Bembridae
View in CoL
View at ENA
,
Hoplichthyidae
,
Platycephalidae
, and
Triglidae
.—
Traditionally, the
Bembridae
,
Hoplichthyidae
, and
Platycephalidae
have been treated as a single evolutionary unit ( Matsubara, 1943; Washington et al., 1984; Fig. 1
View FIG
). As first noted by Imamura (1996), explicit analyses of ‘‘platycephaloid’’ relationships do not recover bembrids in a clade with the hoplichthyids and platycephalids. Instead, Imamura’s (1996) study demonstrated that
Platycephalidae
was sister to a clade of
Hoplichthyidae
þ
Triglidae
. These three families were then hypothesized to be sister to
Bembras
, and that clade was subsequently hypothesized to be sister to
Parabembras
( Imamura, 1996; Fig. 1
View FIG
). Our results support Imamura’s (1996) hypothesis that
Platycephalidae
is sister to a clade composed of
Hoplichthyidae
þ
Triglidae
. However, our results place this
Hoplichthyidae
þ
Platycephalidae
þ
Triglidae
clade sister to all other scorpaenoids. This relationship supports the view that the less flattened bembrids are more closely related to scorpionfishes and stonefishes than to hoplichthyids, platycephalids, and triglids.
The
Bembridae
View in CoL
is a small, deep-water Indo-Pacific marine family whose limits have varied across studies. Jordan and Hubbs (1925) first separated the
Parabembridae
View in CoL
from the
Bembridae
View in CoL
, but this separation was not followed in most subsequent studies. For example, Washington et al. (1984) and Nelson (2006) included
Bambradon
View in CoL
,
Bembradium
View in CoL
,
Bembras
View in CoL
,
Brachybembras
View in CoL
(not discussed in Washington et al. [1984]), and
Parabembras
View in CoL
in their
Bembridae
View in CoL
. Imamura (1996) not only recognized a separate
Bembridae
View in CoL
and
Parabembridae
View in CoL
, but he also classified one traditional bembrid,
Bembradium
View in CoL
, as a member of the
Plectrogeniidae
View in CoL
. Molecular studies have not sufficiently sampled the
Bembridae
View in CoL
, and they have recovered their included bembrids sister to
Congiopodidae
View in CoL
,
Hoplichthyidae
View in CoL
,
Platycephalidae
View in CoL
,
Plectrogeniidae
View in CoL
,
Synanceiidae
View in CoL
, or a clade composed of the
Bembropidae
þ
Scorpaenidae
View in CoL
( Smith and Wheeler, 2004, 2006; Smith and Craig, 2007; Lautredou et al., 2013; Near et al., 2013; Smith et al., 2016; Betancur-R. et al., 2017). Molecular studies that have included
Bembras
View in CoL
and
Parabembras
View in CoL
have consistently resulted in these genera forming a clade ( Near et al., 2013, 2015; Betancur-R. et al., 2017), thus not requiring the recognition of a separate family-level status for
Parabembridae
View in CoL
. The current study is the first study with molecular data that included
Bembradium
View in CoL
,
Bembras
View in CoL
, and
Parabembras
View in CoL
. Given the alignment of
Bembradium
View in CoL
with
Plectrogenium
View in CoL
and the separate grouping of
Bembras
View in CoL
and
Parabembras
View in CoL
, we recommend classifying
Bambradon
View in CoL
,
Bembras
View in CoL
,
Brachybembras
View in CoL
, and
Parabembras
View in CoL
as a revised
Bembridae
View in CoL
(Appendix 2). Further, and as discussed below, our findings support the results of Imamura (1996) who placed
Bembradium
View in CoL
and
Plectrogenium
View in CoL
in the
Plectrogeniidae
View in CoL
. We recovered the
Bembridae
View in CoL
sister to a clade composed of
Neosebastidae
View in CoL
þ
Plectrogeniidae
View in CoL
þ
Scorpaenidae
View in CoL
þ
Synanceiidae
View in CoL
( Fig. 3
View FIG
). This sister group relationship is supported by the loss of the lateral-line canal on the pterotic (character 22, state 0), two spines on the first dorsal-fin pterygiophore (character 56, state 0), and the presence of an adductor dorsalis (character 100, state 0).
