Life Attached: Examining the Implications of Epibiosis on a North Pacific Cirripede and a Gulf of Mexico Seep Sabellid by Lauren N. Rice A dissertation accepted and approved in partial fulfillment of the requirements for the degree of Doctor of Philosophy in Biology Dissertation Committee: Michelle Wood, Chair Craig M. Young, Advisor Aaron W.E. Galloway, Core Member Erik E. Cordes, Core Member Edward B. Davis, Institutional Representative University of Oregon Summer 2024 2 © 2024 Lauren N. Rice This work is licensed under a Creative Commons BY Attribution License. 3 DISSERTATION ABSTRACT Lauren N. Rice Doctor of Philosophy in Biology Title: Life Attached: Examining the Implications of Epibiosis on a North Pacific Cirripede and a Gulf of Mexico Seep Sabellid Epibiotic species, which can either facultatively or obligatorily settle on living hosts, are commonly found in marine habitats. Despite this commonality, the biology and ecology for many epizoic organisms remain unknown and understudied. In this dissertation, I investigated how two marine invertebrate species accommodate life on living hosts. In Chapter II, I discuss the reproductive and settlement patterns for the barnacle Solidobalanus hesperius and how they correlate to the molting patterns for host crab species in the Oregon subtidal. I found that S. hesperius reproduces year-round and that brooded embryos hatch in approximately a week. Furthermore, I utilized a new method to examine the spatial distributions of barnacle individuals on their crab hosts and they were tightly correlated to the microtopography of the host carapace. The remaining chapters of the dissertation focus on a facultative epibiotic relationship found at methane seeps in the Gulf of Mexico, involving a sabellid polychaete species. In Chapter III, we found that the species are gregarious settlers and are abundant within the methane seep habitats investigated. Furthermore, we present morphological and phylogenetic evidence and identify the sabellid as belonging to a new genus and species: Seepicola viridiplumi sp. nov. 4 As the newly described sabellid is facultatively epibiotic, Chapter IV examined the trophic ecology of the species using stable isotopes. Additional tables showing the statistical pairwise comparisons highlighting the effects of season, sample site, and microhabitat on carbon, nitrogen, and sulfur isotopic ratios are provided as supplemental materials. We found that S. viridiplumi are generalist suspension feeders within the methane seeps and, using microbial evidence, show that the species does not rely on chemosynthetic symbionts. The rarefaction curves for the sequencing depth is also provided in the supplemental material section. However, individuals can occupy differing trophic niches depending on whether they are epibiotic or free- living. The different trophic niches occupied by epibiotic and free-living S. viridiplumi individuals may impact other aspects of the biology for this species. To test this, we examined and compared the reproductive output for individuals from each microhabitat using paraffin histology. In doing so, we found that epibiotic individuals consistently had slightly larger oocytes and higher levels of fecundity. The individual oocyte size distributions for all female sabellids examined in this study are shown as a supplemental figure. We also observed an apparent lack of gametogenic seasonality in this sabellid species. Taken together, the work presented in this dissertation provides unique insights into how epibiotic associations can develop and persist within an ecosystem. The results also provide additional insight into the adaptations and biology for epizoic species, which can aid in attempts for modeling community functioning. This dissertation includes unpublished co-authored material. 5 CURRICULUM VITAE NAME OF AUTHOR: Lauren N. Rice GRADUATE AND UNDERGRADUATE SCHOOLS ATTENDED: University of Oregon, Eugene, Oregon, USA University of Maine, Orono, Maine, USA DEGREES AWARDED: Doctor of Philosophy, Biology, 2024, University of Oregon Bachelor of Science, summa cum laude, Marine Science, 2017, University of Maine AREAS OF SPECIAL INTEREST: Deep-sea biology Reproductive ecology Marine Ecology PROFESSIONAL EXPERIENCE: Graduate Employee, Department of Biology, University of Oregon, Eugene September 2018 – June 2024 Research Technician, Waller laboratory, School of Marine Sciences, University of Maine, Orono Research Technician, Resource Access International, LLC Labs, Brunswick, Maine Summer 2014 – Summer 2017 GRANTS, AWARDS, AND HONORS: Donald E. Wimber Fund Award, University of Oregon, 2023 Oregon Society of Conchologists Scholarship, Oregon Society of Conchologists, 2022 William R. Sistrom Memorial Scholarship, University of Oregon, 2020 University of Oregon First Year Merit Award, University of Oregon, 2018 6 PUBLICATIONS: R.A. Beinart, S.M. Arellano, M. Chaknova, J. Meagher, A.J. Davies, J. Lopresti, E.J. Cowell, M. Betters, T.A. Ladd, C.Q. Plowman, L.N. Rice, D. Davis, M. Heffernan, V. Jimenez, T. Beaver, J. Becker, S. Bergen, L. Brunner, A. Calhoun, M. Hauer, A. Taradash, T. Giachetti, C.M. Young (2024) Deep seafloor hydrothermal vent communities buried by volcanic ash from the 2022 Hunga eruption. Communications Earth and Environment 5: 254. S. Rist, L.N. Rice, C.Q. Plowman, C.T. Fountain, A.E. Calhoun, C. Ellison, C.M. Young (2022) Reproductive biology of the bathyal asteroid Ctenodiscus crispatus in the NE Pacific. Invertebrate Biology. doi: 10.1111/ivb.12384 R.G. Waller, R.P. Stone, L.N. Rice, J. Johnstone, A.M. Rossin, E. Hartill, K. Feehan, C.L. Morrison (2019) Phenotypic plasticity or a reproductive dead end? Primnoa pacifica (Cnidaria: Alcyonacea) in the Southeastern Alaska Region. Frontiers in Marine Science 6 (709). doi: 10.3389/fmars.2019.00709. L.N. Rice, P.D. Rawson, S.M. Lindsay (2018) Genetic homogeneity among geographically distant populations of the blister worm Polydora websteri. Aquaculture Environment Interactions 10: 437-446. doi:10.3354/aei00281. 7 ACKNOWLEDGMENTS This work is thanks in large part to the continued support and assistance of family, friends, collaborators, and mentors. You all have my deepest gratitude. First, my most sincere thank you to my advisor, Dr. Craig Young. You have given me so many amazing opportunities over the years, starting with the chance to work in your lab as a PhD student. You have taught me so much, from how to build experimental equipment for deployment at sea, how to prep for a research cruise, the best ways to use a microscope, and how to pivot when things aren’t going according to plan. There have been so many moments working with you that I will cherish. I am ever thankful to my advisory committee members. Michelle Wood, you have provided so much advice and guidance over the past several years, and I have always been appreciative of all the discussions over coffee. Edward Davis, thank you for always keeping me on track with statistics and for your advice. Aaron Galloway, thank you for pushing me to look at the bigger picture and for your advocacy. Erik Cordes, thank you for all the advice, wisdom, and help over the years Erik Cordes. I could not have asked for a better committee. Thank you all for the encouragement and kind words along the way. My biggest and most sincere gratitude is extended to my lab mates: Caitlin Plowman and Avery Calhoun. Caitlin, you welcomed me wholeheartedly from the onset and provided friendship, mentorship, and guidance countless times over the years. Words cannot express the depth of my gratitude and appreciation. Avery, you always brought such a unique perspective and found a way to keep everyone in the lab smiling. Thank you for all your help and friendship and commiseration. 8 A huge thank you to the whole of the Oregon Institute of Marine Biology (OIMB) community. This campus has been my home for the past 6 years, and my work would not have been possible without all of you. Trish Mace, Laura Screen, Jeremy Worthington, Ian Washington, Bradd Beckett, James Johnson, Trystan Berry: thank you all for your friendship over the years, and for all that you do to keep this campus running. To the OIMB grad student community (and extended partners), thank you for all your advice, guidance, support, commiseration, and friendship. Erin Jezuit, Christina Ellison, Nicole Nakata, Jesse Borland, you have all done so much to make this tiny campus feel like home and have brought so much to this community. This work would not have been possible without the support of the William R. Sistrom Memorial Fellowship of the University of Oregon, and the Oregon Society of Conchology Scholarship. This work and my degree was also supported by the NSF grants 1851383 and 1737382. Lastly, I must thank my parents, Mike and Lori Rice, as well as my brothers, Garrett, and Ryan. You have all supported this crazy dream of mine since I first set my heart towards this path so many years ago. Your encouragement never wavered, despite all the late-night calls, years spent apart due to distance and COVID, and even when you had no idea what I was talking about. Words cannot capture my gratitude and love. 9 DEDICATION And to my grandmothers and my parents. You gave me all that I have, believed in me from the start, and reminded me how deep resilience can be in the face of hardship. 10 TABLE OF CONTENTS I. INTRODUCTION .................................................................................................... 15 II. PATTERNS OF DISTRIBUTION AND REPRODUCTION IN THE EPIZOOIC BARNACLE SOLIDOBALANUS HESPERIUS AND THEIR CORRELATION WITH THE LIFE HISTORIES OF THEIR HOSTS ...................... 19 1. Introduction ...................................................................................................... 19 2. Materials and Methods .................................................................................... 21 2.1. Reproduction in Solidobalanus hesperius ................................................ 21 2.2. Distribution of Barnacle Settlers on Metacarcinus magister .................... 24 2.3. Statistical Analysis ................................................................................... 26 3. Results ............................................................................................................. 27 4. Discussion ....................................................................................................... 35 5. Conclusions ...................................................................................................... 38 III. A NEW GENUS AND SPECIES OF FEATHER DUSTER WORM (ANNELIDA, SABELLIDA) FROM SHALLOW HYDROCARBON SEEPS IN THE GULF OF MEXICO .......................................................................... 40 1. Introduction ...................................................................................................... 40 2. Materials and Methods .................................................................................... 41 2.1. Sample Collection .................................................................................... 41 2.2. Species Abundance Estimates................................................................... 42 2.3. Molecular Analysis .................................................................................. 43 3. Results ............................................................................................................. 46 3.1. Systematics .............................................................................................. 46 3.2. Phylogenetic Analysis ............................................................................... 69 3.3. Species Abundance Measures .................................................................. 71 4. Discussion ....................................................................................................... 