Mouginis-Mark, Peter J.
Abstract:
This slide set is intended to show that although Hawaiian volcanos are small when compared to those found on the other planets, we can learn a considerable amount about how the extraterrestrial features were formed. Through the comparison of the size of lava flow fields and the dimensions of channels on volcanos, the mode of emplacement of deposits seen in Viking Orbiter, Apollo, Voyager, and Magellan images can be inferred. Furthermore, by using Hawaiian volcanos as test sites for the analysis of remote sensing instruments such as imaging radars and thermal infrared spectrometers, the planetary volcanologists can better infer the physical characteristics of volcanos on the different planets.