The
Hoplichthyidae
View in CoL
is an Indo-Pacific marine family of 17 species that has been variously classified among mail-cheeked fishes but has been allied generally with the platycephalids. Traditional higher-level phylogenetic studies (e.g., Gill, 1888; Regan, 1913; Matsubara, 1943; Quast, 1965; Washington et al., 1984) placed the hoplichthyids as a separate family, closely related to the platycephalids. Greenwood et al. (1966) had a similar classification, but they treated the hoplichthyids as their own suborder, Hoplichthyoidei. Winterbottom (1993) suggested that the hoplichthyids might even be close relatives to the gobioids, so the family’s placement has been historically varied. As noted above, Imamura (1996) first suggested that hoplichthyids are more closely related to the triglids than the platycephalids, and his results suggested that
Hoplichthys
View in CoL
was sister to a clade composed of
Peristedion
View in CoL
þ
Satyrichthys
View in CoL
. Molecular data, beginning with Smith and Wheeler (2004), have suggested alternative placements for the hoplichthyids ranging from a close relationship with Ovalentaria to sister to the
Bembridae
View in CoL
,
Normanichthyidae
View in CoL
,
Synanceiidae
View in CoL
, a clade composed of
Bembridae
View in CoL
þ
Platycephalidae
View in CoL
, a clade composed of the ‘‘cottoids and allies’’ (Anoplopomatoidei, Cottoidei, Gasterosteioidei, Hexagrammoidei, and Zaniolepidoidei) þ
Triglidae
View in CoL
, a clade composed of Cottoidei þ Gasterosteioidei þ Hexagrammoidei þ
Triglidae
View in CoL
þ Zoarcoidei, and a clade composed of the ‘‘cottoids and allies’’ þ
Scorpaenidae
View in CoL
þ
Triglidae
View in CoL
( Smith, 2005; Smith and Wheeler, 2006; Smith and Craig, 2007; Lautredou et al., 2013; Near et al., 2013, 2015; Smith et al., 2016; Betancur-R. et al., 2017; Fig. 2
View FIG
). Our results ( Fig. 3
View FIG
) place the
Hoplichthyidae
View in CoL
sister to the
Triglidae
View in CoL
, similar to the findings of Imamura (1996, 2004; Fig. 1
View FIG
). This sister group relationship is supported by the presence of tubercles on the neurocranium (character 13, state 1), the loss of one postcleithrum (character 48, state 1), the increase in the number of free pectoral-fin rays to three or more (character 49, state 3), the fusion of the cartilaginous caps on the anterior portion of the pelvis (character 51, state 1), the presence of a hyohyoides inferioris (character 84, state 1), the attachment of dorsal elements of pelvic-fin muscles to the pectoral girdle (character 97, state 1), and the obliquus superioris bypassing and lying ventrally to Baudelot’s ligament (character 104, state 1). As with the
Congiopodidae
View in CoL
, the placement of the hoplichthyids is inconsistent across studies. Most studies ally the hoplichthyids more with the
Triglidae
View in CoL
(often combined with the included ‘‘cottoids and allies’’). Given the ambiguity, we recommend treating the
Hoplichthyidae
View in CoL
, diagnosed by 20 morphological synapomorphies (Appendix 2), as a separate scorpaenoid family.
The
Platycephalidae
View in CoL
is a modestly large family of 84 species that is found in brackish and marine environments in the Indo-Pacific region ( Nelson, 2006). As has been found in previous studies, the
Hoplichthyidae
View in CoL
and
Platycephalidae
View in CoL
were recovered as independent monophyletic groups with the traditional limits ( Keenan, 1991; Imamura, 1996; Appendix 2; Fig. 3
View FIG
). The interrelationships of the family have been discussed above, and our results support the findings of Imamura (1996) that the
Triglidae
View in CoL
þ
Hoplichthyidae
View in CoL
is recovered as the sister group to the platycephalids. This sister group relationship is supported by the presence of a tooth plate on the second epibranchial (character 39, state 1). Additionally, our limited sampling of platycephalids corroborates the phylogeny and classification presented in Imamura (1996).
The
Triglidae
View in CoL
is a large family of 171 species that are found in tropical, temperate, and deep-water habitats across all oceans ( Nelson, 2006). Traditional classifications (e.g., Gill, 1888; Matsubara, 1943; Washington et al., 1984; Imamura, 1996;
Eschmeyer
View in CoL
et al., 2017) often treat the
Peristediidae
View in CoL
and
Triglidae
View in CoL
as independent, closely related families. Our study corroborates the findings of Smith (2005) and Portnoy et al. (2017) that place the traditional peristediids (our peristediines) within the
Triglidae
View in CoL
. Other than the placement of peristediines inside the triglids, our hypothesized relationships support the phylogenies of Imamura (1996) and Richards and Jones (2002). Similarly, our phylogeny supports the phylogeny of Portnoy et al. (2017), including the placement of peristediines inside the
Triglidae
View in CoL
. This placement and resulting expansion (and monophyly) of the
Triglidae
View in CoL
is supported by both morphological and molecular data, and our study recovers seven characters supporting the monophyly of this expanded family (Appendix 2).
