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An extinct species of Basella: pollen evidence from
sediments (~80 ka) in Kerala, India
Anjum FarooquiANJUM FAROOQUI, Joseph G. RayJOSEPH G. RAY & Arti
GargARTI GARG
To cite this article: Anjum FarooquiANJUM FAROOQUI, Joseph G. RayJOSEPH G. RAY & Arti
GargARTI GARG (2019): An extinct species of Basella: pollen evidence from sediments (~80 ka) in
Kerala, India, Grana, DOI: 10.1080/00173134.2019.1630479
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Grana, 2019
https://doi.org/10.1080/00173134.2019.1630479
An extinct species of Basella: pollen evidence from sediments (~80 ka)
in Kerala, India
ANJUM FAROOQUI1, JOSEPH G. RAY2 & ARTI GARG3
1
Birbal Sahni Institute of Palaeosciences, Lucknow, India, 2School of Biosciences, Mahatma Gandhi University, Kottayam,
India, 3Botanical Survey of India, Allahabad, India
Abstract
The genus Basella belongs to family Basellaceae and is comprised of five species. Out of these, Basella alba is pantropical in
distribution, B. paniculata is endemic to south-eastern Africa and the other three species viz. B. excavata, B. leandriana and
B. madagascariensis are endemic to Madagascar. The palynological study of an organic layer buried ~80 ka in Chaganacherry, Kerala revealed a rich diversity of rainforest pollen and estuarine/marine palynomorphs indicating warm and humid
climate coupled with sea level high stand. The Basella pollen recorded from this sediment shows intermediate characters of
two extant Basella species. While it resembles B. paniculata in being pantocolpate (20), it shows affinity with B. alba in
sexine characters. The recovered pollen was therefore, ascertained to be a new species, named here as B. keralensis sp. nov.
The age correlation of the studied sediment was carried out by fingerprinting (Rare Earth Elements) of Youngest Toba
Tuff (YTT) (glass shards) which spread in the atmosphere through a volcanic eruption in Sumatra ~74 ka and also with
marine palynomorph markers correlating the interglacial Marine Isotopic Stage 5a (~80 ka). It is inferred that earlier, the
genus Basella comprised of six species out of which Basella keralensis sp. nov. became extinct and until now neither the fossil
record nor the extant form of this is known in records from any part of the World.
Keywords: Basella keralensis, southern-Western Ghats, Kerala, late Quaternary
The tropical montane rainforest in southern Western Ghats, Kerala (Barboni et al. 2003) is a home
to many endemic floras (Pascal 1982; Pascal et al.
1982). This flora is the legacy of the Paleogene/
Neogene time period (Ramanujam 1987) and has
continued to exist during Pleistocene (Prasad et al.
2009; Farooqui et al. 2010, 2014) where species
extinction and migration cannot be ruled out. The
vegetation affirms the presence of a monsoon-like
atmospheric circulation over southern Western
Ghats in India since the Middle Miocene Climate
Optimum (MMCO) (Ramanujam et al. 1991; Campanile et al. 2008). Scant records of rainforest pollen
taxa during Quaternary glacial and interglacial
cycles are available from Arabian Sea sediments
(Van Campo et al. 1982; Caratini et al. 1994; Bentaleb et al. 1997; Prabhu et al. 2004) and from
Kerala (Vasanthy 1988; Narayanan et al. 2002;
Kumaran et al. 2008). At present southern Western
Ghats montane vegetation occupies temperate habitats at tropical latitudes. The relics of an ecoclimatic
and geologic past are preserved in its pristine form
and have been described as fossil rainforest ecosystem. The palynological records on land from Palani
and Annamalai Hills in southern Western Ghats
showed prevalence of savanna grassland vegetation
during the last glacial cycle of the Quaternary
(Vishnu-Mittre & Gupta 1971; Blasco & Thanikaimoni 1974; Vasanthy 1988; Gupta & Bera 1996;
Rajagopalan et al. 1997). This time period was
extremely adverse and could not sustain many
plant species. For example, the pollen of Ongokea
gore (Hua) Pierre, now confined to Congo-adjoining
areas and in more humid southeast Asia was
reported from marine sediment, off Kerala during
Marine Isotopic Stage 5a (MIS 5a) (Farooqui et al.
