The total magnetic intensity (TMI) and residual anomaly maps (Fig. 5 and Fig. 6) were contoured from the digitized data. Visual assessment of the TMI and residual anomalous maps reveals intricate form of magnetic signatures of both short and long wavelengths (Fig. 5 and Fig. 6), this is an indication of variable magnetic intensities from diverse geologic sources as supported by the work of Okonkwo et al. (2012) and these variable magnetic intensities is well pronounced in the study area. The mangetic intensity values of the TMI and residual anomalous maps ranges from 7800 to 8200 nT and -220 to 240 nT respectively (Fig. 5 and 6). There are strong evidences of igneous intrusion when juxtaposed with the geologic map of the area. These intrusions account for the high level of faulting and folding around the study area.
More so, these areas mentioned above possess mostly close-spaced contour lines and this implies thinner sedimentary infillings (that is the depth to the top of the basement is shallow); Again, oval contours also encounter in this area may also be an indication of intrusive igneous bodies or lineaments containing groups of mineral deposit of great economic values as evident in the study area like Koton-Karfi, Abaji, Bida and Paiko.
At the central parts (Pategi, Baro, Gulu, Lafiagi) of the study area,contains widely spaced contour, signifying thick sedimentary infilling (that is deeper magnetic sources) within these areas (Fig. 5). It is therefore logical to conclude that the widely spaced contours in conjunction with the high magnetic intensity values detected in the area may have been related with a vein bearing mineral this assertion is supported by the geologic map of the study (Fig. 7 and 8).
The structural alignment of the area was evaluated using the anomalous residual shaded maps (Fig. 9) produced from the residual acoustic field intensity map. The major trend of the lineament were NE-SW and minor ones trending E-W and NW-SE. This structural direction is in conformity with previous work by (Chinwuko, et al 2012, 2014 and Ojonugwa, et al 2018). There are high lineament concentration which suggests intense tectonic activities that affected the deeply seated basement rock and it’s abutting Cretaceous sequences. According to previous works such as Abraham et al, (2014), Ojonugwa et al (2018); Obaje et al. (2013) propose that the NE-SW NNE-SSW and NW-SE within the study area are regarded as Pan-African Orogeny while the E-W may probably have been Pre-Pan-African Orogeny. The structures can serve as migrating path for geothermal and fluid.
The residual magnetic anomalies data were subjected to both Peter’s half-slope method and spectral analysis for depth calculation (sedimentary thicknesses) and depth modelling within the study area (Fig. 10). The result of the analysis is shown in Table 1. The interpreted result reveals two-layer depth model; the shallower magnetic depth bodies which varies from 0.54 to 1.87km (for Peter’s slope method), and 1.27 to 1.96km; for spectral analysis interpretation, deeper magnetic bodies of depth range of 2.01 to 3.27km (for Peter’s slope method) and 2.01 to 4.27km for spectral analysis. Again, the depth to the centroid obtained through the spectral analysis reveals depth range of 9.79 to 15.75km across the area (Table 1).