Neosebastidae
View in CoL
and
Plectrogeniidae
View in CoL
.— The placement of
Neosebastidae
View in CoL
and
Plectrogeniidae
View in CoL
has been historically problematic; they are often represented as early diverging scorpaenoid lineages or ‘‘ancestral’’ forms ( Matsubara, 1943; Imamura, 1996). Although the current study is the first study to unite these two families ( Fig. 3
View FIG
), Imamura (2004), Smith and Wheeler (2004, 2006), Smith and Craig (2007), and Smith et al. (2016) have often found them relatively closely related. In this study, this sister-group relationship was supported by the separation of the first and second hypurals (character 68, state 0).
The
Neosebastidae
View in CoL
is a predominantly anti-tropical Indo-Pacific marine family of 18 species that has been often separated from the core scorpionfishes in a separate family or subfamily in modern phylogenies and classifications ( Imamura, 2004; Motomura, 2004; Nelson, 2006). Beginning with Matsubara (1943) and supported by Washington et al. (1984) and Nelson (2006), the
Neosebastidae
View in CoL
has been treated as a separate subfamily (Neosebastinae) of the
Scorpaenidae
View in CoL
. Matsubara (1943) hypothesized that the neosebastids were allied with the sebastines, and Ishida (1994; Fig. 1
View FIG
) allied the neosebastids with the setarchines and recognized them as a separate family. Imamura (2004; Fig. 1
View FIG
) also recognized the clade as a separate family and suggested a non-scorpaenid relationship for the neosebastids; he resolved them with the more flattened scorpaenoids in the families
Bembridae
View in CoL
,
Hoplichthyidae
View in CoL
,
Platycephalidae
View in CoL
,
Plectrogeniidae
View in CoL
, and
Triglidae
View in CoL
. Molecular studies have grouped the neosebastids with several non-scorpaenoid groups (e.g.,
Acanthistius
View in CoL
or bembropids; Smith and Wheeler, 2006; Smith et al., 2016) or with congiopodids ( Smith and Wheeler, 2004; Smith and Craig, 2007). Our finding of a
Neosebastidae
View in CoL
þ
Plectrogeniidae
View in CoL
clade adds additional complications to the placement of the
Neosebastidae
View in CoL
, but this result is closer to the findings of Imamura (2004) and several molecular studies (e.g., Smith and Wheeler, 2004, 2006) that have plectrogeniids among the closest relatives of the neosebastids.
Species in the
Plectrogeniidae
View in CoL
are relatively widespread with collections ranging from the western Indian Ocean to Hawaii despite the family including just four species ( Imamura, 1996; Nelson, 2006;
Eschmeyer
View in CoL
et al., 2017). Fowler (1938) first emphasized the distinctiveness of
Plectrogenium
View in CoL
. Matsubara (1943) supported Fowler’s (1938) assertion, suggesting that the genus may represent the ancestral condition of some of the deeper water, flattened scorpaenoids. He noted that
Plectrogenium
View in CoL
shared the loss of the gas bladder and the presence of several rows of prominent head spines and notched pectoral fins with some scorpaenids (e.g.,
Sebastolobus
View in CoL
) while also showing characteristics in common with the bembrids. Washington et al. (1984) further corroborated this hypothesis by pointing to similarities in the scales and caudal fin between
Parabembras
View in CoL
and
Plectrogenium
View in CoL
. Subsequently, Imamura (1996, 2004) supported a placement of an expanded
Plectrogeniidae
View in CoL
(including
Bembradium
View in CoL
) sister to the clade composed of
Bembridae
View in CoL
þ
Hoplichthyidae
View in CoL
þ
Platycephalidae
View in CoL
þ
Triglidae
View in CoL
that was united by the presence of a posterior pelvic fossa. Molecular studies have not fully supported or refuted these morphological hypotheses. Smith and Wheeler (2004) and Smith and Craig (2007) recovered
Plectrogenium
View in CoL
sister to
Bembridae, Lautredou et al. (2013)
View in CoL
recovered
Bembradium
View in CoL
sister to
Synanceiidae
View in CoL
(their analysis did not include any bembrids), and Smith et al. (2016) recovered
Plectrogenium
View in CoL
sister to the
Scorpaenidae
View in CoL
. This is the first molecular study to include both
Bembradium
View in CoL
and
Plectrogenium
View in CoL
, and we found a unique relationship for plectrogeniids sister to
Neosebastidae
View in CoL
. The monophyly of the
Plectrogeniidae
View in CoL
(Appendix 2) is supported by five characters and corroborates Imamura’s (1996) hypothesis and the recognition of this distinct family.
