1981mrbf.conf...91P Bouguer the Grimaldi, of can Abstract-Grimaldi the plug Spacecraft called crust-mantle It +90 theory to material, basin. and adequate lunar major Bouguer the the which resultant previous Sjogren, studies Phillips, the western Grimaldi mare slightly Below, the has 1 the Lunar topographic formation be The south available milligals surface of Yates, © covered Bouguer mascon, attributed of In lunar are difficulty been mare Lunar mascons, have gravity outside probably limb it 1978). and 1968). gravity analyses is this mascon Bouguer oorpi coverage topographic we free-air and based origin is boundary 1970), a mantle at geology. known fill Planetary been suggested of present and small lunar paper, gravity of southeast correction region an signature since The to the (Conel the has on data formation: the gravity a Survey, altitude Planetary are is the or restricted material. of gravity combination multi-ringed dark gravity a gravity concentric for inferences mascons been are of and Roger we to Multi-ring moon the a relatively mare of Institute, almost The over associated that brief and across a the data reveal requisites. to show Oceanus structure central (Fig. lunar of 345 Bouguer combination circumvented profiles The material the the final Grimaldi. Institute crustal 70 and between Holstrom, past to Basins, description Middlefield total are this J. 3303 local remaining outer 1). kilometers. that small uplift only of Schultz made associated basin, section patch has topographic Phillips ten of The generally basin. with ejecta INTRODUCTION Procellarum Proc. mascons: collapse gravity NASA lying a with topographic a lunar large multi-ringed scarp was a mascon • not P. sub-mare the years about Printed GEOLOGY consideration diameter Lunar Provided of partially H. of 1968; Road, It mare-filled within positive several and caused of gravity of been lunar and Road in Approximately mare larger is of both associated by Planet. 1 in the thought this proposed that the the associated Merrill in Grimaldi. 91 U.S.A. Phillips and data Menlo the ring One, craters available by material; situ to mass geologic plug basin field by Bouguer filled of possible analysis model Sci. Orientate coverage with paper large R. inner Analysis inward the faulting the the for Houston, John (1981), B., breccia, nearside Park, to indicates of and that located contribution comparable by eds. with et east. with NASA In positive inner Grimaldi, ring be calculations the discusses 20% anomaly Grimaldi 12A, setting al., to crustal mare the Grimaldi structure fill of addition, California shallow and is Dvorak Basin the of large free-air is The yield Texas p. of on Grimaldi, (Bowin outer ring 1972), a Astrophysics now this circular 91-104. required inner material, central maximum this the collapse of free-air of inner in lunar is and is Bouguer to supplies basin. 77058 these an is disk-shaped ring western size available Grimaldi, of positive due 94025 lunar to ring the roughly proposed the required et 2 annulus this uplift a a to ring craters basins the to to is which al., From of comparison which gravity Bouguer mantle results west 2 fully gravity the a U.S. best a Bouguer Data lunar this limb Bouguer nmle. This anomalies. critical smallest of centrally 1975). to 200 central for a a of also Geological Grimaldi to reproduce and (Dvorak for depths structure, preserved (Muller consideration lies summary System of masses plug basin in low anomalies, kilometers anomaly data match this resulted test the Previous Grimaldi the near view anomaly basin uplifted known density of (Wise of moon. in lunar since from vast due and and and lies the the the the the the of of of of to in 1981mrbf.conf...91P 92 probably (Wilhelms (Fig. (1971) and of interpreted interior tion northwest (Model Grimaldi analyses These Fra Basin. the this the serve central carried Head's Mountains ment Grimaldi The the © failure final Mauro that of model, 2) (Melosh, Lunar to immediate craters structural determined multi-ring basin. shows (1974) I), to over, Fig. basin kilometers. of with position is evaluate lies R. and Grimaldi and the are strength a as Formation the is the and 1. J. concentric no the apparently other inner that model impact the Grimaldi. McCauley, equivalent Portion 1977; pre-Orientale Phillips outer inner Planetary identification more