Summary

Portrait of Simon Newcomb Simon Newcomb 1911 Encyclopædia Britannica, Volume 21… (1911)

When a superior planet is in opposition to the sun it rises at sunset and is visible all night. This is also the time when nearest the earth, and therefore when the circumstances are most favourable for observation.
The greater the distance of a planet from the sun the less is the speed with which it moves in its orbit. The orbit being larger, the time of its revolution is greater in a yet larger degree. An approximation to the general laws of speed in different planets is that the linear speed is inversely proportional to the square root of the mean distance.
Source: Wikisource

Portrait of Simon Newcomb Simon Newcomb 1911 Encyclopædia Britannica, Volume 21… (1911)

On this theory every molecule of a gaseous spheres mass is completely disconnected from every other and is in rapid motion, its velocity, which may amount to one or more thousand feet per second, depending on the temperature and on the atomic weight of the gas. At any temperature the velocities of individual molecules may now and then increase without any well-defined limit. If at the boundary of an atmosphere the velocity should exceed a certain limit fixed bythemass and force of gravity of the planet, molecules might fly away through space as independent bodies.
Source: Wikisource

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