k Dark Matter Signature of dark matter. First in a series of three colourcoded images showing a possible gravitational lensing event by a brown dwarf star in the halo around our galaxy. The arrow points to a star in the Large Magellanic Cloud LMC before the lensing event. A brown dwarf is a type of starlike object too small to burn, and is thus almost invisible, but still has a gravitational field strong enough to act as a lens. As a type of MACHO Massive Compact Halo Object it could help account for the missing dark matter which should make up about 90 of the mass of the Universe. Compare with R670045 and R670046. Editorial Stock Photo - Afloimages
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Dark Matter Signature of dark matter. First in a series of three colour coded images showing a possible gravitational lensing event by a brown dwarf star in the halo around our galaxy. The arrow points to a star in the Large Magellanic Cloud  LMC  before the lensing event. A brown dwarf is a type of star like object too small to  burn , and is thus almost invisible, but still has a gravitational field strong enough to act as a lens. As a type of MACHO  Massive Compact Halo Object  it could help account for the missing  dark matter  which should make up about 90  of the mass of the Universe. Compare with R670 045 and R670 046.
ED

Dark Matter

Signature of dark matter. First in a series of three colour-coded images showing a possible gravitational lensing event by a brown dwarf star in the halo around our galaxy. The arrow points to a star in the Large Magellanic Cloud (LMC) before the lensing event. A brown dwarf is a type of star-like object too small to 'burn', and is thus almost invisible, but still has a gravitational field strong enough to act as a lens. As a type of MACHO (Massive Compact Halo Object) it could help account for the missing 'dark matter' which should make up about 90% of the mass of the Universe. Compare with R670/045 and R670/046.

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ID
10628191

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License type
Editorial

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Creation date
22-11-2010

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