ESA    Life in Space    Expanding Frontiers    Improving Daily Life    Protecting the Environment    Benefits for Europe  
   
Media Centre
Press ReleasesESA TelevisionLaunch Media CornerExhibitions
Services
CalendarPublicationsFrequently asked questionsESA-sponsored ConferencesHelpSite CreditsPortal terms of useCommentsSubscribe
 
 
 
Bookmark and Share
 
 
 
 
Postcards from Venus: enter the Planetary Society Art Contest
 
16 December 2005

Download:
 HI-RES JPEG (Size: 508 kb)  HI-RES TIFF (Size: 7468 kb)


Credits: ESA
 
 
Venus’s atmosphere is composed almost entirely of carbon dioxide, with very little water vapour. It has significant amounts of corrosive sulphur-bearing gases and rapidly moving clouds of sulphuric acid droplets. The dense clouds scatter back to space about 80% of the radiation received from the Sun.

Despite only the small amount of solar flux reaching the surface, enough energy is trapped by gases and particles present in the lower atmosphere, to raise the temperature at the surface dramatically, enough to make Venus’s surface the hottest in the Solar System.

Credits: ESA / AOES Medialab

 
 


Credits: ESA
 
 
Looking at VenusArtist's impression of Venus Express orbiting Venus
More about...
Venus Express factsheetVenus Express in-depthStatus reports Winning postcards
Choose a language
 Vollständiger Artikel Vollständiger Artikel Article complet Volledig artikel Til hele historien Noticia completa Koko tarina Article complet Articolo intero Les hele saken Volledig artikel Artigo completo Hela historien Vollständiger Artikel Article complet Articolo intero
 
 
 
   Copyright 2000 - 2012 © European Space Agency. All rights reserved.