- Original Article
- Open Access
Synchronism of naupliar development of Sacculina carcini Thompson, 1836 (Pancrustacea, Rhizocephala) revealed by precise monitoring
Helgoland Marine Research volume 70, Article number: 26 (2016)
Sacculina carcini is member of a highly-specialized group of parasitic cirripeds (Rhizocephala) that use crabs (Carcinus maenas) as hosts to carry out the reproductive phase of their life cycle. We describe the naupliar development of S. carcini Thompson, 1836 from a very precise monitoring of three different broods from three specimens. Nauplii were sampled every 4 h, from the release of the larvae until the cypris stage. Larval development, from naupliar instar 1 to the cypris stage, lasts 108 h at 18 °C. A rigorous sampling allowed us to describe an additional intermediate naupliar instar, not described previously. Naupliar instars are renumbered from 1 to 5. Nauplius 1 (N1) larvae hatch in the interna; N2 are released from the interna and last between 12 and 16 h; N3 appear between 12 and 16 h after release; N4 appear between 28 and 32 h; and N5 appear between 44 and 48 h. The cypris stage appears between 108 and 112 h. The redescribed morphologies allowed us to identify new characters. Antennular setation discriminates naupliar instars 3, 4 and 5. Telson and furca morphologies discriminate all naupliar instars. Furthermore, we demonstrate that the speed of larval development is similar within a single brood and between broods from different specimens, suggesting synchronization of larval development. From precise monitoring of broods every 4 h, we demonstrate that the life cycle of S. carcini includes five instars of naupliar larvae instead of four. The morphological characters of the larvae discriminate these naupliar instars and allow the identification of S. carcini from other Rhizocephala species. S. carcini larvae develop synchronously. Consequently, they might be an informative model to study larval development in crustaceans.
Sacculina carcini is a highly specialized barnacle parasite of several Brachyura crabs including the green crab Carcinus maenas . It belongs to the Rhizocephala, all of which present a highly altered morpho-anatomy at the adult stage, related to their endoparasitic lifestyle. The female adult consists of a root system that colonizes the crab cavity and is connected by a stalk running through the integument of the pleon to an external reproductive sac, the externa. One or two males take up residence inside the externa and develop into testes enclosed in the sac. Nauplius larvae are released by contractions of the externa and develop after several molts into a cypris larval stage, which metamorphoses into an adult after fixation on a suitable host crab.
The systematic positions of S. carcini and other Rhizocephala have been enigmatic. The first report of Sacculina is by Cavolini  who recognized Sacculina nauplii as one-eyed organisms, and grouped them with crustaceans. Thompson  described the S. carcini adult as a parasite and noted its affinity with cirripeds by studying the nauplius larvae.
Currently, larval descriptions are still useful to identify and compare Rhizocephala species, primarily because specific adult taxonomic characters are scarce [4, 5]. Four naupliar instars have been described for S. carcini [6, 7], but several descriptions of other Rhizocephala species count five naupliar instars: Briarosaccus tenellus , Polyascus polygenea , Sacculina pilosella , Peltogasterella gracilis and P. sulcata , and Heterosaccus papillosa . The number of naupliar instars in Rhizocephala is a matter of some debate [11, 13] and our aim was to monitor larval development precisely to determine the exact number of naupliar instars.
In this study, we reared S. carcini specimens on green crabs over a period of several months in order to obtain several larval broods. Larvae of single broods were sampled every 4 h, which allowed a precise description of the larval development.
Collection of Sacculina parisitized crabs
Carcinus maenas crabs parasitized by S. carcini were collected by hand during autumn 2012 and spring 2013 at Saint-Malo, Brittany, France (48°40′33′′N, 1°59′9′′W), on the high level of Fucus serratus tidal belt. They were transported at ambient temperature to Paris in polystyrene boxes containing Fucus algae, without seawater.
