Stephanoceratoidea
Cardioceratidae
Both in situ records of cardioceratid aptychi and their isolated occurrences are only known from the Lower Callovian of the European part of Russia (Mitta and Keupp 2004), while Late Callovian aptychi, which belong to Quenstedtoceras, are also known from northern Poland (Lehmann 1972; Dzik 1986). Surprisingly, mass occurrences of cardioceratids, which sometimes crowded the bedding planes in the Upper Oxfordian or Upper Kimmeridgian black shales are lacking cardioceratid aptychi, albeit the Upper Oxfordian shales of the Kostroma region yielded perisphinctid aptychi. Taking reported uncalcified cephalopod jaws into account, which co-occur with numerous cardioceratids described by Dzik (1986) from the Upper Callovian of Poland and the absence of a calcitic layer in the Early Callovian ones, cardioceratid aptychi could have been fully organic and their absence might be primarily taphonomic in the Upper Jurassic. The shape of cardioceratid aptychi allows them to be described as Praestriaptychus Trauth, 1927.
Kosmoceratidae
Numerous occurrences of kosmoceratid aptychi have become known since recently. Schweigert (2000) described an in situ record of Kosmogranulaptychus Rogov, 2004a (originally referred by Schweigert to Granulaptychus Trauth, 1927) within the body chamber of Late Callovian Kosmoceras. A few years later, the suggested kosmoceratid aptychi, which were assigned to this family by co-occurrence of conchs with corresponding aptychi, were described from the Upper Bathonian (Mitta 2009) and Middle Callovian (Rogov 2004a, b) of the Russian Platform. Finally, Keupp and Mitta (2013) described and illustrated both isolated and well-preserved in situ aptychi of Early Callovian kosmoceratids. It should be noted that generic classification of kosmoceratid aptychi still remains unclear, as in some cases, they are represented by internal moulds without any traces of a calcitic layer, thus they could be assigned either to Kosmogranulaptychus or to Praestriaptychus. However, at least some Early Callovian kosmoceratids bear praestriaptychi (Keupp and Mitta 2013, Figs. 13–14), which can be distinguished from kosmogranulaptychi by a smooth outer calcitic layer. It stands to reason that the early kosmoceratids which bore praestriaptychi could have transformed into kosmogranulaptychi with outer surfaces covered by granules (Keupp and Mitta 2013). Additional records of kosmoceratid aptychi, which are assigned to this ammonite family due to their occurrence in concretions crowded with Kepplerites, were found recently by the authors in the Upper Bathonian of Mordovia. It should be noted that aptychi, which were recovered from the body chambers of Lower Callovian kosmoceratid macroconchs (Keupp and Mitta 2013, Figs. 12, 15) are characterized by a significantly smaller size compared to the corresponding ammonite conchs.
Perisphinctoidea
Perisphinctidae and Ataxioceratidae
During the last decade, findings of aptychi, which belong to the Proplanulitinae, were discovered in the Lower Callovian of European Russia (Rogov and Gulyaev 2003; Keupp and Mitta 2013). In situ records of praestriaptychi are only known from microconchs of these ammonites (Rogov and Gulyaev 2003, Fig. 2), while large-sized aptychi, assigned to perisphinctid macroconchs were found apart from their conch (Keupp and Mitta 2013, Fig. 13e). Similar aptychi were also found within the body chamber of the Late Bathonian Homoeoplanulites from NE Iran (Seyed-Emami and Schairer 2011, Fig. 3B). A poorly preserved Praestriaptychus was also discovered associated with Elatmites (Grossouvriinae, Keupp and Mitta 2013, Fig. 21). Upper Oxfordian clays and black shales, intensively studied in the Kostroma region of European Russia during the last decade (Glowniak et al. 2010; Tesakova et al. 2012), are also known as a source of the suspected perisphinctid aptychi. Praestriaptychus was usually found in black shales as isolated plates (Fig. 3f), but in situ findings are also known. The in situ occurrence of relatively small-sized Praestriaptychus within the body chamber of Dichotomosphinctes from the Upper Oxfordian Serratum Zone of Mikhalenino (Kostroma region, Fig. 2n) is the most interesting among these records. Ataxioceratid ammonites were mainly typical for Sub-mediterranean areas, except their short-lived Subboreal offshoot, separated as the subfamily Gravesiinae by Zeiss (in Fischer and Zeiss 1987). Aptychi were recorded in Early Volgian Gravesia gigas from Northern France (Boulogne-sur-Mer, see Hahn 1963, pl. 13, Fig. 1), and isolated aptychi co-occurred with Gravesia gravesiana in Swabia (Scherzinger et al. 2006). These aptychi should be referred to as Praestriaptychus.