2014). The palynological record shows that the present day southern Western Ghats flora rejuvenated
Correspondence: Anjum Farooqui, Birbal Sahni Institute of Palaeosciences, 53, University Road, Lucknow, India. E-mail: afarooqui_2000@yahoo.com
(Received 27 October 2016; accepted 25 April 2019)
© 2019 Collegium Palynologicum Scandinavicum
2
A. Farooqui et al.
with the onset of warm and humid conditions during
the Middle Holocene (Bera & Farooqui 2000).
The two sedimentary profiles studied earlier from
Chaganacherry (Farooqui et al. 2010) were restudied
as it had great potential to explore pollen diversity
during the interglacial cycle of Pleistocene epoch.
The present work elucidates morphology of new fossil
Basella pollen recovered in the sediment from Chaganacherry which is typical of the genus but differs in
pollen grain morphology when compared to other five
extant species which are distributed world over.
Study site in the southern Western Ghats, India
Vazhapally in Chaganacherry, district Kottayam is
situated southeast of Vembanad Lake and Alleppey
coastline (Figures 1, 2). Two laterite ridges dominate
the Vazhapally area, which is ~25 km from the present
shoreline in the southwest coast of the Indian peninsula. The slope gradient varies from low (300 m above
sea level [a.s.l.]), medium (300–650 m a.s.l.) to highlands (> 650 m a.s.l.). The vegetation is mainly tropical moist evergreen or moist deciduous, receiving
2000–3500 mm of average rainfall from the southwest
and northeast monsoons (Champion & Seth 1968;
Bonnefille et al. 1999). The vegetation is adapted to
temperatures not exceeding 35 °C in summers and
mild winters at low altitudes but cooler/misty weather
conditions at high altitudes, particularly in valleys
harbouring a rich biodiversity. Many plants and animals are endemic to this region and the climate and
vegetation gradient from low to high altitudes is well
documented (Pascal 1988; Barboni et al. 2003).
Classification, distribution and habitat of Basella species
The family Basellaceae is classified under the suborder
Portulacineae (Kubitzki et al. 1993). Total five extant
species of the genus Basella are distributed world over.
Basella alba/B. rubra is pantropical in distribution
(Figure 1). It grows in warm and humid climate
(Swati & Agarwal 2015) and is commonly found in
India, China, Malaysia, Indonesia, Philippines, southern China, New Guinea, Africa, Central America and
several adjoining oceanic islands. Basella excavata
Elliot, B. leandriana H. Perrier and B. madagascariensis
Boivin ex Perrier are endemic to Madagascar. Basella
paniculata Volkens is endemic to Kenya, Tanzania,
Mozambique, Transvaal and Kwazulu-Natal in East
Africa (Stannard 1988; Eriksson 2007). All the species
of Basella are perennial twining herbs (climbers) having glabrous stem and succulent leaves. The sepals are
greenish white or pinkish purple. The petals are green
as well as white to pink purple (Kubitzki et al. 1993).
It is self-pollinated and entomophilous occurring at
altitudes ranging from 20 to 1350 m. The fruits are
berries/drupes that are dispersed by birds.
Material and methods
The sedimentary soil section in Vazhapally, Chaganacherry (Figures 2, 3) is located southeast of Vembanad
Lake at 8° 350ʹ N and 76° 300ʹ E. A well was dug out
Figure 1. Distribution map of extant Basella species and location of extinct Basella keralensis from the Indian subcontinent.
Pollen of an extinct Basella keralensis, India
3
Figure 2. Vegetation pattern in the southern peninsular part of India and location map of Chaganacherry, Kerala, India and the extent of
Youngest Toba Tuff (YTT) ash dispersal (redrawn from Pattan et al. 2001).
manually (2 m in diameter) for the retrieval of groundwater in Vazhapally and samples were collected for
palynological investigation from the exposed sediment
section. The organic matter (OM, 3 min thickness) in
the well section was used for palynological study (FigFigure 3). Other layers in the entire section did not yield
any pollen/spores. Random picking of 10 g sample from
the unconsolidated OM layer between 13 and 13.5 m
was taken for the palynological study as the maximum
pollen yield was at this depth. The OM layer contained
ash, carbonised seeds, plant twigs, abundant resinous
matter and a strong odour of sulphur along with glass
shards of Youngest Toba Tuff (YTT) (Farooqui et al.