Scorpaenidae
View in CoL
and
Synanceiidae
View in CoL
.— The scorpaenids and synanceiids are the most species-rich clades of scorpaenoids, and the species in these families have often been classified together in whole or in part. Gill (1888) grouped these clades together to the exclusion of all other mail-cheeked fishes. Regan (1913) modified Gill’s (1888) arrangement and united scorpaenids, synanceiids, and triglids in his
Scorpaeniformes
View in CoL
(their studies did not include any representatives of the
Neosebastidae
View in CoL
or
Plectrogeniidae
View in CoL
). Matsubara (1943; Fig. 1B
View FIG
) distributed the core scorpionfishes across his ‘‘ Cocotropus- stem,’’ ‘‘ Scorpaena- stem,’’ and ‘‘
Sebastes
View in CoL
-stem’’ based primarily on circumorbital differences. His ‘‘
Cocotropus
View in CoL
-stem’’ was composed of the Japanese synanceiids. His ‘‘
Scorpaena
View in CoL
-stem’’ was composed of
Plectrogenium
View in CoL
and all non-sebastine scorpaenids. Finally, his ‘‘
Sebastes
View in CoL
- stem’’ was composed of the
Neosebastidae
View in CoL
and Sebastinae. The classification of Washington et al. (1984) largely followed Matsubara (1943) except that they combined his ‘‘
Scorpaena
View in CoL
- stem,’’ ‘‘
Sebastes
View in CoL
-stem,’’
Synanceiinae
,
Apistus
View in CoL
, and
Cheroscorpaena
View in CoL
into their more inclusive
Scorpaenidae
View in CoL
. They distributed the remaining synanceiids across four additional families (
Aploactinidae
View in CoL
,
Gnathanacanthidae
View in CoL
,
Pataecidae
View in CoL
, and
Tetrarogidae
View in CoL
) and recognized
Caracanthus
View in CoL
as a distinct family from the
Scorpaenidae
View in CoL
. Ishida’s (1994) phylogenetic hypothesis ( Fig. 1C
View FIG
) and classification recognized 12 families. As noted above, this phylogeny included
Congiopodidae
View in CoL
,
Neosebastidae
View in CoL
, and
Plectrogenium
View in CoL
nested among the included representatives of the
Scorpaenidae
View in CoL
and
Synanceiidae
View in CoL
. Ishida’s (1994) major groupings largely followed Washington et al. (1984) except that Ishida often recognized clades at higher taxonomic levels. Ishida (1994) elevated Washington et al.’s (1984) Apistinae, Neosebastinae, and Setarchinae to the family level. Ishida’s (1994)
Sebastidae
View in CoL
included Washington et al.’s (1984) Plectrogeniinae, Sebastolobinae, and Sebastinae. Ishida’s (1994) classification included a
Synanceiidae
View in CoL
that incorporated Washington et al.’s (1984)
Choridactylinae
,
Minoinae
, and
Synanceiinae
. Finally, his
Scorpaenidae
View in CoL
was restricted to Washington et al.’s (1984)
Pteroinae
and
Scorpaeninae
. As noted by Smith and Wheeler (2004), a computer-aided re-analysis of Ishida’s (1994) matrix recovered many equally optimal trees that were shorter than the tree presented by Ishida (1994). This large assortment of most parsimonious trees resulted in a poorly resolved phylogeny with just three of his families represented by more than one species being recovered as monophyletic:
Aploactinidae
View in CoL
,
Congiopodidae
View in CoL
, and
Pataecidae
View in CoL
. Relative to Ishida (1994), Imamura (2004; Fig. 1D
View FIG
) increased the taxon sampling among closely related groups (e.g.,
Platycephalidae
View in CoL
,
Triglidae
View in CoL
) and recovered a largely complementary phylogenetic classification with a few changes. Imamura (2004) recognized a Sebastolobidae at the family level and relegated the
Setarchidae
View in CoL
of Ishida (1994) to a clade within
Scorpaenidae
View in CoL
. Subsequent work by Shinohara and Imamura (2005) also placed
Caracanthus
View in CoL
into the
Scorpaenidae
View in CoL
. Most recently, Honma et al. (2013) recognized a new family
Perryenidae
View in CoL
for a member of Mandrytza’s (2001)
Tetrarogidae
View in CoL
. This new family and Mandrytza’s (2001) earlier treatment of
Eschmeyeridae
View in CoL
as an additional monotypic family based on former waspfishes casts doubt on tetrarogid monophyly. The proliferation of new waspfish families and Smith and Wheeler’s (2004) re-analysis of Ishida’s (1994) dataset that recovers 5–6 distinct clades of tetrarogids (sensu Ishida, 1994) highlights that traditional ‘‘stonefish’’ taxonomy is becoming complicated with substantial evidence for tetrarogid polyphyly and a diversity of families with three or fewer species (traditional
Apistidae
View in CoL
,
Eschmeyeridae
View in CoL
,
Gnathanacanthidae
View in CoL
,
Pataecidae
View in CoL
, and
Perryenidae
View in CoL
).