Aulacostephanidae
Aptychi of aulacostephanid ammonites were not known previously (Ziegler 1962). During the field work in Sorkappland (Svalbard), our colleagues from the Polar Marine Geological Expedition (Lomonosov, Russia) collected some Kimmeridgian ammonites. In one of the specimens ascribed to as Rasenia cymodoce (d’Orb.) [M], there is a relatively large-sized imprint of Praestriaptychus, characterized by well-visible wide ribs on the opposite side of the slab (Fig. 2i). Our suggestion that these aptychi are belonging to Rasenia cymodoce is based on both its size and shape, while other ammonites, known from the Lower Kimmeridgian cymodoce horizon of Svalbard are characterized by a much smaller conch size compared to those of Rasenia (Rogov 2014a).
Dorsoplanitidae
First reports on the aptychi which belong to dorsoplanitid ammonites were published by Blake (1875) who mentioned an “Aptychus” from his Bed 38 of the Kimmeridge Clay of the Kimmeridge area in Dorset (Lower Volgian Elegans Zone, see Cope 1967) as well as a co-occurrence of Aptychus biplex (nomen dubium) with a conch of Ammonites biplex auct. non Sow. (species used for most Late Kimmeridgian [sensu anglico = Early Volgian and earliest Middle Volgian] British ammonites prior to 1913, cf. Cope 1967, p. 5) found in bituminous shales near Fulletby (Lincolnshire). These historical records were not figured or described, but their assignment to dorsoplanitid ammonites is based on the absence of other ammonite groups within the discussed strata. Typical praestriaptychi, which belong to Pavlovia were figured by Oates (1974, pl. 10, Fig. 3) from the Hartwell Clay of Buckinghamshire and additional records were made by Etches (Etches and Clarke 1999; refigured herein, Fig. 2a) while aptychi of older dorsoplanitids (Pectinatitinae: Pectinatites or Paravirgatites) were discovered by Etches at Dorset (Etches and Clarke 1999; refigured herein, Fig. 2b). In both these cases, the aptychi assignment to the conchs of particular ammonite genera was based on their co-occurrences with ammonites. Few in situ aptychi of later dorsoplanitids were found in Svalbard. The Praestriaptychus, which was found in the body chamber of Dorsoplanites sp., shows thin radial striae (Fig. 2m), whereas more typical Praestriaptychus was found in the body chamber of Laugeites lambecki (Ilov.) from the latest Middle Volgian (Fig. 2s). The aptychi, very similar to those from the body chamber of Svalbard Laugeites, were also found together with L. parvus Donovan of the same age in the Kuhn Island (East Greenland) by the CASP expedition (Fig. 2j, k). Very similar isolated aptychi, which could be assigned either to Laugeitinae or to Craspeditinae were found in the Middle–Upper Volgian of the Veselovskaya 5 well (Western Siberia, Fig. 2l) and the Nordvik section (Northern Siberia, Fig. 2h). Isolated Praestriaptychus (Fig. 2q) from the Middle Volgian Nikitini Zone of the Yaroslavl region should be also assigned to Dorsoplanitidae, as other ammonites are unknown from these strata. The latter record possibly belongs to either Epivirgatites, Laugeites or Lomonossovella. This aptychus, as well as a specimen from the body chamber of Dorsoplanites from Svalbard shows not only concentric ribs, but also thin radial striae (they are visible near the transition from the lateral to frontal margin), which became common in some Cretaceous praestriaptychi.
Virgatitidae
Virgatitids are short-lived (latest Kimmeridgian–Middle Volgian) Subboreal ammonites with a narrow geographic distribution (one endemic species is described from Subpolar Urals, while other taxa are restricted to the European part of Russia and Poland). Several relatively narrow praestriaptychi were found together with an early member of this family, the Late Kimmeridgian Sarmatisphinctes (Fig. 2u), however, some uncertainties concerning the aptychi assignment remain as they were found close to—but outside of the body chambers of ammonites. It should be noted, however, that such praestriaptychi were also found in the Autissiodorensis Zone of the Peri-Caspian depression, where ammonite assemblages consist of Sarmatisphinctes and lamellaptychi-bearing oppeliids. Middle Volgian praestriaptychi (P. volgensis Rogov), which are characterized by even more narrow valves, were primarily assigned to either Pavlovia or Zaraiskites (Rogov 2004a). They were collected outside of ammonites, but their comparison with true aptychi of Pavlovia and other dorsoplanitids gave ground to the assumption that they should be ascribed to Zaraiskites. Very similar narrow-valved praestriaptychi, which probably belong to virgatitid ammonites, were also found in the uppermost part of the Lower Volgian (Fig. 3h).