72 IV. TROPHIC NICHES AND THE ASSOCIATED MICROBIAL COMMUNITY FOR A NEWLY DESCRIBED METHANE SEEP SABELLID .................................................................................................................. 74 1. Introduction ...................................................................................................... 74 2. Materials and Methods .................................................................................... 79 2.1. Sample Collection .................................................................................... 79 2.2. 16S rRNA Sequencing and Analysis ........................................................ 81 11 2.3. Stable Isotope Analysis ............................................................................ 84 3. Results ............................................................................................................. 85 3.1. Microbial Communities ........................................................................... 85 3.2. Nutrient Resources ................................................................................... 90 3.3. Trophic Niches for Epibiotic and Free-living Seepicola viridiplumi ....... 94 4. Discussion ....................................................................................................... 96 5. Conclusions ..................................................................................................... 100 V. IMPACTS OF EPIBIOSIS ON THE REPRODUCTIVE PATTERNS OF A SABELLID POLYCHAETE FROM GULF OF MEXICO METHANE SEEPS ..................................................................................................... 102 1. Introduction ...................................................................................................... 102 2. Materials and Methods .................................................................................... 104 2.1. Study Sites ............................................................................................... 104 2.2. Sample Collection .................................................................................... 105 2.3. Histology .................................................................................................. 108 2.4. Reproductive Analysis ............................................................................. 109 2.5. Statistical Analysis ................................................................................... 111 3. Results ............................................................................................................. 112 4. Discussion ....................................................................................................... 118 5. Conclusions ..................................................................................................... 122 V. CONCLUSION ....................................................................................................... 124 REFERENCES CITED ................................................................................................ 127 SUPPLEMENTAL FILES ........................................................................................... 143 12 LIST OF FIGURES Figure Page 2.1 Live Cancer productus crab with Solidobalanus hesperius barnacles ................. 22 2.2 Gametogenic ranking of Solidobalanus hesperius ovaries ................................... 23 2.3 Percent frequency distributions for Solidobalanus hesperius gametogenic stage ...................................................................................................................... 29 2.4 Linear relationships for Solidobalanus hesperius against host crabs ................... 30 2.5 Average barnacle size and proportion of new settlers by collection month ......... 32 2.6 Solidobalanus hespeirus distributions in relation to carapace microtopography ................................................................................................... 34 3.1 In situ images of Seepicola viridiplumi ................................................................ 49 3.2 Radiolar crown and thoracic region for Seepicola viridiplumi ............................. 51 3.3 Seepicola viridiplumi anterior and posterior views .............................................. 52 3.4 Seepicola viridiplumi radiole morphology ............................................................ 53 3.5 Thoracic chaete of Seepicola viridiplumi ............................................................. 56 3.6 Collar and abdominal chaete for Seepicola viridiplumi ........................................ 57 3.7 Apical view of peristomium for Seepicola viridiplumi ......................................... 58 3.8 Scanning electron micrographs of thoracic chaete ............................................... 59 3.9 Abdominal chaete and uncini under SEM ............................................................ 60 3.10 Maximum likelihood tree showing sabellid phylogenetic relationships.............. 70 4.1 Artistic depiction of the microhabitats occupied by Seepicola viridiplumi .......... 78 4.2 Microbial diversity associated with Seepicola viridiplumi radiolar crowns ......... 87 4.3 Comparisons of microbial diversity on Seepicola viridiplumi ............................ 89 4.4 Isotopic ratios for the three study sites by collection ............................................ 93 13 4.5 Trophic niche plots for Seepicola viridiplumi ..................................................... 95 5.1 Map of study sites within the Gulf of Mexico ...................................................... 105 5.2 Color corrected in situ images of Seepicola viridiplumi ....................................... 107 5.3 Gametogenic stages for Seepicola viridiplumi .................................................... 110 5.4 Comparisons of body length between epibiotic and free-living Seepicola viridiplumi ............................................................................................................ 113 5.5 Oocyte size frequency histograms by site and collection ..................................... 115 5.6 Percent frequency distributions of pooled gametogenic stages ............................ 116 5.7 Comparisons of reproductive output between epibiotic and free-living Seepicola viridiplumi ............................................................................................ 118 14 LIST OF TABLES Table Page 2.1 Proportions of observed Solidobalanus hesperius barnacles with broods by collection month............................................................................................... 28 2.2 Proportions of brooded embryos against ovarian gametogenic stage ................... 28 3.1 Specimen IDs for Seepicola viridiplumi with accession numbers ........................ 45 3.2 Distinctive features of the genera Seepicola, Perkinsiana, Potamilla, and Pseudopotamilla ............................................................................................ 63 4.1 Collection information and sample sizes for Seepicola viridiplumi .................... 80 4.2 Sample collection information and 16s rRNA bioinformatic details .................... 83 4.3 Average isotopic values by collection .................................................................. 91 4.4 Results of two-way ANOVAs examining stable isotopic trendss ........................ 92 5.1 Collection information and sample sizes .............................................................. 106 5.2 Kruskal-Wallis test results comparing oocyte size distributions .......................... 114 5.3 Mean oocyte sizes for each site and collection of Seepicola viridiplumi ............ 115 15 CHAPTER I INTRODUCTION Habitats along continental shelves and slopes are dominated by soft bottom habitats composed of sand and mud, and rocky substrata are often patchy and scarce. The marine communities that occur on hard surfaces are frequently dominated by sessile invertebrate fauna, leading to competition for space and access to settlement locations (Jackson 1977, Osman 1977, Harder 2009, Wahl 2009). This intense competitive pressure is thought to have given rise to a commensal, spatial association known as epibiosis (Wahl 1989). In this association, a sessile organism called an epibiont, settles on and attaches to the surface of a living host, called a basibiont (Wahl 1989, 1997, 2009). Epibiotic organisms are represented by a diverse array of taxa, including polychaetes, bryozoans, tunicates, mollusks, diatoms, rotifers, barnacles, and sponges (Wahl 2009). Epibiotic species can be further categorized as epizoans (animals) or epiphytes (algae) and can either facultatively or obligatorily settle on living substrates (Wahl & Mark 1999). Epibiotic associations have been regarded as non-symbiotic due to their predominantly facultative nature and lack of obligate trophic exchange (Wahl 1989, 2009, Wahl & Mark 1999, Romero et al. 2022). However, epibiosis is still frequently categorized as an interspecies relationship (McLeod et al. 2020) where differing species “live together” in physical contact (Martin & Schwab 2012, Esteban & Fenchel 2020). In this dissertation, we identify epibiosis as a symbiotic, commensal association in recognition of the broad definition of symbiosis (Martin & Schwab 2012), the previous studies categorizing the outcomes of these associations (e.g. Uriz et al. 1992, Silina & Zhukova 2014, Puccinelli & McQuaid 2021), and the examples of obligate epibiotic species (e.g. Thamrin et al. 2001, Nájera-Hillman et al. 2012, Robinson et al. 2019). 16 Although there are some notable exceptions (McLeod et al. 2020), epibiotic species are usually smaller than their hosts and frequently act as abundant, primary consumers (Chen et al. 2021). Epibiotic associations can be observed at most latitudes, depths, and marine habitats (Wahl 2009). Despite this ubiquitous presence, many epizoan species are understudied compared to the host taxa. This is primarily due to the smaller size of epizoic species, greater difficulty in sampling and processing, epizoans compared to hosts, and that epizoans often belong to taxa with poor phylogenetic resolution and are difficult to identify (Chen et al. 2021). The advantages and disadvantages of epibiotic settlement has been well studied (Wahl 1989, 1997, 2009, Harder 2009). More frequently, however, studies attempt to identify and categorize the nature of epibiotic relationships from the perspective of the basibiont (e.g. Xu & Burns 1991, Wargo & Ford 1993b, Manning & Lindquist 2003, Eschweiler & Buschbaum 2011, Burris et al. 2014, Silina & Zhukova 2014). This focus often fails to capture the dynamic nature of the relationships (Zapalski 2011) and overlooks the biology and ecology of the epizoan. In this dissertation, I sought to investigate how epizoan species adapt to life on living hosts. Some generalizations have been proposed for how epibiotic species have adapted, including abbreviated life spans compared to free-living relatives, the ability to facultatively or obligately undergo asexual reproduction, and general trophic independence from their host (Wahl & Mark 1999, Fernandez-Leborans 2010). However, quantitative evidence supporting these claims remains scant, especially given the commonality of epibiotic associations. The following chapters focus on two different epizoic species and examine how epibiotic life impacts settlement timing, patterns of reproduction, and trophic ecology. In Chapter II, I discuss a species of balanid barnacle local to the Oregon subtidal that is primarily attached to crab hosts. While the barnacle is known to be a short-lived species, I 17 hypothesized that it has adapted its reproductive cycle to coordinate with the regular molting of the host exoskeleton. Additionally, I developed a novel way to investigate the spatial distributions of barnacle individuals on the host exoskeleton. Chapter