166
Journal of Paleontology 92(2):157–169
can be explained as a result of a chemical reaction in a slightly acid or neutral (as opposed to alkaline) bottom water medium (Fox, 1966) causing melanin (the main ink component providing the black color) to precipitate into a solid phase while still in the coleoid body. In an alkaline environment, melanin would be dispersed colloidally (Fox, 1966). To preserve the ink, the burial environment must have also been anoxic or strongly dysoxic, which is the case for the Bear Gulch Limestone in Montana, the Wewoka Formation in Oklahoma, and the Stark Shale in Nebraska. By contrast, the Illinois occurrence is thought to have been a shallow-water deposit in a delta, however, rapid concretion formation acted as an oxygen shield, which preserved the ink in the coleoids.
Recent knowledge on the early to late Carboniferous shelled coleoids.—The first recognized Carboniferous coleoids— Hematites, Paleoconus, and Bactritimimus—were distinguished by the presence of a well-developed rostrum covering a brevi- conic phragmocone (Flower and Gordon, 1959). An ultra- structural approach for recognition of Carboniferous coleoids was introduced at the end of the twentieth century. This method is based on the evolutionary stability of shell ultrastructure in cephalopods (for more information, see Doguzhaeva, 1994, 1996, 2002a, 2008, 2012; Doguzhaeva et al., 1996, 1999, 2002a, 2006b, 2010a, 2017). Ultrastructural methods were used to help recognize the late Carboniferous coleoid Shimanskya Doguzhaeva, Mapes, and Mutvei, 1999 in which the shell wall, as in extant Spirula Lamarck, 1799 and the Early Cretaceous spirulid Adygeya Dogushaeva, 1996, lacks a nacreous layer (Doguzhaeva et al., 1999). Shimanskya shell-wall type was also identified in several taxa that were earlier described as bactritoids (Mapes, 1979). The taxa ‘Bactrites’ quadrilineatus Mapes, 1979, ‘Ctenobactrites’ lesliensis Mapes, 1979, and ‘Rugobactrites’ jacksboroensis Mapes, 1979 from North America are now considered to be coleoids (Mutvei et al., 2012). Based on shell-wall ultrastructure, ‘Bactrites’ carbonarius Smith, 1903 is referred to Coleoidea as well (Doguzhaeva and Mapes, 2017). Using ultrastructural exam- ination of the concretion matrix in front of conch apertures, the arm hooks were revealed and defined as a coleoid affiliation of Saundersites from the Mazon Creek Lagerstätte in Illinois (Doguzhaeva et al., 2007a) and Gordoniconus from Bear Gulch Bes in Montana (Mapes et al., 2010a). This approach also helped identify the arm hooks, a Saundersites-type radula, and the cartilaginous capsule of an unnamed coleoid from Eudora Shale, Oklahoma preserved without any traces of a mineralized conch (Doguzhaeva et al., 2010b). Therefore, we now know that Carboniferous coleoids
possessed the following innovative structures: (1) a rostrum with a free postalveolar portion (Hematites, Gordoniconus, Saunder- sites), (2) a primordial rostrum (Mutveiconites Doguzhaeva, 2002a), (3) a thin sheath-like rostrum(Donovaniconus, Oklaconus n. gen.), (4) loss of the body chamber (Hematites), (5) a shell wall without nacre (Shimanskya,
‘Bactrites’ quadrilineatus,
B. carbonarius, ‘Ctenobactrites’ lesliensis, ‘Rugobactrites’ jacksboroensis, Oklaconus n. gen.), (6) a proostracum-like structure (Donovaniconus,
Saundersites, Gordoniconus,
Oklaconus n. gen.), (7) an ink sac (Gordoniconus, Saundersites, Donovaniconus, Flowerites Mapes et al., 2010a, Oklaconus n.
gen.), (8) arm hooks (Gordoniconus; Saundersites; unnamed coleoid from Eudora Shale, Oklahoma, Doguzhaeva et al., 2010b), (9) lamellar-fibrillar nacre in the septa (Shimanskya, Donovaniconus), (10) a radula with two marginal plates on each side, which is atypical for nautiloids (Saundersites; unnamed coleoid fromEudora Shale, Oklahoma, Doguzhaeva et al., 2010b), and (11) a muscular mantle on the conch surface (assumed in all; observed in Saundersites and Oklaconus n. gen.). These novelties, together with morphological structures derived from the ancestral bactritoid stock (i.e., a spherical protoconch, a straight phragmo- cone, a small ventral siphuncle, thin nonbiomineralized connecting rings, a long body chamber, a nacreous layer in the shell wall, and columnar nacre in the septa) provide the diverse morphological combinations considered to be high-level taxonomic traits. These diverse combinations of both ancestral and innovative structures show that Carboniferous coleoids possessed high morphological plasticity with a capacity for being altered (Doguzhaeva et al., 2010a). Novelty appeared in Carboniferous