The first records of deep-sea fauna – a correction and discussion

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Introduction
When books or review-papers give in their introductory section a short overview of the history of deep-sea research, the recovery of a basket star by Sir John Ross in 1818 from deep waters of the Northwest Passage is often cited as the first organism that was brought up from the deep sea (Menzies et al., 1973;Tyler, 1980;Gage and Tyler, 1991;Ramirez-Llodra et al., 2010).This is not correct.The first published record is considerably older: the upper bathyal stalked crinoid Cenocrinus asterius (Linné) was brought up, probably on fishing lines on several occasions, in the Caribbean (Thomson, 1873), and two specimens reached Europe and were already described in 1761 and 1762, respectively.In addition, several descriptions of deep-sea fishes appeared in the late 18th and early 19th century, again predating Ross' finding of the basket star.
To put these historical finds in context, we want to give in the following paragraphs an overview of the historical records of basket stars and stalked crinoids; possible explanations why the Ross expedition became uncritically cemented in the deep-sea literature, whereas the earlier finds of Cenocrinus asterius and other captures of deep-sea creatures were neglected.
For practical reasons all the depths given in the historical literature are converted to meters.

Sounding and sampling the deep sea
Sounding water depths with line and plummet had been in use since the first ships went to the oceans yet it had always been the shallow waters near the land that were in the focus of the navigators.Those soundings were used for the first time in nautical maps in the 16th century, and isobathic coastal maps were introduced in 1737 (Murray, 1895;Murray and Hjort, 1912).We here follow Gage and Tyler (1991), Herring (2002), Tyler (2003), Thistle (2003), Snelgrove and Grassle (2008) and others and let the deep sea start below 200 m.As bathyal species we we designate those that have their main distribution between 200 and 1000 m.The first scientific attempt at sounding the deep sea is ascribed to Magellan who tried in 1521 unsuccessfully to reach the bottom between two pacific coral islands with a line measuring between 180 and 360 m (Murray, 1895;Murray and Hjort, 1912).The conclusion that the expedition had here arrived at the deepest part of the ocean appears rather naïve (Murray, 1895).
The next sounding that found its way into the deep-sea literature was in an apparent depth of 1250 m, recorded in 1773 east of Iceland by Captain Constantine Phipps aboard the HMS Racehorse (Rice, 1975) but this depth must be read with caution (see below).The soundings undertaken in 1818 during the John Ross expedition searching for the Northwest passage in the Arctic (Ross, 1819)  an animal was brought up from a depth that seemed to be accurately recorded.But of course there are major problems with this expedition.The captain's diary, the shipboard recordings, and the subsequent publications were inaccurate and sometimes contradictory (Rice, 1975).The actual depths of the deepest soundings were only around half of the published values and did certainly not exceed 1100 m (Rice, 1975).The famous basket star that was allegedly caught entangled in the sounding line 370 m above the weight (!) must also have come from a depth of around 1000 m.This is still impressive, and had this result been more widely disseminated, it had perhaps prevented the uncritical prevalence of Forbes' theory of an azoic zone below 550-600 m (Forbes, 1844;Rice, 1975;Anderson and Rice, 2006).
Similar problems with a large divergence between apparent and true depth certainly apply to all the deep soundings of the early 19th century.The James Clark Ross expedition for example allegedly sounded in the Atlantic east of Brazil with a line in excess of 8400 m without reaching the bottom (Ross, 1847;Murray, 1895).Yet such depths are nowhere to be found in this region.
The scientific sampling of the deep sea received a veritable boost when dredging the seabed became possible at ever greater depths.The brilliant naturalist Edward Forbes was a pioneer in that field.By 1839 he had already dredged at various places around the northern British Isles (Anderson and Rice, 2006) and had developed a zonation of life from the littoral down to mid-shelf depths.In 1840 Forbes joined a campaign on the HMS Beacon to conduct surveys in the eastern Mediterranean.It was his work on the bathymetric distribution of life in the Aegean Sea, based on more than 100 dredgings to a depth of 240 m (Murray, 1895) that proved most influential.Forbes noted that life became ever sparser with increasing depth and concluded by interpolation that life would probably vanish below a depth of about 550 m (Forbes, 1844).Such a theory of the azoic deep sea had already been developed, e.g., by the French naturalist François Péron, who thought that the bottom of the deep sea was covered with eternal ice (!) and therefore without life (Murray, 1895).Likewise, the British geologist Henry de la Beche had postulated a lifeless deep sea on theoretical grounds (An-Figures

