Skip to main content Accessibility help
×
Hostname: page-component-8448b6f56d-c4f8m Total loading time: 0 Render date: 2024-04-25T05:12:51.500Z Has data issue: false hasContentIssue false

University Education in the next Century

from 1 - University Education

Published online by Cambridge University Press:  01 June 2011

D. McNally
Affiliation:
University of London Observatory, Mill Hill Park, London NW7 2QS
L. Gouguenheim
Affiliation:
Observatoire de Paris, Meudon
D. McNally
Affiliation:
University College London
J. R. Percy
Affiliation:
University of Toronto
Get access

Summary

The Present

There is no doubt that the science of astronomy is now in an exhilarating state. We are in the era of the 10 m optical telescope. Radio astronomy rivals optical astronomy in both positional precision and sensitivity. Observation from space has opened access to a wide range of frequencies in the electromagnetic spectrum. The spectacular achievements of the Hubble Space Telescope underline the success story of space astronomy. At all wavelengths, detector technology has made striking advances in sensitivity and, coupled with cheap, sophisticated and powerful computers, raw data can be transformed into useful scientific data with breathtaking speed. One has only to add up the number of papers published in the three major astronomical journals to realise that one must read 100 journal pages a day (every day) to keep up with the literature in these three journals alone. Astronomy at the close of the 20th century is indeed exhilarating.

But there are indications that all is not well. Not unexpectedly the cost of new astronomical facilities is being called into question. Currently, no one nation can afford to finance a new telescope of the 10 m class and international consortia are now a commonplace to finance such facilities, e.g. the ESO 4 × 8 m telescopes in Chile. The great cost of science more generally, is now being seriously questioned, particularly in those areas of science which are fundamental, e.g. astronomy, particle physics, and which are not regarded as being currently relevant to industrial and commercial activity.

Type
Chapter
Information
Publisher: Cambridge University Press
Print publication year: 1998

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
×