The description and use of the globes and the orrery: To which is prefix'd, by way of introduction, a brief account of the solar system — John Shaqi
The description and use of the globes and the orrery: To which is prefix'd, by way of introduction, a brief account of the solar systemHarris, Joseph
History
The description and use of the globes and the orrery: To which is prefix'd, by way of introduction, a brief account of the solar system
Harris, Joseph
Astronomical models; Globes
The figures of the Comets are observed to be very different; some of
them send forth small beams, like hair, every way round them; others
are seen with a long fiery tail, which is always opposite to the Sun.
Their magnitudes are also very different, but in what proportion they
exceed each other, it is as yet uncertain. Nor is it probable, that
their numbers are yet known, for they have not been observed with due
care, nor their theories discovered, but of late years. The ancients
were divided in their opinions concerning them; some imagined that they
were only a kind of _Meteors_ kindled in our atmosphere, and were there
again dissipated; others took them to be some ominous prodigies: But
modern discoveries prove, that they are Worlds subject to the same laws
of motion as the Planets are; and they must be very hard and durable
bodies, else they could not bear the vast heat that some of them, when
they are in their _Perihelia_, receive from the Sun, without being
utterly consumed. The great Comet which appeared in the year 1680, was
within ¹/₆ part of the Sun’s diameter from his surface; and therefore
its heat must be prodigiously intense beyond imagination. And when it
is at its greatest distance from the Sun, the cold must be as rigid.
[Illustration]
SECT. II.
_Of the_ FIXED STARS.
[Sidenote: The fixed Stars are at immense distance from us.]
The fixed Stars are those bright and shining bodies, which in a clear
night appear to us every where dispersed through the boundless regions
of space. They are term’d fix’d, because they are found to keep the
same immutable distance one from another in all ages, without having
any of the motions observed in the Planets. The fixed Stars are all
placed at such immense distances from us, that the best of telescopes
represent them no bigger than points, without having any apparent
diameters.
[Sidenote: The fixed Stars are luminous bodies like the Sun.]
It is evident from hence, that all the Stars are luminous bodies, and
shine with their own proper and native light, else they could not be
seen at such a great distance. For the _Satellites_ of _Jupiter_ and
_Saturn_, tho’ they appear under considerable angles through good
telescopes, yet are altogether invisible to the naked eye.
[Sidenote: The distance from us to the Sun is nothing in comparison of
the vast distance of the fixed Stars.]
Although the distance betwixt us and the Sun is vastly large, when
compared to the diameter of the Earth, yet it is nothing when compared
with the prodigious distance of the fixed Stars; for the whole diameter
of the Earth’s annual orbit, appears from the nearest fixed Star no
bigger than a point, and the fixed Stars are at least 100,000 times
farther from us than we are from the Sun; as may be demonstrated from
the observation of those who have endeavoured to find the Parallax of
the Earth’s annual Orb, or the angle under which the Earth’s orbit
appears from the fixed Stars.
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