NEW FOSSIL LACEWINGS AND ANTLIONS … FOSSIL LACEWINGS AND ANTLIONS (INSECTA, NEUROPTERA) FROM THE...
Transcript of NEW FOSSIL LACEWINGS AND ANTLIONS … FOSSIL LACEWINGS AND ANTLIONS (INSECTA, NEUROPTERA) FROM THE...
NEW FOSSIL LACEWINGS AND ANTLIONS (INSECTA,
NEUROPTERA) FROM THE LOWER CRETACEOUS
CRATO FORMATION OF BRAZIL
by FEDERICA MENON* and VLADIMIR N. MAKARKIN�*School of Earth, Atmospheric and Environmental Sciences, University of Manchester, Williamson Building, Oxford Road, Manchester M13 9PL, UK;
e-mail: [email protected]
�Institute of Biology and Soil Sciences, Far Eastern Branch of the Russian Academy of Sciences, Vladivostok 690022, Russia; e-mail: [email protected]
Typescript received 8 August 2006; accepted in revised form 22 January 2007
Abstract: Remarkable new fossil taxa of Neuroptera from
the laminated limestone of the Crato Formation, north-east
Brazil, are described: Nuddsia longiantennata gen. et sp. nov.
(Osmylidae, Gumillinae), the first fossil record of this family
from South America, Parapalaeoleon magnus gen. et sp. nov.
(Palaeoleontidae), and Triangulochrysopa formosa sp. nov.
(Mesochrysopidae). A diagnosis of Gumillinae is provided;
Epiosmylidae is considered to be a synonym of this subfam-
ily. A revised diagnosis of Palaeoleontidae is provided, based
on a new interpretation of venational characters evident on
the exceptionally well-preserved specimen of P. magnus; vein
homologies are determined and the fusion of MP and CuA is
discussed. The genus Triangulochrysopa has been known pre-
viously only from the Lower Cretaceous of Las Hoyas, Spain.
Key words: Araripe, Crato Formation, Nova Olinda Mem-
ber, Neuroptera, Osmylidae, Palaeoleontidae, Mesochrysopi-
dae, taxonomy.
The Crato Formation is well known for the diversity and
quality of its fossil insects; three-dimensional features and
colour pattern are often preserved (Martill and Frey 1995;
Heads et al. 2005). The formation ranges across the Ara-
ripe Plateau in the states of Ceara, Pernambuco and Pia-
uı, north-east Brazil. It is composed of a series of finely
laminated limestones that accumulated at the bottom of a
lagoon during the initial phase of the opening of the
Atlantic Ocean (Martill 1993). Its precise age is somewhat
unclear: it is generally considered to be Late Aptian–Early
Albian, 110–120 Ma (Berthou 1994), and has been dated
as Late Aptian on the basis of palynological data (Pons
et al. 1991). The formation is subdivided into three mem-
bers: Nova Olinda, Barbalha and Jamacaru. The basal
Nova Olinda Member is the most fossiliferous: insects are
found together with other arthropods, plants and wood,
fish, pterosaurs and other vertebrates (Maisey 1991).
The order Neuroptera is one of the most significant
and diverse groups of insects found in the Crato Forma-
tion, with 55 species having been described (Martins-Neto
2000, 2003, 2005; Heads et al. 2005; Makarkin and
Menon 2005, 2007; Menon et al. 2005; Nel et al. 2005). A
vast amount of material in a variety of museums remains
unstudied. We describe here two new genera and three
new species belonging to the families Osmylidae, Pala-
eoleontidae and Mesochrysopidae, based on specimens
housed at the Staatlisches Museum fur Naturkunde Stutt-
gart, Germany. No fossil record of Osmylidae was known
hitherto from South America.
MATERIAL AND METHODS
All specimens described here are from the lowest member
of the Crato Formation. They were probably collected by
workers in one of the small mines or stone yards around
Nova Olinda, although the exact locality is unknown.
They are preserved as limonitic replacements after pyrite
(Martill and Frey 1995). The specimens were prepared
on-site by the collectors. An aeroneedle was used, where
necessary, to remove any residual sediment and dust
(Selden 2003).
Drawings were made using a camera lucida attached to
a Wild stereomicroscope; photographs were taken with a
Sony DCS-717 digital camera and a D1X digital camera
attached to a Wild M8 stereo-zoom microscope.
SYSTEMATIC PALAEONTOLOGY
Wing venation terminology follows Comstock (1918), with a few
exceptions in accordance with current usage in neuropterology
(see Archibald and Makarkin 2006; Wedmann and Makarkin
2007). Terminology of wing spaces follows Oswald (1993)
[Palaeontology, Vol. 51, Part 1, 2008, pp. 149–162]
ª The Palaeontological Association doi: 10.1111/j.1475-4983.2007.00740.x 149
Venation abbreviations used in the text and figures are as fol-
lows: 1A–3A, anal veins; bf, anterior Banksian fold; Cu, cubitus;
CuA, anterior cubitus; CuA1, most proximal branch of anterior
cubitus; CuP, posterior cubitus; M, media; MA, anterior branch
of media; mfl, median flexion line; MP, posterior branch of
media; MP1, most proximal branch of MP; R, radius; R1, first
branch of radius; Rs, radial sector; Rs1, most proximal branch of
radial sector; Sc, subcosta.
