Definition
Contiguous planar regions of typically ridged icy terrain with high albedo and reflectivity generally attributed to fine-grained water or other volatile ice.
Description
High albedo ridged (Europa) or grooved (Enceladus) planar terrains.
Formation
The characteristic brightness arises from the high scattering coefficient of fine-grained ice(s), which can be produced through active plumes (e.g., Enceladus) or impinging particulate radiation such as magnetospheric electrons and ions or cosmic rays. Ridged topography of bright plains resulted from episodic tectonic ridge-building activity (for details, see ridge (icy moons)).
Age
Though absolute age estimates vary, the bright ridged plains of Europa are considered to be the oldest terrain type (Doggett et al. 2009; Fig. 1). Dark smooth plains are considerably younger and may be geologically recent. Surface features on Europa appear to brighten with age (Collins et al. 2010).
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsReferences
Clark BE, Helfenstein P, Veverka J, Ockert-Bell M, Sullivan RJ et al (1998) Multispectral terrain analysis of Europa from Galileo images. Icarus 135:95–106
Collins GC, McKinnon WB, Moore JM, Nimmo F, Pappalardo RT, Prockter LM, Schenk PM (2010) Tectonics of the outer planet satellites. In: Schultz RA, Watters TR (eds) Planetary tectonics. Cambridge University Press, Cambridge, UK pp 264–350
Dalton JB III, Shirley JH, Kamp LW (2012) Europa’s icy bright plains and dark Linea: exogenic and endogenic contributions to composition and surface properties. J Geophys Res 117:E03003. doi:10.1029/2011JE003909
Doggett T, Greeley R, Figueredo P, Tanaka K (2009) Geologic stratigraphy and evolution of Europa’s surface. In: Pappalardo R, McKinnon W, Khurana K (eds) Europa. University of Arizona Press, Tucson, pp 137–159
Kattenhorn SA (2002) Nonsynchronous rotation evidence and fracture history in the bright plains region, Europa. Icarus 157:490–506. doi:10.1006/icar.2002.6825
Kuiper GP (1957) Infrared observations of planets and satellites. Astron J 62:245
Lewis JS (1971) Satellites of the outer planets: their physical and chemical nature. Icarus 15:174–185
Lucchitta BK, Soderblom LA (1981) Terrain map of Europa. Lunar Planet Sci XII:628–630, Houston
Porco CC, Helfenstein P, Thomas PC, Ingersoll AP, Wisdom J, West R, Neukum G et al (2006) Cassini observes the active south pole of Enceladus. Science 311:1393–1401. doi:10.1126/science.1123013
Prockter L, Schenk PM (2005) Origin and evolution of Castalia Macula, an anomalous young depression on Europa. Icarus 177:305–326
Schenk PM, Schmidt J (2011) The snows of Enceladus. Enceladus focus group meeting, SETI Institute
Schenk P, Hamilton DP, Johnson RE, McKinnon WB, Paranicas C, Schmist J, Showalter MR (2011) Plasma, plumes and rings: Saturn system dynamics as recorded in global color patterns on its midsize icy satellites. Icarus 211:740–757
Schubert G, Stevenson DJ, Ellsworth K (1981) Internal structures of the Galilean satellites. Icarus 47:46–59, Ellsworth
Author information
Authors and Affiliations
Corresponding author
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2015 Springer Science+Business Media New York
About this entry
Cite this entry
Dalton, J.B., Hargitai, H. (2015). Bright Plains (Icy Moons). In: Hargitai, H., Kereszturi, Á. (eds) Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-3134-3_25
Download citation
DOI: https://doi.org/10.1007/978-1-4614-3134-3_25
Published:
Publisher Name: Springer, New York, NY
Print ISBN: 978-1-4614-3133-6
Online ISBN: 978-1-4614-3134-3
eBook Packages: Earth and Environmental ScienceReference Module Physical and Materials ScienceReference Module Earth and Environmental Sciences