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Summary on Comets

 
     
 

 

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What Is A Comet?

A comet is a celestial body made up mainly of ice and dust, revolving around the sun. Whenever a comet gets near the sun, the sun’s heat causes some of the ice to melt. As a result, the dust particles suspended in the ice are released. This released dust trails behind the comet for a while and if we happen to see it we would see a long luminous tail behind the comet. Eventually some of this dust spreads around the comet’s orbit and some stays close to the comet. And when the paths of the earth and the comet cross, we see a spectacular show termed as a meteor shower.

Comets can be seen only when they are near to the sun. The main feature that distinguishes comets from other celestial bodies is their nebulous appearance and elongated orbits.

 

How long have comets been in existence?
According to the most widely believed theory, comets are believed to be as old as the solar system itself.  They are said to be the remnants of planet formation, i.e., whatever did not join any planet during formation got left over as comets. Which is why comets and planets exhibit similar patterns of movement – in an orbit around the sun. The reason for comets having extremely elongated orbits is attributed to the gravitational pull of the planets.

Comets have been sighted by man since time immemorial and till 1577, they were considered an atmospheric phenomenon. Proof of man having sighted comets as early as the eleventh century has been found in an illustration in a Bayeaux Tapestry which shows a group of people pointing out to a body in the sky with a blazing tail.

Early astronomers to have worked on comets were Danish astronomer Tycho Brahe, who proved that comets were celestial bodies, and British scientist Sir Isaac Newton, who in the 17th century demonstrated the similarities between movement of comets and planets. 

Naming of comets
It has been customary to name comets after the astronomers who discovered them. And the name that comes to mind when encountering the word ‘comet’, is almost always Halley’s comet. Halley’s comet has been named after the British astronomer Edmond Halley who showed the comet of 1682 to be identical with two others. The other two had appeared in 1607 and 1531. He also predicted that the comet would reappear in 1759 and time did prove him true. In 1986, the Halley’s comet made another appearance. It makes a reappearance every 76 years.  

Comet Tempel-Tuttle, which is seen once every 33 years, is named jointly after two astronomers Ernst Wilhelm Liebrecht Tempel, who saw it in December 1865, and Horace Parnell Tuttle, who saw it in January 1866, just a month later than Tempel. But as both the discoveries were independent of each other the comet was named after both of them.


Haley’s comet

What are comets made of and how big are they?
Frozen water and fine carbon dust are the main components of a comet. The dust and gas, which form a comet, on getting heated by the sun, create tails that are millions of times larger than the nucleus of the comet. These tails are often large enough to be visible from the earth.

Photographs of the Halleys comet taken in 1986 by the Giotto spacecraft (launched by the USSR in 1986) show a nucleus at the core of the comet. The color of the nuclei was found to be black. The nucleus appears to be covered by a crust made up of fine dust particles. The size of the nuclei itself is quite small.

Observations of the Halley’s comet showed its dimensions to be 15 kilometers by 8 kilometers. Its mass was estimated to be 1017 grams.  The time taken by a comet to orbit the sun once – of many comets have also been calculated. For instance, the Donati’s Comet takes two thousand years, while the Comet Hyakutake takes ten thousand years.

Different types of comets
On the basis of their life span, comets are classified as short period comets and long period comets. The short-period comets have a life span of  less than 200 years and the long-period ones exist for more than 200 years. The US probe known as the International Cometary Explorer, launched in 1985, was the first attempt at investigating comets. The comet investigated by this probe was Comet Giacobini-Zinner. 

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