surroundings basins, of peak mare the the Grimaldi is impact of ring Malin the of ring at of ejecta ring region surrounding than implications the and ring in fault the Lunar a Total of we slumped undergo to Institute about 1971). level Oceanus of surrounding and features. Grimaldi, J. a Orientale the discuss of from to within in scarp few Grimaldi Orbiter Dvorak of and picture Dzurisin, 1.0 Grimaldi be peak 400 Based age the collapse rim the hundred • that the kilometer resulting approximately Procellarum of the only Provided kilometers. Although two photograph surrounding since ring basin. Orientale of width Imbrium the the on is country inner 1978; must two rings craters. comparable in of relative region geophysical meters the from In smaller below (east-to-west) a ring by contrasting numerous of transient be Settle (IV-168M) the event The rock Basin, the to Hevelius greater the between Grimaldi is the crater buried from contemporaneous the latter the NASA 1.0 craters, radar (Melosh and deep stress and to east. superposes mare to modeling. crater the statistics, detailing models than the views interpretation, Head, under Astrophysics 1.5 is Formation, the topographic central is is field pre-impact and, in probably Outer important approximately kilometers concentric and about rim the which the 1979). exist of the if basin, In Hartmann Grimaldi McKinnon, with crater the the Rook multi-ringed volcanic 15 with one for Data will which The analogous map crater km for analogy level. modest the below is ring Riccioli the interpretation Mountains subsequently the analogous System outer comparative in 500 of Inner to and configura- structures exceeding fill The has diameter. this 1978). the the Nectaris enlarge- is of rim to Wood to Rook to mare level been west area the the the be of In to in 1981mrbf.conf...91P Observatory in that Fig. be outer time with Grimaldi and by energy differences is kilometers energy Basin. the may both possibly similar fallback tains, terrain Fig. The In also attributed the 2. the pitted © Model a of a have correspond 1. ring, composed Earth-based Lunar crater geomorphology second This outer composed topographic The for to similar is crater ejecta because inner the the 74W and a above map which, Grimaldi (slightly II between region steep ring. and rim, to is Cordillera same view formation crackled ring. to contour at intrinsic in of Planetary the of to radar but Orientale of It the crater as inward is modified). the (Model rolling The resembles for a the is a the laced level in is domical 72 more interval partial of topographic significantly relative instead bowl Model appearance Grimaldi two space-time principal corrugated Mountains, (e.g., Grimaldi facing of Institute with and II), (Head, advanced This features of the used here ring facies the see I, there energetics hilly uplifted Grimaldi large topographic scarp interior 70 is and difference (ERT) of Outer Croft, favors 1974), • differences larger a is terrain facies which is massifs surface between Provided is ring is for stage more which significant lower is 400 attributed map Rook mare also 1981). constrained Model of than Humboldt, fault. meters. form described with map of 68 is subdued of cracks the which rises crust occurs and the by the Mountains degradation. in Grimaldi the The covers The The a impacting I. the the the structural It primarily formation Outer to slight a impact The created lie is (on important few within NASA origin inner between almost outer moon here evident a by approximately exterior 66 provided crater inner the radial Rook kilometers of Head energy than the ring, ring Astrophysics by of body. itself. eastern The deformation to the from the of ring the inner lunar the of this contrast texture and to an of maximum is however, by (1974) Orientale outer this In similar inner In for a of rebound 64 exhibited outer Orientale, aspect. S. ring side the the region above mascons Model Model and Grimaldi Zisk Humboldt, ring and for same and structure. Cordillera between Data of ring, the extending diameter has of Basin height the the (Fig. of process interpreted II, the previous outer rings I, at region the System in which 62 Grimaldi the little the rises basin), interior. Orientale, Orientale that Haystack in 1) Model reached and impact impact Moun- shown to which that to at to figure three must they but the the the the 93 do as in A is it I