2010). The radiocarbon age (carbon-14, 14C) of the
organic carbon in bulk sediment was analysed in Birbal
Sahni Institute of Palaeosciences (BSIP), Lucknow,
India and calibrated following Stuiver et al. (1998).
Since the radiocarbon (14C) age of the studied OM
goes back to > 40 000 yr BP (Figure 3), which is beyond
the limit of this methodology for dating, to ascertain the
time period of the buried OM the fingerprinting of trace
and rare earth elements (REE) in glass shards (Farooqui et al. 2010) was carried out using inductively
coupled plasma mass spectrometry (ICP-MS) (Varian
820-MS). The REE results were in conformation with
the earlier records of REE for the YTT ash that erupted
~74 ka (Rose & Chesner 1987; Chesner et al. 1991;
Pattan et al. 2001).
For palynology, about 10 g of sediment was treated with a warm 10% potassium hydroxide solution
(in deionised water) and sieved through a 150 mesh
(105 µm pore size). The filtrate was settled over-
4
A. Farooqui et al.
keralensis pollen constituting 1.02% were recorded.
It was observed that the morphology of the fossil
pollen was intermediate, showing affinities with
two extant species, i.e. B. alba/B. rubra and B. paniculata. Thus, the fossil pollen did not show resemblance with any of the five extant Basella species and
therefore, it has been assigned to a status of new
species. The systematic description and detailed pollen morphology is given here.
Systematic palynology
Family Basellaceae
Genus Basella
Basella keralensis sp. nov.
(Figures 4A–F, 5)
Etymology. — The specific epithet is derived from
Kerala (India), the area of collection of the fossil
sediments.
Figure 3. Lithology, sediment texture and pollen percentage in
the sedimentary section, Chaganacherry, Kerala, India.
night and the supernatant drained. The residue was
treated with 40% hydrofluoric acid and later acetolysed following Faegri and Iverson (1989). Subsequently, it was sieved through 650 mesh size
(10 µm) and the residue was mounted on glass slides
in glycerine jelly for palynological study under a high
power light microscope (Olympus BX-51). Out of
320 total pollen counts, only four grains of Basella
pollen were recovered (Figure 3). Pollen characteristics of five extant Basella species (Table I) were
documented referring to Erdtman (1952), Kubitzki
et al. (1993), Nowicke (1996), Punt et al. (2007),
Halbritter (2015) and Halbritter et al. (2018). The
reference pollen slide of B. alba L. housed in a
pollen repository of the French Institute, Pondicherry (India) was also studied under a light microscope (Figure 4) for its comparison with the fossil
pollen. Figures 4A–F, 5 show the light microscope
images of a single fossil pollen grain of B. keralensis.
A drop of homogenised maceral was mounted in
glycerine medium and the identified pollen was
rolled by ticking on coverslip in order to capture
images in different orientation for the study of pollen morphology.
Results
Among all the pollen/spores recorded in the OM
(Figure 3) only four grains of rare fossil Basella
Holotype. — Pollen specimen BSIP Slide No.
15822. Coordinates: G 3 (Figure 4A).
The slides are deposited in the museum of BSIP,
Lucknow.
Type locality and stratigraphic horizon. — The sediment was retrieved from a well section in Vazhapally, Chaganacherry (Figures 2, 3), Kottayam
district at 8° 35ʹ N and 76° 300ʹ E, Alleppey coastline, Vembanad Lake, Kerala. Figure 3 shows the
OM in which the pollen was recovered. The fingerprinting of REE of glass shards embedded in the
OM layer revealed the remains of YTT indicating
the deposition of sediment prior to or during this
event and also coincided with the highest sea level
stand on the basis of estuarine/marine palynomorph
record of MIS 5a, i.e. ~80 ka (Farooqui et al. 2010;
Fairbanks & Mathews 1978).
