4.1. Sedimentological and Lithofacies Descriptions
The lithological units encountered between 1500 m to 4600 m interval of the well are summarised in Fig. 3. Five main lithounits were identified; these include, sand-shale heterolith, sand, shale, gypsiferous shaly sand, and silty clay. The heterolithic unit is very thickly bedded and of similar characteristics to those described by Odusina et al. (1983), Avbovbo et al. (1986) and Olugbemiro (1997) in Kanadi and Albarka wells, Ola–Buraimo and Boboye (2011) in Tuma – 1 well, and Ayinla et al. (2013) in Kemar – 1 well. The shale constituent is brownish to greyish, while the sand component is fine to coarse-grained, angular to subrounded shape and poorly sorted grains, with varying shale/sand ratio at different intervals. The occurrence of the unit is limited to the lower and the middle horizons of the well, at the 4450–4600 m, 3750–3850 m, and 2700–2850 m intervals (Fig. 3).
The sand lithofacies occurs as a medium to thickly bedded units, distributed within the stratigraphic intervals of the well and often intercalated with other facies (Fig. 3). It is fine to very coarse-grained, subangular to rounded in shape and moderate to poorly sorted, generally characterised by off white to reddish-brown colouration. The shale lithofacies are very prominent within the penetrated sequences of the Gaibu – 1 well, this facies is more predominant in the middle part of the well (Fig. 3). Thick to very thick-bedded black shale is present within 1620–2660 m and 2760–2900 m intervals. Shale lithofacies at 3450–3520 m and 2660–2750 m intervals of the well are medium to thickly bedded, greyish to brownish, fissile, and relatively ferruginised.
The gypsiferous sandy-shale is not common in the stratigraphic section of the well, its occurrences are mainly within the 3500–3600 m and 2450–2580 m intervals (Fig. 3). The lithofacies is characterised by frequent pale greyish to blackish pigments on the shaly components whereas the sandy parts are of fine to coarse grains, angular to subangular and poorly sorted. Estimated percentage of sand/shale/gypsum ratio in this unit is 31:59:10. The silty clay lithofacies is fairly present at the lower and upper part of the well and typified by brownish coloured grains, and some ferruginisation imprints. The lithofacies occurs at depths of 3450–3460m, 1650–1710m and 1540–1590 m, and as rare intercalations with shale beds (Fig. 3). Presented below are the detailed descriptions of the encountered lithostratigphic intervals based on lithology, palynomorphs’ distribution and bioevent charts (Figs. 3–5).
4.1.1. Bima Formation
This is the oldest stratigraphic unit in the study area, and it represents the basalmost penetrated unit by the Gaibu-1 well. It occurs within the 3700 to 4600 m interval with an estimated 900m thick unit (Fig. 3). The Bima Formation primarily consists of shaly sandstone and sand-shale heterolith. The sands are brownish, poorly sorted, fine to coarse-grained and moderate to largely supported by the fissile shale units. The ferruginised clay units at the upper end (3700 to 3790 m) of the formation in this study occur as intercalation with greyish sand – shale heterolith units. The sand grains are predominantly medium-grained and sub-angular to subrounded at the lower end (Fig. 3). This interval consists of some land derived forms (Cyathidites minor) with the sparse occurrence of marine species such as fungal and dinocyst indeterminate (see Fig. 4–5). Thus, suggesting, a distinct continental to brackish setting. This formation correlates to the Middle - Upper Bima subdivisions of Guiraud (1990), and the Bima Sandstone of Okosun (1995).
4.1.2. Yolde Formation
This formation represents transitional deposit that conformably overlies the Bima Formation. It occurs within the depth interval of 3350–3700 m (Fig. 3) in the Well. The Yolde Formation is predominantly characterised by interbeds of brownish-greyish sands, siltstone, and thin-bedded reddish shale with the occurrences of subordinate carbonaceous and ferruginous materials. The sands are medium to coarse-grained, moderately to poorly sorted, angular to sub-angular in shape. The depositional environment of the lithofacies is interpreted to range from lagoonal estuarine to marginal marine environments due to the occurrence of non-marine palynomorphs, such as Laevigatosporites spp, and Cyathidites minor (see Fig. 4). Botryococcus braunii, fungal spore and dinocyst indeterminate, which are major marine palynomorphs found in the overlying successions were not found within the analysed detritus of the Yolde Formation (Figs. 4 and 5). Yolde Formation has not been frequently mentioned in the stratigraphy of the Bornu Basin (Fig. 2). However, the presence of this lithofacies in the Gaibu-1 Well, attests to its presence in the southern Bornu Basin. The lithological characteristics of this interval correlates to Akande et al. (1998)’s description of the Yolde Formation in the contiguous Gongola Arm of the Northern Benue Trough (see Fig. 1). The naming of this Formation in other exploration wells (e.g.,, Kinasar-1, Saa-1, Wadi-1, Murshe-1, Ziye-1) drilled in the southern Bornu Basin by Adekoya et al. (2014) further attest to its presence in the sedimentary successions of the Southern Bornu Basin.