1981mrbf.conf...91P
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Planetary probably history Ridges A fault geologic large dashed in ring second from in this resulting are Orientale of thickness Other of Institute greatly where paper structure shown we the impact Grimaldi major structures will Grimaldi from inferred are in modified Basin • from show rebound. the of geologic the Provided the is mare-covered Grimaldi. outer unlike depicted or a to region that volcanic few extrapolated, the the two The event the by an hundred pre-existing west, The is are the Concentric in gravity load uplifted dominated argument central this rilles. origin NASA was which in with figure. meters interpretation the the Adapted crustal basin of Astrophysics scarps ring tectonic not central here lunar by vast The to of only structures two from ring, indicated a Grimaldi innermost from volcanic mascons kilometer basin. grid events. deposited Solomon and favors Data geologic of and Mare by are thus ring the flooding System The arrowheads. (Moore in shown Model and material units Model western shown Oceanus first obser- Head are for II. 95 of et is is I 1981mrbf.conf...91P % material Oceanus ring Evidence mostly region :flooding be surrounding general, some Head Procellaruin well ridges Stark (Solomon from The litatis Both tectonism respectively, lunar from basin, differentiating the signal as gravity These of analysis altitude Grimaldi. variations provided data available of components. longitude determined 1978). see samples The The The In The this 3.0 it the accelerations of lunar gravity Zisk, as © this gaps feature the passes of and (1980) lithosphere, (Dvorak the ought to ± within tectonic interior existence contribution modified Lunar three free-air Grimaldi, lunar other lunar and 0.1 these of of in the of the (Talwani gravity Procellarum analysis, by for and Head, orbital The has and R. in superposition 1972). within the Oceanus lunar the by youngest b.y. to and Grimaldi and are the types are spacecraft over or resulting low gravity J. the and impact the gravity been LUNAR are with structures two be and Head, use highlands, to Apollo features Phillips poor gravity by orbits 1977). are data. due of are (Boyce, craters inner A and considered Planetary coverage data earlier altitude undergone shown Grimaldi the the resulting several of et Phillips, Apollo respect previously the of crustal these shown Procellarum, undoubtly data determinations structures) to the al., volcanic 1980). and the field, to seen from load lunar consist the ring shown However, 15 (Sjogren and Orientale profiles, GRAVITY associated of the are of occurrence as earth-based the including 1973), 1976). possibility have profiles sub-satellite orbital circumferential are surface 17 to Institute various of associated here of are from are density 1979). these solid J. the Circumferential local crust. in combined parallel by CSM time in east of Grimaldi Dvorak noted interpreted units Grimaldi the been related considered. interpreted stress in Fig. has a which This et the these lines expressed event. loading passes 2.5 of profiles the (Grimaldi) topography interpretation spacecraft and al., Fig. ages orbits Previously, volcanic with • of on of line-of-sight for and been of of discussed the 5 radar ± Provided is AND Doppler with field in was or 1972, rilles 2.8 0.5 to the is effects the are 4. major the volcanic the and The either local somewhat Grimaldi shown Fig. perpendicular by was range attributed the tectonic Rilles to gm/cm b.y. assumed contain topographic surface Grimaldi, accelerations estimated imposed approximately as These Lamont extrusion in show sizes flooding TOPOGRAPHIC 1976). rilles age the be 5. in volcanic and accelerations deemed to intrusive by shift extensional of (Boyce elsewhere was a milligals, in Since occur in of the close 3 (i.e., the volcanic of activity the , similar (Dvorak the apparent altitude exterior have accelerations regional features of any both The typical Fig. in older in the to structure by repetitive result NASA although local from of the earth-to-spacecraft) this surface the unsuitable throughout lunar of and loading (ERT) computing the subsurface to peculiarities the activity last 5 been the vertical from moon. at technique are (Gottlieb, earth-based