File:Dominion Radio Astrophysical Observatory largest dish.jpg
Original file (1,058 × 1,600 pixels, file size: 1.18 MB, MIME type: image/jpeg)
Captions
Captions
Summary[edit]
| Description |
The largest "dish" telescope at the Observatory is 26 metres in diameter. Its curved surface is a mirror which reflects the incoming radio waves to the focal point near the top of the tripod. Here a small antenna collects the radio energy and feeds it to a sensitive radio receiver. The receiver boosts the weak signal which is then sent down a cable to the control building, where it is recorded for later analysis. The 26-metre telescope is mainly used to receive radio waves of 21 -centimetre wavelength. At any instant, it records the radio emission from an area of sky about the size of the full moon. The telescope can be pointed in any direction above the horizon by motors that drive it around two perpendicular axes, and it can "track" a certain object in the sky as the earth rotates. It is used for studies of diffuse clouds of hydrogen gas in our galaxy by observing the 21 -centimetre-wavelength radio waves that are emitted by hydrogen atoms. In addition, clouds of interstellar gas that have been heated by newly-formed stars have been investigated. The high temperature of these clouds results in very agitated motions of their atoms and electrons, producing radio emission. Superimposed on this general emission from the hot gas are weak radio signals, at specific wavelengths, from atoms other than hydrogen. Studies of these "trace" elements will provide insight into the composition of gas clouds such as the one out of which the sun and solar system formed. -DRAO |
| Date | |
| Source |
|
| Author | Darren Kirby from Penticton, BC, Canada |
| Camera location |  | View this and other nearby images on: OpenStreetMap |  |
|---|
Licensing[edit]
- You are free:
- to share – to copy, distribute and transmit the work
- to remix – to adapt the work
- Under the following conditions:
- attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
- share alike – If you remix, transform, or build upon the material, you must distribute your contributions under the same or compatible license as the original.
|
This image, originally posted to Flickr, was reviewed on August 5, 2010 by the administrator or reviewer File Upload Bot (Magnus Manske), who confirmed that it was available on Flickr under the stated license on that date. |
File history
Click on a date/time to view the file as it appeared at that time.
| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 20:02, 5 August 2010 | | 1,058 × 1,600 (1.18 MB) | File Upload Bot (Magnus Manske) (talk | contribs) | {{Information |Description=The largest "dish" telescope at the Observatory is 26 metres in diameter. Its curved surface is a mirror which reflects the incoming radio waves to the focal point near the top of the tripod. Here a small antenna collects the ra |
You cannot overwrite this file.
File usage on Commons
The following 2 pages use this file:
File usage on other wikis
The following other wikis use this file:
- Usage on arz.wikipedia.org
- Usage on de.wikipedia.org
- Usage on fr.wikipedia.org
- Usage on lb.wikipedia.org
- Usage on pt.wikipedia.org
- Usage on www.wikidata.org
