Planetary, Lunar, and Solar Positions


Book Description




Planetary, Lunar, and Solar Positions, 601 B.C. to A.D. 1, at Five-day and Ten-day Intervals


Book Description

The need for these tables became pressing when hundreds of astronomical cuneiform tables in the British Museum became available for study, partly through the copies made in the 1880s and 1890s. All these texts originally came from some archive in Babylon which was discovered by Arabs in the middle of the 19th century. Most of the texts were written from about 330 B.C. to the first century A.D. Many of the texts are fragments of the original clay tables which have broken. In many cases, a fragment contains only parts of a few legible lines. Much of the information is of an astronomical character. It is evident that for investigations of these tablets the possibility of rapid scanning of accurately dated planetary positions is of primary importance.







Planetary, Lunar, and Solar Positions


Book Description

These tables cover the period from the mid-17th to the 19th cent. when astronomical ephemerides were evolving most rapidly. These tables resemble those previously pub. by the APS: Tuckerman's "Planetary, Lunar, and Solar Positions, 601 B.C. to A.D. 1" and "A.D. 2 to A.D. 1649" and Goldstine's "New and Full Moon, 1001 B.C. to A.D. 1651." The tables contain features consistent with the almanacs and ephemerides pub. in this period: planetary positions are computed for 12 hours U.T. (noon); and the Julian day number is given for new and full moons. An analytical essay examines the theoretical and computational developments in almanac-making in the period that bridges between Kepler and Laplace.










Python Programs for Astronomical Solutions


Book Description

This book gives ready-made scripts of Python coding for the solution to all practical problems in Astronomy such as finding Planetary positions at any instant of time on any date, Detailed calculation of lunar and solar eclipses, past or future, with a production of visual simulations like videos, pictures and maps. It gives insight into the technics of Python-programming and in-depth knowledge of Astronomical calculations. It is a must for every astronomical enthusiast and students of computer programming.







Next Time You See the Moon


Book Description

This fascinating book will stay with children every time they gaze up at the night sky. Through vivid pictures and engaging explanations, children will learn about many of the Moon’s mysteries: what makes it look like a silvery crescent one time and a chalk-white ball a few nights later, why it sometimes appears in the daytime, where it gets its light, and how scientists can predict its shape on your birthday a thousand years from now. Next Time You See the Moon is an ideal way to explain the science behind the shape of the Moon and bring about an evening outing no child—or grown-up—will soon forget. Awaken a sense of wonder in a child with the Next Time You See series from NSTA Kids. The books will inspire elementary-age children to experience the enchantment of everyday phenomena such as sunsets, seashells, fireflies, pill bugs, and more. Free supplementary activities are available on the NSTA website. Especially designed to be experienced with an adult—be it a parent, teacher, or friend—Next Time You See books serve as a reminder that you don’t have to look far to find something remarkable in nature.




The Babylonian Theory of the Planets


Book Description

In the second millennium b.c., Babylonian scribes assembled a vast collection of astrological omens, believed to be signs from the gods concerning the kingdom's political, military, and agricultural fortunes. The importance of these omens was such that from the eighth or seventh until the first century, the scribes observed the heavens nightly and recorded the dates and locations of ominous phenomena of the moon and planets in relation to stars and constellations. The observations were arranged in monthly reports along with notable events and prices of agricultural commodities, the object being to find correlations between phenomena in the heavens and conditions on earth. These collections of omens and observations form the first empirical science of antiquity and were the basis of the first mathematical science, astronomy. For it was discovered that planetary phenomena, although irregular and sometimes concealed by bad weather, recur in limited periods within cycles in which they are repeated on nearly the same dates and in nearly the same locations. N. M. Swerdlow's book is a study of the collection and observation of ominous celestial phenomena and of how intervals of time, locations by zodiacal sign, and cycles in which the phenomena recur were used to reduce them to purely arithmetical computation, thereby surmounting the greatest obstacle to observation, bad weather. The work marks a striking advance in our understanding of both the origin of scientific astronomy and the astrological divination through which the kingdoms of ancient Mesopotamia were governed. Originally published in 1998. The Princeton Legacy Library uses the latest print-on-demand technology to again make available previously out-of-print books from the distinguished backlist of Princeton University Press. These editions preserve the original texts of these important books while presenting them in durable paperback and hardcover editions. The goal of the Princeton Legacy Library is to vastly increase access to the rich scholarly heritage found in the thousands of books published by Princeton University Press since its founding in 1905.