coleoids at an early evolutionary stage in one taxon, but the ‘old’ traits existed for a long time after the novelty appeared in other taxa. An example of this phenomenon is the lack of a body chamber in the early Carboniferous Hematites (Doguzhaeva et al., 2002a). Hematites and Gordoniconus are the earliest recorded Carboniferous coleoids (dated 318–333 Ma), however, Gordoniconus has a long body chamber (Mapes et al., 2010b). Many of the younger coleoids, e.g., the late Carboniferous Oklaconus n. gen. and Donovaniconus in the Donovaniconida, and juvenile Mutveiconites in the Aulacocerida, have body chambers (Doguzhaeva, 2002a; Doguzhaeva et al., 2002d, 2003, 2006b; herein). In Hematites, loss of the body chamber did not lead to formation of a proostracum or proostracum-like structure. This illustrates forms at an early stage of coleoid evolution that lacked skeletal protection in the form of a body chamber, yet did not have dorsal support for the body in the shape of a proostracum (Doguzhaeva, 2012). Another character of the Carboniferous stage of coleoid
evolution is the independent appearance of new morphological traits and their further convergent evolution. This is exemplified by rostrum development. The early Carboniferous Hematites has a comparatively massive rostrum with a unique ultrastruc- ture (Flower and Gordon, 1959; Doguzhaeva et al., 2002a), whereas the early to late Carboniferous donovaniconids Gordoniconus, Saundersites, Donovaniconus,and Oklaconus n. gen. have thin sheath-like rostra, and the late Carboniferous aulacocerid Mutveiconites has a primordial rostrum continuing as a sheath-like rostrum along the phragmocone (Doguzhaeva, 2002a; Doguzhaeva et al., 2006b). These observations suggest that the long-term (~60 Myr) Carboniferous evolution of coleoid cephalopods included many experimental attempts before a comparatively stable coleoid model, similar to that of modern gladius-bearing taxa, appeared in the Early Triassic (Olenekian) (Brayard et al., 2017). Kröger et al. (2011), in our opinion, erroneously suggested that the orders Hematitida and Donova- niconida could represent the evolutionary lineage that gave rise to Middle–Late Triassic phragmoteuthids and Permian–Cretac- eous belemnitids. Fuchs et al. (2013, fig. 12) also erroneously assumed that the Carboniferous Donovaniconida and the Middle Triassic–Early Jurassic Phragmoteuthida gave rise to all of the Mesozoic coleoids. It is worth noting in this context
Page 1 |
Page 2 |
Page 3 |
Page 4 |
Page 5 |
Page 6 |
Page 7 |
Page 8 |
Page 9 |
Page 10 |
Page 11 |
Page 12 |
Page 13 |
Page 14 |
Page 15 |
Page 16 |
Page 17 |
Page 18 |
Page 19 |
Page 20 |
Page 21 |
Page 22 |
Page 23 |
Page 24 |
Page 25 |
Page 26 |
Page 27 |
Page 28 |
Page 29 |
Page 30 |
Page 31 |
Page 32 |
Page 33 |
Page 34 |
Page 35 |
Page 36 |
Page 37 |
Page 38 |
Page 39 |
Page 40 |
Page 41 |
Page 42 |
Page 43 |
Page 44 |
Page 45 |
Page 46 |
Page 47 |
Page 48 |
Page 49 |
Page 50 |
Page 51 |
Page 52 |
Page 53 |
Page 54 |
Page 55 |
Page 56 |
Page 57 |
Page 58 |
Page 59 |
Page 60 |
Page 61 |
Page 62 |
Page 63 |
Page 64 |
Page 65 |
Page 66 |
Page 67 |
Page 68 |
Page 69 |
Page 70 |
Page 71 |
Page 72 |
Page 73 |
Page 74 |
Page 75 |
Page 76 |
Page 77 |
Page 78 |
Page 79 |
Page 80 |
Page 81 |
Page 82 |
Page 83 |
Page 84 |
Page 85 |
Page 86 |
Page 87 |
Page 88 |
Page 89 |
Page 90 |
Page 91 |
Page 92 |
Page 93 |
Page 94 |
Page 95 |
Page 96 |
Page 97 |
Page 98 |
Page 99 |
Page 100 |
Page 101 |
Page 102 |
Page 103 |
Page 104 |
Page 105 |
Page 106 |
Page 107 |
Page 108 |
Page 109 |
Page 110 |
Page 111 |
Page 112 |
Page 113 |
Page 114 |
Page 115 |
Page 116 |
Page 117 |
Page 118 |
Page 119 |
Page 120 |
Page 121 |
Page 122 |
Page 123 |
Page 124 |
Page 125 |
Page 126 |
Page 127 |
Page 128 |
Page 129 |
Page 130 |
Page 131 |
Page 132 |
Page 133 |
Page 134 |
Page 135 |
Page 136 |
Page 137 |
Page 138 |
Page 139 |
Page 140 |
Page 141 |
Page 142 |
Page 143 |
Page 144 |
Page 145 |
Page 146 |
Page 147 |
Page 148 |
Page 149 |
Page 150 |
Page 151 |
Page 152 |
Page 153 |
Page 154 |
Page 155 |
Page 156 |
Page 157 |
Page 158 |
Page 159 |
Page 160 |
Page 161 |
Page 162 |
Page 163 |
Page 164 |
Page 165 |
Page 166 |
Page 167 |
Page 168 |
Page 169 |
Page 170 |
Page 171 |
Page 172 |
Page 173 |
Page 174 |
Page 175 |
Page 176 |
Page 177 |
Page 178 |
Page 179 |
Page 180 |
Page 181 |
Page 182 |
Page 183 |
Page 184 |
Page 185 |
Page 186 |
Page 187 |
Page 188 |
Page 189 |
Page 190 |
Page 191 |
Page 192 |
Page 193 |
Page 194 |
Page 195 |
Page 196 |
Page 197 |
Page 198 |
Page 199 |
Page 200 |
Page 201 |
Page 202 |
Page 203 |
Page 204