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Vandalism removed. Mickman1234 ( talk) 06:39, 14 December 2008 (UTC)
http://www.pro-physik.de/Phy/leadArticle.do?laid=12813
here is said that new obervations show that tritons atmosphere has a pressure from 40 to 65 microbars.
original: Originalveröffentlichung: E. Lellouch, C. de Bergh, B. Sicardy, S. Ferron, H.-U. Käufl.: Detection of CO in Triton's atmosphere and the nature of surface-atmosphere interactions. Astronomy & Astrophysics, 512, L8 (2010) dx.doi.org/10.1051/0004-6361/201014339
this observations were made with :Cryogenic High-Resolution Infrared Echelle Spectrograph (CRIRES) on VLT from ESO
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This article was the subject of a Wiki Education Foundation-supported course assignment, between 18 January 2022 and 9 May 2022. Further details are available
on the course page. Student editor(s):
Jdjr34 (
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This article was the subject of a Wiki Education Foundation-supported course assignment, between 16 January 2024 and 10 May 2024. Further details are available
on the course page. Student editor(s):
Gnobis84 (
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— Assignment last updated by Gnobis84 ( talk) 17:17, 18 March 2024 (UTC)
Hello. I added the dust devil hypothesis in the paragraph under the Voyager 2 plume observations. My class did not have any reviewers assigned, so it may need to be copyedited. Let me know if there is anything that should be fixed Gnobis84 ( talk) 22:02, 10 April 2024 (UTC)
![]() | This article is rated Start-class on Wikipedia's
content assessment scale. It is of interest to the following WikiProjects: | ||||||||||||||||||||||||||
|
![]() | A fact from Atmosphere of Triton appeared on Wikipedia's
Main Page in the
Did you know column on 6 January 2008, and was viewed approximately 1,508 times (
disclaimer) (
check views). The text of the entry was as follows:
| ![]() |
Vandalism removed. Mickman1234 ( talk) 06:39, 14 December 2008 (UTC)
http://www.pro-physik.de/Phy/leadArticle.do?laid=12813
here is said that new obervations show that tritons atmosphere has a pressure from 40 to 65 microbars.
original: Originalveröffentlichung: E. Lellouch, C. de Bergh, B. Sicardy, S. Ferron, H.-U. Käufl.: Detection of CO in Triton's atmosphere and the nature of surface-atmosphere interactions. Astronomy & Astrophysics, 512, L8 (2010) dx.doi.org/10.1051/0004-6361/201014339
this observations were made with :Cryogenic High-Resolution Infrared Echelle Spectrograph (CRIRES) on VLT from ESO
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This article was the subject of a Wiki Education Foundation-supported course assignment, between 18 January 2022 and 9 May 2022. Further details are available
on the course page. Student editor(s):
Jdjr34 (
article contribs).
This article was the subject of a Wiki Education Foundation-supported course assignment, between 16 January 2024 and 10 May 2024. Further details are available
on the course page. Student editor(s):
Gnobis84 (
article contribs).
— Assignment last updated by Gnobis84 ( talk) 17:17, 18 March 2024 (UTC)
Hello. I added the dust devil hypothesis in the paragraph under the Voyager 2 plume observations. My class did not have any reviewers assigned, so it may need to be copyedited. Let me know if there is anything that should be fixed Gnobis84 ( talk) 22:02, 10 April 2024 (UTC)