“s ' ‘w'w . ‘ A GRAVITY SURVEY IN THE VI-CINITY OF ; MELLEN, WISCONSIN O 421—“— Thesis for the Degree of M. S. MICHIGAN STATEUNIVERSITY JONATHAN BORK‘ _ 1.967 é€$%3n&m . ABSTRACT A GRAVITY SURVEY IN THE VICINITY OF MELLEN, WISCONSIN by Jonathan Bork In June, 1966, a regional gravity survey was run in north-central Wisconsin near the small town of Mellen. Most of the survey centered over the Mellen Granite, a 3-by-5 mile acid intrusive found on the south limb of the Lake Superior Basin. Due to glacial cover, complex faulting, and considerable intrusive activity, the geology remained obscure. Therefore 220 gravity stations were occupied within an l8-by-lS mile area to define the structural geometry of the Mellen Granite and the gross geology of the surrounding area. The Lake Superior Basin is an east-west trending, assymetric, Precambrian trough filled with Keweenawan basalts and sediments. With the center of the structure underlying the lake, the outcrops, including thick gabbro sills, appear predominantly around the edges. In Wisconsin the Keweenawan series rests unconformably on erosional remnants of an older geosyncline. The Mellen Granite lies on the more steeply dipping south limb surrounded by Keweenawan mafics and sediments. Gravity stations were observed at intervals from 1/u mile to 2—3 miles depending on their proximity to the Granite. A total of seven base stations were occupied Jonathan Bork throughout the area and were read at two hour intervals to eliminate drift and tidal variations. All stations were tied to the international network of gravity values. Stations were located on topographic maps with the aid of an automobile odometer. Station elevations were observed with an aneroid altimeter and tied to points of known elevation. A C. D. C. 3600 digital computer converted all gravity readings to milligals and corrected for variations in elevation, latitude, drift, and near surface mass. Terrain corrections were ignored. Rock samples were collected from important sedi- mentary and igneous facies with their densities determined by the water immersion technique. A large density varia- tion was found in the sixteen samples taken from the granite. The granite varied from porphyritic granite (2.65 gms/cm.3) at the top of the intrusion to diorite (2.78 gms./cm.3) found near the base. Overall, the average density was 2.72 gms./cm.3 A The Bouguer gravity map revealed a gravity maxima traversing the area in an east-west direction with gravity minimas to the north and south. This maxima, part of the mid-continent gravity high, coincides with high density basalts and gabbros. The Bouguer gravity anomaly was separated into regional and residual components by graph- ical and statistical means. Both yielded the same type of regional map; however, the least squares residual map was inferior to the cross-profile residual. Jonathan Bork The residual anomaly over the Granite was a steep- sided, flat-bottomed gravity minima of 6-7 milligals. The anomaly did not close, however, due to the lower density sediments found to the north. In general, gravity maximas were found over the high density gabbros, basalts, and iron—formation with minimas revealed over schists, gneisses, Animikean metasediments, granophyre, Keween- awan sediments and the Granite. Two kinds of faulting were interpreted in this area: thrust faults parallel to the east-west strike, and cross faults which are perpendicular to the strike. One thrust fault runs across the entire north of the area and may connect the Lake Owen thrust fault, found several miles to the west, with the Keweenaw thrust fault traced into the eastern portion of the area. Two and three dimensional theoretical gravity pro- grams were used to calculate the anomalies of various assumed body shapes. The anomaly of a rectangular- shaped slab, 2NOO feet in depth, with a density contrast 3 of -.21 gms./cm. fits the Granite's anomaly reasonably well. ‘A GRAVITY SURVEY IN THE VICINITY OF MELLEN, WISCONSIN By Jonathan Bork A THESIS Submitted to Michigan State University in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE Department of Geology 1967 ACKNOWLEDGMENTS I want to express my gratitude to the following people without whose help this investigation could not have been completed: To Michael Katzman, who made known to me the details of his investigation, aided in collecting samples, and reviewed the initial manuscript, To Graham Williams and Michael Spurgat who assisted me in computer programming for the gravity reduction, least squares and the two-dimensional gravity calculation programs, To Michigan State University for donating the time with the C. D. C. 3600 computer, To Doctors Trow and Bennett and my colleagues at Pan-American Petroleum Corporation for evaluating the initial manuscript, To Doctor Hinze who guided me from the beginning stages of planning through the final writing and inter- pretation, and, lastly, To my wife, Mary, who performed many of the onerous calculations and typed and proofread the manuscript. ii TABLE OF CONTENTS ACKNOWLEDGMENTS . . . . . . . . . . . . LIST OF LIST OF Chapter I. II. III. IV. VI. VII. TABLES I O O O O 0 O O O O O O FIGURES O O O O O O O O O O O 0 INTRODUCTION . . . . . . . . . AREA OF STUDY 0 o o o o o 'o o 0 Geography . . . . . . . . . . Physiography . . . . . . . .