Maintenance of Sacculina-parisitized crabs
Parisitized crabs were maintained in artificial seawater (salinity of 35 g/L, Instant Ocean, Aquarium Systems, Eastlake, Ohio), in a 160 L aquarium with a filtration system, which consists of a filter grid beneath a layer of gravel at the bottom of the aquarium, and prevents the aspiration of Sacculina larvae.
This system is composed of two different water circuits. In the first, water is aspirated at low flow rates through the gravel layer by a filter pump (Superfish AquaPro QS 400, 1000 L/h). In the second, water is circulated to the surface through a tube containing a bubbling stone connected to an air supply to provide aeration. Both systems cause suspended particles to be gently drawn to the bottom of the aquarium and degraded naturally by bacteria. The water temperature was maintained at 18 °C (the nominal temperature of seawater at the northern coast of France during the summer) by a water thermoregulator (Teco TC10). The aquarium contained between 15 and 20 crabs. A total of 64 crabs were maintained in total, and fed with mussels three times per week.
Sampling of S. carcini larvae
Thirty-four single broods of S. carcini were obtained directly from aquaria containing Sacculina-parasitized crabs at 18 °C, by checking with a light source placed at the corner of the aquarium three times per day. Samples were collected for 10 min at the light source where the larvae concentrated due to their positive phototropism and transferred with pipettes to vessels containing filtered natural seawater. The direct release of larvae from S. carcini externae was observed three times and these larvae were sampled immediately. Nine broods were obtained prematurely in stress conditions, by removing the crab from the water and touching the ostiole in the externa with a needle and then reimmersing the crab and collecting the larvae directly.
Raising S. carcini larvae
Twenty-seven broods were sampled as soon as they were observed to identify the first naupliar instar. Seven broods were allowed to mature to the cypris stage. Larvae were transferred to a 0.5 L glass vessel containing natural seawater filtered through a 150 µm pore filter. Vessels were covered with perforated aluminium foil and placed in an 18 °C incubator without light. Seawater was changed every 24 or 48 h, depending of the density of larvae. For three of the broods, larvae were sampled every 4 h until the cypris stage. The other four broods were sampled less regularly in order to confirm the development chronology. For each instar, the time indicated in hours corresponded to the duration since the larvae were released.
Fixation and preservation of larvae
For each sampling, an aliquot of about 100 larvae (nauplii or cypris) was fixed in 1% formalin. Larvae used for measurements and observations were rinsed three times (20 min each) in phosphate buffer saline (PBS), then preserved by transferring them through three ethanol baths (25, 50 and 70%), for 20 min each.
Naupliar instars are numbered from nauplius 1 (N1) to nauplius 5 (N5) (Table 1), as for Polyascus polygenea . Larvae were referred to as “early” if just after the molt and “late” if just before the next molt. The method of counting antennulary setae may vary according to the publications. Walossek et al. , Rybakov et al.  and Ponomarenko et al.  numbered antennulary setae from S1 for the preaxial seta to S5 for the postaxial seta. Collis and Walker  numbered from postaxial to preaxial. We decided to number from preaxial to postaxial setae. We used the term “portions” to designate the subdivisions of the antennules .
Sexes of broods
For seven broods, live cypris larvae were relaxed for 10 min in seawater containing tricaine mesylate (MS-222)  before fixation in order to extend the antennules and thus determine the sex of the larva by the morphology of their antennular aesthetascs [14, 15].
Identification, drawing, and measurement of the larval instars
A minimum of 20 PBS-rinsed larvae from each 4-hr sample were placed in depression slides and observed with an optical microscope to identify the larval instar. We measured naupliar instars from one brood of male larvae and one brood of female larvae. Dimensions of the larvae digitally photographed at 10× magnification were measured using AnalySIS Work v.5 software (Olympus SZX7 associated with DP 20 camera). Nauplii larvae were measured for maximal length and for width without the frontal horns. The furcae were also measured for length and for maximal width at their base. Cypris larvae were measured for maximal length. Measurements were calibrated with a micrometric slide.
