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How Were the Comets Made? Explaining the composition of these 4.5 billion-year-old relics may require scientists to revise their models of the primitive solar nebula
Joseph A. Nuth III
Vol. 89, No. 3 (MAY-JUNE 2001), pp. 228-235
Published by: Sigma Xi, The Scientific Research Society
Stable URL: http://www.jstor.org/stable/27857469
Page Count: 8
You can always find the topics here!Topics: Comets, Solar nebulae, Silicates, Nebulae, Olivine, Materials, Accretion disks, Dust grain, Stars, Chemical composition
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American Scientist © 2001 Sigma Xi, The Scientific Research Society