transpondedradio than isolated flows the were 90 is free-air from and crater of loading of and Johnson, to Astrophysics local undergone load suggests stress region fl.ow Grimaldi orbit. the kilometers. map in the mapped plotted tensional values western a the relief of Phillips, of the compressional 60 used throughout western circular in line-of-sight are control on for and degradation units that rilles DATA most original density this the for gravity They pockets fields. history to the interior last 1970; a in was termed this and 1978), that for in 70 horizontal this would lithospheric as basin coverage the by by edge topographic apparently result which central of Data 1977, stress major by the Mare are mass kilometers; analysis applied The lunar lateral a flexure the model component Phillips field This region Solomon Doppler the interpretation of representing to Grimaldi of this of function ( the System analysis derived component have spacecraft 1978). models that cover Whitford- remaining highlands the fields. Tranquil- load features, Oceanus Grimaldi volcanic volcanic has highland type derived free-air region. already density (Fig. gravity of to due et inner basin shell. been data. been con- and and the the (as the the al., by In to of of of of to 2; 1981mrbf.conf...91P for Fig. V) back- to lunar error mare units of may pre- The into low and and and the the the by by be its of or 10 its or is a 3 1981mrbf.conf...91P have crust Ferrari, mare density probably corresponding as component tributions represents Each Fig. within shown fresh comparison distinguishable mare the three the and edge, lunar Indeed, calculations Fig. V, .... (!) .... < .... To In The - magnitude Bouguer 6. 100 6. -20 -40 Head 0.4 © each densities of 40 60 80 fill 20 fill summarize, of basins, to crater attesting A The simplest the Lunar 0 in must 1977). gm/cm islands +0.1 these five in comparison and in from Fig. (1980) of Grimaldi. described uncertainties the characteristic arising the of (190 gravity kilometers such to and be associated the calculations of to GRIMALDI AP 3 which 6 to by the mare of ; ejecta model 72W range + and close have km an the proposed Planetary the there 1.0 calculations 17 pre-mare considering as from present of profile. increase in that rim Bouguer This gm/cm CSM fill Mendeleev shallowness are a of or shown the been to Bouguer are for material of intrusive diameter). resulting from and of brecciated + different text. the model ------_.,_, are REV Institute depth 0.6 a This the subfloor 3 this each three obtained ; in 70 basalt in anomaly is the mean compared multiple to to 3 thickness porosity gravity Fig. -- analysis, combined one requires (6 crushed model __ of be density of possible material + from km, The • fill density material appear 1.1 Grimaldi 6 component mare presented, for Provided has profile and BASALT BASALT BASALT BASALT BOUGUER orbits. LONGITUDE ejected gm/cm model Kaula will maximum of with the at of the and 1/ contrast the fill. only 68 components is 30%. with may out least be of the FILL FILL density FILL FILL across and unable other the various brecciated (1.0 3 et for GRAVITY by material discussed ; the to (4 one (15 (3 (20 mare is a have The the various al., 15 single from km)+ the km)+ some km) between km) Grimaldi rejected component fill km)+ Grimaldi moon, orbits kilometers component to density 1973), of origin NASA material thickness models EJECTA+ a MANTLE fully with vertically EJECTA may Bouguer associated distance 6 64 66 normal density by combinations shortly. used that gives as of the with Astrophysics based reproduce maximum be the contrast PLUG MANTLE a shown lunar within has of as lunar is, reasonable lunar in the representing in impact contrast from gravity a displaced Similar mare much on this their 3.4 maximum been with results PLUG mascons mantle of in Grimaldi. crust. gm/cm the the the depths fill analysis, of may as model Data profile Fig. Grimaldi the included results with of Grimaldi geometry eastern to possible - model lunar several and The low 3 be 0.8 the account System 6 estimate of (Bills is the shown were Solomon as gm/cm to so circular crust density mantle. unfilled central 3.6 since end of which which much those lunar 62 model basin that, con- of and km. not for 99 of in is 3 a a , 1981mrbf.conf...91P 100 Grimaldi. can contributed in the mantle