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Clear, practical guidance for anyone who needs to understand how astronomy, navigation, and civil time fit together. This book explains the systems behind clock time and sky-based measurement with careful attention to the links between sidereal time, solar time, leap seconds, and calendar rules. It is written for readers who want more than definitions, they want to know how time is actually used, converted, and checked in real observing and technical work.
Starting from the basics of time as an instant, interval, and epoch, the book builds a solid foundation in coordinate systems, time scales, and angular measurement. It then moves through the major topics that often cause confusion, including Greenwich and local sidereal time, the equation of time, UT1 and Earth rotation irregularities, atomic time scales such as TAI and TT, and the role of leap seconds in keeping human time aligned with Earth's changing rotation.
Inside you will find:
The book is especially useful for astronomers, observers, software developers, educators, and students who need dependable methods for scheduling, logging, or interpreting time-sensitive data. Each chapter supports real-world use, from pointing telescopes and planning observation sessions to verifying timestamp conversions and building reliable workflows.
What makes it especially valuable is its emphasis on both concept and computation. You get the physical meaning behind each time scale, along with worked examples and reference recipes that help turn theory into practice. Whether you are correcting for longitude, comparing civil time with solar time, or preparing ephemeris-ready inputs, this guide offers a structured path through the most important timekeeping systems used in astronomy.
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