Identification of
Maupasella mucronata
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Maupasella mucronata
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was originally described in the genus
Schultzellina Cépède 1910
, which was established in memory of Max Schultze, a prominent zoologist of that time. Cépède (1910) characterized the monotypic genus
Schultzellina
by a conspicuous skeletal apparatus and dense somatic ciliature. However, Heidenreich (1935) considered
S. mucronata
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to be a junior synonym of
M. nova Cépède 1910
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. De Puytorac (1954) accepted the transfer of
S. mucronata
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into the genus
Maupasella
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but not the synonymization of
M. mucronata
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with
M. nova
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.
Schultzellina
was found to be a junior synonym of
Maupasella
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by all subsequent reviser authors ( Aescht 2001; Corliss 1979; de Puytorac 1972).
Cépède (1910) discovered
M. murconata
in the middle part of the digestive tract of the earthworm “
Allurus tetraedrus
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” (=
Eiseniella tetraedra
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). Heidenreich (1935) assigned all ciliates identified as
M. mucronata
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or
M. nova
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( Bhatia and Gulatti 1927; Cheissin 1930; Eksemplarskaja 1931; Pertzewa 1929; Rossolimo 1926) to the
M. nova
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complex. However, none of these authors reported
M. mucronata
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or
M. nova
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from
Eiseniella tetraedra
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, the type host of
M. mucronata
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. As mentioned above, de Puytorac (1954) and then Lom (1961) did not follow Heidenreich’ s (1935) synonymization of
M. mucronata
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with
M. nova
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, and their reports of
M. mucronata
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came exclusively from the type host
Eiseniella tetraedra
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. In addition to
Eiseniella tetraedra, Dixon (1975)
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detected
M. mucronata
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along with
M. cepedei de Puytorac 1954
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(=
M. nova
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according to Dixon 1975) and
M. herculei de Puytorac 1954
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in
Eisenia fetida
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,
Lumbricus castaneus ( Savigny 1826)
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, and
Aporrectodea caliginosa
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. However, these records are not substantiated by any morphological data. Unfortunately, there is a taxonomic chaos and trustworthy morphological features for distinguishing
M. mucronata
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,
M. nova
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,
M. cepedei
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, and
M. herculei
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are not known.
Cépède (1910) stated that the body length of
M. mucronata
ranges from 20 to 30 μm, and there are 15 ciliary rows on each side. Heidenreich (1935) recognized two size forms in the
M. nova
complex: the smaller form is 22–35 μm long, free swimming in the gut content and possibly serves for infestation, while the larger form is 35–76 μm long and usually attached to the intestine epithelium by the means of the apical spine. Cépède (1910) also mentioned two size forms in
M. nova
(smaller form up to 82 × 39 μm, larger form 117 × 18 μm) but not in
M. mucronata
. De Puytorac (1954) stated that the observed specimens of
M. mucronata
were about 90 × 48 μm in size immediately after division and had 46 ciliary rows. Lom (1961) provided an average size of 67 × 21 μm and a variation range of 41–50 ciliary rows. The presently studied population was about 90–95 × 43–63 μm in size and had 21– 23 rows on the ventral side and approximately 19 rows on the dorsal side. Our values are thus most similar to those of de Puytorac (1954) and Lom (1961). Although they are quite different from those of Cépède (1910), we cannot exclude that he observed only en-/excysting cells or overlooked the larger form, which was reported in other possibly closely related Maupasella species (see above). Because our measurements are close to those of the revising authors ( de Puytorac 1954; Lom 1961) and the host organisms match, we assign our population to
M. mucronata
. To solve the taxonomic problem, detailed morphological and molecular data from populations resembling
M. mucronata
and
M. nova
isolated from various host earthworms are needed.
Evolution and phylogenetic systematics of astome ciliates
As we have already thoroughly discussed elsewhere ( Obert and Vďačný 2019, 2020), astomes show an interesting eco-evolutionary trend. Their phylogeny has very likely proceeded through specialization to various ecological/systematic groups of their host organisms. On the other hand, there is only little correlation between the traditional morphology-based classifications of astomes and their groupings in the phylogenetic trees ( Fokam et al. 2011; Obert and Vďačný 2019, 2020; Rataj and Vďačný 2018, 2019; Sauvadet et al. 2017). Thus, various morphologically dissimilar astomes belonging to the genera
Njinella Ngassam 1983
,
Paraclausilocola Fokam et al. 2011
,
Eudrilophrya de Puytorac 1969
, and “
Metaradiophrya sp.
” sensu Fokam et al. 2011, which were isolated from the endogeic megascolecid earthworm
Eupolytoreutus
, group together in the 18S rRNA gene phylogenies. Likewise, highly morphologically dissimilar astomes of the genera
Metaracoelophrya de Puytorac and Dragesco 1969
and
Almophrya de Puytorac and Dragesco 1969
, which were isolated from the endogeic glossoscolecid earthworm
Alma Grube 1855
, cluster together in the phylogenetic trees.
Maupasella
and
Subanoplophrya Obert and Vďačný 2020
, which were isolated from the endogeic lumbricid earthworms of the genera
Eiseniella Michaelsen 1900
and
Octolasion Örley 1885
, are depicted as independent and not closely related lineages within the paraphyletic endogeic cluster containing astomes living in megascolecid and glossoscolecid earthworms.
Njinella
,
Almophrya
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, and
Anoplophrya
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were traditionally classified within the family
Anoplophryidae
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due to the lack of holdfast organelles ( de Puytorac 1994; Jankowski 2007; Lynn 2008).
Haptophrya Stein 1867
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,
Subanoplophrya
, and
Paraclausilocola
also do not have any attachment apparatus, but they were placed in nominotypical families or incertae sedis in the Astomatia due to their conspicuous morphological/genetic differences ( Fokam et al. 2011; Obert and Vďačný 2020; Rataj and Vďačný 2018).
Eudrilophrya
,
Metaracoelophrya
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, and
Metaradiophrya
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were traditionally assigned to the family
Radiophryidae
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based on the Λ- shaped cytoskeletal attachment organelle. However, all three genera are phylogenetically fairly distant ( Figs. 5
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, 6
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, and 7). The traditional classification of astomes into families is thus not reflected in the phylogenetic trees at all, i.e.,
Anoplophryidae
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and
Radiophryidae
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are polyphyletic and taxa without attachment organelles are scattered over the astome tree of life and mixed with taxa equipped with a holdfast apparatus. This systematic chaos was very likely caused by two evolutionary phenomena—adaptive radiation and host-driven diversification. The presence of adaptive radiation is indicated by clustering of morphologically dissimilar taxa inhabiting the same host organism, while host-driven speciation is suggested by clustering of taxa within a clade according to the ecological group of their host organisms. Adaptive radiation is evidenced by clades containing morphologically dissimilar astomes obtained exclusively from megascolecid and glossoscolecid earthworms. Host-driven diversification is evidenced by taxa clustering within the genera
Anoplophrya
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and
Metaradiophrya
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according to the ecological groups of their host earthworms ( Obert and Vďačný 2019, 2020; present study).
The present as well as the previous phylogenetic analyses show that the systematics of the subclass Astomatia is in a need of revision. The reconciliation of the traditional and molecular frameworks will very likely require accounting for adaptive radiation and host-driven diversification, evolutionary phenomena that might have shaped and governed the evolution of astome ciliates. However, much larger genetic sampling of the morphological and ecological diversity of astomes is required to obtain a clearer picture of the evolutionary trends in this peculiar clade of endosymbiotic ciliates.