Dustiest Star Could Harbor a Young Earth
The Zodiacal Light as photographed from Mauna Kea shortly after the end of evening twilight. The wedge-shaped glow (whitish glow at center) is produced by the scattering of sunlight by the small amount of dust remaining from the formation of the solar system. In a system like BD +20 307 the density of the dust is thought to be about one-million times more dense than currently exists in our solar system to create this glow. Digital photo obtained with Nikon D1X camera using a 14mm f/2.8 lens exposed for 120 seconds.
Credit:Gemini Observatory
About the Image
Id: | gemini0506b |
Type: | Photographic |
Release date: | July 20, 2005, 8 p.m. |
Related releases: | gemini0506 |
Size: | 2542 x 1629 px |
About the Object
Name: | Gemini North, Maunakea |
Category: | Gemini Observatory |