Diagnostic characters. — The pollen grains of Basella
keralensis sp. nov. are dice shaped (in one view),
heteropolar with one axis longer, medium sized
(~26 µm), pantocolpate, amb varying from rectangular/octangular to circular having ridges and
grooves, colpi located on ridges, crassisexinous
with perforated tectum. It is close to B. paniculata
in having more number of colpate apertures, spinulose and punctate tectum (Nowicke & Skvarla
1979). It shows affinities with B. alba in apertural
shape and exine pattern. It is also close to B. excavata in terms of pollen size.
Detailed description of Basella keralensis (Figure
4A–F). — Grains pantocolpate, brevicolpate, colpi
Table I. A comparative account of pollen morphology and morphometry of fossil grain Basella keralensis and five extant species of Basella (after Woodehouse 1935; Erdtman 1952; Nowicke &
Skvarla 1979; Nowicke 1996; Halbritter et al. 2018).
Pollen Characters
B. alba
B. paniculata
(B. keralensis sp. nov. present work)
Aperture number,
position and
character (NPC)
Colpus character
Hexacolpate, brevicolpate with one colpus arranged
diagonally in each of the six faces of the cube.
9 – (–12) Pantocolpate, colpi very
short straight, scattered on
surface cutting off many ridges.
Very short, sometimes irregular –
4 μm (4–5).
Pantocolpate (20), colpi very short, scattered
on surface cutting off many ridges.
Short, narrow to slit-like, 6 μm (5–6).
Very short – 4 μm (4–4.5) long, 2–2.5 μm
broad.
Tectum reticulate and deeply punctate, muri with or
without spinules.
Tectum spinulose and punctate.
Complete, almost as thick as
foot layer, sparsely channelled.
Tectum spinulose and punctate, complete,
almost as thick as foot layer.
Sexine (= ectoexine)
Exceedingly thick walled, rather opaque.
Thick walled, twice thicker than
endoexine, columella of variable
size.
Thick walled, twice thicker than endoexine,
columella of variable size.
Nexine
(= Endoexine)
Apertural endexine a thin layer of granules, nonapertural absent to finely granular.
Uniformely thin.
Surface pattern in
Apertural field
Large thin walled, each with one colpus. Surface
psilate or minutely spinulose. almost straight.
Apertural and non-apertural are
similar in form of a layer of very
fine granules.
Not well demarcated.
Exine of Apertural
field
Thin walled, short. Thick at ridges with elongated
columellae.
Thick walled, columellae variable,
progressively elongated on ridges to form
dome shaped buldges.
Large lumen
Punctae
Rods or columella
Occasionally with a free columellae.
More circular than angular.
Variable in length, short to elongate within a grain.
Ending in muri; some are free; rarely projecting
beyond to form spinule. Elongated along ridges,
shortened nearer the apertural fields and colpus.
Thin. Not fused.
Thick walled, columellae variable,
not of uniform length both short
and long present (around the
aperture).
Free columellae absent.
More angular than circular.
Projects out of muri at places.
Uniform in length. As thick as
long as the thickness of foot
layer. Surfaces slightly granular.
Uniform, well developed, as thick
or slightly thicker than tectum.
Foot layer
Reticuloid.
Free columellae absent.
More angular than circular.
End in muri sometimes projecting to form
spinules. Variable in length. Elongated to
double length in all ridges, shortened
nearer to apertural fields and colpus.
Uniform, well developed, almost as thick as
tectum, not fused.
Hexacolpate. One
colpus in each of the
six faces of cube.
B. leandriana 5 (5–6)
B. excavata 4 (range
3–4)
B. madagascariensis
5 (5–6) slit like.
Psilate and deeply
punctuate or more
rarely with larger
perforations, without
spinules.
Thick walled, thicker
than endoexine.
columella partially
fused. Foot layer
uniform.
—
Narrow, thin walled,
granular or minutely
spinulose, almost
straight.
Thin walled, granular
or minutely
spinulose.
—
—
Short to elongate within
a grain.
—
Pollen of an extinct Basella keralensis, India
Surface
ornamentation
(tectum
character)
B excavata, B.
leandriana and B.
madagascariensis
(Continued )
5
Mostly spheroidal grains with one axis
longer. The shape is a modified form of
cube.
Perfect cuboidal.
Pollen shape
Mostly spheroidal, one axis longer
than the other.