4.1.3. Gongila Formation
The Gongila Formation occurs between 2950–3350 m in the well. It overlies the Yolde Formation. It consists of reddish-brown, ferruginised sandy shale sequences with minute occurrence of carbonaceous detritus (Figs. 3 and 4). This 400 m thick greyish shale contains very thin interbeds of sands. The sands are fine to medium grain, sub-angular in shape. The formation is characterised as a marginal marine to inner shelf deposit based on the occurrences of non-marine taxa (Cyathidites spp., Cyathidites infectus, Longaperities marginatus) and marine palynomorphs (Spiniferites membranceous, Botryococcus braunii, Odontochitina costata). It is remarkable that volcanic intrusive independently reported by Alalade and Tyson (2013), Ilozobhie et al. (2015) and Okosun (1995) in the Gongila Formation is not seen in the studied Well. Thus, the intrusion must have been localised to the northern and northeastern parts of the basin.
4.1.4. Fika Shale
The Fika Shale spans the depth of 1620–2950 m with an estimated thickness of 1330 m, it lies conformably on the Gongila Formation (Figs. 3 and 4). Careful sedimentological description of ditch cuttings within this interval revealed that the formation is not entirely shaly as previously documented by earlier authors based on wells from the northern segment of the basin (see Okosun, 1995; Olugbemiro et al. 1997), but rather shows intercalation with essentially siliciclastic sandstone and silty materials (Moumouni et al. 2007). We subdivided the Fika Shale into three (3) units based on observed physical and textural characteristics. The depth interval of 2550–2950 m marked the lowermost part of the sequence that contains greyish, coarse-grained, poorly sorted, and vividly angular shaly sand with off-white sandstone (Fig. 2).
The middle part of the sequence is characterised by black sandy shale deposited between 1900 and 2550 m, with the sands characterised by medium to coarse-grained, subangular, and poorly sorted materials. The uppermost part comprises of thick greyish to brownish shale unit between intervals 1620–1900 m. It consists of minute brownish, medium to coarse-grained, subrounded geometry and moderately sorted sandstone/sand. The unit is capped by ~ 30 m of calcareous siltstone (Figs. 3 and 4). Gypsum sporadically occurs as an accessory mineral. The palaeoenvironment of deposition of the formation is suggested to be mainly marginal marine due to the presence of palynomorphs such as Cyathidites ssp, Psilatricolporites triangulates, Psilatricolpites spp., Retimonocolpites spp with the occurrence of Odontochitina costata and Botryococcus that are marine-derived forms (Figs. 4 and 5). However, transporting medium might be of relatively high energy and erosive in nature (turbidity currents) which might be responsible for the presence of coarser particles in the shale during deposition. The recorded thickness conforms with earlier workers (see Carter et al. 1963; Moumouni et al. 2007; Okosun, 1995; Olugbemiro, 1997).
4.1.5. Gombe Formation
The Gombe Formation occurs within the interval 1500–1620 m with an estimated thickness of 120 m (Figs. 3 and 4). The formation consists of a basal sandstone unit intercalated with thin beds of shale at the lower part of the interval (Fig. 3). The sand is reddish-brown in colour, medium to coarse in grain size, sub-angular to angular in shape and poorly sorted. Significant amounts of reddish sands are distributed within the interval. The interplay between the colour composition of the sediments and the visible grain sizes,in addition to the presence of palynomorphs such as Milfordia spp, Monosulcites spp., Oligosphaeridium spp Longapertities marginatus, Periretisyncolpites spp, Monoporites annulatus characteristically suggest an environment of deposition indicative of distal continental to proximal fluviatile (Figs. 4 and 5). The Gombe Formation was recorded missing in some selected wells (including Gaibu-1) by Moumouni et al. (2007). However, our data has shown that the formation is present in the Gaibu-1 Well.
