and composition of the clouds.
The composition of the clouds varies with depth and increasing pressure.
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Composition of the cloud particles, however, is not very well known, including their nature other than containing varying concentrations of sulfuric acid particulate, microorganisms and shape.
This coagulation-inhibited case is not meant to represent an expected behavior in the clouds, but rather to represent an extreme end member for quantifying the effects of the efficiency of coalescence on the distribution and composition of the Venus clouds.
We focus on these three types of atmosphere-surface interactions because they appear to play major roles in determining the composition of the atmosphere, clouds, and the surface, e.g. by serving as a sink for SO2, by controlling the extent and rate of basalt oxidation, or by acting as a sink/source for atmospheric water.
Older, population II stars have substantially less metallicity than the younger, population I stars due to the composition of the molecular clouds from which they formed.
In addition to upsetting long-held assumptions about how asteroids and comets behave, the finding could challenge what we thought we knew about the composition of the Oort cloud, which astronomers previously believed was made up almost exclusively of icy bodies.
In the low metallicity environments of the LMC and the SMC the mass balance between SiC and C in carbon stars will differ from those found in Galactic carbon stars (e.g. Sloan et al., 2006b), as the required carbon is produced by the star itself, but the silicon abundance reflects the composition of the natal cloud.
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