Astronomical Curiosities: Facts and FallaciesGore, J. Ellard (John Ellard)
Science
Astronomical Curiosities: Facts and Fallacies
Gore, J. Ellard (John Ellard)
Astronomy -- Miscellanea; Solar system -- Miscellanea
"A few years ago, when christening celestial formations was more in
fashion than it is now, a man simply had to use a telescope for an
evening or two on Mars or the moon, and spice the relation of his
seeings with something in the way of novelty, when his name would be
pretty certainly attached to an object and hung in the heavens for all
time! A writer in the _Astronomical Register_ for January, 1879,
humorously suggested that 'the matter should be put into the hands of
an advertising agent,' and 'made the means of raising a revenue for
astronomical purposes.' Some men would not object to pay handsomely
for the distinction of having their names applied to the seas and
continents of Mars or the craters of the moon."
An occultation of Mars by the moon is recorded by Aristotle as having
occurred on April 4, 357 B.C.[113]
Seen from Mars the maximum apparent distance between the earth and moon
would vary from 3½' to nearly 17'.[114]
CHAPTER VII
The Minor Planets
Up to 1908 the number of minor planets (or asteroids) certainly known
amounted to over 650.
From an examination of the distribution of the first 512 of these small
bodies, Dr. P. Stroobant finds that a decided maximum in number occurs
between the limits of distance of 2·55 and 2·85 (earth's mean distance
from sun = 1), "199 of the asteroids considered revolving in this
annulus." He finds that nearly all the asteroidal matter is concentrated
near to the middle of the ring in the neighbourhood of the mean distance
of 2·7, and the smallest asteroids are relatively less numerous in the
richest zones.[115]
There are some "striking similarities" in the orbits of some of the
asteroids. Thus, in the small planets Sophia (No. 251 in order of
discovery) and Magdalena (No. 318) we have the mean distance of Sophia
3·10, and that of Magdalena 3·19 (earth's mean distance = 1). The
eccentricities of the orbits are 0·09 and 0·07; and the inclinations of
the orbits to the plane of the ecliptic 10° 29' and 10° 33'
respectively.[116] This similarity may be--and probably is--merely
accidental, but it is none the less curious and interesting.
Some very interesting discoveries have recently been made among the minor
planets. The orbit of Eros intersects the orbit of Mars; and the following
have nearly the same mean distance from the sun as Jupiter:--
Achilles (1906 TG), No. 588,
Patrocles (1906 XY), No. 617,
Hector (1907 XM), No. 624,
and another (No. 659) has been recently found. Each of these small planets
"moves approximately in a vertex of an equilateral triangle that it forms
with Jupiter and the sun."[117] The minor planet known provisionally as HN
is remarkable for the large eccentricity of its orbit (0·38), and its
small perihelion distance (1·6). When discovered it had a very high South
Declination (61½°), showing that the inclination of the plane of its
orbit to the plane of the ecliptic is considerable.[118]
Public-domain text, read in full here on John Shaqi.
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