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Home > Astronomy > Solar System > The Sun



The Sun


Credit: image by NASA, source: http://www.nasa.gov


In many mythologies the Sun is called God and is believed to have special powers. Greeks named it Helios and Romans, Sol. The Sun is 4,6 billion years-old and is the biggest star in our solar system. Its mass is of 1.9891 x 1030 kg (99,8% of the solar systemís mass), which equals to 332 946 Earths. The Sun is composed of 70% of hydrogen and 28% of helium by mass.


This heavenly body has a specific structure. In the center, there is the core where nuclear reactions occur. The energy liberated goes through the radiation zone, taking the shape of photons. It takes those photons about 170 000 Earthís years to reach the convection zone, where some cold and hot plasma current mix. After passing through this section, the photons enter the photosphere, where they are transformed into heat, light, and some other forms of radiation. Then they penetrates the chromosphere, a layer above the photosphere. The last part of the Sun is the corona. It is out of our sight most of the time. It can only be seen when a lot of light is emitted, concealing the photosphere.


Credit: Sakurambo, source: http://www.wikipedia.org
Published under the terms of the GNU Free Documentation License, Version 1.2


Not only does the Sun emit light and heat, but it also gives off some charged particles (electrons and protons). This stream of particles is called the solar wind, whose speed of propagation is 450 km/sec. From time to time, a strange phenomenon called auroras can be observed, especially by people who live near to the Earthís poles. Auroras are engendered when particles of the solar wind collide with the Earthís atmosphere. Then, some blue, green, and sometimes yellow lights appear on the sky, best visible during night.



Credit: image by NASA, source: http://www.nasa.gov


We can also observe sunspots on the surface of the Sun. They are situated where there is a lot of magnetic activity and in colder areas (3800 K), where convection is inhibited. Those spots are very dark, but their periphery is a bit lighter.



Credit: image by NASA, source: http://www.nasa.gov


Another phenomenon observable from the Earth is a solar eclipse. Since the Moon and the Sun have the same apparent size in the sky as viewed from the Earth sometimes the Moon passes between the Earth and the Sun casting shade on part of the Earth.



Credit: Luc Viatour, source: http://www.wikipedia.org
Published under the terms of the GNU Free Documentation License, Version 1.2


Spectacular loops and prominences are often visible on the Sun's limb.


Credit: image by NASA, source: http://www.nasa.gov




Credit: image by NASA, source: http://www.nasa.gov


The Sun is being studied by spacecrafts recently launched, for example Ulysses, Wind, ACE, SOHO, and many others. Scientists obtain a lot of new information and photos of the Sun, which help them increase their knowledge of this great star, the center of our solar system.




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