To produce larval drawings, larvae rinsed in PBS were slightly crushed between a slide and coverslip to observe the antennulary setae, and traced at 400× magnification with Lucida camera (Wild M20). Lines were thickened and the tracings were then scanned.
Scanning electron microscopy (SEM)
Larvae preserved in 1% formalin were washed with PBS, placed in 74 μm mesh size inserts (Netwell, Corning, Pittston, Pennsylvania), and progressively dehydrated in 30-min baths of ethanol (30, 50, 70, 95%, and three times in 100%). They were progressively passed from 100% ethanol to 20-min baths of hexamethyldisilazane (Sigma-Aldrich, Gillingham, United Kingdom) at 30% and 70%, and two times in 100%. Larvae were dried in a fume hood for 5 min and preserved in a desiccation chamber.
Larvae were mounted on stubs and then sputter-coated in gold (108 Manual Sputter Coater, Ted Pella Inc., Redding, California). The SEM observations were performed with a TESCAN-VEGA-II-LSU scanning electron microscope (courtesy of the Direction des Collections SEM facility of the Muséum National d’Histoire Naturelle, Paris) with an accelerating voltage of 15 kV. Electron micrograph images were taken with an Everhart–Thornley detector.
Statistical analyses of larval instar dimensions
Larval instar dimensions were analysed using R software . Results were considered statistically significant at p ≤ 0.05. To verify the sexual dimorphism of S. carcini naupliar larvae, the dimensions of fixed male and female larvae from broods that had been retrospectively sexed at the cypris stage were measured at instars N2–N5 (n = 25 per instar). The measurements for each characteristic were pooled and their normal and homoscedastic distributions were tested [17, 18]. Differences between the dimensions of male and female larval instars were analysed by the Kruskal–Wallis test  and a post hoc test , using the “agricolae” package .
Sex-specific dimensions of S. carcini larvae
In single-sex broods, the measurements for each characteristic and each stage were distributed normally, which was consistent with populations containing a single sex. Males were significantly longer and wider at each naupliar instar (N2–N5) than females (p < 0.0001) (Table 2). Male furcae were significantly longer than female furcae at N2 (p < 0.001) and N3 (p < 0.001). At the cypris stage, male larvae (n = 49; 276.5 ± 6.9 µm) were also significantly longer than female larvae (n = 31; 238.4 ± 5.1 µm) (p < 0.0001).
Morphology of the naupliar instars of S. carcini
Discriminating morphological characters are summarized in Table 3. For each instar (N2–N5), these characters are identical between male and female nauplii.
Nauplius 1 (N1)
The N1 present an ovoid shape (Figs. 1a, 2a, 3a). Diffuse brown and red pigments are present in the cephalic region (Fig. 1a). Frontal horns are short, directed rearward (Figs. 1a, 2a), with a triangular shape and an apical anterior spine, without terminal fringe (Fig. 3b). Each antennule has three portions (Fig. 1a) and bears five setae (S1–S5) (Figs. 2b, 3c), in which S1, S2, and S5 are shorter than S3 and S4, and S1 is conspicuous. Setae S1–S4 are inserted in the distal portion of the antennule. S5 is separated from the others on the distal edge of the second portion (Figs. 2b, 3c). The two furcal rami have a triangular shape and are short (Figs. 1a, 2a, c,3a, d).
Nauplius 2 (N2)
The N2 present an elongated shape (Figs. 1b, 2a, 3e). N2 are significantly shorter (p < 0.001) than N3, N4, and N5 within a same sex (Table 2). Brown and red pigments are located in the same region as N1 (Fig. 1b). Frontal horns are elongated, oriented laterally (Figs. 2a, 3e), and subdivided into three portions by two discrete grooves (Fig. 3f). Horns terminate with two spines, one anterior and one posterior, within the fringes of setae which are joined to each other (Fig. 3f). Setation of antennules is the same as in N1, with S1 conspicuous (Figs. 2b, 3g). The furcal rami are slightly thick (Figs. 1b, 2c, 3h) and without setules on the proximal third, but thin and with numerous long setules on the distal two-thirds (Fig. 3h). For each sex, the furcae are significantly shorter than in N3 and N4 (p < 0.01).
