Literature DB >> 34992490

First record of the genus Discorhabdella (Porifera, Demospongiae, Poecilosclerida, Crambeidae) from Sagami Bay, Japan with description of two new species.

Yuji Ise1, Jean Vacelet2, Takato Izumi3, Sau Pinn Woo1, Shau Hwai Tan1.   

Abstract

Two new species of Discorhabdella are described from Sagami Bay, Japan. Discorhabdella has been suggested to have an ancient Tethyan origin according to discovery of their unique pseudoastrose acanthostyles from late Eocene to Oligocene deposits. This is the first record of the genus from the northwest Pacific and first record of the family Crambeidae from Japan. Discorhabdellahispida sp. nov. is distinctive within the genus by possession of special sigmoid microscleres and C-shaped isochelae with short alae. Discorhabdellamisakiensis sp. nov. is characterized by short choanosomal subtylostyles, and their length overlapped with that of the ectosomal subtylostyles. Only one other species, Discorhabdellatuberosocapitata (Topsent, 1890), has the same spicule composition. However, all spicule types are larger in D.tuberosocapitata than those of D.misakiensis sp. nov., and the shape of the isochelae is different: the alae are more widely opened in D.tuberosocapitata. An identification key to species of the genus Discorhabdella is also provided. The discovery of two new species from warm temperate northwest Pacific extends the geographical distribution of the genus Discorhabdella. Yuji Ise, Jean Vacelet, Takato Izumi, Sau Pinn Woo, Shau Hwai Tan.

Entities:  

Keywords:  Central Kuroshio Current; Tethys Sea; biodiversity; northwest Pacific; relict species; sponge taxonomy

Year:  2021        PMID: 34992490      PMCID: PMC8677707          DOI: 10.3897/zookeys.1076.37278

Source DB:  PubMed          Journal:  Zookeys        ISSN: 1313-2970            Impact factor:   1.546


Introduction

Sponges of the genus Dendy, 1924 are characterized by the possession of smooth ectosomal subtylostyles, long choanosomal styles/subtylostyles with swollen lumpy bases, and tuberculate club-shaped pseudoastrose or heavily spined acanthostyles that form an erect hymedesmioid skeleton and various cheloid microscleres (Maldonado et al. 2001, Van Soest 2002). It has been suggested that originated in the Tethys Sea (Boury-Esnault et al. 1992, Maldonado and Uriz 1996, Maldonado et al. 2001), as their unique pseudoastrose acanthostyles were discovered from the late Eocene to Oligocene deposits in New Zealand (Hinde and Holmes 1892, Łukowiak 2015, 2016). Seven extant species are currently known from the genus (Van Soest et al. 2019). Of these, Dendy, 1924 is reported only from its type locality Three King’s Islands, New Zealand. Maldonado, Carmona, Van Soest & Pomponi, 2001 and Maldonado, Carmona, Van Soest & Pomponi, 2001 are reported from off the Pacific coast of Panama. is also reported from Gulf of California (Aguilar-Camacho and Carballo 2012). Boury-Esnault, Pansini & Uriz, 1992 is reported from the Alboran Sea, and (Topsent, 1890) is reported from Azores, Canaries and Madeira (Van Soest 2002, Van Soest et al. 2019). Two recently described species have been discovered from north of Madagascar ( Vacelet & Cárdenas, 2018) and Gulf of Mexico ( Díaz & Pomponi, 2018). A recent faunal survey of benthic animals in Sagami Bay, Japan yielded several undescribed species of the family (Ise 2017), and the descriptions of two new species of are provided herein.

Materials and methods

The sponges described in the present study were collected by dredging from the R/V - of Misaki Marine Biological Station, the University of Tokyo. The sampling was carried out at the northeastern part of Sagami Bay during the period of 10–13 January 2012 (Fig. 1). The specimens were kept alive in seawater for several hours and directly preserved in 90% ethanol afterwards. Dry fragments of the sponge were digested using hydrogen peroxide in order to obtain clean spicules. They were then cleaned using distilled water, centrifuged, and resuspended three times. Cleaned spicules were then placed on glass slides, dried, embedded in mounting medium Eukitt® (O. Kindler), cover-slipped, and then observed under a light microscope. Spicules were also placed on copper stub, coated with 400Å platinum, and observed by scanning electron microscope (JEOL JSM-6380LV). Spicules were measured with calibrated ocular micrometer directly under a microscope. Measurements were carried out along randomly chosen transects across the slide, ignoring unfocused, broken, or malformed spicules. Measurements of choanosomal subtylostyles of sp. nov. were only taken from the width of base and shaft as they are usually broken during spicule preparation steps. About 30 spicules for each type of spicule were measured. Spicule sizes are given as a range, followed by the mean in parenthesis. Spicule and morphological nomenclature follows Boury-Esnault and Rützler (1997), and terminology of cheloid microscleres follows Hajdu et al. (1994). Terminology for geographical distribution of each species basically follows descriptions of the original references; however, the data are corrected in Table 1 according to Marine Ecoregions of the World (Spalding et al. 2007). Specimens were deposited in National Museum of Nature and Science, Tsukuba, Japan (NSMT).
Figure 1.

