Skip to main content Accessibility help
×
Hostname: page-component-5c6d5d7d68-7tdvq Total loading time: 0 Render date: 2024-08-27T02:12:55.413Z Has data issue: false hasContentIssue false
This chapter is part of a book that is no longer available to purchase from Cambridge Core

19 - Black holes: trapdoors to nowhere

from Part III - Frontiers

J. B. Kennedy
Affiliation:
University of Manchester
Get access

Summary

Anyone hauling a boulder to the top of a skyscraper and dropping it on to the street below would expect a catastrophic impact: flying shards of rock and road, streaks of sparks and smoke, the clap and crack of the reverberating bang. Similarly, when a planet, comet or any other material falls into a star, the resulting explosion is often dramatic. It can produce blinding flashes, bursts of high-energy X-rays and gigantic glowing flares of fiery gases.

But, in early 2001, astronomers observing a strange object 6,000 light-years from Earth with the orbiting Hubble Telescope reported that they had seen the opposite. Massive clumps of hot gases many times larger than Earth were being sucked down into a large, invisible object. As they raced downwards, the accelerated jostling heated them, and they glowed and pulsed with incredible energies. Then nothing. The gases just disappeared. There was no explosion, no flashes, no flares – just nothing.

Einstein's theory of general relativity predicts the existence of black holes: bodies so dense that their gravity captures everything close by and prevents it from escaping. Not even light, the fastest and most nimble signal known, can climb up and away from a black hole. They are colourless, invisible, wholly black patches in the sky. For this reason, physicists doubted for many years that black holes could ever be seen at all. And if they could not be observed, they doubted they were a serious part of empirical science.

Type
Chapter
Information
Space, Time and Einstein
An Introduction
, pp. 188 - 192
Publisher: Acumen Publishing
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
×