Table 1
Depth calculation using Spectral Analysis
|
Spectral Analysis
Peter's Slope method
|
Peter's Slope method |
|
|
|
Anomaly
|
Depth to Top
Of Basement
Zt (km)Zp (km)
|
Depth to Botton of Basement
|
Zo (km)
|
Curie Point Depth (km)
|
dT/dZ (oC/km)
|
q(mWm2)
|
1
|
2.09
|
1.86
|
14.73
|
27.37
|
24.733
|
61.834
|
2
|
3.11
|
2.41
|
12.84
|
22.57
|
28.046
|
70.116
|
3
|
1.49
|
2.88
|
15.11
|
28.73
|
23.359
|
58.397
|
4
|
0.96
|
0.56
|
13.45
|
25.94
|
24.380
|
60.950
|
5
|
2.42
|
2.64
|
12.88
|
23.34
|
28.238
|
70.594
|
6
|
3.18
|
2.93
|
10.06
|
16.94
|
23.191
|
57.977
|
7
|
3.05
|
2.71
|
13.92
|
24.79
|
23.800
|
59.499
|
8
|
1.52
|
1.83
|
12.87
|
24.22
|
26.197
|
65.492
|
9
|
1.14
|
2.05
|
14.31
|
27.48
|
28.798
|
71.996
|
10
|
1.08
|
2.61
|
12.95
|
24.82
|
20.781
|
51.953
|
11
|
0.53
|
2.28
|
16.28
|
32.03
|
25.043
|
62.608
|
12
|
2.46
|
1.42
|
12.21
|
21.96
|
25.641
|
64.103
|
13
|
3.22
|
2.33
|
11.04
|
18.86
|
22.516
|
56.289
|
14
|
3.07
|
2.39
|
14.53
|
25.99
|
23.761
|
59.402
|
15
|
1.49
|
1.71
|
16.84
|
32.19
|
30.240
|
75.600
|
16
|
0.45
|
2.14
|
15.06
|
29.67
|
28.087
|
70.2179
|
17
|
2.71
|
3.27
|
13.01
|
23.31
|
24.545
|
61.363
|
18
|
3.24
|
1.81
|
9.09
|
14.94
|
26.316
|
65.789
|
19
|
3.19
|
2.96
|
11.23
|
19.27
|
24.017
|
60.041
|
20
|
2.85
|
2.57
|
13.69
|
24.53
|
24.618
|
61.545
|
21
|
2.25
|
1.74
|
14.47
|
26.69
|
24.733
|
61.834
|
22
|
2.33
|
1.71
|
12.61
|
22.89
|
27.154
|
67.884
|
23
|
2.08
|
2.01
|
11.89
|
21.7
|
26.839
|
67.099
|
24
|
2.86
|
2.11
|
14.05
|
25.24
|
24.670
|
61.676
|
25
|
3.23
|
2.42
|
13.11
|
22.99
|
25.709
|
64.273
|
26
|
2.98
|
1.72
|
9.47
|
15.96
|
26.902
|
67.254
|
27
|
1.81
|
1.79
|
13.22
|
24.63
|
22.222
|
55.556
|
28
|
1.65
|
0.78
|
16.51
|
31.37
|
21.978
|
54.945
|
29
|
2.13
|
0.83
|
14.83
|
27.53
|
24.278
|
60.695
|
30
|
3.17
|
2.15
|
16.32
|
29.47
|
24.116
|
60.291
|
31
|
3.22
|
1.44
|
11.63
|
20.04
|
23.761
|
59.402
|
32
|
2.08
|
0.76
|
13.83
|
25.58
|
26.364
|
65.909
|
33
|
2.01
|
1.96
|
12.94
|
23.87
|
30.950
|
77.375
|
34
|
2.14
|
1.38
|
15.77
|
29.4
|
25.483
|
63.708
|
35
|
2.33
|
1.97
|
13.22
|
24.11
|
24.744
|
61.860
|
36
|
2.79
|
2.38
|
15.64
|
28.49
|
23.043
|
57.608
|
37
|
2.47
|
1.16
|
14.85
|
27.23
|
27.397
|
68.493
|
Average
|
2.29135135
|
2.01
|
13.52594595
|
24.76054054
|
25.277
|
63.173
|
The magnetic depth calculation result (Table 1) shows that Curie isotherm depth varing from 19.18 to 30.95 km with an average of 23.12 km. Also, the geothermal gradient ranges from 21.98 to 30.95 oC/km, with an average of 25.27 oC/km. The Heat flow (flux) obtained varies from 51.95 to 77.37 mWm2 with an average of 63.17 mWm2.
From the depth calculations using spectral analysis, two anomalous depth sources were interpreted. The deeply seated magnetic anomalous sources varying from 1.91 to 3.78 km, and shallower seated magnetic anomalous sources which ranges from 0.98 to 1.98 km (Fig. 11). Deeply seated magnetic anomalous sources may possibly denote depth to the basal crystalline rocks, while the shallower seated magnetic anomalous sources maybe associated with intrusive igneous and/or magnetized bodies coved by sediment. The basal depth is abysmal in the entire south and central part of the study area, whereas, at other parts of the area such as Kutawenji, Lafiaji, Koton-Karfi and Lapai areas have shallower sources.