Nauplius 3 (N3)
This naupliar instar has been overlooked in previous publications [6, 7]. The N3 body shape is similar to that of N2 (Figs. 1c, 2a, 3i). Brown and red pigments are located in the same region as in N1 and N2 (Fig. 1c). Frontal horns terminate with two spines, as in N2, but the fringe setules are individualized (Fig. 3j). On the antennules, the second portion is swollen (Fig. 1c) and the S1 is inconspicuous (Figs. 2b, 3k). The furcal rami of N3 are slender and diverged (Figs. 1c, 2c, 3l). Within the same sex, N3 furcal rami are significantly longer than in N2. On the rami, setules are present on the distal two-thirds and evenly spaced (Fig. 3l).
Nauplius 4 (N4)
The N4 shape is similar to those of N2 and N3 (Figs. 1d, 2a, 3m). Brown and red pigments are located in the same region as N1–N3 (Fig. 1d). Frontal horns of N4 (Fig. 3m, n) are identical to the horns of N3 (Fig. 3i, j). On the antennules, the second portion in N4 (Fig. 1d) is more swollen than in N3 (Fig. 1c) and the S1 is absent (Figs. 2b, 3o). A tubercle with setules is present between the two furcal rami, in ventral view (Figs. 2c, 3p).
Nauplius 5 (N5)
The body shape of N5 is more elongated than in N2–N4 (Figs. 1e, f, 2a, 3q). Future thoracopods are visible under the cuticle (Fig. 1e, f). At 52 h, the young N5 present brown pigments in the cephalic region (Fig. 1e). At 104 h, two spots of red pigments are present in the lateral part of the posterior region under the head shield of the late N5 (Fig. 1f). Frontal horns are identical to those in N4 (Figs. 1e, f, 2a, 3r). On the antennules, the second portion of the antennule is bulbous (Fig. 1e, f). S1 is absent and S5 is inconspicuous and inserted on the third antennular portion (Figs. 2b, 3s). A tubercle with setules is present between the two furcal rami, in ventral view (Figs. 2c, 3t). The telson presents two symmetrical and lateral notches, with a spine (Figs. 2c, 3t). At the base of the rami, sleeves can be present or absent, depending on the specimen (Fig. 3t).
Chronology and synchronism of the larval development
In the nine broods obtained under stress conditions, N1 were always present and one was a mix of N1 and N2. Among the 34 broods obtained under normal conditions in aquaria, N2 was generally the first instar sampled.
We studied larval development over time in seven different broods in natural conditions: two male, one female, and four of mixed-sex. Instar durations were similar among the three broods sampled every 4 h (one mixed-sex, two male) and were confirmed in the four other broods sampled less regularly (one female, three mixed-sex). Times of molts were indicated by the presence of exuviae in the aliquots. N2 lasted between 12 and 16 h; N3 appeared between 12 and 16 h after release and lasted about 16 h. N4 appeared between 28 and 32 h and lasted also about 16 h. N5 appeared between 44 and 48 h and lasted about 64 h. The cypris stage appeared between 108 and 112 h and were maintained up to two weeks at 4 °C.