B. excavata 28 (range
26–31)
B. leandriana 51
(43–59)
B. madagascariensis 46
(43–48).
Cuboidal to
subcuboidal rarely
almost spheroidal.
Longest axis × shortest axis: 27.5 × 22 μm
(range 22–28 × 21–27 μm).
42 (36–46).
31 × 31 μm (range 29–33).
Pollen size
Pollen Characters
B. alba
B. paniculata
(B. keralensis sp. nov. present work)
B excavata, B.
leandriana and B.
madagascariensis
A. Farooqui et al.
Table I. (Continued ).
6
Figure 4. Light microscope images of Basella keralensis (A–F,
different views of a single pollen). A–D. Basella keralensis, pollen
monad, medium-sized, heteropolar, pantoaperturate pollen with
a dice-shaped appearance. C. Shows measurements of a single
dice view and the columellae length at the ridge. E, F. Spherical
shape in polar view showing about 20 pantocolpate apertures
marked with ridges/bulges due to longer columellae. F. (inset)
Schematic representation of four to five dices overlapping at
varied angle perhaps shows the ridges of the pollen in this manner; X – spinules; Y –length of short colpi/rugae. G, H. The exine
morphology and size dimensions of Basella alba (courtesy of the
French Institute, Pondicherry) showing exine morphology and
dice shaped grain which is typical of the genus. H. Shows measurements of the dice along with the length of the columellae at
the ridge in B. alba. Scale bars – 10 µm.
is 4–4.5 µm × 2–2.5 µm, up to 20 in number, sparsely
and evenly distributed across the surface of the grains,
arranged in four corners of the dice-shaped (Figure 4D)
Pollen of an extinct Basella keralensis, India
7
Discussion
Figure 5. Light microscope images of Basella keralensis. A–F.
Basella keralensis: different views of the grain showing amb
which exhibits much variability from quadrangular/octangular/
polygonal/circular outline in different polar views with prominent
ridges corresponding to aperture number. In all the image views a
reticulate, free-standing columellae is observed, near the rugae
the sexine consists of low elements giving reticulate/spinulose
appearance. However at a greater distance from the rugae
(colpi) at the corners of the dice, very long columellae appear
and the tectum gives angular perforated reticuloid pattern. At
places the muri is either free or spinulated. Scale bars – 10 µm.
grains as shown in different views, typical of the genus
Basella. Exine crassisexinous (sexine twice as thick as
the nexine), exceptionally thicker on ridges forming
dome shaped bulges (ridges), very long sexinous rods
appear near the ridges forming a spinulose-reticuloid
surface (Figure 5A–F) at the ridge margins; columellae
2.5–2.6 µm long at ridges, reducing to 1–1.5 µm all over
the grain, at ridges it is longer than two times. Tectum
not continuous, angular perforations and reticulate pattern observed with muri with or without spinules at
some places. Foot layer does not appear fused, intine
is uniformly thin all over the grain and the pollen measures 22 µm × 26 µm.
A comparative account of the five extant Basella species
and the recovered fossil pollen with respect to pollen
size, aperture and exine features differentiated it into a
new Basella species preserved in Pleistocene sediments
from Kerala, India. The pollen size in B. alba is relatively smaller and almost similar to B. excavata (26–
31 µm) followed by B. paniculata (36–46 µm) and the
larger size are of B. madagascariensis (43–48 µm) and B.
leandriana (43–59) as documented by Nowicke (1996).
Thus, the pollen size of B. keralensis is very close to B.
alba and B. excavata. The shape is perfect cuboidal in B.
alba but sub-cuboidal in B. excavata, B. leandriana and
B. madagascariensis, however, it is spheroidal in B. paniculata. Basella paniculata pollen is characterised by 12–
15 colpi having spinulose and punctate tectum (Nowicke & Skvarla 1979; Nowicke 1996). Except for B.
paniculata, all the other four extant species have similar
number of pollen apertures, i.e. six colpi (Erdtman
1952). The grains are brevicolpate and each colpi measures 4.5–6 µm long in B. paniculata. However, in B.
keralensis the length of each colpi is relatively shorter (4–
4.5 µm) perhaps due to the increased number of colpi
and smaller grain size as compared to B. paniculata.
