Canadian Journal of Zoology

The life history and feeding ecology of velvet shell, velutina (: ), a specialist predator of ascidians

Journal: Canadian Journal of Zoology

Manuscript ID cjz-2018-0327.R1

Manuscript Type: Article

Date Submitted by the 03-Jun-2019 Author:

Complete List of Authors: Sargent, Philip; Northwest Atlantic Fisheries Centre, Fisheries and Canada Hamel, Jean-Francois; Society for the Exploration and Valuing of the EnvironmentDraft Mercier, Annie; Memorial University of Newfoundland, Sciences

Is your manuscript invited for consideration in a Special Not applicable (regular submission) Issue?:

Velutina velutina, velvet shell, velutinid, gastropod, invasive , Keyword: specialist predator, ascidian

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The life history and feeding ecology of velvet shell, (Gastropoda: Velutinidae), a specialist predator of ascidians

P. S. Sargent*, J-F. Hamel, and A. Mercier

P. S. Sargent1 Department of Ocean Sciences, Memorial University, St. John’s (Newfoundland and Labrador) Canada A1C 5S7 Email: [email protected]

J-F Hamel Society for the Exploration and ValuingDraft of the Environment (SEVE), Portugal Cove-St. Philips (Newfoundland and Labrador) Canada A1M 2B7 Email: [email protected]

A. Mercier Department of Ocean Sciences, Memorial University, St. John’s (Newfoundland and Labrador) Canada A1C 5S7 Email: [email protected]

* Corresponding Author: Philip S. Sargent Department of Fisheries and Oceans Canada, Northwest Atlantic Fisheries Centre,

80 East White Hills Road, St. John’s, Newfoundland and Labrador, Canada, A1C 4N1

Email: [email protected] Phone: 1 (709) 772-4278 Fax: 1 (709) 772-5315

1 Current Contact Information for P. S. Sargent: Department of Fisheries and Oceans Canada, Northwest Atlantic Fisheries Centre, 80 East White Hills Road, St. John’s, Newfoundland and Labrador, Canada, A1C 4N1 Email: [email protected]

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The life history and feeding ecology of velvet shell, Velutina velutina

(Gastropoda: Velutinidae), a specialist predator of ascidians

P. S. Sargent*, J-F. Hamel, and A. Mercier

Abstract

Velvet shell, Velutina velutina (O. F. Müller, 1776), is a specialist predator of ascidians, like other members of the gastropod family Velutinidae. Globally, invasive ascidians have become problematic, ecologically and economically, yet ecological knowledge of velutinids remains limited. This study outlines the life history and feeding ecology of V. velutina in eastern CanadaDraft based on laboratory work complemented by field observations. The life history of V. velutina is closely linked with ascidians, which serve as prey and protection for their egg capsules. Egg capsules were embedded within tunics of Aplidium glabrum (Verrill, 1871) and Ascidia callosa Stimpson, 1852, but the latter was preferred. Seasonal behavioural shifts were consistent annually and corresponded with seawater temperature cycles. Feeding dominated during the coldest months (January – May), growth occurred as water temperature increased to the annual maximum (June and July), transitioned to mating during the warmest period

(July/August), and egg capsule deposition dominated as water temperature declined

(November – January). Larvae hatched between January and July after 2 – 4 months of development. Velvet shell preyed on all ascidian species presented during this study, including golden star , Botryllus schlosseri (Pallas, 1766), and vase tunicate,

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Ciona intestinalis (Linnaeus, 1767), two non-indigenous species, although solitary

species were preferred.

Keywords Velutina velutina, velvet shell, velutinid, gastropod, invasive species, specialist predator,

ascidian

Introduction

Members of the gastropod family Velutinidae (formerly Lamellariidae) are

specialized predators of ascidians that closely associate with their prey (Fretter and

Graham 1962; Ghiselin 1964; Behrens 1984; Dias and Delboni 2008) and deposit their egg capsules within the tunic of ascidiansDraft (Diehl 1956; Strathmann 1992; Page 2002; Dias and Delboni 2008). The close association of velutinids and ascidians has even been

described as a symbiotic (sensu lato) relationship (Queiroz and Sales 2016).

Available literature on velutinids consists primarily of anatomical and

taxonomical descriptions (e.g. Gulbin and Golikov 1997; 1999), observational references

to biogeography, depth distributions, and habitat associations (e.g. Fretter and Graham

1981; Gulbin 2005). Scarcity of ecological and biological information on velutinids may

be due in part to their cryptic nature and the fact that few specimens have ever been

collected (Lambert 1980). The of most velutinid species partially or completely

covers a thin and weakly calcified shell (Gulbin and Golikov 1997) and often mimics the

colour and texture of the tunic of ascidians (Ghiselin 1964; Lambert 1980; Behrens

1984). This renders velutinids almost indistinguishable from their prey (Ghiselin 1964;

Behrens 1980; Lambert 1980). Furthermore, velutinids are commonly misidentified as

dorid nudibranchs (Jeffreys 1867; Behrens 1984; Dias and Delboni 2008) and some

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species are nocturnal, remaining concealed during the day (Sarma and Pattanaik 1986). In

general, our understanding of the ecological role of velutinids in subtidal communities is

limited.

The velvet shell, Velutina velutina (O. F. Müller, 1776), is one of the most

common and widely distributed velutinid species in northern seas (Derjugin 1950). It is a

sublittoral species with a boreal-arctic distribution (Gulbin and Golikov 1999; Gulbin

2005) found to depths of 1000 m (Fretter and Graham 1981; Gulbin 2005). In the

northwest Atlantic, this species extends from the Arctic to as far south as Cape Cod

(Massachusetts, USA) but becomes increasingly rare and occurs deeper towards its

southern range (Fretter and Graham 1981). Members of the Velutina have an

external shell and the mantle may onlyDraft cover a portion of the shell’s surface along the

edge of the (Fretter and Graham 1981). To our knowledge, the only ecological

studies of V. velutina were conducted in northern Europe and examined predation on and

egg deposition in the ascidian Styela coriacea (Alder and Hancock, 1848) (Diehl 1956),

copulation (Diehl 1956), and planktonic larval development (Lebour 1935; Thorson

1946; Mileikovsky 1960; Fretter and Pilkington 1970; Thiriot-Quiévreux 1974).

