Can we make a star on Earth [videorecording] / directed and produced by Gideon Bradshaw ; a BBC/Science Channel Co-production

Contributor(s): Publication details: London : BBC, 2009Description: 1 videodisc (50 min.) : sd., col., ; 4 3/4 inSubject(s): Production credits:
  • Camera, Kevin White ; sound, George McMillan ; production coordinator, Donna Dixon ; editor, Martin Johnson
Summary: Nuclear fusion has kept our Sun burning for five billion years. Might it be harnessed here on Earth as an energy source? This program illustrates the race to create artificial stars that can ensure humanity's earthbound survival. Several facilities and projects are profiled-including the Joint European Torus, or JET, which initiates nuclear fusion at a rate far higher than that inside the Sun; a bigger version of JET known as ITER, now under construction in southern France; an American approach known as inertial fusion underway at the National Ignition Facility in California; and the so-called Z-Machine in New Mexico, designed to produce astronomically high temperatures and, possibly, the birth of a star-like object
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MEDIA PERPUSTAKAAN TUN SERI LANANG PERPUSTAKAAN TUN SERI LANANG MEDIA-P. TUN SERI LANANG (ARAS 2) dvd QC791.73 .C365 (Browse shelf(Opens below)) 1 Available 00002041262

Camera, Kevin White ; sound, George McMillan ; production coordinator, Donna Dixon ; editor, Martin Johnson

Nuclear fusion has kept our Sun burning for five billion years. Might it be harnessed here on Earth as an energy source? This program illustrates the race to create artificial stars that can ensure humanity's earthbound survival. Several facilities and projects are profiled-including the Joint European Torus, or JET, which initiates nuclear fusion at a rate far higher than that inside the Sun; a bigger version of JET known as ITER, now under construction in southern France; an American approach known as inertial fusion underway at the National Ignition Facility in California; and the so-called Z-Machine in New Mexico, designed to produce astronomically high temperatures and, possibly, the birth of a star-like object

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