Institutional abbreviation. SMNS, Staatliches Museum fur
Naturkunde Stuttgart, Germany.
Class INSECTA Linnaeus, 1758
Order NEUROPTERA Linnaeus, 1758
Family OSMYLIDAE Leach, 1815
Subfamily GUMILLINAE Navas, 1912
1912 Gumillini Navas, p. 191 (as a ‘tribe’ of Osmylidae).
1988 Gumillinae Lambkin, p. 455 (as a subfamily of
Osmylidae).
1980 Epiosmylidae Panfilov, in Dolin et al., p. 100, syn.
nov.
Type genus. Gumilla Navas, 1912 (Recent).
Diagnosis. Medium-sized osmylids that may be distin-
guished from other species of the family by the following
combination of character states: (1) antennae exceedingly
elongate, much longer than forewing [much less than
forewing length in other subfamilies]; (2) scape strongly
enlarged [moderately enlarged in other osmylids]; (3)
basal sinuous crossvein r-m in hindwing absent, character
state shared with Stenosmylinae [present in other subfam-
ilies]; (4) outer gradate series of crossveins absent in both
wings, as in Porisminae [present in other subfamilies]; (5)
trichosors limited at most to apical part of wings [nor-
mally present at least in distal half of wings in other os-
mylids].
Included genera. Gumilla (Recent, Brazil; one or two species);
Epiosmylus Panfilov, in Dolin et al. 1980 (Upper Jurassic, Kara-
tau, Kazakhstan, Karabastau Formation; Middle–Upper Jurassic,
Daohugou, Inner Mongolia, China; two species); Nuddsia gen.
nov. (Lower Cretaceous, Upper Aptian, Araripe Basin, Brazil,
Crato Formation; one species).
Remarks. Three taxa with extremely long antennae, at
least 1.5 times longer than the forewing length, are known
within Neuroptera. These include the extant Chrysopidae,
in the majority of Apochrysinae and a few genera of
Chrysopinae, and the Osmylidae, in the subfamily Gumil-
linae and the fossil Epiosmylidae.
The family Epiosmylidae was erected to accommodate
Epiosmylus longicornis Panfilov, 1980 (Upper Jurassic of
Karatau, Kazakhstan). Another species of this genus
(E. panfilovi Ren and Yin, 2002) was added later from the
Middle–Upper Jurassic of China (Ren and Yin 2002).
Since its establishment, Epiosmylidae has been generally
treated as either a synonym of Osmylidae (e.g. Pono-
marenko 1980; Makarkin 1990b; Ren and Yin 2002) or a
taxon whose status is unclear, ‘either an isolated branch
within Osmylidae or else a separate family’ (Makarkin
and Archibald 2003, p. 175). Recently, Ponomarenko
(2003) described another osmylid-like species with extre-
mely long antennae, ‘Nymphites cf. lithographicus’, from
the Upper Jurassic of Solnhofen, Germany, and assigned
it to the Nymphitidae. However, the photograph and
drawings of this specimen provided indicate the possibil-
ity that it belongs to Osmylidae (possibly to Gumillinae
because of its long antennae); its venation is most similar
to that found in this family, and its relation to the true
Nymphites lithographicus Handlirsch, 1906 is unclear, as
its holotype is very poorly preserved.
The subfamily Gumillinae has not been formally
defined. The ‘tribe’ Gumillini was created by Navas
(1912) within Osmylidae for the genus Gumilla Navas,
including the two extant Brazilian species, G. adspersa
Navas, 1912 and G. longicornis (Walker, 1853), which
should perhaps be considered synonyms (Adams 1977).
Navas (1912) grouped all other osmylids in the ‘tribe’
Osmylini; thus the actual rank of these ‘tribes’, according
to Navas (1912), could be considered at the subfamily
level. Gumilla was subsequently excluded from the family
by Kruger (1913, 1915), then included again by Adams
(1969, 1977). Adams (1969, p. 2) mentioned that this
genus is highly aberrant and ‘is too poorly known for
meaningful discussion’. He correctly concluded that Nav-
as’ (1912, fig. 24) drawing of the forewing is reasonably
accurate, and provided some additional diagnostic fea-
tures of the genus (Adams 1977). Unfortunately, the char-
acters of the male terminalia are largely unknown, beyond
the short description of Navas (1912, p. 57) (‘cercis cylin-
dricis, pilosis, brevibus, externe convexis’), and they have
never been illustrated.
It is reasonable to assume that Epiosmylidae and
Gumillinae might be the same, as they share some impor-
tant character states (see diagnosis, above), even though
Epiosmylus and Gumilla, their type genera, differ quite
considerably by the configuration of MA, MP, CuA and
CuP in the forewing, which are straighter with branching
that is fairly regular in the former and strongly irregular
in the latter (see also note of Lambkin 1988, p. 455).
