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P1-The Sun

Holly Hutchings Inglés 1 página

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Nearly all of the mass in our Solar System is in the Sun. The Sun is very large. Its diameter is 109 times the Earth's. The Sun is the source of nearly all the energy we receive. For many years, it was a mystery as to where this came from and this baffled the leading scientists. It is now understood that the nuclear fusion is the energy source. In nuclear fusion, smaller nuclei come together and form larger nuclei. For example hydrogen nuclei are joined together to make helium nuclei. This releases enormous amounts of energy.

hydrogen nucleus + hydrogen nucleus → helium nuclei

In stars larger than our Sun helium nuclei can be fused together to create larger atomic nuclei. As the Earth contains many of these larger atoms, like carbon, oxygen, iron, etc, scientists believe that our Solar System was made from the remains of an earlier star.

Gravity pulls the dust and gas together.

How stars and planets are formed As the gas falls together, it gets hot. A star forms when it is hot enough for a nuclear fusion reaction to start. This releases energy, and keeps the star hot. The outward pressure from the expanding hot gases is balanced by the force of the star's gravity. This happened about 5 billion years ago. This is quite recent in the history of the Universe, which is currently believed to be 14 billion years old.

The Sun is halfway through its 10 billion year stable phase

Gravity pulls smaller amounts of dust and gas together, which form planets in orbit around the star.

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Apunte sobre P1-The Sun, creado por Holly Hutchings el 06/05/2014.
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Holly Hutchings
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