More so, the 3-D surface plot of depth to the top of the anomalous magnetic body shows presence of peaks (uplifts) and depressions (troughs). Around Agaje, Egbako, Olle, Mopa and Abaji areas, there visible linear depressions and these areas reveal higher sediments than the other parts such as Kutaeregi, Paiko, Lapai, Lafiagi, Aiyegunle, and Koton-Karfi areas which have prevalent uplifts (peaks) in conjunction with lower sedimentary thicknesses (Fig. 12). The presence of these peaks (uplifts) suggests that there are numerous intrusive bodies around these areas; as a result, there are more tectonic activities in the areas associated with depressional feature. According to Biswas et al, (2016 and 2017) and also Biswas (2015), these identified igneous intrusives generally occur as silly and dykes.
Prevalent Intrusive sources and Geologic model across a profile in the area
The geologic model (Fig. 13 and 14) obtained from the quantitative interpretation of the residual magnetic data reveals four geological stages namely: sedimentary stage, ferromagnetic bodies, paramagnetic bodies and lower crust bodies. The sedimentary infilling along this profile has a variable thickness which ranges from 0.20- 3.21 km. The deepest sedimentary cover occurs at the eastern and western ends of the profile (Egbe) (Fig. 14a) while the shallowest is at the middle. More so, the ferromagnetic bodies underlain the sedimentary layer and it has an average thickness of 6.1 km, the depth to the ferromagnetic bodies range from 12.04 to 13.0 km in this profile. Also, the paramagnetic bodies which are associated with Curie point depths and upper mantle have depth range of 13.10 to 24.01 km. It is believe that the heat from the mantle must have reworked the magnetic body making them to loss the magnetism. The model suggests that the deepest Curie point depth occurs in both left and right hand side of the model while at the middle, the Curie point depth is shallowest. The model interpretation is also shown in Fig. 14b.
Core Sample Analysis and Its Implication around Koton-Karfi
Core sample analysis within Koton-Karfi reveals different lithologic units within the sample locations. The depth to the oolitic iron ore obtained across the area ranges from 20.79 to 101.2m with an average of 38.52m (Table 2).
Table 2
Oolitic Iron Ore Deposit Level with respect to Mean Sea Level (MSL)
Borehole Co-Ordinates
|
Elevation
(m)
|
Borehole Depth
(m)
|
Oolitic Ore Deposit level w.r.t. MSL (m)
|
N08009’305” E006050’48.1”
|
260
|
42.56
|
217.44
|
N08009’305” E006050’48.1”
|
263
|
35.2
|
227.8
|
N08009’30.7” E006051’12.6”
|
267
|
39.68
|
227.32
|
N08009’30.7” E006051’208”
|
269
|
42.82
|
226.18
|
N08009’22.3” E006050’482”
|
259
|
42.65
|
216.35
|
N08009’22.4” E006050’56.4”
|
258
|
39.34
|
218.66
|
N08009’22.4” E006051’12.7”
|
266
|
39.33
|
226.67
|
N08009’22.7” E006051’20.8”
|
275
|
42.38
|
232.62
|
N08009’22.7” E006051’20.8”
|
271
|
42.59
|
228.41
|
N08009’14.2” E006050’48.3”
|
243
|
42.62
|
200.38
|
N08009’14.9” E006051’04.7”
|
265
|
42.37
|
222.63
|
N08009’06.1” E006050’56.4”
|
266
|
42.34
|
223.66
|
N08009’06.1” E006051’04.7”
|
266
|
40.32
|
225.68
|
N08009’0.63” E006051’12.9”
|
270
|
41.61
|
228.39
|
N08009’0.64” E006051’21.1”
|
265
|
42.61
|
222.39
|
N08008’58.0” E006050’56.4”
|
283
|
40.45
|
242.55
|
N08008’58.1” E006051’04.8”
|
262
|
42.61
|
219.39
|
N08008’58.2” E006051’13.1”
|
254
|
24.05
|
229.95
|
N08008’58.1” E006051’21.0”
|
250
|
20.79
|
229.21
|
N08008’58.0” E006050’48.4”
|
262
|
25.53
|
236.47
|
N08009’06.09” E006050’48.3”
|
270
|
20.79
|
249.21
|
N08009’14.2” E006051’56.4”
|
265
|
23.05
|
241.95
|
N08009’14.3” E006051’12.6”
|
284
|
23.05
|
260.95
|
N08009’14.5” E006051’21.1”
|
258
|
23.05
|
234.95
|
N08009’30.6” E006050’56.2”
|
229
|
101.2
|
127.8
|
Average
|
263.20
|
38.52
|
224.68
|
The elevation map of Koton-Karfi area (Fig. 15) was produced for effective correlation with the ooolitic iron ore level map (Fig. 15). Nevertheless, the ooolitic iron ore level with respect to mean sea level across Koton-Karfi area were computed by subtracting depths to oolitic iron ore layers deduced from the core drilling from surface elevations obtained during the data acquisition (Table 2). Thus, maps of the oolitic iron ore levels with respect to elevations were generated in order to depict the possible trend of the oolitic iron ore level across the study area (Fig. 16). Considering elevation and oolitic iron ore maps of Koton-Karfi area (Figs. 15 and 16), it is evident that the trend of the oolitic iron ore level is predominantly in NE-SW direction and mineralogically, the mineralization will flow this trend.
