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An Updated Classification of the Recent Crustacea

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ine isopods that has been posted on <strong>the</strong> World<br />

Wide Web by B. Kensley and M. Schotte (http://<br />

www.nmnh.si.edu/iz/isopod). However, in that<br />

compilation, <strong>the</strong> various suborders and <strong>the</strong>ir constituent<br />

superfamilies and families are arranged alphabetically.<br />

Brusca and Wilson (1991), while proposing<br />

some phylogenetic changes that would seriously<br />

alter <strong>the</strong> arrangement <strong>of</strong> groups as presented<br />

here (and at <strong>the</strong> same time countering several <strong>of</strong><br />

<strong>the</strong> hypo<strong>the</strong>ses forwarded earlier by Wägele, 1989),<br />

stopped short <strong>of</strong> proposing a new classification<br />

based on <strong>the</strong>ir hypo<strong>the</strong>sis. Their feeling was that<br />

insufficient evidence had been amassed for proposing<br />

classifications based on <strong>the</strong> phylogenetic hypo<strong>the</strong>ses<br />

<strong>the</strong>y were presenting as testable ideas. The<br />

Brusca and Wilson (1991) analysis was criticized<br />

by Wägele (1994), who in fact used <strong>the</strong>ir paper to<br />

point out potential pitfalls in any attempt at computer-generated<br />

cladistic analyses. Wägele (1994)<br />

was in turn rebutted by Wilson (1996), who was<br />

answered by Wägele (1996), and it would seem<br />

that we have a long way to go before any consensus<br />

concerning isopod phylogeny (not to mention phylogenetic<br />

method) is reached. Thus, our classification<br />

is in some ways a step backward in that we<br />

continue to recognize some groups, such as <strong>the</strong> Flabellifera,<br />

that appear clearly paraphyletic (following<br />

<strong>the</strong> analyses <strong>of</strong> both Brusca and Wilson, 1991,<br />

and Wägele, 1989) but for which no alternative<br />

classifications have been proposed. In <strong>the</strong> most recent<br />

overall treatment <strong>of</strong> isopods, Roman and Dalens<br />

(1999) continue to recognize <strong>the</strong> Flabellifera as<br />

well while acknowledging that it is a heterogeneous<br />

assemblage.<br />

Additionally, many changes, especially those concerning<br />

names and dates <strong>of</strong> <strong>the</strong> authorities credited<br />

with establishing families but also concerning<br />

whe<strong>the</strong>r or not to recognize a particular family,<br />

have been incorporated at <strong>the</strong> request <strong>of</strong> some <strong>of</strong><br />

<strong>the</strong> major workers (e.g., L. Holthuis, B. Kensley, R.<br />

Brusca, G. Poore, W. Wägele, and G. Wilson) via<br />

personal communications. It has not always been<br />

possible for us to verify <strong>the</strong>se suggestions. Often,<br />

despite a ra<strong>the</strong>r large library on crustacean systematics<br />

at our disposal, we have been unable to see<br />

<strong>the</strong> original references. In cases where we received<br />

conflicting information (such as whe<strong>the</strong>r <strong>the</strong> family<br />

Arcturidae should be credited to White, 1850 vs.<br />

Bate and Westwood, 1868 vs. Sars, 1899) and/or<br />

we could not verify by checking on all <strong>of</strong> <strong>the</strong> suggested<br />

references ourselves, we have chosen <strong>the</strong> first<br />

known usage (in this case, using Arcturidae White,<br />

1850, which turns out to be correct according to<br />

G. Poore, who owns <strong>the</strong> book) in accordance with<br />

ICZN article 50.3.1. One such change involves <strong>the</strong><br />

establishment <strong>of</strong> a large number <strong>of</strong> families and superfamilies<br />

credited to Latreille. L. Holthuis (pers.<br />

comm.) assures us that 1802 is <strong>the</strong> correct date for<br />

<strong>the</strong> many taxa that have been, in <strong>the</strong> past, credited<br />

