This is the story of humankind's quest over centuries to learn the true
nature of the most dominant object in our Solar System: the Sun.
Award-winning science writer Peter Bond describes in detail how our
ideas about the Sun have changed over the millennia, starting with the
simple observations of classical astronomy and continuing through
telescopic observations to the age of nuclear physics. He shows how we
discovered the Sun's basic characteristics - its distance, size,
temperature and composition - and then describes how, with evermore
sophisticated instruments, we have learned about the Sun's enormous
energy output, its atmosphere and the explosive eruptions that blast
clouds of magnetized gas and high-energy particles toward our world.
Most of this book focuses on the Space Age, when suborbital rockets and
satellites have probed every aspect of our nearby star. Each of these
missions is described in detail, with summaries of their objectives,
spacecraft designs, scientific payloads and results. The book also looks
forward, describing forthcoming missions that will shed new light on
remaining solar mysteries, notably the source of the energy that heats
the outer corona to millions of degrees.
Richly illustrated with mission photos, design diagrams, and infocharts,
this book is a fascinating read for anybody interested in the Sun and
our attempts to unravel its secrets.