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the objective lens has the power of that lens inscribed on it
Specifically if you increase the diameter of the main lens, or of the main mirror (depending on the type of the telescope), you'll be able to observe dimmer objects (stars, planets, etc.). Also, the telescope's resolving power (angular resolution) improves with a bigger mirror/lens. For example, with a bigger mirror/lens you'll be able to distinguish two stars that are closer together as separate objects.
20 refers to the amplification, 70 mm to the diameter of the main lens or mirror. Note: This diameter is by far the most important piece of information.
The eyepiece is usually 10x, so multiply the objective by 10 to get true magnification
it would be 15 times 40 which is 600 times magnification
Because the 2cm lens has 4 times the area of a 1cm lens. (area = Pi*r2)
Field diameter of lens B equals field diameter of lens A times total magnification of lens A divided by total magnification of lens B
the naswe is 400
This is a variable power scope- from 6 power to 24 power. The front lens (objective lens) is 40mm in diameter.
It magnifies 4 times, and the objective (front lens) is 40 mm in diameter. A 3x9-40 would be a 3 to 9 power variable magnification scope, with a 40mm objective lens.
Yes, both have to do with the diameter of the objective mirror/lens
The oil immersion lens or objective has power 90X-100X and an eyepiece lens generally in light microscope comes with 10X so total magnification of oil immersion lens is 100X10 = 1,000
A fast lens will take a parallel beam of light and focus it in a relatively short distance. For example a 1 centimetre diameter lens that focusses the light to a spot 2 centimeters after the lens is quite fast. It has a short focal length, only two times longer than the diameter of the lens. We say it is an f/2 lens. Very few fast lenses are faster than f/1. It is dificult to design fast lenses that have good image blurring, high light transmission and low image distortion. Good ones are expensive. A long focal length lens for example that focusses a parallel beam to a spot at a distance 20 times its diameter after the lens would becalled a slow lens.
This is a variable power scope- from 3 to 9 power (first two numbers). The front lens is 40 mm in diameter.
40X
10 times
Provided that the parabolic shapes of the surfaces of both reflectors are similarly accurate,the "gains" are proportional to the areas, which also means proportional to the square ofthe diameters.(300m/50m)2 = (6)2 = 36 times moreor the larger reflector has 10log(36) = 15.6 dBmore gain, at any specific wavelength.