to Latrielle (1803) (see earlier section on names,<br />

dates, and <strong>the</strong> ICZN).<br />

Major papers suggesting changes in how we or-<br />

ganize <strong>the</strong> Isopoda that have appeared subsequent<br />

to Bowman and Abele (1982) include Wägele<br />

(1989) and Brusca and Wilson (1991). Poore<br />

(2001a) presented a phylogeny <strong>of</strong> <strong>the</strong> <strong>An</strong>thuridea<br />

suggesting relationships among <strong>the</strong> six families<br />

(two new), but to our knowledge, <strong>the</strong>re have not<br />

as yet been names proposed for <strong>the</strong> divisions suggested<br />

by him. The most recent review, by Roman<br />

and Dalens (1999), recognizes eight suborders.<br />

Their arrangement differs from ours in that (1) <strong>the</strong>y<br />

recognize <strong>the</strong> suborder Gnathiidea, which we do<br />

not, and (2) <strong>the</strong>y do not recognize <strong>the</strong> suborders<br />

Microcerberidea and Calabozoidea, which we do,<br />

for reasons discussed below.<br />

Concerning <strong>the</strong> former suborder Gnathiidea,<br />

Brusca and Wilson (1991) suggested that <strong>the</strong> gnathiids<br />

were derived from among <strong>the</strong> families traditionally<br />

thought <strong>of</strong> as ‘‘flabelliferan’’ isopods (a<br />

group that <strong>the</strong>y demonstrate is not monophyletic).<br />

Wägele (1989, pers. comm.) also would remove <strong>the</strong><br />

gnathiids from <strong>the</strong>ir own suborder, but his preference<br />

was to place <strong>the</strong>m among <strong>the</strong> Cymothoida, a<br />

group he recognizes as containing a large number<br />

<strong>of</strong> former Flabellifera families. We have, for <strong>the</strong><br />

current classification, removed <strong>the</strong> gnathiids from<br />

<strong>the</strong>ir own superfamily and have placed <strong>the</strong>m within<br />

<strong>the</strong> Flabellifera, knowing that <strong>the</strong> Flabellifera itself<br />

is not monophyletic and must some day be extensively<br />

revised. L. Holthuis (pers. comm.) has suggested<br />

that we credit <strong>the</strong> family name Gnathiidae<br />

to Leach (1814) ra<strong>the</strong>r than to Harger (1880), as<br />

was used by Bowman and Abele (1982) and Roman<br />

and Dalens (1999).<br />

SUBORDER PHREATOICIDEA<br />

Wilson (pers. comm.) suggests that many <strong>of</strong> <strong>the</strong><br />

subfamilies <strong>of</strong> <strong>the</strong> Amphisopodidae recognized by<br />

Nicholls (1943, 1944) will need to be elevated to<br />

family level (e.g., as Hypsimetopodidae, Mesamphisopodidae,<br />

Phreatoicopsididae) once this suborder<br />

is revised (see also Wilson and Johnson,<br />

1999; Wilson and Keable, 1999, 2001). Our classification<br />

follows Roman and Dalens (1999) in recognizing<br />

three families (<strong>the</strong> same three that appear<br />

in Bowman and Abele, 1982). By listing <strong>the</strong> phreatoicids<br />

first among all isopod suborders, we are acknowledging<br />

<strong>the</strong> primitive nature <strong>of</strong> <strong>the</strong>se isopods.<br />

Brusca and Wilson (1991) and Wilson and Johnson<br />

(1999) have indicated that <strong>the</strong> phreatoicideans, all<br />

<strong>of</strong> which are restricted to Gondwanan fresh waters,<br />

may be ‘‘<strong>the</strong> earliest derived isopod Crustaca’’ (Wilson<br />

and Johnson, 1999:264). The phreatoicidean<br />

fossil record extends back to <strong>the</strong> Carboniferous<br />

(Wilson and Johnson, 1999).<br />

SUBORDER ANTHURIDEA<br />

Within this suborder, <strong>the</strong> family <strong>An</strong><strong>the</strong>luridae was<br />

described by Poore and Lew Ton (1988) and <strong>the</strong><br />

families Expanathuridae and Leptanthuridae were<br />

described recently by Poore (2001a; see also Poore,<br />

1998). Our treatment differs from that <strong>of</strong> Roman<br />

38 � Contributions in Science, Number 39 Rationale

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