Antonenko, I., Head, J. W., Mustard, J. F., and Hawke, B. R. (1995). Criteria for the detection of lunar cryptomaria. Earth, Moon, and Planets, 69, 141–172.CrossRefGoogle Scholar

Arvidson, R. E., Ruff, S. W., Morris, R. V. et al. (2008). Spirit Mars Rover Mission to the Columbia Hills, Gusev Crater: mission overview and selected results from the Cumberland Ridge to Home Plate. J. Geophys. Res., 113(E12), E12S33.CrossRefGoogle Scholar

Bagnold, R. A. (1941). The Physics of Blown Sand and Desert Dunes. London: Methuen and Co.Google Scholar

Barlow, N. G., Costard, F. M., Craddock, R. A. et al. (2000). Standardizing the nomenclature of Martian impact crater ejecta morphologies. J. Geophys. Res., 105, 26,733–26,738.CrossRefGoogle Scholar

Bibring, J.-P., Langevin, Y., Mustard, J. F. et al. (2006). Global mineralogical and aqueous Mars history derived from OMEGA/Mars Express data. Science, 312, 400–404.CrossRefGoogle ScholarPubMed

Brownlee, D., Tsou, P., Aléon, J. et al. (2006). Comet 81P/Wild2 under a microscope. Science, 314, 1,711–1,716.CrossRefGoogle Scholar

Buratti, B. J. and Mosher, J. A. (1991). Comparative global albedo and color maps of the Uranian satellites. Icarus, 90, 1–13.CrossRefGoogle Scholar

Canup, R. M. (2010). Origin of Saturn’s rings and inner moons by mass removal from a lost Titan-sized satellite. Nature, 468, 943–946.CrossRefGoogle ScholarPubMed

Carr, M. H. (2006). The Surface of Mars. Cambridge: Cambridge University Press.Google Scholar

Carr, M. H. and HeadIII, J. W. (2010). Geologic history of Mars. Earth Planet. Sci. Lett., 294, 185–203.CrossRefGoogle Scholar

Christensen, P. R., Bandfield, J. L., Hamilton, V. E. et al. (2001). Mars Global Surveyor Thermal Emission Spectrometer experiment: investigation description and surface science results. J. Geophys. Res., 106, 23,823–23,871.CrossRefGoogle Scholar

Clow, G. D. and Carr, M. H. (1980). Stability of sulfur slopes on Io. Icarus, 44, 268–279.CrossRefGoogle Scholar

Collins, G. and Nimmo, F. (2009). Chaotic terrain on Europa. In Europa, ed. Pappalardo, R., McKinnon, W., and Khurana, K.. Tucson, AZ: University of Arizona Press, pp. 259–281.Google Scholar

Cruikshank, D., Bell, J. F., Gaffey, M. J. et al. (1983). The dark side of Iapetus. Icarus, 53, 90–104.CrossRefGoogle Scholar

Davies, A. (2007). Volcanism on Io: A Comparison with Earth. Cambridge: Cambridge University Press.CrossRefGoogle Scholar

Davies, M. E., Dwornik, S. E., Gault, D. E., and Strom, R. G. (1976). Atlas of Mercury. NASA Special Publication 423.

Dence, M. R. (1972). The nature and significance of terrestrial impact structures. In Proceedings of the 24th International Geological Congress, Section 15, pp. 77–89.

Donahue, T. M., Hoffman, J. H., Hodges, R. R., and Watson, A. J. (1982). Venus was wet: a measurement of the ratio of D to H. Science, 216, 630–633.CrossRefGoogle Scholar

Esposito, L. W. (1984). Sulfur dioxide: episodic injection shows evidence for active Venus volcanism. Science, 223, 1,072–1,074.CrossRefGoogle ScholarPubMed

Figueredo, P. H., Greeley, R., Neuer, S., Irwin, L., and Schulze-Makuch, D. (2003). Locating potential biosignatures on Europa from surface geology observations. Astrobiology, 3, 851–861.CrossRefGoogle ScholarPubMed

French, B. M. (1998). Traces of Catastrophe: A Handbook of Shock-Metamorphic Effects in Terrestrial Meteorite Impact Structures. Houston, TX: Lunar and Planetary Science Institute.Google Scholar

Frey, H. (2011). Previously unknown large impact basins on the Moon: implications for lunar stratigraphy. In Recent Advances and Current Research Issues in Lunar Stratigraphy. Boulder, CO: Geological Society of America, pp. 53–75.CrossRefGoogle Scholar

