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

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