A better understanding of the ecology of velutinids would not only increase our

knowledge of this poorly understood gastropod family but may also be relevant to the

control of some aquatic invasive species. Non-indigenous ascidians have proven to be

very successful invasive species globally (Lambert 2007). Invasive ascidians may have

significant impacts both ecologically, by altering community structure (Lambert and

Lambert 2003; Valentine et al. 2007), and economically, by fouling man-made structures, especially shellfish aquaculture infrastructure (Carver et al. 2003; LeBlanc et al. 2007;

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Rocha et al. 2009). Yet, knowledge of biotic resistance of benthic marine communities to

such invasions is lacking (Lambert 2007; Epelbaum et al. 2009). Determining the

response of benthic communities to invasive species (e.g. presence and role of potential

predators such as velutinids) is crucial to understand and mitigate species invasions.

The purpose of the present study was to investigate the life history and feeding

ecology of V. velutina and provide insight into the role of velutinids within the subtidal

communities they inhabit. It combined laboratory studies complemented by field

observations to determine diet and feeding habits (preferences, rates, and periodicity) as

well as seasonal behavioural patterns. Mating, egg laying, larval development and

hatching were characterized and the role of environmental factors in the control of these

behaviours were also examined. As Drafta specialist predator of ascidians, V. velutina may

represent a natural means of mitigating the impacts of some non-indigenous ascidians.

Materials and methods

Collections and field sites

Most field observations and collections of V. velutina were made

opportunistically (77.8% of dives) while conducting dives for other purposes. Field

observations of habitat associations and behaviours of V. velutina were recorded2 and

used to complement observations recorded in the laboratory. Over the course of 41 dives

(mean = 36 min dive time) conducted between November 2005 and August 2011 around

insular Newfoundland, 105 velutinids were observed and 75 individuals were collected

and transferred to Memorial University’s Oceans Science Centre3. Five additional

2 as per Table S1 and S2, respectively 3 Tables S1 and S3

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6 individuals were collected over four dives between March and May 2017 (mean = 44 min dive time) and transferred to the Northwest Atlantic Fisheries Centre3. In 2006 and 2007, samples of callused tunicate, Ascidia callosa Stimpson, 1852, were collected from two sites4 and examined for the presence of developing or previously hatched egg capsules and settled larvae of V. velutina.

Holding conditions and maintenance

Unless otherwise stated for specific experiments, velutinids were maintained in laboratory microcosms consisting of tanks (23 and 40 L) supplied with flow-through unfiltered seawater (1.5 – 3.0 L min-1) at ambient temperature under either natural or fluorescent lighting (25 – 70 lux) set on timers to follow the natural daylight cycle.

Seawater temperature in tanks was recordedDraft on a daily to weekly basis. An inline chiller was used between July and October to maintain temperature below 14 °C, as observed in their natural habitat.

Velutinids (juveniles and adults) were provided various ascidian species ad libitum. Based on availability, velutinids were maintained primarily on pyriformis (Rathke, 1806) with opportunistic additions of other indigenous species, including Aplidium glabrum (Verrill, 1871), Didemnum albidum (Verrill, 1871), Ascidia callosa Stimpson, 1852, echinata (Linnaeus, 1767), Molgula citrina Alder and

Hancock, 1848, and Molgula griffithsii (MacLeay, 1825). Pieces of encrusting algae, including Lithothamnion glaciale Kjellman, 1883 and Clathromorphum compactum

(Kjellman) Foslie, 1898, and pieces of shale rock, encrusted with L. glaciale, were placed in tanks for shelter.

4 Table S3

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Feeding

General feeding behaviour

Feeding behaviour was recorded weekly from April 2006 to June 2011.

Observations of velutinids were classified5 and feeding positions on ascidians were

confirmed by the presence of feeding holes. Approximate length of proboscis relative to

shell length of feeding velutinids was noted.

To examine fine-scale behavioural shifts, as well as length of time spent feeding

on ascidians, complementary daily observations (from September 2008 to September

2009) were made on five isolated adult velutinids fed the following ad libitum: Aplidium

glabrum, Ascidia callosa, Boltenia echinata, Halocynthia pyriformis, and Molgula

citrina. Intervals between feeding bouts,Draft and number of ascidians consumed over time

were recorded. Some ascidian prey where dissected to assess the proportion of remaining

tissues/organs (n = 16) while others were retained to assess mortality rates from predation

events (n = 8).

Prey preferences: feeding experiments

A series of feeding experiments were conducted in the laboratory to test the null

hypothesis that V. velutina exhibits no preferences among available ascidian prey species

(see Table 1). For experiments with non-indigenous ascidian species, every 1 – 3 d up to

30% of water and all wastes from tanks were removed and bleached for 24 h before being

discarded, to avoid propagation. Before each experiment, ascidians were acclimated for 2

– 3 d and velutinids were introduced after being starved for 4 d to standardize hunger

levels. When predation was suspected, velutinids were removed from ascidians for

5 Table S2

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8 confirmation and thereafter replaced haphazardly in their tank. Confirmation of a predation event was recorded when a hole was drilled through the tunic.

Growth

Shell length (SL) of 42 velutinids (mean initial SL = 15.7 mm, range = 6.7 – 24.2 mm) was measured monthly from October 2007 to January 2010 as the maximal shell diameter to the nearest 0.1 mm to examine seasonal growth patterns.

Mating and egg laying

Interactions between individual V. velutina6 were recorded weekly in the laboratory. Grouped or paired individuals were examined for copulation, and whether they were acting as males, females, or both simultaneously. Copulation was described based on 81 observed copulation eventsDraft from July 2006 to December 2008. Egg laying and associated behaviours were recorded weekly in the laboratory. Numbers of intact and hatched egg capsules were also recorded in the laboratory to estimate the total number of capsules deposited annually per velutinid. Complementary data were gathered from 5 isolated adult velutinids from September 2008 to September 2009 to examine behavioural responses and preferences for egg laying in different ascidian species (Ascidia callosa,

Molgula citrina, Boltenia echinata, and Aplidium glabrum). Relative position and behaviour of individual velutinids were recorded every 1 – 4 d, while number of egg capsules laid by each velutinid, and in which ascidian species, were recorded weekly.