Craspeditidae
Craspeditid aptychi have been discovered only recently in the Upper Volgian of the Middle Volga region (Rogov and Mikhailova 2006). Intensive studies of the Upper Volgian succession in the Moscow region lead to numerous records of aptychi (Praestriaptychus fulgens Mironenko) and upper jaws in Kachpurites (Mironenko 2014). Additional occurrences of aptychi, which belong to Garniericeratinae are also known, providing possibilities to compare evolutionary changes of shell versus aptychi shape. This subfamily consists of the two genera Kachpurites and Garniericeras, which show quick anagenetic evolutionary changes from nearly evolute well-sculptured early Kachpurites to keeled oxyconic Garniericeras (Rogov 2013, 2014b). Evolutionary changes in the shape of praestriaptychi, associated with these ammonites (Fig. 2d–g), generally coincide with this trend, but aptychi evolution seems more gradual (Fig. 4). Some praestriaptychi, collected from the lower part of the Upper Volgian from European Russia could belong to Craspedites (Craspeditinae), but to date only one record of Praestriaptychus (Hryniewicz et al. 2015, Fig. 9D, refigured herein, Fig. 2c) from the upper part of the Upper Volgian Okensis Zone should be ascribed to this genus. Surprisingly, the intensive search for aptychi in the ammonite-rich sites of the earliest Cretaceous age (Ryazanian and Valanginian) did not provide any additional occurrences of craspeditid aptychi, although several ammonoid upper jaws were discovered in the Ryazanian of Northern Siberia
(they will be described elsewhere).
Aspidoceratidae s.l.
Although aspidoceratids are not truly Boreal ammonites and they are typical for Tethyan areas, they sometimes invaded Boreal seas, in some cases reaching the Pechora region and Subpolar Urals. Two subfamilies, included in the Aspidoceratidae (Aspidoceratinae and Peltoceratinae) are characterized by significant differences in their inner whorls (including presence of ‘parabolic nodes’ in aspidoceratins) suggesting that the Aspidoceratidae, as conventionally recognized, is polyphyletic and two subfamilies evolved from different groups of pseudoperisphinctins (Page 2008). Aptychi of Late Jurassic peltoceratins are unknown, but their Callovian ancestors (Binatisphinctes) are associated with Praestriaptychus anglicus (Page 1991; Rogov 2004a, b). The single known record of an aptychus within the body chamber of Peltoceras (Frerichs 2004, Fig. 1) is preserved as an imprint of the inner surface and its identification as Praestriaptychus is only preliminary. Aspidoceratins developed very thick aptychi (Laevaptychus Trauth 1927), which clearly differ from aptychi of other ammonoid groups by their remarkable porous outer surface (Rogov 2004a, b), albeit the imprints of their inner surface could be compared with those of praestriaptychi (Fig. 2r). These aptychi are known from nearly all levels of the Subboreal Callovian and Upper Jurassic, which are characterized by aspidoceratins, i.e. from the Upper Callovian, Upper Oxfordian, Lower and Upper Kimmeridgian and uppermost Lower Volgian (Rogov 2004a, b). However, aptychi of microconchiate aspidoceratins were poorly known and their taxonomy remains controversial. Ziegler (1974) ascribed aptychi of Sutneria apora (Opp.) as Laevilamellaptychus Trauth, 1930, while Schweigert (1998) suggested that aptychi of Sutneria should be considered as small-sized Laevaptychus. Here, we are presenting a first report of aptychi found in situ within the body chamber of the Late Oxfordian aspidoceratid Mirosphinctes [m] (Figs. 2o, p, 3a). Surprisingly these aptychi differ from those of associated macroconchs Euaspidoceras not only by size and shape, but also by their structure. Laevaptychi associated with macroconchs are characterized by a clearly visible porous structure, whereas aptychi of microconchs have a relatively homogenous calcitic layer (Fig. 3b, c) and could be classified within the paragenus Laevilamellaptychus. Published data on laevilamellaptychi microstructure (Farinacci et al. 1976, pl. 7–8) indicates the presence of a tubular structure in this taxon, which was not found in our specimens. It should be noted that the shape of laevilamellaptychi, which co-occurred with Mirosphinctes is identical to those known as an imprint of the inner surface in the body chamber of Epipeltoceras (cf. Enay 1962, pl. IV, Fig. 3). In contrast to Laevaptychus, which are only associated with aspidoceratin macroconchs, Laevilamellaptychus are known in association with clearly separated ammonoid clades, such as Stephanocerina (Aspidoceratidae) and Haplocerina (Haploceratidae, see Trauth 1934). It is worth noting that the laevaptychi, which were found inside the body chambers of two Late Oxfordian Euaspidoceras are significantly smaller than the apertures of these ammonites (in both recorded shells the height of aptychi is approximately 80 % of the height of the aperture), whereas in brevidomic microconchs Mirosphinctes the size of aptychi is nearly equal to the size of the aperture (Fig. 2o).
