Skip to main content Accessibility help
×
Hostname: page-component-84b7d79bbc-7nlkj Total loading time: 0 Render date: 2024-07-28T00:17:58.997Z Has data issue: false hasContentIssue false

11 - Clusters, nebulae, and galaxies

Published online by Cambridge University Press:  22 September 2009

Michael A. Covington
Affiliation:
University of Georgia
Get access

Summary

The lure of the deep sky

The “deep sky” is the sky beyond the Solar System, and while it theoretically includes all stars except the Sun, in practice “deep-sky observing” means observing star clusters, nebulae, and galaxies.

For many amateur astronomers, including myself, deep-sky observing is the most interesting specialty, the most far-ranging form of celestial sightseeing. We bought our telescopes in order to see the universe. For the variety of sights and the variety of astrophysical processes behind them, deep-sky observing is unsurpassed.

Critics point out that deep-sky observers are unlikely to contribute anything to science, since most of the objects are near the limit of visibility in amateur telescopes, and apart from occasional supernovae in distant galaxies, there is nothing that amateur equipment can discover. That doesn't deter us. Seeing the sights is enough.

Deep-sky objects

Asterisms

An asterism is any small group of stars that catches the eye, whether or not the stars form a cluster in space. M73, for instance, is an asterism of four stars in Aquarius.

In recent years, amateur astronomers have given colorful names to numerous telescopic asterisms, many of which were enumerated by Philip S. Harrington in The Deep Sky: An Introduction (Sky Publishing, 1998). That book is actually an excellent overall guide to deep-sky observing and includes a small but useful star atlas. I must confess to having subsequently named two asterisms myself, Webb's Horseshoe (p. 207) and the Perfect Right Angle (p. 245).

Type
Chapter
Information
Celestial Objects for Modern Telescopes
Practical Amateur Astronomy Volume 2
, pp. 144 - 164
Publisher: Cambridge University Press
Print publication year: 2002

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
×