Larval development, hatching, and settlement

Egg capsules of V. velutina laid in the laboratory and collected from the field were sampled periodically throughout their development (from initial deposition to

6 as defined in Table S2

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hatching). To examine developing larvae, the cap was removed from each capsule and

larvae were extracted with a pipette, counted, and photographed using a stereomicroscope

(Nikon SMZ1500). Egg capsules deposited in the laboratory were counted and examined

weekly for signs of hatching. Dates of when capsules first started hatching and when the

last egg capsule hatched were recorded. Observations of veliger larvae naturally hatching

from capsules were recorded on two occasions and information on larval behaviour was

noted. Observations of settled larvae from ascidians collected in the field were also

reported.

Seasonal behaviour

Seasonal behavioural patterns were determined by recording weekly relative

position in the tank and behaviour ofDraft individual V. velutina7 between October 28, 2006

and May 3, 2009. During that period the mean number individuals in the tank was 18 but

ranged from a high of 30 individuals in 2007 to a low of 5 individuals at the end in 2009.

Velutinids were numbered with India ink on their dorsal shell surface to track them

individually. As ink labels faded over time, they were retraced as necessary.

Statistical analysis

Prey preference results were scored as presence/absence of a predation event on

each species. Choices among native species and between B. schlosseri and native species

were analysed using generalized linear models (GLM) with binomial distributions and

logit links. Results for the pairwise feeding experiment with C. intestinalis were analyzed

using a GLM with a binomial distribution. Monthly shell growth was compared against

monthly change in water temperature using a GLM. GLMs and ANOVAs on them were

7 as per Table S2

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run in R (R Core Team 2018). Descriptive summary data are provided as mean ±

standard deviations.

Results

Field observations and habitat characteristics

Velutinids were observed (n = 110) and collected (n = 80; mean = 12.6 mm SL;

range 0.6 – 26.9 mm SL) primarily on vertical bedrock substrates or on undersides of

rocks at depths between 5.0 and 16.5 m8. Individuals were collected mostly in autumn

(October, n = 14; November, n = 16) in association with Aplidium glabrum and Ascidia callosa for deposition of egg capsules, or in spring (April, n = 13; May, n = 14) when feeding on various ascidians9.

Feeding Draft

Velutina velutina (O. F. Müller, 1776) preyed on all indigenous solitary ascidian species collected sympatrically (Ascidia callosa, Boltenia echinata, Halocynthia pyriformis, Molgula citrina) and non-sympatrically (Molgula griffithsii) but preyed less frequently on indigenous colonial species (Aplidium glabrum and Didemnum albidum).

In feeding trials with non-indigenous species, V. velutina showed limited feeding on the

colonial Botryllus schlosseri but consumed most internal organs (≥ 90%) when preying

on the solitary Ciona intestinalis. Velutina velutina (O. F. Müller, 1776) preyed on a wide

size range of ascidians, from those that were considerably smaller than the individual

velutinid to many times its size.

8 see Table S3 9 See Table S1

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During the multi-choice feeding experiment with native ascidian species,

predation was observed on B. echinata (n = 6) and H. pyriformis (n = 5), but was not

detected on A. callosa, A. glabrum or D. albidum. Results of the ANOVA performed on

the GLM confirmed that prey species was significant in predicting the number of

predation events (Chi-square, χ² = 66.375, df = 2, P < 0.001). In the complementary

multi-prey choice experiment including the non-indigenous species Botryllus schlosseri,

V. velutina preyed on all species examined but preyed more on the solitary species (H.

pyriformis, n = 35; M. citrina, n = 10; B. schlosseri, n = 2; A. glabrum n = 1), and A.

glabrum was only preyed on after all solitary species had been consumed. Results of the

analyses indicated that prey species was a significant predictor of number of predation

events (Chi-square, χ² = 41.627, df =Draft 4, P < 0.001), and that all species were preyed upon

significantly less often than H. pyriformis (P < 0.003). In the pair-wise feeding

experiment with the non-indigenous Ciona intestinalis, predation was detected on all

species but A. callosa (C. intestinalis, n = 2; B. echinata, n = 2; H. pyriformis, n = 1; M.

citrina, n = 1). Prey species was again significant in predicting the number of predation

events (Chi-square, χ² = 230.01, df = 5, P < 0.001) but due to the low number of

predation events it was not possible to determine specific species preferences. Results of

these feeding experiments reject the null hypothesis that V. velutina exhibits no

preferences among available ascidian prey species and demonstrates that solitary ascidian

species are preferred.

Feeding behaviour in V. velutina (Fig. 1A) included: cleaning the prey ascidian’s

tunic surface with the ; drilling a hole through the tunic; inserting the proboscis

through the hole (Fig. 1B – 1D); and extending the proboscis up to 1.5 times its shell

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12 length inside the prey to consume internal organs (Fig. 1E, 1F). Predation was not observed on dead ascidians but velutinids occasionally fed through recently abandoned holes drilled by congeners.

Velutina velutina (O. F. Müller, 1776) exhibited feeding behaviour for 84.6 ± 25.9 d and preyed on 5.2 ± 2.4 ascidians annually. Average time between feeding events was

45.5 ± 65.6 d but one individual went 245 d between feeding events. Velutina velutina

(O. F. Müller, 1776) demonstrated preferred feeding positions for each ascidian species

(Fig. 2). Field observations were similar, as 71.4% of velutinids that drilled or fed on H. pyriformis did so near the base, and the single observation of predation on M. citrina was through the side. In contrast, feeding on A. callosa in the field was observed twice through the side and once on top, nearDraft a siphon, as the base of the ascidian was inaccessible. Ascidians dissected post-feeding showed up to ~95% of internal tissues consumed (Fig. 1E, 1F) and all ascidians that were preyed upon eventually died.

Growth

Average growth of V. velutina was negligible throughout most of the year but increased significantly in June and July, which corresponded with the peak in water temperature (Fig. 3). Results of the ANOVA performed on the GLM indicated that change in water temperature is significant in predicting shell growth (Chi-square, χ² =

57.452, df = 1, P < 0.001). However, some smaller individuals (< 10 mm initial SL) exhibited growth throughout the year. Of the 42 individuals measured monthly, 21 survived to provide annual growth rates. Annual growth rates declined with increasing initial SL but beyond 16.9 mm initial SL growth stabilized at 0.5 ± 0.5 mm yr-1.

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Maximum growth rate recorded for an individual was 3.8 mm mo-1 (July 2009, initial SL

= 12.3 mm) and 7.9 mm yr-1 (initial SL = 9.0 mm).