Simbirskitidae
Aptychi of simbirskitid ammonites have been known since the end of the nineteenth century when Weerth (1884) depicted Aptychus inverselobati (Weerth 1884, pl. VII, Fig. 2), recovered from the body chamber of “Olcostephanus inverselobatus Neum. et Uhl.”, presently considered to belong to the simbirskitid genus Speetoniceras (Rawson 1971). This aptychus was included by Trauth (1937) in the paragenus Praestriaptychus. Additional records of simbirskitid aptychi were reported recently. Engeser and Keupp (2002, Fig. 7) and Frerichs (2004, Figs. 10–12) have described Late Hauterivian Simbirskites from Northern Germany with Praestriaptychus in their body chambers, while some years later Baraboshkin and Shumilkin (2010) described aptychi of Simbirskites from the coeval strata of the Volga area, ascribed to the new species Praestriaptychus simbirskense (Synaptychus after Baraboshkin and Shumilkin 2010, Fig. 2). New in situ aptychi were found in the body chamber of Speetoniceras (Fig. 5). This aptychus could be determined as Praestriaptychus inverselobatus (Weerth). It should be noted that the length of this aptychus slightly exceed the measured whorl height of the ammonite (54.1 and 50.5 mm, respectively), while the width of both valves are ~1 cm narrower compared to whorl breadth.
Desmoceratoidea
Desmoceratidae
Aptychi of Late Cretaceous desmoceratid ammonites are relatively well known (Tanabe 1983) and they consist of a single valve (anaptychus), which, however, shows remains of the symphysis (“intermediate type”, showing transition from anaptychus-type to the aptychus-type, see Tanabe et al. 2015) and possibly it originated not from a true Anaptychus, but from bivalved aptychi. This hypothesis is supported by a recently described aptychus associated with the desmoceratid ammonite Grantziceras from the Lower Albian of Kamtchatka (Cape Hajryuzova, see Palechek et al. 2005). This aptychus is represented by two clearly isolated valves and possibly could be ascribed to as Praestriaptychus, while its original assignment to Synaptychus Basse, 1953 (S.? hairyusovi Baraboshkin in Palechek et al. 2005, pl. 1, Fig. 4) seems to be incorrect.
Hoplitoidea
Hoplitidae
Engeser and Keupp (2002) wrote that hoplitids are characterized by praestriaptychi, but in support of this view the authors cited Trauth (1927, 1930), who used the generic name Hoplites for all Early Cretaceous tuberculated forms, now included in Berriasellidae, Himalayitidae, Neocomitidae, Hoplitidae, Deshayesitidae and Parahoplitidae. Among the aptychi mentioned by Trauth, there are some Early Cretaceous praestriaptychi characterized by the presence of radial striae (P. columbi: Trauth 1937, pl. 11, Fig. 2; P. subtriangularis: Trauth 1937, pl. 11, Figs. 3–4), but they are Neocomian in age and associated with berriasellid and neocomitid ammonites. Similar Berriasian aptychi were recently described in association with berriasellid ammonites from the Western Bermuda Rise (Renz 1979, pl. 1, Figs. 1, 9–10). The only record of an aptychus in association with Albian hoplitids was mentioned by Baraboshkin (in Palechek et al. 2005, p. 89) who compared desmoceratid aptychi with those from the Middle Albian of the Moscow region. As aptychus-bearing beds of this area are characterized exclusively by hoplitid ammonites (Baraboshkin and Mikhailova 1987), the mentioned aptychus very likely belongs to hoplitids, but its true taxonomy remains unclear.