> PREVIOUS INVESTIGATIONS . . . . REGIONAL GEOLOGY . . . . . . . Introduction . . Stratigraphy . . Intrusives . . . Faulting . . . LOCAL GEOLOGY . . . . . . . . . Introduction . . . . . . . . Stratigraphy . . . . . . . . GRAVITY SURVEY . . . . . . . GRAVITY REDUCTION . . . . . . . Introduction . . . Observed Gravity . Latitude Correction Free Air Correction Mass Correction . . Terrain Correction Error Analysis . . iii 0 O O O O O O O O O O Page 11 vi tUOLAJI-J \ON Chapter VIII. IX. XI. XII. BIBLIOGR APPENDIX ROCK DENSITIES . . . . . . . . . . . . INTERPRETIVE TECHNIQUE . . . . . . . . Introduction . . , -. . Least Squares Statistical Technique Cross- Profile Graphical Technique . Theoretical Gravity Formula . . . . INTERPRETATION o o o o o o o o ' o o o 0 General Remarks . . .-. Regional Magnetic Anomaly . . . . . . Regional Gravity Anomaly . . . . . . Local Gravity Anomalies . . . . . . . Interpretation of the Mellen Granite CONCLUSIONS . . . . . . . . . . . . . . RECOMMENDATIONS o o o o o o y o o ' o o o o APHY o o o o_o o o o o 0'. o o o o o o o o o o o o o o o o o o o o o o o o o ’ iv 0 O O O O O O O O O O O O O O O O O Page 77 81 LIST OF TABLES Table Page 1. Density of Rock Samples . . . . . . . . .,. . . A3 Figure LIST OF FIGURES Area of Investigation . . . . . . . . . . . . . Stratigraphic Succession of Precambrian Rocks in Wisconsin . . . . . . . . . . . . . Generalized Geologic Map of Wisconsin . . . . . Gravity Station Location Map . . . . . . . . . Density Sample Location Map . . . . .‘. . . . . Elements of 3-Dimensional Gravity Calculations Bouguer Gravity Map . . . . . . . . . . . . . . Regional Magnetic Map . . . . . . . . . . . Least Squares Regional O-3'rd Degree . . . . . Cross Profile Regional . . . . . . . . . . O-3'rd Degree Residual . . . . . . . . . . Cross-Profile Residual . . . . . . . . . . . . A Composite Geologic Map . . . . . . . . . . . Observed Gravity vs. Computed Profile (N-S) Observed Gravity vs. Computed Profile (E-W) . vi 0 Page 11 16 3LI LI1 LI8 52 5n 56 57 61 62 63 71 73 CHAPTER I INTRODUCTION In the spring of 1966 a gravity survey under the auspices of Michigan State University's Geology Depart- ment was planned for an area in north-central Wisconsin. The survey was centered over the Mellen Granite, a Precambrian intrusion, and was timed to coincide with a simultaneous geological investigation. Michael Katzman, a Ph. D. candidate from Michigan State University, conducted the geological survey of the Granite. The Mellen Granite lies on the south limb of the Lake Superior Syncline, a Precambrian trough. Certain features of the granite make it an interesting subject for investigation by the gravity method. First, it is singu- larly located in the midst of mafic intrusives which stretch scores of miles to either side. Second, the geology of this area is particularly difficult due to the extreme faulting and deformation. Third, the northern sector of the granite is covered with glacial drift which makes actual outcrop surveillance impossible. With these problems in mind, the survey was planned to determine the structural relationship of the Mellen Granite with the surrounding rocks. More specifically, the object was to determine the areal extent and structural configuration of the Mellen Granite. CHAPTER II AREA OF STUDY Geography Most of the survey was centered about the small town of Mellen, Wisconsin. Mellen, a town of 1000, lies Just to the east of the Mellen Granite in country of moderately rugged topographic relief. Roughly one-half of the survey area is government owned forest land that is thickly overgrown. Much of the remaining land is owned by mining companies. Twenty miles to the north lies Lake Superior and Ashland, Wisconsin, a city of 10,000. The prominent Bayfield Peninsula lies immediately to the west of Ashland. The area of the survey includes townships: TAAN,R2W; TAAN,R3w, THAN,Ruw; TASN,R2W; Th5N,R3w; Tusw,Ruw; and the southern halves of TA6N,R3W and TA6N,RAW (Figure l). The entire area lies in Ashland county between latitudes 46° lA'26.3" and A6°27'33.8" and between longitudes 90°33'A.2" and 90°55'33.2". The area approximates an l8-by—15 mile rectangle centering over the Granite with the extreme northeast sector removed. This sector is part of the Bad River Indian Reservation and was inaccessible. _ $39... zo_Eo_5m>z_ Lo 3% muz> .Z “.0 n_<_>_ 010040.”.111110 QMN_I_40 I IIIIIIII IIIII IIIIIII III/I ... \ IIIIIIIII IIIII .. .U>5 \\ .Qv \ N tho ”WNW 1t O . l l 0' .—. o .0 9w 0 3w 9&0 am 0 c . I no I 0' F Qfi L3 ‘20 O G V! ... ....» o o o ‘30 h! s 2‘ 1 3: u! a! o \3 sin”. ~30 n! o k . 0 o o o o o o c o q ‘o t x v! a! o 93 9! ix N: .i o h! bum. o .3 % I o 0 o n h! \2 I o o 9% s\\ k“. k. 1. .6 \ x O O a: CM 0. 1 r .n u 1 2 _ 1 _ 1 1 .n u 0 o I: \n? .1 90., :O‘ I I n .m V n H _ Us. 0 :0 o o o: ‘0‘ o Obxo Q.\0 8‘ 2520023 .ZmJIEE _ l1 . 