Mating

Mating behaviours of V. velutina included aggregation, pairing, and copulation,

all of which showed some degree of overlap. Most notable was the overlap between

aggregating and pairing behaviours which typically co-occurred between late June and

early December, while copulation (Fig. 4A) persisted until late January. In the laboratory,

aggregating (n = 97 individuals) and pairing (n = 103 individuals) velutinids were mainly

concealed (80.4% and 65.0% of observations, respectively). Aggregations of up to 9

individuals were observed in clusters or in a line beneath rocks, coralline algae, or

ascidians. Likewise, in the field, aggregationsDraft of up to 7 individuals were observed under

rocks, in crevices of vertical rock walls, or near the bases of Ascidia callosa. All field

observations of pairings (n = 4 pairs) were on the undersides of rocks. In the laboratory,

copulation (n = 153 observations) occurred more frequently concealed beneath rocks and

coralline algae (41.2%) than on A. callosa (24.8%), whereas in the field, copulation (n =

6 individuals) occurred more frequently on A. callosa (66.7%) than in rock crevices

(33.3%).

Velutina velutina (O. F. Müller, 1776) copulated face to face but somewhat off-

centred to align reproductive organs located on their right sides (Fig. 4A). Velutinids

were observed undergoing sex role alternation during copulation as one pair, observed for

1.75 h, initially acted in one sex role but upon separation at the end of this period were

found to have switched sex roles. Laboratory observations of copulation were

predominantly unilateral (91.3%) but a few pairs (3.8%) exhibited simultaneous

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reciprocal copulation. During one reproductive season (2008/2009), individual velutinids

copulated on average 4.1 ± 1.3 times. Individuals acted as either male or female in

roughly equal proportions (43.6% as males, 38.5% as females) and less frequently as

male and female simultaneously (10.3%). The smallest individual V. velutina observed

copulating was 10.7 mm SL, yet one smaller individual (9.0 mm SL) was observed laying

an egg capsule, indicating this species may be mature by 9.0 mm SL.

Egg laying

Velutina velutina (O. F. Müller, 1776) can store spermatozoa for extended periods

or else is capable of self-fertilizing. Three of five individuals isolated to examine fine-

scale behavioural shifts and feeding rates were observed mating prior to isolation. These

velutinids were initially deprived of Draftsuitable ascidian species for egg capsule deposition.

Consequently, some attempted to lay capsules on other substrates including the surface of

Boltenia echinata, a clam shell, and even the tank surface, but these capsules did not develop. When later provided suitable ascidian species, all isolated velutinids began laying egg capsules, between 148 and 178 d after isolation. However, larvae from only three of those isolated velutinids developed and hatched.

Velutina velutina (O. F. Müller, 1776) only deposited egg capsules in Aplidium glabrum and Ascidia callosa but preferred the latter. One isolated velutinid was provided

A. glabrum and A. callosa simultaneously, but deposited capsules only in A. callosa.

Another isolated velutinid, initially provided A. glabrum, began to deposit capsules within it, but when A. callosa was later introduced, it deposited its remaining capsules in

A. callosa. Velutinids associated with A. glabrum and A. callosa in summer (late July –

early August), 3 – 4 months prior to initiation of egg laying in autumn. During this time,

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maturing gonads with bright orange oocytes were often observed through the posterior

portion of the shell.

While embedding egg capsules, V. velutina firmly attached to an ascidian’s tunic

(Fig. 4B). If forcibly removed, velutinids were often observed holding the capsule in their

ventral pedal gland, a circular indentation near the center of the foot. After interrupting

capsule deposition, capsules exposed on the tunic surface did not develop viable larvae,

and often burst open. However, egg capsules that were partially embedded when the

velutinid was removed would embed themselves in the ascidian tunic with no further

assistance from the parent, and the cap formed a bubble on the tunic surface. If

uninterrupted, velutinids embedded egg capsules in the ascidian tunic, leaving a striated

cap flush on the tunic surface (Fig. 4C).Draft As larvae began to develop, egg capsules

expanded in size with larvae taking up the lower portion of the capsule (Fig. 4D). Veliger

larvae of V. velutina were observed hatching from egg capsules in Ascidia callosa on two

occasions in April 2006. Most larvae emerged in groups of 2 – 3, hovered briefly, and

then swam to the surface where they remained. During the first hatching observation, the

host A. callosa broadcasted gametes soon after velutinid larvae began to emerge (Fig.

4E). When all larvae emerged, an empty cavity was left in the ascidian’s tunic (Fig. 4F).

Over time the empty capsule filled in with growth of new tunic tissue and a dark circle

remained as a scar where the capsule opening was located.

Based on data from 2006/2007 and 2007/2008, individual velutinids laid up to 18

egg capsules annually (mean = 8.2). In the laboratory and in the field, multiple velutinids

often converged on an individual A. callosa to deposit egg capsules (Fig. 4B). Up to 9

velutinids in the laboratory and 2 velutinids in the field, exhibited egg laying behaviour

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16 on an individual A. callosa. In the laboratory, as many as 53 intact capsules were recorded in an individual A. callosa. In the field, one large A. callosa (L: 90.0 × W: 63.3

× H: 45.5 mm) contained more than 30 intact capsules with evidence of at least 30 recently hatched capsules. In contrast, even a very small A. callosa (L: 9.9 × W: 8.3 × H:

4.8 mm), smaller than most adult V. velutina, was found containing 2 capsules. Mean number of larvae per capsule was 1392 and ranged from 408 – 1944 in the field and 538

– 3356 in the laboratory.

Larval development, hatching, and settlement

Egg capsules of V. velutina were opened periodically and larvae were photographed throughout their development (Fig. 5). Eggs (Fig. 5A) developed into 4- cell embryos after about 3 – 4 d (Fig.Draft 5B). They reached early veliger stage after ~2 weeks of development (Fig. 5D, E) and became fully developed echinospira veligers

(Fig. 5F, G, H) ~3 weeks of age. There was no evidence that V. velutina used nurse eggs to feed developing offspring. Larvae hatched (Fig. 4E) from early January to mid-July

(Table 2) and swam in the water column as planktonic echinospira veligers (Fig 5F, G,

H). In the communal tank, egg capsules laid at the start of each egg laying period (late

October/early November), took on average 71 d to hatch (range 60 – 81 d). Water temperature during those three incubation periods averaged 4.9 ºC (1.1 – 9.0 ºC).

However, from three isolated velutinids in 2009, egg capsule deposition started near the end of the egg laying season (mid-February/mid-March) and took on average 111 d to hatch (range 109 – 113 d), as water temperature averaged 2.1ºC (-1.9 – 10.5 ºC).