4.2. Palynological Assessment and Palynostratigraphy
Recovered palynomorphs are fairly preserved and the miospore recovery is moderate to barren at different intervals (Figs. 4 and 5). The species that are of well-known stratigraphic ranges in other contemporaneous basins of Western Africa (see Lawal and Moullade, 1986; Deaf et al., 2014) and Northern South America (see Herngreen, 1973; Germeraad et al. 1968) were used as a guide in deducing the biozones (Fig. 6). Recovered palynomorphs were classified into four major groups based on their botanical affinity, which are, (i) angiosperm pollen, (ii) gymnosperm pollen, (iii) spores, and (iv) dinoflagellate cysts. These, respectively represent an estimated 48.40%, 26.39%, 16.97% and 8.24% of the total recovered taxa (Fig. 7A). Constructed palynomorphs’ frequency distribution chart (Fig. 7B) indicated that angiosperm pollens dominated the recovered forms across the five stratigraphic intervals (formations), having its peak in the 2950–3350 m interval, which corresponds to the Gongila Formation (see Figs. 3 and 7B). Like the angiosperm, the gymnosperm, and spores both peaked at the 2950–3350 m interval. Though it is generally of lesser frequency compared to the other three palynomorph groups, the dinocysts show an uphole increment, thus indicating possible marine influence in the Fika (1620–2950 m) and Gombe (1500–1620 m) Formations (Fig. 7B)
Figure 8 shows the overall frequencies of recovered taxa associated with the four identified botanical affinity. Tricolporopollenites spp. (69) and Psilatriporites spp. (30) are the angiosperms with the highest frequencies (Fig. 8A). The gymnosperm pollens generally recorded lower frequencies of ≤ 6 except for Podocapidites spp. (63), Alnus vera (48), and Inaperturopollenites spp. (22), compare to their angiosperm counterparts (Fig. 8B). Spore count ranges from 1 in Polypodiaceoisporites caperatus to 32 in Laevigatosporites spp. (Fig. 8C). The counts of dinoflagellate cysts are generally low ranging from 2 to 7 (Fig. 8D). Palaeoconditions that favoured the abundance of angiosperms and rare incursions of marine can be construed from the high frequencies of angiosperm pollen taxa (Fig. 8A) and the low counts of the dinoflagellates (Fig. 8D), respectively.
Palynozonation interpretation was generally based on the evolution of the miospores, their extinction and their relative frequencies depend on the ecology and other environmental factors (Brenner, 1968; Deaf et al., 2014). Thus, four palynozones denoted as Zones A1 – A4 (Figs. 5 and 6), were erected base on the assemblages of diagnostic forms that were confirmed from earlier researchers (Jardine and Magloire, 1965; Lawal and Moullade, 1986; Williams, 1975; 1977). These palynozones are discussed below.
Zone A (1): Triorites africaensis Assemblage Zone
Interval: 3420–4600 m
Age: Late Cenomanian
Characteristics:
This is the oldest palynozone encountered in the studied well (Fig. 5). It represents the deepest horizon penetrated by the well (total depth = 4600 m). This assemblage zone was proposed earlier as a major palynological zonation across the West Africa basins (Blotenhagen, 1980; Jardine and Magloire, 1965; Lawal and Moullade, 1986) and North-South America (Muller, 1981; Regali, 1989) to date the late Cenomanian. The top of the interval is placed at 3420 m based on the appearance of Cicatricosisporities spp. co-existing with the presence of Classopollis spp. and Triporate spp., following Jardine and Malgloire, (1965) and Deaf et al. (2014). However, the presence of Triorites spp. and first downhole occurrence (FDO) of T. Africaensis (Abubakar et al. 2006; Deaf et al. 2014; Jardine and Magloire, 1965) support the top interval to be of late Cenomanian (Fig. 5).
The microfloral assemblages present within this zone include Cyathidites spp., Verrucatosporites spp., Polypodiaceiosporities spp., Retimonocolpites spp., Triporate spp., Retitricolpites spp., Cyathidites minor, and Retitricolporities spp. This assemblage interval is characterised by few associated elaterate pollen grains and noticeable triporate angiosperm pollens, which could have allowed this interval to be named Afropollis jardinus sub-zone of the pollen PO – 304 assemblage zone in the Northern Benue Trough (Lawal and Moullade, 1986). This can be inferred into the southern part of the Bornu Basin. Nevertheless, the reference point of Afropollis jardinus implies that its stratigraphic importance based on its associated taxa are delimited to middle Cenomanian in some other works around Africa (Deaf et al. 2014; Jan Du Chene et al. 1978; Said et al. 1994). Thus, this assemblage zone can be correlated with zone VI of Schrank and Ibrahim (1995) and zone I of El Beialy et al. (2011) as indicative of late Cenomanian.