Location of sampling site. Open star indicates Sagami Bay.

Table 1.

Morphological comparison of spicules and geographical distribution of extant species. Locality is described as ecoregions and province following Spalding et al. (2007). Spicule sizes are given as the range, followed by the mean in parenthesis. All spicule measurements in µm.

Species Locality Depth (m) Ectosomal subtylostyle Choanosomal style/subtylostyle Pseudoastrose acanthostyle or acanthostyle Isochelae Sigma spined microxea Other microsclere Reference
length × width length × width length × base width length, number of alae length × width length × width length
D.hindei Boury-Esnault et al., 1992 Alboran Sea, Mediterranean Sea534–604276–445 (367) × 5.2855–1556 (1086) × 34–52 (43)43–57 (48) × 36–39 (38.5)22–27 (23), 8 alae11–16 (12) × 1–1.3 (1.3)nonenone Boury-Esnault et al. 1992
D.incrustans Dendy, 1924Three King‘s North Cape, Northern New Zealand180357–592 (496.8) × 10–15 (12.6)900–1700 × 28–61 (43.1)36–53 (45.4) × 32–43 (37.2)33–51 (44), up to 7 alaenone26–34 (31.4)none Van Soest 2002
D.littoralis Maldonado et al., 2001 Nicoya, Tropical East Pacific10–30130–180 × 2.5–4117–300 × 5–1026–40 × 10–18.5none13–15 × 1nonenone Maldonado et al. 2001
D.pseudaster Vacelet & Cárdenas, 2018Western and Northern Madagascar, Western Indian Ocean346–349240–370, 9–10more than 600 × 40–5635–45 × 35–4512–15, 4–5 alaenonenonepseudoaster, 12.5–18 in diameter Vacelet and Cárdenas 2018
D.ruetzleri Díaz & Pomponi, 2018Floridian, Tropical Northwestern Atlantic60–80260–340 (300) × 3–7.55 (4)470–810 (598) × 5–13 (10.5)17–40 (29.6) × 7.5–20 (15)20–25, unknown12–1815–18none Díaz and Pomponi 2018
D.tuberosocapitata (Topsent, 1890)Azores Canaries Madeira, Lusitanian550–736330c.a. 650 × c.a. 28c.a. 13025, 4–8 alaenonenonenoneBoury-Esnault et al. 1992, Van Soest 2002
D.urizae Maldonado et al., 2001 Nicoya, Tropical East Pacific55–73180–220 × 5–7380–750 × 19–4223–37 × 15–2626–29, 5 alae13–16 × 119–26 × 2–3none Maldonado et al. 2001
Cortezian, Warm Temperate Northeast Pacific344175–220 (197.5) × 2.5–7.5 (4.75)220–610 (423.3) × 17.5–35 (25.8)30–42.5 (36.6) × 23–3735–42 (36.6), 3 alae15–20 (17.1)15–22.5 (21.6)none Aguilar-Camacho and Carballo 2012
D.hispida sp. nov. Central Kuroshio Current, Warm Temperate Northwest Pacific113–223292.2–392.5 (335.4) × 13.4–16.7 (15.2)814–1500 × 42.0–56.5 (50.3)84–127.5 (103.6) × 41.1–57.7 (48.0)27.3–38 (31.7), 3–7 alaenonenonesigmoid microsclere 20.7–31.2 (26.3)this study
D.misakiensis sp. nov. Central Kuroshio Current, Warm Temperate Northwest Pacific255–318203–257 (232) × 10.6–14.1 (11.7)252.0–336.4 (295.2) × 18.6–26.6 (22.6)73.0–91.3 (82.0) × 27.9–42.0 (34.2)17.5–21.9 (19.8), 6 alaenonenonenonethis study
Morphological comparison of spicules and geographical distribution of extant species. Locality is described as ecoregions and province following Spalding et al. (2007). Spicule sizes are given as the range, followed by the mean in parenthesis. All spicule measurements in µm. Location of sampling site. Open star indicates Sagami Bay.

