Brunsell 's personal annotations on this page
Brunsell bookmarked
on 2009-09-08
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Dark matter and normal matter have been wrenched apart by the tremendous collision of two large clusters of galaxies. The galaxies are observed in the optical (shown in orange and white). Most of the normal mass in the clusters (pink) is associated with gas heated in their collision. Dark matter is not visible, but is inferred (blue) from gravitational lensing effects
This link has been bookmarked by 2 people . It was first bookmarked on 08 Sep 2009, by Brunsell.
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A whopping 96% of the essence of our universe lies in the dark sector, where essence refers to everything that controls evolution and large-scale properties of the cosmos. Dark matter is unseen matter -- unseen in the sense that it emits no detected electromagnetic radiation (light, radio waves, etc) -- but it has been definitively spotted nonetheless because its gravity has measurable effects on stars, things that we can see.
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Dark energy, on the other hand, is not a form of matter at all (nor is it literally "dark" -- that is just a poetic way of saying that it is mysterious). It is the source of the outward acceleration of the cosmos, and, based on reasonable assumptions about our current understanding of elementary particle physics, may arise from the vacuum, which has quantum properties that provide energy to the cosmos. Alternatively, dark energy may be a feature of gravity that produces cosmic repulsion on a large scale.
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Dark matter and normal matter have been wrenched apart by the tremendous collision of two large clusters of galaxies. The galaxies are observed in the optical (shown in orange and white). Most of the normal mass in the clusters (pink) is associated with gas heated in their collision. Dark matter is not visible, but is inferred (blue) from gravitational lensing effects
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