Examination of the photograph of the holotype of G. ad-
spersa reveals that its forewing venation is somewhat
anomalous (the venation of right and left wings is
strongly asymmetrical). The forewing venation of Nuddsia
(e.g. configuration of MP, CuA, CuP) is also irregular to
150 P A L A E O N T O L O G Y , V O L U M E 5 1
some extent (Text-fig. 2), providing additional support
for placing it in Gumillinae. The hindwing venation of all
species (including the holotype of G. adspersa and the
new species) does not differ in its main character states.
Ocelli are absent in the extant Gumilla (present in all
other osmylids) but are not detectable in fossil taxa
because of poor preservation or as the head is missing.
Gumillinae is considered here to be a subfamily of
Osmylidae because its venation generally agrees well with
that of this family, and to be the sister group of all other
osmylids because of the clear differences between them
(see diagnosis above). The loss of the basal sinuous cross-
vein r-m in the hindwing and the absence of the outer
gradate series of crossveins in both wings, shared by
Gumillinae with Stenosmylinae (the former) and Porismi-
nae (the latter) might be convergent.
Genus NUDDSIA gen. nov.
Type and only species. Nuddsia longiantennata sp. nov.
Derivation of name. After Dr John Nudds, Head of the Palaeon-
tology Research Group at the University of Manchester. Gender
feminine.
Diagnosis. May be distinguished from other genera of the
subfamily by the following combination of character
states: (1) antennae nearly 2.5 times as long as forewing
[not more than 1.5 times in Epiosmylus, Gumilla]; (2) M
in forewing forked highly proximal to origin of Rs1
[slightly distal in Gumilla]; (3) distal half of CuA in fore-
wing arched [parallel to hind margin in Epiosmylus].
Remarks. Nuddsia gen. nov. represents the first fossil
record of this family from South America. Interestingly,
the single living genus of this subfamily (Gumilla) also
occurs in Brazil, and the wing venation of both genera is
quite similar.
Nuddsia longiantennata sp. nov
Text-figures 1–2
Derivation of name. Latin, longus, long, and Medieval Latin
antenna, sail yard (translation of Greek keraia, insect feeler,
yard-arm), in reference to the extremely long antennae of this
species.
Holotype. SMNS 66000 ⁄ 263. An almost complete specimen
exposed in ventral aspect.
Type locality and horizon. Brazil, Ceara, Araripe Basin (Chapada
do Araripe), vicinity of Nova Olinda; Crato Formation (Nova
Olinda Member), Lower Cretaceous (Upper Aptian).
Diagnosis. As for the genus.
Description. Head twice as wide as long (1 mm long, 2 mm
wide); large compound eyes. Antennae extremely long (60 mm),
filiform; scape very large, bulky; pedicel elongate, rounded, larger
than flagellar segments. Prothorax nearly quadrate, c. 1 mm
long. Mesothorax not clearly visible, apparently wide. Legs not
preserved. Abdomen incomplete, 4 mm long as preserved. Head,
thorax and abdomen strongly compressed. Exoskeleton of most
portions of head, thorax and abdomen not preserved.
Forewing elongate, 25.5 mm long, c. 6.5 mm wide; apex sub-
acute. Trichosors prominent, restricted to apical portion of wing.
Costal space 0.6 mm maximum width, narrow basally, slightly
dilated near proximal third, then narrowed towards apex. Sub-
costal veinlets simple, straight, nearly perpendicular to Sc in
basal two-thirds of costal space, increasingly more oblique dis-
tad; veinlets of Sc+R1 closely spaced, strongly oblique. Subcostal
space narrow, dilated near fusion of Sc, R1. Sc, R1 fused 4 mm
from wing apex. Sc+R1 entering margin before wing apex. Rs
originating near wing base. Stem of Rs zigzagged, forked api-
cally, entering margin slightly before wing apex. R1 space wider
than costal space, 0.8 mm, strongly narrowed apically, with 23
more or less regularly spaced crossveins proximad fusion of Sc,
R1, one distad (left wing). Rs with six branches, distal branch
deeply forked. Origin of Rs1 at approximately one-third wing
length, c. 8 mm from base (left wing); origins of Rs1–Rs3 widely
spaced, other three branches restricted to apical portion of wing.
Radial crossveins numerous, regularly spaced (except for apical
portion of space, where crossveins rare), not forming gradate
series. Fork of M considerably distal to origin of Rs but much
proximal to origin of Rs1. MA straight, with four pectinate, obli-
que branches distally. MP basally straight, parallel to MA, con-
figuration of distal portion somewhat irregular with 2–3
branches, most proximal of which long, dichotomously
branched. Fork of Cu not preserved, apparently near wing base.
Configuration of distal portion of CuA rather irregular, dichoto-
mously branched. CuP poorly preserved; distal half clearly
arched; short, simple distalmost branches preserved. Anal veins
not preserved. Crossveins rather regularly spaced, except for
most distal portion of radial space, where crossveins are scarce.
Gradate series of crossveins not detected.