II is unpublished but will include Dr. Craig M. Young as a co-author, as he provided editorial assistance. Chapters III, IV, and V focus on a facultative hyper-epibiotic species of sabellid feather duster polychaete from shallow methane seep habitats within the Gulf of Mexico. While the species is highly abundant, the sabellid has remained unidentified. In Chapter III, I present the morphological and phylogenetic description of the sabellid and simultaneously erect a new genus. This chapter is unpublished and will include co-authors Dr. Mariana Tovar-Hernandez for assistance with the morphological description; Christina Ellison, who contributed to the genetic identification; and Dr. Craig M. Young who provided funding. All coauthors contributed to manuscript preparation. While individuals of the newly described sabellid are commonly found in authigenic carbonate along the seafloor, they can also be found atop a file clam that is an obligate epizoan on tubeworms within methane seeps. This means that epibiotic sabellids may be a meter or more above their free-living conspecifics and provides an ideal system to examine the impacts of epibiosis on a species from a chemosynthetic habitat, which had not previously been examined. In Chapter IV, I hypothesized that the difference in height above the seafloor could impact the diet of the sabellid individuals. As a sabellid species at methane seeps off Costa Rica was recently found to harbor chemosynthetic bacterial symbionts (Goffredi et al. 2020), I also investigated the microbial communities associated with the newly described sabellid between each microhabitat. Chapter IV is unpublished but will include Dr. Stilianos Louca for assistance with microbiome analysis and manuscript preparation, Dr. Erik Cordes for project guidance and assistance with data 18 interpretation, and Dr. Craig M. Young for funding and manuscript preparation assistance. In Chapter V, I hypothesized that any potential differences in diet and trophic ecology may influence the overall fitness of sabellids from each microhabitat. Thus, I examined the reproductive patterns of the newly described sabellid in order to: 1) obtain the first reproductive data for any deep-water sabellid species, and 2) determine if there was a difference in reproductive output (i.e. fecundity and oocyte size) between epibiotic and free-living sabellids. Chapter V is unpublished but will include Dr. Craig M. Young as a coauthor for providing funding and assistance with manuscript preparation. Despite the commonality of epibiotic species in marine ecosystems, many epizoans remain unidentified (Chen et al. 2021), and the biology and ecology of these organisms largely remain unknown. As these associations have the potential to drive environmental change (McLeod et al. 2020), there is a need to better understand the species diversity that exists for epizoans and their ecological roles both from a trophic perspective and due to the influences they can exert on host taxa (Wahl 1989, 2009, Chen et al. 2021). The work presented here directly addresses some of these key knowledge gaps. 19 CHAPTER II PATTERNS OF DISTRIBUTION AND REPRODUCTION IN THE EPIZOOIC BARNACLE SOLIDOBALANUS HESPERIUS AND THEIR CORRELATION WITH THE LIFE HISTORIES OF THEIR HOSTS This work includes coauthor Dr. Craig Young as contributor to manuscript preparation. 1. INTRODUCTION Continental shelves are generally dominated by soft-bottom habitats made of sand and mud, and rocky substrata can be scarce and patchy. Sessile invertebrates living on marine hard bottoms often experience intense competition for settlement sites and space to grow (Osman 1977, Harder 2009, Wahl 2009). Epibiosis is a common strategy among sessile suspension- and filter- feeding species (Wahl 1989), and biological substrata increase the available surfaces that can be used for settlement (Gili et al. 1993). For example, crabs and other decapods found in areas with sandy bottoms often support epibiotic communities (Heath 1976, Gili et al. 1993, Negreiros- Fransozo et al. 1995, Key et al. 1997, Pasternak et al. 2002, McGaw 2006, Campos et al. 2022, Dvoretsky & Dvoretsky 2023). Potential advantages of epibiotic settlement on a crab include increased access to food particles due to the activities of the host (Heath 1976) and protection from predators (Key et al. 1997, Harder 2009, Wahl 2009). At the same time, epibionts must contend with host behaviors such as hiding in crevices, burial (Negreiros-Fransozo et al. 1995, Becker & Wahl 1996), and the periodic molting of the exoskeleton (Gili et al. 1993). Many epibiotic species have high rates of growth and reproduction as well as abbreviated life cycles (Jackson 1977, Seed 1985), which may allow epibionts to accommodate to the ephemeral availability of a crab exoskeleton. In this study, we sought to examine a short-lived acorn barnacle to determine if the reproductive patterns might be related to the molting of their host crabs. 20 Acorn barnacles are frequently found as epibionts and have been well-documented on sea turtles (Farrapeira 2010, Razaghian et al. 2019, Robinson et al. 2019), shellfish (Gabaev 2013, Silina & Zhukova 2014, Puccinelli & McQuaid 2021), corals (Newman et al. 1976, Lewis 1992, Thamrin et al. 2001, Frick & Ross 2002), crabs (Heath 1976, Key et al. 1997, McGaw 2006, Campos et al. 2022), and horse shoe crabs (Key et al. 1996, Lim et al. 2021). On crabs, epibiotic barnacles have been shown to concentrate in grooved regions of the carapace (Heath 1976, Key et al. 1997, McGaw 2006). The barnacle Solidobalanus hesperius (formerly Hesperibalanus) is broadly distributed across the North Pacific, with most observations and studies from the Sea of Japan (Zhukova 2000, Silina 2002, Korn & Scherbakova 2012). Fewer observations come from Washington (Barnes & Barnes 1959) and Oregon (Shanks 2001, Carlton 2007, Meyer et al. 2018) despite a long-term history of presence in the area (Zullo & Marincovich 1990). Solidobalanus hesperius frequently settle as epibionts on crabs and cultured shellfish (Zhukova 2000, Korn & Scherbakova 2012, Gabaev 2013) and are readily outcompeted for space by other organisms such as algae (Ovsyannikova 2010). The species is reported to have a short life span of six to seven months, with few individuals surviving longer than a year (Ovsyannikova & Levin 1982), and has been described as a pioneer species (Meyer et al. 2018). However, little is known about the ecology and settlement patterns of S. hesperius outside the Sea of Japan, and no study has examined adult populations in the Eastern Pacific. This study investigated aspects of distribution and life-history biology in S. hesperius barnacles attached to Dungeness (Metacarcinus magister) and red rock crabs (Cancer productus). Both crab species are abundant off Oregon, important to local fisheries, and can be found overlapping in several habitats (Orensanz & Gallucci 1988). While epibiotic communities for M. 21 magister and C. productus have been examined in British Columbia (McGaw 2006), the relationship between S. hesperius and the crab hosts remains unstudied. Here, we sought to investigate the reproductive and settlement patterns for S. hesperius in relation to the known molting patterns of the host crab species. Furthermore, recent work examining the distribution patterns of epibiotic barnacles on crabs have relied on methods that divide the host exoskeleton into broad regions (Heath 1976, Key et al. 1997, McGaw 2006). Such methods do not capture fine- scale patterns and are often difficult to replicate on new host species. We developed and utilized a novel method to examine the density and spatial distributions of S. hesperius on the dorsal surfaces of M. magister. This method can easily be applied to other species. 2. MATERIALS AND METHODS 2.1 Reproduction in Solidobalanus hesperius To determine the reproductive seasonality of Solidobalanus hesperius, we collected live specimens monthly from host crabs between June 2022 and May 2023, except for October and November 2022. Metacarcinus magister and Cancer productus crabs with epibiotic barnacles were collected using baited crab pots deployed from either the pier at the Oregon Institute of Marine Biology campus (43°20'59"N 124°19'49"W), or the nearby docks at the Charleston Marine Life Center (43°20'43"N 124°19'41"W) during times of significant swell. Monthly collections were at least three weeks apart. Crab pots were deployed for 8-hour intervals and were checked hourly. Any crabs with attached barnacles were kept for further processing. The carapace length and width of each crab were measured, with carapace width being defined as the distance between the bases of the tenth pair of anterolateral spines. We measured from the base of the anterolateral spines to avoid inconsistencies caused by broken or eroded spines. Carapace length was measured as the distance between the tip of the rostrum and the 22 posterior edge of the carapace. Epibiotic barnacles were identified using Light and Smith’s manual (Carlton 2007), counted, and approximate locations on the crab host were recorded (i.e. dorsal, ventral, appendages). Crabs were then imaged using a Canon PowerShot G12 digital camera (Figure 2.1). Only barnacles identified as Solidobalanus hesperius were removed using a scraper and forceps and isolated into individual bowls of seawater filtered through a 0.45 μm membrane filter. This was done to ensure that hatching nauplii (if present) could be counted and tracked to an individual barnacle. For each collection, barnacles were randomly chosen across the full available size range. We measured both carnia-rostrum and lateral diameters for each barnacle before removing the visceral mass to expose the ovary and coelomic cavity. Using a Zeiss Stemi 508 microscope fitted with a Zeiss Axiocam 208 camera, micrographs were taken of the ovary (Figure 2.2), which was then ranked for gametogenic stage using the protocols of Hines (1976) and Yan et al. (2006). Figure 2.1. Live Cancer productus crab bearing adult Solidobalanus hesperius (sh) and newly settled individuals (ns). Scale bar represents 2 cm. 23 Figure 2.2. Gametogenic ranking of Solidobalanus hesperius ovaries: (A) Stage 1– no ovary is visible in the basal membrane (bm); (B) Stage 2 – rudimentary ovarian structures (ro) are faintly discernible as a grainy texture; (C) Stage 3 – a moderately developed ovary (o), which has a yellow coloration and slight grainy appearance; (D) Stage 4 – a fully developed, opaque yellow ovary filled with observable ova (oa) with visible testes. All scale bars represent 1 mm. If present, brooded embryos from each barnacle were transferred into separate bowls of 0.45 μm filtered seawater and kept partially submerged in a flow-through seawater table. Water temperature was recorded daily. Water was changed daily, and developmental stage was checked every 24 hours to determine an estimated time to hatching. As the time of fertilization was 24 unknown, the appearance of certain features (individual cells, appendages, eyespots, first movement, appearance of pigment) was used to track progression until hatching. To ensure accuracy, only broods judged to be in “early” developmental stages (individual cells visible, but no naupliar structures) were included in the final estimates of hatching time. Hatched nauplii from all brooding S. hesperius individuals were counted to obtain measurements of fecundity. 