Five naupliar instars in S. carcini
From our regular sampling of larvae every 4 h, we identified five naupliar instars (N1–N5) whereas previous studies identified only four: N1–N4 [6, 7], which correspond to the N1, N2, N4 and N5 that we observed (Table 1). Giard  and Delage  also counted four molts until the cypris stage, i.e. four naupliar instars. The N2 and N3 are morphologically similar and last about 16 h each which may explain why they were described as a single instar previously. In other Rhizocephala species, four naupliar instars are usually described, but the frequencies of samplings were not specified [7, 24, 25]. The first description of five naupliar instars concerns a cold-water Rhizocephala, Briarosaccus tenellus . Its development is very long (26–30 days at 5 °C), which likely helped reveal the five naupliar instars. After this work, investigators began to count exuviae and fix rhizocephalan larvae samples more frequently. Five naupliar instars were subsequently described in other Sacculinidae species: Polyascus polygenea , Sacculina pilosella  and Heterosaccus papillosus . Five instars were also found in Peltrogastridae: Peltogasterella sulcatus, P. gracilis  and Peltogaster reticulatus . In contrast, some authors still found only four naupliar instars in Sacculina sinensis by sampling every day  and in Polyascus plana by sampling every 6 h .
In Thecostraca, which includes the Cirripedia, Ascothoracida and Facetotecta, six naupliar instars are usually found, but many taxa have fewer instars or the larvae hatch as cyprids . When nauplius larvae are present, instar numbers vary from four to six in the cirripeds Acrothoracica [29, 30] and Thoracica species . In Ascothoracida, which are all parasites in echinoderms and anthozoans , Ulophysema oeresundense present two naupliar instars  while Baccalaureus falsiramus present six naupliar instars . All abbreviated developments in Thecostraca are linked to lecithotrophy, reducing the amount of energy allocated to larval development [35, 36]. We suggest that the lecithotrophy and abbreviated development in Rhizocephala are adaptive responses to their parasitic life. Abbreviated development facilitates the life cycle progression of these parasites because invasive stages are attained more rapidly. For example, in the rhizocephalan Akentrogonidae, which are parasites of crustaceans, cypris larvae hatch directly . However, there is a trade-off because hatching at the cypris stage does not permit large larval dispersion, although dispersion time is reduced. Moreover, we suggest that Rhizocephala nauplii disperse passively towards the light, whereas competent cyprids actively seek their hosts .
New insights on the morphology and dimensions of the naupliar instars of S. carcini
We compared our results to the previous work of Walker . Our statistical analyses show that males are significantly longer than females from N2 to N5 (Table 2), which confirms previous observations. We also observed that our N4 and N5 length were shorter than the corresponding instars studied by Walker  (Table 1). As our measurements differ from those of Walker , it is not possible to determine if the naupliar instar overlooked previously is N2 or N3. Body and furcal lengths are significantly different in these instars and can be used to discriminate N2 from N3 within a same sex.
Compared to previous morphological observations , the two spines of the frontal horns in our observations are located anteriorly and posteriorly rather than dorsally and ventrally. In our observations, the second antennular portion of S. carcini swells progressively from N2 to N5, whereas Collis and Walker  found a swelling only in N3 and N4. Our N1 is identical to their N1 and our N4 is similar to their N3, except that we observe lateral spines only in N5. Our N5 is clearly the same larva as their N4. In addition, we found two previously undescribed N5 characters on the antennules. First, the postaxial seta (S5) is reduced compared to its size in N4 (Fig. 2b). Second, the insertion of S5 changes between the N4 and N5 instars from the second to the third antennular portion. S5 needs to be traced through the cuticle during molts, to ensure that it is the same seta from N1 to N5. Moreover, the red pigments in posterior region are useful for identifying late N5 larvae. By comparison, we can conclude that our N2 is similar to their N2. In both N2 descriptions, the preaxial seta (S1) is not reduced. In previous drawings of N2 (Figs. 1B and 24B in ), the second portion of the antennules is not swollen. Also, the furcal rami of their N2 are slightly thicker and shorter than in their N3 and present long and numerous setules. Thus, their N2 corresponds to our N2. From these comparisons, we conclude that our N3 is a previously undescribed naupliar instar.
Morphological characters of S. carcini larvae compared to other Rhizocephala larvae
Morphological characters of the nauplii are important for rhizocephalan systematics and phylogeny .
