Jump to content
Main menu
Main menu
move to sidebar
hide
Navigation
Main page
Recent changes
Random page
Help about MediaWiki
Special pages
Niidae Wiki
Search
Search
Appearance
Create account
Log in
Personal tools
Create account
Log in
Pages for logged out editors
learn more
Contributions
Talk
Editing
History of physics
(section)
Page
Discussion
English
Read
Edit
View history
Tools
Tools
move to sidebar
hide
Actions
Read
Edit
View history
General
What links here
Related changes
Page information
Appearance
move to sidebar
hide
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
===Radiation experiments=== [[File:J.J Thomson.jpg|thumb|upright|[[J.J. Thomson]] (1856–1940), discoverer of [[electron]] and [[Isotope|isotopy]], and inventor of [[mass spectrometer]], received 1906 [[Nobel Prize in Physics]].]] In the 19th century, experimenters began to detect unexpected forms of radiation: [[Wilhelm Röntgen]] caused a sensation with his discovery of [[X-ray]]s in 1895; in 1896 [[Henri Becquerel]] discovered that certain kinds of matter emit radiation on their own accord. In 1897, [[J. J. Thomson]] discovered the [[electron]], and new radioactive elements found by [[Marie Curie|Marie]] and [[Pierre Curie]] raised questions about the supposedly indestructible atom and the nature of matter. Marie and Pierre coined the term "[[radioactive decay|radioactivity]]" to describe this property of matter, and isolated the radioactive elements [[radium]] and [[polonium]]. [[Ernest Rutherford]] and [[Frederick Soddy]] identified two of Becquerel's forms of radiation with electrons and the element [[helium]]. Rutherford identified and named two types of radioactivity and in 1911 interpreted experimental evidence as showing that the atom consists of a dense, positively charged nucleus surrounded by negatively charged electrons. Classical theory, however, predicted that this structure should be unstable. Classical theory had also failed to explain successfully two other experimental results that appeared in the late 19th century. One of these was the demonstration by [[Albert A. Michelson]] and [[Edward W. Morley]] – known as the [[Michelson–Morley experiment]] – which showed there did not seem to be a [[preferred frame]] of reference, at rest with respect to the hypothetical [[luminiferous ether]], for describing electromagnetic phenomena. Studies of radiation and radioactive decay continued to be a preeminent focus for physical and chemical research through the 1930s, when the [[discovery of nuclear fission]] by [[Lise Meitner]] and [[Otto Frisch]] opened the way to the practical exploitation of what came to be called [[Nuclear power|"atomic" energy]].
Summary:
Please note that all contributions to Niidae Wiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
Encyclopedia:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Search
Search
Editing
History of physics
(section)
Add topic