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The dispersal of pyroclasts from Apollinaris Patera, Mars: implications for the origin of the Medusae Fossae Formation.

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The dispersal of pyroclasts from Apollinaris Patera, Mars: implications for the origin of the Medusae Fossae Formation. / Kerber, Laura; Head, James; Madeleine, Jean-Baptiste et al.
In: Icarus, Vol. 216, No. 1, 11.2011, p. 212-220.

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Kerber L, Head J, Madeleine J-B, Forget F, Wilson L. The dispersal of pyroclasts from Apollinaris Patera, Mars: implications for the origin of the Medusae Fossae Formation. Icarus. 2011 Nov;216(1):212-220. doi: 10.1016/j.icarus.2011.07.035

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Kerber, Laura ; Head, James ; Madeleine, Jean-Baptiste et al. / The dispersal of pyroclasts from Apollinaris Patera, Mars: implications for the origin of the Medusae Fossae Formation. In: Icarus. 2011 ; Vol. 216, No. 1. pp. 212-220.

Bibtex

@article{60f8643d236a4cfb8419aa4ac8685d9c,
title = "The dispersal of pyroclasts from Apollinaris Patera, Mars: implications for the origin of the Medusae Fossae Formation.",
abstract = "The Medusae Fossae Formation (MFF) has long been thought to be of Amazonian age, but recent studies propose that a significant part of its emplacement occurred in the Hesperian and that many of the Amazonian ages represent modification (erosional and redepositional) ages. On the basis of the new formational age, we assess the hypothesis that explosive eruptions from Apollinaris Patera might have been the source of the Medusae Fossae Formation. In order to assess the likelihood of this hypothesis, we examine stratigraphic relationships between Apollinaris Patera and the MFF and analyze the relief of the MFF using topographic data. We predict the areal distribution of tephra erupted from Apollinaris Patera using a Mars Global Circulation Model (GCM) combined with a semi-analytical explosive eruption model for Mars, and compare this with the distribution of the MFF. We conclude that Apollinaris Patera could have been responsible for the emplacement of the Medusae Fossae Formation.",
keywords = "Volcanism, Mars , Geological processes , Mars, Surface , Mars, Atmosphere",
author = "Laura Kerber and James Head and Jean-Baptiste Madeleine and Fran{\c c}ois Forget and Lionel Wilson",
year = "2011",
month = nov,
doi = "10.1016/j.icarus.2011.07.035",
language = "English",
volume = "216",
pages = "212--220",
journal = "Icarus",
issn = "0019-1035",
publisher = "ELSEVIER ACADEMIC PRESS INC",
number = "1",

}

RIS

TY - JOUR

T1 - The dispersal of pyroclasts from Apollinaris Patera, Mars: implications for the origin of the Medusae Fossae Formation.

AU - Kerber, Laura

AU - Head, James

AU - Madeleine, Jean-Baptiste

AU - Forget, François

AU - Wilson, Lionel

PY - 2011/11

Y1 - 2011/11

N2 - The Medusae Fossae Formation (MFF) has long been thought to be of Amazonian age, but recent studies propose that a significant part of its emplacement occurred in the Hesperian and that many of the Amazonian ages represent modification (erosional and redepositional) ages. On the basis of the new formational age, we assess the hypothesis that explosive eruptions from Apollinaris Patera might have been the source of the Medusae Fossae Formation. In order to assess the likelihood of this hypothesis, we examine stratigraphic relationships between Apollinaris Patera and the MFF and analyze the relief of the MFF using topographic data. We predict the areal distribution of tephra erupted from Apollinaris Patera using a Mars Global Circulation Model (GCM) combined with a semi-analytical explosive eruption model for Mars, and compare this with the distribution of the MFF. We conclude that Apollinaris Patera could have been responsible for the emplacement of the Medusae Fossae Formation.

AB - The Medusae Fossae Formation (MFF) has long been thought to be of Amazonian age, but recent studies propose that a significant part of its emplacement occurred in the Hesperian and that many of the Amazonian ages represent modification (erosional and redepositional) ages. On the basis of the new formational age, we assess the hypothesis that explosive eruptions from Apollinaris Patera might have been the source of the Medusae Fossae Formation. In order to assess the likelihood of this hypothesis, we examine stratigraphic relationships between Apollinaris Patera and the MFF and analyze the relief of the MFF using topographic data. We predict the areal distribution of tephra erupted from Apollinaris Patera using a Mars Global Circulation Model (GCM) combined with a semi-analytical explosive eruption model for Mars, and compare this with the distribution of the MFF. We conclude that Apollinaris Patera could have been responsible for the emplacement of the Medusae Fossae Formation.

KW - Volcanism

KW - Mars

KW - Geological processes

KW - Mars, Surface

KW - Mars, Atmosphere

U2 - 10.1016/j.icarus.2011.07.035

DO - 10.1016/j.icarus.2011.07.035

M3 - Journal article

VL - 216

SP - 212

EP - 220

JO - Icarus

JF - Icarus

SN - 0019-1035

IS - 1

ER -