Flowers of the SkyProctor, Richard A. (Richard Anthony)
Science
Flowers of the Sky
Proctor, Richard A. (Richard Anthony)
Astronomy
But it may perhaps occur to some that the distance of the sun may be
changing. The earth might be drawing steadily in towards the sun, and so
all our measurements might be deceptive. Nay, the painful thought might
present itself that when the observations of 1769 were made, the sun
really was farther away than at present by more than 3,000,000 of miles.
If this were so, the earth would, in the course of a century, have
reduced her distance by fully one-thirtieth part, so that, supposing the
approach to continue, she would in 3,000 years fall into the sun, while,
long before that period had elapsed, the increased heat to which she
would be exposed would render life impossible.
Fortunately, we know quite certainly that no such approach is taking
place. It is known that the distance of the earth from the sun cannot
change without a corresponding change in her period of revolution--that
is, in the length of the year. The law connecting these two (indicated
in the note, page 279) is such that, on the reduction of the distance by
any moderate portion the period would be reduced by a portion half as
great again. For instance: if the distance of the earth from the sun
were reduced by a thirtieth part (or about 3,000,000 miles) the length
of the year would be reduced by a thirtieth and half a thirtieth--that,
is, by a twentieth part, or by more than eighteen days. We know that no
such change has taken place during the last century, or since the
beginning of history. Nay, from the Chaldean estimate of the length of
the year, which only exceeded ours by about two minutes, it is easily
shown that the distance of the earth from the sun has not diminished 200
miles within the last 2,500 years. So that, assuming even that the earth
is approaching the sun at this rate, or eight miles in a century, it
would be 1,250,000 years before the distance would be diminished by
100,000 miles, which is the probable limit of error in the determination
of the sun's distance.
Public-domain text, read in full here on John Shaqi.
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