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Experimental studies of sublimation of highly volatile ices in relevance to the ices of the solar system

Identyfikatory
Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
Studies of sublimation of complex ices prepared by deposition of gaseous CO, CH4, N2, and NH3 molecules on a cold plate have been performed. The low pressure and low temperature system was used: 10−9–10−5 mbar and the lowermost temperature 10 K. Diagnostic of composition of evaporates (at an actual temperature) was done by means of the mass spectrometer. The latter allowed following simultaneously the partial pressure of five different ions or radicals escaping from the substrate. It has been found that highly volatile molecules that were used simultaneously with the low volatile ones to form the complex ices (mixtures or clathrates) present a different sublimation pattern than the sublimation of pure high-volatile ices. In particular, the high-volatile component sublimes at two or even three different temperature regimes: At low temperature that is typical for sublimation of this component, as well as at much higher temperatures. This effect seems to be important when degassing and outbursts from cometary nuclei are considered. It can be also important for modeling of cryovolcanic processes on the icy satellites.
Słowa kluczowe
Czasopismo
Rocznik
Strony
1304--1321
Opis fizyczny
Bibliogr. 23 poz.
Twórcy
  • University of Warsaw, Institute of Geophysics, Warsaw, Poland
autor
  • Polytechnic University of Valencia, Department of Applied Physics, Alcoy, Spain
Bibliografia
  • 1. Bockelée-Morvan, D., J. Crovisier, M.J. Mumma, and H.A. Weaver (2004), The composition of cometary volatiles. In: M.C. Festou, H.U. Keller, H.A. Weaver (eds.), Comets II, University of Arizona, Tucson, 391–423.
  • 2. Byrne, S., C.M. Dundas, M.R. Kennedy, M.T. Mellon, A.S. McEwen, S.C. Cull, I.J. Daubar, D.E. Shean, K.D. Seelos, S.L. Murchie, B.A. Cantor, R.E. Arvidson, K.S. Edgett, A. Reufer, N. Thomas, T.N. Harrison, L.V. Posiolova, and F.P. Seelos (2009), Distribution of mid-latitude ground ice on Mars from new impact craters, Science 325,5948, 1674–1676, DOI: 10.1126/science.1175307.
  • 3. Campins, H., K. Hargrove, N. Pinilla-Alonso, E.S. Howell, M.S. Kelley, J. Licandro, T. Mothé-Diniz, Y. Fernandez, and J. Ziffer (2010), Water ice and organics on the surface of the asteroid 24 Themis, Nature 464,7293, 1320–1321, DOI: 10.1038/nature09029.
  • 4. Crotts, A. (2011), Water on the Moon, I. Historical overview, Astron. Rev. 6,8, 4–20.
  • 5. Fortes, A.D., and M. Choukroun (2010), Phase behaviour of ices and hydrates, Space Sci. Rev. 153,1–4, 185–218, DOI: 10.1007/s11214-010-9633-3.
  • 6. Fray, N., and B. Schmitt (2009), Sublimation of ices of astrophysical interest: A bibliographic review, Planet. Space Sci. 57,14–15, 2053–2080, DOI: 10.1016/ j.pss.2009.09.011.
  • 7. Gronkowski, P., and Z. Sacharczuk (2010), Cometary outbursts — a search for a cause of the comet 17P/Holmes outburst, Mon. Not. Roy. Astron. Soc. 408,2, 1207–1215, DOI: 10.1111/j.1365-2966.2010.17194.x.
  • 8. Gronkowski, P., Z. Sacharczuk, and S. Topolewicz (2011), Features of a comet nucleus: The case of 103P/Hartley 2, Astron. Nachr. 332,8, 785–794, DOI: 10.1002/asna.201111585.
  • 9. Hand, K.P., C.F. Chyba, R.W. Carlson, and J.F. Cooper (2006), Clathrate hydrates of oxidants in the ice shell of Europa, Astrobiology 6,3, 463–482, DOI: 10.1089/ast.2006.6.463.
  • 10. Hersant, F., D. Gautier, and J.I. Lunine (2004), Enrichment in volatiles in the giant planets of the Solar System, Planet. Space Sci. 52,7, 623–641, DOI: 10.1016/j.pss.2003.12.011.
  • 11. Hsieh, H.H. (2010), Asteroids: A frosty finding, Nature 464,7293, 1286–1287, DOI: 10.1038/4641286a.
  • 12. Jewitt, D., C.A. Garland, and H. Aussel (2008), Deep search for carbon monoxide in cometary precursors using millimeter wave spectroscopy, Astronom. J. 135,1, 400–407, DOI: 10.1088/0004-6256/135/1/400.
  • 13. Kossacki, K.J., and S. Szutowicz (2011), Comet 17P/Holmes: Possibility of a CO driven explosion, Icarus 212,2, 847–857, DOI: 10.1016/j.icarus.2011.01.007.
  • 14. Leliwa-Kopystyński, J., M. Maruyama, and T. Nakajima (2002), The waterammonia phase diagram up to 300 MPa: Application to icy satellites, Icarus 159,2, 518–528, DOI: 10.1006/icar.2002.6932.
  • 15. Luna, R., C. Millán, M. Domingo, and M.Á. Satorre (2008), Thermal desorption of CH4 retained in CO2 ice, Astrophys. Space. Sci. 314,1–3, 113–119, DOI: 10.1007/s10509-008-9746-2.
  • 16. Lunine, J.I., and D.J. Stevenson (1987), Clathrate and ammonia hydrates at high pressure: Application to the origin of methane on Titan, Icarus 70,1, 61–77, DOI: 10.1016/0019-1035(87)90075-3.
  • 17. Marboeuf, U., O. Mousis, J.M. Petit, and B. Schmitt (2010), Clathrate hydrates formation in short-period comets, Astrophys. J. 708,1, 812–826, DOI: 10.1088/0004-637X/708/1/812.
  • 18. Moses, J.I., K. Rawlins, K. Zahnle, and L. Dones (1999), External sources of water for Mercury’s putative ice deposits, Icarus 137,2, 197–221, DOI: 10.1006/icar.1998.6036.
  • 19. Richardson, M.I., and R.J. Wilson (2002), Investigation of the nature and stability of the Martian seasonal water cycle with a general circulation model, J. Geophys. Res. 107,E5, 7-1–7-28, DOI: 10.1029/2001je001536.
  • 20. Roush, T.L. (2001), Physical state of ices in the outer solar system, J. Geophys. Res. 106,E12, 33315–33323, DOI: 10.1029/2000JE001334.
  • 21. Rivkin, A.S., and J.P. Emery (2010), Detection of ice and organics on an asteroidal surface, Nature 464,7293, 1322–1323, DOI: 10.1038/nature09028.
  • 22. Vasavada, A.R., D.A. Paige, and S.E. Wood (1999), Near-surface temperatures on Mercury and the Moon and the stability of polar ice deposits, Icarus 141,2, 179–193, DOI: 10.1006/icar.1999.6175.
  • 23. Zheligovskaya, E.A., and G.G. Malenkov (2006), Crystalline water ices, Russ. Chem. Rev. 75,1, 57–76, DOI: 10.1070/RC2006v075n01ABEH001184.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-f13d3d3c-1055-4113-85c5-4c0de35e00e3
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