Skip to main content Accessibility help
×
Hostname: page-component-84b7d79bbc-7nlkj Total loading time: 0 Render date: 2024-07-27T16:13:29.173Z Has data issue: false hasContentIssue false

9 - The gas-giant planets

Published online by Cambridge University Press:  04 August 2010

Get access

Summary

Out beyond the terrestrial planets and the asteriods, the gas-giant planets are the dominant bodies of the Solar System. As is the case for Venus, we can never see the surfaces of Jupiter, Saturn, Uranus and Neptune. We see just the upper layers of their atmospheres. Consequently, most of our observations of these worlds are concerned with their atmospheric phenomena.

Observing Jupiter

Jupiter is the easiest target for planetary observation. It is also one of the most fascinating. Orbiting the Sun at a distance of 778 million km, its vast globe spans 49 arcseconds at opposition. At such times a magnification of about ×40 will show the planet through the telescope as large as the full Moon looks when seen with the unaided eye. Even at conjuction the disc still spans 32 arcseconds, when a power of ×62 will enlarge it to the same extent as before. Moreover, the planet comes into opposition every 13 months and it is observable somewhere in the sky virtually all year round, apart from a month or two near the time of conjunction.

Nomenclature

Jupiter is a planet in turmoil. Even more exciting, from the point of view of the amateur astronomer, small telescopes show abundant detail. A 6-inch or 8-inch (152 mm or 203 mm) reflector is adequate for the serious study of the planet, anything larger being a bonus. As always with planetary observation, instrumental quality is to be preferred over sheer size.

Type
Chapter
Information
Publisher: Cambridge University Press
Print publication year: 1997

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
×