Spawning times of four out of the six species encountered here were not yet described for the Red Sea and to our knowledge, this is the first field observation of a basket star releasing female gametes. Relatively little is known about the life history of A. nuda, but our observations suggest that this species—like many Ophiuroids—relies on broadcast spawning. Apart from our description of mass egg release in the north-western Red Sea, the only other in situ description of spawning appears to be a single A. nuda individual releasing sperm two nights before the full moon (July 2012) on the Red Sea reef Al Fahal (Saudi Arabia) (Bouwmeester 2013). Astroboa nuda are known to return to the same location on the reef at night to feed (Tsurnamal and Marder 1966), and this behaviour did not appear to be affected by their spawning activity.
Observations of natural spawning of the two sea star species have previously been described in the Red Sea on Al Fahal Reef (Bouwmeester et al. 2016). They found a single individual of M. clavigera and four individuals of L. leachi that released sperm in April, 4–5 days after the full moon, and a single L. leachi that spawned two days after the May full moon in 2014 (Bouwmeester et al. 2016). Together with our observations in June, this might indicate that both species have a relatively extended period of potential spawning, yet a more thorough assessment is needed to support this hypothesis. Other sea star species from the Red Sea have been observed to spawn in winter, spring and summer (Pearse 1968). Although both species have a relatively broad distribution range, observations of spawning are scarce. Komatsu (1973) describes a single L. leachi sea star in an aquarium, which released eggs for ~ 1 h from the dorsal–lateral parts of the arms (August 11, 1972, at 10:00 h). Very little is known about the reproduction and development of these sea stars—and tropical sea stars in general (Bos et al. 2008)—except that both species appear to produce relatively small eggs (~ 140 µm diameter) and have a planktonic-feeding larval stage (Yamaguchi 1975; Chia et al. 1993).
The holothurian P. graeffei is found throughout the wider tropical Indo-Pacific and has been recorded spawning in various locations, including Thailand (Scott et al. 2015), the South China Sea (Purwati 2003), Great Barrier Reef (Purcell et al. 2012), the Maldives, the Seychelles and Mozambique (Friedman 2008). Described individuals are generally found exhibiting the typical characteristics of sea cucumber spawning, with the anterior part of the body stretched and in a vertical position, while the posterior part of the body remained on the substrate. Similar to our observation, this species has been described spawning simultaneously with other echinoderms (Scott et al. 2015) and in most recordings two or more individuals were encountered a few meters apart. The observed P. graeffei on the Marsa Shagra reef are the first to our knowledge to be found exhibiting spawning behaviour in the Red Sea. Previously described encounters in other geographical regions occurred between 15:00 h and sunset, and the lunar phase was usually between waning crescent and new moon. The individuals encountered in the Red Sea differ from these previous sightings at they were found releasing gametes in full darkness around 20:00 h and under a waxing gibbous moon.
The only description of reproduction in T. dentatus is a case of stimulated egg release by exposing several individuals to variable temperatures in a controlled aquarium environment (Eisawy 1970). Each female released approximately 1 million eggs. The same article provides some details regarding observations of T. dentatus spawning in its natural environment, but extensive descriptions are essentially absent. Eisawy (1970) described a spawning period ranging from April until July with an approximate lunar periodicity (and at an optimum water temperature of 27–28 °C), which complies with our observations in June. The reproduction in T. dentatus appears to be comparable to other Trochidae species. Trochus niloticus males have also been observed to release sperm in the evening (18:00–22:00 h), and for an extended period of time (10 min to an hour) on the Great Barrier Reef, while females spawned for up to 15 min (Heslinga and Hillmann 1981). Although the sexes of T. dentatus are separate (Eisawy 1970), we did not observe any females releasing eggs. Spawning in Trochidae species is generally initiated by males, although females do not always spawn in response to sperm release (Heslinga and Hillmann 1981). It is possible that T. dentatus females released eggs later in the night or even several days later. Until our spawning observation, T. dentatus snails had rarely been observed on top of the reef of Marsa Shagra. Like many of the closely related Trochidae species, T. dentatus are known to spend most of their time hidden. Their increased activity and displacement to the reef surface at nights around the full moon, however, has also been described for T. niloticus (based on anecdotal evidence from fishermen).
The spawning behaviour of T. maxima appears to correspond to previous descriptions of natural gamete release in the Red Sea. The reproductive strategy of T. maxima is relatively well described (See Roa-Quiaoit (2005) and references therein). This is partly because these clams are fished and cultured for commercial purposes (food, shell craft industry and the aquarium trade) (Lucas 1994). Throughout the Red Sea, T. maxima spawn June–December (Kilada et al. 1998), although the length of the spawning season can differ due to latitudinal variations in water temperature or the availability of food (Roa-Quiaoit 2005). Female gametes reach their largest diameter in June (~ 95 µm) shortly before spawning—which coincides with the timing of our observations—and are generally released within hours after the male gametes. Like many hermaphroditic broadcast spawners, this strategy reduces the chance of self-fertilization (Lucas 1994).
Spawning observations reported here contribute to the still poorly documented spawning of non-coral invertebrates in the Red Sea and shed light on their spawning behaviour. Previous reports combined with our findings provide evidence for synchronized inter-taxa mass spawning on the coral reefs of the Red Sea. Only a few dedicated surveys to document spawning in invertebrates have been conducted in the Red Sea, and it is to be expected that many more species spawn around the same period.