The Calculation Of Solar Eclipses Without Parallaxes

Focusing on the methodology of calculating solar eclipses, this book provides a comprehensive guide that eliminates the need for parallaxes. It features a practical example from the total solar eclipse of May 11, 1724, making it a significant resource for astronomers and scientists interested in eclipse studies. Originally published in 1724, this facsimile reprint aims to preserve the historical significance of the work while ensuring accessibility to modern readers. Some imperfections may be present due to its antiquarian nature.