A New Species of Mucronalia (Gastropoda: Eulimidae) Parasitizing the Ophiocomid Brittle Star Ophiomastix Mixta in Japan

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A New Species of Mucronalia (Gastropoda: Eulimidae) Parasitizing the Ophiocomid Brittle Star Ophiomastix Mixta in Japan DOI: http://doi.org/10.18941/venus.77.1-4_45 Short Notes ©The Malacological Society of Japan45 Short Notes A New Species of Mucronalia (Gastropoda: Eulimidae) Parasitizing the Ophiocomid Brittle Star Ophiomastix mixta in Japan Tsuyoshi Takano1,2*, Hayate Tanaka3,4 and Yasunori Kano2 1Meguro Parasitological Museum, 4-1-1 Shimomeguro, Meguro, Tokyo 153-0064, Japan; *[email protected] 2Atmosphere and Ocean Research Institute, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8564, Japan 3Graduate School of Science, The University of Tokyo, 7-3-1, Hongo, Bunkyo, Tokyo 113-0033, Japan 4National Museum of Nature and Science, 4-1-1 Amakubo, Tsukuba, Ibaraki 305-0005, Japan Gastropods of the family Eulimidae Over 30 species have been described in this genus, (Caenogastropoda: Vanikoroidea) are parasites of largely based on the presence of a mucronate apex or echinoderms including all five classes of the a calloused inner lip (e.g., Pease, 1860; Habe, 1974). phylum, namely Asteroidea, Crinoidea, Echinoidea, However, Warén (1980a) has transferred more Holothuroidea and Ophiuroidea (Warén, 1984). than half of them to other eulimid genera such as The Eulimidae contain numerous extant and extinct Echineulima Lützen & Nielsen, 1975, Hypermastus species (Bouchet et al., 2002; Lozouet, 2014), but Pilsbry, 1899 and Melanella Bowdich, 1822 or to many remain to be described (Warén, 1984). This the cerithioid family Pelycidiidae (see Ponder & has led to a number of recent publications on eulimid Hall, 1983: fig. 1C; Takano & Kano, 2014). Some systematics that aim at a better understanding of ten described species remain in Mucronalia, all their ecological, morphological and species diversity of which bear the mucronate apex, parietal callus (e.g., Matsuda et al., 2010, 2013; Dgebuadze et and curved outer lip of the shell (Warén, 1980a). al., 2012; Souza & Pimenta, 2014; Nekhaev, 2016; The spiral bands may be present or absent, with Takano et al., 2017). Mucronalia lepida Melvill, 1906 and Mucronalia Mucronalia A. Adams, 1860 is a poorly oxytenes Melvill, 1904 as examples of colorless known genus of the Eulimidae inhabiting shallow species. Shell color and color pattern are consistent subtidal to bathyal waters in temperate to tropical within each eulimid species, whereas variation exists regions worldwide. The type species of the genus, among congeneric species (Warén, 1984). The genus Mucronalia bicincta A. Adams, 1860, has been Eulima Risso, 1826, for example, includes species collected only as empty shells from 40–150 m with and without spiral bands (Bouchet & Warén, depths along the coasts of Honshu and Kyushu 1986). Islands, Japan (A. Adams, 1860; Hori & Matsuda, Among the species of Mucronalia sensu Warén 2017), and thus no ecological, anatomical or genetic (1980a), host information is available for only two information is available for the species (Warén, species (Warén, 1980a; Hori & Matsuda, 2017). 1980a). The shell of M. bicincta is characterized by Both are ectoparasites of brittle stars: Mucronalia (1) a cylindrical outline, (2) a height of up to 9 mm, exilis A. Adams, 1862 on Amphioplus laevis (Lyman, (3) a “mucronate” apex with a projecting protoconch 1874) in the Amphiuridae and Ophioplocus sp. in and a nearly planispiral first whorl of the teleoconch, the Hemieuryalidae; Mucronalia trilineata Warén, (4) brownish spiral bands on the teleoconch whorls, 1980 on Ophiarachnella septemspinosa (Müller (5) an aperture with a parietal callus, and (6) a & Troschel, 1842) in the Ophiodermatidae. Warén strongly curved outer lip with its most protruding (1980a, 1984) has hence speculated that all their part at 2/3 of aperture height from the suture (Warén, congeners depend on Ophiuroidea, conforming 1980a, 1984; Hori & Matsuda, 2017: pl. 103, fig. 5). to the general rule that eulimids in a single genus http://zoobank.org/urn:lsid:zoobank.org:pub:121AB97A-BDCE-498F-B010-EB3844323078 46 VENUS 77 (1–4), 2019 or a terminal clade parasitize hosts of the same Systematics echinoderm class. We herein describe a new species of Mucronalia Family Eulimidae Philippi, 1853 from the ophiocomid brittle star Ophiomastix Genus Mucronalia A. Adams, 1860 mixta Lütken, 1869, collected shallow subtidally Type species: Mucronalia bicincta A. Adams, in Manazuru, Kanagawa, Japan. Type specimens 1860, by monotypy. and their hosts have been deposited in the National Museum of Nature and Science, Tokyo (NSMT) and Mucronalia alba n. sp. Meguro Parasitological Museum (MPM). (Figs 1–7) Figs 1–5. Mucronalia alba n. sp. and its host Ophiomastix mixta. 1. Oral view of O. mixta (Om1), showing attachment site of holotype (arrowhead) and egg masses (em). Live-taken photograph in bottom left box. 2. Paratype 2 on arm of another host (Om2) with egg masses. Arrowhead denotes attachment site of Paratype 1. 