Space Terms

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Chandrasekhar Limit

The Chandrasekhar limit is the value at which the mass of bodies composed by electron-degenerated matter is restricted. These bodies consist of nuclei, which are immersed in a gas of electrons. The limit is about 1.4 solar masses. This is the reason why white dwarfs, which are made up of electron-degenerate matter are unable to

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Celestial Sphere

The celestial sphere is an imaginary surface on which astronomical objects are located. Its center is the center of the Earth. However, the celestial sphere is too large in proportion to Earth’s size making its center considered as the same point of the observer. It is used in describing the location and movement of the

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Celestial Pole

The celestial pole is an imaginary point where the axis of the Earth on which it rotates is intersecting the presumed rotating spheres of the stars. There are two celestial poles namely the north and the south. The former appears directly overhead at the North Pole of our planet and the latter is at the

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Catadiopotric Telescope

Telescopes are made in such a way that its reflecting system continues to be improved. The mirrors are used in combination with the lens, which use both reflective and refractive properties of a system to form images called catadioptric. Catadioptric telescopes are special types of telescopes that combine the process of a refraction and reflection

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Carbonaceous Chondrite

When a meteoroid or any other outer space debris falls to Earth, it is called a meteorite. The stones that are recovered from the impact are truly out-of-this world, because of their differences in the chemical composition when compared from rocks in this planet. Some of these meteorites are called chondrites.

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Carbon Star

Carbon stars are gigantic stellar masses similar to red giants, but their atmosphere contains more carbon than oxygen. They are rare and they are so big they can swallow whole planets in our Solar System, indicating an advanced stage of evolution. Yes, stars too have different phases in their infinitesimal billion-year lifetime.

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