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
By observing the eclipses of _Jupiter_’s satellites, it was first
discovered that light is not propogated instantaneously, though it
moves with an incredible swiftness: For if light came to us in an
instant, an observer in T will see an eclipse of one of the satellites,
at the same time that another in K would. But it has been found by
observations, that when the Earth is in K, at her nearest distance from
_Jupiter_, these eclipses happen much sooner than when she is in T.
Now having the difference of time betwixt these appearances in K and
T, we may find the length of time the light takes in passing from K to
T, which space is equal to the diameter of the Earth’s annual orb. By
these kinds of observations it has been found, that light reaches from
the Sun to us in the space of eleven minutes of time, which is at least
at the rate of 100,000 miles in a second.
_FINIS._
[Illustration]
AN INDEX OF THE ASTRONOMICAL TERMS Made Use of in this BOOK.
_Acronical_ Rising and Setting of the Stars Page 96
_Almacanthers_ 63
_Altitudes_ ib.
——— _Meridian Altitude_ 63
_Amplitude_ 62
_Amphiscians_ 91
_Annual Motion_ 7
_Antœci_ 92
_Antarctic Circle_ 53
——— _Pole_ ib.
_Antipodes_ 93
_Arctic Circle_ 52
_Arctic Pole_ 53
_Ascension_ 68
——— _Right_ ib.
——— _Oblique_ 69
_Ascensional Difference_ ib.
_Ascians_ 91
——— _Heteroscians_ ib.
_Asterisms_ 36
_Atmosphere_ 81
_Axis_ 43
——— _of the World_ 49
_Azimuth_ 61
Babylonish _Hours_ 71
_Bissextile_ 78
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