Space Terms

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Airy Disk

When light is passed through an aperture small enough, what you get is not a bright image of a dot, but a bright disc surrounded with more circular rings alternately bright and dark. The bright central dot is called an Airy disk and the pattern that surrounds it is called an Airy pattern, named after […]

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Active Optics

Telescopes need mirrors to reflect and collect light. Before the 1980s, reflective mirrors for telescopes were usually very thick so they can hold their shape to the required precision as it moves across the sky. Their sizes have set a physical limit to how big they can get. Mirrors of this type are usually just

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Achromatic Lens

In the physics of light, known as optics, light can be bent using lenses. As you may have observed on a daily basis, concave and convex mirrors distort the image that it reflects. Magnifying lenses can enlarge an object. These properties are all due to the capability of these mirrors and lenses to bend light.

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Absorption Line

Quantum mechanical models of atoms predict that atoms can absorb specific wavelengths of the electromagnetic spectrum and release the absorbed energy in other forms such as heat. Working on the visible light spectrum, or commonly called as just “light”, each wavelength translates to colors. Different wavelengths correspond to the different colors perceivable with the naked

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Absolute Zero

Absolute zero is the theoretical temperature at which entropy is at minimum. It is a physical limit to the lowest possible temperature. When a system reached absolute zero, pressure, volume and internal pressure also become zero. At this temperature, the energy of the matter involved is at the minimum, though it is not correct to

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Cosmic Rays

Cosmic rays refer to the energetic particles from space that enters the earth’s atmosphere. The earliest observers thought that these particles were rays and thus named them as such. However further in the future we were able to discern that these particles come in individual protons or alpha particles instead of a steady stream of

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Cosmological Constant

Cosmological constant is a physics term generally denoted by the symbol lambda. Lambda is a Greek letter that looks like a triangle missing its base. The cosmological constant was developed by Albert Einstein to be a modification to his original Theory of Relativity. At that time Einstein was trying to posit that the universe is

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