|
|||
|
Optical telescope - Wikipedia, the free encyclopedia
|
|||
|
The light gathering power of a telescope is directly related to the area (or to the square of the diameter) of the main mirror or lens.
http://stargazing.suite101.com/article.cfm/astronomical...
|
|||
|
|||
|
observing deep sky objects such as faint galaxies and nebulae requires dark skies with excellent sky transparency and wide apertures of at least 8-10" as light-gathering power is especially important in determining the ability to see faint objects such as distant stars, nebulae & galaxies, ... telescope resolving power:
|
|||
|
Slide # 11: Telescope Terms ... the light gathering power depends on the collecting area of the objective ... 362 times more light gathering power!
|
|||
|
Next: Resolving Power of a Telescope; ... Light Gathering Power (Page 101) (Problem 5-1); ... The larger the diameter of a telescope mirror, the more light it collects. Similarly, the larger the mirror, the less time it takes it to collect a given amount of light. This second relation can be expressed as:
|
|||
|
Let's say you are an astronomer living on a planet orbiting Alpha Centauri, 4.3 light years away, and you want to build a telescope with which to study Earth at optical wavelengths. You want to be able to observe the planet Earth in fine detail.
|
|||
|
Light Gathering Power Example: Human Eye vs. Hale Telescope ... Back to first slide ... View graphic version...
|
Copyright © 2009, Dictionary.com, LLC. All rights reserved.