Skip to main content Accessibility help
×
Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-22T20:46:52.106Z Has data issue: false hasContentIssue false

Introduction

Published online by Cambridge University Press:  05 September 2017

Get access

Summary

Galaxies are one of the most fascinating phenomena in the universe. The diversity of their forms is an indication of various interaction processes which take place within or between galaxies.

Galaxies can be described abstractly as collections of gas, dust, and stars. However, a look at the astrophysics of galaxies allows one to better understand their morphology. Only shortly after their discovery, the study of the forms and evolution of galaxies led to fundamental questions about the nature of the universe.

THE FIRST GALAXY CATALOGUES

One of the early telescopic observers was Charles Messier, who catalogued the first galaxies in the second half of the eighteenth century. His motivation was to avoid confusing these specks of light with new comets. The first edition of the Messier catalogue was published in 1774 and extended in 1780 and 1781. In the Messier catalogue, there was no classification of nebulae according to their appearance. The first galaxy in the Messier catalogue is M 31, the Andromeda Galaxy. In the original catalogue, Messier describes M 31 as “the beautiful nebula in the belt of Andromeda, in the form of a spindle, similar to two opposite cones or pyramids whose bases touch”. The galaxies M 32 and M 33 follow in the catalogue. M 32 is described as a “small, round nebula” and one reads about M 33 that “the nebula is of white light which is almost uniform, but somewhat brighter at two-thirds of its diameter”. These prosaic texts describe the objects, but do not allow a comparison or classification since such descriptions depend on the individual impressions at the telescope and the size of the instrument.

A further pioneer in the observations of galaxies was Friedrich Wilhelm Herschel (known as William Herschel after his emigration to England) who, aided by his sister Caroline, actively looked for further such nebulae and star clusters. Their observations led to several catalogues of “new Nebulæ, nebulous Stars, planetary Nebulæ, and Clusters of Stars” which were published in 1786, 1789, and 1802. William Herschel writes in the preface to his third catalogue that “our stock of materials is now so increased, that we should begin to arrange them more scientifically”.

Type
Chapter
Information
Publisher: Cambridge University Press
Print publication year: 2017

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 [email protected] 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
×