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Full derson and Rice, 2006), but it was the detailed investigations of Forbes that ensured a staying power for the theory of azoic deep-sea bottoms.In those days it seemed only logical that the dark, ice-cold environment without primary production where huge pressures acted would be hostile to life (Anderson and Rice, 2006).
Of course there were already in 1840 strong indications that life was present in the deep sea below 550 m.The John Ross Arctic expedition had in 1818 recovered life from much greater depths.Dredgings made between 1839 and 1843 during the Antarctic expedition of James Clark Ross had brought up samples full of life from depths up to 730 m (Murray, 1895; but again these depths must be read with caution).
Especially influential was the work of the Norwegian naturalist Michael Sars who published in 1850 a list of animals that were dredged from depths of more than 550 m off the coast of northern Norway (Murray, 1895).Later work was done together with his son Georg Ossian Sars, and they published their new finds from deep waters, including the stalked crinoid Rhizocrinus lofotensis (Sars, 1868).This new species was the first stalked crinoid to be brought up from a defined depth.It spurred considerable interest among fellow marine researchers, mainly Thomson and Carpenter, and had a large impact on the future direction of deep-sea research (see below).When a telegraph cable between Britain and America was being planned, further evidence for life at great depths was found.In 1860, Georg Charles Wallich aboard the HMS Bulldog sounded and sampled the seabed in the northern Atlantic.In one sounding to a depth of 2300 m, he found several brittle stars entangled around the rope (Wallich, 1862).For Wallich this proved that life existed at great depths and was by far the most important sounding ever (and at the same time he dismissed similar results obtained by others; see Rice et al., 1976;Rozwadowski, 2005).Yet his results and conclusions were not widely accepted, which later led him to engage in a bitter feud with Thomson and Carpenter (Rice et al., 1976).
Conclusive proof for the existence of life on very deep bottoms came when a telegraph cable laid in 1857 between Sardinia and the north African coast failed in 1860.with the cable, many animals from the seabed were recovered.Most notable were some specimens that were attached to the cable itself, especially a coral of the genus Caryophyllia that had its base moulded on the structure of the cable (Murray, 1895).Further indications for rich life at great depths came from various sources, e.g., the dredgings from Torrell's expedition to Spitsbergen in 1864, and the recovery of the glass sponge Hyalonema by fishermen, first in Japan, then in 1868 from the deep sea off Portugal (Murray, 1895).In the following years sporadic successful dredgings from deep environments were obtained, e.g., 1867 and 1868 by Pourtalès and Mitchell in the Strait of Florida down to 1555 m (Agassiz, 1888).But systematic investigations of the deep-sea floor really only commenced with the British expeditions aboard the HMS Lightning in 1868 and the HMS Porcupine in 1869/1870.The objective of these expeditions was to investigate the distribution of life on the deep-sea floors, to look for "living fossils" and to document the temperatures of Atlantic waters (Mills, 1983;Rozwadowski, 2005).Especially the Porcupine cruise was highly successful, with many dredgings full of life to a depth of more than 3500 m (Murray, 1895;Mills, 1983;Rozwadowski, 2005).It was also during these expeditions that new dredges, sounding devices and other equipment were tested for their application in deep-sea research (Mills, 1983;Rozwadowski, 2005).The results of these expeditions were also instrumental for the writing of what could be called the first textbook on deep-sea biology (Thomson, 1873).Finally, during the subsequent circumnavigation of the HMS Challenger (1872-1876) it was proven once and for all that life existed in all oceans and at all depths (although life at the greatest hadal depths, > 10 000 m, was only finally documented by the Danish deep-sea expedition aboard HDMS Galathea in 1951; Bruun, 1956).Figures
Because the echinoderm groups of the basket stars and the stalked crinoids played a crucial role in the history of deep-sea research, both these groups are treated in more detail below.

