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you can find the telescope on cp at the beacon which is on top of the light house.
Please refer to the link below. This will take you to a web site that discusses this. Multiwavelength astronomy is dedicated to observing the various spectrums of radiation emitted. That is called its light gathering ability. The 'aperture size' determines the amount of light (radiation) a telescope gathers This site might help you obtain a more in depth answer imagine.gsfc.nasa.gov IT IS CALLED "LIGHT GRASP" in an optical telescope and "RF GAIN" in a radio-telescope.
light house
radio telescope detects radio waves and a light telescope views light waves.
light from the they orbit makes it difficult to locate extrasolar planets with telescope
The Galilean telescope ray diagram helps us understand how light rays pass through the lenses of the telescope to produce an image. This diagram is important because it shows how the lenses in the telescope work together to magnify distant objects, allowing us to see them more clearly. By studying this diagram, we can better grasp the optical principles behind the Galilean telescope's functioning.
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light from the they orbit makes it difficult to locate extrasolar planets with telescope
A radio telescope detects light in the form of radio waves and a refracting telescope detects light in the visible wavelengths
To find the aperture of a reflecting telescope, you would measure the diameter of the primary mirror. The aperture of a telescope is the diameter of its primary light-gathering element, which in the case of a reflecting telescope, is the primary mirror.
The light gathering power of a telescope is directly proportional to the area of the objective lens of the telescope.
To make a tv telescope