Home > Research > Publications & Outputs > Volcanism in the Solar System.

Associated organisational unit

View graph of relations

Volcanism in the Solar System.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Published

Standard

Volcanism in the Solar System. / Wilson, Lionel.
In: Nature Geoscience, Vol. 2, No. 6, 06.2009, p. 389-397.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Wilson, L 2009, 'Volcanism in the Solar System.', Nature Geoscience, vol. 2, no. 6, pp. 389-397. https://doi.org/10.1038/ngeo529

APA

Vancouver

Wilson L. Volcanism in the Solar System. Nature Geoscience. 2009 Jun;2(6):389-397. doi: 10.1038/ngeo529

Author

Wilson, Lionel. / Volcanism in the Solar System. In: Nature Geoscience. 2009 ; Vol. 2, No. 6. pp. 389-397.

Bibtex

@article{ad746d5b1cd1432faaa258ac0dc64275,
title = "Volcanism in the Solar System.",
abstract = "The myriad bodies that occur in the Solar System have a wide range of properties, from giant gaseous planets such as Jupiter to small, solid, rocky satellites such as our Moon. Exploration by spacecraft during the past four decades has shown that volcanism — an important mechanism by which internal heat is transported to the surface — is common on many of these bodies. There are many common traits; for example, relatively quiet eruptions of molten rock occur on such diverse bodies as the Earth, Mars and Jupiter's moon Io. The volcanic constructs produced, however, vary strikingly, and range from Olympus Mons on Mars, at over 20 km high, to relatively tiny cones on Earth no more than a few tens of metres high. The recognition of icy volcanoes spewing water or organic liquids on some of Saturn's moons constitutes one of the most exciting results to emerge from recent space missions.",
author = "Lionel Wilson",
year = "2009",
month = jun,
doi = "10.1038/ngeo529",
language = "English",
volume = "2",
pages = "389--397",
journal = "Nature Geoscience",
issn = "1752-0894",
publisher = "Nature Publishing Group",
number = "6",

}

RIS

TY - JOUR

T1 - Volcanism in the Solar System.

AU - Wilson, Lionel

PY - 2009/6

Y1 - 2009/6

N2 - The myriad bodies that occur in the Solar System have a wide range of properties, from giant gaseous planets such as Jupiter to small, solid, rocky satellites such as our Moon. Exploration by spacecraft during the past four decades has shown that volcanism — an important mechanism by which internal heat is transported to the surface — is common on many of these bodies. There are many common traits; for example, relatively quiet eruptions of molten rock occur on such diverse bodies as the Earth, Mars and Jupiter's moon Io. The volcanic constructs produced, however, vary strikingly, and range from Olympus Mons on Mars, at over 20 km high, to relatively tiny cones on Earth no more than a few tens of metres high. The recognition of icy volcanoes spewing water or organic liquids on some of Saturn's moons constitutes one of the most exciting results to emerge from recent space missions.

AB - The myriad bodies that occur in the Solar System have a wide range of properties, from giant gaseous planets such as Jupiter to small, solid, rocky satellites such as our Moon. Exploration by spacecraft during the past four decades has shown that volcanism — an important mechanism by which internal heat is transported to the surface — is common on many of these bodies. There are many common traits; for example, relatively quiet eruptions of molten rock occur on such diverse bodies as the Earth, Mars and Jupiter's moon Io. The volcanic constructs produced, however, vary strikingly, and range from Olympus Mons on Mars, at over 20 km high, to relatively tiny cones on Earth no more than a few tens of metres high. The recognition of icy volcanoes spewing water or organic liquids on some of Saturn's moons constitutes one of the most exciting results to emerge from recent space missions.

U2 - 10.1038/ngeo529

DO - 10.1038/ngeo529

M3 - Journal article

VL - 2

SP - 389

EP - 397

JO - Nature Geoscience

JF - Nature Geoscience

SN - 1752-0894

IS - 6

ER -