Despite its all-important role in our lives, to the rest of the
universe our Sun is a very average star. Average in its size, brightness,
temperature, and even age (about 4.5 billion years). Like all stars,
the Sun is a huge ball of gases that creates and emits radiation,
including the light and heat responsible for our existence. The
Sun's light takes 8 minutes to travel the approximately 93 million
miles to the Earth, but other forms of energies take as little as
seconds or as long as days to make the trip.
Scientists use observatories both here on Earth and on satellites
to study the energy that comes from the Sun. We can observe directly
the Sun's three outer layers, but there are three more layers within
the Sun that we know of only through indirect
observations. By studying what happens in the visible regions
of the Sun, what energy comes from the Sun, and how that energy
moves through the Sun, scientists have been able to determine what
goes on in those hidden layers.