Results

Phylum Grant, 1836

Class Order Family

Dendy, 1924 6ADC38FB-8B60-50CB-968A-E5EF3049DFAF

Diagnosis.

Smooth ectosomal subtylostyles, long choanosomal styles/subtylostyles with swollen lumpy bases and tuberculate club-shaped pseudoastrose or heavily spined acanthostyles forming erect hymedesmioid skeleton; microscleres anchorate unguiferous isochelae and may include spined microxea with two lumpy swellings or sigma-like spicules (slightly modified from Van Soest 2002).

Type species.

Dendy, 1924: 376 (by monotypy).

sp. nov.

78C4541D-E956-51EC-8FD0-8E31E59E6FDE http://zoobank.org/025E3E24-8A78-4AD1-9BD6-44FD92B55A35 Figs 2A–C , 3 , 4
Figure 2.

A–C External view of sp. nov., holotype (NSMT-Po-2489). A Alive B in ethanol preserved C magnified view of surface of preserved specimen. Note a number of choanosomal subtylostyles vertically protruding with their tips outward D external view of sp. nov., holotype (NSMT-Po-2490) in ethanol preserved state. Note most part of the sponge was already used for spicule preparation. Scale bars: 5 mm (A, B); 500 µm (C); 3 mm (D).

Figure 3.

Spicules of sp. nov., holotype (NSMT-Po-2489). A Choanosomal subtylostyle B magnified view of base of subtylostyle C–E ectosomal subtylostyle D tyle E tip F magnified view of tip. Note the surface is microspined. Scale bars: 300 µm (A); 50 µm (B); 10 µm (D, E); 5 µm (F).

Figure 4.

Spicules of sp. nov., holotype (NSMT-Po-2489). A Acanthostyles B isochelae C magnified view of one extremity of isochelae. a, alae D sigmoid microscleres. Scale bars: 20 µm (A); 10 µm (B, D); 2 µm (C).

Material examined.

NSMT-Po-2489. Off Misaki, eastern part of Sagami Bay (Fig. 1), Japan ( to ), 223–113 m depth, dredge, 13 January 2012.

Description of holotype.

Thinly encrusting, surface hispid due to protruding choanosomal large subtylostyles. Color greenish ochre in life, grayish white in ethanol. Size, 22 × 17 mm, about 0.3 mm thick (Fig. 2A–C). Oscules not observed in the living specimen; probably contracted in preserved state. Ostia observed only in preserved specimen, rounded, evenly distributed, 150–300 µm in diameter. A–C External view of sp. nov., holotype (NSMT-Po-2489). A Alive B in ethanol preserved C magnified view of surface of preserved specimen. Note a number of choanosomal subtylostyles vertically protruding with their tips outward D external view of sp. nov., holotype (NSMT-Po-2490) in ethanol preserved state. Note most part of the sponge was already used for spicule preparation. Scale bars: 5 mm (A, B); 500 µm (C); 3 mm (D). Hymedesmioid skeleton made by large choanosomal subtylostyles making the sponge surface hispid and by perpendicular acanthostyles with their bases attached on substrate. Ectosomal subtylostyles arranged perpendicular to surface with tips outward. Anchorate unguiferous isochelae and sigmoid microscleres roughly dispersed throughout the sponge. Choanosomal subtylotyles (Fig. 3A, B), long slightly curved near the base, maximum diameter at the base gradually tapering to sharp point (Fig. 3A). Base smooth and slightly lumpy (Fig. 3B). Size, 814–1500 µm in length, 42.0–56.5 (50.3) µm in shaft width, 52.4–70.8 (61.7) µm in base width. Spicules of sp. nov., holotype (NSMT-Po-2489). A Choanosomal subtylostyle B magnified view of base of subtylostyle C–E ectosomal subtylostyle D tyle E tip F magnified view of tip. Note the surface is microspined. Scale bars: 300 µm (A); 50 µm (B); 10 µm (D, E); 5 µm (F). Ectosomal subtylostyles (Fig. 3C–F), fusiform, smooth and straight; with smooth and slightly swollen base (Fig. 3D). Maximum diameter at middle region, then gradually tapering to a sharp point (Fig. 3E). Microspined sparsely around the shaft and densely around the tip (Fig. 3F). Size, 292.2–392.5 (335.4) µm in length, 13.4–16.7 (15.2) µm in shaft width, 10.7–14.0 (12.9) in tyle width. Acanthostyles (Fig. 4A), club-shaped head with conical spines having blunt ends. Shaft straight, fusiform, and densely covered with prominent spines with tips sharply pointed, devoid of spines on the last 10–20 µm towards extremity. Terminal holes or orifices of spines especially around head could be detected. Size, 84.0–127.5 (103.6) µm in length, 41.1–57.7 (48.0) µm in head width including spines, 26.3–42.4 (31.1) µm in head width without spines, 24–35.9 (27.8) µm in width of shaft including spine, 16.2–27.5 (21.3) µm in width of shaft without spine. Anchorate unguiferous isochelae (Fig. 4B, C), strongly curved C-shaped shaft with lateral expansion that forming a pair of fimbriae along its entire length. Both extremities bearing 3–7 short and unequal shaped alae. The alae closest to the lateral fimbriae sometimes reduced or nearly absent, and connected to the fimbriae. Size, 27.3–38.0 (31.7) µm in length, 2.9–4.0 (3.5) µm in shaft width. Spicules of sp. nov., holotype (NSMT-Po-2489). A Acanthostyles B isochelae C magnified view of one extremity of isochelae. a, alae D sigmoid microscleres. Scale bars: 20 µm (A); 10 µm (B, D); 2 µm (C). Sigmoid microscleres (Fig. 4D), strongly curved shaft and irregular in shape. Size, 20.7–31.2 (26.3) µm in length, 0.7–1.0 (0.8) µm in shaft width.

Distribution.

Known only from type locality, Misaki, eastern part of Sagami Bay, Japan.

Etymology.

Specific epithet refers to its hispid surface appearance.

Remarks.

The present species appears well characterized by its spicule complement, especially its microscleres. The isochelae have a unique shape, with a strongly curved shaft compared to all other species of , which have a straight or feebly curved shaft. However, the isochelae of sp. nov. are similar to the anchorate isochelae of (Dendy, 1922) (see also Lévi 1961, Vacelet et al. 1976). The presence of a sigmoid microsclere that is different from the true sigma, is also distinctive. Sigmas are present in four other species: ; ; and ; however, in these species, there are several differences in the other spicule characters (see Table 1). sp. nov. differs from by having acanthostyle (length: 84.0–127.5 µm) instead of pseudoastrose acanthostyles (length: 43–57 µm) in , a less tuberculated base of the choanosomal styles and a less developed tyle of the ectosomal subtylostyles. It differs from by larger choanosomal subtylostyles (814–ca 1500 µm vs 117–300 µm), by having acanthostyles instead of pseudoastrose acanthostyles, and a more tuberculated base of choanosomal subtylostyles. It differs from by larger choanosomal subtylostyles (814–1500 µm vs 470–810 µm), larger acanthostyles (84.0–127.5 µm vs 17–40 µm), larger isochelae (27.3–38.0 µm vs 20–25 µm), absence of spined microxea. It differs from by larger choanosomal subtylostyles (814–1500 µm vs 220–750 µm in length), absence of spined microxeas and a less tuberculated base of the choanosomal styles. Acanthostyles that are more than 90 µm long have been observed only in and in sp. nov. described in this study. But both species lack sigmoid microscleres and have choanosomal subtylostyles with a well-developed lumpy base. Tubercles around the base of choanosomal subtylostyles are not well developed in sp. nov. and can be comparable with those recently found in and . However, sp. nov. totally lacks peculiar pseudoaster of and also lacks spined microxea of . EEB6EE11-92D1-5A09-9704-DFCF290CD8C2 http://zoobank.org/636E3E9C-BF02-45D5-8CEE-222468D4C945 Figs 2D , 5 , 6
Figure 5.

Spicules of sp. nov., holotype (NSMT-Po-2490). A–C Choanosomal subtylostyle B magnified view of base of subtylostyle with prominent lumpy projections C tip D–F ectosomal subtylostyle E tyle F tip. Scale bars: 50 µm (A, D); 20 µm (B, C); 10 µm (E, F).

Figure 6.

Spicules of sp. nov., holotype (NSMT-Po-2490). A Acanthostyles B comaparative view of acanthostyle and isochelae C isochelae D back side view of broken isochelae. a, alae. Scale bars: 20 µm (A, B); 5 µm (C); 2 µm (D).

NSMT-Po-2490. Off Misaki, eastern part of Sagami Bay (Fig. 1), Japan ( to ), 318–255 m depth, dredge, 10 January 2012. Small, very thinly encrusting sponge, about 0.2 mm thick, with velvet surface, white in alcohol. Size, 8 × 5 mm (Fig. 2D). Ostia and oscules not observed either in live or in the preserved specimen. Hymedesmioid skeleton made by choanosomal subtylostyles and acanthostyles. Choanosomal subtylostyles mostly arranged perpendicular to surface with tips oriented upward. Anchorate unguiferous isochelae distributed in whole body. Choanosomal subtylostyles (Fig. 5A–C), straight, almost uniform in thickness along shaft gradually tapering to a sharp point (Fig. 5C). Lumpy base bearing many prominent smooth projections (Fig. 5B). Size, 252– 336.4 (295.2) µm in length, 18.6– 26.6 (22.6) µm in shaft width, 33.2–45.6 (40.2) µm in base width. Spicules of sp. nov., holotype (NSMT-Po-2490). A–C Choanosomal subtylostyle B magnified view of base of subtylostyle with prominent lumpy projections C tip D–F ectosomal subtylostyle E tyle F tip. Scale bars: 50 µm (A, D); 20 µm (B, C); 10 µm (E, F). Ectosomal subtylostyles (Fig. 5D–F), fusiform, smooth and straight, with smooth and slightly swollen tyle (Fig. 5E). Maximum diameter at middle region, then gradually tapering to sharp point (Fig. 5F). Size, 203–257 (232) µm in length, 10.6–14.1 (11.7) µm in shaft width, 7.9–9.9 (8.9) µm in tyle width. Acanthostyles (Fig. 6A, B), straight, surface covered with prominent spines especially at club-shaped head with longer spines. Spines on shaft slightly recurved with tips sharply pointed. Shaft devoid of spines from extremity up to ca. 10–20 µm. Size, 73–91.3 (82.0) µm in length, 27.9–42.0 (34.2) µm in head width including spines, 15.6–21.8 (19.8) µm in head width without spines. Spicules of sp. nov., holotype (NSMT-Po-2490). A Acanthostyles B comaparative view of acanthostyle and isochelae C isochelae D back side view of broken isochelae. a, alae. Scale bars: 20 µm (A, B); 5 µm (C); 2 µm (D). Anchorate unguiferous isochelae (Fig. 6B–D), shaft nearly straight, with a pair of fimbriae along whole shaft; bearing 6 alae (Fig. 6B–D). Size, 17.5–21.9 (19.8) µm in total length, 2.0–2.7 (2.2) µm in shaft width, 6.7–8.0 (7.3) µm in alae length. Known only from type locality, Misaki, eastern part of Sagami Bay, Japan. Specific epithet refers to type locality: Misaki. sp. nov. has only isochelae as microscleres. This composition of spicules can be found in one other species of the genus, from Azores, Canaries and Madeira (Van Soest 2002, Van Soest et al. 2019). The two species can be clearly differentiated by the size of their spicules: all spicules are smaller in sp. nov. (see Table 1). In addition, they can be differentiated by the shape of their isochelae. Although the isochelae of and sp. nov. have similar number of alae, the alae in are more widely opened. The reported number of isochelae alae in is rather confusing because different authors reported different number of alae despite all of them observing the same type material: four in Boury-Esnault et al. (1992), four to five in Van Soest (2002) and seven to eight in Maldonado and Uriz (1996). This is possibly due to differences in the interpretation of the fused alae. Boury-Esnault et al. (1992) and Van Soest (2002) considered the two alae fused at the base as one, while Maldonado and Uriz (1996) counted them as two. The alae number of sp. nov. is here counted as six; however, the two frontal alae seem to fuse at the base or might be regarded as one ala divided into two (Fig. 6D). Further evidence of separation of these two species is their distant geographical distribution: is reported from Azores, Canaries and Madeira (Van Soest 2002, Van Soest et al. 2019) but sp. nov. is found only from the type locality, Sagami Bay, Japan. The dichotomous central ala is also found from “eight-toothed isochelae” of (Maldonado and Uriz 1996); however, sp. nov. and are clearly separated by the possession of sigma in the latter species. Furthermore, has been reported only from Alboran Sea (Maldonado and Uriz 1996), which is very distant from type locality of sp. nov. The choanosomal subtylostyles of the new species are relatively small, and their length overlapped with that of the ectosomal subtylostyles. In , this pattern is found only in (see Table 1). However, and sp. nov. are clearly separated by the size of acanthostyles (26–40 µm vs 73.0–91.3 in length), the presence of isochelae (absent in ), and of sigmas (absent in sp. nov.). has been only reported from off the Pacific coast of Panama (Maldonado et al. 2001), which also exhibits distant geographical distribution from type locality of sp. nov.

Discussion.

The present study adds two new species to the genus , which now has nine species. This is the first record of the genus and family from Japanese waters. Thus the discovery of these two new species from warm temperate northwest Pacific extends the geographical distribution of the genus (see Table 1). Vacelet and Cárdenas (2018) raised doubts to the hypothetical polyaxial nature of the choanosomal styles/subtylostyles and the pseudoastrose acanthostyles that has been proposed by Uriz and Maldonado (1995) and Maldonado and Uriz (1996). The authors proposed instead, a monaxonal origin for the spicule shaft with secondary axes for bulges. In our study, we could not precisely distinguish axes on the choanosomal subtylotyles or the acanthostyles. Feeble microspines around the distal tips of ectosomal subtylostyles have been first reported from Maldonado & Benito, 1991 and later considered as a possible common character of the genera and , both in the family (Maldonado and Uriz 1996). In this study, this character was observed in sp. nov. (e.g. Fig. 3F) but seems to be absent in sp. nov. (Fig. 5F). This character was not mentioned in the recently described species, and (Vacelet and Cárdenas 2018, Díaz and Pomponi 2018). The actual affinity between and has not been revealed as yet (Maldonado and Uriz 1996), but the feeble microspines around the distal tips of the ectosomal subtylostyles may be a symplesiomorphy for these two genera. The evolutionary aspect of morphological divergence among sphaeroclones, pseudoastrose acanthostyles, and typical acanthostyles has long been discussed and the question remains as to whether the amount of change between sphaeroclones and astrose acanthostyles is more important than the whole set of shared morphological features in determining the phylogenetic relationships between and (Uriz and Maldonado 1995, Maldonado and Uriz 1996). Our findings on the two new species add more knowledge on acanthostylose derivatives in . To date, long acanthostyles have been found only in (with ca 130 µm in length), but in all other species of they are less than 60 µm (see Table 1) and thus regarded as pseudoastrose acanthostyle because of the putative polyaxial nature contrasting the monoaxial nature of typical acanthostyles of other demosponge taxa (Uriz and Maldonado 1995, Maldonado and Uriz 1996). In the two new species, acanthostyles are longer than 70 µm in length, which means the alleged possession of long acanthostyles differing from typical pseudoastrose acanthostyles, is not unusual in . They also provide clues for solving the trait of gradual morphological divergence between sphaeroclones, pseudoastrose acanthostyles, and acanthostyles along with pseudoaster recently found from (Vacelet and Cárdenas 2018). A molecular phylogenetic study is necessary to unravel the diversification of sphaeroclones, pseudoastrose acanthostyles, acanthostyles and pseudoasters as well as the affinity of and within the order (Maldonado and Uriz 1996, Vacelet and Cárdenas 2018).
1Pseudoasters present D.pseudaster
Pseudoasters absent 2
2Chelae present 3
Chelae absent D.littoralis
3Microscleres isochelae only 4
More types of microscleres in addition to isochelae 5
4Size of choanosomal subtylostyles much larger than those of ectosomal subtylostyles D.tuberosocapitata
Size of choanosomal subtylostyles overlapping with those of ectosomal subtylostyle D.misakiensis sp. nov.
5Standard sigmas present 6
Standard sigmas absent 7
6Spinose microxea present 8
Spinose microxea absent D.hindei
7Other sigmoid microscleres present D.hispida sp. nov.
Other sigmoid microscleres absent D.incrustans
8Ectosomal subtylostyles longer than 250 µm D.ruetzleri
Ectosomal subtylostyles shorter than 250 µm D.urizae
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