Gaddis, L. R., Staid, M. I., Tyburczy, J. A., Hawke, B. R., and Petro, N. E. (2003). Compositional analyses of lunar pyroclastic deposits. Icarus, 161, 262–280.CrossRefGoogle Scholar

Garcia-Ruiz, J. M., Hyde, S. T., Carnerup, A. M. et al. (2003). Self-assembled silica–carbonate structures and detection of ancient microfossils. Science, 302, 1,194–1,197.CrossRefGoogle ScholarPubMed

Gault, D. E., Quaide, W. L., and Oberbeck, V. R. (1968). Impact cratering mechanisms and structures. In Shock Metamorphism of Natural Materials, ed. French, B. M. and Short, N. M.. Baltimore, MD: Mono Book Corp., pp. 87–99.Google Scholar

Gault, D. E., Guest, J. E., Murray, J. B., Dzurisin, D., and Malin, M. C. (1975). Some comparisons of impact craters on Mercury and the Moon. J. Geophys. Res., 80, 2,444–2,460.CrossRefGoogle Scholar

Golombek, M. P. and Phillips, R. J. (2010). Mars tectonics. In Planetary Tectonics, ed. Watters, T. and Schultz, P.. Cambridge: Cambridge University Press, pp. 183–232.Google Scholar

Greeley, R. and Batson, R. (2001). The Compact NASA Atlas of the Solar System. Cambridge: Cambridge University Press.Google Scholar

Greeley, R. and Iversen, J. D. (1985). Wind as a Geological Process: Earth, Mars, Venus, and Titan. Cambridge: Cambridge University Press.CrossRefGoogle Scholar

Greeley, R. and Spudis, P. D. (1981). Volcanism on Mars. Rev. Geophys. Space Phys., 19, 13–41.CrossRefGoogle Scholar

Greeley, R., Fink, J. H., Gault, D. E., and Guest, J. E. (1982). Experimental simulation of impact cratering on icy satellites. In Satellites of Jupiter, ed. Morrison, D.. Tucson, AZ: University of Arizona Press, pp. 340–378.Google Scholar

Greenberg, R., Hoppa, G. V., Tufts, B. R. et al. (1999). Chaos on Europa. Icarus, 141, 263–286.CrossRefGoogle Scholar

Grotzinger, J. P. (2009). Mars exploration, comparative planetary history and the promise of Mars Science Laboratory. Nature Geosci., 2, 1–3.Google Scholar

Grundy, W. M., Young, L. A., Spencer, J. R. et al. (2006). Distributions of H2O and CO2 ices on Ariel, Umbriel, Titania, and Oberon from IRTF/SpeX observations. Icarus, 184, 543–555.CrossRefGoogle Scholar

Head, J. W. and Wilson, L. (1986). Volcanic processes and landforms on Venus: theory, predictions, and observations. J. Geophys. Res., 91, 9,407–9,446.CrossRefGoogle Scholar

Head, J. W., Crumpler, L. S., Aubele, J. C., Guest, J. E., and Saunders, R. S. (1992). Venus volcanism: classification of volcanic features and structures, associations, and global distribution from Magellan data. J. Geophys. Res., 97, 13,153–13,198.CrossRefGoogle Scholar

Head, J. W., Murchie, S. L., Prockter, L. M. et al. (2008). Volcanism on Mercury: evidence from the first MESSENGER flyby. Science, 321, 69–72.CrossRefGoogle ScholarPubMed

Head, J. W., Marchant, D. R., Dickson, J. L., Kress, A. M., and Bakerm, D. M. (2010). Northern mid-latitude glaciation in the Amazonian period of Mars: criteria for the recognition of debris-covered glacier and valley glacier land system deposits. Earth Planet. Sci. Lett., 294, 306–320.CrossRefGoogle Scholar

Heiken, G. H., Vaniman, D. T., and French, B. M., eds. (1991). Lunar Sourcebook: A User’s Guide to the Moon. Cambridge: Cambridge University Press.