As seen with the morphological studies, molecular phylogenies that have included representatives of both the
Scorpaenidae
View in CoL
and
Synanceiidae
View in CoL
have recovered varied phylogenetic results, but the clades themselves have been largely repeated. These studies have also echoed some morphological results. For example, molecular studies, like morphological studies, consistently recover a polyphyletic
Tetrarogidae (sensu Ishida, 1994)
View in CoL
and
Plectrogenium
View in CoL
separate from the sebastines ( Smith and Wheeler, 2004, 2006; Smith and Craig, 2007; Smith et al., 2016). The molecular results have also largely recovered reciprocally monophyletic scorpaenid and synanceiid clades. Smith and Wheeler (2004) recovered independent clades of the
Scorpaenidae
View in CoL
and
Synanceiidae
View in CoL
with a diversity of included taxa (including non-scorpaeniforms) in the MRCA. Smith and Wheeler (2006) recovered the scorpaenids sister to epinephelids and synanceiids sister to the triglids with an MRCA that includes the ‘‘cottoids and allies’’ as well as scorpaenoid and serranid fishes. Smith and Craig (2007) recovered relationships similar to Smith and Wheeler (2006) except that the MRCA excluded the
Epinephelidae
and included the
Anthiadidae
,
Niphonidae
,
Percidae
View in CoL
,
Serranidae
View in CoL
, and
Trachinidae
View in CoL
. With more families sampled, Lautredou et al. (2013) and Smith et al. (2016) recovered a clade composed of
Plectrogeniidae
View in CoL
þ
Scorpaenidae
View in CoL
þ
Synanceiidae
View in CoL
. Finally, Betancur-R. et al. (2017) recovered a clade composed of
Scorpaenidae
View in CoL
þ
Synanceiidae
View in CoL
, but their analysis only included two synanceiids and did not include any congiopodids, neosebastids, or plectrogeniids, so their phylogeny is of limited comparative value. Our current analysis is the first to recover a clade composed of
Neosebastidae
View in CoL
þ
Plectrogeniidae
View in CoL
þ
Scorpaenidae
View in CoL
þ
Synanceiidae
View in CoL
, and this clade was supported by the loss of the fourth circumorbital (character 9, state 1).
Despite continued iterative improvement, the march toward a monophyletic taxonomy based on morphological and molecular data has been incompletely accepted by the major fish classifications (e.g., Nelson, 2006; Nelson et al., 2016;
Eschmeyer
et al., 2017). For example, Nelson (2006) largely follows the pre-phylogenetic study of Washington et al. (1984) except for the placement of Ishida’s (1994)
Tetrarogidae
in their
Scorpaenidae
. Nelson et al. (2016) followed Nelson (2006) except they placed
Caracanthus
in the
Scorpaenidae
and recognized
Eschmeyeridae
as a separate family from their Tetraroginae. Curiously, they left the Tetraroginae within the
Scorpaenidae
and continued to recognize
Perryena
in the
Congiopodidae
despite the evidence for both tetrarogine changes being presented in the same study ( Mandrytza, 2001). In contrast,
Eschmeyer
et al. (2017) largely followed Ishida (1994) except for the placement of
Caracanthus
in the
Scorpaenidae
(presumably following Shinohara and Imamura, 2005) and the recognition of a separate
Plectrogeniidae
(presumably following Imamura, 1996),
Eschmeyeridae
(presumably following Mandrytza, 2001), and
Perryenidae
(presumably following Honma et al., 2013). Betancur-R. et al. (2017) largely followed
Eschmeyer
et al. (2017) including the retention of a nonmonophyletic (in their study)
Scorpaenidae
. Presumably, their minimal changes relative to
Eschmeyer
et al. (2017) are due to limited sampling where only 11 of their 21 platycephaloid, scorpaenoid, or trigloid families were examined. All of these previous studies highlight the need to combine molecular and morphological data to generate a complete and holistic phylogenetic hypothesis that can become stable and more widely accepted.