Zone A (2): Cretacaeiporites scabratus - Odontochitina costata Assemblage Zone
Interval: 2940–3420 m
Age: Turonian
Characteristics
The top of the zone coincides with the FDO of Odontochitina costata and Cupanieidites reticularis at 2940 m (Fig. 4) while the base corresponds to the disappearance of Proxapertities spp, which was classed by Lawal and Moullade (1986) with Gnetaceaepollenites sp. 1 as an Upper Cenomanian index species. This zone is likened to the acme zone of Lawal and Moullade (1986), which is characterised by the dominance of Cretacaeiporites scabratus (Herngreen, 1975) and Cretacaeiporites mulleri.
Odontochitina costata recorded by Moustafa and Lashin (2012) from the western desert of Egypt, as an important Turonian index form with the presence of other associated dinoflagellate cysts. The abundance of Odontochitina costata, and the last downhole occurrence (LDO) of Botryococcus (Chlorococcalean green algae) in the present zone is coeval to the characteristic of tricolporate – triporate – Cretacaeiporites mullerii Assemblage Zone (Fig. 4). A major zone of northern Kordofan (Schrank, 1994a) chronologically, and the upper part of the Chlorococcalean green algae interregnum zone from the lower Turonian of the northwestern Desert of Egypt (Ibrahim, 1996). Other species in this zone are Inaperturopollenites spp, Cyathidites spp., Psilatricolporites triangulates, Psilatricolpites spp., Psilatricolporities spp., Monosulcites spp., Verrucatosporites spp. and Retimonocolpites spp. These assemblages are indicative of Turonian.
Zone A (3): Droseridites senonicus Assemblage Zone
Interval: 2500–2940 m
Age: Santonian – Campanian
Characteristics
This zone was first proposed as an acme zone by Lawal and Moullade (1986), the details of this zone are provided in Abubakar et al. (2011) work. The top of the interval is characterized by FDO of Buttinia andreevii. Other palynomorphs within this interval include Canningia capillata, Proteacidites sigalii, Polypodiaceoisporites retitrugatus, Cyathidites infectus, Monocolpites spp, Verrucatosporites spp., Tricolporopollenites spp. and Spiniferites ramosus. The base of this zone is characterized by the highest occurrence of Tricolporopollenites spp. The presence of Proteacidites sigalii shows that this section of the well is pre-Santonian (Fig, 5). Owing to the paucity of miospore, particularly marker species within this section, the Santonian – Campanian boundary could not be defined. This zone is assigned pre – Santonian to Campanian (Fig. 5). The associated assemblages for this zone are similar to the foraminifera – controlled Coniacian – Santonian successions (Deaf et al. 2014) discussed by Lawal and Moullade (1986) in northeast Nigeria, Morgan (1978) in the Angola Basin and Schrank and Ibrahim (1995) in early Santonian sediments from Egypt.
Zone A (4): Syncolporites / Milfordia spp Assemblage Zone
Interval: 1500–2500 m
Age: Maastrichtian -? Younger
Characteristics
The FDO of Cyathidites infectus and LDO of Bombacacidites spp. mark the base of the interval (Fig. 5). The interval is characterised by the appearances of Milfordia spp, Monosulcites spp., Oligosphaeridium spp Longapertities marginatus, Periretisyncolpites spp, Monoporites annulatus, Spiniferites spp., Lejeunecysta spp., Batiacasphaera spp. and Cyathidites spp. and microplanktons such as Senegalinium spp., Polysphaeridium spp., and Dinogymnium spp., and microforaminiferal wall lining. This interval is composed of assemblages of palynomorphs that are depictive of Maastrichtian to Early Tertiary (Fig. 5).
4.3. Palynofacies and Palaeoenvironments Interpretation
The application of quantitative and qualitative palynomorphs in this section provide insights on the environments of deposition (Figs. 4–5). Several studies have demonstrated the usefulness of palynofacies analysis and palynomorph assemblages in providing reliable and useful information on the depositional environments of sedimentary detritus (e.g., Traverse, 1994; Tyson, 1995; Ibrahim, 1996; Herngreen et al, 1996; Schrank and Mahmoud, 1998, Dino et al., 1999; Schrank, 2001). The general composition of the palynomorphs in the Gaibu-1 well indicates mixed pteridophyte – gymnosperm – angiosperm vegetation (Figs. 4–5). The sparse occurrence of marine/dinoflagellate cysts and much presence of some terrestrial microflora (represented by thick-walled pollens and smooth trilete spores) (Fig. 5) implies the deposition of the Cenomanian sediments (3420–4600 m) took place in continental/coastal environment with fluctuation of brackish water.