Hindwing elongate, 24.5 mm long, 5.5 mm wide, with sub-
acute apex. Trichosors restricted to apical portion. Nygmata
not detected. Costal space very narrow, 0.5 mm wide basally
(left wing), slightly dilated in pterostigmal region. Subcostal
veinlets simple, perpendicular to Sc in basal half of costal
space, increasingly more oblique distad; veinlets of Sc+R1 clo-
sely spaced, strongly oblique. Subcostal space very narrow for
most of its length, slightly dilated near fusion of Sc, R1. Sc, R1
fused at 3.5 mm from apex. Sc+R1 entering margin slightly
before apex. Rs originating near wing base. R1 space 0.8 mm
wide medially, strongly narrowed apically; with 21 more or less
regularly spaced crossveins before fusion of Sc, R1, long hypo-
stigmal cell after. Rs strongly zigzagged, forked apically, enter-
ing margin at apex, with 6–7 branches, mostly zigzagged, with
deep marginal forks. Origin of Rs1 at approximately one-third
wing length. Radial, medio-radial crossveins numerous, regu-
larly spaced, not forming gradate series. Basal crossveins m-r
M E N O N A N D M A K A R K I N : C R E T A C E O U S F O S S I L L A C E W I N G S A N D A N T L I O N S F R O M B R A Z I L 151
not detected, probably absent. Origin of M, its division into
MA and MP not preserved; MA straight for entire preserved
length, pectinately branched distally, with five branches, most
proximal of which forked twice. MP zigzagged, with three dis-
tal branches, most proximal of which long, pectinately
branched (two branches). CuA long, zigzagged, parallel to hind
margin, pectinately branched, with at least 12 rather short,
simple branches. Crossveins in medial, medio-cubital spaces
numerous, more or less regularly spaced. CuP, anal veins not
preserved.
A
B
TEXT -F IG . 1 . Nuddsia longiantennata gen. et sp. nov. A, photograph, and B, line drawing of the holotype, SMNS 66000 ⁄ 263. Scale
bar represents 10 mm.
152 P A L A E O N T O L O G Y , V O L U M E 5 1
Family PALAEOLEONTIDAE Martins-Neto, 1992
1992 Palaeoleontinae Martins-Neto, p. 810 (as a subfamily
of Myrmeleontidae).
1997 Palaeoleontidae; Dobruskina et al., p. 93.
Type genus. Palaeoleon Rice, 1969, from the Albian–Cenomanian
of Labrador, Canada.
Revised diagnosis. Large myrmeleontoids (forewing 36–
70 mm long) with relatively long antennae, unusually
dense crossvenation in the majority of genera, easily dis-
tinguished from other myrmeleontoid families by the fol-
lowing combination of character states: (1) antennae
long, filiform, neither dilated nor clavate distally [dilated
distally in Myrmeleontidae, Araripeneuridae; clavate in
Ascalaphidae]; (2) origin of Rs situated near wing base in
both wings [removed from base in Myrmeleontidae,
Araripeneuridae, Ascalaphidae, Nemopteridae, Babinskaii-
dae]; (3) presectorial crossveins absent in both wings
[present in Myrmeleontidae, Ascalaphidae, Nemopteridae,
Babinskaiidae]; (4) ‘oblique vein’ present in forewing
[absent in Nymphidae].
Revised description of venation. In forewing, origin of Rs close to
wing base; without presectorial crossveins; Rs1 convex, profusely
branched distally; single well-developed median longitudinal fold
present from wing base to apex; fork of M far removed from wing
base (Palaeoleon, Baisopardus); MA strongly concave, simple;
basal part of MP represented by ‘oblique vein’, distal MP fused
with CuA; Cu divided into CuA, CuP close to wing base; CuA,
MP+CuA convex, both parallel to MA; MP+CuA, MP+CuA1 and
TEXT -F IG . 2 . Nuddsia longiantennata
gen. et sp. nov., holotype, SMNS
66000 ⁄ 263. A, left forewing. B, right
forewing. C, left hindwing. D, right
hindwing. Scale bar represents 5 mm.
M E N O N A N D M A K A R K I N : C R E T A C E O U S F O S S I L L A C E W I N G S A N D A N T L I O N S F R O M B R A Z I L 153
its basalmost branch form large triangular area characteristic of
higher myrmeleontoids; CuP relatively short, pectinately branch-
ing, not fused with 1A; 1A from short, nearly simple to long,
pectinately branched. In hindwing, origin of Rs close to wing base,
without presectorial crossveins; Rs1 profusely branched distally;
M forked very close to wing base; MA simple; MP with long
pectinate branches; Cu forked close to wing base; CuA parallel to
hind margin basally, arched, pectinately branched distally; CuP
short, close, parallel to hind margin, pectinately branched; anal
area very restricted by short simple veins.
