File:Artist's impression of Beta Pictoris.jpg
From Infogalactic: the planetary knowledge core
![File:Artist's impression of Beta Pictoris.jpg](/w/images/thumb/4/46/Artist%27s_impression_of_Beta_Pictoris.jpg/800px-Artist%27s_impression_of_Beta_Pictoris.jpg)
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Summary
This artist's concept illustrates the preferred model for explaining ALMA observations of Beta Pictoris. The new observations from ALMA now show that the disc around the star is permeated by carbon monoxide gas. The presence of carbon monoxide could indicate that the Beta Pictoris planetary system may eventually become a good habitat for life. At the outer fringes of the system, the gravitational influence of a hypothetical giant planet (bottom left) captures comets into a dense, massive swarm (right) where frequent collisions occur.
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 20:17, 30 September 2017 | ![]() | 3,839 × 2,160 (2.52 MB) | Thales (talk | contribs) | This artist's concept illustrates the preferred model for explaining ALMA observations of Beta Pictoris. The new observations from ALMA now show that the disc around the star is permeated by carbon monoxide gas. The presence of carbon monoxide could in... |
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