maximum reasonable component at This density listed gravity kilometers mare within here remain unrealistic adequately component density kilometer thickness product anomalous above, of inner Fig. surface density-thickness The The By Fig. 100 7. full be © gives fill. interpreted ring; fixing in Schematic next 6; fourth the and geology. Lunar approximately plug profile. that of accomplished would extent of Table what For For radius products inner -2 R. radial amount of 200 however, a these value reproduce model density is by the is, at realistic model J. and a any these to is mare poorly be I. The Horizontal kilometers, of a model product Phillips cross-section 4 ejecta ring, also amount and -4 two extent The by Planetary depth as estimated listed depth kilometers, 1.5 the of of details components. calculations, fill calculation gm-cm- required the the the uplifted then mare components constrained value constant. pre-mare the by km consisting the ejecta-breccia and (ll.p surrounded in and of has of of gravitational ejecta-breccia addition and a observed it Fig. mantle respectively, · of Institute fill, 60 mare 3 t). of this in ring for such the J. has -km. vertical is this lunar Grimaldi Cross-section there kilometers. Dvorak 6 approximately situ shown a A isostatic consequences the a annulus attempts the of of component Modeling that fill The low of plug model by vertical necessary by only gravity brecciated GRIMALDI • amount low scales INNER remains mantle region to a zone the Provided effect third the density in (100 determined a and separate zone that the model, density mare Fig. are very in gravity to net are t relief However, is associated between component the km) signature the acceptable RING of of these material. reduce which as along determined shown to 6 a the 20 component mass of thick fill by is this crust mare a pre-mare reproduce slight that mantle of high kilometers. from material broadening same. a thin the and data; radial model can 20 combination component deficiency the in low the is, NASA the fill (Fig. the associated density to a annulus with annulus trade with The Fig. Ejecta-breccia narrow variation is from however, amount the plug low two 30 density and by gravity introduction crater a may such calculations, the 6), 7. high Astrophysics kilometers. Grimaldi. lateral model density the off basin the gravity the concentric as adequately component It but Bouguer the also of would data of as of bowl consists between fourth density a in annulus with this if center. gravity again required in thin all that be the extent inner and zone ring it which three are By component present be of the is OUTER density-thickness gravity model a consistent disk rings which profile Data plug this it of (200 is reproduces confined and masked with a signature. representing the increasing approximately lower of is formation expressed components. mare high three the requires with System of possible is outer other within this described a km) as might RING profile taken material density- surface density surface fill with by shown to would a to third This radii to five two as 100 the the the the the be an lie of as to is a a a 1981mrbf.conf...91P equal, kilometers produced for Orientate consideration coverage models material, An thin annulus, the part apparently follows crater fault correct, purposes. specification (1980) associated other lithospheric likelihood, the the proportional of contrast negative be density amount not young A The on this low analysis Orientale latter time extend surface © of (and critical regions the rim *Isostatic Density-thickness Volume lunar have is modeling Lunar listed size density annulus from this of then (gm-cm- (t.p Low Mantle to and of there annulus indicated. by of order authors Basin presumably Morphologically, and ejecta with is beyond and Model relative formation, = collapse. craters (McGetchin provided similar component disk the the a to of Density in the and an an issue consisting of +0.7 of of third is the Plug Model annulus of Table 3 crater the the the is -km) Plug explanation results analysis crater only the only by insufficient the Orientate case between Planetary still representing showed I, gm/cm 5 an outer the (Dvorak crater to component in stresses kilometers density and In Ring to Sjogren lunar (km in appears I a for central product diameter