Included genera. Baisopardus Ponomarenko, 1992a (Lower Cre-
taceous, Lower Valanginian, Baissa, Transbaikalia, Russia; Crato
Formation; 3–4 species); Parapalaeoleon gen. nov. (Crato Forma-
tion; monotypic); Neurastenyx Martins-Neto and Vulcano, 1997
(Crato Formation; monotypic); Paraneurastenyx Martin-Neto,
1998 (Crato Formation; monotypic); Palaeoleon (Lower–Upper
Cretaceous, Albian–Cenomanian, Labrador, Canada; monotypic);
Samsonileon Ponomarenko, in Dobruskina et al. 1997 (Upper
Cretaceous, Lower Turonian, Israel; monotypic); Metahemerobius
Makarkin, 1990a (Upper Cretaceous–Palaeogene, Maastrichtian–
Danian, Antibes, Siberia, Russia; monotypic).
Remarks. The diagnosis of this family provided by
Dobruskina et al. (1997) and Heads et al. (2005) is par-
tially erroneous, being based on misinterpretation of the
venation in more poorly preserved specimens, particularly
concerning M and CuA. The new material provides the
opportunity to clarify this. According to these authors,
‘MP’ in the forewing is forked into ‘MP1’ and ‘MP2’ in
the proximal portion of the wing, with ‘MP1’ profusely
branched distally, and ‘MP2’ simple. However, this fork is
not detected confidently in any species. The well-pre-
served venation of the forewing of Parapalaeoleon magnus
(Text-fig. 3C) shows that this ‘MP1’ is actually Rs1. The
homology of Rs1 in all species is unequivocal: this vein is
always convex, and is followed posteriorly by a strongly
concave simple vein (we interpret this as MA). Compari-
son of Palaeoleon ferrogeneticus Rice, 1969 and Baisopar-
dus cryptohymen Heads et al., 2005 shows that the
structure of Rs2 is also similar in these species: convex
basally and concave distally.
Examination of photographs of these specimens reveals
that what the authors interpreted as the proximal part of
‘MP1’ (Heads et al. 2005, fig. 3A) and ‘M1’ (Rice 1969, fig.
2) is actually the proximal part of a longitudinal vein-like
fold running between Rs and M. Its course is completely
coincident with that of the median flexion line in some
insects with anteroposteriorly symmetric wings, such as Si-
alis Latreille, 1802 (Wootton 2002, fig. 3A), running longi-
tudinally from the wing base to the wing apex between the
radial and medial vein systems and distally crossing the
branches of Rs (Wootton 2003, fig. 5). The wings of many
extant Myrmeleontidae that have anteroposteriorly asym-
metric wings appear to possess the distal part of this line
(appearing as a fold), which is often accompanied by a
false longitudinal vein formed by the bending of branches
of Rs and the crossveins connecting them, called the ‘ante-
rior Banksian line’ (Tillyard 1916; Krivokhatsky 1998).
This fold will be called herein ‘the anterior Banksian fold’
as its homology with the distal part of the median flexion
line of species with the anteroposteriorly asymmetric wings
is unclear. In Parapalaeoleon magnus, the median flexion
line appears as a true flexion line running (as in other
Neuroptera with anteroposteriorly asymmetric wings:
Wootton 2002, fig. 4B) between MA and Rs, then Rs1, ter-
minating far distal to the origin of the anterior Banksian
fold, which begins slightly distal to Rs1 (i.e. distal part of
the median flexion line and proximal part of the anterior
Banksian fold are divergent). In other species (e.g. Palaeo-
leon ferrogeneticus, Baisopardus cryptohymen) in which the
origin of Rs1 is situated very near the origin of Rs, the
median flexion line crosses Rs1 near its base and continues
further as a concave fold towards the wing apex. In these
species the median flexion line proximally and the anterior
Banksian fold distally form a single straight line, called
here the median longitudinal fold. Basally, this line
appears to be vein-like in compression fossils, as in P. fer-
rogeneticus. Such secondary vein elements are frequently
reformed from membrane (Kukalova-Peck 1991).
