File:Eso0204b.jpg

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English: Io, the volcanic moon of Jupiter, as imaged with the VLT NAOS-CONICA Adaptive Optics instrument on 5 December 2001, through a near-infrared, narrow optical filter (Brackett-gamma at wavelength 2.166 \xc2\xb5m). Despite the small angular diameter of Io, about 1.2 arcsec, many features are visible at this excellent optical resolution.
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Source http://www.eso.org/public/images/eso0204b/
Author European Southern Observatory

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Date/TimeThumbnailDimensionsUserComment
current12:53, 4 January 2020Thumbnail for version as of 12:53, 4 January 2020602 × 621 (43 KB)BevinKacon (talk | contribs)Cropped 25 % horizontally, 24 % vertically using CropTool with lossless mode. tighter crop, no data in black area
12:45, 4 January 2020Thumbnail for version as of 12:45, 4 January 2020800 × 820 (43 KB)BevinKacon (talk | contribs)actual size from source
04:46, 1 October 2015Thumbnail for version as of 04:46, 1 October 20151,280 × 1,312 (53 KB)8a jhon mario (talk | contribs)=={{int:filedesc}}== {{Information|description={{en|1= Io, the volcanic moon of Jupiter, as imaged with the VLT NAOS-CONICA Adaptive Optics instrument on 5 December 2001, through a near-infrared, narrow optical filter (Brackett-gamma at wavelength 2.16...
04:30, 1 October 2015Thumbnail for version as of 04:30, 1 October 20151,280 × 1,312 (53 KB)8a jhon mario (talk | contribs)=={{int:filedesc}}== {{Information|description={{en|1= Io, the volcanic moon of Jupiter, as imaged with the VLT NAOS-CONICA Adaptive Optics instrument on 5 December 2001, through a near-infrared, narrow optical filter (Brackett-gamma at wavelength 2.16...

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