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Mars : a geologically active planet.

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Mars : a geologically active planet. / Mitchell, Karl L.; Wilson, Lionel.
In: Astronomy and Geophysics, Vol. 44, No. 4, 08.2003, p. 16-20.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Mitchell, KL & Wilson, L 2003, 'Mars : a geologically active planet.', Astronomy and Geophysics, vol. 44, no. 4, pp. 16-20. https://doi.org/10.1046/j.1468-4004.2003.44416.x

APA

Mitchell, K. L., & Wilson, L. (2003). Mars : a geologically active planet. Astronomy and Geophysics, 44(4), 16-20. https://doi.org/10.1046/j.1468-4004.2003.44416.x

Vancouver

Mitchell KL, Wilson L. Mars : a geologically active planet. Astronomy and Geophysics. 2003 Aug;44(4):16-20. doi: 10.1046/j.1468-4004.2003.44416.x

Author

Mitchell, Karl L. ; Wilson, Lionel. / Mars : a geologically active planet. In: Astronomy and Geophysics. 2003 ; Vol. 44, No. 4. pp. 16-20.

Bibtex

@article{e2907348cbbd44b2ba4b0762baf3e4bc,
title = "Mars : a geologically active planet.",
abstract = "Recent and continuing missions to Mars are showing that the Red Planet may be more geologically active than previously thought. Volcanoes and erosion by running water have shaped the surface. And evidence is growing that fluvial and possibly volcanic processes have been active in the very recent past.",
author = "Mitchell, {Karl L.} and Lionel Wilson",
year = "2003",
month = aug,
doi = "10.1046/j.1468-4004.2003.44416.x",
language = "English",
volume = "44",
pages = "16--20",
journal = "Astronomy and Geophysics",
issn = "1366-8781",
publisher = "Oxford University Press",
number = "4",

}

RIS

TY - JOUR

T1 - Mars : a geologically active planet.

AU - Mitchell, Karl L.

AU - Wilson, Lionel

PY - 2003/8

Y1 - 2003/8

N2 - Recent and continuing missions to Mars are showing that the Red Planet may be more geologically active than previously thought. Volcanoes and erosion by running water have shaped the surface. And evidence is growing that fluvial and possibly volcanic processes have been active in the very recent past.

AB - Recent and continuing missions to Mars are showing that the Red Planet may be more geologically active than previously thought. Volcanoes and erosion by running water have shaped the surface. And evidence is growing that fluvial and possibly volcanic processes have been active in the very recent past.

U2 - 10.1046/j.1468-4004.2003.44416.x

DO - 10.1046/j.1468-4004.2003.44416.x

M3 - Journal article

VL - 44

SP - 16

EP - 20

JO - Astronomy and Geophysics

JF - Astronomy and Geophysics

SN - 1366-8781

IS - 4

ER -