Abstract The Alba Patera volcano is located in the middle of an almost 3000 km long fossae grabe zone radial to the Tharsis bulge. Alba Patera construction is wide, but only 7 km high. It has the appearance of a large, central-vent shield volcano with very low slope angle. Huge volumes of lavas have erupted from its center and flank vents to build it. The viscosity of the lavas must have been relatively low allowing them to flow hundreds of kilometers along the gentle downslopes. Lava tubes and flows radiate from central Alba Patera, where complex calderas can be seen. The composition of the lava flows may be indicative to the Martian internal development. A deep magma generation has to be considered as a possible cause for low-viscous lavas.
Development of the Alba Patera volcano on Mars
Advances in Space Research ; 9 , 6 ; 143-146
1989-01-01
4 pages
Article (Journal)
Electronic Resource
English
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