File:Secondary-to-primary mass ratio versus average separation (geminiann08022b).jpg

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Secondary-to-primary_mass_ratio_versus_average_separation_(geminiann08022b).jpg (500 × 377 pixels, file size: 38 KB, MIME type: image/jpeg)

Captions

Captions

Secondary-to-primary mass ratio versus average separation (in units of the primary’s radius). The dashed box represents the known binary asteroids, the largest separation barely exceeds a secondary-to-primary mass ratio of 100.

Summary

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Description
English: Secondary-to-primary mass ratio versus average separation (in units of the primary’s radius). The dashed box represents the known binary asteroids, the largest separation barely exceeds a secondary-to-primary mass ratio of 100. With equal mass and a separation that is more than 2,000 times the radius of each of its components, 2001 QW322 (top right corner) is unique.
Date 28 October 2008, 18:26:00 (upload date)
Source Secondary-to-primary mass ratio versus average separation
Author International Gemini Observatory/NOIRLab/NSF/AURA
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current22:32, 23 October 2023Thumbnail for version as of 22:32, 23 October 2023500 × 377 (38 KB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/large/geminiann08022b.jpg via Commons:Spacemedia

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