2.2 Distribution of Barnacle Settlers on Metacarcinus magister To examine patterns of settlement and spatial distribution of S. hesperius on M. magister hosts, molted carapaces were collected daily from a one kilometer transect spanning the sandy intertidal area in Devil’s Kitchen State Park, Oregon (43°04'57"N 124°26'10"W), from April 30th, 2020 to April 30th, 2021. Each day, the total number of observed M. magsiter carapaces and the number with epibiotic barnacles were recorded. We carefully brushed all carapaces bearing epibiotic barnacles to remove sand. A total of 1481 carapaces were collected over the study period, and a random subsample of 610, ranging from 2-260 each month depending on availability, was selected for image analysis. Carapaces were imaged using a Canon G12 Powershot camera mounted on a tripod, and only intact carapaces were included. Images were analyzed in Adobe Photoshop (versions 23 and 24.6). Width and length of the crab carapace, as well as carnia-rostrum and lateral diameters of barnacles were measured using the Ruler Tool. Only barnacles attached to the host carapace were examined; individuals affixed on top of other barnacles were excluded. As multiple barnacle species can settle on crab hosts, such as Balanus crenatus and B. glandula, all attached barnacles were identified using the Light and Smith Manual (Carlton 2007). As individuals could lack the tergum and scutum, the shape of the shell plates were used for species identification. Newly settled barnacles were identified as individuals with carnia-rostrum diameters 25 less than 1.5 mm. This diameter was selected based on the growth rates described by Ovsyannikova & Levin (1982), who reported that metamorphosing S. hesperius cyprids were approximately 0.8 mm in diameter and individuals 2.0 mm in diameter were about a month old. There was a heightened degree of uncertainty for the species identification of smaller, newly settled individuals (<2 mm), and data may include low numbers of other species such as B. crenatus and B. glandula. Using a novel method with Adobe Photoshop, we analyzed a subset of 483 carapaces, including representatives from every size class, to examine spatial patterns of S. hesperius on the dorsal surface of M. magister. First, images were straightened so the tenth pair of anterolateral spines were horizontal at 180o. Images were then proportionally transformed so the carapace width was scaled to 350 mm (arbitrary cutoff). Next, a digital axis origin was manually set in the middle of each carapace using the intersection of lines representing carapace length and width as guides. The center of each barnacle was then recorded and marked using the coordinate-system built into the Photoshop software. The location and number of barnacle clusters, defined as when two or more barnacles were in contact, were also recorded. The transformation of carapace length created a unified observation area and consistent coordinate plane among crabs of various body sizes. This enabled the spatial distributions to be aggregated and viewed against a hypothetical, standardized dorsal carapace. To investigate the effects of carapace microtopography on barnacle settlement, a random, intact M. magister carapace lacking epibiotic barnacles was imaged using an iPhone 13 (iOSv 17.2.1). A three-dimensional point cloud and mesh were then generated using Agisoft Metashape software version 1.22.6 (2016). The resulting mesh was cleaned and aligned before a 25-step interval was applied to generate a scalar height map in CloudCompare version 2.12.4 (2022). 26 2.3 Statistical Analysis All statistical analyses were conducted in RStudio version 4.2.3 (R Core Team 2023). The commonality of C. productus and M. magister bearing S. hesperius varied each month. Thus, we pooled measurements of oogenic frequency, fecundity, and barnacle diameter collected from both host species into a single dataset prior to statistical analysis. Linear regression analysis was used to determine the effect of barnacle size (carnia-rostrum diameter) on fecundity for the live-caught barnacles. Chi-square contingency table analyses were used to compare the frequency of oogenic stages between collection months. Pearson correlation tests were used to examine the linear dependence of the two size metrics recorded for each species. After finding strong correlations between the barnacle diameters (t = 162.5, p = 2.2e-12) and the carapace measurements (t = 152.99, p = 2.2e-12), we used carnia- rostrum diameters and carapace width measurements in all subsequent statistical tests as proxies for barnacle and crab size. Linear regression was used to examine the relationship between the size of molted M. magister carapaces and the number and size of attached S. hesperius individuals. We also examined the relationship between carapace size and the number of barnacle clusters. The statistical distributions and variances of barnacle size on molted carapaces were examined using the Shapiro-Wilk test (Shapiro & Wilk 1965) and Levene’s Test (Levene 1960), respectively. Measurements of barnacle size for each month were compared using the Kruskal-Wallis Test (Kruskal & Wallis 1952) and Dunn’s post hoc test (Dunn 1964) with p-value adjustments made using the Holm Method (Holm 1979). To examine the spatial point patterns for individual S. hesperius barnacles and barnacle clusters, point distributions were compared to a Complete Spatial Randomness (CSR) model using the quadrat method with a 15 x15 division across a standardized representation of an M. magister carapace. Spatial distributions were then tested for both 27 randomness and levels of spatial clustering, with significance being determined using a chi-squared distribution. 3. RESULTS Of the 1232 live barnacles observed on 37 captured crab hosts, the majority were on the dorsal carapace (n = 652) and relatively few were found on the ventral side (n = 210). Collected crabs had a wide range of epibiotic loads, with several individuals having only a single barnacle and one Cancer productus having 150 barnacles. Instances of high epibiotic load were only observed in July and August, 2022 and most of the observed barnacles during these months were identified as new settlers. A total of 162 Solidobalanus hesperius barnacles were dissected to check oogenic stage and look for brooded embryos. Brooded embryos were observed at most times of the year, with peaks of higher occurrence in June and August 2022, as well as March 2023 (Table 2.1). Broods did not appear to correspond to a specific oogenic stage but were slightly more common in individuals with ovaries at stages 2 and 4 (Table 2.2). Oogenic stage frequencies varied throughout the study period (χ2 = 109.2, p <0.0001; Figure 2.3). The frequency of individuals with stage 1 ovaries was significantly higher in January and April, and significantly lower in July. Individuals with stage 2 ovaries were observed in every month except March and May and had statistically significant increases in abundance in December, January, and February (Figure 2.3). Individuals with stage 3 ovaries were not observed in December, January, and April. However, stage 3 individuals were significantly more common in July, August, and May. Mature stage 4 ovaries were observed in every month except January and were significantly more common in November and March (Figure 2.3). 28 Table 2.1. Proportions of observed Solidobalanus hesperius barnacles with brooded embryos by month, starting in June 2022 and concluding in May 2023. Month Total Number of Barnacles Observed Number with Broods Proportion with Broods (%) June 16 8 50 July 19 4 21.1 August 19 12 63.2 November 16 2 12.5 December 10 0 0 January 11 0 0 February 9 2 22.2 March 21 8 38.1 April 21 3 14.3 May 20 2 10 Table 2.2. Proportions of brooded embryos corresponding to each ovarian gametogenic stage for Solidobalanus hesperius collected between June 2022 and May 2023. Total Observed Number with Broods Proportion (%) Stage 1 43 7 16.3 Stage 2 19 6 31.6 Stage 3 43 9 20.9 Stage 4 54 18 33.3 29 Figure 2.3. Percent frequency distribution of each oogenic stage for each collection month, starting in June 2022 and concluding in May 2023. The number of Solidobalanus hesperius individuals examined is shown in Table 2.1. Solidobalanus hesperius individuals collected from both Metacarcinus magister and Cancer productus hosts were pooled to compensate for erratic collections from each host. A total of 41 live S. hesperius barnacles were observed with brooded embryos. Of these, 30 could be used for fecundity counts and 19 were identified as “early” in development. Barnacles collected from the same host crab often had brooded embryos at varying stages of development, with some broods hatching upon dissection and others being recently deposited. Barnacle fecundity increased with body size in a roughly linear relationship (R2 = 0.45, p <0.0001), with larger 30 individuals often having larger broods (Figure 2.4A). The sizes of reproductive S. hesperius individuals varied; the smallest individual with a stage 4 ovary had a diameter of 3.8 mm and the largest had a diameter of 14 mm. The smallest individual with mature testes was 3.0 mm in diameter, and the smallest with an observed brood was 4.5 mm. Figure 2.4. Linear relationships between: (A) barnacle fecundity and carnia-rostrum diameter for all brooding females observed in this study (n = 30); (B) the number of barnacles by molted carapace width; (C) the number of observed barnacle clusters by molted carapace width; (D) the carnia-rostrum diameters for barnacles by molted carapace width. The equations and R2 values for each regression are indicated. Barnacles are S. hesperius and molted carapaces are from M. magister. 31 Embryos developed rapidly, with all 19 broods beginning to hatch as nauplii five to seven days after first observation. Isolated broods were exposed to natural fluctuations in seawater temperature, which ranged from 10oC to 15oC depending on the season. Broods collected in February and March 2023 experienced colder temperatures (10 – 12oC) compared to those collected in July and August 2022 (14-15oC). Broods exposed to temperatures around 12oC hatched in an average of 6.7 days after first observation (SD ± 0.6), while those reared in temperatures around 14.5oC hatched in an average of 5.7 days after first observation (SD ± 0.9). From the molted Metacarcinus magister carapaces, the morphometrics of 2158 S. hesperius individuals were recorded. Mean S. hesperius sizes fluctuated each month during the study period (Figure 2.5A; Table 2.3). The largest body sizes were seen in winter (Nov-Jan) and the next highest in late spring (May-Jun). Both peaks were followed by small average body sizes in February and August, respectively (Figure 2.5A). The lowest mean body sizes, seen in august, correspond to the largest settlement pulse observed during the study (Figure 2.5B). Although this trend could include data from Balanus crenatus and B. glandula. A similar peak was also seen to a lesser degree in July and September, but the proportions of new settlers remained at approximately 20% of the population for the rest of the year (Figure 2.5B). Of the 2158 S. hesperius examined for morphometrics, 926 were observed in clusters and a total of 325 clusters were identified. Clusters consisted of an average of 2.5 (SD ± 1.8) individuals, although clusters with 19 S. hesperius were also observed. 32 Figure 2.5. (A) The average carnia-rostrum diameter for observed Solidobalanus hesperius barnacles attached to molted Metacarcinus magister carapaces each month during the collection period, beginning in May 2020 and ending in April 2021. Error bars represent 95% confidence intervals. (B) The proportion of new settlers, defined as individuals smaller than 1.5 mm in carnia-rostrum diameter, observed each month starting in May 2020 and concluding in April 2021. 