More so, Fig. 15 reveals that the anomalous body level (Ooilitic iron ore level) is deep around northeast and southwestern parts of Koton-Karfi; whereas at northwestern part of Koton-Karfi, the depth to the anomalous body (Ooilitic iron ore) is shallow with average oolitic iron ore deposit level as 225m.
Furthermore, profiles running from T-Tl at Fig. 14 and U-Ul at Fig. 15 were superimposed in order to establish the variation phenomenon across the area. Here, it was observed that the oolitic iron ore level follows the topographical level which implies that the topography controls the configuration of the iron ore level (Fig. 17).
Result from qualitative interpretation reveals that the area is extremely fractured, with fractures trending NE-SW direction and minor ones in NW-SE and E-W directions, the trend of these structures is in conformity with the trend of structures within the Nupe basin. These fractures can serve as migrating pathway for both geothermal energy flow and fluids like hydrocarbon. The work of Ojonugwa et al, (2018) believes that the stratified nature of the carbonaceous shale with intercalated sandstone found within the study area may probably favour fluid migration into potential reservoir rocks that are made up mostly of fluvial deposit, flood plain and shelf sandstones of the Lokoja and the Patti Formations.
Quantitatively, the depth to the top of magnetic basement rock (sedimentary thickness) within the study area have been delineated along seven different profile lines using Peter’s half slope and Spectral analysis of aeromagnetic data and the result shows two depth model across the area, namely; the shallower magnetic sources which vary from 0.56 to 1.96 km and the deeper magnetic sources which vary from 2.01 to 4.27 km. The Curie isotherm depth result revealed deeper depth at Kutiwenji, Egbako, Lapai, Paiko, Olle, Mapo and Baro areas, ranging from 22.60 to 27.91 km, in other parts, the Curie isotherm depth was shallower and ranged from 19.18 to 22.20 km. The calculated thermomagnetic properties reveals average values of 23.12 km Curie isotherm depth, 25.27 oC/km geothermal gradients and 63.17 mWm2 heat flows in the area.
Result from the core drill data reveals that the anomalous body level (Ooilitic iron ore level) is deep around northeast and southwestern parts of Koton-Karfi; whereas at northwestern part of Koton-Karfi, the depth to the anomalous body (Ooilitic iron ore) is shallow with average oolitic iron ore deposit level as 225m.
Integrating all the results and deductions obtained in this work, it can be deduce that those regions (such as Baro, Kutaeregi, Kutiwenji and Koton-karif) with shallow or low sedimentary thicknesses are possible areas that are associated with magnetic mineral ore deposits like oolitic iron ore identified in Koton-Karfi area (Fig. 18). Actually, these areas might not support hydrocarbon generation.
However, the sedimentary infillings around Pategi, Agaje, Olle and Baro area is relatively high in conjunction with the high geothermal gradient and heat flow; will possibly pave way for hydrocarbon potential in this area provided that all other conditions for hydrocarbon generation is available. Previous workers such as, Ikumbur et al, (2013), Okubo et al, (1985), Adeleye. (1974), Ojo and Akande (2012) suggest that the study area contains carbonaceous shales intercalated with sandstone and clay, which is a potential source rock.