Fusion of MP and CuA in the forewing. This fusion has
apparently occurred independently many times in the
evolution of the Neuroptera. It is found in a few genera
of the extant Hemerobiidae (Nusalala Navas, 1913, Micro-
mus Rambur, 1842), Dilaridae (Nallachius Navas, 1909),
and in a Lower Cretaceous psychopsid-like genus from
the Baissa locality (Makarkin, unpublished). In two speci-
mens of the extant Gerstaeckerella chilensis (Hagen, 1859)
(Mantispidae) examined in this study, MP and CuA are
fused abnormally for short distance at the crossvein 2m-
cu (which is consequently lost) in the manner that occurs
in Parapalaeoleon magnus. Interestingly, CuA in Gers-
taeckerella Enderlein, 1910 (as in other mantispids) is
short. In Mesochrysopidae, all intermediate stages are
present, from MP and CuA widely spaced to touching
(Makarkin and Menon 2005; Nel et al. 2005). The fullest
fusion of these veins, however, occurs in the forewing of
the myrmeleontoid lineage (Palaeoleontidae, Araripeneu-
ridae, Myrmeleontidae, Ascalaphidae, Nemopteridae, and
probably Babinskaiidae), in which MP resembles a cross-
vein (‘oblique vein’) often not distinguished from true
crossveins (see discussions in Tillyard 1916, 1918; Com-
stock 1918; Adams 1996). The venation of P. magnus
(Text-figs 3B, 4B) rather clearly demonstrates that this
full fusion might have resulted from touching or short
fusion of a long pectinate MP and short CuA, almost
exactly in the way predicted by Tillyard (1916, fig. 8b; his
154 P A L A E O N T O L O G Y , V O L U M E 5 1
‘Cu2’ is, however, actually CuA1). Moreover, MP and
CuA in the forewing of Paraneurastenyx ascalaphix Mar-
tins-Neto, 1998 are almost touching but not fused (Mar-
tins-Neto 1998, fig. 1A), as in some Mesochrysopidae
(Makarkin and Menon 2005, fig. 3B). Based on this
hypothesis, it is reasonable to assume that the most prox-
imal pectinate branch of MP+CuA (i.e. MP+CuA1) repre-
sents the distal portion of CuA (Text-fig. 3B); the next
branch, MP+CuA2 (fused with MP+CuA1 distally in this
specimen), might have originated from the most proximal
branch of MP (MP1), and other branches of MP+CuA all
originate from MP. Some species of the extant Myr-
meleontidae show a remarkable reversal of the conditions
of these veins, indirectly supporting this hypothesis. In
the Australian Mjoberbia fulviguttata Esben-Petersen, 1918
and Protoplectron pallidum Banks, 1910, MP and CuA are
not fused, and CuA has few branches (New 1985, figs
263, 290, but see intraspecific variation, e.g. fig. 265).
Notes on generic and specific composition of Palaeoleonti-
dae. Palaeoleon was erected for P. ferrogeneticus, repre-
sented by a single, well-preserved, apical two-thirds of a
wing. We examined photographs of the holotype and
found that the original description and figures of Rice
(1969, p. 3, figs 1, 3; pl. 1) appear to be fairly adequate,
although the venation could possibly be interpreted dif-
ferently: Rice’s M1 is the median flexion line (basally)
and Rs2 (distally), M2 is Rs1, Cu1 is MA, Cu2 is MP (see
reasoning above).
According to Martins-Neto (1997) the genus Neuraste-
nyx includes N. gigas Martins-Neto and Vulcano, 1997
(type species), N. polyhymnia Martins-Neto, 1997 and N.
araripensis (Martins-Neto 1992). All of these species were
placed in Baisopardus (see below), along with Baisopardus
gigas, by Heads et al. (2005) who consequently synonym-
yzed these two genera. However, in our opinion, Neurast-
enyx is valid and consists of N. gigas only. The holotype
of the type species is poorly preserved (Martins-Neto and
Vulcano 1997, fig. 7), but it possesses a combination of
the character states that distinguish the species from other
palaeoleontids: large size (forewing length about 70 mm)
and very widely spaced crossveins.
Baisopardus is considered to include four species
(Heads et al. 2005). The type species, B. banksianus Pon-
omarenko, 1992a, is known from two isolated hindwings,
the holotype and paratype, from the Lower Cretaceous of
Baissa, Transbaikalian Russia (Ponomarenko 1992a). The
genus was included by Dobruskina et al. (1997) in this
family with some doubt, whereas Heads et al. (2005)
listed it among the genera of Palaeoleontidae with cer-
tainty. In the original description, however, the venation
was misinterpreted by Ponomarenko (1992a, p. 49, fig.
5A): his ‘MA’ is our Rs1, ‘MP’ is MA, ‘CuA’ is MP, ‘CuP’
is CuA, ‘1A’ is CuP.
Palaeoleon araripensis was the first species of this family
to be described from the Crato Formation (Martins-Neto
1992). Later, it was transferred to Neurastenyx by Martins-
Neto (1997), and to Baisopardus by Dobruskina et al.
(1997). The holotype is an almost complete specimen, but
lacks the abdomen, and has incomplete hind- and fore-
wings, which are overlapped pairwise. Ponomarenko (in
Dobruskina et al. 1997) noted that the hindwing venation
of the type specimen was partially incorrectly drawn by
Martins-Neto (1992, p. 811, fig. 5a): the proximal branches
of his CuA [actually MP, see above] belongs to CuP [actu-
ally CuA]; therefore, the configuration of MP and CuA are
similar to those of the type species (see also below).
Baisopardus cryptohymen is represented by a beautifully
preserved, complete, single specimen. The species has a
hindwing shape and venation similar to those of the type
species, B. banksianus, so we find it quite reasonable that it
is assigned to Baisopardus. The single major difference
between these species is that the former possesses closely
spaced subcostal crossveins, which the latter lacks. The
interpretation of the venation in the original description
and figures of Heads et al. (2005, fig. 3) is partially incor-
rect (see reasoning above) and should be emended. In the
forewing, their MA is Rs1 (basally) and Rs2 (distally),
MP1 is the median flexion line (basally) and Rs1 (distally),
MP2 is MA, CuA is MP+CuA, CuA1 is MP+CuA, CuA2 is
MP+CuA1; in the hindwing, their MA is Rs1 (basally) and
Rs2 (distally), MP1 is the median flexion line (basally) and
Rs1 (distally), MP2 is MA, CuA1 is MP, CuA2 plus CuP is
CuA, 1A is CuP (see above for reasoning).
