The book progresses methodically, beginning with fundamental principles like stellar properties and planetary formation, then delving into specific detection techniques. It covers transit photometry, highlighting missions like Kepler and TESS, radial velocity measurements and direct imaging, including spectroscopic analysis of exoplanet atmospheres. A unique aspect of the book is its integration of theory with practical data analysis, making it valuable for students and researchers alike.
The book emphasizes that a complete understanding of exoplanet detection methods is essential to advance the study of planetary formation, habitability, and the possibility of life beyond Earth.