File:New Camera at WIYN images an Asteroid with a Long Tail (noao1307e).tiff

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New_Camera_at_WIYN_images_an_Asteroid_with_a_Long_Tail_(noao1307e).tiff (284 × 445 pixels, file size: 70 KB, MIME type: image/tiff)

Captions

Captions

R band profiles from Keck (top: Jewitt et al. 2012) and pODI (bottom). The shape and extent of the tail are controlled by the ratio of radiation pressure to gravitational accelaeration, and the ejection velocity.

Summary

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Description
English: R band profiles from Keck (top: Jewitt et al. 2012) and pODI (bottom). The shape and extent of the tail are controlled by the ratio of radiation pressure to gravitational accelaeration, and the ejection velocity. Hence the profile yields the particle size distributiona and mass in the tail. As seen here, from the pODI image we are able to sample the profile out to much longer distances (> 15') from the nucleus.
Date 4 June 2013 (upload date)
Source New Camera at WIYN images an Asteroid with a Long Tail
Author NOIRLab
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current18:16, 23 October 2023Thumbnail for version as of 18:16, 23 October 2023284 × 445 (70 KB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/original/noao1307e.tif via Commons:Spacemedia

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