All wings of ‘Neurastenyx’ polyhymnia are so strongly
overlapped that few details of the venation may be clearly
identified (Martins-Neto, 1997, fig. 7). Its systematic posi-
tion, therefore, may possibly be determined confidently
only after close re-examination of the type. The assign-
ment of this species to Baisopardus (as well as to Neurast-
enyx) should be considered tentative, based on the
general impression of its venation rather than on analysis
of particular character states.
Samsonileon and Metahemerobius are apparently closely
related genera; this is indicated by their similar forewing
venation, in particular, MP+CuA1 and CuP run parallel
and very close for a considerable distance, and 1A is
long and pectinately branched. Unfortunately, both gen-
era are represented by incomplete wings, lacking basal
portions in known specimens. Makarkin’s (1990a, fig. 5)
designations of the veins of Metahemerobius kalligram-
mus Makarkin, 1990a are partially incorrect: his MA is
Rs2, anterior branch of MP is Rs1, posterior branch of
MP is MA, CuA is MP+CuA, CuP is MP+CuA1, A1 is
CuP. The venation of Samsonileon fragmentatus Pon-
omarenko, in Dobruskina et al. 1997 is interpreted simi-
larly here: Ponomarenko’s MA is Rs1 (basally) and the
anterior Banksian fold or Rs2 (distally), MP1 is probably
M E N O N A N D M A K A R K I N : C R E T A C E O U S F O S S I L L A C E W I N G S A N D A N T L I O N S F R O M B R A Z I L 155
the median flexion line (basally) and Rs1 (distally), CuA
is MP+CuA, CuP and A1 are CuP and 1A respectively.
Cretoleon Ponomarenko, 1992b is a monotypic genus
represented by a forewing of C. acanthoclysoides Pono-
marenko, 1992b from the Lower Cretaceous (Aptian)
deposits of Bon-Tsagan, Mongolia (Ponomarenko 1992b).
It was considered possibly to belong to Palaeoleontidae by
Ponomarenko (in Dobruskina et al. 1997), and listed
among the genera of this family by Heads et al. (2005). It is
tentatively excluded from the family here because it differs
in the following features of the forewing: the costal space is
broad; Rs originates relatively distant from the wing base;
the anterior Banksian fold is absent; the subcostal veinlets
in the pterostigmal region are very closely spaced and sim-
ple; crossveins are rare in the distal portion of the wing.
Genus PARAPALAEOLEON gen. nov.
Type and only species. Parapalaeoleon magnus sp. nov.
Derivation of name. Greek, para, near, and Palaeoleon, a generic
name. Gender masculine.
Diagnosis. May be distinguished from other genera of the
family by the combination of the following forewing char-
acter states: (1) origin of Rs1 far removed from origin of
Rs [near origin of Rs in Baisopardus, Palaeoleon]; (2) Rs1
shallowly branched, highly distal to the Banksian fold
[deeply branched, at most slightly distal to the Banksian
fold in Baisopardus, Palaeoleon]; (3) maximum width of
wing at mid-point [in distal portion in Baisopardus and
in proximal portion in Palaeoleon].
Remarks. The new genus is most similar to Baisopardus
and Palaeoleon; other genera are very distant from it.
Parapalaeoleon and Baisopardus both occur in the Crato
Formation and are clearly distinguished from each other
(see diagnosis above). In general, all three genera differ in
the shape of the wing: wide basally with a somewhat elon-
gated apex in Palaeoleon, narrower basally and widest at
mid-length in Parapaleoleon; maximum width after the
mid-wing in Baisopardus. The wing shape of Baisopardus
araripensis, however, is more similar to that of Parapalaeo-
leon magnus, than to other species of Baisopardus, but it
possesses other character states of Baisopardus, e.g. Rs1
originates near the base of Rs and is deeply branched.
Parapalaeoleon magnus sp. nov.
Text-figures 3–4
Derivation of name. Latin adjective, magnus, large, in reference
to the large size of the species.
Holotype. SMNS 66000 ⁄ 268. An incomplete specimen exposed
in lateral aspect, including head, thorax with appendages, and
right forewing.
Type locality and horizon. As for Nuddsia longiantennata above.
Diagnosis. As for the genus.
Description. Head 4 mm long. Compound eyes 2.5 mm in diam-
eter. Antennae 25 mm long, composed of 71 preserved segments:
scape not preserved; first visible segment wider than other flagel-
lar segments, which are square basally, transverse distad. Thorax
not complete (9 mm long as preserved), compressed, exoskeleton
mostly not preserved; prothorax apparently comparatively short.
