Skip to main content Accessibility help
×
Hostname: page-component-848d4c4894-xm8r8 Total loading time: 0 Render date: 2024-06-16T15:32:01.386Z Has data issue: false hasContentIssue false

2 - Choosing your imaging equipment

Published online by Cambridge University Press:  05 September 2016

Get access

Summary

Shared, fundamental characteristics

Photolenses, refractors, and reflectors share two basic characteristics and a derived one.

  1. • The focal length, or optical distance between the objective or the main mirror and the image sensor; this determines the size of the image. This is not the most important factor because this magnification can easily be increased or decreased as long as it is not excessive with respect to the diameter and the optical quality.

  2. • The diameter of the objective or of the main mirror; this determines the resolving power (accuracy), the contrast, and the sensitivity to turbulence.

  3. • The focal-length/diameter ratio, or F/D ratio, an important parameter for photography; it determines the exposure duration, the ease of focusing, and some geometrical characteristics which affect the image field.

A golden rule is that, when the focal length is large with respect to the diameter, optical flaws are minimized. As the diameter increases, the F/D ratio of an achromatic refractor has to increase if we are to maintain a comparable quality (e.g. from F/D = 8 for an 80-mm (3-in) achromatic refractor up to F/D = 15 for a 150-mm (6-in) achromatic refractor). Reflectors and apochromatic refractors are less affected. Furthermore, devices with “slow” optics (when the F/D ratio is more than 8 or so) are cheaper because they are easier to manufacture while maintaining the same – or better – optical quality, easier optical adjustment, and possibly a better ease of use even with a basic focuser. Lunar imaging, unlike most astrophotographical subjects, does not demand a “fast” (<6) F/D ratio.

Optical flaws

Chromatism and astigmatism affect the entire image. Other optical deformations affect mainly the corners of the image.

  1. • Coma transforms points at the corners into little comet-like spots.

  2. • Distortion either stretches the corners or inflates the center.

  3. • Astigmatism transforms points into crosses when the image is focused, or vertical or horizontal lines when it is out of focus.

  4. • Chromatism is the impossibility for the optics to make all colors converge at the same place. While the image is sharp in red, it is somewhat unfocused in blue. In addition, lenses suffering from chromatism also focus the blue poorly and waste light.

Type
Chapter
Information
Shoot the Moon
A Complete Guide to Lunar Imaging
, pp. 17 - 90
Publisher: Cambridge University Press
Print publication year: 2016

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×