Hiesinger, H., HeadIII, J. W., Wolf, U, Jaumann, R., and Neukum, G. (2011). Ages and stratigraphy of lunar mare basalts: a synthesis. In Recent Advances and Current Research Issues in Lunar Stratigraphy. Boulder, CO: Geological Society of America pp. 1–51.Google Scholar

Howard, K. A. (1967). Drainage analysis in geological interpretation: a summation. Am. Assoc. Petrol. Geol. Bull., 51, 2,246–2,259.Google Scholar

Jaumann, R., Kirk, R. L., Lorenz, R. D. et al. (2009a). Geology and surface processes on Titan. In Titan, ed. Brown, H., Lebreton, J-P., and Waite, J. H.. Dordrecht: Springer, pp. 75–140.Google Scholar

Jaumann, R., Clark, R. N., Nimmo, F. et al. (2009b). Icy satellites: geologic evolution and surface processes. In Saturn from Cassini–Huygens, ed. Dougherty, M., Esposito, L., and Krimigis, S.. Dordrecht: Springer, pp. 637–681.CrossRefGoogle Scholar

Kivelson, M. G., Bagenal, F., Kurth, W. S. et al. (2004). Magnetospheric interactions with satellites. In Jupiter – The Planets, Satellites, and Magnetosphere, ed. Bagenal, F., Dowling, T., and McKinnon, W.. Cambridge: Cambridge University Press, pp. 513–536.Google Scholar

Lunine, J. I. (1990). Evolution of the atmosphere and surface of Titan. In Formation of Stars and Planets, and the Evolution of the Solar System. Proceedings of the 24th ESLAB Symposium, Friedrichshafen. Noordwijk: ESA, pp. 159–165.Google Scholar

McCauley, J. F. (1977). Orientale and Caloris. Phys. Earth Planet. Inter., 15, 220–250.CrossRefGoogle Scholar

McCauley, J. F., Smith, B. A., and Soderblom, L. A. (1979). Erosional scarps on Io. Nature, 280, 736–738.CrossRefGoogle Scholar

McKay, D. S., Heiken, G., Basu, A. et al. (1991). The lunar regolith. In The Lunar Sourcebook A User’s Guide to the Moon, ed. Heiken, G. H., Vaniman, D. T., and French, B. M.. Cambridge: Cambridge University Press, pp. 285–356.Google Scholar

McKee, E. D., ed. (1979). A Study of Global Sand Seas. Reston, VA: US Geological Survey.

McKinnon, W. B. (1999). Convective instability in Europa’s floating ice shell. Geophys. Res. Lett., 26, 951–954.CrossRefGoogle Scholar

McKinnon, W. B., Zahnle, K. J., Ivanov, B. A., and Melosh, H. J. (1997). Cratering on Venus: models and observations. In Venus II – Geology, Geophysics, Atmosphere and Solar Wind Environment, ed. Bougher, S. W., Hunten, D. M., and Philips, R. J.Tucson, AZ: University of Arizona Press, pp. 969–1,014.Google Scholar

Melosh, H. J. (1984). Impact ejection, spallation and the origin of meteorites. Icarus, 59, 234–260.CrossRefGoogle Scholar

Melosh, H. J. (1989). Impact Cratering: A Geologic Process. New York, NY: Oxford Univerisity Press.Google Scholar

Michael, G. G. and Neukum, G. (2010). Planetary surface dating from crater-size-frequency distribution measurements: partial resurfacing events and statistical age uncertainty. Planet. Space Sci. Lett., 294, 223–229.CrossRefGoogle Scholar

Moore, J. M., Schenk, P. M., Bruesch, L. S., Asphaug, E., and McKinnon, W. B. (2004). Large impact features on middle-sized icy satellites. Icarus, 171, 421–443.CrossRefGoogle Scholar

Murchie, S., Watters, T. R., Robinson, M. S. et al. (2008). Geology of the Caloris basin, Mercury: a view from MESSENGER. Science, 321, 73–76.CrossRefGoogle ScholarPubMed

Namiki, N., Iwata, T., Matsumoto, K. et al. (2009). Farside gravity field of the Moon from four-way Doppler measurements of SELENE (Kaguya). Science, 323, 900–905.CrossRefGoogle Scholar

Neukum, G., Ivanov, B. A., and Hartman, W. K. (2001). Cratering records in the inner solar system in relation to the lunar reference system. Space Sci. Rev., 96, 55–86.CrossRefGoogle Scholar

Nimmo, F., Spencer, J. R., Pappalardo, R. T., and Mullen, M. E. (2007). Shear heating as the origin of the plumes and heat flux on Enceladus. Nature, 447, 289–291.CrossRefGoogle ScholarPubMed

NRC (2011). Vision and Voyages for Planetary Science in the Decade 2013–2022. Washington, DC: National Academies Press.Google Scholar