The historical record of basket stars
Most basket stars live on hard bottoms, often clinging to corals or sponges, in deeper shelf and upper bathyal environments (Lyman, 1882;Koehler, 1909;Clark, 1915;Hendler, 1996) but some also occur in water depths as shallow as 10 m as well as in abyssal depths (e.g.Clark, 1915;Emson et al., 1991;Hendler, 1996).Up to the times of the first deep-sea expeditions every finding/recovery of these animals was a lucky incident that, not least because of their strange appearance, received considerable attention.Their unusual morphology is reflected in their naming: "Caput medusae", "Gorgonocephalus", head of the medusa.They are among the largest ophiuroids and are voracious predators that feed on megaplankton (Emson et al., 1991;Rosenberg et al., 2005).
The oldest valid name is Gorgonocephalus caputmedusae (Linné, 1758)  trated the Mediterranean species (Rondelet, 1555, p. 121), which was later copied by Gessner (1558) and Aldrovandi (1602).In 1675, a northern European species was described for the first time (Martens, 1675; he gives a strange description p. 88: "The other starfish, body decagonal, below (mouth) six-rayed star"; our translation), which might indicate that this specimen was hexamerous.This was followed in 1705 by an Indo-Pacific basket star (Rumph, 1705).Linck (1733) was probably the first to recognize several distinct species, but his names predate the 10th edition of Linné's Systema Naturae and are hence not valid.Linné (1758) based his name on a specimen from Norway that he had described earlier (Linné, 1754).It is not evident why he did not mention the description of Rondelet (or Gessner), as he usually did so, but the various forms recognized by Linck (1733) were for Linné all the same.Today, of course, these are indeed recognized as different species: Rondelet's Mediterranean species is Astrospartus mediterraneus (Risso, 1826) and the one described by Martens from "Weyhegatt" (probably Weygate Straits, Svalbard) appears to be Gorgonocephalus arcticus Leach (1819), although six jaws are otherwise not known in that species (S.Stöhr, personal communication, 2014).
Rumph's species cannot be determined, as the figures do not show any key characters.However, Gorgonocephalus caputmedusae can be excluded (S.Stöhr, personal communication, 2014).Unfortunately, that name is routinely used when Rumph's specimen is discussed in the literature (e.g.Reich (2010) in his essay on the "Swabian Caput Medusae", which is the crinoid Seirocrinus subangularis (Miller, 1821) from the lower Jurassic Posidonia Shale).When describing natural wonders of the island Cuba, Parra (1787) mentioned and figured two "Estrella ramosa" that were the first published basket stars from the Caribbean.The figures are not very accurate but the specimens probably belong to Astrophyton muricatum (Lamarck, 1816), which has a rather wide distribution in the Caribbean (Hendler et al., 1986).
5 The historical record of stalked crinoids and the notion of "living fossils" The finds of stalked crinoids from deep waters of the Caribbean around 1750 must be considered the first records of deep-sea animals that were published.Yet they were not recognized as that because there were no sounding records tied to those catches, but today we know that they are bathyal species and therefore true deep-sea forms.Already then, however, it was obvious that these finds somehow related to fossils from the distant past, and the concept of "living fossils" was developed almost 100 years before Darwin (1859) introduced this term when discussing the platypus and the South American lungfish (Rudwick, 2005).Much later another species was recovered from a known depth in bathyal environment off northern Norway and immediately caught the attention of the scientific community.It was recognized both as a deep-sea animal occurring well below the depth limit for life according to Forbes and his disciples, as well as a living fossil (see section on Conocrinus lofotensis).This proved to have a major impetus for the succeeding planning of deep-sea explorations.Introduction

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Full 5.1 The "sea palm" Cenocrinus asterius Guettard (1761) described the first known stalked crinoid in detail as "Palmier marin" (Fig. 2).Linné (1767) later named it Isis asteria and Lamarck (1816) Encrinus caput medusa.It is an isocrinid and is now known as Cenocrinus asterius (Linné).The remains of the animal were kept as "palmier marin" in the cabinet (collection) of a M.
de Boisjourdain at Martinique who obtained it from an officer of a vessel making port there.Unfortunately, the exact location of the catch, presumably by a fisherman, is unknown.However, this crinoid is common in the Caribbean at 200-300 m although it has also been observed as shallow as 183 m (Macurda Jr. and Meyer, 1974).It was in fact Madame Boisjourdain who made the link between the living animal and the fossil remains of isocrinids with their pentagonal column and star-shaped columnal facets (Guettard, 1761).Guettard thus presented this animal as a survivor of a disappeared marine world whose pierres étoilées (encrinites, entroques, trochites) were topics of doubts as to their nature.Guettard seemed to have been happy to be able to resolve these doubts.He even went on to count the total number of ossicles of the crinoid and arrived at the astonishing figure of at least 128 675.This was even more than Rumph (1705) had counted for his "Caput medusae" with 81 840 ossicles.Guettard also mentioned a superficially similar animal that was caught by whale-fishers in deep waters off Greenland and described by Mylius (1753).Yet this was certainly no crinoid (Guettard 1761) but rather an umbellulid pennatulacean (see Ellis, 1755; see also Walch, 1769).Shortly thereafter a second specimen was brought to the attention of the public.It was found near Barbados and described by Ellis (1762).With only the lower part of the crown preserved it was less complete than Guettard's specimen (Fig. 3).This crinoid has survived and is now in the Hunterian Museum and Art Gallery in Glasgow (M. Reilly, personal communication, 2015).Ellis also compared his "Encrinus" to British fossils from the Lower Jurassic.In the meantime, Cenocrinus asterius has become Introduction