Settled larvae of V. velutina were observed on 8 individual A. callosa (17.4%) collected in April 2006 (Fig. 5I) but none were observed on A. callosa collected in March

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or November 2007. All settled larvae under laboratory conditions died unexpectedly soon

after. Settled velutinid larvae were not detected on any other ascidian species or substrate.

Seasonal behaviour

Velutina velutina (O. F. Müller, 1776) exhibited consistent annual succession of

behaviours (Fig. 6, Table 2). The proportion of feeding V. velutina increased as water

temperature decreased in winter and rapidly declined as water temperature increased in

summer (Fig. 6). Rapid transitions between feeding and mating modes occurred between

June and July (Fig. 6). Mating was the dominant behaviour observed during the warmest

time of year, late summer to late autumn (4.2 – 9.9 °C). Egg laying then became the

dominant behaviour as water temperature started to decline in late November (from 7.2

°C in 2007) and in early December (fromDraft 5.7 °C in 2008), peaking in December/early

January and progressively declined as water temperature reached its lowest level of the

year in late March/early April (Fig. 6). Velutinids were generally concealed under

coralline algae and rocks and fed near the base of ascidians from April to October. From

November to March, which coincided with the egg laying period, velutinids were more

exposed, mobile, or observed on the sides or tops of ascidians. Behavioural observations

from the field (n = 69) were consistent with the succession of behaviours recorded in the

laboratory (Fig. 6). Feeding field observations (n = 15) occurred mainly (73.3%) from

April to June. Mating in the field occurred (n = 12) primarily (91.7%) from October to

December. Egg laying behaviour in the field (n = 20) was mostly (80.0%) between

November and April. Further, evidence of developing or recently hatched egg capsules of

V. velutina in A. callosa collected from the field were found primarily in the spring.

Overall, 39.1% of A. callosa (n = 46) showed evidence of egg capsules in April 2006,

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13.2% (n = 38) in March 2007, and only 3.8% (n = 52) in November 2007. Occurrences of egg capsules may have been underestimated as biofouling on A. callosa made identification of capsules difficult.

Discussion

Velutina velutina (O. F. Müller, 1776) was consistently found on hard substrates, such as vertical rock walls and undersides of rocks, near ascidians, upon which they fed and deposit egg capsules, as reported in northern Europe (Jeffreys 1867; Diehl 1956;

Fretter and Graham 1981). Unlike some previous reports, V. velutina was not found associated with mud, sand (North and Baltic Seas; Ankel 1936), gravel/pebble mixtures, or macroalgae beds (Gulbin and Golikov 1999). In general, velutinids live on variety of substrates provided ascidians are nearbyDraft (Gulbin 2005).

Velutina velutina (O. F. Müller, 1776) preyed upon all ascidian species tested in the present study but preferred solitary species. This preference was also reported in the

North and Baltic Seas (Ankel 1936; Diehl 1956), and in San Juan Islands (northeast

Pacific; Young 1985). Preferred feeding locations on each ascidian species were detected, which may be related to mechanical, physical, and chemical anti-predator defences exhibited by different ascidians (see Lambert 2005), and how velutinids overcome those defences. During this study, predation on Halocynthia pyriformis occurred predominantly near the attachment base, as was likewise reported by Diehl (1956) for Styela coriacea.

This feeding location may reduce risk of exposure of V. velutina to potential predators and, as suggested by Young (1985), this area of the tunic may be softer, compared to the anterior end. In contrast, Boltenia echinata exhibits large, flexible spines over a thick leathery tunic, which in this study restricted predation by V. velutina to the bare base or

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siphons. Moreover, V. velutina preyed less frequently on A. callosa than other solitary

ascidians, likely due to its thick tunic and because it bioaccumulates vanadium (Stacey

2009), a heavy metal that may inhibit predation (Stoecker 1980; Young 1986). The low

predation observed on A. callosa may also be explained by the fact that V. velutina used

them to lay their egg capsules.

Here, V. velutina commonly formed spawning aggregations on or near A. callosa,

within which they deposit egg capsules. Many gastropods aggregate for reproduction on

their feeding grounds at sites suitable for egg deposition (Fretter 1984) to optimize use of

suitable sites for larval development where predation on capsules is limited (Martel et al.

1986). Velutina velutina (O. F. Müller, 1776) began aggregating in summer and persisted

until egg laying concluded in the spring.Draft In Atlantic Canada, gastropods such as

Buccinum undatum Linnaeus, 1758 and Nucella lapillus (Linnaeus, 1758), likewise

aggregate for mating and spawning, until egg capsules are laid (Feare 1970; Martel et al.

1986). Spawning aggregations of N. lapillus may consist of thirty or more individuals

that do not feed between bouts of copulation and egg laying (Fretter and Graham 1962).

Velutina velutina (O. F. Müller, 1776) also copulated between egg laying bouts but, in

contrast, fed throughout the spawning period.

Members of the genus Velutina are simultaneous (Ankel 1936;

Fretter 1984). Here, copulation was primarily unilateral with individuals behaving as

male or female in roughly equal proportions but occasionally individuals behaved as male

and female simultaneously. Diehl (1956) also observed mutual copulations between

individual V. velutina in the laboratory. For slow moving or sparsely distributed species it

is advantageous to be hermaphroditic such that any encounter with a mature conspecific

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may lead to fertilization (Tomlinson 1966; Ghiselin 1969). This may also be important

for species that occur in low abundance, like most velutinid species. Velutina velutina (O.

F. Müller, 1776) also exhibited polygamy, as reported for other gastropods (see Murray

1964; Martel et al. 1986; Johannesson et al. 2016).

The present study suggests that V. velutina can store viable spermatozoa for up to

6 months until a suitable ascidian host for egg laying becomes available. Eupleura

caudata (Say, 1822) and Urosalpinx cinerea (Say, 1822) may store spermatozoa for 6 to

9 months (Hargis and MacKenzie 1961), and Littorina saxatilis (Olivi, 1792) for at least a year (Johannesson et al. 2016). Sperm storage may allow selection of favourable time and location to deposit egg capsules (Martel et al. 1986). Polygamy and long-term sperm storage likely evolved in species withDraft limited mobility, like V. velutina, to prevent

impoverishment of their gene pools (Murray 1964).

