The Heavens Above: A Popular Handbook of AstronomyRolfe, W. J. (William James)
Science
The Heavens Above: A Popular Handbook of Astronomy
Rolfe, W. J. (William James)
Astronomy
The volume of the sun is 1,305,000 times that of the earth.
139. _The Mass of the Sun._--The sun is much less dense than the earth.
The mass of the sun is only 330,000 times that of the earth, and its
density only about a fourth that of the earth.
To find the mass of the sun, we first ascertain the distance the
earth would draw the moon towards itself in a given time, were the
moon at the distance of the sun, and then form the proportion: as
the distance the earth would draw the moon towards itself is to the
distance that the sun draws the earth towards itself in the same
time, so is the mass of the earth to the mass of the sun.
Although the mass of the sun is over three hundred thousand times that
of the earth, the pull of gravity at the surface of the sun is only
about twenty-eight times as great as at the surface of the earth. This
is because the distance from the surface of the sun to its centre is
much greater than from the surface to the centre of the earth.
[Illustration: Fig. 155.]
140. _Size of the Sun Compared with that of the Planets._--The size of
the sun compared with that of the larger planets is shown in Fig. 155.
The mass of the sun is more than seven hundred and fifty times that of
all of the planets and moons in the solar system. In Fig. 156 is shown
the apparent size of the sun as seen from the different planets. The
apparent diameter of the sun decreases as the distance from it
increases, and the disk of the sun decreases as the square of the
distance from it increases.
[Illustration: Fig. 156.]
141. _The Distance of the Sun._--The mean distance of the sun from the
earth is about 92,800,000 miles. Owing to the eccentricity of the
earth's orbit, the distance of the sun varies somewhat; being about
3,000,000 miles less in January, when the earth is at perihelion, than
in June, when the earth is at aphelion.
"But, though the distance of the sun can easily be stated in
figures, it is not possible to give any real idea of a space so
enormous: it is quite beyond our power of conception. If one were to
try to walk such a distance, supposing that he could walk four miles
an hour, and keep it up for ten hours every day, it would take
sixty-eight years and a half to make a single million of miles, and
more than sixty-three hundred years to traverse the whole.
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