33 The number of S. hesperius barnacles did not increase in relation to M. magister carapace width (R2 = 0.042, p <0.0001; Figure 2.4B). Crabs 75 mm and larger often had more than 10 barnacles, but many had only a single S. hesperius. Similarly, the number of barnacle clusters was not dependent on the size of the crab host (R2 = 0.0004, p >0.1), with crabs frequently having only one to two clusters regardless of size (Figure 2.4C). Carnia-rostrum diameters of barnacles also varied greatly on M. magister carapaces regardless of host size (R2 = 0.003, p <0.001; Figure 2.4D). The coordinate locations of 1738 individual barnacles and 237 S. hesprius clusters were identified in relation to 483 host crab carapaces. The spatial distributions were pooled and viewed against a hypothetical, standardized dorsal carapace (Figure 2.6A). Spatial distributions for both individual barnacles and S. hesperius clusters were non-random (clusters: X2 = 216.9, p <0.0001; individuals: X2 = 3323.6, p <0.0001) and strongly aggregated in space (clusters: X2 = 216.9, p <0.0001; individuals: X2 = 3323.6, p <0.0001). Solidobalanus hesperius individuals and clusters were commonly found within areas marked by depressions in the host M. magister dorsal carapace (Figure 2.6B), notably in the frontal area behind the rostrum, the depressions in the central region of the carapace above the brachial lobes, and along the outer-most edge of the carapace. The epi- and mesobrachial regions, characterized by higher ridges on the carapace had a lower barnacle presence (Figure 2.6). 34 Figure 2.6. (A) Aggregated distribution of all individual Solidobalanus hesperius barnacles (grey) and barnacle clusters (red) across a standardized representation of the dorsal surface of a Metacarcinus magister carapace. (B) Color coded visualization of the dorsal microtopography present on the dorsal carapace of a M. magister. The bar indicates carapace height scaling (cooler colors indicate lower areas, warm colors indicate higher regions). The scan was made of an individual 145 mm in width that had no epibiotic barnacles. 35 4. DISCUSSION The majority of epibiotic barnacles were found on the dorsal carapaces for both Metacarcinus magister and Cancer productus hosts, as opposed to the ventral carapace and appendages for each species. Similar trends have been reported for other epibiotic taxa on crab hosts (Gili et al. 1993, Negreiros-Fransozo et al. 1995, Key et al. 1997, Dvoretsky & Dvoretsky 2023), and several key factors likely influence this pattern. The dorsal carapace is likely the most exposed portion for both M. magister and C. productus hosts. Both species are known to bury themselves in sand with only portions of their dorsal carapace remaining visible (Bellwood 2002) and can remain covered for prolonged periods of time (McGaw 2005). The ventral carapace likely experiences higher rates of abrasion, either from the action of burial in sand or by movement of the host over the seafloor (Negreiros-Fransozo et al. 1995), which may result in a lower abundance of S. hesperius barnacles. Furthermore, the dorsal surfaces of C. productus and M. magister are more exposed to light and cyprid larvae of other species have been shown to use light fields to aid in orientation before settlement (Visscher 1928, Crisp 1974). Larval settlement for Solidobalanus hesperius appears to consistently occur in late summer for populations in Oregon. In addition to the patterns seen here, the only other reported recruitment event we have found for this species was also documented by Meyer et al. (2018) between August and October 2014. These results reflect similar findings in the Sea of Japan, where S. hesperius larval recruitment peaks from August into the fall (Ovsyannikova & Levin 1982, Korn 1999, Gabaev 2013). It has been hypothesized that S. hesperius settlement is influenced by changes in the velocity of benthic currents (Ovsyannikova & Levin 1982), and indeed observations off Oregon seem to corroborate this (Meyer et al. 2018). Mature ovaries with discernible ova were observed every month between June 2022 and 36 May 2023, with January being the sole exception. The consistency in oogenic stages, and number of broods, observed throughout the sampling period indicate that S. hesperius reproduction may be continuous at the population level and that larvae could be produced throughout the year. Continuous reproduction has also been reported for populations in the Sea of Japan (Ovsyannikova & Levin 1982), where spawning was observed throughout the year. The lack of advanced oogenic stages and broods seen in winter (Dec-Jan) months in this study could reflect a reduced sample size in those months. Broods were particularly abundant in the June and August collections. This species is known to feed on detritus, with an increasing dependence on diatoms as individuals grow in size (Zhukova 2000). Diatoms often become increasingly abundant off Oregon throughout the summer season due to upwelling (Du & Peterson 2014) and could provide S. hesperius the nutrition needed to increase reproductive output. Brooded embryos were observed in individuals of various oogenic stages. This could indicate the potential for a rapid turnaround between brood cohorts, which was supported by the rapid developmental times for broods. Brooding times are known to vary widely among barnacle species and across temperature ranges within species, with hatching for Balanus crenatus occurring between 15 and 37 days (Hoeg et al. 1987), and between 22 and 27 days for B. glandula (Hines 1976). As one-month-old S. hesperius are approximately 2.0 mm in diameter (Ovsyannikova & Levin 1982), the small body sizes for reproductively mature individuals seen here provide evidence for rapid development and early reproduction in this species. While S. hesperius larvae may be present within the plankton throughout the year, peaks in settlement and brooding in S. hesperius seemingly correlate with the molting patterns in host crabs. Cancer productus are known to molt from June to August (Knudsen 1964), and M. magister molt from March through June (Rasmuson 2013). The increased number of competent cyprids in July 37 and August could allow for a large and effective recruitment on the abundant, newly hardened crab carapaces. As the adults for both host crab species are known to molt annually, this peak in S. hesperius settlement ensures that most individuals have the maximal amount of time to grow and reproduce. Like most crab species however, M. magister and C. productus juveniles can molt several times within a year. The continuous production of larvae and settlement of S. hesperius throughout the year could ensure that this species is able to take advantage of any available biological substratum. This could include crabs, but also various mollusk species such as scallops (Silina & Zhukova 2014). Rapid maturation and a short life cycle of this species probably increase the likelihood that individuals on young crabs can reproduce before their host molts. When settling on a crab host such as M. magister, S. hesperius individuals appear to favor attachment in low points of the microtopography of the dorsal carapace. This is expected, as barnacles are well known to settle in depressions and areas of increased topography (Crisp & Barnes 1954). Similar patterns have also been documented in other cases of barnacle epibiosis on crabs (Heath 1976, Key et al. 1997, McGaw 2006). Barnacles settled on the higher regions of the carapace are more exposed to abrasion when the host crab buries into sand (Negreiros-Fransozo et al. 1995, Key et al. 1997). Solidobalanus hesperius is well adapted to make use of ephemeral, biological substrata. While this barnacle species is also reported to settle on bivalves and gastropods, S. hesperius appears strongly r – selected (Pianka 1970). Decapod crustacean exoskeletons have been described as unsuitable for a variety of epibiotic taxa due to their temporary nature (Gili et al. 1993). However, the quick brooding times, coupled with the correlation of S. hesperius reproduction and settlement with the molting patterns of common crab species, allow S. hesperius to maximize the potential benefits of epibiotic life. These benefits have been well described (Wahl 1989) and 38 reviewed (Key et al. 1996). Specifically for S. hesperius, which is readily outcompeted for space (Ovsyannikova 2010), settlement on crabs and other organisms likely free individuals from competitive pressure. The effects of epibiotic organisms on decapod crustacean hosts is an active area of research. The nature and composition of the epibiotic community found on the host carapace is known to provide information about the growth, molting frequency, and behavior of the host (Abelló et al. 1990, Gili et al. 1993). This can be particularly useful when the host species is targeted by fisheries, as is the case for both M. magister and C. productus. Furthermore, examinations of epibiotic communities from a biodiversity prospective can provide insight for shifts in species abundance patterns (Farrapeira 2010, Lim et al. 2021, Dvoretsky & Dvoretsky 2022, 2023). In general though, many studies on epibiota and epibiotic barnacles seek to understand the nature of the association and its potential influence on the health of the host, especially as a high epibiotic load is known to have negative impacts (Key et al. 1997, Ovsyannikova 2010, Babu et al. 2012, Gabaev 2013, Campos et al. 2022). While knowledge of the biology and ecology of the epibiotic species can be gleaned from these studies (Dvoretsky & Dvoretsky 2022), research directly investigating the epibiotic species remains comparatively rare. 5. CONCLUSIONS By directly examining the reproductive patterns of Solidobalanus hesperius, we revealed that this species has an extremely accelerated life history marked by the early onset of reproductive maturity. Furthermore, by reproducing year-round and having a rapid reproductive cycle, S. hesperius can accommodate settlement on an unpredictable and ephemeral substratum. Many barnacle individuals die, as evidenced by the high numbers of barnacles on molted Metacarcinus magister crab carapaces. The reproductive strategies described here ensure that enough members 39 of the population can reproduce successfully. We also found that the spatial distributions of S. hesperius closely followed the microtopography of the host carapace, and likely enabling individual barnacles to persist despite detrimental host behaviors such as burial. BRIDGE In Chapter II, I focused on examining how a short-lived epibiotic barnacle species has adjusted its reproductive patterns to accommodate life on an ephemeral host crab exoskeleton. Nex, I investigated a similar relationship, but in a facultative epibiotic sabellid polychaete found in the specialized environment of hydrocarbon methane seeps. For Chapter III, I focused on describing the morphology and phylogenetics of the sabellid polychaete. 40 CHAPTER III A NEW GENUS AND SPECIES OF FEATHER DUSTER WORM (ANNELIDA, SABELLIDA) FROM SHALLOW HYDROCARBON SEEPS IN THE GULF OF MEXICO This chapter contains unpublished coauthored material. Dr. Mariana Tovar-Hernandez assisted with the morphological description, Christina Ellison contributed to the genetic analysis and phylogenetic identification, and Dr. Craig Young provided funding. All coauthors contributed to manuscript preparation. This chapter is written in the style of Biodiversity Data Journal. 1. INTRODUCTION Polychaetes in the family Sabellidae are diverse with 512 named species across 42 genera (Capa et al. 2021). Sabellids are also recognized as a ubiquitous group with representatives appearing in a variety of marine habitats, although most species have been described from shallow- water systems (reviewed by Capa et al. 2019). However, sabellids have been reported up to depths of 9735 meters (Levenstein 1961). Sabellid diversity in deep-water habitats is relatively undescribed, with only a few reports identifying sabellids to genus name only and others identifying only to taxonomic family (Capa et al. 2021). Only two sabellid species have been identified from deep-sea chemosynthetic habitats, both belonging to the genus Bispira Krøyer, 1856. Bispira wireni (Johansson 1922) was described from hydrothermal vent systems in the Okinawa Trough off southern Japan at a depth of 1335 meters (Capa et al. 2013). The second species was identified to the genus Bispira, and was found at methane seeps from Jaco Scar, Costa Rica at depths of 1768 to 1887 meters depth (Goffredi et al. 2020). This latter species is a newly identified example of chemosynthetic bacterial symbiosis, where strains of methanotrophic Methylococcales bacteria were embedded in the cuticle of the 41 radioles (Goffredi et al. 2020). In the present study, we report findings of a third sabellid species observed at chemosynthetic systems. This species is found in hydrocarbon seeps on the Upper Louisiana Slope in the northern Gulf of Mexico. Individuals are facultative, hyper-epibionts and can be found burrowed into the valves of Acesta oophaga Järengren, Schander and Young, 2007 file clams as well as free-living within authigenic carbonate. These worms have a mix of morphological features like those described in the genera Perkinsiana Knight-Jones, 1983 and Pseudopotamilla Bush, 1905, but not the genus Bispira. The new species described here also has several unique features, allowing for the establishment of a new genus and a new species. These findings were also supported through genetic analysis. 2. MATERIALS AND METHODS 2.1 Sample Collection Specimens were collected from the hydrocarbon seeps Bush Hill, Green Canyon 234, and Brine Pool NR1 using either ROV Jason deployed from the R/V Thomas G. Thompson (expedition TN391) or HOV Alvin deployed from the R/V Atlantis (expedition AT50-04). Collections occurred in June 2021 and October 2022, respectively. On each collection, individuals from both authigenic carbonate and A. oophaga valves were gathered using the vehicle manipulator arm and subsequently transported to the surface in insulated collection boxes. After recovery to the ship, carbonate slabs were broken into smaller pieces using a hammer and chisel and sabellids were isolated from both substrate types using dental picks. Samples were then fixed in buffered formalin, washed in water, and stored in 70% ethanol. Tissues used in genetic work were frozen to -80oC at sea. Tissue samples from two additional sabellid individuals were post-fixed in Osmium 42 Tetroxide for two hours before being dehydrated in a graded ethanol series ending in two 100% ethanol baths for 20-minutes each. The tissues were then critical point dried with CO2, mounted on stubs, and coated with 20 nm of gold. The stubs were viewed on a Tescan Vega II SBU and ZEISS Ultra-55 scanning electron microscope. Complete specimens were measured for their mid-thoracic width, trunk length (from chaetiger 1 to pygidium) and radiolar crown length. Other features such as the number of radiolar pairs, thoracic, and abdominal segments were also counted. Description of the new species is based on the holotype, with paratype variations indicated in parentheses. The thoracic glandular pattern was described by staining specimens with methyl green. Type specimens were deposited in the following collections: Colección Poliquetológica de la Universidad Autónoma de Nuevo León (UANL) and Colección Nacional de Anélidos Poliquetos de México, Instituto de Ciencias del Mar y Limnología, Universidad Nacional Autónoma de México (CNAP–ICML, UNAM). 2.2 Species Abundance Estimates Observations of sabellid abundance were quantitatively examined from video footage from either the ROV Jason in June 2021, or the HOV Alvin October 2022. Representative image frames were randomly selected for analysis from video footage of sabellid collections. As the primary mission for the dives was to conduct sample collections and to place scientific instrumentation, clear and continuous footage of the seafloor was scattered. Additionally, scaling lasers were haphazardly enabled throughout the dives and were often not visible in image frames. Thus, the visible surface area for each frame (the area that is well lit and in focus) was estimated using a scaling approach based on observable equipment present in the image. The equipment used had 43 known dimensions and helped to ensure consistent and accurate scaling. Visible sabellid tubes within each frame were counted using ImageJ (NIH). Epibiotic sabellid density was measured by counting the number of tubes present on each valve of host Acesta oophaga. All collected A. oophaga had their shell length and width recorded. 2.3 Molecular Analysis We extracted DNA from each specimen using DNEasy Blood and Tissue Kit (Qiagen) following the manufacturer’s protocol. We attempted to amplify and sequence the Folmer region of the mitochondrial protein-coding gene cytochrome c oxidase I from each individual using universal primers LCO1490 5' GGTCAACAAATCATAAAGATATTGG and HCO2198 5' TAAACTTCAGGGTGACCAAAAAATCA (Folmer et al. 1994). Each PCR was performed in a 20 µL volume using 2 µl of unquantified DNA extract, 200 µM of dNTPs (NE Biolabs), 500 nM of each primer (IDT) and 1 unit of Go Taq polymerase with supplied buffer (Promega). We used the following thermocycling profile: initial denaturation at 95°C for 2 min, followed by 35 cycles of: 1) denaturation, 95°C, 40 s; 2) primer annealing, 45°C, 40 s; 3) primer extension, 72°C, 1 min; followed by final extension at 72°C for 2 min. We verified PCR products with gel electrophoresis and purified products producing single bright bands of expected size using SV Wizard Gel and PCR clean up kit (Promega) according to the manufacturer’s protocol. PCR products were sequenced at Sequetech (Mountain View, CA) in both directions using PCR primers. We used resulting chromatograms (.ab1 files) in Geneious Prime (Biomatters) for all initial sequence processing. Sequences with a low percentage of high-quality bases (< 50%) were excluded from subsequent analysis. For included sequences, we trimmed off PCR primers and low-quality end-regions, aligned opposing strands, and manually resolved disagreements between 44 them to produce a consensus sequence. Nucleotide bases with combined Phred scores of < 20 were converted into “N”s in the consensus sequence or trimmed off. Subsequently, we translated each consensus sequence into amino acids using the Invertebrate Mitochondrial code and checked for the presence of stop codons. We used NCBI nucleotide BLAST search (GenBank) to screen for contamination and aid in species identification. The top 20 BLAST matches (based on highest pairwise identity to our specimens) were downloaded and included for subsequent analysis. The dataset was then pared to retain a single sequence per species/location and exclude sequences originating from beyond the Americas. Due to the appearance of morphological features commonly present in both Perkinsiana and Pseudopotamilla genera, sequences from both these genera were specifically included in phylogenetic analyses: the type species of Pseudopotamilla (P. reniformis (Bruguière 1789) and Perkinsiana fonticula (Hoagland 1919), both from their natural range of distribution. In addition, species of Eudistylia Bush, 1905 and Schizobranchia Bush, 1905 were also included since they constitute part of the apomorphic clade including Perkinsiana and Pseudopotamilla. Resulting sequences were aligned using the MAFFT plug-in in Geneious Prime using default parameters. The alignment was visually inspected for gaps and irregularities. The final COI alignment was trimmed to 594 bp and contained a total of 24 sequences (including seven generated in this study). The resulting alignment was used to construct a neighbor-joining tree (not shown) to evaluate pairwise diistances among sequences in the study. All original sequences produced in this study have been deposited in Barcode of Life Datsystems (BOLD) and GenBank (Table 3.1). We used MEGA X (ver.10.1.8): Molecular Evolutionary Genetics Analysis across computing platforms (Kumar et al. 2018) on the same alignment to determine the best fitting substitution model for the data (using “Find Best DNA/Protein Models ML”) and to estimate the 45 phylogeny using Maximum Likelihood. The best fitting model for the dataset was HKY+I, but not by a very wide margin, so we used the top six models to assess the resulting phylogeny’s sensitivity to the substitution model: HKY+I, HKY+G+I, TN93+I, TN93+G+I, GTR+I, GTR+G+I; (I = has invariant sites G = has a gamma distribution of the data). For each estimation we used 1,000 bootstraps, SPR (subtree pruning regrafting heuristic method) level 5, and a branch swap filter of “very strong.” For all other settings, we used the default. Table 3.1. Table of specimen IDs of Seepicola viridiplumi sp, nov. and BOLD accession numbers. Collection Location Latitude Longitude Depth (m) Sample ID BOLD Process ID Bush Hill 27.78237117 -91.50830855 543 BHSa26 GMSE004-24 BHSa46 GMSE005-24 BHSa68 GMSE006-24 BHSa70 GMSE007-24 Green Canyon 234 27.74614894 -91.22191704 538 GCSa44 GMSE008-24 GCSa47 GMSE009-24 GCSa49 GMSE010-24 46 3. RESULTS 3.1 Systematics Order SABELLIDA Latreielle, 1825 Family SABELLIDAE Latreille, 1825 Seepicola new genus Type species. Seepicola viridiplumi n. sp., herein designated, by monotypy. ZOOBANK RECORD: urn:lsid:zoobank.org:act:71A03636-1E5F-4734-85F1-C69906B4D666 DIAGNOSIS Medium-size species in the subfamily Myxicolinae with a moderate number of radioles arranged in semicircular radiolar lobes. Radiolar crown symmetrical with all radioles nearly same length. Radiolar crown with basal, dorsal and ventral flanges. Palmate membrane, radiolar flanges and radiolar eyes absent. Pinnules paired. Radiolar tips entire (unbranched). Dorsal lips with mid- rib (radiolar appendages) and dorsal pinnular appendages. Ventral lips and parallel lamellae present. Ventral sacs absent. Ventral peristomial chambers present, located between the ventral lappets and parallel lamellae. Peristomial loops absent. Peristomial eyes present. Collar chaetae narrowly hooded. Glandular ridge on chaetiger 2 absent. Ventral shields are well differentiated. Thoracic chaetae with a superior group of narrowly hooded chaetae, inferior group with paleate chaetae. Neurochaetae with tear-drop shaped companion chaetae and avicular uncini (teeth above main fang of equal size, hood absent, breast well developed, expanded, handles of medium length). Interamal eyespots absent. Abdominal chaetae elongate, broadly hooded (a basal broad knee and distal end narrowing abruptly sensu Knight-Jones 1983). Abdominal avicular uncini with teeth above the main fang of equal size, breast well developed, short handled. Pygidium without anal cirrus. Pygidial eyes absent. 47 ETYMOLOGY The genus name refers to the fact that the type species was found in hydrocarbon seeps (Seeps, combined with the Latin -cola = ‘dweller’). It should be regarded as invariant compound noun in apposition (Read et al. 2017; pg. 19). Seepicola viridiplumi sp. nov. Figures 1-10 ZOOBANK RECORD: urn:lsid:zoobank.org:act:78FAA822-18F2-4D0E-A31C-FA223BC469E6 TYPE MATERIAL: Holotype (CNAP–ICML, UNAM, 0000): BHSa144, Cruise Code TN391, 14 June 2021, 27.78237117, -91.50830855, 562 m, epibiotic on Acesta oophaga. Paratype 1 (CNAP–ICML, UNAM, 0000): BPSa115, Cruise Code AT50-04, 16 October 2022, 27.723677, -91.279372, 651 m, epibiotic on Acesta oophaga. Paratype 2 (CNAP–ICML, UNAM, 0000): BHSa167, Cruise Code TN391, 14 June 2021, 27.78237117, -91.50830855, 562 m, epibiotic on Acesta oophaga. Paratype 3 (UANL-0000): BPSa92, Cruise Code AT50-04, 16 October 2022, 27.723677, - 91.279372, 651 m, epibiotic on Acesta oophaga. Paratype 4 (UANL-0000): BHSa127, Cruise Code AT50-04, 15 October 2022, 27.723677, - 91.279372, 562 m, free-living in authigenic carbonate. 48 Paratype 5 mounted in stubs 1 and 2 for SEM (CNAP–ICML, UNAM, 0000): BPSa88, Cruise Code AT50-04, 16 October 2022, 27.723677, -91.279372, 651 m, epibiotic on Acesta oophaga. Paratype 6 mounted in stubs 4 and 5 for SEM (CNAP–ICML, UNAM, 0000): BPSa123, Cruise Code AT50-04, 16 October 2022, 27.723677, -91.279372, 651 m, epibiotic on Acesta oophaga. DIAGNOSIS Radiolar crown symmetrical with all radioles nearly same length, except 2-3 ventral-most developing radioles that are shorter than the dorsal radioles. Radiolar tips variable: long-filiform or short button-like. Those radioles with short tips have a massive, unknown brown tissue along their internal margins. Peristomial chambers ventrally located between the ventral lappets and parallel lamellae. Anterior peristomial ring is slightly exposed dorso-laterally between dorsal pockets and the lateral collar margin. Mid-dorsal collar margins fused to fecal groove. DESCRIPTION Gregarious, facultative hyper-epibiotic sabellid with individuals found free-living in authigenic carbonate cements and on the file clam Acesta oophaga Järnegren, Schander, and Young, 2007 (Figure 3.1). Commonly found at depths between 562 and 651 meters. Radiolar crowns a soft green and body a cream to red-brown color in live worms. Preserved worms have a dark to pale cream colored body with radiolar crowns appearing whitish. Radiolar crown length is 7.2 mm (4 – 7.5 mm) with 12 pairs of radioles (all paratypes with 12 pairs). Trunk length is 39 mm (28 – 32 mm) with a body width of 2.5 mm (1.4 – 2 mm). Thoracic segments number 15 (13 – 18) with 121 abdominal chaetigers (97 – 143). 49 Figure 3.1. In situ images of Seepicola viridiplumi sp. nov. A) Epibiotic individuals on a host Acesta oophaga file clam. Red-pink plumes belong to the siboglinid tube worm Lamellibrachia luymesi. B) Close up of free-living individuals and plumes on authigenic carbonate. C) Aggregation of individuals on authigenic carbonate. D) Tube of Seepicola viridiplumi sp. nov. with a muddy outer lining and a curled end. Scale bar represents 2 mm. 50 Radiolar crown is mostly symmetrical (Figure 3.3B) with the 2 – 3 ventral-most developing radioles with long, filiform radiolar tips as long as the space of 12 pinnules (Figure 3.4A). These are 1/8 the length of the dorsal radioles. Radiolar lobes are short, as long as the collar segment (Figure 3.2A – C), with dorsal flanges. The dorsal pair of basal flanges is long, narrow, erect, and translucid (Figure 3.2C, E, 4A) and the ventral pair is short, broad, has a rounded margin, and is translucid (Figures 3.2D, 3D, 4A). Radiolar flanges and palmate membrane is absent (Figure 3.2D). Pinnules are very long, of a similar length along the radioles. Radiolar eyes are absent. Except for the ventral-most radioles, the radioles of the holotype have button-like tips and are as short as the space of one pinnule (Figure 3.4B). The radioles with short tips have a massive brown tissue along their internal margins (Figures 3.4C – H). Near the radiolar tip this tissue is broader than that basally, forming a rounded tip that seems like a distal radiolar eye, but this structure lacks ommatidia (Figure 3.4D – G). Some paratypes have mixed radiolar tips (long-filiform, short button-like). Radiolar skeleton is composed of 4 cells in side view (Figure 3.4E, H). Apparently, the crown of paratype 1 (BPSa115) is undergoing regeneration: it is shorter in comparison to the holotype and other paratypes, and the pinnules are incipient. 51 Figure 3.2. Seepicola viridiplumi sp. nov. A) Radiolar crown and thorax, dorsal view. B) Thorax and base of radiolar crown, ventrolateral view. C) Thorax and base of radiolar crown, dorsal view. D) Detail of the dorsal basal flange of the radiolar crown. E) Detail of the dorsal basal flange of the radiolar crown. A-E) Holotype (CNAP–ICML, UNAM, 0000). Abbreviations: bdf = basal dorsal flange, vbf = ventral basal flange. Scale bars: A) 1 mm, B-E) 0.8 mm. 52 Figure 3.3. Seepicola viridiplumi sp. nov. A) Collar, ventral view with the right radiolar lobe removed. B) Radiolar crown, lateral view. C) Base of the right radiolar lobe. D) Detail of the dorsal lip and ventral basal flange of the radiolar crown. E) Posterior end and pygidium. F) Peristomium, frontal view with the radiolar crown removed, peristomial chambers indicated with arrows. G) Detail of the mouth and peristomial chambers pointed with arrows. A, C, F-G) Paratype 3, B, D-E) Holotype (CNAP–ICML, UNAM, 0000). Abbreviations: d = dorsal, dl = dorsal lip, pl = parallel lamella, v = ventral, vbf = ventral basal flange. Scale bars: A-C) 1 mm, D-E, G) 0.5 mm, F) 1.5 mm. 53 Figure 3.4. Seepicola viridiplumi sp. nov. A) Base of the radiolar crown, lateral view (Paratype 2). B) Radiolar tips. C – G) Details of the radiolar tips showing cartilaginous skeletal cells and massive tissue on the inner margin of the radioles, attached to the base of the pinnules. H) Detail of radiolar and pinnular skeletal cells. A) Holotype (CNAP– ICML, UNAM, 0000), B-H) Paratype 1 (CNAP–ICML, UNAM, 0000). Abbreviations: d = dorsal, v = ventral, rt = radiolar tips. Scale bars: A) 1 mm, B-G) 150 μm, H) 75 μm. 54 The anterior peristomial ring is slightly exposed dorso-laterally between dorsal pockets and the lateral collar margin (Figures 3.2E, 7A). The posterior peristomial ring collar has mid-dorsal margins fused to fecal groove (Figures 3.2E, 7A) and the dorsal collar margins form two low, rounded lappets (Figure 3.2A, C). The dorso-lateral collar margins are entire, forming a “V” (Figure 3.2A, C, E). Ventral lappets are triangular with rounded distal margins that are divided mid-ventrally by an incision (Figures 3.2D, 3A, 7A). Parallel lamellae are present, forming a triangular structure surrounding the mouth ventrally (Figures 3.3A, F – G, 3.7A). A pair of translucent chambers lies between the ventral lappets and parallel lamellae, with brown spots inside (Figures 3.3A, F – G, 3.7A-B). Peristomial eyes are seen in paratypes 1 (BPSa115) and 2 (BHSa167) when radiolar crowns were removed (Figure 3.3F). The dorsal lips are triangular, erect, and have a mid-rib (radiolar appendages) (Figure 3.3A, C – D) and dorsal pinnular appendages; ventral lips are short and rounded, ventral sacs are absent. Chaetiger 1 (collar chaetiger): two groups of hooded chaetae (Figures 3.6A-C, 3.7A, C), the anterior one with long, narrowly hooded notochaetae (Figures 3.6A-B, 3.7C), and the inferior one half as short than the superior one with hoods slightly broader than the superior group (Figures 3.6C, 3.7C). The ventral shield is rectangular, slightly divided transversally, and higher than the following thoracic shields (Figure 3.3A). Chaetigers 2 – 16 (2 – 13, 2 – 15, 2 – 16, or 2- 18) have rectangular ventral shields divided transversally in two equal parts; the tori do not contact the ventral shields (separated by a reduced space) (Figures 3.2B, 3.3A). Chaetigers have noto- and neurochaetae (Figure 3.5A). Notochaetae have two groups (Figure 3.5C, 3.8A): superior group are elongate and narrowly hooded; inferior ones paleate and arranged in two rows with pointed mucro (Figure 3.5D, 3.8A-C). Neurochaetae with companion chaetae and avicular uncini (Figure 3.5A – B, 3.8E-F). Avicular uncini have several rows of small, similar sized teeth above the main fang 55 (covering half of the main fang) (Figure 3.8D), the breast is well developed with a high crest above the main fang and handles as long as 2.5 times the length of the main fang (or half of handles of companion chaetae) (Figure 3.5E – F). The companion chaetae have symmetrical membranes and are teardrop-shaped (Figures 3.5B, E, 3.8E-F) with long handles (Figure 3.5A, E). Abdominal segments with elongate neurochaetae and broadly hooded (Figures 3.6A-D, 3.9A), with a basal, broad knee and the distal end narrowing abruptly in all chaetigers (Figures 3.6E, 3.9F). Those from the last quarter of the body are very long (twice as long as those in the anterior abdominal segments) (Figure 3.9B). Notopodial uncini are avicular with several rows of teeth above the main fang and extending over ¾ of the main fang (Figure 3.9C, E-G). The breast is well defined, and the handles are very short, shorter than the length of the main fang (Figure 3.6F – H). The pygidium is rounded and without eyes (Figure 3.3E). The tubes are composed of fine sand and curl tightly at the end (Figure 3.1D). Gametes were not observed in either the holotype or the paratypes. 56 Figure 3.5. Seepicola viridiplumi sp. nov., thoracic chaetae. A) Thoracic noto- and neurochaetae. B) Companion chaetae. C) Notochaetae. D) Inferior rows of paleate chaetae. E). Avicular uncini and companion chaetae. F) Detail of heads (main fangs) of uncini. A-F) Holotype (CNAP–ICML, UNAM, 0000). Magnification: A) 4 x, B, D-E) 40 x, C) 10 x, F) 100 x. 57 Figure 3.6. Seepicola viridiplumi sp. nov., collar and abdominal chaetae. A) Collar chaetigers (chaetigers 1). B) Superior group of collar chaetigers composed of elongate, narrowly hooded and slightly curved chaetae. C) Inferior group of collar chaetigers composed of elongate, hooded chaete broader than the superior group. D) Abdominal chaetae. F) Abdominal torus of avicular uncini. G) Details of uncini in side view. A-H) Holotype (CNAP–ICML, UNAM, 0000). Magnification: A) 10 x, B-H) 40 x. 58 Figure 3.7. Seepicola viridiplumi sp. nov. Scanning electron microscopy of peristomium. A) Apical view of peristomium (crown removed) and vascular chambers pointed with white arrows, B) detail of vascular chambers between right ventral lappet of collar and parallel lamella, C) collar chaetiger with two groups of elongate narrowly hooded chaetae. A-B) Stub 1, C) Stub 2 (BPSa88, CNAP–ICML, UNAM, 0000). Abbreviations: apr: anterior peristomial ring, d: dorsal, fg: faecal groove, pl: parallel lamellae, pprc: posterior peristomial ring collar, v: ventral, 1, 2 and 3 in A indicates number of chaetigers. Scale bars: A) 500 μm, B) 200 μm, C) 100 μm. 59 Figure 3.8. Seepicola viridiplumi sp. nov., thoracic chaetae and uncini under SEM. A) Chaetiger #2, B) chaetiger #5, C) detail of paleate chaetae from chaetiger #5, D) dentition of uncini from chaetiger #5, E) torus 5, F) detail of companion chaetae from chaetiger # 5. A) Stub 1 (BPSa88, CNAP–ICML, UNAM, 0000), B-C) Stub 5 and D-F) Stub 4 (BPSa123, CNAP–ICML, UNAM, 0000). Scale bars: A) 200 μm, B) 100 μm, C) 50 μm, D) 20 μm, E) 100 μm, F) 50 μm. 60 Figure 3.9. Seepicola viridiplumi sp. nov., abdominal chaetae and uncini under SEM. A) Anterior abdominal chaetiger, B) posterior abdominal chaetiger, C) anterior abdominal torus, D) detail of chaetae from anterior abdomen, E, G) uncini dentition, F) detail of broadly hooded chaetae. A-B, D, F) Stub 4 (BPSa123, CNAP–ICML, UNAM, 0000), C, E, G) Stub 2 (BPSa88, CNAP–ICML, UNAM, 0000). Scale bars: A-B, D) 200μm, C) 50 μm, E) 20 μm, F) 100 μm, G) 8 μm. 61 GLANDULAR PATTERN The ventral shield of the collar, thoracic and abdominal shields stained a deep, uniform blue (Figures 3.2B, 3.3A, E). ETYMOLOGY The species epithet refers to the color of the radiolar crown in living specimens, from the Latin viridi, meaning green and -plumi, meaning many plumes. REMARKS Placing the taxon described here in either Pseudopotamilla Bush, 1905 or Perkinsiana Knight-Jones, 1983 is a difficult task when morphology is first examined. The specimens described here from hydrocarbon seep habitats in the Gulf of Mexico have dorsal and ventral basal flanges at the base of the radiolar crown, such as is described in Pseudopotamilla. However, it lacks the remarked compound radiolar eyes and the asymmetrical radiolar crown common in Pseudopotamilla species (Table 2). On the other hand, the genus Potamilla Malmgren, 1866 also lacks radiolar eyes (Knight-Jones 1983, Fitzhugh 1989). Our specimens cannot be attributable to Potamilla because these have dorsal lips elongate, triangular, with mid-rib (radiolar appendages) and lacks a palmate membrane, whereas Potamilla have dorsal lips without radiolar appendages, but a palmate membrane is present, among other differences (Table 3.2). Regarding the genus Perkinsiana, some authors already commented on the existing problems. Fitzhugh (1989) emphasized that Perkinsiana Knight-Jones, 1983 