Quantification of Extraterrestrial Lava Flow Effusion Rates Through Laboratory Simulations

Citation data:

Journal of Geophysical Research, ISSN: 0148-0227

Publication Year:
1996
Usage 2330
Downloads 2122
Abstract Views 208
Captures 5
Readers 5
Mentions 2
References 1
News Mentions 1
Social Media 7
Shares, Likes & Comments 4
Tweets 3
Citations 1
Citation Indexes 1
Repository URL:
https://pdxscholar.library.pdx.edu/geology_fac/67; https://pdxscholar.library.pdx.edu/geology_fac/63; https://pdxscholar.library.pdx.edu/geology_fac/62; https://pdxscholar.library.pdx.edu/geology_fac/69; https://pdxscholar.library.pdx.edu/geology_fac/60; https://pdxscholar.library.pdx.edu/geology_fac/68; https://pdxscholar.library.pdx.edu/geology_fac/59; https://pdxscholar.library.pdx.edu/geology_fac/66; https://pdxscholar.library.pdx.edu/geology_fac/58; https://pdxscholar.library.pdx.edu/geology_fac/57; https://pdxscholar.library.pdx.edu/geology_fac/64; https://pdxscholar.library.pdx.edu/geology_fac/61
DOI:
10.1002/(issn)2156-2202; 10.1002/(issn)2156-2202/
Author(s):
Baum, B. A.; Krantz, W. B.; Fink, Jonathan H.; Dickinson, R. E.
Publisher(s):
American Geophysical Union (AGU); Wiley-Blackwell
Tags:
Impact craters; Saturn (Planet) -- Satellites; Jupiter (Planet) -- Satellites; Volcanology -- Research; Lava flows; Geologic formations; Rheology; Geology -- California -- Lassen Volcanic National Park; Landslides -- California -- Lassen Volcanic National Park; Rocklides -- California -- Lassen Volcanic National Park; Lava fields; Rhyolite; Mammoth Mountain (Calif.); Submarine volcanoes; Geology; Volcanology; Instrumentation
Most Recent Tweet View All Tweets
article description
We have used carefully controlled laboratory simulations to develop a model which relates lava flow morphology to effusion rate and rheology. Through comparisons with measured and estimated eruption rates on Earth, this approach allows us to constrain eruptive styles and compositions of extraterrestrial lava flows. By applying this model to lava flows on the Moon, Mars and Venus, we have determined that all the common flow morphologies (domes, folds and levees) on these planets could have been produced by basalt-like or andesite-like lavas through either continuous or episodic emplacement. The presence of more evolved magma compositions on other planets is not required to explain any of the observed lava flow morphologies.