The
Scorpaenidae
View in CoL
is a worldwide marine family of 370 species that have been collected in environments ranging from shallow to deep water and from the poles to the tropics ( Nelson, 2006;
Eschmeyer
View in CoL
et al., 2017). This group includes the traditional
Caracanthidae
,
Scorpaenidae
View in CoL
,
Sebastidae
View in CoL
, and
Setarchidae
View in CoL
(sensu Ishida, 1994; Appendix 2) and includes animals with reproductive modes ranging from more traditional broadcast spawning to live birth ( Breder and Rosen, 1966; Muñoz, 2010). Most inexplicit and explicit morphological studies and one large-scale molecular study generally have resolved the rockfishes (Sebastinae) as an ancestral or stem grade within the scorpaenoid radiation ( Matsubara, 1943; Ishida, 1994; Imamura, 1996, 2004; Lautredou et al., 2013). In contrast, Smith and Wheeler (2004, 2006), Smith and Craig (2007), Smith et al. (2016), and Betancur-R. et al. (2017) have recovered the Sebastinae as a deeply nested lineage. This revised phylogenetic hypothesis implies that the scorpaenoids originated in warmer waters and transitioned to deeper (e.g., Setarchinae) and colder habitats (e.g., Sebastinae) rather than the previous hypotheses that would necessitate transitioning from cooler waters into more temperate and tropical regions. This more traditional hypothesis may have been largely driven by the evolutionary perspective that the colder, overwhelmingly North Pacific cottoids and allies were the closest allies to a sebastine-stem scorpaenoid radiation ( Smith and Busby, 2014). This Sebastinae was resolved as the sister group to a clade composed of
Adelosebastes
View in CoL
þ
Sebastolobus
View in CoL
, which have generally been allied with or nested among the core sebastines in previous morphological and molecular studies ( Figs. 1
View FIG
, 2
View FIG
). As might be expected with the revised placement of these core rockfishes, we recover this clade nested within a larger assemblage that includes all other sampled deeper and cooler water genera (i.e.,
Ectreposebastes
View in CoL
,
Pontinus
View in CoL
,
Setarches
View in CoL
, and
Trachyscorpia
View in CoL
). In this study, this colder-habitat clade of scorpaenids was recovered as the sister group to a
Scorpaenodes
View in CoL
þ
Pteroinae
clade. This is in contrast to several previous studies (e.g., Imamura, 2004; Smith and Craig, 2007) that have found multiple clades of deep-water scorpaenoids sister to the pteroine lionfishes and allies ( Figs. 1
View FIG
, 2
View FIG
). One of the most consistent results across scorpaenid studies is the sister-group relationship between
Scorpaenodes
View in CoL
and pteroine lionfishes (e.g., Ishida, 1994; Imamura, 2004; Lautredou et al., 2013; Smith et al., 2016; Betancur-R. et al., 2017). The final scorpaenid clade recovered in our analysis is a primarily tropical and subtropical clade composed of
Caracanthus
View in CoL
,
Pteroidichthys
View in CoL
,
Scorpaena
View in CoL
,
Scorpaenopsis
View in CoL
, and
Taenionotus
. This clade was sister to the cold-water scorpaenoids þ lionfishes and allies and has been consistently recovered in molecular studies ( Smith and Craig, 2007; Lautredou et al., 2013; Smith et al., 2016; Betancur-R. et al., 2017). In contrast, morphological studies have typically recovered these fishes as a grade with
Scorpaenodes
View in CoL
and
Pteroinae
(and potentially other genera) nested within the group ( Ishida, 1994; Shinohara and Imamura, 2005). It is clear that the inversion of scorpaenid relationships with sebastines deeply nested with the family that is recovered in this combined study and several other molecular studies ( Smith and Wheeler, 2004, 2006; Smith and Craig, 2007; Smith et al., 2016; Betancur-R. et al., 2017) has dramatically altered the polarity of morphological transformations and the impact this has on the evolutionary relationships in this commercially important clade.