Haploceratoidea
Aconeceratidae
Aptychi, which belong to pre-Barremian Haploceratoidea are so well known, numerous and diverse in pelagic carbonate deposits of the Tethys that the succession of these aptychi (generally called lamellaptychi, which now are subdivided into a few separate genera, see Měchová et al. 2010) are used for zonal subdivision and correlation. In contrast to “Neocomian” deposits, the Barremian is mainly lacking in lamellaptychi: only few records are known from the Upper Barremian of the Eastern Carpathians (Gräf and Turculeţ 1988) and their relation with certain ammonoid groups remains unclear. Although aptychi belonging to Aptian aconeceratids are relatively well known, some uncertainties concerning their systematic position remain. Aptychi of Sinzovia from the Early Aptian of the Volga area, studied in thin sections, showed some calcification of their apical part (Doguzhaeva and Mutvei 1990), which led to ascribing these aptychi to rhynchaptychi (Engeser and Keupp 2002). However, such interpretation contradicts known records of aptychi within or close to the body chambers of aconeceratids (Thomson 1972, Fig. 3; Riccardi et al. 1987, pl.11, Fig. 13; Lehmann 1995), as these aptychi show outlines and sculptures typical for lamellaptychi. Unfortunately, aconeceratid aptychi recorded from the Early Aptian concretions (Fig. 3d, e) of the Volga area generally lack a calcitic layer due to taphonomic loss and their classification is unclear. Aptychi recorded from black shales are commonly preserved with remains of a calcitic layer (Fig. 3j, k), but also cannot be precisely determined due to their small size. However, by analogy with lamellaptychi of Antarctic aconeceratids, which are characterized by a backward rib direction near the symphysis (Thomson 1972, Figs. 2–3) and taking into account new records (Fig. 6), these aptychi could be tentatively referred to as Didayilamellaptychus Turculet, 1994. It should be noted, however, that rib curvature in aptychi of Sinzovia is rather close to the earliest members of this genus (Měchová et al. 2010, Fig. 11A–C) or to some Thorolamellaptychus (Měchová et al. 2010, Fig. 10E), and the systematic position of these aptychi remains unclear. Additional records of aptychi in the body chamber of Sinzovia supports the latter interpretation that calcification of the apex could be partially caused by taphonomic processes as well as by remains of well-calcified embryonic aptychi (Mironenko and Rogov 2015). It should be noted that one of the figured aconeceratid aptychi has healed injuries (Fig. 3d), which strongly resemble abnormalities documented in jaws of modern Nautilus (Kruta and Landman 2008). The same kind of healed injuries is also known in some Late Cretaceous Scaphites (Landman et al. 2010, Fig. 13E).
Ancyloceratoidea
Crioceratitidae
Aptychi of crioceratids were recently figured and briefly described in Hauterivian Aegocrioceras and Crioceratites from Northern Germany by Engeser and Keupp (2002, Figs. 5–6) and Frerichs (2004, Figs. 6–9). All these aptychi are characterized by prominent radial ribs and were ascribed by Engeser and Keupp (2002) to anaptychi. It should be noted, however, that these aptychi differ from typical anaptychi by the presence of remains of the symphysis and should be further considered as a separate genus as well as aptychi of Late Cretaceous desmoceratids (see above). However, this is not the only type of aptychi known in crioceratitids. In the Lower Hauterivian of Kelevudagh Mt (Azerbaijan), early crioceratitids (Criosarasinella and Crioceratites) were associated with Praestriaptychus (Figs. 2t, 3j).
Ancyloceratidae
Ancyloceratid ammonites are characterized by the same types of aptychi, which are known from crioceratitids. Praestriaptychi were mentioned by Wright et al. (1996) as belonging to Ancyloceras and praestriaptychi were found in the body chamber of Proaustraliceras. However, closely related ancyloceratids, such as Australiceras whitehousei, are known to bear striated “anaptychi” resembling those of crioceratitids (Doguzhaeva and Mikhailova 2002, Fig. 1). In addition to these two types of aptychi, the Early Barremian ancyloceratid ammonite Karsteniceras has bivalve aptychi with prominent concentric ribs, which were primarily referred to the “Lamellaptychus-type” (Lukeneder and Tanabe 2002). However, concentric ribs at the outer surface of these aptychi are of a different type than those of true lamellaptychi: they are not tile-like, but rather look like thick growth lines (Lukeneder and Tanabe 2002, Figs. 5–6). Therefore, these aptychi should be assigned to a new type, intermediate between lamellaptychi and praestriaptychi.
Deshayesitoidea
Deshayesitidae
Deshayesitids represent a group of ammonoids with monomorphic shells, which originated from heteromorph heteroceratids (Mikhailova and Baraboshkin 2009). Aptychi recorded from the body chamber of juvenile Deshayesites from the Early Aptian of the Middle Volga area were described and figured by Doguzhaeva et al. (1995, Fig. 1). The shape of this aptychus along with additional records of isolated aptychi, possibly belonging to Deshayesites (Fig. 3g), permits its assignment to Praestriaptychus.