Beschreibung
The orbit of the Moon is tilted to the plane of the orbit of the Earth. Eclipses can occur only at certain points where the Moon’s orbit crosses that of the Earth, called the nodes. The shadows of the Earth and Moon play a a large role in determining where in the world a given eclipse can be seen. Also, the location of the Moon compared to the Earth's orbit determines why eclipses do not occur every month.
Straightforward explanations are offered to explain the common maps and diagrams used for describing solar and lunar eclipses. Illustrated definitions are given for all the terminology typically shown on these maps and diagrams. The circumstances of solar and lunar eclipses are explained that affect the duration and appearance of eclipses, along with useful information for choosing a suitable viewing location.
In this way, the reader can obtain a sophisticated understanding of eclipses and the factors that produce them. Continue your study of the amazing eclipse phenomenon by reading ECLIPSES Book 2!