RUS  ENG JOURNALS   PEOPLE   ORGANISATIONS   CONFERENCES   SEMINARS   VIDEO LIBRARY   PACKAGE AMSBIB
General information
Latest issue
Forthcoming papers
Archive
Impact factor
Subscription
Guidelines for authors
Submit a manuscript

Search papers
Search references

RSS
Latest issue
Current issues
Archive issues
What is RSS



UFN:
Year:
Volume:
Issue:
Page:
Find






Personal entry:
Login:
Password:
Save password
Enter
Forgotten password?
Register


UFN, 2005, Volume 175, Number 7, Pages 767–777 (Mi ufn202)  

This article is cited in 11 scientific papers (total in 11 papers)

INSTRUMENTS AND METHODS OF INVESTIGATION

Deep Impact experiment: possible observable effects

B. A. Klumova, V. V. Kimb, I. V. Lomonosovb, V. G. Sultanovb, A. V. Shutovb, V. E. Fortovc

a Max Planck Institute for Extraterrestrial Physics
b Institute of Problems of Chemical Physics, Russian Academy of Sciences
c Institute of Extremal States Thermophysics, Scientific Association for High Temperatures, Russian Academy of Sciences

Abstract: A hypervelocity collision of a metal impactor and the nucleus of the Tempel 1 comet is to be carried out in July 2005 in the framework of the Deep Impact active experiment in space. This paper discusses certain observable consequences of this impact. Numerical simulation of the impact process made it possible to evaluate the diameter of the impact-produced crater as a function of the initial density and porosity of the cometary nucleus. A substantial part of the shockwave-compressed cometary material that is evaporated at the unloading stage may become heated to temperatures on the order of $(1-2)\times 10^4$ K. A change in the chemical composition of the hot vapor in the process of its expansion was computed using a model elemental composition of the cometary nucleus; this may prove useful for determining the parameters of the flash induced by the impact in the visible optical, UV, IR, and radio wavelength bands.

DOI: https://doi.org/10.3367/UFNr.0175.200507f.0767

Full text: PDF file (3080 kB)
Full text: http://www.ufn.ru/.../f
References: PDF file   HTML file

English version:
Physics–Uspekhi, 2005, 48:7, 733–742

Bibliographic databases:

PACS: 47.40.-x, 62.50.+p, 82.20.Wt, 96.35.-j, 96.50.Gn
Received: June 7, 2005

Citation: B. A. Klumov, V. V. Kim, I. V. Lomonosov, V. G. Sultanov, A. V. Shutov, V. E. Fortov, “Deep Impact experiment: possible observable effects”, UFN, 175:7 (2005), 767–777; Phys. Usp., 48:7 (2005), 733–742

Citation in format AMSBIB
\Bibitem{KluKimLom05}
\by B.~A.~Klumov, V.~V.~Kim, I.~V.~Lomonosov, V.~G.~Sultanov, A.~V.~Shutov, V.~E.~Fortov
\paper Deep Impact experiment: possible observable effects
\jour UFN
\yr 2005
\vol 175
\issue 7
\pages 767--777
\mathnet{http://mi.mathnet.ru/ufn202}
\crossref{https://doi.org/10.3367/UFNr.0175.200507f.0767}
\adsnasa{http://adsabs.harvard.edu/cgi-bin/bib_query?2005PhyU...48..733K}
\transl
\jour Phys. Usp.
\yr 2005
\vol 48
\issue 7
\pages 733--742
\crossref{https://doi.org/10.1070/PU2005v048n07ABEH004489}
\isi{http://gateway.isiknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&DestLinkType=FullRecord&DestApp=ALL_WOS&KeyUT=000233309400005}


Linking options:
  • http://mi.mathnet.ru/eng/ufn202
  • http://mi.mathnet.ru/eng/ufn/v175/i7/p767

    SHARE: VKontakte.ru FaceBook Twitter Mail.ru Livejournal Memori.ru


    Citing articles on Google Scholar: Russian citations, English citations
    Related articles on Google Scholar: Russian articles, English articles

    This publication is cited in the following articles:
    1. S. V. Bulychev, D. V. Vyalykh, A. E. Dubinov, I. L. L’vov, S. A. Sadovoǐ, V. D. Selemir, “Generating cumulative jets on the surface of granular medium”, Dokl Phys, 51:9 (2006), 486  crossref  adsnasa  isi  elib  scopus
    2. Kim V.V., Fortov V.E., Lomonosov I.V., Matveichev A.V., Ostrik A.V., “3D computer modeling of high-velocity impact phenomena”, Shock Compression of Condensed Matter - 2005, AIP Conference Proceedings, 845, no. 1&2, 2006, 327–330  crossref  adsnasa  isi  scopus
    3. Sultanov V.G., Kim V.V., Lomonosov I.V., Shutov A.V., Fortov V.E., “Numerical modelling of deep impact experiment”, Shock Compression of Condensed Matter, AIP Conference Proceedings, 955, 2007, 1413–1416  adsnasa  isi
    4. Sultanov, VG, “Numerical modeling of Deep Impact experiment”, International Journal of Impact Engineering, 35:12 (2008), 1816  crossref  isi  scopus
    5. Berezhnoy, AA, “Impacts as sources of the exosphere on Mercury”, Icarus, 195:2 (2008), 511  crossref  adsnasa  isi  elib  scopus
    6. Ostrik A.V., “Method of Finite-Dimension Particles in the Cell for Numerical Modeling of High-Velocity Interaction of Heterogeneous Bodies”, Russ. J. Phys. Chem. B, 2:4 (2008), 643–649  crossref  isi  elib  scopus
    7. Klumov B.A., Morfill G.E., “Structural properties of complex (dusty) plasma upon crystallization and melting”, JETP Letters, 90:6 (2009), 444–448  mathnet  crossref  adsnasa  isi  scopus
    8. L. V. Ksanfomality, “Disintegration of comet nuclei”, Phys. Usp., 55:2 (2012), 137–146  mathnet  crossref  crossref  adsnasa  isi  elib  elib
    9. V. V. Emel'yanenko, B. M. Shustov, “The Chelyabinsk event and the asteroid-comet hazard”, Phys. Usp., 56:8 (2013), 833–836  mathnet  crossref  crossref  adsnasa  isi  elib
    10. M. F. Ivanov, A. D. Kiverin, B. A. Klumov, V. E. Fortov, “From combustion and detonation to nitrogen oxides”, Phys. Usp., 57:3 (2014), 234–249  mathnet  crossref  crossref  adsnasa  isi  elib  elib
    11. Berezhnoy A.A., “Chemistry of Impact Events on Mercury”, Icarus, 300 (2018), 210–222  crossref  isi  scopus
  • Успехи физических наук Physics-Uspekhi
    Number of views:
    This page:321
    Full text:69
    References:57
    First page:1

     
    Contact us:
     Terms of Use  Registration  Logotypes © Steklov Mathematical Institute RAS, 2019