The surface ornamentation of pantropical B. alba pollen is similar to B. excavata, B. leandriana and B. madagascariensis but differs with B. paniculata and B.
keralensis in having spinulose tectum. The length of
columellae at ridges varies within all five species. In B.
alba and B. keralensis the columellae at ridges are twice
longer than all over the grain. In B. alba (Figure 4G, H)
the columellae are 4.5 µm at the ridges and tapers to
2.5–2.6 µm in mesocolpium. In B. keralensis, the columellae at ridges are 2.5–2.6 µm, tapering to about 1.2–
1.4 µm (Figure 4C). Hence, in terms of exine characters
B. keralensis is closer to B. alba. In the rest of the four
extant species there is only a slight variation in the
length of columellae at the aperture (Nowicke 1996)
and therefore, ridges are not prominent, particularly in
the B. paniculata pollen. Tectum is uniformly perforate
in all species. Volkens (1907) first described B. paniculata to be comparable with B. alba; mainly because B.
paniculata is described as having tectum typical of the
order, punctae more angular and at places spinulate or
without spinulate conditions but varied in the length of
columellae at ridges. The collumellae, both at ridges
near colpi and mesocolpium are relatively longer in B.
alba than B. keralensis. However, the ratio of collumellae length at ridges and non-ridge area is similar in B.
alba and B. keralensis as well. Based on several relevant
plant morphological characters, both B. paniculata and
B. alba are considered congeneric (Baker & Wright
1913; Nowicke 1996). However, the flowers of B. paniculata are very different from B. alba (Stannard 1988)
and also vary in the pollen morphology. It is observed
8
A. Farooqui et al.
that pollen morphological affinity of B. keralensis is with
B. paniculata in respect to number of apertures which is
the primary character (NPC, number position character) to classify a taxon (Woodehouse 1935; VishnuMittre 1964; Nair 1965, 1970; Walker & Doyle 1975;
Perveen 2000) and with B. alba/B. rubra with respect to
exine structure which is secondary in character for
identification. Hence, B. keralensis exhibits intermediate character and shows closer lineage with two extant
Basella species, i.e. B. paniculata and B. alba/B. rubra. It
is concluded that B. keralensis occurred in India, around
80 ka perhaps when the climate was warmer and more
humid than present during the interglacial cycle (MIS
5a, Shackleton [2000]) of Quaternary period. The present study therefore, confirms the existence of six species of Basella in the past, of which B. keralensis is
considered as extinct until any reports of this pollen/
plant is reported in future from any part of the world.
Conclusions
The thin organic layer at 13–13.5 m deep sediment
buried ~80 ka in a sedimentary sequence from a wellsection in Chaganacherry, Kerala, India, yielded Basella pollen of family Basellaceae. Out of the five extant
species of Basella, the recovered fossil pollen shows
affinity with B. paniculata in primary characters of
pollen, namely number of apertures (~20 sunken, pantocolpate) but resembled B. alba in secondary characters viz. exine morphology and columellar
morphometry. The fossil pollen was ascribed to a
new species, B. keralensis as it was recovered from
Kerala state in India and shows intermediate characters of B. paniculata and B. alba. To date, this is the
first record of B. keralensis, in the geological time period and it grew until ~74 ka in the Indian sub-continent. As it has been not found elsewhere either in fossil
records or as extant species it is considered as an
extinct species. Thus, a total of six species of Basella
occurred in the past out of which only five are living.
Acknowledgements
The authors thank the Director, Birbal Sahni Institute of Palaeosciences (BSIP) for granting permission to this collaborative work. The authors
sincerely thank S Prasad, French Institute, Pondicherry for sparing the time to study the reference
slides and provide valuable suggestions. Thanks are
also due to MS Chauhan, ex-scientist, BSIP and to
Director, Botanical Survey of India, Allahabad for
encouragement. The authors are highly grateful to
Thomas Denk, Department of Palaeobotany, Swedish Museum of Natural History, Sweden and Friðgeir Grímsson, University of Vienna, Austria for
their valuable suggestions that helped improve the
presentation of the data.
Disclosure statement
No potential conflict of interest was reported by the
authors.
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