The egg laying period for V. velutina occurred over five months (early November

to late March), starting as water temperature declined and ending as the lowest annual

temperature was reached. In Norway, V. velutina was observed to deposit egg capsules

between January and March (E. Svensen, personal communication, 2018), whereas

Mileikovsky (1960) suggested that reproduction of V. velutina in the Barents, Norwegian,

and White Seas occurred over one month or less, soon after the lowest annual water

temperatures. However, Mileikovsky’s (1960) report was based on accounts of early

larvae of V. velutina in the , rather than direct observation, as in this study. In the

northeast Pacific, rhombica (Dall, 1871) and V. plicatilis (O. F. Müller, 1776)

also spawns in winter, from January to March (McCloskey 1973; Strathmann 1992),

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while in northern Scotland perspicua (Linnaeus, 1758) spawns from February

to May (Jeffreys 1867).

Velutina velutina (O. F. Müller, 1776) preferred to deposit egg capsules in the

solitary ascidian Ascidia callosa, consistent with previous reports that members of the

genus Velutina spawn primarily in solitary ascidians. Reports from Europe found V.

velutina deposited egg capsules in Styela coriacea in the Baltic Sea (Diehl 1956) and in

Ascidia virginea Müller, 1776 in the Norwegian Sea (Moen and Svensen 2004). In the

northeast Pacific, Strathmann (1992) reported V. plicatilis deposited egg capsules in

Ascidia paratropa (Huntsman, 1912) and Chelyosoma productum Stimpson, 1864.

Locally, V. velutina may prefer to deposit egg capsules in A. callosa because its thick

tunic and bioaccumulation of vanadiumDraft (Stacey 2009) may deter predation (Stoecker

1980; Young 1986). Velutina velutina (O. F. Müller, 1776) laid up to 18 egg capsules

annually and spawning aggregations led to deposition in an individual A. callosa of 50 or

more egg capsules in the laboratory and more than 30 capsules in the field. Similarly,

Dias and Delboni (2008) reported that Lamellaria mopsicolor Ev. Marcus, 1958 may

deposit up to 20 egg capsules annually, and up to 53 egg capsules per ascidian host were

collected in the field.

Members of the superfamily are reported to prepare the initial point

of egg capsule deposition by creating a hollow in the tunic of an ascidian with their

radula (Ankel 1936; Diehl 1956). Here however, V. velutina used the ventral pedal gland

to forcibly embed egg capsules within the tunic with no evidence that the radula was

used. The ventral pedal gland is very muscular with a protrusible central region that can

be used as a ramrod to push the egg capsule into position (Fretter and Graham 1994). The

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22 relatively soft tunics of A. callosa and A. glabrum may allow V. velutina to use its pedal gland alone to deposit egg capsules. Diehl (1956) reported that after V. velutina partially imbedded a capsule in the tunic of Styela coriacea, the tunic grew around it, leaving only the cap exposed on the surface, as was observed here. Diehl (1956) suggested this reaction was either caused by the capsules themselves, as seemed to be the case here, or due to a teasing motion of the velutinid’s radula, which was not observed. However, during this study, egg capsules were typically fully embedded by the parent V. velutina.

Feeding and spawning periods of V. velutina overlapped during this study, and feeding peaked as spawning activity declined. In contrast, Diehl (1956) suggested that V. velutina did not feed during its spawning period, to avoid consuming ascidians in which it deposits egg capsules. However, V.Draft velutina preyed very little on A. callosa in this study, thus avoiding destruction of its developing larvae or future spawning grounds.

Egg capsules of V. velutina contained between 400 – 3400 larvae in this study.

This is similar to , which reportedly contain at least 1000, but usually well over 3000 larvae per capsule (Ankel 1935). In contrast, egg capsules of L. mopsicolor contained only 13 – 164 larvae (Dias and Delboni 2008). There was no evidence in this study that V. velutina use nurse eggs to nourish developing larvae. This concurs with Diehl (1956), who reported that larvae of V. velutina are nourished by a yolk reservoir in the hepatopancreas.

Only planktonic larval development of V. velutina has been previously described

(Lebour 1935; Thorson 1946; Diehl 1956; Fretter and Pilkington 1970; Thiriot-Quiévreux

1974). This is the first study to document the complete development of V. velutina from egg capsule deposition to larval hatching. Egg capsules of V. velutina took 2 – 4 months

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to hatch, depending on when they were laid. Capsules deposited at the start of the

spawning period were subject to warmer water temperatures (average 4.9 ºC) and their

larvae developed more rapidly than those in capsules deposited later in the period when

water temperatures were colder (average 2.1 ºC) and near the annual minimum (-1.9 ºC).

In the northeast Pacific, Strathmann (1992) found that larvae of V. plicatilis hatched in 36

d at 10 – 13 ºC, while in Brazil, Dias and Delboni (2008) found that larvae of Lamellaria

mopsicolor began hatching after 6 d at 23 – 26 ºC. Water temperature is a well-known

driver of larval development times (Scheltema 1967; Hoegh-Guldberg and Pearse 1995).

Egg capsules hatched over roughly seven months during the coldest months of the

year (January – April) until water temperatures reached the annual maximum (around

mid-July). Northern European studiesDraft have not reported hatching times for V. velutina but

several recorded the occurrence of their larvae in the plankton. Near Plymouth, UK,

Fretter and Shale (1973) collected larvae of V. velutina as early as April, while Lebour

(1935) reported them from May through the summer. Mileikovsky (1960) found Stage I

larvae of V. velutina as early as mid-March in the Norwegian Sea, and suggested larvae

entered the plankton in April in the Barents Sea, and in late May in the White Sea, where

they persisted until early July.

Adult V. velutina exhibited seasonal growth that peaked in summer, as water

temperature increased to its maximum, and stalled the rest of the year, similar to other

gastropod species (Largen 1967; Ota and Tokeshi 2000). Smaller individuals that were

likely immature exhibited growth throughout the year, as has also been reported for other

gastropods (Ota and Tokeshi 2000; Ishida 2004).