The
Synanceiidae
View in CoL
, a family of 133 species, is primarily a marine clade with a few fresh- or brackish-water representatives (e.g.,
Gymnapistes
View in CoL
,
Neovespicula
View in CoL
) that is distributed from the western Indian Ocean to the South Pacific Ocean (
Eschmeyer
View in CoL
and Rama-Rao, 1973; Nelson, 2006). The largest taxonomic change we are recommending in this study is the consolidation of the traditional
Apistidae
View in CoL
,
Aploactinidae
View in CoL
,
Eschmeyeridae
View in CoL
,
Gnathanacanthidae
View in CoL
,
Pataecidae
View in CoL
,
Perryenidae
View in CoL
,
Synanceiidae
View in CoL
, and
Tetrarogidae
View in CoL
(all sensu
Eschmeyer
View in CoL
et al., 2017) into a monophyletic
Synanceiidae
View in CoL
. This expanded
Synanceiidae
View in CoL
is diagnosed by the evolution of the lachrymal saber as well as five additional morphological transformations (Appendix 2). Additionally, Leis and Rennis (2000) provided evidence from larval morphology that separates these fishes from the remainder of the core scorpaenoids. We recommend this higher-level change because of the proliferation of family-level names that are already emanating from the former
Tetrarogidae
View in CoL
(i.e.,
Eschmeyeridae
View in CoL
,
Perryenidae
View in CoL
) and that are likely to continue. Our results, previous molecular studies ( Smith and Wheeler, 2004, 2006; Smith and Craig, 2007; Smith et al., 2016), and the computer aided re-analysis of Ishida’s (1994) scorpaenoid study in Smith and Wheeler (2004) that have all sampled multiple species of tetrarogids (sensu
Eschmeyer
View in CoL
et al., 2017) have suggested that upwards of four or five additional small or monogeneric families will likely be needed to generate a monophyletic taxonomy. Instead of describing a diversity of new waspfish families, the alternative strategy is chosen here where the diversity of existing comparatively small families of stonefishes and waspfishes can be consolidated into a single, well supported, consistently supported, and taxonomically stable family with the retention of subfamilies as warranted and needed (e.g., Apistinae, Aploactininae, Pataecinae,
Synanceiinae
). Further, our classification largely returns the subfamilial taxonomy to that recommended by Matsubara (1943). Our results recover the typical placement for the Apistinae as the earliest diverging lineage in the
Synanceiidae
View in CoL
. Regan (1913) included this group among his
Scorpaenidae
View in CoL
, which was composed of our
Scorpaenidae
View in CoL
,
Apistus
View in CoL
,
Erisphex
View in CoL
(an aploactine), and six genera of ‘‘tetrarogids’’ (sensu Ishida, 1994). Matsubara (1943), Ishida (1994), and Imamura (2004) all treated
Apistus
View in CoL
as the earliest branching lineage in his clade that is largely equivalent to our
Synanceiidae
View in CoL
. The placement of Apistinae is one of the most consistently recovered relationships in scorpaenoid phylogenetics, but it is important to note that Washington et al. (1984) highlighted a number of features that potentially group the Apistinae with the
Triglidae
View in CoL
: a bilobed gas bladder with an intrinsic muscle, elongate pectoral-fin rays (also found in hoplichthyids,
Choridactylus
View in CoL
,
Inimicus
View in CoL
, and
Minous
View in CoL
), and an expansion of the circumorbitals. Thus, continued work is warranted. Our phylogeny, like previous morphological studies ( Ishida, 1994; Imamura, 2004), recovers a monophyletic
Synanceiinae
deeply nested within the
Synanceiidae
View in CoL
. Our study recovers a clade composed of the Aploactininae and Pataecinae sister to the restricted
Synanceiinae
. Other than his inclusion of the
Congiopodidae
View in CoL
in this clade, Ishida (1994) recovered this same relationship. Finally, we have a grade composed of the various ‘‘tetrarogid’’ or formerly ‘‘tetrarogid’’ genera and
Gnathanacanthus
View in CoL
as a diversity of lineages more closely related to
Synanceiinae
than to Apistinae.
