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Solar scientists use both ground and space based
telescopes to observe the Sun. The two space based observatories
that you can use to get near-real time data from are the SOHO (Solar and
Heliospheric Observatory) and ACE (Advanced Composition Explorer).
On this page we explain what a simple orbit is and then go on to show you the
unusual orbits that the solar observatories are in.
The first person to work out how orbits worked was 23 year old Isaac Newton in
1666. Up until then, people thought that things in orbit,
like the Moon, were made of something completely different to ordinary matter on
Earth - like the matter you, me and apples are made of. They even had a
name for this stuff; quintessence. They reasoned that ordinary
matter fell to earth - like apples, whilst things made of
quintessence did not.
The young
Newton came up with a startling new way of looking at things like the Moon.
He said that they were made of the same stuff that made up apples and, just like
apples dropping from a tree, they were falling too.
Newton imagined a cannon firing cannon balls.

The balls flew in a curve. The more gunpowder
that was put in the cannon, the faster the ball flew, the more shallow the curve
and the further it went before it hit the ground. Newton reasoned
that if you could get the ball moving fast enough the curve would be the
same as the curve of the Earth and it would never hit the ground. It
would be in orbit. 
Have a virtual go at this experiment
with NASAs Jet Propulsion Lab by clicking this globe
It took nearly three hundred years after
Newton's idea for mankind to put artificial satellites into orbit. when Russia
launched Sputnik in October 1957.
Most satellites are launched into
circular or elliptical orbits around the Earth. The orbits of
the SOHO and ACE observatory satellites are in much more unusual orbits. 1.5 million
kilometres towards the Sun, far beyond the orbit of the Moon, there is a point where the gravity of the Earth and
the Sun cancel each other out. This is called the L1 Lagrangian point.
The observatories are in a 'halo' orbit around this point. As the
Earth orbits the Sun once a year, the observatories in their halo orbits get
dragged around with us. From
here they get a 24 hr a day look at the Sun. All previous orbiting
observatories were in Earth orbit and spent half of their time with their view
of the Sun blocked by the planet.


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