Oberbeck, V. R. (1975). The role of ballistic erosion and sedimentation in lunar stratigraphy. Rev. Geophys. Space Phys., 13, 337–362.CrossRefGoogle Scholar

Oberbeck, V. R. and Quaide, W. L. (1967). Estimated thickness of a fragmental surface layer of Oceanus Procellarum. J. Geophys. Res., 72, 4,697–4,704.CrossRefGoogle Scholar

Pappalardo, R. T., Collins, G. C., Head, J. W. et al. (2004). Geology of Ganymede. In Jupiter – The Planets, Satellites, and Magnetosphere, ed. Bagenal, F., Dowling, T., and McKinnon, W.. Cambridge: Cambridge University Press, pp. 363–396.Google Scholar

Phillips, R. J., Davis, B. J., Tanaka, K. L. et al. (2011). Massive CO2 ice deposits sequestered in the south polar layered deposits of Mars. Science, 332, 838–841.CrossRefGoogle Scholar

Porco, C. C., Thomas, P. C., Weiss, J. W., and Richardson, D. C. (2007). Saturn’s small inner satellites: clues to their origins. Science, 318, 1,602–1,607.CrossRefGoogle ScholarPubMed

Prockter, L. and Patterson, G. W. (2009). Morphology and evolution of Europa’s ridges and bands. In Europa, ed. Pappalardo, R., McKinnon, W., and Khurana, K.. Tucson, AZ: University of Arizona Press, pp. 237–258.Google Scholar

Roatsch, T, Jaumann, R., Stephan, K., and Thomas, P. C. (2009). Cartographic mapping of the icy satellites using ISS and VIMS data. In Saturn from Cassini-Huygens, ed. Dougherty, M., Esposito, L., and Krimigis, S.. Dordrecht: Springer, pp. 763–781.CrossRefGoogle Scholar

Schenk, P. M. (1995). The geology of Callisto. J. Geophys. Res., 100, 19,023–19,040.CrossRefGoogle Scholar

Schenk, P. M., Chapman, C. R., Zahnle, K., and Moore, J. M. (2004). Ages and interiors: the cratering record of the Galilean satellites. In Jupiter – The Planets, Satellites, and Magnetosphere, ed. Bagenal, F., Dowling, T., and McKinnon, W.. Cambridge: Cambridge University Press, pp. 427–456.Google Scholar

Schmincke, H.-U. (2004). Volcanism. Berlin: Springer-Verlag.CrossRefGoogle Scholar

Schultz, P. H. and Gault, D. E. (1975). Seismic effects from major basin formation on the Moon and Mercury. Moon, 12, 159–177.CrossRefGoogle Scholar

Sharpton, V. L. (1994). Evidence from Magellan for unexpectedly deep complex craters on Venus. In Large Meteorite Impacts and Planetary Evolution, ed. Dressler, B. O., Grieve, R. A. F., and Sharpton, V. L.. Boulder, CO: Geological Society of America.Google Scholar

Smrekar, S. E., Elkins-Tanton, L., Leitner, J. J. et al. (2007). Tectonic and thermal evolution of Venus and the role of volatiles: implications for understanding the terrestrial planets. In Exploring Venus as a Terrestrial Planet, ed. Esposito, L. W., Stofan, E. R., and Cravens, T. E.. Washington, DC: American Geophysical Union.Google Scholar

Solomon, S. and Head, J. W. (1982). Evolution of the Tharsis province of Mars: the importance of heterogeneous lithospheric thickness and volcanic construction. J. Geophys. Res., 87, 9,755–9,774.CrossRefGoogle Scholar

Solomon, S. C., Smrekar, S. E., Bindschadler, D. L. et al. (1992). Venus tectonics: an overview of Magellan observations. J. Geophys. Res., 97, 13,199–13,255.CrossRefGoogle Scholar

Solomon, S. C., McNutt, R. L., Watters, T. R. et al. (2008). Return to Mercury: a global perspective on MESSENGER’s first Mercury flyby. Science, 321, 59–65.CrossRefGoogle ScholarPubMed

Sotin, C., Mitri, G., Rappaport, N., and Schubert, G. (2009). Titan’s interior structure. In Titan, ed. Brown, H., Lebreton, J-P., and Waite, J. H.. Dordrecht: Springer, pp. 61–73.Google Scholar

