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Understanding The Nature Of Turbulence Gases In Planet-forming Protoplanetary Disks
2013-04-03 11:15:12

University of Tennessee's National Institute for Computational Sciences Many newly formed stars are surrounded by what are called protoplanetary disks, swirling masses of warm dust and gas that can constitute the core of a developing solar system. Proof of the existence of such disks didn´t come until 1994, when the Hubble telescope examined young stars in the Orion Nebula. Protoplanetary disks may potentially become celestial bodies such as planets and asteroids. But just how they...


Word of the Day
reremouse
  • A bat.
The word 'reremouse' comes from Middle English reremous, from Old English hrēremūs, hrērmūs ("bat"), equivalent to rear (“to move, shake, stir”) +‎ mouse.
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