15. These appearances led Tycho to frame an hypothesis like that which
Sir William Herschel afterwards proposed, that the stars are formed by
the condensation of luminous nebulous matter. Nor is it easy to think of
such phenomena (of which several others have been observed, though none
so conspicuous as these), without regarding them as showing that the
matter of the fixed stars, occasionally at least, passes through changes
of consistence as great as would be the condensation and extinction of a
luminous vapor. And if such changes have been but few within the
recorded period of man's observation of the stars, we must recollect how
small that period is, compared with the period during which the stars
have existed. The stars themselves give us testimony of their having
been in being for millions of years. For according to the best estimates
we can form of their distances, the time which light would employ in
reaching us from the most remote of them, would be millions of years;
and, therefore, we now see those remote stars by means of the light
emitted from them millions of years ago. And if, in the 2,000 years
during which such observations are recorded, only 200 stars have
undergone such changes in a degree visible to the earth's inhabitants;
in a million of years, change going on at the same rate, 100,000 stars
would exhibit visible progressive change, showing that they had not yet
reached a permanent condition. And how much of change may go on in any
star without its being in any degree perceptible to the most exact
astronomical scrutiny!
16. The tendency of these considerations is, to lead us to think that
the fixed stars are not generally in that permanent condition in which
our sun is; and which appears to be alone consistent with the existence
of a system such as the solar system.[14] These views, therefore, fall
in with that which we have been led to by this consideration of the
Nebulæ: that the Solar System is in a more complete and advanced state,
as a system, than many at least of the stellar systems can be; it may
be, than any other.
Public-domain text, read in full here on John Shaqi.
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