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blank Our glorious universe
blank The Sun
The Sun and solar system
Early knowledge
The structure of the Sun
The outer layers
Solar activity
Northern lights
Solar eclipses
The development of the Sun
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Modern journeys into space
SOHO supervises the Sun
The solar satellite Hinode
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blank Physics of space plasma
blank Our neighbour planet Venus
blank Exploring the planet Mars
blank In Saturn’s Orbit
blank Satellites in orbit
blank Space probes and manned spacecrafts
blank The Earth seen from satellites
blank Satellites monitor the Earth
blank Earth Observation and GIS
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Satellite images
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The development of the Sun
The development of the Sun When the Sun was created 4.6 billion years ago it had gone through a stage when it had been much cooler and larger than today.
On the other hand it shone up to 100 times more strongly than today.
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How has the Sun changed since birth?
At its birth the Sun had shrunk to a “normal” star, but it was not quite like the present Sun.
It emitted 36 % less energy than it does today.
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Climatic impact on the Earth
Because of the atmosphere and the oceans the temperature on the Earth may in fact increase faster in the future than the Sun’s increase of radiation indicates.
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The reserves of hydrogen in the nucleus are being emptied
Finally the nucleus of the Sun will run short of fuel. The pressure in the nucleus will sink and the gravitation forces will gain ascendancy. This will cause the nucleus of the Sun to shrink – it will become denser and warmer.
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Sarepta is provided by the Norwegian Centre for Space-related Education, www.narom.no
in co-operation with the Norwegian Space Centre, www.spacecentre.no.
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