A Solar Eclipse occurs when the moon gets in the way of the
sun as seen from the Earth. It is a special event to see and only visible along
a narrow path.
A Solar Eclipse can only happen during the lunar phase known
as the New Moon. At the same time the Moon must be crossing the ecliptic. The
Moon's Orbit is inclined by about five degrees relative to the eclipticthus not
every New Moon results in a solar eclipse and not every Solar Eclipse is a
Total Solar Eclipse.
There is an amazing cosmic coincidence that the Moon is
about 400 times closer to the Earth than the Sun. At the same time, the Sun is
about 400 times larger than the Moon. What this means is that the angular size
of the Sun and Moon as seen from the surface of the Earth is about the same in
the sky. When viewed from the surface of Earth, both the moon and sun appear to
be about one half degree in angular size – that is, about the size of your
thumbnail when you extend your arm.
Because the size of the Moon and Sun in the sky is just
about the same, there are times when you might see a Total Solar Eclipseand
other times an Annular Solar Eclipse if you are in the right location - the
central path of totality or annularity. If you are outside this path you might
see a partial eclipse or no eclipse at all.
In astronomical terms, the Sun and Moon have roughly the
same angular size. This makes it possible for a solar eclipse to occur. No
other planets in our solar system enjoys the same one-to-one ratio between the
size of a moon and the Sun.
The result is a very small shadow cast from the Moon onto
the Earth. The shadow is in the shape of a cone. When it intersects with the
planet Earth it is an oval shape about 100 miles across with a varying major
axis size. There are two parts of the shadow, the umbra, the darkest part, and
the penumbra, the surrounding ring that is not quite as dark. To see a total
solar eclipse you must be inside the umbra. A partial eclipse is seen when you
are in the penumbra.
During a Total Solar Eclipse you can see parts of the sun
not normally visible to the eye such as the corona and prominences. These items
are only visible during the short time between second contact and third contact
of a Total Solar Eclipse.
By,EDILENA
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