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Full one of the most studied living stalked crinoids, including numerous in situ observations (Baumiller et al., 1991).

Crinoid finds between 1762 and 1864
In the years after the publications of Guettard (1761) and Ellis (1762), new stalked crinoid species were sporadically recovered.They were all accidental catches from the Caribbean with no defined depth attached to them.They were largely neglected by marine biologists and had no impact on deep-sea research in the following decades.
In his description of natural objects of Cuba, Parra (1787) gave a figure and a description of another isocrinid and called it "palma animal".He also undertook the sport of counting the ossicles of this crinoid and arrived at 62 660 without counting the stalk and the cirri.His figure was later reproduced by Gervais (1835) who erected the new species Encrinus parrae.This species is today recognized as Endoxocrinus (Endoxocrinus) parrae (Gervais in Guérin, 1835), which occurs over a depth range of 154-520 m in the tropical Western Atlantic, and may be locally abundant (David et al., 2006;Améziane and Baumiller, 2007).Shortly thereafter another crinoid was described from deep waters of the Caribbean.It was the peculiar Holopus rangii d'Orbigny, 1837 which cements to the substrate (Orbigny, 1837;Grimmer and Holland, 1990).This species has been observed on hard bottoms, preferentially under overhangs, in depths between 100 and 654 m, but its main distribution is upper bathyal (Améziane et al., 1999;Donovan and Pawson, 2008).A further species, Pentacrinus muelleri, was erected by Oersted in 1856 and later described in more detail by Lütken (1864).However, P. muelleri is considered today a junior synonym of Endoxocrinus parrae (David et al., 2006).Finally, Pentacrinus decorus was described by Thomson in 1864 (see Carpenter, 1884).This species which is now known as Neocrinus decorus (Thomson, 1864) has a wide distribution from the Bahamas to Venezuela and occurs between 154 and 1220 m (Meyer et al., 1978;Pawson et al., 2009).It is semi-sessile and is capable of rapididly crawling along the bottom with the aid of its arms (Baumiller and Messing, 2007).Introduction

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Conocrinus lofotensis
In 1864 Sars mentioned the find of a new stalked crinoid named Rhizocrinus lofotensis (Fig. 4).It was dredged from a depth of about 550 m off the Lofoten Islands and belongs to the bourgueticrinids, a type known at the time only from fossils.The species, now named Conocrinus lofotensis (Sars, 1868), was described in detail by M. Sars in 1868, who contended that the deep-sea floor was a refuge for living fossils.The find caused extreme interest in the scientific world that such a living fossil, a sort of degraded Apiocrinite (Carpenter, 1884, p. 246), was still to be found in Recent seas.This first living example of a stalked crinoid recovered from a known depth was one of the reasons that Thomson and Carpenter, both interested in these animals, persuaded the British Admiralty to use the navy paddle-steamers HMS Lightning and HMS Porcupine for deep-sea dredging operations (Thomson, 1873).
It should be notet that a few years earlier, in 1853, a strange asteroid was dredged off Norway and described as Brisingia endecacnemos Asbjörnsen, 1856.Its morphology appeared intermediate between asteroids and ophiuroids, and it was therefore also considered to be an archaic species, much like the stalked crinoids (Asbjörnsen, 1856).Yet brisingids are specialized modern asteroids that use their long, flexible arms for suspension feeding (Lawrence, 1987).