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The consistent succession of behaviours exhibited by V. velutina during this study primarily followed annual changes in seawater temperature. Feeding dominated during the coldest temperatures of the year and declined as temperature increased to its maximum in summer. At the end of the feeding period, velutinids exhibited growth, as water temperature reached its maximum, before transitioning to mating. Ishda (2004) reported that the gastropod Drupella margariticola (Broderip, 1833) annually reallocate energy from growth to reproduction. Here, behaviour alternated between feeding and mating before eventually transitioning to mating in June and July (2007 and 2008). This alternation seemed partly related to food supply in the laboratory. As prey became depleted, velutinids switched to mating but when prey supply was replenished feeding resumed. In August, despite availableDraft prey, velutinids entered mating season throughout warmer months. Egg laying started as water temperature decreased in late autumn, and ended when temperature reached the lowest annual level in the spring. Although water temperature may influence the timing of spawning, multiple factors (e.g. photoperiod, physiological changes, prey availability, water temperature) likely work in combination or succession to fine tune this behaviour in V. velutina, as in other marine taxa (Giese

1959).

In this study, V. velutina was more active and exposed during the egg laying period but tended to be concealed and inactive the remainder of the year, possibly driven by predator avoidance. From November to March, potential predators may be less active

[e.g. cunner, Tautogolabrus adspersus (Walbaum, 1792); Green and Farwell 1971], absent from shallow waters (<15 m) [e.g. juvenile Atlantic cod, Gadus morhua Linnaeus,

1758; Hanson 1996; Cote et al. 2004], or engaged in reproductive activities [e.g. polar sea

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star, Leptasterias (Hexasterias) polaris (Müller and Troschel, 1842); Himmelman et al.

1982; Hamel and Mercier 1995].

To date, little attention has focused on the role of indigenous predators in limiting

the success of non-indigenous species (Harley et al. 2013) and studies that examined

potential predators of non-indigenous ascidians have focused on generalist rather than

specialist predators (e.g. Osman and Whitlatch 2004; Simoncini and Miller 2007;

Epelbaum et al. 2009). The dynamics of specialist predators are tightly linked to one or a

few prey species and may play a role in structuring communities by controlling their prey

species densities (Snyder and Ives 2001). Members of the gastropod superfamily

Cypraeoidea have been previously reported to prey on invasive ascidian species.

Gitternberger (2007) reported LamellariaDraft sp. (likely L. perspicua) and Trivia arctica

(Pulteney, 1799) preyed on the colonial species, Didemnum sp. (later identified in

Lambert 2009 as D. vexillum Kott, 2002) in the Netherlands. Here, V. velutina preyed on

the non-indigenous C. intestinalis, but showed limited predation on the colonial species,

B. schlosseri. However, due to the relatively low abundance and low feeding rates of V.

velutina in this study and the rapid colonization rates and high abundance reported for C.

intestinalis (Carver et al. 2003; Ramsay et al. 2008), it may take time for V. velutina to

exhibit biotic resistance against populations of C. intestinalis. Therefore, predator-prey

interactions between V. velutina and C. intestinalis should continue to be monitored.

Acknowledgements

For invaluable assistance in the field we thank S. Bettles, R. Boland, W. Coffey,

J. Flight, C. Lewis, K. Matheson, D. Mouland, R. Murphy, A. Noseworthy, A. Storch, R.

O’Donnell, and B. Wringe. We thank S. Baillon, G. Doyle, K. Gale, N. Laite, J. So, and

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Z. Sun for assistance in laboratory maintenance and monitoring. We thank J. Stacey for allowing us to examine Ascidia callosa specimens for velutinid egg capsules and settled larvae; E. Svensen for providing observations of Velutina velutina feeding and spawning in Norway; E. Geissinger and E. Pedersen for providing advice on statistical analyses; and V. Ramírez for her suggestions and support. We also appreciated the constructive comments and suggestions of two anonymous reviewers.

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Fig. 1. Velvet shell (Velutina velutina) feeding on Halocynthia pyriformis. A – multiple

V. velutina attached near the base of H. pyriformis; B – V. velutina with proboscis

inserted through tunic of H. pyriformis; C – close-up of V. velutina proboscis inserted

through tunic of H. pyriformis; D – feeding hole of V. velutina near the base of H.

pyriformis; E - dissected intact H. pyriformis; F – dissected H. pyriformis after preyed

upon by V. velutina. Scale bars: A = 17 mm; B = 9.5 mm; C = 1.5 mm; D = 15 mm; E =

15 mm; F = 14 mm.

Fig. 2. Relative feeding positions of velvet shell (Velutina velutina) on common

indigenous ascidian species of Newfoundland, Halocynthia pyriformis, Boltenia

echinata, Ascidia callosa, and MolgulaDraft citrina. Shaded areas indicate observed feeding

and unshaded areas indicate drilling. BP = base papillae (on H. pyriformis only); B =

base; NB = near base; S = side; NT = near top; T = top; NS = near siphons; TS = through

a siphon.

Fig. 3. Average monthly growth rates (mm mo-1) ± Standard Error of velvet shell

(Velutina velutina) and daily tank water temperature data for 2008 (upper panel) and

2009 (lower panel).

Fig. 4. Velvet shell (Velutina velutina) copulation, embedding egg capsules, and hatching

larvae. A – copulation; B – egg capsules being embedded in Ascidia callosa; C – egg

capsules recently embedded in the tunic of an A. callosa; D – egg capsule with larvae

settled to bottom; E – larvae hatching as A. callosa simultaneously releases spawn; F –

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34 empty egg capsule in A. callosa tunic. Scale bars: A = 16 mm; B = 14 mm; C = 3 mm; D

= 3 mm; E = 23 mm; F = 3 mm.

Fig. 5. Velvet shell (Velutina velutina) larval development. A – Newly deposited eggs; B

– 4-cell stage embryos; C – transition stage between late embryos and early larvae; D – early veliger larvae; E – early veliger with echinospira clearly visible; F – retracted veliger showing its well-developed echinospira; G – frontal view of well-developed veligers swimming within an egg capsule; H – lateral view of a well-developed echinospira veliger; I – just settled larvae (arrows) on tunic surface of Ascidia callosa, insert showing one larva (length 920 µm). Scale bars: A = 360 µm; B = 380 µm; C = 200 µm; D = 295 µm; E = 150 µm; F = 230Draft µm; G = 700 µm; H = 800 µm.

Fig. 6. Laboratory and field behavioural activity patterns of velvet shell (Velutina velutina) and corresponding laboratory water temperatures in 2007 (upper panel) and

2008 (lower panel). Note: Numbers adjacent to symbols for field observations indicate the number of individuals observed exhibiting the behaviour at that time.

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Table 1. Summary of feeding experiments conducted on velvet shell (Velutina velutina) in the laboratory.

