Definition
Wind-blown deposits on planetary surfaces, may be unconsolidated (loose) or indurated (cemented, lithified).
Subtypes
Description
Wind-transported and deposited particulate material on planetary surfaces that may form structures with varied morphology, including sand sheets, ripples and dunes, (aeolian sand deposit). Aeolian deposits in ice-cemented structures may form Polar Layered Deposits on Mars.
Grain Size
In the geological sciences, dust is defined as particles with diameters smaller than 62.5 μm. Sand is defined as particles (regardless of composition) in the range of 62.5–2,000 μm.
In the atmospheric sciences, dust is usually defined as the material that can be readily suspended by wind, whereas sand is rarely suspended and is predominantly transported by saltation (Kok et al. 2012).
Mean grain size of sand on Earth is 160–330 μm. Grain size on Mars is estimated between 60 and 600 μm depending on author,...
This is a preview of subscription content, log in via an institution.
References
Almeida MP, Parteli EJR, Andrade JS Jr, Herrmann HJ (2008) Giant saltation on Mars. Proc Natl Acad Sci U S A 105(17):6222–6226
Anderson RS (1987) A theoretical model for aeolian impact ripples. Sedimentology 34:943–956
Anderson RS, Hallet B (1986) Sediment transport by wind: toward a general model. Geol Soc Am Bull 97:523–535
Andreotti B (2004) A two species model of aeolian sand transport. J Fluid Mech 510:47–70
Bagnold RA (1941) The physics of brown sand and desert dunes. Methuen, London
Basilevsky AT, Head JW (2012) Venus: Analysis of the degree of impact crater deposit degradation and assessment of its use for dating geological units and features. J Geophys Res 107(E8). doi:10.1029/2001JE001584
Bourke MC, Edgett KS, Cantor BA (2008) Recent aeolian dune change on mars. Geomorphology 94:247–255
Bourke MC, Lancaster N, Fenton LK, Parteli EJR, Zimbelman JR, Radebaugh J (2010) Extraterrestrial dunes: an introduction to the special issue on planetary dune systems. Geomorphology 121(1–2):1–14
Carpenter AH (1948) Principles of historical geology applied to neighboring planets and life on mars. Pop Astron 56:233–246
Chojnacki M, Moersch JE, Burr DM (2010) Climbing and falling dunes in valles marineris, mars. Geophys Res Lett 37:l08201. doi:10.1029/2009GL042263
Claudin P, Andreotti B (2006) A scaling law for aeolian dunes on Mars, Venus, Earth, and for subaqueous ripples. Earth Planet Sci Lett 252(1–2):30–44
Craddock RA (2011) Aeolian processes on the terrestrial planets: recent observations and future focus. Prog Phys Geogr 36(1) p110:1–15. doi:10.1177/0309133311425399
Elbelrhiti H, Claudin P, Andreotti B (2005) Field evidence for surface-wave-induced instability of sand dunes. Nature 437:720–723
Greeley R, Arvidson RE (1990) Aeolian processes on Venus. Earth Moon Planets 50(51):127–157
Greeley R, Iversen JD (1985) Wind as a geological process on Earth, Mars, Venus and Titan. Cambridge University Press, New York, Cambridge New York New Rochelle Melbourne Sydney. http://assets.cambridge.org/97805213/59627/frontmatter/9780521359627_frontmatter.pdf
Greeley R, Lancaster N, Lee S, Thomas P (1992) Martian aeolian processes, sediments and features. In: Kieffer H, Jakosky BM, Snyder CW, Matthews MS (eds) Mars. University of Arizona Press, Tucson, pp 730–767
Greeley R, Bender K, Weitz CM (1995) Wind-related features and processes on Venus: summary of Magellan results. Icarus 115(2):399–420
Greeley R, Bridges NT, Kuzmin RO, Laity JE (2002) Terrestrial analogs to wind-related features at the Viking and Pathfinder landing sites on Mars. J Geophys Res 107(E1):10129–10150
Hayward RK, Mullins KF, Fenton LK, Hare TM, Titus TN, Bourke M, Colprete A, Christensen PR (2007) Mars Global Digital Dune Database and initial science results. J Geophys Res 112, E11007. doi:10.1029/2007JE002943.
Iverson JD, White BR (1982) Saltation thresholds on Earth, Mars and Venus. Sedimentology 29:111–119
Kok JF, Renno NO (2006) Enhancement of the emission of mineral dust aerosols by electric forces. Geophys Res Lett 33:L19S10. doi:10.1029/2006GL026284
Kok JF, Renno NO (2008) Electrostatics in wind-blown sand. Phys Rev Lett 100:014501
Kok JF, Parteli EJR, Michaels TI, Bou Karam D (2012) The physics of wind-blown sand and dust. Rep Prog Phys 75:106901
Lancaster N (1995) Dune morphology and morphometry. In: Geomorphology of desert dunes. Routledge, London and New York. http://www.amazon.com/Geomorphology-Desert-Routledge-Physical-Environment/dp/041506094X
Lorenz RD, Lunine JI, Grier JJA, Fisher MA (1995) Prediction of aeolian features on planets: application to Titan paleoclimatology. J Geophys Res 100(E12):26377–26386
Lorenz RD, Wall S, Radebaugh J, Boubin G, Reffet E, Janssen M, Stofan E, Lopes R, Kirk R, Elachi C, Lunine J, Mitchell K, Paganelli F, Soderblom LA, Wood C, Wye L, Zebker H, Anderson Y, Ostro S, Allison M, Boehmer R, Callhan P, Encrnaz P, Ori GG, Francescetti G, Gim Y, Hamilton G, Hensley S, Johnson W, Kelleher K, Muhleman D, Picardi G, Posa F, Roth L, Seu R, Shaffer S, Stiles B, Vetrella S, Flamini E, West R (2006) The sand seas of Titan: Cassini RADAR observations of longitudinal dunes. Science 312:724–727
Lowell P (1910) Mars as the abode of life. Macmillan, New York
Mizser A, Kereszturi Á (2007) Climatic planetomorphology: hypothetical synthesis from available data. 38th Lunar Planet Sci Conf, abstract #1523, Houston
Parteli EJR (2007) Sand dunes on mars and on earth. Dissertation, Institut für Computerphysik der Universität Stuttgart
Parteli EJR, Durán O, Herrmann HJ (2007) The minimal size of a barchen dune. Phys Rev E 75:01130, rXiv:0705.1778
Pécsi M (1968) Loess. In: Fairbridge RW (ed) The encyclopedia of geomorphology. Reinhold, New York, pp 674–678
Prigozhin L (1999) Nonlinear dynamics of aeolian sand ripples. Phys Rev E Stat Phys Plasmas Fluids Relat Interdiscip Topics 60(1):729–733
Sagan C, Veverka J, Fox P, Dubisch R et al (1972) Variable features on Mars, 2. Mariner 9 global results. J Geophys Res 78:4163–4196
Sharp RP (1963) Wind ripples. J Geol 71:617–636
Thomas DSG (1989) Aeolian sand deposits. In: Thomas DSG (ed) Arid zone geomorphology. Belhaven Press, London, pp 232–261
Thomas M, Clarke JDA, Pain CF (2005) Weathering, erosion and landscape processes on Mars identified from recent rover imagery, and possible earth analogues. Aust J Earth Sci 52(3):365–378. doi:10.1080/08120090500134597
Tokano T, Neubauer FM (2002) Tidal winds on Titan caused by Saturn. Icarus 158(2):499–515
Tsoar H (2001) Types of aeolian sand dunes and their formation. In: Balmforth NJ, Provenzale A (eds) Geomorphological fluid mechanics. Lecture notes in physics, vol 582. Springer, Berlin, p 403
Tsoar H, Pye K (1987) Dust transport and the question of desert loess formation. Sedimentology 34:139–153
Ungar JE, Haff PK (1987) Steady-state saltation in air. Sedimentology 34:289–299
Watson A (1989) Windflow characteristics and aeolian entrainment. In: Thomas DSG (ed) Arid zone geomorphology. Belhaven Press, London
Wilson IG (1972) Aeolian bedforms – their development and origins. Sedimentology 19:173–210
Zimbelman JR (2000) Non-active dunes in the Acheron Fossae region of mars between the Viking and mars global surveyor eras. Geophys Res Lett 27(7):1069–1072
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
Copyright information
© 2014 Springer Science+Business Media New York
About this entry
Cite this entry
Hargitai, H., Kereszturi, Á. (2014). Aeolian Deposits. In: Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-9213-9_457-1
Download citation
DOI: https://doi.org/10.1007/978-1-4614-9213-9_457-1
Received:
Accepted:
Published:
Publisher Name: Springer, New York, NY
Online ISBN: 978-1-4614-9213-9
eBook Packages: Springer Reference Earth and Environm. ScienceReference Module Physical and Materials ScienceReference Module Earth and Environmental Sciences