The Sun is an ordinary star and is the brightest object
in our sky. As such you should certainly
never look at the Sun directly and certainly never through binoculars or a
telescope.
It’s one of more than one hundred billion stars that
populate our Milky Way galaxy. It’s a
gigantic ball of hydrogen 870,000 miles wide.
The Sun has a diameter 109 times that of the Earth and is one third of a
million times its mass.
The Sun collapsed from a cloud of hydrogen gas approximately
4.5 billion years ago. The pressure and
temperature of the hydrogen in its centre became so great that nuclear fusion chain
reactions started where 600,000,000 tons of hydrogen are converted into helium
each second. In the process, under
Einstein’s famous equation E equals M C squared, a small amount of mass is lost
as energy including light.
This energy is what we and all living things depend on
for our existence. The visible light we
see from the Sun takes eight minutes to travel the 93 million miles before it
reaches our eyes and is only a small part of the energy released from our
star. Its nuclear reactions also produce
vast quantities of ultra violet light along with deadly x-rays and gamma ray
radiation. Indeed if it wasn’t for the
Earth’s protective magnetic field this radiation would strip off our life-giving
atmosphere and all life on Earth would be burnt to a crisp.
Temperatures at the core of our star Sun reach a
staggering 10 million degrees Celsius, but it’s surface is less hot at about
5,000 degrees Celsius.
FEEL THE PB&J (PASSION, BEAUTY, AND JOY) OF THE COSMOS? SHARE IT!
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