The Science Book

(Elle) #1

103


Schiehallion was chosen as the site
for the experiment because it was
symmetrically shaped and isolated
(and therefore less affected by the
gravitational pull of other mountains).

See also: Isaac Newton 62–69 ■ Henry Cavendish 78–79 ■ John Michell 88–89


EXPANDING HORIZONS


to select an appropriate mountain.
He chose Schiehallion in Scotland,
and Maskelyne spent nearly four
months making observations from
both sides of the mountain.


The density of rocks
The orientation of the plumb line
compared to the stars should have
been different at the two stations
even without any gravitational
effects, because of the difference
in latitude. However, even when
this was accounted for, there was
still a difference of 11.6 seconds of


arc (just over 0.003 degrees).
Maskelyne used a survey of the
shape of the mountain and a
measurement of the density of its
rocks to figure out the mass of
Schiehallion. He was assuming
that the whole Earth had the same
density as Schiehallion, but the
deviation of the plumb lines
showed a measured value of less
than half of what he was expecting.
Maskelyne realized that the density
assumption was not correct—the
density of Earth was clearly much
greater than that of its surface
rocks, probably, he reasoned, due
to the planet having a metallic
core. The actual observed angle
was used to figure out that the
overall density of Earth is about
double that of Schiehallion’s rocks.
This result disproved one
theory of the time, advocated by
English astronomer Edmond Halley,

...the mean density of the
earth is at least double of that
at the surface...the density of
the internal parts of the earth
is much greater than near
the surface.
Nevil Maskelyne

Nevil Maskelyne Born in London in 1732, Nevil
Maskelyne became interested
in astronomy at school. After
graduating from Cambridge
University and being ordained a
priest, he became a member of
the Royal Society in 1758, and
was the Astronomer Royal from
1765 until his death.
In 1761, the Royal Society sent
Maskelyne to the Atlantic island of
St. Helena to observe the transit
of Venus. Measurements taken
as the planet passed across the
Sun’s disk allowed astronomers to
calculate the distance between
Earth and the Sun. He also spent

much time trying to solve the
problem of measuring longitude
while at sea—a major issue of
the day. His method involved
carefully measuring the
distance between the Moon
and a given star, and consulting
published tables.

Key works

1764 Astronomical Observations
Made at the Island of St Helena
1775 An Account of
Observations Made on
the Mountain Schehallien
for Finding its Attraction

that said Earth was hollow. It also
allowed the mass of Earth to be
extrapolated from its volume and
average density. Maskelyne’s value
for the overall density of Earth was
280 lb/ft^3 (4,500 kg/m^3 ). Compared
with today’s accepted value of
344 lb/ft^3 (5,515 kg/m^3 ), he had
figured out the density of Earth
with an error of less than 20 percent,
and in the process had proved
Newton's law of gravitation. ■
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