A Popular History of Astronomy During the Nineteenth Century: Fourth EditionClerke, Agnes M. (Agnes Mary)
History
A Popular History of Astronomy During the Nineteenth Century: Fourth Edition
Clerke, Agnes M. (Agnes Mary)
Astronomy -- History -- 19th century
M. Faye, of the Paris Academy of Sciences, was the first to propose a
coherent scheme of the solar constitution covering the whole range of
new discovery. The fundamental ideas on the subject now in vogue here
made their first connected appearance. Much, indeed, remained to be
modified and corrected; but the transition was finally made from the old
to the new order of thought. The essence of the change may be conveyed
in a single sentence. The sun was thenceforth regarded, not as a mere
heated body, or--still more remotely from the truth--as a cool body
unaccountably spun round with a cocoon of fire, but as a vast
_heat-radiating machine_. The terrestrial analogy was abandoned in one
more particular besides that of temperature. The solar system of
circulation, instead of being adapted, like that of the earth, to the
distribution of heat received from without, was seen to be directed
towards the transportation towards the surface of the heat contained
within. Polar and equatorial currents, tending to a purely superficial
equalisation of temperature, were replaced by vertical currents bringing
up successive portions of the intensely heated interior mass, to
contribute their share in turn to the radiation into space which might
be called the proper function of a sun.
Faye's views, which were communicated to the Academy of Sciences,
January 16, 1865,[433] were avowedly based on the anomalous mode of
solar rotation discovered by Carrington. This may be regarded either as
an acceleration increasing from the poles to the equator, or as a
retardation increasing from the equator to the poles, according to the
rate of revolution we choose to assume for the unseen nucleus. Faye
preferred to consider it a retardation produced by ascending currents
continually left behind as the sphere widened in which the matter
composing them was forced to travel. He further supposed that the depth
from which these vertical currents rose, and consequently the amount of
retardation effected by their ascent to the surface, became
progressively greater as the poles were approached, owing to the
considerable flattening of the spheroidal surface from which they
started;[434] but the adoption of this expedient has been shown to
involve inadmissible consequences.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account