Fronto-lateral horns of N2–N5
In S. carcini, frontal horns end in two spines and a fringe of setules between them (, this study). These two apical spines are specific to Sacculinidae . In Peltogastridae, frontal horns are ornamented by one seta on the middle portion in P. gracilis and P. sulcata , and two setae in B. tenellus . Apical fringe of setules are common to all Rhizocephala [8, 9, 11, 12, 28]. From our study, S. carcini frontal horns are divided into three portions at N2 (Fig. 3f). These subdivisions of the frontal horns were previously found only in Peltogastridae [8, 11].
Morphology and setation of antennules
The swelling of the second antennular portion of S. carcini has also been reported in other Rhizocephala species [9, 11, 12]. Swelling of antennules is also common in Thoracica  and is related to the formation of the cypris adhesive disc .
In S. carcini, as in almost all other Rhizocephala species, the N1–N3 naupliar instars present five setae on their antennules; S1 and S5 are shortest, S2 is intermediate, S3 and S4 are longest. Moreover, the S1 is reduced in size at N3 and disappears at N4 [9–12]. Briarosaccus tenellus is an exception because S1 disappears at the second instar . In S. carcini, the S5 becomes inconspicuous at N5. To our knowledge, this reduction has not been described previously, but a progressive reduction in size between N2 and N4 appears in drawings of Heterosaccus papillosus antennulae . The S5 at N2 presents a small spine at its base (Fig. 3g). A spine has also been described in the Rhizocephala observed in SEM: B. tenellus , P. sulcata and gracilis , and H. papillosus . In the two latter descriptions, the authors proposed that it is a 6th seta. Nonetheless, in S. carcini, this tip is not present on all larvae, and when it is present, it is inserted randomly and directly on the S5. These observations suggest that S5 presents a variable morphology and that the tip could not be interpreted as a vestigial 6th seta in S. carcini.
Our observations on S. carcini indicate that the setae S1–S4 are inserted on the apical portion. S5 is clearly inserted on the distal edge of the second portion at N1 and N2 (Fig. 3c, g), on the limit of the two last portions at N3 and N4 (Fig. 3k, o) and on the apical portion at N5 (Fig. 3s). This “jump” of setae between the antennular portions during the naupliar development has been previously described in cirripeds by Grygier .
Telson and furca
Furca and telson characters are useful for discriminating S. carcini naupliar instars at low magnification. The furca is longer at N3 than at N2 and could be useful for discriminating these instars within the same sex (Table 2). The furcal rami of the naupliar instars of S. carcini are almost as long as in S. pilosella  and in H. papillosus . They are about one third shorter in P. polygenea .
In S. carcini, furcal rami are thick and short at N2, and thin and long at N3. We observe the same obvious characters in P. sulcata SEM images , suggesting that this character could be useful for identifying larval instars in several taxa.
The morphology of the telson (lateral spines in notches and tubercle) can also be used to discriminate the other naupliar instars (N1, N4 and N5) of S. carcini (Figs. 2c, 3d, p, t). Lateral spines on the telson are visible only in our N5 (Fig. 3t). These spines are present earlier at N4 in P. sulcata and P. gracilis , and in S. pilosella .
The tubercle between the furcal rami is visible in ventral view at N4 and N5 in S. carcini. Tubercles are also present in the Sacculinidae P. polygenea  and H. papillosus  at the same instars, but not in the Sacculinidae S. pilosella  and the Peltogastridae B. tenellus  and P. gracilis . This character seems variable within the rhizocephalans and even within the Sacculinidae, and could be a useful taxonomic character.
N1, intermediate instar between embryos and larvae
N1 larvae of S. carcini are only present in premature releases provoked by stress. Premature hatching of first instar larvae can also be provoked in the Acrothoracica species Trypetesa nassarioides  and in the Ascothoracida species Baccalaureus falsiramus .
