File:41Daphne-Keck.jpg

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41Daphne-Keck.jpg(149 × 123 pixels, file size: 2 KB, MIME type: image/jpeg)

File information
Description

41 Daphne and satellite as seen using Adaptive optics (AO) on the W.M. Keck II telescope in 2008.

Source

Lunar and Planetary Institute website: Discovery of an Extreme Mass-Ratio Satellite of (41) Daphne in a Close Orbit

Date

2008

Author

W. M. Keck Observatory

Permission
(Reusing this file)

Fair use

This image qualifies for fair use in the articles 41 Daphne since:

1) Illustrates the discovery and significance of binary asteroids.
2) No freely available alternative to this unique image since Adaptive optics are beyond the means of most telescopes, and thus not easily reproducible.
3) Does not make the work as a whole less valuable to the copyright holder since the image was created for scientific purposes.

For commercial use of this image please contact Keck Observatory at http://keckobservatory.org/contact


File history

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Date/TimeThumbnailDimensionsUserComment
current17:38, 24 January 2012Thumbnail for version as of 17:38, 24 January 2012149 × 123 (2 KB)Kheider (talk | contribs){{Information |Description=41 Daphne and satellite as seen using Adaptive optics (AO) on the W.M. Keck II telescope in 2008. |Source=Lunar and Planetary Institute website: [http://www.lpi.usra.edu/meetings/acm2008/pd
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