3. Shell of holotype, apertural and lateral views. Arrowheads indicate growth pause scars. 4. Close-up view of protoconch and first teleoconch whorl of holotype (arrowhead for boundary). 5. Shell of Paratype 1, apertural view. Short Notes 47 Type locality: Kotogahama, Manazuru, Kanagawa, columellar lip straight, thick, tilted at 20° from Honshu Island, Japan (35°08′54″N, 139°08′57″E). coiling axis of body whorl in holotype; parietal Type material: Holotype NSMT-Mo 79008 and callus thin but present, colorless; basal lip round two paratypes MPM Coll. No. 21461, all collected and inflated (Fig. 3). Umbilicus absent. Protoconch from the type locality on 1 August 2015, found of slightly more than 2 whorls, pupiform, glassy, attached to the ventral side of the arms of translucent with brownish tinge, tilted at 10° from Ophiomastix mixta living under stones at depths of teleoconch axis; exposed part 210 μm wide and 250 1–2 m (Figs 1, 2). The two paratypes were found on μm high (Figs 4, 6). Operculum thin, yellowish. the same arm of another host (Table 1). Eyes black; reddish-purple contents of esophagus Etymology: The name refers to the translucent visible through shell (Fig. 3, apertural view). white shell without color bands. Holotype and Paratype 2 accompanied by several Diagnosis: Shell slender for genus, conical, egg masses of < 1 mm diameter (Figs 1, 2). Each translucent white with no spiral bands. Teleoconch mass contained eggs or trochophores or veligers at whorls asymmetrically convex, irregularly increasing same stage of development. in diameter. Growth pause scars distinct, irregularly Distribution: In addition to the type locality, this spaced, slightly brownish. Aperture oblong-ovate; species has been collected from Misaki, Kanagawa columellar lip straight, tilted at 20° from coiling axis (35°10′N, 139°37′E) and Tateyama, Chiba (35°00′N, of body whorl. 139°50′E), all on the Pacific coast of central Honshu. Description: Shell conical with mucronate apex, The specimens from the latter two localities were up to 5.5 mm high, thin but not fragile, translucent identified by the authors from photographs provided white. Teleoconch of up to 6.6 asymmetrically by M. Okanishi and S. Tsuzuki (pers. comm.). convex whorls, irregularly increasing in diameter; Remarks: The generic position of the present growth pause scars distinct, somewhat brownish, new species is readily determined by its mucronate situated at 3.6, 5.6 and 6.3 whorls in holotype (Fig. apex, the parietal callus and the curved outer lip of 3), each accompanied by slight change of coiling the aperture. Furthermore, the ectoparasitic mode axis (Fig. 7); growth lines numerous and faint. of life on ophiuroids (Figs 1, 2) conforms to the Aperture oblong-ovate; outer lip simple, curved, concept of Mucronalia as interpreted by Warén with most protruding part at half of aperture height; (1980a, 1984). Ophioarachnicola biformis Warén, 1980, the monotypic species of the genus, also parasitizes ophiuroids and shows some resemblance to certain Mucronalia in shell form (Warén, 1980b: 287, figs 24, 25), but its straight apical slopes suggest a distant relationship. Mucronalia alba n. sp. differs from all congeners, including the type species M. bicincta, in having a colorless, conical shell with asymmetrically convex whorls. Its shell profile resembles those of M. exilis (another species of the genus from temperate waters Figs 6, 7. Line drawings of M. alba n. sp. 6. Apex of in Japan) and M. trilineata (Queensland, Australia), holotype from same angle with Fig. 4, showing boundary between protoconch and teleoconch but the latter two species are characterized by the (arrowhead). 7. Growth pause scar at 3.3 whorls of presence of brownish spiral bands on the teleoconch teleoconch in Paratype 1 (arrowhead). whorls. The shape of the aperture is also different, Table 1. Shell measurements of three specimens of Mucronalia alba n. sp. Shell Shell Number of Specimen Voucher Host Preservation height width teleoconch whorls Holotype NSMT-Mo 79008 Om1 5.5 mm 2.0 mm 6.6 Dry Paratype 1 MPM Coll. No. 21461 Om2 3.1 mm 1.4 mm 4.5 Pure ethanol Paratype 2 MPM Coll. No. 21461 Om2 c. 4 mm* 1.7 mm > 5* Pure ethanol *Specimen preserved in situ on host and exact measurements unavailable (see Fig. 2). 48 VENUS 77 (1–4), 2019 with the columellar lip tilted 20° in M. alba or almost (1944), a preliminary molecular phylogeny of perpendicular in M. exilis and M. trilineata (Warén, the family shows its position within the hyper- 1980a; Hori & Matsuda, 2017). The three species diverse, holothuroid-parasitic genus Melanella (T. further differ in their habitat and host characteristics. Takano, unpublished data). Its shell morphology also The new species attaches by the proboscis to the arm warrants the reallocation of “Mucronalia lactea” to of Ophiomastix mixta on a subtidal rocky bottom. the latter genus (see e.g., Hori & Matsuda, 2017: Mucronalia exilis parasitizes Amphioplus laevis and pl. 99 for similar shells). The species name lactea, Ophioplocus sp. on soft bottoms at depths of 10 to however, seems to be preoccupied in Melanella 50 m (Hori & Matsuda, 2017).
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