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Modelling of Lunar Effusive and Intrusive Domes

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Lunar Domes

Part of the book series: Springer Praxis Books ((ASTRONOMY))

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Abstract

This chapter describes how the dimensions of the dikes through which the dome-forming magma ascended to the surface can be modelled. Furthermore, a modelling approach to encompass the physical conditions under which putative intrusive lunar domes were formed is outlined.

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Authors and Affiliations

  1. via Cartesio 144, 00137, Roma, Italy

    Raffaello Lena

  2. Faculty of Electrical Engineering and Information Technology Image Analysis Group, TU Dortmund University, Otto-Hahn 4, Dortmund, 44227, Germany

    Christian Wöhler

  3. Bull St. 101, 29401, Charleston, USA

    James Phillips

  4. Via Martiri della Liberazione 4, 16043, Chiavari, Italy

    Maria Teresa Chiocchetta

Authors
  1. Raffaello Lena
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  2. Christian Wöhler
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  3. James Phillips
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  4. Maria Teresa Chiocchetta
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Corresponding author

Correspondence to Raffaello Lena .

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© 2013 Springer-Verlag Italia

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Lena, R., Wöhler, C., Phillips, J., Chiocchetta, M. (2013). Modelling of Lunar Effusive and Intrusive Domes. In: Lunar Domes. Springer Praxis Books(). Springer, Milano. https://doi.org/10.1007/978-88-470-2637-7_4

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