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Submitted on 1 Jan 1987
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FORMATION AND DECOMPOSITION OF ICY CLATHRATES
R. Smoluchowski
To cite this version:
R. Smoluchowski. FORMATION AND DECOMPOSITION OF ICY CLATHRATES. Journal de
Physique Colloques, 1987, 48 (C1), pp.C1-687-C1-688. �10.1051/jphyscol:19871109�. �jpa-00226250�
JOURNAL DE PHYSIQUE
C o l l o q u e
C1,s u p p l e m e n t au n o 3, Tome 48, m a r s 1987
FORMATION
ANDDECOMPOSITION O F I C Y CLATHRATES
R. SMOLUCHOWSKI
University of Texas, Austin, TX 78712, U.S.A.
A b s t r a c t
:R e c e n t e x p e r i m e n t a l s t u d i e s (1) o f t h e f o r m a t i o n and decomposition of CD2 - c l a t h r a t e s , from and i n t o H e i c e and m,
seemto indicate
an extremely low apparent a c t i v a t i o n energy (2) f o r t h e s e processes. A rough estimate of t h e probable energy associated with volume diffusion of (332 molecule through hexagonal openings i n the c l a t h r a t e cage has been made. It suggests t h a t these reactions occur primarily on surfaces of ice grains. The observed suppression of decomposition of c l a t h r a t e s by pressure (3) is i n q u a l i t a t i v e agreement with these conclusions. These and e a r l i e r r e s u l t s (4) indicate t h a t porosity of cometary n u c l e i should play an important r o l e i n a f f e c t i n g t h e r a t e of escape of t h e entrapped m l e c u l e s i n t o t h e cometary
coma.References
(1) Davidson D.W. e t al;, J. Incl. Phen., 2, (1984), 231.
(2) Smluchowski R.,
EXXNov. 12 (1985) .
(3) Davidson D.W. e t dl., t o appear i n Geochem. C o m h e m . A c t a .
(4) Klinger J. e t al., t o appear i n Astroroids, Comets and Meteors, Uppsala (1985).
COMMENTS
Name of Speaker :E. WHALLEY for SMOLUCHOWSKI
Relative to Prof. Glen's request for comment on formation of the empty clathrate hydrate, I believe that non polar guest molecules in thin deposite offer the hope of seeing this in the
#120 K range. We have observed that warming of a 6 micron thick H2S hydrate into the 140 K range causes the HOD 0-D stretch band to move to a position between the
nr2925 c m ' l hydrate value and the 2410 cm-I ice value (10K values). However, the sharpness of the band resembled ice Ic and leads us to believe it was not the empty clathrate structure.
Name of Speaker :E. WHALLEY for SMOLUCHOWSKI
Is it known what happens to a clathrate hydrate when it is cooled to a low temperature and then placed in a low-pressure environnement
?Do the guest molecules leave
?If so what happens to t'ne cage structure
?Does it survive in the same way as the high presure phases of ice at low temperature
?If not does it become amorphous
?Does this not have important implications for the behaviour of clathrates in astrophysical situations such as those discussed by Dr. Smoluchowski
?If the cage does survive it might be most interesting to measure its thermal
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:19871109
C1-688