The Stratigraphic, Palaeobiogeographic and Phylogenetic Significance of Aquilapollenites

DOI: 10.4236/ojg.2019.910051   PDF   HTML   XML   59 Downloads   93 Views  


Angiosperm evolved and diversified during Cretaceous. During this course of evolution and radiation, various pollen of uncertain origin had evolved. Aquilapollenites represents the early stock of angiosperms attaining its acme with respect to diversity and dominance during Campanian and Maastrichtian age. It was globally present (except Antarctica) however more dominant in northern hemisphere (Canada, North America, Sakhlain Oblast and China). In India, the Aquilapollenites sp. is present in Maastrichtian aged deposits. The pollen affinity has been associated with Loranthaceae and Santalaceae plant families. Here, a comparative description of all the Aquilapollenites sp. comprising a wide range of morphological diversity has been discussed. The wider morphological diversity and ecological adaptability of Aquilapollenites sp. infer that it is globally significant and warrants a more detailed study.

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Mishra, S. , Nagaraju, S. , Bansal, M. and Prasad, V. (2019) The Stratigraphic, Palaeobiogeographic and Phylogenetic Significance of Aquilapollenites. Open Journal of Geology, 9, 597-600. doi: 10.4236/ojg.2019.910051.

1. Introduction

Aquilapollenites sp. [1] was amended with the advancement in the field of microscopy [2] [3] . Aquilapollenites sp. belongs to a group of Triprojectacites [4] . This group includes angiosperm pollen with three equatorial projections and a polar projection on each side. Aquilapollenites sp. attained its maximum abundance and diversity during Campanian and Maastrichtian [5] . It is believed to evolve during the Turonian [6] ; there are several pre-Turonian records from northern and southern hemisphere. Records of this pollen extend up to Eocene but most are reworked [7] .

There is a total of 180 species of Aquilapollenites sp. out of which only twelve occur in Indian sub-continent, restricted to Maastrichtian aged deposits [8] . The pollen is morphologically very diverse and consists of a wide variety of features. The pollen affinity has been discussed in detail by Jarzen [9] and assigned to Loranthaceae and Santalaceae plant family with uncertainty. Here we present the comparative description of morphological variation in the Aquilapollenites sp. along with its stratigraphic, palaeobiogeographic and phylogenetic significance.

2. Comparative Morphological Description of Aquilapollenites sp.

Aquilapollenites sp. bears a unique morphology with three equatorial protrusion and one polar protrusion on each side. It constitutes heteropolar, subisopolar to isopolar pollen forms. The size of the polar protrusion varies considerably. Pollen which either have one very small polar projection (less than half of the developed polar projections) or bear only one polar projection have been transferred to the genus Mancicorpus [3] . The number of equatorial projections is 3 - 4, oriented either equatorially or meridional. The shape of equatorial protrusion ranges from cylindrical, auriculate to conical. There is a wide difference between the ratio of polar and equatorial protrusion. In few species both protrusions are well developed while in others either of the two is well-developed. In Indian Aquilapollenites sp. forms, polar protrusion is well developed while equatorial protrusions are very small peg like structure [8] . The apertures are 3 to 4 in number and situated either equatorially or meridionally. The most common aperture type of Aquilapollenites sp. is colpi, rarely demicolpi (common in Indian species) and only one species of tricolporate pollen (A. amicus).

There is a wide variety of morphological diversity in the exine ornamentation, supratectal elements and their distribution. Pollen mostly bear reticulate and striatoreticulate ornamentation. However, psilate, punctate, foveolate, retipilate, infrareticulate and granulate also occur in some species. The supratetcal elements mostly consist of acuminate spines with few species having pila, scale or crystal shaped spines. Most of the Indian Aquilapollenites sp. bear striatoreticulate ornamentation and are devoid of supratectal elements. In few species, dimorphism is very common in Aquilapollenites sp. showing different ornamentation on equatorial, polar and central region of the pollen. Sometimes spines only occur at the borders of the colpi extending from one end to the other forming a “Dragon Comb” like structure [10] .

3. Stratigraphic, Palaeobiogeographic and Phylogenetic Significance of Aquilapollenites sp.

Aquilapollenites sp. represents the early stock of angiosperm. It originated during the Early Cretaceous when the world was represented by one phytogeographical province [11] . The increased tectonic activity during the late Cretaceous resulted in the formation of new continental assembly and changing global precipitation pattern and climate [12] . The angiosperms diversified during this time gave rise to nine phytogeographical provinces [13] . The Aquilapollenites phytogeographical province was majorly restricted to northern hemisphere due to its higher abundance and diversity in this region. However, Aquilapollenites sp. was globally present in the late Cretaceous palynoassemblages except Antarctica. Its affinity has been related to parasitic plants of Loranthaceae and Santalaceae families with uncertainty [9] . Thus, Aquilapollenites sp. holds an interesting history of angiosperm diversification and adaptation which warrants more detailed study. The vast array of data regarding Aquilapollenites sp. needs to be compiled and analyzed using phylogenetic approach to identify its affinity, contribution in angiosperm evolution and palaeobiogeographic distribution.


I (S.M.) gratefully acknowledge Dr. Vandana Prasad, Director, BSIP, Lucknow for permitting us to publish. I am also thankful to Prof. Gang Li and the organizing committee of UNESCO/IUGS/IGCP 679 2019 for their help and travel support.

Conflicts of Interest

The authors declare no conflicts of interest regarding the publication of this paper.


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