Why the early records vanished from the textbooks
The John Ross expedition with its groundbreaking soundings to an alleged depth of more than 1950 m and the recovery of a basket star from such a depth was initially neglected and not cited in the pertinent literature of the early 19th century (Rice, 1975).It was only "rediscovered" after opponents of the azoic theory of Forbes were assembling the facts that would prove that animal life existed on deep-sea floors.Afterwards however and well into the 21st century, the John Ross episode became uncritically When in 1761/62 the first modern stalked crinoids were reported from the Caribbean, they came from an unknown depth and the scientific interest centered more on their Mesozoic appearance and their role as "living fossils" (e.g.Walch, 1769).The deepsea fishes that were described between 1770 and 1810 likewise came from unknown depths or even surface waters.Only later did we learn that these were bathyal species.Risso (1810) was the first to develop a bathymetric distribution scheme for fishes but this was not tied to actual soundings and open to criticism.The reasons why deep-sea organisms were not recognized as such in the 19th century were thus manyfold: deep-sea organisms brought up by fishing or sounding lines were considered for a long time less reliable than dredgings.It was suspected that organisms might have become entangled higher up in the water column.This also applied to organisms like stalked crinoids, brittlestars or basket stars that are now known to be strictly benthic (Rice, 1975).
-For demersal deep-sea fishes, a bathymetric zonation was developed only after the Challenger expedition (Günther, 1887).This took even considerably longer for bathypelagic fishes.Some researchers maintained that there was in the open ocean a zone devoid of life between the surface waters and the deep-sea bottom (Agassiz, 1888), while others believed in the existence of an intermediate fauna.
This was only settled in favor of the second opinion after the German Valdivia expedition (Chun, 1900).
- stalked crinoids (Carpenter, 1884).Murray's chapter was highly influential and inspired many subsequent historical summaries either directly or indirectly.It should therefore come as no surprise that the early finds of Caribbean crinoids were omitted in most historical introductions (e.g.Murray and Hjort, 1912;Menzies et al., 1973;Gage and Tyler, 1991;Ramirez-Llodra et al., 2010), a rare exception being Mills (1983).Murray also confounded Gorgonocephalus arcticus with G. caputmedusae (= G. linckii), and the latter name persisted in many of the above mentioned texts.
-While in the times of Forbes the deep sea started at around the shelf break, during the 20th century the deep sea was equated by many with deeper bathyal depths or the abyss, i.e., water-depths of more than 500 or 1000 m (e.g.Canganella and Kato, 2007).This was perhaps an additional reason that the historical finds of bathyal animals were neglected.

Conclusions
The published record of deep-sea organisms goes back to the middle of the 18th century.Stalked crinoids from the Caribbean were the first among these early records.Originally they were not perceived as deep-sea animals yet were instrumental in developing the concept of "living fossils".Consequently, these finds were discussed in the paleontologic literature but largely omitted in the field of marine biology.
When the systematic exploration of the deep sea commenced during the early 19th century, only dredgings from a "known" depth (even if that depth-sounding was grossly in error) were accepted by the scientific community as reliable indicators of deep-sea life.Apart from 1860, epizoans on telegraph cables that were brought up for repair also became accepted as proof of life in the deep sea.The catch of a basket star at great depths during the John Ross expedition only became scientific Thomson, Carpenter and others started to assemble the facts that would disprove Forbes' theory of the azoic deep sea.Accidental catches that would emerge as important evidence of deep-sea life such as those of stalked crinoids from the Caribbean persistently remained neglected through much of the 20th century.This has much to do with the lasting influence of Murray's remarkable chapter on the history of oceanography and deep-sea research in the Challenger report summary (Murray, 1895) from which some errors and omissions were perpetuated in the newer literature.It is therefore important that the historical literature is carefully read, evaluated and compared with the original sources, and summary treatments from the 20th and 21st century should not be uncritically followed.Introduction

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deep soundings and dredgings up to the times of the Challenger expedition; Discussion Paper | Discussion Paper | Discussion Paper | with alleged depths of up to 1950 m in Baffin Bay appeared like a quantum leap.Furthermore, for the first time Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | The 70 km brought up for repair came from a depth of more than 2000 m, and, together Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | but different basket stars were already recorded earlier.Rondelet described and nicely illus-Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Ramirez-Llodra et al., 2010; see Leach, 1819).Ross' specimen is perhaps still in the possession of the Natural History Museum in London Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | cemented in the deep-sea literature.Discussion Paper | Discussion Paper | Discussion Paper | In his masterly treatment of the history of deep-sea research, Murray (1895) gathered all the results of deep-sea explorations that pointed to rich life on deep-sea floors, as had Thomson (1873) done before with lesser depth.It was these texts that hailed John Ross' expedition as an early record-breaking cruise and took the published results at face value.At the same time Murray omitted (in contrast to Thomson, 1873) the occurrences of the deep-water stalked crinoids from the Caribbean, although they were of course treated in the Challenger report on the Introduction Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper |