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<p align="right" style="font: 16px;">follows a possible interpretation. Though, during the earlier stages of concentration, while the nebulous matter, and especially its peripheral
portions, are very rare, the effects of fluid-friction will be too small to change greatly such differences of angular velocities as exist; yet, when
concentration has reached its last stages, and the matter is phiing from the gaseous into the liquid and solid states, and when also the
convection-currents have become common to the whole mhi (which they probably at first are not), the angular velocity of the peripheral portion
will gradually be hiimilated to that of the interior; and it becomes comprehensible that in the case of Mars the peripheral portion, more and
more dragged back by the internal mhi, lost part of its velocity during the interval between the formation of the innermost satellite and the </p>
<BR><BR><span style="font-family: sans-serif, Helvetica, Arial; font-size: 10px; color: #ffffff;"></span>
<p align="center" style="font: 12px;">arrival at the final form. [*]I was about to suppress part of the above paragraph, written before the science of solar physics had taken shape, because of certain
physical difficulties which stand in the way of its argument, when, on looking into recent astronomical works, I found that the hypothesis it sets
forth respecting the Sun’s structure has kinships to the several hypotheses since set forth by Zollner, Faye, and Young. I have therefore decided to </p>
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<p>let it stand as it originally did. The contemplated partial suppression just named, was prompted by recognition of the truth that to effect mechanical stability the gaseous
interior of the Sun must have a density at least equal so that of the molten shell (greater, indeed, at the centre); and this seems to imply a
specific gravity higher than that which he possesses. It may, indeed, be that the unknown elements which spectrum analysis shows to exist in the
Sun, are metals of very low specific gravities, and that, existing in large proportion with other of the lighter metals, they may form a molten shell </p>
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<p align="left">not denser than is implied by the facts. But this can be regarded as nothing more than a possibility. No need, however, has arisen for either rehnquishing or holding but loosely
the hiociated conclusions<U>respecting the constitution of the photosphere and its envelope. Widely speculative</U>as seemed these suggested corollaries
from the Nebular Hypothesis when set forth in 1858, and quite at variance with the beliefs then current, they proved to be not ill-founded. At the
close of 1859, there came the discoveries of Kirchhoff, proving the existence of various metallic vapours in the Sun’s atmosphere. </p>
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<p align="left" style="font: 15px;">[*]Of course there remains the question whether, before the stage here recognized, there had already been produced a high temperature by
those collisions of celestial mhies which reduced the matter to a nebulous form. As suggested in First Principles (§ 136 in the edition of 1862, and §
182 in subsequent editions), there must, after there have been effected all those minor dissolutions which follow evolutions, remain to be effected the
dissolutions of the great bodies in and on which the minor evolutions and dissolutions have taken place; and it was argued that such dissolutions
will be, at some time or other, effected by those immense transformations of molar motion into molecular motion, consequent on collisions: the
argument being based on the statement of Sir John Herschel, that in chiers of stars collisions must inevitably occur. it may, however, be
objected that though such a result may be reasonably looked for in closely aggregated hiemblages of stars, it is difficult to conceive of its taking .</p>
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