File:Beta Pictoris system annotated.jpg

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描述 This composite image represents the close environment of Beta Pictoris as seen in near infrared light. This very faint environment is revealed after a very careful subtraction of the much brighter stellar halo. The outer part of the image shows the reflected light on the dust disc, as observed in 1996 with the ADONIS instrument on ESO's 3.6 m telescope; the inner part is the innermost part of the system, as seen at 3.6 microns with NACO on the Very Large Telescope. The newly detected source is more than 1000 times fainter than Beta Pictoris, aligned with the disc, at a projected distance of 8 times the Earth-Sun distance. Both parts of the image were obtained on ESO telescopes equipped with adaptive optics.
日期
来源 https://www.eso.org/public/images/eso0842b/
作者 ESO/A.-M. Lagrange et al.
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其他版本 See [1]. Non-annotated version.

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Composite image of the close environment of Beta Pictoris in near infrared light.

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老人增四

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当前2008年11月24日 (一) 10:222008年11月24日 (一) 10:22版本的缩略图990 × 985​（152 KB）wikimediacommons>MER-C{{Information |Description=This composite image represents the close environment of Beta Pictoris as seen in near infrared light. This very faint environment is revealed after a very careful subtraction of the much brighter stellar halo. The outer part of

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