The Turonian to Campanian sediments (2540–3420 m) are interpreted to have been deposited in a fluctuating system of lagoonal estuarine to marginal/shallow marine environment alongside freshwater incursion. This interpretation was based on the presence of thick-walled spores, thin-walled pollens, the occurrence of fungal spore and Botryococcus braunii, coupled with the presence of fern spores such as Cyathidites and Cicatricosisporites probably reflects local pteridophyte vegetation growing on wetlands (Schrank and Mahmoud, 1998).
The Santonian-Maastrichtian sediments are interpreted to have been deposited under the influence of anoxic condition, as deduced from the moderate occurrence of glauconite in the lithologic unit. According to Rull (1997) and Germeraad et al. (1968) the presence of Pachydermites diederexi, Verrucatosporites spp and Laevigatosporites spp., indicate a swampy freshwater or brackish water environment, these species with Polypodiaceiosporites spp., are common in the upper section of the well.
The Maastrichtian sediments (1500–2500 m) are characterised by the common occurrences of dinocysts (Spiniferites, Oligosphaeridium), microforaminiferal linings with fungal spore and Botryococcus braunii, suggesting incursions of marine events into the interpreted distal continental to proximal fluviatile depositional setting in the Maastrichtian (see Sect. 4.1.5). The uphole increment in distribution and frequency of Botryococcus and other algae in this study (Fig. 5) is suggestive of the influence of marine influx or water depth fluctuations. Taking clues from Fig. 6, the late Cenomanian section is certainly sparse of dinoflagellates and marine index palynomorphs, whereas the Maastrichtian is typified by more occurrences of dinoflagellates. The abundance of chlorococcalean green algae (Botryococcus braunii) alongside the highest occurrence of dinocysts (Figs. 4 and 6) vis-à-vis the dominantly shale-sand intercalations of sediments (Figs. 2–3) within this succession further justify intermittent marine incursions.
4.4. Palynofloral Provinces and Palaeoclimate Interpretation
Sequential palynofacies record is of importance in constraining ecosystem and their respective climatogenic conditions (Poumot, 1989). Akande et al. (2005) and Chateauneuf (1980) have demonstrated climatic variation across the earth is responsible for differential vegetation at various geological times Herngreen and Chlonova (1981) established eight palynofloral provinces: (i) the pre-Albian West Africa – South America province (WASA), (ii) the Boreal lower Cretaceous province of the northern hemisphere, (iii) the middle Cretaceous (Albian to Cenomanian) Africa – South America province (ASA), (iv) the late Cretaceous Normapolles province, (v) Aquillapollenites province, (vi) the late Cretaceous Palmae province of Africa and Northern South America, (vii) the Gondwana province and the (viii) Senonian Northofagidites province.
The palynofloral assemblages recovered from the Cretaceous sediments in the Gaibu-1 Well contains a reasonable occurrence of Palmae type monocolpate and tricolpate pollen taxa, such as Acrostichum aureum, Spinizonocolpites, Proxapertites, Longapertites, Retimonocolpites and Retitricolpites (Fig. 5), which have affinities to modern palms (see Muller, 1968; Thanikaimoni et al. 1984; Schrank, 1987; El Beialy, 1995). Referred to as Nypa by Atta-Peters and Salami (2006), these pollens are reliable indicators of coastal to mangrove environments in the humid tropics (Adebanji, 2012; Herngreen, 1998; Schrank, 1987). These monocolpate pollen taxa have been locally recovered from Maastrichtian sediments such as the Patti Formation of the southern Bida subbasin (Ojo and Akande, 2004; Ojo 2009), Nkporo Shale in the Calabar Flank (Edet and Nyong, 1994), Ojo-1 Well in the Dahomey Embayment (Jan Du Chene et al. 1978), Araromi Shale and Abeokuta Formation in the Dahomey Basin (Salami 1982; 1988), and the Anambra Trough (Salami 1990) in Nigeria. Similarly, these taxa correlate with the Palmae Province of Senegal and Ivory Coast (Jardiné and Magloire, 1965), Brazil (Herngreen, 1975), Northern Somalia (Schrank, 1994b), Egypt (El Beialy, 1995; Schrank, 1987), and other areas stated by Atta-Peters and Salami (2004).
