Summary

Portrait of Simon Newcomb Simon Newcomb 1911 Encyclopædia Britannica, Volume 17… (1911)

The diurnal changes of temperature, being diminished by an atmosphere, must be greater on Mars than on the earth, so that the vicissitudes of temperature are there very great, but cannot be exactly determined, because they must depend upon the conductivity and thermal capacity of the matter composing the surface of the planet. What we can say with confidence is that, during the Martian winter of between eight and twelve of our months, the regions around either pole must fall to a temperature nearer the absolute zero than any known on this planet.
Source: Wikisource

Portrait of Simon Newcomb Simon Newcomb 1911 Encyclopædia Britannica, Volume 17… (1911)

Indeed the more cautious astronomers, who have not specially devoted themselves to the particular phenomena, reserve a doubt as to how far the apparent phenomena of the finer canals are real, and what the markings which give rise to their appearance might prove to be if a better and nearer view of the planet than is now possible could be obtained. Of the reality of the better marked ones there can be no doubt, as they have been seen repeatedly by many observers, including those at the Lick Observatory, and have actually been photographed at the Lowell Observatory.
Source: Wikisource

Portrait of Simon Newcomb Simon Newcomb 1911 Encyclopædia Britannica, Volume 17… (1911)

Around the inner circle, representing the earth’s orbit, are marked the months during which the earth passes through the different parts of the orbit. It will be seen that the distance of Mars at the time of any opposition depends upon the month in which opposition occurs. The least possible distance would occur in an opposition about the end of August, a little before Mars reached the perihelion, because the eccentricity of the earth’s orbit throws our planet a little farther from the sun and nearer the orbit of Mars in July than it does in August.
Source: Wikisource

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