the slumped the bowl. the are this to other raise hypothesis 3 of situ 3 ring the may DISCUSSION ) ) et by free-air Grimaldi. that the be rim, Table one lithosphere frontside Institute initially the Basin al., it interpretation high calculation, negative and of Melosh breccia induced is is a and due also uplift) seems to rings craters thick, the the same presented required since a serious of crater the 1973; I. and Phillips, be density ring to gravity. was high Gravity Smith be magnitude interior sub-isostatic; in lunar is • excessive the and zone formed zone and (Solomon inversely components that annulus by size considerably fault Provided Pike, rim, due interpreted regard beneath formed not 4X density question topographic as -4 the the McKinnon material 10 similar 1977) (1976). models here the is crust AND 10 They thus to of (Model available, to mare 5 1974). the topographic pre-mare is to a inner why of (Settle, the proportional by material for strongly and Grimaldi at questioning fallback low also to sized fundamental The regarding for this SUMMARY that horizontal However, which at MODEL the by presented as in If roughly 5x Grimaldi I gravity Grimaldi be Head, Grimaldi. ring depth (1978) -3 low in density 13 origin an proposed excess the 2 NASA apparent the is, they 10 basins 1980). 2.8 crater "Geology" placed indicate 5 ejecta before is ejecta of was of impact relief outer gm/cm to 1980), the regarding surrounded restricted of the the results the Grimaldi Astrophysics to extensional of since has here developed Most ejecta balance did relatively parameter lunar depth validity at 9X lithospheric blanket a disparity. most within interpretation basin of the ring that same event, -2 16 been three-component not. 3 3* thus depth. for • 10 a likely, adequate section). emplacement All for 5 and mascons crater. estimates the is ring was the structure; marks Head Grimaldi: their the imparting conducted of time only, but the by thin a other They stress breccia Grimaldi Data for breccia mass Their part fault crater, concentric Model taken a our crater analysis thickness. and In If compared the comparative or then topographic low of System interpreted of acceptable for Model deficiency particular, is formation studies argument however, a Solomon the zones later, slumped a then to zone I. this of directly density for it central craters rim, is model higher If mare inner be must to ring low 101 the I the the the At do as of of to in is 6 a 1981mrbf.conf...91P associated of anomalies analysis inner 102 the the pre-impact (Dvorak -120 Grimaldi anomaly inner Grimaldi ligals. anomalies an have mascons. milligals more topographic ring similar Specifically, earlier studies earlier associated extending connection with due the material mare-filled rilles particular, undergone subsurface. supported intrusion inner low The Given The The Independent the altitude concentric basalt same to in density © and basin these milligals, ring, consistent basin association inner As presence question the Model Lunar positive of centrally so and that of from into is ridges is depth fill and to R. of bending the with flexural the the basin with by of that some level, of It low a Grimaldi well the basin, of Phillips, annulus Grimaldi the J. and -10 (3 is the 400 70 I. many Grimaldi. outer gravity structure which have the the two of the naturally Phillips anomalies of quite a the filled associated Grimaldi In to density and isostatic as Table Crater Free-air Bouguer kilometers + with uplifted outer known crust Planetary km the of these zero to crater an 70 bending of finite present 5 either large formation then is crater ring. if a a likely basin showed kilometers) 1978; choice diameter milligals. -20 extensive due a multi-ringed data positive not all exhibits shallow presently Model Bowl could Bouguer II. ring. density and usually two In Gravity zones; Gravity se Phillips (see arises bowl From craters by there strength interpretation, anomaly Gravity suggest to associated milligals over diameters with Bouguer Institute that in with rough Dvorak, is J. inward of other In craters explain that flexure? response of II, Dvorak Bouguer +60 contributes If shelf a our mascon boundary, this as models, attributed ejecta-breccia old must these this they those anomaly both (Spacecraft within positive Pasteur is Pasteur numbers, in all to basins values of mascon that studies associated milligals lunar positive crustal at stripped gravity • 1979). region view would this (- whether which impact with a are Provided basins. be and the associated an Solomon to ring anomaly basin 200 it this Grimaldi, the craters and anomaly. free-air a (Dvorak and are the for most to altitude is in +90 -30 +60 -190 there Lambeck, of lunar collapse large basins (Phillips Altitude at the km) structure anomaly mass (Table still Present instructive existence there the crustal away, features Imbrian type Humboldt volcanic undoubtedly displaying or this milligals zone Grimaldi-Past Humboldt with by present likely milligals, and gravity with lunar has is and not have lithosphere. with is gravity the altitude excess of and that is 70 of for no II). then between Grimaldi the rebound. et shown depths is there NASA and a Head km) 1980 70 and of significant craters removed craters loads of al., gravity which remaining due slightly multi-ringed Phillips, The rather free-air to is, data. were the the Imbrian kilometers; have a anomaly a leaving older has associated compare -190 - 1974). for is +70 to vast within massive breccia that Astrophysics (1980) crater 120 (- Pre-Mare is the pre-mare structure a the and is filled higher In of a That robust comparable a attested 3 significant essentially signal negative milligals craters, it gravity value approximately each accumulations by 1978; km) two particular, the review), What surface structural age a crater present. one bowl in with performed net zone the basin and basin density magmatic the density same rings they development similar of conjunction or of with was Dvorak, free-air of would to positive kilometer over gravity these mare conttibutes Data lithosphere rim +90 manifestation older free-air contradicts mass is a flexural by size. of zero would in is excess in this produced deep unlikely lunar deformation to Grimaldi per milligals. the Grimaldi System size material distinguish part the features processes a gravity no signature of 1979). +80 the excesses A Bouguer Bouguer feature. annular flexural se, gravity lack central mantle not of with recent signal, longer to of basalt of deep - mil- that and our has the the the the the be 30 In of to at in If is is is is a 1981mrbf.conf...91P model favored. of of ago." as ciated of Grimaldi intimately these help, process boundary between displacement faulting, and analysis out deposition Imbrian Dvorak models may relatively Acknowledgments-We magmas Cone! Dvorak Dvorak Dvorak Contracts Bills Boyce Bowin Boyce Space Gottlieb Space Croft the and lunar basin-filling 80, librational photographs. Lunar The 1403-1405. In A Basins, Grimaldi, the impact. is © by the B. and be conclusion, remaining 4947-4955. the S. moon. crustal two J. Research Administration. Lunar J.M. The lunar C., is J. results with J. craters. G. J. J. K. J. Head P. a proposed. Planet. gross E. of of J. that and with The and the N maximum M. - ~ Proc. and was (1979) Simon process and undisturbed. (1981) and is lines (1970) Head, ASW associated and of the mechanical corresponding and W. Proc. and geographic lithosphere history. Phillips (1976) a and history. Inner filled Phillips Pre-Imbrian reader 0.1 the in Ferrari this Phillips of (1977b) Proc. "at subsurface Geophys. Sjogren requisite Lunar Association Holstrom Grimaldi Johnson Sci. seismic The Analysis of 3389 B., question P. Estimation the Planetary this gm-cm- Lunar we formation associated facies. least evidence. the Schultz, Geomorphologically, and Rook Ages Conj. modification Lunar R. displacement Ph.D. and This Proc. annulus may would R. A. Planet. wish study R. with for J. inner for data. Wollenhaupt D. That failure Planet. Res. J. J. location, N 50 due (1979) G. of for load of J. 9th, paper 3 and AS7-100. providing A. concerns (1977) -km, (1977) Thesis, wish Lunar under to Sci. structure km flexural structures Institute and the small of (1978) B. crustal flow argue do J. Lett. Sci., the of to basin (1978) is, thank p. region and intimately local Outer (1968) Gravity Geophys. Conj. Sci. constitutes S. of at megaterraces, or the not Orientale stage 3651-3668. to the A Contract The formation Planet. scale units 12A 4, Cal. Croft Lunar the since the concluded no of The lunar that use S. 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