|[Picture of solar eclipse March 20th 2015 9:20am, Picture by Sidra Malik, Dundalk, Ireland ]|
|[Simulation of solar eclipse viewed from space]|
One of the most prominent features of the sky is the Moon. Over the thousands of years man has looked up at the night sky and has always seen he same side of the Moon. However the one thing that does change in appearance, is the sides that are illuminated so its appearance changes regularly throughout the day and seasons.
Whether it is today, tomorrow, next week or next year, the same side of the Moon and same patterns will still be observed. Many people make a false observation by thinking the Moon does not rotate however in fact the Moon does rotate on its axis. It rotates once for every revolution it makes around the earth and always keeping the same face towards the earth. This is quite an amazing phenomenon called synchronous rotation as the revolution and rotation are synchronized with perfection. The rotation is slightly elongated causing the near side always face towards the earth.
|[Simulation of rotation of Moon around Earth]|
The other side of the Moon which we seldom see in fact the far side or dark side of the Moon spends around the same amount of time in sunlight as the near side. This was unknown to man until recent advancement in space flight and technology.
|[(simulation) Far side of moon receiving light from the Sun]|
"Blessed is He Who made constellations in the skies (Space),
And placed therein a lamp (Sun)
And a Moon which has reflected light." - Al Quran
Unlike the Sun, the Moon does not have a source of light of its own, it reflects and shines by the light received from the Sun.
There are three types of solar eclipse; total, partial and annular. A total solar eclipse occurs when the Moon completely blocks the disk of the Sun. This is one of the most amazing sights man can witness in nature.
A partial solar eclipse occurs when the Moon only partially covers the Sun.
An annular solar eclipse occurs when the Moon is slightly further away from the Earth in its orbit and appears smaller in sky, it goes over the sun but does not completely block it.
[A total solar eclipse]
[A partial solar eclipse]
[An annular solar eclipse]
However you may be wondering despite all of this how is it that the Moon and the Sun seem to be the same size ?
This is due to a remarkable phenomenon by where the Sun and Moon appear to be the same size when we view from Earth. The Sun has a diameter which is about 400 times greater than the Moon but at the same time the Sun is also about 400 times farther away. The diameter of the Sun is 1,391,684 km, distance of Sun from Earth is 149,600,000 km. The diameter of the Moon is 3,476 km with a distance of 384,400 km.
A remarkable coincidence indeed!
One of the important astronomers of the years 858-929 was Al-Battani, Abu'Abudallah Muhammad ibn Jabir also know as Albateginus. An Arab astronomer who demonstrated that the Sun's distance from the Earth, its apparent angular size, varies which explained why both lunar and solar eclipses are made possible. He made the first truly accurate calculations of the solar year (365.24 days).
|[Crater on Moon named in honor of Albateginus]|
He also produced a number of important trigonometric equations that are now commonly used across many disciplines of Engineering and other Sciences . Data produced by Albateginus continues to be used even today.
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To see a total solar eclipse you must be located at at a very narrow band where the Moon's shadow is cast onto the face of the Earth.
NASA's SDO (Solar Dynamics Observatory) which makes its path around earth in 24 hours is situated in a geosynchronous rotation around earth and is in unique situation where it views an eclipse where the Moon is covering the Sun and another eclipse where the Earth eclipses the Sun.
We are not as lucky to see such eclipses simultaneously but the next eclipse to occur and be visible from Ireland will be in the year 2026 and hopefully it wont be cloudy day with such poor visibility as we had this time, so until next time goodbye!
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