Hostname: page-component-cb9f654ff-nr592 Total loading time: 0 Render date: 2025-09-06T21:03:42.615Z Has data issue: false hasContentIssue false

Changes in the morphology of interstellar ice analogues afterhydrogen atom exposure

Published online by Cambridge University Press:  13 February 2013

E. Congiu
Affiliation:
LERMA-LAMAp, UMR 8112 du CNRS, Observatoire de Paris et Université de Cergy-Pontoise, 5 mail Gay-Lussac, 95000 Cergy Pontoise Cedex, France;. e-mail: econgiu@u-cergy.fr
M. Accolla
Affiliation:
LERMA-LAMAp, UMR 8112 du CNRS, Observatoire de Paris et Université de Cergy-Pontoise, 5 mail Gay-Lussac, 95000 Cergy Pontoise Cedex, France;. e-mail: econgiu@u-cergy.fr DMFCI, Università di Catania, Viale Doria 6, 95125 Catania, Italy
F. Dulieu
Affiliation:
LERMA-LAMAp, UMR 8112 du CNRS, Observatoire de Paris et Université de Cergy-Pontoise, 5 mail Gay-Lussac, 95000 Cergy Pontoise Cedex, France;. e-mail: econgiu@u-cergy.fr
H. Chaabouni
Affiliation:
LERMA-LAMAp, UMR 8112 du CNRS, Observatoire de Paris et Université de Cergy-Pontoise, 5 mail Gay-Lussac, 95000 Cergy Pontoise Cedex, France;. e-mail: econgiu@u-cergy.fr
J.-L. Lemaire
Affiliation:
LERMA-LAMAp, UMR 8112 du CNRS, Observatoire de Paris et Université de Cergy-Pontoise, 5 mail Gay-Lussac, 95000 Cergy Pontoise Cedex, France;. e-mail: econgiu@u-cergy.fr
H. Mokrane
Affiliation:
LERMA-LAMAp, UMR 8112 du CNRS, Observatoire de Paris et Université de Cergy-Pontoise, 5 mail Gay-Lussac, 95000 Cergy Pontoise Cedex, France;. e-mail: econgiu@u-cergy.fr
E. Matar
Affiliation:
LERMA-LAMAp, UMR 8112 du CNRS, Observatoire de Paris et Université de Cergy-Pontoise, 5 mail Gay-Lussac, 95000 Cergy Pontoise Cedex, France;. e-mail: econgiu@u-cergy.fr
G. Manicò
Affiliation:
DMFCI, Università di Catania, Viale Doria 6, 95125 Catania, Italy
V. Pirronello
Affiliation:
DMFCI, Università di Catania, Viale Doria 6, 95125 Catania, Italy

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Interstellar water ice is mainly amorphous, but the nature of its morphology stillremains poorly known. The experimental study described in this work focuses on howrelevant changes of the ice morphology result from atomic hydrogen exposure and subsequentrecombination. We show that there is an exponential decrease in the porosity of theamorphous water ice sample following hydrogen-atom irradiation. These and other laboratoryresults lead us to suggest that water ice in space is almost certainly amorphous andnon-porous (compact).

References

Références

Accolla, M., et al., 2011, Phys. Chem., Chem. Phys., 13 , 8037 Google Scholar
Austen Angell, C., 2004, Annu. Rev. Phys. Chem., 55 , 559 CrossRef
Cuppen, H.M., & Herbst, E., 2007, ApJ, 668 , 294 CrossRef
Hollenbach, D., & Salpeter, E.E., 1971, ApJ, 163 , 155 CrossRef
Jenniskens, P., et al., 1995, ApJ, 455 , 389 CrossRef
Li, D., & Goldsmith, P.F., 2003, ApJ, 585 , 823 CrossRef
Manicò, G., et al., 2001, ApJ, 163 , 155
Oba, Y., et al., 2009, ApJ, 701 , 464 CrossRef
Palumbo, M.E., et al., 2010, J. Mol. Struct., 972 , 64 CrossRef
Palumbo, M.E., 2006, A&A, 453 , 903
Raut, U., et al., 2008, ApJ, 687 , 1070 CrossRef