What part of an optical telescope determines the magnification level?
Magnification of a telescope is actually a relationship between two independent optical systems: the telescope itself and the eyepiece you are using. To determine power, divide the focal length of the telescope (in mm) by the focal length of the eyepiece (in mm).
Magnification depends on the ratio of the telescope's focal length to the focal length of the eyepiece. To calculate this, divide the focal length of the telescope (ft) by the focal length of the eyepiece (fe): M = ft / fe.
For all telescopes, it is the eyepiece that determines how much an image is magnified. Some telescopes come with a variety of eyepieces so that you can change the magnification. The thing to note is that as the magnification is increased, the viewing area of the telescope is decreased.
In a REFRACTING TELESCOPE, light from a distant object is collected and focused by a convex lens called the OBJECTIVE LENS. A second lens, called the EYEPIECE LENS, works as a magnifying glass to enlarge the image.
Both of these microscopes have an objective lens, which is closer to the object, and an eyepiece, which is the lens you look through. The eyepiece lens typically magnifies an object to appear ten times its actual size, while the magnification of the objective lens can vary.
Eyepieces and telescopes are denoted by their focal lengths. Together, the two focal lengths produce a magnification, calculated as the telescope's focal length divided by the eyepiece's focal length (for more on this, read our guide to telescope stats).
Magnification is determined by the ratio of the focal lengths and the objective and eyepiece lenses.
The light-gathering power of a telescope is directly proportional to the area of the objective lens. The larger the lens, the more light the telescope can gather. Doubling the diameter of the lens increases the light gathering power by a factor of 4.
The resolving power of a telescope can be calculated by the following formula: resolving power = 11.25 seconds of arc/d, where d is the diameter of the objective expressed in centimetres.
Telescope components
Primary mirror (for reflecting telescopes), which carries the same role as the primary lens in a refracting telescopes. Eyepiece, which magnifies the image. Mounting, which supports the tube, enabling it to be rotated. Telescopes can be divided into two main categories: refractors and reflectors.
Which part of a telescope is responsible for magnifying an image quizlet?
Reflecting telescopes suffer from chromatic aberration because the light must pass through the glass. Refracting and reflecting telescopes form an image that is small, inverted, and difficult to observe directly; therefore, an eyepiece is normally used to magnify the image and make it convenient to view.
The most important aspect of any telescope is its aperture, the diameter of its main optical component, which can be either a lens or a mirror. A scope's aperture determines both its light-gathering ability (how bright the image appears) and its resolving power (how sharp the image appears).
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