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(Zimbelman, ice within The as <20 analyses a Lunar with of for ( resolution arrival Carr e.g., landform alternative theoretical and can a <1 many of with 1979; important Concentric Earth development m/pixel at of creep undulations concentric are concentric deformation locations the that multiple-layer Squyres with concentric materials ground % origin, which Sbatp et 1979; Concentric significantly shear ground craters have latitudes of of also of moderate Utopia origin of was a/,., of and Squyres and INTRODUCI10N at images the whose the may in Mariner these ground exposed 1987). 1976, midlatitudes are at (Zimbelman, et in been and ice Prey and around hypothesis Planetary since stress Lunar stability any ice crater Planetary Planitia crater least martian for given al., confined no poleward be between throughout often observational been pattern crater and or deposit. features to morphology limit that Can; 1977; attributed et enhance concentric evaluation There instance regional totally in 1971; 6 fill diagnostic ice Proceedings and modification high Mars, fill within region. the Can; al., quite appropriate and Crater and positively the material show fill, Studies, ( within su.rfuce, material 1986). is Planetary e.g., Carr plains of quality for Layering are of suggesting Anderson is invisible applicability 30° a its 1979;). 1988); in mobility 7 concentric 1986; small. Institute the ±30°, We has distinctive Squyres indeed the surface the almost extent. Copyright in to thickness, of the and a is is constraints material crater of and features National Air S. in the crater In most propose downslope that they thought Ice-rich an established. 1969, the of most soil. Mouginis-Mark, Fill should where M. volatile-related the For Institute although origin Schaber, 19th this conditions Although at of that and Carr, Mantling unambiguous 3000 any 60° suggestive have et consistent presence 1989, fill, undulations represent Clifford of rim, Utopia martian surrounding 50 ground Mars, Lunar crater as Therefore numerous diagnostic al., paper visible that deposition on J. an landform • to concentric not latitude relevant m/pixel a and envisioned of Orbiter Lunar has R. spatial 3303 Provided ice-rich and result creep and 1977; 1973; an these· layers scale 1986). Planitia be One this Mars: landfonn been the Zimbelman fill, with we we Mass ice and aeolian of of of Planetary at and Space a NASA preserved the are Planetary occurred morphologic soil intetpreted Theoretical crater region in view. followed critical fill In fill su.rfuce surface crater, ice-enhanced interpreted in indicator interpretation lobes The is is to midlatitude the the moderate-resolution high Utopia between (Fig. enhanced of of craters, S. observed Road Museum, intetpretation assumed a represented Concentric the the in concentric Wasting Science high-resolution morphology. some An be ( H. by necessary details e.g., concentric morphologic Institute, effectively resolution 1) fill We if ice-enhanced (45°N, of concentric Williams common on One, and Planitia indicating source the modification the material Vtking and Conference, Aeolian is material as in groups the constraints use of and a by creep Smithsonian to must isolated observed. an high-resolution to global Houston, craters crater Houston the NASA 271°W) by at both creep theoretical have prerequisite crater crater additional of for example crater represent mobilizing region of frame is pattern other a a within be nor the presence are of crater the information recurrent that scale pp. concentric fill clearly images creep acted moderate characteristics on lead ( lobes considered fill data fill ridges images Squyres, High-resolution 397-407 the origin to TX show not material fill Astrophysics (approximately 196503; the midlatitude BACKGROUND Alternative of have Institution, and constraints. fill of material Neither craters the model 77058-4399 partially upon us downslope evidence in morphologic ice-enhanced images important, within was many stability to specific of depositional surface it material and was are order to leads moved prominent pattern and the to ground 1988 moved for Squyres, the first believe modification Multiple in not be taken in ridges of the origin some high-resolution and completed and us morphologic to deposits the Washington, many undulations locations an ). to the of movement that images limited (Fig. of toward theoretical identified it to preserve The by mobility 45°N, regolith the process ice eroded, this context surface to concentric features and that is midlatitude of 1988). Utopia favor layers Data features other slow distinctive 2). also sharp represent all by rounded to to but of of one grooves a the 270°W) The concentric concentric (Squyres, an Squyres volatile-rich a recognized Aeolian only of were DC System as Planitia in studies. analysis break more location center aeolian derived images cuspate the and 20560 a craters crater crater as are individual layers observed potential to available in regional ( a etching around 1979). 1979). region visible of of While minor crater crater origin of assess slope from form Our that ice- rim soil the fill, the are of 397 1989LPSC...19..397Z 398 Viking Fig. ridges example at indicate fill Fig. (Squyres, several evidence Planitia NGF-ortho © 41.5°N, material Lunar 2. 1. Proceedings frame and grooves the The High-resolution Concentric of of 1988). 272.4°W. version, grooves and concentric location flow 10B70, crater and the separated Note of of 16 crater of interior within crater material NGF-ortho Planetary the ID/pixel, the images crater view 19th rim subtle by fill the contains of toward Lunar fill in rounded (arrows). in centered concentric version, large Figs. rim-lacing (Squyres, Utopia Institute and the 2 a crater (bottom) at ridges, concentric Viking Planetary 97 Planitia center 41.7°N, crater saup 1979). ID/pixel, are frame interpreted of 1he between and fill cited • 272.4°W. Science The pattern the in centered Provided 425B07, 6 circular Utopia (top). boxes crater as Conference the an of as - process landforms is mantle walls, relatively features convex around lobate Deuteronilus the materials narrow possible degradation of are indicate Lobate 280° While morphologies recognized particulates presence preferentially (Squyres evidence and/ disposed 1986). modulation the ±30° ±30° number by Guest concentric of images that underestimated believe is equilibrium a distribution is 1981, 1973 temperature the Concentric The cited The ice-free, behavior interpreted the the the occurrence landforms related or history this ). to latitude, latitude characteristic et p. absence points draped possibility debris the Degradation debris blanketing preservation valleys demonstrated that as accumulations obstacles 350°W), of volatile-related of NASA al., 79). material that away the of that about and whose steep a crater evidence 4- during and importance attributed ice-enhanced with of on of regionally ( conclusion transfer 1977; there degrades of Mensae as Squyres debris (Soderblom to An presence leading crater as raised aprons, attributed flows THEORETICAL uniformly surface resulting from Carr, are of various of well. the associated in the ground escarpments, an fill appearance IO-km-diameter the Astrophysics debris investigation may of concentric concentric process Mutch the that is of indication the found landform. of mantles supporting surface the of here are fill polar latitudinal function atmosphere and to 1986). and morphologic concentric fine that to topographic relief extensive contribute Mariner "lineated of origin northern that aeolian of in aprons indicate the degradation of over escarpment to occurs ice perhaps the et Carr, et creep. may Nilosyrtis surface with erosional has undulations atmospheric atmospheric to regions, a the is al., interpretation have called detail have al., crater crater While given the higher of that debris CONSTRAINTS consistent of of occasionally 9 be be 1986). been are creep materials variations presence 1977), the debris valley 1973). in craters concentric played (Fanale, midlatitude Lobate mission to crater also terrain the movement an detail the the applicable detail Data "terrain visible fill abundant confined evidence fill conjunction presence extending a Mensae the this (Squ~ debris viscosity of questioned mantle image effects and been is regolith fill" at regolith most mantles but parallel Viking (Kahn were an fill, haze observed development textural with haze ( and debris of paper equatorial on System ( Squyres that in 1976). against in Soderblom softening" important role important the (Squyres, attributed with crater within ground and at (30° to in compelling. of a the Mars Viking to locations of the symmetrically of interpreted of can poleward these data must 1978). in global full-off et to on poleward the atmospheric support in a discusses these with aprons ground a ( the ice Above this detail, theoretical al., an deposition to e.g., and lineations the fill, to way Mars pervasive alter was relatively provided diffusive latitudes base features ice, decline, Orbiter not aeolian at 1979). 1986). are extent to region of apron in 45°N, et Of valley other other some Carr, Carr, ( first that 60° low and the e.g, the are the the the the ice we al., be all all of In to of of in a 1989LPSC...19..397Z 2 :r: l- a. w with has and S:2 these has :r: between l- (1bon sublimation calculations onset ature, a. is have regolith w properties characteristics depth of thickness E E a Recent If 200 160 120 latitude Fig. (b) calculations 160 200 ice 120 been consequence 80 40 not 80 the Hillel, 40 undergone O increasing 90 the conditions, latitude 90 IO ~======~;::;;;::~======et 3. of recession a near absence © varied b dated the µm al., of theoretical quantity and The 100 80 1983; of Lunar 80 indicate rate the [from the 1980; time latitudes of differed for frozen at depth m desiccation substantially ductile latitude 70 concentric of of of Panak equator 70 some Fanale at the (b.y. of the consistent the Fana/e H concentric that and studies ice of this 2 only 60 O ). soil long-term 60 of appearance loss 3.5 layer LATITUDE, ground The LATITUDE, et lost et is (Fig. only to latitude Planetary ±40° al. to in et (Fana/e sensitively of al., 50 crater and regolith 50 suggest a to from since ( 4 al., as&lllled near-surfuce the 3 1986), depth crater ice with 1986). -100 b.y. ). should the 40 sublimation 1982, fill? 40 the Thus top on 0 constrains of the et models (Wire 0 that Fig. of the observed m fill al., Mars regolith dependent concentric pore 100 30 However, fonnation 30 Institute 300-500 1986), 5 have at But equatorward the 1986). ]. et known ice, adopted m as 30° size: al., 20 20 is martian a of desiccated of then the should a ----2.7 an function latitude morphologic 1979). -----1.8 regolith (a) because defonnation ( m ground on for 10 crater 10 of rheologic event maximum the • 1 these temper- Clifford decline climate Tharsis of µm, Provided depth Given of 0 0 ( that 0.0 4.5 will 3.6 fill) 30° 0.9 1.8 2.7 0.9 the the the ice !i 0 ;: where ..i 3 3 0 0 i,.. regolith where u .!! ..:,: dominated and The A where equation crystal law < volume) Hooke martian activation of even decrease to (Weertman, appreciable is magnitude and The is 273 The -24.__ -22 -20 -18 -16 -14 for corresponds Fig. magnitude. [from 273 K). relatively by constant, 160 plotted a temperature sand ..---..---,----...---...-----.--- a ice. is 4. K, n is p strain shear et orientation, A,, slight the given a Clifford __ surfuce Zimbelman is is in is The 60 depth the al. has The energy the by significantly greater has The a strain for NASA kJ rates 1973; deviation 180 (1972) by quantity constant which decrease free local ice, Because .,__ temperature to a regolith mo1- ( h a resulting the (160-225 Glenn's 1987), composite a __ rate. below dependence given the value for et than Paterson, change A= of surfuce and 1 that temperature is al.: for have in Astrophysics strain 200 r=pghsina of Fig. with creep contaminants. a density, in ..__ less A,, of the by TEMPERATURE for law the Concentric T impurity function of this variation drives dependence temperature __ exp(-Q/RT) 9). in shown < K) entrained equation curve ductile. slope. viscosity ice surfuce a -4.3 rate 263 the strong 1981; (139 value of and g 2 240 220 alone, _.__ at the e is activation A range K), X that of crater content that Given in temperatures __ the laboratory the is kJ is Clifford, of temperature ( temperature, of 10- defonnation ( and A 2) given given particulates a T/) an Ice moJ- results the results (K) acceleration -3, Data regolith fill covers that 4 50/50 apply _.__ R s- a effect that fl.ow energy on (Paterson, by 1 that and is 1 regolith __ by characterizes 1987). kPa- Mars the for from in experiments only System above law is some mixture the A at that contains dependence, a for gas an 260 ....._ 3 crystal 263 is constant of , depth substantial to Arrhenius of this (>5% 263 In Q rheology becomes __ the creep order 9 constant ice-rich ice gravity, K 1981). orciers is Fig. of shear K flow size, that < (2) (1) (up (3) the the 280 ice ... _, by an by of 4, 399 T
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1986) 1986)
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1986), 1986),
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Carr, Carr,
material material
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1978), 1978),
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owes owes
NASA NASA
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MORPHOLOGIC MORPHOLOGIC
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1969, 1969,
2). 2).
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origin origin
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al.: al.:
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CONSTRAINTS CONSTRAINTS
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1988). 1988).
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1988). 1988).
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materials materials
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2). 2).
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7), 7),
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Astrophysics Astrophysics
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148 148
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of of A A 1989LPSC...19..397Z surface of larger in was be by requires required suggests appears distribution compaction of completely circular over aeolian interior type fill than Zimbelman, that the unit been many emplacement morphology l~ erosional 1986; mass-wasting remnants a The Exhumed a inferred. the Viking surface and younger probably several (B), observed while less-prominent by well Hills, emplaced visible topography gross other blanket local unit more have deposit © graben-like substantial that to rather do remnants images developed (B the Lunar The mantle burial/ produce 1988). craters is over stratigraphy of 1988). mass of they not unit unit ), very consistent places and laterally interpretation exposed crater layering that than presence presumably the craters that closely since erosion were (C). (B) topography wasting. 608A erosion as fresh-looking the loading The has outside highs with Two fractures remnant being and the on in undergoes may in Figure continuous The experienced underlying formed with crater the and Fig. of with resemble 1-16 Fig. of observed craters interior of Mars on of Planetary episodes The be merely (after degree the the the an unit 9, caused the surface last 9 a 11 and/ of are eroding in interior and depositional fill older is or layering by (Fig. crater Utopian fill ejecta; larger exhumation. existence (C) Hills, deduced their erosional a is crater those local deposits or the thought by and morphology topography of 572A have layer subsequent an surface (A). deposits by 10). (Fig. the compaction compaction deposition precludes 1988), into than similar visible crater remnants presumably origin. in Institute incomplete example plains occurred fill Elsewhere sufficiently 1-16 presence from 9). Utopia; In are of than to remnants a 10 (A) episode The fill. hence, in valley-and-ridge two ( be each in all (McGill, units km of Williams erosion Most the (Fig. a that the of a It thickn~ flow of of nue by induced that widespread surface of they in to others centripetal lack disruption is a they of in remnants burial case • is is 9). unit unit occur unit thick produce a material regional possible interior origin. Utopia, or remain buried appear similar visible Provided rather crater crater 1985, have One and (C) (B) (B) (B) can the the to of to in Viking frame Fig. undergone undergoing protected smoothnes.s sculpted km north to 59.8°N, 71 1.3°S, by be m/pixel, crater Zimbelman 10. the 728A62, of from 173.1°W. frame ridges Alba 105.6°W (arrow), Examples NASA by regional of centered its downslope 521883, Patera the NGF the remain rim. (c) et interior deposit al.: located stripping (b) crater The rectiliner Viking of Astrophysics indicates at Concentric in SCR 57.6°S, crater In layer mass an southwest frame rim a version, exhumed of version, being region interior that 305.0°W. wasting. an from crater 578001, erodible (arrow) it eroded 18 of is of crater 17 wind deposits fill Hellas, m/pixel, an Data (a) m/pixel, southern NGF-ortho surface in erosional on from (arrow), The erosion. this Mars is that System too atop centered 5-km centered layer, shape Amazonis extensive have remnant. partially version, this Viking crater wind- and not 10- at at 405 C b 1989LPSC...19..397Z 406 best southwestern and centripetal orders concepts. layer( that required Aeronautics 30° correct, D. the rim. authors earlier Planetary Research No. Acknowledgments. Modification 2. 3. 1. Wilhelms, -60°, 679. ice-enhanced interior © is Fig. morphology. Continued At explained 13 The High-resolution appear s) versions less of were m/pixel, Lunar for ~on there the by 11. Institute, Utopia magnitude the However, completely movement and the the Proceedings S. of incompatible temperatures either Utopia of The Squyres, should strain Space following erosion creep of by centered the the craters and creep crater Viking which the under the manuscript. Staff Administration we crater reveal rate eroded images too be model required and of may Planetary martian The emplacement at fill are contract exhibit evidence believe or reasons. SUMMARY the is small frame of K 35.6°N, in uniform characteristic with produce than rim comments V!Siting not operated of Edgett 19th ice-rich this This by concentric to surfu.ce 328A40, necessarily is no. arguable only. Lunar that crater 272.7°W. the the of typical account This work were NASW-4066 layering Scientists more Institute flow by regolith creep concentric and extent If and paper of undergoing by was most in the NGF-ortho the evidence on of of E. crater Planetary removal the burial/ for mutually hypothesis. supported in Theilig, is a both Universities at the helpful creep of appears with the Utopian LPI ridge-and-valley the the fill • crater deformation exhumation latitudes exhumation sides fill Contribution of the amount of Science Provided craters Lunar in exclusive model version, P. while deposits flow craters. National aeolian several revising Spudis, of fill Space Conference the and the on of of in is is Anderson Carr Carr Carr Carr Clifford Clifford Jones Jones Durham Easterbrook Fanale Fanale Francis Fanale Frey by Guest Hills Hooke Kahn Lucchitta Lucchitta J J Second from of of 92, Mars. Cutts lom 232 Geopbys. equatorial geochemical ejecta Masursky temperature: Salvail deformation regolith New R£s., studies.] distribution Mars: pp. of observations Science Res., of containing ice.J Houston 1-18. distribution deposits texture Sci Geopbys. Geopbys. the Sciences, M. LS. H., Mariner M. M. M. the R, S. 9135-9152. S. 670-674. tbe Conj pp. J. E L 82, E York 84, the R P. E J. J. S. J. S. H. by Lowry Glaciol., Implications In J. H., ( W. Guinness H. A, P., H., giant E., B. D. W. B. NASA 1988) Internati.onal ( A, P. Conference ( M. P., L, M. in 4111-4120. R 8097-8113. Viking Third and 1982) surface and Res., 1978) in Salvail H. Permafrost: Geopbys. D. K (1981) Veverka 17th, B., Crumpler K, region ( M., 462 and Butterworth dispersed 6 Duxbury Masursky Viking Res., Res., and ( Dahlin Washington, (1987) Banerdt 1976) the of and 1982) J. ( rate. polygons in ( of Preliminary B. Schaber and Heard Ferguson National 1979) atmosphere 1977) Buried 78, Gatto 28, debris Wood (1969) pp. orbiter The inf the Hillel Triaxial L, polycrystalline E., J. International 87, northern 84, flow.J ofMars.J migration Icarus, 4073-4083. 7 Astrophysics J., Orbiter 171-177. R, 1be and and Res., for B. Martian Seasonal XIX, Cydonia 8075-8086. 9881-9889. confined Geophys. imagery Polar T., landslides fine H. L .. L and W. mantles. topography Martian H., Zent C. D. G. Conference, D., Research of 1be crustal imaging Arvidson Principles H. Suiface Chase W., Greeley S., Geopbys. REFEREN~ testing 87, C., P. DC. pp. 28, A results.] (1983) sandJ G. B., Mars Wellman Baum lowland and basal M., images Cutts of A S., Geophys. and North (1982) of 10,215-10,225. and volatiles: ( region 495-496. carbon 179-202. for compressive Res., Saunders 1977) Icarus, P., impact and S. composition Mars: and subsurface Kauper of (abstract). experiment. H in Council R, melting of Ugolini evidence R A Glaciol., W. Conference Kirby and 2 J. Res., as The 0 of polycrystalline Valles 91, and Geopbys. plains, Summers pp. American J. ( Guest of Mars. ( Absence a Greeley A, dioxide 1986) Martian A, Res., ice Geomorphology. 1979) Experimental B. 66; controlling Postawko stability craters El66-El74. 82, Their Mars Data Lunar 449-508. implications M. S. Greeley R ( Marineris, of ( E Blasius on at 22-38. 11, 1976) J. 88, Mars. 4055-4065. strength H. Yale of ice In T. Canada. Loss S., from Res., and high Science, E., Pseudocraters 1973) Mars. C. exchange R and degassing pp. of permafrost permafrost 2456-2474. (1983) Lunar (1972) and Contributi.on System on of on Johansen Smith (1986) S. silicic Proc. Univ., R, volatile (1977) of K Preliminary 88, ice. ractor 327-336. National Viking. Planetary pressure ground E. J Mars. fine-scale emplacement Mars. of R, Permafrost, An Guest for and 193, B377-B392. ( and In Geopbys. polycrystalline Lunar B. 1986) Experimental volcanism Creep McGraw-Hill, New between examination Briggs in Sedimentary the history Proceedings J A, J abundance. Icarus, features. theoretical terrain 766- Geological L. ice Planetary J. the Academy Geophys. on and Geopbys. Institute, A., Soderb- inferred E., Haven. surface to Planet. results Global in of origin G. 776. Mars. Res., low and and and the the the 67, on ice A, on of J 1, 1989LPSC...19..397Z McGill Mutch Mouginis-Mark McGill Paterson Scott Sharp Sharp Soderblom Squyres Variations plains. and (abstract). Morris Geophys. Geophys. Res., Icarus, 82, 380 region surface distribution 331-342. D. R. R. 4039-4054. Planetary pp. G. G. 78, T. S. © H. W. P., P. Geophys. of E. 34, E. W. E. A., 4117-4122. of ( Res., Res., Soderblom L and Lunar S. Mars.J C. 1973) with ( In 600-613. (1985) (1978) B. A, 1986) Mars, of Arvidson ( P. Lunar Institute, Tanaka 84, ( 82, 1977) a 1981) Kriedler crater Res. J. 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