Simon Newcomb

Simon Newcomb

Summary

Portrait of Simon Newcomb Simon Newcomb 1911 Encyclopædia Britannica (1911)

PLANETS, MINOR. The minor planets, commonly known as asteroids or planetoids, form a remarkable group of small planetary bodies, of which all the known members but three move between the orbits of Mars and Jupiter. Until recently they were all supposed to be contained within the region just I mentioned; but the discovery of one, which at perihelion comes far within the orbit of Mars, and of two others, which at aphelion pass outside the orbit of Jupiter, shows that no well-defined limit can be set to the zone containing them.
Source: Wikisource

Portrait of Simon Newcomb Simon Newcomb 1911 Encyclopædia Britannica (1911)

NEPTUNE, in astronomy, the outermost known planet of our solar system; its symbol is ♆. Its distance from the sun is a little more than 30 astronomical units, i.e. 30 times the mean distance of the earth from the sun, or about 2,796,000,000 m. It deviates greatly from Bode's law, which would give a distance of nearly 39. Its orbit is more nearly circular than that of any other major planet, Venus excepted. Its time of revolution is 165 years. Being of the 8th stellar magnitude it is invisible to the naked eye.
Source: Wikisource

Portrait of Simon Newcomb Simon Newcomb 1911 Encyclopædia Britannica (1911)

A few of the minor planets are of such special interest that some pains will doubtless be taken to determine their orbits and continue observations upon them at every available opposition. To this class belong those of which the orbits are so eccentric that they either pass near that of Jupiter or approach near that of the earth. With most of the others little more can be done than to compute their elements with a view of subsequently identifying the object when desired. Unless followed up at several oppositions after discovery, the planet is liable to be quite lost.
Source: Wikisource

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