Dino et al. (1999) stressed the inappropriateness of inferring palaeoclimate based on the presence of pollen and spore plants alone in sedimentary terrains. This is because factors, such as physiographic/biotic processes exert significant controls on their distributions, owing to the interplay of sedimentary materials/successions and vegetation. However, sorting recovered palynomorphs into their botanical affinity groups or associations is a veritable and acceptable means to constrain prevailing palaeovegetation zone and palaeoclimate condition during sediment deposition (see Dino et al. 1999; Jianguo et al. 2015). Thus, the classification of palynomorphs based on botanical affinities in Sect. 4.2. was adopted to aid palaeoclimate interpretation (Figs. 7–8).
The domination of angiosperm pollens over other botanical groups of palynomorphs in tropical forest is an indicator of less seasonal, wetter, and cooler climate (Boyce et al. 2010). Taking clues from the documented predominance of angiosperm (ca. 48.40 % ) as indicated in Figs. 5 and 7, vis-à-vis the high occurrences of taxa such as Tricolporopollenites, Triporate, Triorites, Retimonocolpites and Psilatriporites (Figs. 5 and 8) in the studied succession is thus alluding to a wet or humid tropical climate. This agrees with Herngreen (1998), and consequently indicate that the successions in southern Bornu Basin encompass the wet lowland forest that is associated with the Nypa mangrove zone. The late Cretaceous Palmae Province is implied from this elevated habitat and suggestive of a tropical - subtropical climate system (T-SCS). According to Vakhrameev (1991), the T-SCS is typified by assemblages that are indicative of a warm (e.g., Classopollis spp., Alnus vera etc) and humid (Inaperturopollenites spp. Proxapertites spp., Spinizonocolpites baculatus etc) climate as recorded in this study (see Fig. 8). Similarly, Jianguo et al. (2015) narrated that Cupaniedites (regarded as Sapindaceae), and Proteacidites (of proteaceous origin) (see Figs. 5 and 8) have their modern representatives as trees and shrubs known to inhabit and flourish in the tropical and subtropical climate, and arid conditions, respectively. Although, the taxa recorded few incidences in the studied successions (Fig. 8A), their presence reasonably buttressed a palaeoclimate system affiliated to tropical, subtropical, and warm – temperature zones (Ibid).
The Cenomanian in the studied succession is typified by a low diversification and sparse occurrence of sporomorphs with an accompanied rarity of dinoflagellates (see Fig. 4). This, in addition to the inferred continental/coastal environment of the upward coarsening, generally angular, and brownish sediment successions (Fig. 4) signify a warm arid to semi-arid palaeoclimate condition. Though very rare, the occurrence of the gymnosperm pollen, Classopollis (Fig. 8B), which is presumably an autochthonous fossil plant, is indicative of mid-dry zones (semi-arid) under warm climate (Dino et al. 1999). The nonattendance of elaterate pollens together with its associated palynomorphs within the Cenomanian interval of the Gaibu − 1 Well suggests the interval does not belong to the Albian–Cenomanian African–South America (ASA) palynofloral province (see Herngreen, 1974; Dino et al. 1999).
The upper section (Turonian - younger) of the studied well yielded increasing occurrences of dinoflagellate cysts (see Figs. 4 and 7B) that could reflect increasing marine tendencies uphole, and by implication implying possible progressive semi-arid with a humid condition. The Campanian – Maastrichtian brownish shale and sands in this study contain mangrove palms of Nypa vegetation such as Acrostichum aureum (Figs. 4 and 8C), Spinizonocolpites, Proxapertites, and Longapertites (Figs. 5 and 8A) that are related to those from northern South America and West Africa. Their existences in the studied successions also indicate tropical to subtropical climate (Dino et al. 1999; Schrank 1987). The Nypa vegetation is a prominent component of the mangrove environment in humid tropics (Herngreen, 1998; Schrank, 1987). It is thus deducible that the sequences penetrated by the Gaibu-1 Well were deposited apt into the late Cretaceous Palmae Province of Africa – northern South America (Herngreen and Chlonova, 1981; Herngreen et al. 1996) that typifies the documented palynologic complexes of Equatorial (palm) region of western Africa and South America (Vakhrameev, 1991). This is substantiated by the appreciable frequency of taxa attributed to the Palmae (e.g., Proteacidites spp., Psilatricolpites spp., Spinizonocolpites baculatus), and the concomitant dearth of Normapolles – group of pollens (Atta-Peters and Salami, 2004).