Evolution of the
Scorpaenoidei
.— The combined morphological and molecular phylogeny presented herein provides an opportunity to reconcile the often conflicting datasets and look at the implications for this updated hypothesis on the evolution of this species-rich clade. One of the major findings in this study was the discovery of the lachrymal saber. As noted above, this specialization is hypothesized to have a primarily defensive role. The maxillary rotation of the lachrymal saber has two major anti-predator impacts. First, it expands the width of the head by projecting the spine(s) outward ( Figs. 4– 7
View FIG
View FIG
View FIG
View FIG
). This expansion increases the rostral width of the fish by 10– 25% and would greatly increase the gape required by a would-be predator ( Price et al., 2015). Second, the presence of an outwardly directed and sharp spine should reduce predation because of the potential for the saber to pierce a would-be predator. Cowan (1969) described a similar defensive role for the outward projection of the preopercular spines in the closely allied psychrolutids that have enlarged antler-like modifications (e.g.,
Enophrys
View in CoL
,
Icelinus
View in CoL
; Yabe, 1985). In addition to its role in avoiding or reducing predation, it is possible that the lachrymal saber is used for intraspecific competition. As seen in the evolution of antlers and horns ( Chapman, 1975), the lachrymal saber could play a role when synanceiids compete for mates or territories. The one synanceiid species examined for biofluorescence (
Centropogon australis
View in CoL
) had a green fluorescent lachrymal saber that contrasted with nonfluorescent or red-fluorescent regions on the head of these animals ( Fig. 9
View FIG
). Recent studies (e.g., Sparks et al., 2014; Anthes et al., 2016; Gruber et al., 2016) have demonstrated that a number of fish groups have green and red fluorescence that appears to be playing an ecological and/or evolutionary role. As such, it is possible that the synanceiids could be advertising or highlighting this specialization with this fluorescence in a similar role as the bioluminescence associated with the defensive dorsal spines in etmopterid sharks ( Claes et al., 2013) or that the lachrymal saber is involved in intraspecific competition and mate choice where synanceiid species are advertising their sabers to conspecifics.
In addition to exploring the evolution of the lachrymal saber, the revised scorpaenoid hypothesis has implications for the evolution of viviparity in this clade. The deeply nested placement of Sebastinae within the
Scorpaenidae
corroborates Wourms’ (1991) assertion about the evolution of live birth and corresponding intermediate stages in the transition from an ovuliparous (classical oviparous) ancestor among the non-scorpaenid scorpaenoids. As noted by Smith and Wheeler (2004), there appears to be an evolutionary transition from a more common ovuliparous ancestor in the platycephalids, synanceiids, and triglids to an oviparous species that releases fertilized eggs within a gelatinous egg mass in genera such as
Dendrochirus
,
Pterois
,
Scorpaena
,
Scorpaenodes
,
Scorpaenopsis
, and
Sebastolobus
( Wourms, 1991; Koya and Muñoz, 2007). This intermediate reproductive mode is further modified in
Helicolenus
where species in the genus have internal fertilization and zygoparity where fertilized ova are held by the mother before being released into the ocean ( Wourms, 1991). The reproductive mode of
Hozukius
is unknown, but it shares a II-3 ovarian type with most scorpaenids (e.g.,
Caracanthus
,
Dendrochirus
,
Helicolenus
,
Scorpaena
; Cole, 2003; Koya and Muñoz, 2007). The more derived viviparous sebastine rockfishes (
Sebastes
and
Sebastiscus
) have a type II-1 ovarian type ( Koya and Muñoz, 2007). This suggests that
Hozukius
is likely to be more similar to
Helicolenus
or
Scorpaena
and not be live bearing. The evolution of reproductive modes and live birth in scorpaenoids has been discussed in considerably more detail in other studies ( Wourms, 1991; Koya and Muñoz, 2007; Muñoz, 2010; Pavlov and Emel’yanova, 2013), but their interpretations have implicitly or explicitly relied on the hypothesized placement of sebastines at the base of the scorpaenoid tree. The inversion of the phylogeny of scorpaenoids proposed in this study is more consistent with traditional views on the evolution of viviparity where there is a transition from external fertilization to internal fertilization with the retention of either the developing eggs or embryos within the mother ( Wourms, 1991; Wourms and Lombardi, 1992). These are two examples demonstrating the impact of the proposed phylogeny on the evolution of the scorpaenoid fishes. We hope that this revised hypothesis for the relationships of scorpionfish and allies will allow researchers to test additional evolutionary hypotheses for this important percomorph clade.