1 O O O . . oonw Iq%\ 1! d9 3‘ ’ N K 3 n I ’ t K o n O O .0 \Orn \nbfl \Opt h»? \Opn \ p \ b CHAPTER VII GRAVITY REDUCTION Introduction Observed gravity values are read at stations with various elevations, latitudes and terrains. To make the data useful for these varying situations, corrections must be made. After these corrections have been made, the resulting value is called the Bouguer gravity anomaly. The complete Bouguer gravity anomaly can be cal- culated with a computer according to the following equation: nga = go—gl+ge-gm+gt where: G = complete Bouguer gravity anomaly go = observed gravity gl = latitude correction ge = free-air correction g = mass correction gt = terrain correction 35 36 Observed Gravity The gravity observations were made by the author in the summer of 1966. All stations were corrected for drift by returning to the base station at two-hour intervals. Since all of the base stations were tied to the primary base, the observed gravity values were tied to the inter- national datum. The observed gravity readings are con- verted to milligals by simply multiplying the drift- corrected reading by the gravimeter scale constant. The scale constant for the Worden #99 gravimeter was 0.099u5 mgal./scale division. Latitude Correction Due to the increase in sea level gravity values from the equator to the north pole, all gravity stations must be corrected for latitude variation. This was accomplished by calculating the theoretical gravity given by the International Gravity Formula: 2 gl=978.0u9(1+0.005288u sin2¢- 0.0000059 sin 20) where 0 is the latitude. This was accomplished with the use of a high-speed computer. Free-Air Correction Since the gravitational attraction of the earth's mass varies as the square of the distance to its center, stations observed at varying elevations must be corrected 37 to a common datum or common radial distance from the earth's center. Usually this common datum is mean sea level. This correction is called the free-air correction and was cal- culated to sea level with the aid of a digital computer using the following expression: ge = (0.0009 cos 20) h where latitude 23' 6- II II elevation above mean sea level. Mass Correction The free air correction ignores the mass of material between the station elevation and sea level. The gravity effect of this mass must be subtracted from the observed gravity to fully reduce all stations to a common datum. 3 A density of 2.67 grams/cm. was used for this material and gives a correction constant of 0.03u096 mgal./ft. Although this density is undoubtedly too high for certain rocks and too low for others, it has the advantage of tying this survey with others using the same density. 3 Moreover, a density of 2.67 gms./cm. seems to be the best average for crystal rocks. 38 Terrain Correction The mass correction assumes that the topography around a station is perfectly flat. This, however, is seldom true, and the gravitational effects of hills and valleys around a station must be added to the observed gravity. Although elevations ranged from 700 to 1800 ft. within the area, care was taken to place stations in locations where the topography in the immediate vicinity was relatively flat. Since the majority of any possible terrain error is found in the near vicinity of the stations and because of the regional nature of this survey, the terrain correction was omitted. Error Analysis Possible sources of error in a gravity survey include the instrumental constant, the instrument drift, earth tides, terrain errors, and inaccuracies in elevation and station location. The instrumental constant as reported by the manu- facturer has been checked by the Department of Geology of Michigan State University. Drift and earth tides were eliminated by returning to a base station at two-hour intervals. The largest possible error results from discrepancies in elevation. An aneroid barometer is usually considered to have an accuracy of i5 ft. Assuming a maximum error 39 of five ft. in elevation, an error of $0.3 mgal. results in the Bouguer gravity anomaly. The station locations were determined from Geological Survey base maps, and should have accuracies within .05 mi. which would give an error in the latitude correction of $.05 mgal. Of course, errors in instrument readings are inevitable, but large errors of this sort were removed by reoccupying stations which were inconsistent with neigh- boring stations. Lastly, a negative error is introduced in the readings near the Gogebic Range. From theoretical calcu- lations and assuming the range is 300 feet high, 650 feet in width, and infinite in length, with a density contrast of 3.u2 gms./cm.3, a curve of error versus distance was obtained. At a distance of 1200 ft. from the iron forma- tion, the gravitational effect of the range was found to be less than 0.10 mgal. Since most of the stations were much farther than this from the range, this error is negligible over most of the survey. Summing all of the possible errors from elevation, mass, free air and latitute (flfllld result in an error of :.50 mgals. Such a combination is highly unlikely, however, since the signs of each possible error are likely to differ. CHAPTER VIII ROCK DENSITIES The gravitational attraction of rock masses depends upon this density; consequently, rock samples were taken from all significant facies in the area. Their densities were determined by the water immersion method, by first weighing them in air and then in water and using the following formula: AIR (w ‘0 II - TARE) AIR ' H 0 where density '0 ll W = weight in air 2: I — weight in water *3 11> :U m ll weight in water of the container holding the rock samples. Thirty-nine samples were measured with Table 1 sum— marizing the finds and Figure 5 illustrating outcrop location. Granite samples were subdivided into porphyritic granite, transition rock, granodiorite, and diorite. There appears to be a noticeable change in density toward the HO 2.1 of Mn ...... aft of a.» co 3 . . :2. . 3n... . 3:. . . . m mew _n_ + I. i. + T..." :Imo TWO \O—L OTm 0 9:9. ltth «Two 2"... TB}. $.36 nTmo cum. 0.? mi .1; 0 time Elmo t-m o mlwno hlwo + 73 IT warm“? #8.»? [T 9.3.? .3 i Muzimo .-uzmmwuémo WWW” _ o NYInNIN ~-mo o fwmrnzWMNo syzmmeWoN 73.3.. o me a 7m 0 ...sz ....o. o o o 1.6-8 78.8 29» «l... o swims: «02.3 o . znvh 333.9 :3 IT IT .1— 1T .+. .3 i 00:! v n a _ lazlo C. 238 32519. 252009; .Zw._I1_wE _.I L ob» ....n :2. .03. 32. .@c .0.» it: .nsn .o a... A2 base of the granite, that is, the diorite zone. The 3 average value for sixteen granitic rocks was 2.72 gms./cm. which is a little above the normally accepted value of 3 2.67 gms./cm. .- The densities varied from a low of 3 3 2.65 gms./cm. in the porphyritic phase, to a high of 2.78 gms./cm. over the dioritic phase. Twelve samples of gabbro were measured with their density found to be 2.93 gms./cm.3. This also has a higher density than the normally accepted value of 2.90~gms./cm.3., The COpper Harbor conglomerate, overlying the granite, has an average density of 2.62 gms./cm.3. This value agrees well with the value obtained by Birch (195U, p. 8) of 2.65 gms./cm.3. White (1966, p. 35), using a density that made his calculated gravity profiles fit the observed gravity, also used a value of 2.62 3 3 gms./cm. . A value of 2.62 gms./cm. makes the average 3 density of the conglomerate only .03 gms./cm. lower than the porphyritic phase of the Granite. Only one sample of Keweenawan basalt was measured, and consequently, the average value of 2.90 gms./cm.3 determined by Thiel (1956, p. 1087) was used for the gravity interpretation. The density of the Ironwood formation reveals the degree to which it has been metamorphosed. Large amounts of magnetite have given it the extremely high density of 3.42 gms./cm.3. 143 TABLE l.--Density of Rock Samples. Iientiflaation 1 1 ’7 k)a.VTD_Le AIO. "\ U r‘ E. ensity ms./cm. #1 Density #2 gms./cm.3 Granite . Forphyritic Granite m r\ .1) " r I] SO IIE 36 SN SQ SE 27 SW 2 23 SW 36 an 3% NW 1 ( i 7‘.) [\J R) .'\J M m I o o o if» \‘ CD \3 0‘» C7“. "\1 C‘. 1:"fo \] LA.) \f C . 9 2 Q U ’1 A L. Q U MMNNMMMFU ONU‘C‘0.0\C3\.G‘ 0‘1 WW (11(wa U\\fl b. Transition Rock 83 P; 1 2.65 2.68 c. Granodiorite 25 SF 5 2.87 2.80 33 Hi 1 2.76 2.60 a. Dioritc 30 SE 7 2.82 2.83 33 HR 9 2.77 2.76 _3(' :;YI‘IIV :7 2.7:) 2.70 Th as *n 2.59 2.81 Average 2.72 gws,/gm,5 Gabbro F 2.86 a? 2 an :‘7 ?.E"? C8 3 ”1 Flt 2.53 l-ll—9 2.88 [-7.73-IJ“? 3.11 5-30-15 2.08 “-l3-3 3. 8 5-; t—j‘ 8.03 r-SK-l 3.01 {—54-0 8.82 Average 2.93 gms./... Coyper Harbor' lw—Sf.(A) 2.62 Conglereraflo 17—3H (r) 2.01 Averarn k.h; Average 3.U2 Average 2.78 gms./cm. SIC IT; s): ng./cm.3 0' o ()1; up .“1 LA) LA.) A .75 MR) Basalt Tyler Slate Average (Tyler ’2 1’) 7-". ... i b—JF—J H CH (Exx‘u. U) U13 Slate) 2.69 gms./cm. 3 .86 1‘0 .67 .69 .72 M R) K: D.) .79” Quartzite Basalt Granophvre SIN 811 2.75 2.50 2.99 2.70 *This value appears to be in error and was omitted from the density calculations. CHAPTER IX INTERPRETIVE TECHNIQUES Introduction All Bouguer gravity anomaly maps can be resolved into two separate components: the regional effects and the areally smaller residual effects. The regional effects are due to large, deep density variations and are assumed to vary in a smooth, regular fashion. Residuals are the difference between the regional effects and the Bouguer gravity anomalies. They are usually more discrete and somewhat sharper than regional variations. Two separate methods were used to separate the regional from the Bouguer gravity map: (1) the cross profile graphical technique, and (2) the least squares statistical method. Least Squares Statistical Technique The least squares technique is a mathematical method of analyzing mappable data. The basic assumption under- lying this technique is that the regional surface can be approximated by a smooth equation called a polynomial expression. Polynomials can approximate anticlines, homo- clines and other simple shapes. .The various kinds of polynomial expressions are termed orders and are determined HM “5 by their highest power. Usually, the higher orders fit the data too well and eliminate much of the residual while very low orders do not sufficiently approximate the regional. Essentially, this method fits a three-dimensional surface represented by various order polynomials to a discrete set of points. In this case, the points are gravity stations located along an X and Y coordinate system with the gravity values in the Z direction. The various order polynomials are made to fit the points in such a way that the sum of the squares of the residuals must be a minimum. The coefficients of the polynomial are calculated to make the equation fit the data with the above require- ment.- The general polynomial used is: - p q A¢ regional — a00+alOX + aOlY + . . . aqu Y where a's = the coefficients of the equation. ThiseXpression is solved for the coefficients by the use of matrices and is easily done by a digital computer. The Bouguer gravity value is subtracted from the regional polynomial with the resulting value being the residual. While being completely unbiased, this technique has a "moderating" effect on the data. That is, it has a tendency to distort the magnitude and extent of the anomalies. M6 Furthermore, this method cannot take advantage of the experience or insight of the trained interpreter. Figure 9 is a map of a 0-3rd degree least squares regional found to be the best polynomial fit. Cross-Profile Graphical Technique Briefly, this method consists of profiles of the Bouguer gravity map which intersect at right angles. Smooth surfaces are drawn through each profile and are drawn to approximate the regional surface. The regional values at each intersection must be the same. Through a process of trial and error, an approximation of the regional is determined. This method has the advantage of giving a quick and simple look at the residual and allows the interpreter to use its flexibility to incorporate a knowledge of the area into the resulting regional. Its accuracy, however, is limited and if used arbitrarily can give misleading results. Figure 10 is the regional map made using this technique. Theoretical Gravity Formula In 1948 M. K. Hubbert demonstrated a theoretical method of calculating the gravitational effects of two- dimensional bodies. In this method he utilized a line integral technique. However, until the advent of the high speed computer, such a method was impractical. Talwani, Worzel, Lamar and Landisman (1959) utilized Hubbert's “7 findings and rearranged them to work in a computer. Since many bodies are approximated by linear models (such as faults and anticlines), this method has had widespread applications. However, many features occurring in nature do not approach linearity. Consequently, Talwani and Ewing (1960) determined a method to calculate the gravi- tational attraction of three-dimensional bodies of arbi- trary shape.v The following procedure is after them. The body that is to be calculated must first be contoured. Each contour is replaced by an n-sided polygon which resembles the actual contours as closely as desired. The gravity is calculated at any external point. The body is split up into thin lamina and the gravitational attraction calculated for each laminae. A curve is plotted showing the gravitational attraction of each laminae versus its height. This curve, then, is inte— grated to give the attraction of the entire body. This entire procedure may be done analytically with a digital computer with the final integration done numerically. In Figure 6, P is the point where the gravity of body M is to be calculated. This point is also chosen as the origin of a left-handed cartesian coordinate system with the Z axis positive downward. A contour of the body is replaced by the polygonal laminae ABCDEF . . . of thickness dz. The gravitational attraction is termed Ag. Then, (1) Ag = de 48 y-«tXIs 91- 4x1; Can {our al- dcpf/v Z ELEMENTS OF 3-D GRAVITY CALCULATIONS (after TALWANI and EWING, I960) FIGURE 6 j “9 where V is the anomaly caused by ABCDEF. . . per unit of thickness. Now V is expressed by a surface integral, the integration being carried over the surface of ABCDEF. Talwani and Ewing reduced this expression to: (2) v = kp [¢dv — ¢2// (r2 + 22)$5 av] where both integrals are evaluated around the polygon and where k = the universal constant of gravitation p = the volume density of the laminae and z, W, and r = the cylindrical coordinates used to define the boundary of ABCDEF. By substituting (3) r = P1 sin(¢i - Wi+l+v) into (2) and noting that Pi’ ¢i’ and Wi+l are all constants, the line integral of any side, say BC, can easily be solved to give the value of: Zcose1 Zcosei - arc sin (P12 + 22);5 (P12 + Z2)% (A) arc sin The total contribution to V of side BC is Zcose (5) kn Wi+l-Wi-arc sin 2 (Pi Zcosei (P12+z2)g. % ; + arc sin +2 )2 50 The total gravity expression of the laminae is determined by summing the expression of all n sides of the polygon to obtain n (6) V = kp iiAEi+ITW1TarC sin Zcose Zcos¢i , +arc sin (pi2+22>¥ (P12+22)g} Noting that Pi’ W1, wi+l’ 0086i and cosd).i can all be expressed terms of xi, yi,tflueco-ordinates of B, and the Xi+l’ Yi+l,tflxeco-ordinates of C, we see that V can be expressed exclusively in termscflfthe co-ordinates of the vertices of the polygon ABCDEF. . The gravitational attraction of the body M is inte— grated from top to bottom by: z top Ag total = f VdZ. z bottom CHAPTER X INTERPRETATION General Remarks Many features are evident upon examination of the Bouguer gravity map in Figure 7. These are listed below: 1. the Bouguer gravity surface approximates a saddle shape, with a gravity maxima trending east-west through the center of the map with minimas trending toward the north and south, 2. a rather broad gravity nose with steep gradients along its sides is found in TA5N,R3W, 3. a positive gravity nose is isolated in the southwest corner of the map, A. an undulating pattern in TASN,RAW, 5. a steep gradient decreasing toward the northwest is found in the northeast corner of the map, 6. a sinusoidal pattern is found in THAN and TA5N,R2W, 7. a flattening of the steep northward gradient is found near the -50.00 mgal. contour and can be traced across the entire northern portion of the area, 8. a gravity nose outlined by the —57.50 mgal. contour at the northwest corner of the map, and 9. a broadening of the contours in the northern part of TAAN,RAW. These features were not evident from previous regional surveys with the exception of points 1 and 5. For example, the highest contour on the present map is -15.00 mgal. 51 52 .on .3 In: 3.0 finch: .o a .3 ‘03.: N mewE d<$_ >t>FZDOU o2<41m< . 2520023 .Zw.._.._wr_ _I .0.» .....n Bum .0.o 3n: 0... .0.» 3': aha .00.? 57 1 d d d d 4 41 .0 0 .0 0 D a c .00 .015 0 .0 0 .0 0 .080 o. “#59... .._¢up£ .5053 . 00.0.... . Frzaoo 025:2 / 252009)) .zm._..mt r L 0r0 0 0 tax 0 0 )0: .0ko 0+0 ’3. .0“ .00 0 58 graphically illustrates the "moderating" effect of the least squares technique. The peak values over the gravity high in the center of Figure 10 are -30.00 mgal. while the highest contours over the same area in Figure 9 are —35.00 mgals. Despite its shortcomings, the statistical regional still maintains the basic saddle shape of the Bouguer gravity anomaly. Thiel's (1956) gravity work in northern Wisconsin as well as the regionals of this survey reveal several features of merit: (l) the mid-continent gravity high passes from west to east through the center of the survey, (2) the gravity high is of a reduced order in the vicinity of Mellen but enlarges toward the east and west, and (3) the gravity high seems to correlate with the Keweenawan basalts and gabbros. Thiel (1956, p. 1089) commenting on the mid-continent gravity high said: The extension of the positive anomaly toward the Keweenaw Peninsula is interrupted in the vicinity of Mellen, Wisconsin. The reduced gravitation there is probably caused by the intrusion of a large mass of lower density granite as mapped by Aldrich. It might be added, however, that a thinner sequence of high density basalts and gabbros could also cause the reduction in the gravity near Mellen. Based on White's interpretation of this area and the cross-profile regional map, it seems probable that the Granite alone could not cause this reduction of the mid-continent gravity 59 high. White (1966, p. E21) and Wold and Osteno (1966, p. 90) have proposed the existence of a Keweenawan positive trending north-south upon which the basalts are considerably thinner. The southern part of this positive extends into the survey area. Thrust faulting in this area may also be partially responsible for the reduced mafic section. Gravity minimas are found to the south and north of the mid—continent gravity high. The northern minima is probably due to a combination of the positive area men- tioned above and a thickening sequence of Upper Keweenawan sedimentary rocks. The cause of the southern minima is unexplained. White (1966, p. E6) shows this minima closing farther to the south. Local Gravity Anomalies The interpretation of the geology in the vicinity of Mellen depends on three interdependent factors: (1) the steep northward dip of the rocks, (2) the intrusions of the gabbro and granite, and (3) extreme thrust faulting which appears to have been controlled by the cross faults in the area. Depending on their age and order of occurrence each of the three have operated on the events following them. Figure 13 is a composite geologic map of the survey area based on geologic work done by Aldrich (1929), Katzman (1966), Leighton (195“), Olmsted (1966), and from inter- pretation of the gravity and magnetic maps. 60 White, as mentioned earlier, traced the Keweenaw fault into the area on the basis of a magnetic low. The Bouguer gravity map and the cross profile residual map (Figures 7 and 12) reveal a slight minima at the extreme northeast corner of the survey. This minima, although based on two widely spaced stations, coincides with the magnetic low. However, both the magnetic and gravity expressions of this fault are lost within several miles of the northeast corner. At this point the thrust fault is probably terminated against a north-south cross fault. Abrupt changes in the contours of the residual gravity map (Figure 12) along this fault and a sudden widening of the Mellen Gabbro farther to the south support this inter- pretation. Patenaude's (1966, p. 118) magnetic map also reveals abrupt changes in contours along this line. West of this cross fault the Keweenaw fault splits into three thrust faults (Figure 13). Two small thrusts are found on either side of the -7.00 mgal. minima in the northern part of TAAN,R2W; and a large continuous thrust can be traced across the entire northern part of T45N,R3 and A. The -7.00 mgal. minima is a reflection of the low density Tyler slate wedged between the Mellen Gabbro to the north and the Ironwood formation to the south. The flattening of the gradient in the Bouguer gravity map (Figure 7), as evidenced by the broadening of the contours between the —US.OO and -50.00 mgal. contours, is 61 .0 0 .».» 3 u c .0.0 32.0.0 .0.» .00.. Wk .0940 _ _ HEDGE . 1_FZDOU QZ> .ZUJJmE ..0.» .0.» 33. .0.0 30...»... .0.» 30¢ .0.» .00.? v .0. r53 62 ...»0 .00 .00 t u x .00 3090.0 .0 0 .0 0 .00 N_ mewE |_¢u.—.Z_ SOPZOU >FZDOU 02(412 23.1.2009; . ZUAJwE 00 00 Du: . 00 fins 00 .00 30¢ 00, .00.; .P ~b .b sf F s» 63 0. n a: gaun- ' nun-u! I I I I :0: 00000 I 50:03:00.0 u .0 ..m 0 :00. .0000. 444 =80... 0.00.000 ll 5!..- 2808 00000.0. ..... sgh‘z‘tx- IS I zvcb BI 55 :5 i2 is D I NVMVNIIMIN-Ifld I...“ '.J>.P L J 3. J l . I I I : IIMO'I J znch j NVMVNIIMIN . .4. I§ngi "5.“: I UIOPI-uz" I ..m. ...»0 0 O? m _ Bum 00000000 n_<_>_ 0.0040mw mtmodioo < .1: . |,..1\.| I” . On >FZDOU oZ<.._Im< z_szom_>> . Zmnhmz ENC a . . 3mm .0 0 .0 0 3!... .00 ..0 meoE .2 1 00000 .... 000000 00000 0000000 00000000000 0 0 0 000000000000000000 zv¢h ............ nu... gnm at .00 3V! .nnbhn 6A the gravitational expression for the large thrust. On the cross profile residual map (Figure 12) this fault is expressed as a series of round to elliptical maximas with amplitudes of 0.00 to 1.00 mgal. The fault trace lies Just to the south of-these maximas. Although offset repeatedly by cross faults, this fault can be traced from the northeastern corner of TMSN,R2W across THSN,R3W where it swings southwesterly and exits the area midway between the northern and southern boundaries of TA5N,RAW. This fault probably continues in a southwesterly direction and connects up with the northeasterly projection of the Lake Owen thrust fault. If this hypothesis is valid, the Keweenaw and Lake Owen thrust faults may be one and the same, and their combined fault system would stretch from Keweenaw Point in Michigan to the western part of Wisconsin. A total of six cross faults have been interpreted in this area; Figure 13 shows their exact locations. These faults were interpreted on the basis of gravity and mag- netic information with as much geologic evidence as possible. The two faults in TUSN,RHW were interpreted on the basis of linear gravity gradients and magnetic infor- mation. The Brunsweiler Mountain fault is easily seen in the gravity residuals (Figures 11 and 12) and from field evidence but the fault to the west has gone undetected in the field. The gravity gradient cm‘ this fault is based on two widely spaced stations but seems to correlate with 65 the magnetic map of Patenaude (1966, p. 118). Both of these faults, as well as several to the east, are ques- tionable in the northern portion of the area. The Penokee Gap fault traced into the Granite by Katzman (1966) has an undetectable gravity expression to the south, but the residual map (Figure 12) has a very good expression of it to the north of the Granite. However, according to the gravity residual, the movement to the north of the intrusion is opposite to the movement south of the Granite. Katzman's (1966) field study yielded the same results; namely, the Penokee Gap fault is a scissors type fault with the fulcrum point somewhere in the center of the Granite. Three possible cross faults are found to the east of the Granite (Figure 13). The far eastern one was mentioned earlier. The other two are questionable faults interpreted on combined geologic and gravitational evi- dence. Both of these faults have subtle gravitational expressions and are found flanking a well defined thrust fault at the base of the Mellen Gabbro. The one nearest the eastern border of the Granite coincides with a prominent southward protrusion of the Mellen Gabbro and a subtle gravity lineament. On the eastern side of thrust, a larger cross fault can be detected in the field by the large block of Mellen Gabbro that is isolated on its eastern side. In the gravity (Figure 12) this fault can be traced 66 northward between two closed 0.00 mgal. contours and possibly further northward where it "pinches" the gravity nose extending northeasterly from the Granite. This fault, like the Penokee Gap fault, may be a scissors type fault. The undulating pattern in THSN,RUW seems to be the result of two factors: (1) a high density gabbro intrusive, and (2) two cross faults on either side of the intrusion. Drag along these faults has given the gabbro a crescent shape configuration which is convex northward. The crescent shape of this body and the minima immediately to the north are based primarily on one station. The high amplitude gravity nose found in TAAN,RAW is the combined result of the high density portion of the Mineral Lake intrusive and metamorphosed Ironwood formation. Although there is little control over the Mineral Lake Gabbro, the anorthositic phase of this intrusive is reflected by a minima trough with a value of —2.00 mgals. The cross faults bounding the gabbro intrusion above the Mineral Lake gabbro do not appear to extend southward into the Mineral Lake intrusion. This may indicate that the Mineral Lake gabbro is younger than the overlying gabbro. The sinusoidal pattern in townships UN and ASN,R2W is the gravity expression of an alternating sequence of high density iron-formation, low density slate, and high density gabbros. All three bodies are expressed very clearly in the gravity map near the Granite, but further 67 toward the east and west, the paucity of stations makes their gravity expressions difficult to trace. The gravity minimas in the lower portions of TH6N,R3 and RAW may be due to steep dips of the basalts on the basinward side of the Lake Owen thrust. Another alternative to the above interpretation is the northward extension of the various cross faults through the Lake Owen fault. The relative highs and lows in TU6N would then be due to areas of greater or less thrusting. The latter interpretation is illustrated in Figure 13, however, the first interpretation could be inserted just as easily. Interpretation of the Mellen Granite The residual anomaly of the Granite (Figures 11 and 12) is a 6-7 mgal. gravity minima with a rather flat peak across the central part of the intrusion. The flanks of the minima are quite nicely defined on the east, west, and south edges of the Granite, however, the anomaly does not close to the north but rather extends northward toward the positive anomaly of the Lake Owen thrust fault. Part of the minimas northward extension noses toward the northeast where it combines with a well defined minima trough that exits the area in the northern part of TUSN,R2W. 68 The Penokee Gap fault mentioned earlier tends to distort the Granite's residual. This fault cuts through the center of the granite and is the reason for the sharp nosing in the —6.00 mgal. contour in the center of T45N,R3W. The Brunsweiler Mountain and Reservoir faults, on the other hand, have aided in defining the limits of the Granite. These two faults have increased the lineations and gradients along the eastern and western edges respectively and have made these boundaries more recognizable. Two small, but discrete, anomalies appear along the northern edge of the Granite. One anomaly, lying Just east of the Brunsweiler Mountain fault, is a circular gravity minima of -8.00 mgals. The other anomaly is an elliptical maxima near the center of T45N,R3W. This anomaly is around 2 mgals. in magnitude and is encompassed by the -5.00 mgal. contour. The composite geologic map of the Granite, utilizing both the geologic findings of Katzman (1966) and the gravity data, is illustrated in Figure 13. There are several changes from previous maps including: 1. the extension of the Penokee Gap fault through the Granite, 2. the elimination of the basalt layer wrapping around the Granite from the northeast, and 3. the approximate solution of the boundary of the granite at the southwest corner. 69 The southwest boundary of the Granite is similar to the findings of Olmsted (1966). He showed this area as predom- inantly granitic with several large basalt xenoliths. This is essentially the interpretation presented in Figure 13 with the exception that only one xenolith of high density material was detected in this area. This, however, could be due to the relatively coarse station spacing. The basalt layer usually shown wrapping around the northeastern portion of the Granite has no expression in the gravity. However, the small but discrete maxima, found in the center of THSN,R3W is probably due to a small isolated block of basalt lying Just north of the Granite and east of the Penokee Gap fault. Perhaps, this basalt is an erosional remnant of a basalt layer or a roof pendant in the Mellen Granite. At any rate, the minima gravity nose to the northeast of the Granite precludes the exis- tence, in_this area, of any basalt layer. Instead, the gravity nose and the minima trough lying farther to the northeast is probably the gravitational effect of a secondary syncline filled with Upper Keweenawan sediments. The -8.00 mgal. gravity minima lying to the north- west of the Granite is probably due to a mass low density granophyre. Katzman (1966) has recorded an outcrOp of granophyre in section 20, TA5N,R3W which verifies this interpretation. 70 Several models were constructed of the Granite using both two and three dimensional computational methods. A 3 density contrast of -O.21gms./cm. was used between the granite and the gabbros, and a contrast of +.03 gms./cm.3 was used between the Granite and the Copper Harbor conglom- erate. Figure 13 gives the location of two profiles where theoretical anomalies were calculated. The results of the ' north-south profile 7-7' are shown in Figure 1A. Since the densities of the Granite grade from north 3% to south; two densities were used in the theoretical computations. The average density value of 2.72 gms./cm.3 was used to define the south flank of the anomaly while a 3 was more compatible with the density of 2.65 gms./cm. north flank. A rectangular slab with a thickness of 2A00 ft. satisfied the minima due to the Granite. The very small density contrast (.03 gms./cm.3) between the northern portion of the Granite and the Upper Keweenawan sediments made it very difficult to determine the struc- tural configuration at this point. However, a thin basalt block 500 ft. thick dipping at a 30° angle to the north seemed to satisfy the small plateau in the observed anomaly. Furthermore, the conglomerates in this area have an average dip of 30°N. Consequently, the northern face of the granite was extended at a 30° angle down to a depth of 2UO0 ft. A basalt block 5600 ft. wide, 1750 ft. thick, and at a depth of 1500 ft. satisfied the positive anomaly due to the thrust fault. 71 ¢_ manor”. ...... 00.00.... 0.5.0.... 0050.200 ...... 00.00.... 002.0000 000.. 00:00.. 00.50200 ....... 02.02 00.00 J... 00.00.... 002.0000 0000 §N A“ 000. ..w 0 n 0000 00.2400 0. J 00.. 00.0.0200 0.: .I o. m V D] Iii?! I II D m // OI. III... r0 h .h 1.55: thaom 72 Figure 15 illustrates the results of the east-west computer profile F-F'. The theoretical model that fits the observed profile is much the same as the model in Figure 1“. A rectangular slab with an average thickness of 2&00 ft. and perpendicular sides satisfied the observed anomaly. The gradual change from porphyritic granite near the top of the intrusion to diorite at the base indicates that the Granite is probably a sill-like intrusion dipping toward the north. The results of profile 7—7', although not conclusive, lend support to this interpretation. The Granite was probably intruded during a period of thrust faulting. The relief of pressure may have melted part of the basement rock of the Keweenawan positive with the resulting magma intruding into the country rock along thrust faults or cross faults. 73 m. manna...— .._l m min—Omn— . min—own. QMPDQEOO .0> min—0mm ow>mwmm0 0.00. 00.0000 0050200 uuuuuuu 02W. Sam I... 0......000 00>00000 0000 , OOON i H 000. M _ . .N.l “\Q. — p000 , 0.] 0. w j 0 T n 1 \\. I .S .. 0L- .lo .0 ... hm