Essays, or discourses, vol. 4 (of 4) : $b Selected from the works of Feyjoo, and translated from the Spanish — John Shaqi
Essays, or discourses, vol. 4 (of 4) : $b Selected from the works of Feyjoo, and translated from the SpanishFeijoo, Benito Jerónimo
Philosophy
Essays, or discourses, vol. 4 (of 4) : $b Selected from the works of Feyjoo, and translated from the Spanish
Feijoo, Benito Jerónimo
Spanish essays -- Translations into English
XX. The common causes of our experiencing more or less heat, or more
or less light from the sun, are the serene or loaded state of the
atmosphere; the oblique direction with which the sun’s rays are reflected
on us; the position, or situation of places; the length or shortness of
the days; the tranquillity or agitation of the winds, and our vicinity
to cold or warm places, such as snowy mountains, or warm subterraneous
effluvia. But, abstracted from any of these sublunary or inferior causes,
I say, that in the sun itself, is contained a cause, that occasions it
to reflect more or less light or heat, and that it actually does reflect
more or less light and heat, at some times than it does at others, and
that this is in virtue of its own proper nature and disposition.
XXI. The reason of which phenomenon is, the transitory spots, which the
astronomers have for some time past observed in the sun. These are a sort
of darkish places, unequal in size and duration, which seem as if they
were on the superficies of the star, and which at different times are
more or less numerous, although it has happened, that for years together
none of them have appeared. Some believe that the antient Chaldeans had
some knowledge of them, for in the Book of Job, we read the following
expression of Job’s friend Eliphaz to him, that the Heavens themselves
are not exempt from their spots: _Cæli non sunt mundi in conspectu
ejus._ On the other hand, the want of telescopes among the ancients, did
not render their making observations on these things impossible; for some
of these spots are so large, as to be visible without a telescope; as
for example that was, which was seen in the year 1706, whose superficies
according to the computation of the astronomers, was thirty-six times
larger than the whole earth; and when they arrive at this magnitude, or
if they are even much less, they may be discerned, by looking at the sun
with a glass tinged with any dark colour.
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