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Page 267
This could have been caused by gas production from the ejecta dust grains themselves . By just one full rotation period after impact ( 41 hours ) , the coma morphology had returned to its pre - impact state , which suggests that the ...
This could have been caused by gas production from the ejecta dust grains themselves . By just one full rotation period after impact ( 41 hours ) , the coma morphology had returned to its pre - impact state , which suggests that the ...
Page 273
If the new source has reached steady production by 20 min after impact , we expect the effective production rate to be a fair estimate of the true value ( the true rate is likely to be larger by a factor up to about 1.6 , i.e. , 1 / 2 ) ...
If the new source has reached steady production by 20 min after impact , we expect the effective production rate to be a fair estimate of the true value ( the true rate is likely to be larger by a factor up to about 1.6 , i.e. , 1 / 2 ) ...
Page 281
The cyanide - to - water production ratio was slightly enhanced in the impact cloud , compared with that of normal comet activity . Dust particles were flowing outward in the coma at > 160 meters per second , accelerated by the gas .
The cyanide - to - water production ratio was slightly enhanced in the impact cloud , compared with that of normal comet activity . Dust particles were flowing outward in the coma at > 160 meters per second , accelerated by the gas .
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Bibliographic information
| Title | Science, Volume 310, Issues 5745-5750 |
| Editor | John Michels (Journalist) |
| Contributor | American Association for the Advancement of Science |
| Published | 2005 |
| Original from | University of Minnesota |
| Digitized | 23 Jan 2018 |
| Export Citation | BiBTeX EndNote RefMan |