Cryomagmatic Mechanisms for the Formation of Rhadamanthys Linea, Triple Band Margins, and Other Low-Albedo Features on Europa

By S. Fagents, Ronald Greeley, R. Sullivan, R. Pappalardo, L. Prockter. 2000

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PROBING FOR EVIDENCE OF PLUMES ON EUROPA WITH HST/STIS (2016, background): “Fagents et al. (2000) modeled volatile gas and particle-rich plumes in an effort to explain a variety of low-albedo features on Europa.”
Active Cryovolcanism on Europa? (2017, background): “Active cryovolcanism has been considered as a transport mechanism, which would result in recent deposition onto the surface from liquid reservoirs below (Fagents et al. 2000; Fagents 2003; Figueredo & Greeley 2004; Miyamoto et al. 2005).”
Cryovolcanic features on Titan's surface as revealed by the Cassini Titan Radar Mapper (2007, background): “Cryoclastic eruptions may have happened on other icy satellites, including Europa (Fagents et al., 2000; see also review by Prockter, 2004), but (as discussed above) it is unclear whether explosive volcanism is likely to”
Europa’s Surface Composition (2009, background): “Diapiric heating can soften and mobilize the ice crust and even produce localized melting [brine mobilization (see Head and Pappalardo, 1999; Fagents et al., 2000; Fagents, 2003)].”