(Translated by https://www.hiragana.jp/)
second (unit of time) -- Britannica Online Encyclopedia
The Wayback Machine - https://web.archive.org/web/20111013155102/http://www.britannica.com:80/EBchecked/topic/531340/second

"Email" is the e-mail address you used when you registered.

"Password" is case sensitive.

If you need additional assistance, please contact .

Enter the e-mail address you used when enrolling for Britannica Premium Service and we will e-mail your password to you.

second

ARTICLE
from the
Encyclopædia Britannica

second, fundamental unit of time, now defined in terms of the radiation frequency at which atoms of the element cesium change from one state to another.

The second was formerly defined as 1/86,400 of the mean solar day—i.e., the average period of rotation of the Earth on its axis relative to the Sun. In the mid-20th century this definition became inadequate because of the need for increased precision in timekeeping. In 1956 the second was redefined by the International Committee on Weights and Measures as 1/31,556,925.9747 of the length of the tropical (seasonal) year 1900. In 1967 the 13th General Conference on Weights and Measures provisionally defined the second as 9,192,631,770 cycles of radiation associated with the transition between the two hyperfine levels of the ground state of the cesium-133 atom (see atomic time). The number of cycles of radiation was chosen to make the length of the defined second correspond as closely as possible to that of the now obsolete astronomically determined second of Ephemeris Time (defined as the fraction of the tropical year given above). As the rate of rotation of the Earth constantly changes, it is necessary to occasionally add (or theoretically to subtract) a second during the year to ensure the atomic timescale Coordinated Universal Time (UTC) stays in synchronization with nature. This represents the sole definition of the second in the International System of Units (SI).

LINKS
Related Articles

Aspects of the topic second are discussed in the following places at Britannica.

Assorted References

  • history  (in  time (physics): Time units and calendar divisions)

    The familiar subdivision of the day into 24 hours, the hour into 60 minutes, and the minute into 60 seconds dates to the ancient Egyptians. When the increasing accuracy of clocks led to the adoption of the mean solar day, which contained 86,400 seconds, this mean solar second became the basic unit of time. The adoption of the SI second, defined on the basis of atomic phenomena, as the...

definitions

  • cesium clock value  (in  atomic clock (instrument);

    In 1967 the 13th General Conference on Weights and Measures redefined the second, the unit of time in the International System of Units, in terms of the cesium standard so as to equal the second of Ephemeris Time. The conference defined the second as “the duration of 9,192,631,770 periods of the radiation corresponding to the transition between the two hyperfine levels of the ground state...

    in  quantum mechanics (physics): Cesium clock )

    The cesium clock is exceedingly stable. The frequency of the oscillator remains constant to about one part in 1013. For this reason, the device has been used to redefine the second. This base unit of time in the SI system is defined as equal to 9,192,631,770 cycles of the radiation corresponding to the transition between the levels F = 4,...

  • Ephemeris Time value  (in  Ephemeris Time (chronology))

    ...the Moon were obtained visually by observations of occultations of stars by the Moon. By the time Ephemeris Time was superseded in 1984, it had served two important purposes: (1) the definition of a second of Ephemeris Time served as the basis for the redefinition in 1967 of the SI second on the atomic time scale, and (2) ET was the reference scale used for comparison with rotational time to...

  • International System of Units  (in  International System of Units (SI) (measurement);

    ...equals 1,000 grams as defined by the international prototype kilogram of platinum-iridium in the keeping of the International Bureau of Weights and Measures in Sèvres, France; for time, the second, the duration of 9,192,631,770 periods of radiation associated with a specified transition of the cesium-133 atom; for electric current, the ampere, which is the current that, if maintained in...

    in  measurement system: Time: second )

    The second is defined as the duration of 9,192,631,770 cycles of the radiation associated with a specified transition, or change in energy level, of the cesium-133 atom.

Other

The following is a selection of items (artistic styles or groups, constructions, events, fictional characters, organizations, publications) associated with "second"

Citations

MLA Style:

"second." Encyclopædia Britannica. Encyclopædia Britannica Online. Encyclopædia Britannica, 2011. Web. 13 Oct. 2011. <http://www.britannica.com/EBchecked/topic/531340/second>.

APA Style:

second. (2011). In Encyclopædia Britannica. Retrieved from http://www.britannica.com/EBchecked/topic/531340/second

 This feature allows you to export a Britannica citation in the RIS format used by many citation management software programs.
Help Britannica illustrate this topic/article.

Britannica's Web Search provides an algorithm that improves the results of a standard web search.

Try searching the web for the topic second.

No results found.
Type a word or double click on any word to see a definition from the Merriam-Webster Online Dictionary.
Type a word or double click on any word to see a definition from the Merriam-Webster Online Dictionary.
No results found.
Type a word to see synonyms from the Merriam-Webster Online Thesaurus.
Type a word to see synonyms from the Merriam-Webster Online Thesaurus.
  • All of the media associated with this article appears on the left. Click an item to view it.
  • Mouse over the caption, credit, links or citations to learn more.
  • You can mouse over some images to magnify, or click on them to view full-screen.
  • Click on the Expand button to view this full-screen. Press Escape to return.
  • Click on audio player controls to interact.
JOIN COMMUNITY LOGIN
Join Free Community

Please join our community in order to save your work, create a new document, upload media files, recommend an article or submit changes to our editors.

Log In

"Email" is the e-mail address you used when you registered. "Password" is case sensitive.

If you need additional assistance, please contact customer support.

Enter the e-mail address you used when registering and we will e-mail your password to you. (or click on Cancel to go back).

Save to My Workspace
Share the full text of this article with your friends, associates, or readers by linking to it from your web site or social networking page.

Permalink
Copy Link
Britannica needs you! Become a part of more than two centuries of publishing tradition by contributing to this article. If your submission is accepted by our editors, you'll become a Britannica contributor and your name will appear along with the other people who have contributed to this article. View Submission Guidelines
View Changes:
Revised:
By:
Share
Feedback

Send us feedback about this topic, and one of our Editors will review your comments.

(Please limit to 900 characters)
(Please limit to 900 characters) Send

Copy and paste the HTML below to include this widget on your Web page.

Copy Link
The Britannica Store

Share This

Other users can view this at the following URL:
Copy

Create New Project

Done

Rename This Project

Done

Add or Remove from Projects

Add to project:
Add
Remove from Project:
Remove

Copy This Project

Copy

Import Projects

Please enter your user name and password
that you use to sign in to your workspace account on
Britannica Online Academic.