Total Number Experiment Sample Frequency of Prey Species Experimental Set-Up Duration of Outcome Type Sizes Observations Observations Each ascidian species had roughly equal surface area (2800 – 3200 Solitary species: mm2) tank-1; Ascidians placed Ascidia callosa, 3 tanks, Multi-species haphazardly on 21 × 28 cm Twice daily Number of Boltenia echinata, 3 V. velutina prey choice with perforated plastic canvas sheets 7.5 d velutinid-1 predation Halocynthia pyriformis; tank-1 135 indigenous and attached with monofilament (May 2006) (0800-1000, events on Colonial species: (9 velutinids ascidian species line (1 canvas sheet tank-1); 2000-2100) each species Aplidium glabrum, total) Flow through ambient seawater; Didemnum albidum Ascidians preyed on were not replaced during the experiment B. schlosseri (4 colonies); H. pyriformis (2 smallDraft individuals); Single Non-indigenous species: M. citrina (2 individuals); and non-indigenousa Botryllus schlosseri; A. glabrum (5 colonies) placed Number of 98 d Once every prey species Indigenous species: simultaneously in 1 tank; Static 1 tank, predation (February to 1-7 d 194 versus multiple Halocynthia pyriformis, conditions maintained near 5 V. velutina events on June 2007) velutinid-1 indigenous prey Molgula citrina, ambient water temperature; each species species Aplidium glabrum Deceased ascidians were removed but not replaced during the experiment Non-indigenous species: C. intestinalis (1 individual) tank-1 Pairwise Ciona intestinalis; paired with an indigenous ascidian 5 tanks, Number of non-indigenousa Indigenous species: (1 individual); Static conditions 1 V. velutina 44 d Once every predation versus Ascidia callosa, maintained near ambient water tank-1 (May to 1-4 d 105 events on indigenous prey Boltenia echinata, temperature; When predation (5 velutinids June 2017) velutinid-1 each species species Halocynthia pyriformis, confirmed, both ascidians replaced total) Molgula citrina to start a new feeding trial a – Both golden star tunicate (Botryllus schlosseri Pallas, 1766) and vase tunicate (Ciona intestinalis Linnaeus, 1767) (formerly C. intestinalis type B) are considered cryptogenic in northeastern North America (Yund et al. 2015; Ma et al. 2017); however, they are likely non-indigenous to Newfoundland waters given limited reports of these species in the area (United States Navy 1951; Hooper 1975) until recently (Callahan et al. 2010; Sargent et al. 2013; Ma et al. 2017). Therefore, the interaction of V. velutina with these two non-indigenous ascidian species in Newfoundland was examined.

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Table 2. Combined laboratory and field observations of copulation, egg capsule laying and hatching for velvet shell (Velutina velutina) from 2006 to 2009.

First Egg Final Egg First Egg Final Egg Years First Copulation Final Copulation Capsule Laid Capsule Laid Capsule Hatch Capsule Hatch

2006 – 2007 Jun. 24, 2006 Jan. 14, 2007 Nov. 4, 2006 Mar. 25, 2007 Jan. 23, 2007 N/Aa

2007 – 2008 May 26, 2007b Jan. 21, 2008 Oct. 28, 2007 Apr. 5, 2008 Jan. 6, 2008 Jun. 29, 2008

2008 – 2009 Jun. 23, 2008 Dec. 14, 2008 Nov. 6, 2008 Mar. 22, 2009 Jan. 4, 2009 Jul. 13, 2009

a – All Ascidia callosa died before egg capsules could all hatch. Some capsules were still intact on May 21, 2007. b – Lack of food in tank at this time may have induced early copulation.

Draft

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Draft

Fig. 1. Velvet shell (Velutina velutina) feeding on Halocynthia pyriformis. A – multiple V. velutina attached near the base of H. pyriformis; B – V. velutina with proboscis inserted through tunic of H. pyriformis; C – close-up of V. velutina proboscis inserted through tunic of H. pyriformis; D – feeding hole of V. velutina near the base of H. pyriformis; E - dissected intact H. pyriformis; F – dissected H. pyriformis after preyed upon by V. velutina. Scale bars: A = 17 mm; B = 9.5 mm; C = 1.5 mm; D = 15 mm; E = 15 mm; F = 14 mm.

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70 Halocynthia pyriformis Boltenia echinata 60 n = 575 n = 39

50

40

30

20

10 Draft

0 BP B NB S NT T NS TS B NB S NT T NS TS 70 Ascidia callosa Molgula citrina

60 n = 28 n = 19

Percentage of Observations of Percentage 50

40

30

20

10

0 B NB S NT T NS TS B NB S NT T NS TS

Relative Feeding Position

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Draft

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Draft

Fig. 4. Velvet shell (Velutina velutina) copulation, embedding egg capsules, and hatching larvae. A – copulation; B – egg capsules being embedded in Ascidia callosa; C – egg capsules recently embedded in the tunic of an A. callosa; D – egg capsule with larvae settled to bottom; E – larvae hatching as A. callosa simultaneously releases spawn; F – empty egg capsule in A. callosa tunic. Scale bars: A = 16 mm; B = 14 mm; C = 3 mm; D = 3 mm; E = 23 mm; F = 3 mm.

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Draft

Fig. 5. Velvet shell (Velutina velutina) larval development. A – Newly deposited eggs; B – 4-cell stage embryos; C – transition stage between late embryos and early larvae; D – early veliger larvae; E – early veliger with echinospira clearly visible; F – retracted veliger showing its well-developed echinospira; G – frontal view of well-developed veligers swimming within an egg capsule; H – lateral view of a well-developed echinospira veliger; I – just settled larvae (arrows) on tunic surface of Ascidia callosa, insert showing one larva (length 920 µm). Scale bars: A = 360 µm; B = 380 µm; C = 200 µm; D = 295 µm; E = 150 µm; F = 230 µm; G = 700 µm; H = 800 µm.

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12 10 8 6 4 2 0 -2 2MM2 Temperature (°C) 1E 2007 3 E 100

80

60

40

20

0

Proportion of Individuals (%) Jan Feb Mar Apr May Draft Jun Jul Aug Sep Oct Nov Dec Jan 12 10 8 6 4 2008/2009 2 0

-2 Temperature (°C) F Field Feeding 2F 1F M Field Mating 2008 6MMM 4 2 2M E Field Egg Laying 2 E 2 E 2 E 100 Feeding Mating 80 Egg Laying

60

40

20

0

Proportion of Individuals (%) Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec Jan Date

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