The Sun


An anti X-ray image of the Sun

The Sun is a type star: a huge sphere of gaseous, incadescent hydrogen.
Its source of energy is hidden into its deepest core where the temperature reaches 15 million grades.
The nucleus can be compared to an endless explosion of enormous nuclear bombs. It converts 4 million tons of hydrogen into heat and light every second. The gas around its nucleus is expelled as energy and is carried to the surface of the Sun, where it is released as heat and light into the space.

A total solar eclipse is an extraordinary event.
For a few minutes the day changes into night: the sky turns dark, planets and stars can be seen, street lamps light up and birds stop twittering.
In a few words, it is a very exciting sight.

Eclipses take place when the sunlight or moonlight is darkened for a short time. They also happen in relation to other planets, when, for instance, Jupiter satellites move in the shadow of the planet but, in that case, they can be seen only through a telescope.

Total solar eclipse of August 11, 1999

It is important to remember that it is necessary to wear a suitable eye protection while looking at the Sun during a solar eclipse.

Sun Statistics

Diameter 1,392,000 km
Flattening 0.001
Rotational period-mean sideral 25.4 days
Rotational period-mean synoptic 27.3 days
Mass (Earth=1) 330,000
Mean density (water=1) 1.41
Escape velocity 617.5 km/s
Surface temperature +5,800° K
Nucleus temperature 15,000,000° K
Rotational period around the galactic centre 225 milion years
Mean distance from Earth (=1AU) 149,597,870 Km
Maximun distance 152,100,000 Km
Minimum distance 147,100,000 Km
Light distance from Earth 8.3 light-minutes
Distance from the Galaxy centre 25,000 light-years
Orbital eccentricity around the galactic centre 0.206
Spectrum type G2
Mean visible magnitude -26,7

Oh shining Sun,
what on earth would you be,
if I were not, down here,
on whom to shine?
(Friedrich Nietzsche)

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