is not a definable group as there is no evidence to support monophyly. Capa (2007) and Tovar-hernández et al. (2012) both described new species of Perkinsiana and remarked on the existing problem of properly assigning species to this genus. In the same context, Pseudopotamilla is not defined by any synapomorphies (Fitzhugh 1989, Capa 2007). In both genera, species are known to burrow in 62 hard limestone, dead coral, barnacles, and mollusk shells (Chughtai & Knight-Jones 1988, Knight- Jones et al. 2017, Capa et al. 2019, Tovar-Hernández et al. 2020). There are 18 valid described species in Perkinsiana and 23 in Pseudopotamilla after Tovar-Hernández et al. (2020), but the status of some nominal species in the latter genus are still questionable. Our specimens lack the palmate membrane and radiolar flanges present in some Perkinsiana species. Additionally, our specimens had abdominal uncini with reduced handles whereas these structures are short to medium length in Perkinsiana. Three types of abdominal chaetae can be present in species of Perkinsiana whereas these are elongate, broadly hooded chaetae in all chaetigers of the new taxon here described. Furthermore, the new species described here have unique, distinctive features not previously described: the peculiar shape of the radiolar tips, the presence of the brown tissue on the radioles, and the presence of a pair of peristomial chambers between the internal wall of ventral lappets and parallel lamellae. Other features of chaetae and uncini are typical of Pseudopotamilla. As the new species here described, some species of Pseudopotamilla also have tubes curl tightly at the end (Knight-Jones et al. 2017), but branched or bifurcated tubes were not seen in the specimens here examined, which is indication of asexual reproduction. Table 3.2. Distinctive features of the genera Perkinsiana Knight-Jones, 1983, Potamilla Malmgren, 1866, Pseudopotamilla Bush, 1905 and Seepicola new genus. Feature Perkinsiana Knight-Jones, 1983 sensu a variety of author as specified in each feature Potamilla Malmgren, 1866 sensu Fitzhugh, 1989 Pseudopotamilla Bush, 1905 sensu Knight- Jones et al. 2017 Seepicola new genus Radiolar crown Symmetrical with most radioles same length (except 2-3 ventral-most developing radioles)(Tovar-Hernández, obs. pers.) ? Asymmetrical with longest radioles dorsally Symmetrical with all radioles same length (except 2-3 ventral-most developing radioles) Dorsal and ventral basal flanges of crown Absent (Tovar-Hernández et al. 2012, Capa et al. 2019) Absent Present Present Palmate membrane Absent (Fitzhugh, 1989, Capa, 2007); present or absent (Tovar-Hernández et al. 2012, Capa et al. 2019) Present Absent Absent 64 Radiolar flanges Absent (Fitzhugh, 1989, Capa, 2007); absent or present (Tovar-Hernández et al. 2012) Absent Absent Absent Radiolar eyes Absent Absent Present, unpaired, compound in all radioles except dorsal most pair and some ventral most radioles, usually limited to proximal half of radioles Absent Peristomial eyes Present in juveniles (Capa et al. 2019 ? May be present Present Mid-rib of dorsal lips (radiolar appendages) Present (Fitzhugh, 1989, Capa 2007, Tovar-Hernández et al. 2012, Capa et al. 2019) Absent Present Present Dorsal pinnular appendages Present (Fitzhugh, 1989); present or absent (Capa 2007, Tovar-Hernández et al. 2012, Capa et al. 2019) Present Present Present 65 Ventral lips Present (Fitzhugh, 1989, Capa 2007, Tovar-Hernández et al. 2012, Capa et al. 2019) Present Present Present Parallel lamellae Present (Fitzhugh, 1989, Capa 2007, Tovar-Hernández et al. 2012, Capa et al. 2019) Present Present Present Ventral sacs Absent (Capa 2007, Tovar- Hernández et al. 2012, Capa et al. 2019) ? Present Absent Peristomial chambers Never reported Never reported Never reported Oval, translucent with a brown spot inside Anterior margin of anterior peristomial ring Low, of even height all around (Fitzhugh, 1989, Capa 2007, Tovar-Hernández et al. 2012) Low, of even height all around Low, of even height all around Low, of even height all around 66 Collar chaetae Arranged in oblique rows, similar to superior notochaetae of following chaetigers (elongate, narrowly hooded) (Capa 2007, Tovar-Hernández et al. 2012, Capa et al. 2019) ? Similar to superior notochaetae of following chaetigers (elongate, narrowly hooded) Two groups of hooded chaetae, the anterior one with long, narrowly- hooded chaetae, and the inferior one half as short than the superior one with hoods slightly broader than the superior group Inferior thoracic notochaetae Paleate, arranged in two or more transverse rows (Fitzhugh, 1989, Capa 2007, Tovar-Hernández et al. 2012) Paleate, arranged in two or more transverse rows Paleate, arranged in two or more transverse rows Paleate, arranged in 2-3 transverse rows Thoracic uncini (avicular) Teeth above main fang of equal size, hood absent, breast well developed, expanded; handles of medium length (Fz, 1989); handles of variable length (Capa 2007, Tovar-Hernández et al. 2012, Capa et al. 2019) Teeth above main fang of equal size, hood absent, breast well developed, expanded; handles of medium length Teeth above main fang of equal size, hood absent, breast well developed, expanded; handles of medium length Teeth above main fang of equal size, hood absent, breast well developed, expanded; handles of medium length 67 Companion chaetae Distal ends as roughly symmetrical, tear-drop shaped membranes (Fitzhugh 1989, Capa 2007, Tovar- Hernández et al. 2012, Capa et al. 2019) Distal ends as roughly symmetrical, tear- drop shaped membranes Distal ends as roughly asymmetrical, tear-drop shaped membranes Distal ends as roughly asymmetrical, tear-drop shaped membranes Abdominal uncini (avicular) Teeth above the main fang of equal size; breast well developed, expanded; long handled (Fitzhugh, 1989); short to medium length handle (Capa 2007, Tovar- Hernández et al. 2012) Teeth above the main fang of equal size; breast well developed, expanded; long handled Teeth above the main fang of equal size; breast well developed, expanded; medium handled Teeth above the main fang of equal size; breast well developed; short handled 68 Abdominal chaetae Elongate, broadly hooded chaetae in all chaetigers (Fitzhugh, 1989, Capa, 2007). Broadly-hooded and progressively tapering to distal tip (type A), or elongate broadly-hooded chaetae (type B), or elongate, narrowly- hooded chaetae (type C) (Tovar-Hernández et al. 2012). Anterior abdominal segments with broadly hooded chaetae and posterior segments with elongate, narrowly hooded chaetae (Capa et al. 2019) Elongate, broadly hooded chaetae in all chaetigers Elongate, broadly hooded chaetae in all chaetigers Elongate, broadly hooded chaetae in all chaetigers, but those from the last abdominal quarter being longer than anterior abdominal segments 69 3.2 Phylogenetic Analysis All phylogenetic estimations recovered the same topology with very minor variations in boostrap support for some clades. All of them recover a clade comprised of only specimens in this study with a high degree of confidence (100% bootstrap support, and less than 1% divergence among all sequences). We present the tree produced using the HKY+I model of sequence evolution as it was the best fitting model for the data (Figure 3.10). The phylogeny suggests that Seepicola viridiplumi sp. nov. is distantly related to the closest sequences in reference databases (Genbank, BOLD; with only 70-75% similarity), which is perhaps not surprising given the paucity of data from sabellids collected in similar habitats and depths. A clade comprised of Seepicola new genus, Eudistylia and Schizobranchia is recovered with low bootstrap support (65%) so is not informative about how the genus is related to other sabellid genera, except that it is distantly related to those in this study. These results provide strong evidence that the specimens collected in this study are unique (at least among the barcoded sabellids) and thus constitute a new genus. The phylogeny and distance calculations also show that the species here is not closely related to either Pseudopotamilla reniformis (27% sequence divergence) or Perkinsiana fonticula (30% divergence), despite the morphological similarities outlined above. 70 Figure 3.10. Maximum Likelihood (ML) tree showing the phylogenetic relationships between Seepicola viridiplumi sp. nov. and four other Sabellidae genera. Numbers refer to bootstrap support (%). The first phylogenetic approach of Sabellidae nested the genera Potamilla, Perkinsiana, Potaspina, Pseudopotamilla, Eudistylia, and Schizobranchia within the “Clade VII” based on morphology (Fitzhugh, 1989). This “Clade VII” resulted monophyletic based on the occurrence of 71 dorsal pinnular appendages and elongate, broadly hooded chaetae in all abdominal fascicles. Potamilla, Potaspina and Perkinsiana formed a polygamy with the Clade Pseudopotamilla- Eudistylia-Schizobranchia, which was defined by the presence of unpaired compound radiolar eyes and dorsal basal flanges of crown (Fitzhugh, 1989). Posteriorly, that group ( “Clade VII” sensu Fitzhugh, 1989) was recovered in a combined analysis using morphological and molecular data, called "clade IB” that includes many other genera, supported by the presence of companion chaetae in thorax and broadly hooded abdominal chaetae (Capa et al. 2011). More recently, using transcriptomes, Eudistylia and Pseudopotamilla were nested within the Tribe Amphiglenini, Subfamily Myxicolinae according to Tilic et al. (2020), which is equivalent to the “clades V, VI and VII" by Fitzhugh (1989) and “Clade IB” by Capa et al. (2011). Under this scenario, Seepicola new genus would belong to the Amphiglenini Tribe, Myxicolinae subfamily. 3.3 Species Abundance Measures The density of the sabellids was variable within the seep systems. From the analysis of ROV images, sabellid density within the seep systems averaged 330 ± 233.3 (stdev) m-2 but ranged from 98 to 655 individuals m-2 within the authigenic carbonate. Sabellid density was most concentrated at vertical facies on authigenic carbonate outcrops and more dispersed on horizontal surfaces (Figure 3.1C). Occasionally, individuals were observed on deposits of shell hash. In situ observations and video footage showed that the sabellid aggregations at each of the collection sites were composed of specimens of varying sizes and likely belonged to younger (shorter sabellid tubes) and older (taller) individuals. Observed sabellid tubes ranged from approximately 4 mm to 72 104 mm and were intermingled within the aggregations. The aggregations at Bush Hill appeared to be more extensive than at Brine Pool NR1 and Green Canyon 234, although this could not be quantified. This difference likely corresponds to the abundance of exposed authigenic carbonate at Bush Hill. Epibiotic Seepicola viridiplumi sp. nov. also had varying densities on host Acesta oophaga file clams. While several A. oophaga bore only a single sabellid, one file clam 10 cm long and 8 cm across, collected from Bush Hill, had a total of 58 individual sabellids. 4. DISCUSSION This study expands the number of sabellid species known from chemosynthetic habitats and identifies a species of high abundance at some of the best described hydrocarbon seeps (Cordes et al. 2009). Seepicola viridiplumi sp. nov. is the third to be identified from chemosynthetic habitats and helps to elucidate the diversity of sabellid polychaetes from these environments. Several species of sabellid polychaetes are known to form dense aggregations similar to Seepicola viridiplumi sp. nov. (Capa et al. 2019), and this may impact ecological aspects of the hydrocarbon seep habitat. Gregarious sabellid species such as Bispira riccardi have been found to significantly increase local meiofaunal diversity and abundance (Enrichetti et al. 2022). Suspension feeding organisms, such as sabellid polychaetes, also