Rescued from obscurity, Feynman's Lost Lecture is a blessing for all Feynman followers. Most know Richard Feynman for the hilarious anecdotes and exploits in his best-selling books Surely You're Joking, Mr. Feynman! and What DoYou Care What Other People Think? But not always obvious in those stories was his brilliance as a pure scientist-one of the century's greatest physicists. With this book and CD, we hear the voice of the great Feynman in all his ingenuity, insight, and acumen for argument. This breathtaking lecture-"The Motion of the Planets Around the Sun"-uses nothing more advanced than high-school geometry to explain why the planets orbit the sun elliptically rather than in perfect circles, and conclusively demonstrates the astonishing fact that has mystified and intrigued thinkers since Newton: Nature obeys mathematics. David and Judith Goodstein give us a beautifully written short memoir of life with Feynman, provide meticulous commentary on the lecture itself, and relate the exciting story of their effort to chase down one of Feynman's most original and scintillating lectures.
Richard Feynman, the rock star of theoretical physics, has left an image that belies the nerdy side revealed in
Feynman's Lost Lecture: The Motion of Planets Around the Sun. Not many bongo-playing surfer beatniks would have spent hours of their spare time proving Newton's law of elliptical planetary motion using only plane geometry, but
Feynman's Lost Lecture shows that the great man did just that. Originally delivered to an introductory physics class at Caltech in 1963, this book contains everything the maths-savvy listener needs to savour the pleasures of applied maths. Caltech physicist David L Goodstein and archivist Judith R Goodstein found the notes and tape amid another professor's papers and set to work making sense of them; unfortunately photographs of the blackboard drawings didn't survive. The book briefly covers their find and recovery work, then presents the proof as reconstructed--crucial reading if one is to follow the lecture. There's nothing easy about it, as Feynman acknowledges in the lecture:
I am going to give what I will call and elementary demonstration. "Elementary" means that very little is required to know ahead of time in order to understand it, except to have an infinite amount of intelligence.
He means, instead, that he is strictly using geometrical methods to reach his destination, which explains why it was so difficult to reconstruct without his diagrams. His charming Brooklyn accent and good humour show through in this lecture, even if the material is quite a bit drier than his fans might expect. Still, those interested in adding a new dimension to their understanding of this unquestionably brilliant scientist--and those with a deep interest in Newtonian physics--will find
The Motion of Planets Around the Sun a rare and unexpected treat. --
Rob Lightner