From naturally released broods obtained in aquaria, the first larval instar of S. carcini is usually N2, with a mix of N1 and N2 observed only once. Giard  observed that, in Rhizocephala, larvae hatched as N1, but molted rapidly in N2, sometimes before their release out of the externa. Later, Delage  confirmed Giard’s observations in S. carcini. These observations suggest that N2 is the most frequent instar released in the field by S. carcini. The N1 instar is very short in duration. N1 larvae develop normally, except if they have not molted after one day . Mixtures of two larval instars at release have been observed in the Rhizocephala Lernaeodiscus porcellanae  and in the Thoracica Balanus amphitrite .
We suppose that in S. carcini, and perhaps in other cirripeds, mantle contractions help in the hatching at N1 and the molting in N2, inside the externa, which allows a majority of N2 to be observed in normal releases.
Synchronous development among larvae of a single brood
This is the first study on S. carcini larval development with a precise chronology obtained by sampling every 4 h. The larval development of S. carcini is remarkably synchronous within the same brood. Furthermore, the durations of naupliar instars are identical between broods obtained from different specimens. Synchronous larval development has been proposed for Rhizocephala [8, 46], but to our knowledge, has never been previously demonstrated until this work.
This synchronism resembles that observed in embryos of several species as the amphipod Parhyale hawaiensis . We posit that, as in embryos, the lecithotrophy in nauplii allows the synchronous larval development and it may be that the synchronism of S. carcini is related to its parasitic lifestyle. The lecithotrophy in nauplii has appeared many times among crustacean taxa . In several cases, lecithotrophy concerns parasitic species: in the Thoracica Anelasma squalicola  and probably in most of Ascothoracida and Facetotecta species , and in some Copepoda .
S. carcini may be a convenient model to study larval development. Its development table should allow further studies on the ontogenetic processes within an instar, rather than in successive instars. The S. carcini model permits studies on a continuous process, as previously recommended for arthropod developmental studies .
From precise monitoring of broods every 4 h, we demonstrate that the life cycle of S. carcini includes five instars of nauplius larvae. The second and third naupliar instars were probably previously identified as a single instar either because their morphologies are similar or because they only last about 16 h each. We also describe these larval instars and present the morphological characters, such as the furca, the fronto-lateral horns, and the setation of the antennules that together discriminate these naupliar instars and identify S. carcini from other Rhizocephala species. Finally, we demonstrate that S. carcini larva development is reproducibly synchronized across different broods.
nauplius instar 1
nauplius instar 2
nauplius instar 3
nauplius instar 4
nauplius instar 5
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FT performed the experiments and analyses, and contributed to the writing of the article. NR co-directed the research with FA and participated in manuscript revisions. LB participated in the analyses and in manuscript revisions. FA co-directed the research with NR, interpreted the data and analyses, and was a major contributor to the writing of the manuscript. All authors read and approved the final manuscript and approved its submission for publication.
We are thankful to the SEM facility of the Direction des Collections located at the Muséum National d’Histoire Naturelle (Paris) for all the SEM images used in this article and Sylvain Pont for training in SEM. The authors also thank Dr. Adrien Bussard and Dr. Marc Eléaume for their advice in statistics and on R, and Dr. Kurt Liittschwager for reviewing the English text.
The authors declare that they have no competing interests.
Availability of data and material
The datasets during and/or analyzed during the current study are available from the corresponding author on reasonable request.
This research was funded by the research project grant “Actions Thématiques du Museum National d’Histoire Naturelle (MNHN): Cycles Biologiques and Formes”.
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Trédez, F., Rabet, N., Bellec, L. et al. Synchronism of naupliar development of Sacculina carcini Thompson, 1836 (Pancrustacea, Rhizocephala) revealed by precise monitoring. Helgol Mar Res 70, 26 (2017) doi:10.1186/s10152-016-0479-2
- Synchronous development
- Nauplius larva