k Voyager 2 image, tinted pale blue, showing the planet Neptunes two major rings. The rings have radii of 53,000 km and 63,000 km and are composed of microscopic dust particles. They are narrow and contain clumps and kinks thought to be associated with tiny shepherd moonlets, too small to be detected directly. Similar narrow, dusty, braided rings have been detected around Saturn the Fring Enke Gap ringlet and Uranus 1986U1R. The image was obtained as the Voyager spacecraft was leaving the Neptune system on 26 August, 1989, from a distance of 1.1 million kilometres. Editorial Stock Photo - Afloimages
Sign up
Login
All images
Voyager 2 image, tinted pale blue, showing the planet Neptune's two major rings. The rings have radii of 53,000 km and 63,000 km and are composed of microscopic dust particles. They are narrow and contain clumps and kinks thought to be associated with tiny 'shepherd' moonlets, too small to be detected directly. Similar narrow, dusty, braided rings have been detected around Saturn (the F-ring & Enke Gap ringlet) and Uranus (1986U1R). The image was obtained as the Voyager spacecraft was leaving the Neptune system on 26 August, 1989, from a distance of 1.1 million kilometres.
ED

Voyager 2 image, tinted pale blue, showing the planet Neptune's two major rings. The rings have radii of 53,000 km and 63,000 km and are composed of microscopic dust particles. They are narrow and contain clumps and kinks thought to be associated with tiny 'shepherd' moonlets, too small to be detected directly. Similar narrow, dusty, braided rings have been detected around Saturn (the F-ring & Enke Gap ringlet) and Uranus (1986U1R). The image was obtained as the Voyager spacecraft was leaving the Neptune system on 26 August, 1989, from a distance of 1.1 million kilometres.

Details

ID
10619934

Collection

License type
Editorial

Photographer

Creation date
19-11-2010

Contact Aflo for all commercial uses.


Keywords
More
Sign in
Member access
Login not found.