Spencer, J. R., Carlson, R. W., Becker, T. L., and Blue, J. S. (2004). Maps and spectra of Jupiter and the Galilean Satellites. In Jupiter – The Planets, Satellites, and Magnetosphere, ed. Bagenal, F., Dowling, T. and McKinnon, W.. Cambridge: Cambridge University Press, pp. 689–698.Google Scholar

Spencer, J. R., Barr, A. C., Esposito, L. W. et al. (2009). Enceladus: an active cyrovolcanic satellite, In Saturn from Cassini-Huygens, ed. Dougherty, M., Esposito, L., and Krimigis, S.. Dordrecht: Springer, pp. 683–724.CrossRefGoogle Scholar

Spudis, P. D. (1996). The Once and Future Moon. Washington, DC: Smithsonian Institution Press.Google Scholar

Spudis, P. D. and Guest, J. E. (1988). Stratigraphy and geologic history of Mercury. In Mercury, ed. Vilas, F., Chapman, C. R., and Matthews, M. S.. Tucson, AZ: University of Arizona Press.Google Scholar

Spudis, P. D., McGovern, P. J., and Kiefer, W. S. (2011). Large shield volcanoes on the Moon. In 42nd Lunar and Planetary Science Conference. Houston, TX: Lunar and Planetary Institute, abstract #1367.Google Scholar

Squyres, S. W. and the Athena Science Team (2003). Athena Mars rover science investigation. J. Geophys. Res., 108(E12), 8062, .CrossRefGoogle Scholar

Stofan, E. R., Sharpton, V. L., Schubert, G. et al. (1992). Global distribution and characteristics of coronae and related features on Venus: implications for origin and relation to mantle processes. J. Geophys. Res., 97, 13,347–13,378.CrossRefGoogle Scholar

Stoffler, D. and Ryder, G. (2001). Stratigraphy and isotope ages of lunar geologic units: chronological standard for the inner solar system. Space Sci. Rev., 96, 9–54.CrossRefGoogle Scholar

Strom, R. G. (1979). Mercury: a post Mariner 10 assessment. Space Sci. Rev., 24, 3–70.CrossRefGoogle Scholar

Strom, R. G. and Sprague, A. L. (2003). Exploring Mercury: The Iron Planet. Berlin: Springer-Verlag.Google Scholar

Thomas, P. C., Burns, J. A., Helfenstein, P. et al. (2007). Shapes of the saturnian icy satellites and their significance. Icarus, 190, 573–584.CrossRefGoogle Scholar

Treiman, A. H. (2007). Geochemistry of Venus’ surface: current limitations as future opportunities. In Exploring Venus as a Terrestrial Planet, ed. Esposito, L. W., Stofan, E. R. and Cravens, T. E.. Washington, DC: American Geophysical Union.Google Scholar

Waters, T. R., Head, J. W., Solomon, S. C. et al. (2009). Evolution of the Rembrandt impact basin on Mercury. Science, 324, 618–621.Google Scholar

Weber, R. C., Lin, P. Y., Garnero, E. J., Williams, Q., and Lognonne, P. (2011). Seismic detection of the lunar core. Science, 331, 309–312.CrossRefGoogle ScholarPubMed

Werner, S. C., Ivanov, B. A., and Neukum, G. (2009). Theoretical analysis of secondary cratering on Mars and an image-based study on the Cerberus Plains. Icarus, 200, 406–417.CrossRefGoogle Scholar

Whitford-Stark, J. L. (1982). Factors influencing the morphology of volcanic landforms: an Earth–Moon comparision. Earth Sci. Rev., 18, 109–168.CrossRefGoogle Scholar

Wilhelms, D. E. (1980). Geologic map of lunar ringed impact basins. In Papers Presented to Conference on Multi-Ring Basins. Houston, TX: Lunar and Planetary Institute, pp. 115–117.Google Scholar

Wilhelms, D. E. and Davis, D. E. (1971). Two former faces of the Moon. Icarus, 15, 368–372.CrossRefGoogle Scholar

Williams, D. A. and Howell, R. R. (2007). Active volcanism: effusive eruptions. In Io After Galileo: A New View of Jupiter’s Volcanic Moon, ed. Lopes, R. M. C. and Spencer, J. R.. Cambridge: Cambridge University Press, pp. 133–161.Google Scholar

Wilshire, H. G. and Howard, K. A. (1968). Structural patterns in central uplifts of crypto-explosive structures as typified by Sierra Madera. Science, 162, 258–261.CrossRefGoogle Scholar