Foreleg: coxa 2 mm long; femur rather stout, 6 mm long; tibia
stout, 5 mm long, armed with apical spine; tarsus 4 mm long,
five-segmented, distalmost segment approximately as long as four
basal segments together; claws very long, 2 mm. Midleg: coxa
2 mm long; femur 6 mm long; tibia 4.5 mm long, apical spines
not detected; tarsus as in forelegs. Hind legs not preserved.
Forewing widest at mid length, 67–68 mm long (estimated), c.
20 mm wide. Costal space narrow, 1.5 mm wide in basal part,
slightly narrowed toward fusion of Sc, R1, strongly expanded
beyond this. Subcostal veinlets simple, perpendicular to Sc in
basal half of costal space, oblique, forked distally. Veinlets of
Sc+R1 long, very oblique, usually dichotomously forked, con-
nected by occasional crossveins not forming a regular gradate
series. Sc and R1 fused at 12 mm from wing apex, entering wing
margin apparently well after apex (apical portion of wing not
preserved). No crossveins in subcostal space. Pterostigma absent
or not discernible. Stem of Rs straight, not zigzagged for entire
length; its origin situated near wing base, inclined at a very acute
angle to R1. No presectorial crossveins detected. R1 space most
dilated at middle portion, strongly narrowed basad and distad;
85 very closely spaced crossveins proximal to fusion of Sc, R1.
Long hypostigmal cell absent. Rs with 13 branches, somewhat
sigmoid in configuration, branched dichotomously distally. Ori-
gin of Rs1 located 21 mm from origin of Rs; branches of Rs
dichotomously branched distally; Rs1 branched much distal to
Banksian fold. Rs2, Rs3 appear fused. Median flexion line dis-
tinct, running between MA, Rs, then Rs1 from wing base to Rs3.
Anterior Banksian fold distinct, beginning slightly distal to Rs1,
directed to wing apex (somewhat posterior to it), unaccompa-
nied by false longitudinal vein formed by bending of branches of
Rs and crossveins connecting them. Radial crossveins very
numerous, not forming gradate series. Origin of M not pre-
served, probably not fused with R at wing base. Fork of M
rather distinct, with origin of MA forming shallow angle with
stem of M, and MP (‘oblique vein’) stouter than crossveins in
median space. MA simple, with only shallow marginal fork,
straight, curved posteriorly distally. ‘Oblique vein’ well devel-
oped, located slightly proximal to most proximal branch of
MP+CuA. CuA, MP+CuA strongly convex, both parallel to MA,
dense crossveins for entire length between these and MA.
MP+CuA with 12 branches, of which most proximal branch
(MP+CuA1) pectinately branched; next branch (MP+CuA2)
fused with it; MP+CuA3 with deep fork; other branches shal-
lowly forked. All branches of MP+CuA connected by numerous
156 P A L A E O N T O L O G Y , V O L U M E 5 1
crossveins; near posterior margin crossveins connected by addi-
tional crossveins forming short irregular pseudo-longitudinal
veins. Crossveins between CuA (also MP+CuA1), CuP numer-
ous, dense. CuP concave basally, rather short, with shallow mar-
ginal fork, seven simple branches, crossveins between them rare.
1A not fused basally with CuP. Two short unbranched anal veins
preserved (1A, 2A).
Family MESOCHRYSOPIDAE Handlirsch, 1906
Genus TRIANGULOCHRYSOPA Nel et al., 2005
Type species. Triangulochrysopa sanzi Nel et al., 2005, by original
designation.
A
C
B
TEXT -F IG . 3 . Parapalaeoleon magnus
gen. et sp. nov., holotype, SMNS
66000 ⁄ 268. A, photograph of the
specimen. B, close-up of forewing
showing fusion of MP and CuA (the
names of the veins are partly
hypothetical; see text for detail). C,
portion of forewing showing median
flexion line (mfl) and anterior Banksian
fold (bf). Scale bars represent 10 mm.
TEXT -F IG . 4 . Parapalaeoleon magnus
gen. et sp. nov., holotype, SMNS
66000 ⁄ 268. A, anterior part of body. B,
forewing. Scale bars represent 5 mm.
M E N O N A N D M A K A R K I N : C R E T A C E O U S F O S S I L L A C E W I N G S A N D A N T L I O N S F R O M B R A Z I L 157
Diagnosis. Prothorax somewhat elongated. Forelegs
rather short, probably raptorial. Forewing: MP touching
(or almost touching) CuA; venation in radial to cubital
spaces highly reticulated. Hindwing triangular in shape
with distinct tornus, rather long (0.67 times forewing
length); apex of wing acute; MP appears to be continua-
tion of M; MA arising from M at right angle or nearly
so.
Included species. Triangulochrysopa sanzi (Lower Cretaceous, Bar-
remian, Las Hoyas, Spain, La Huerguina Formation), T. formosa
sp. nov. (Lower Cretaceous, Upper Aptian, Araripe Basin, Brazil,
Crato Formation).
Remarks. Triangulochrysopa is most similar to the Lower
Cretaceous genera Allopterus Zhang, 1991 and Karenina
Martins-Neto, 1997 in the structure of the pronotum,
and its foreleg and forewing venation. It may be easily
distinguished from these by hindwing size, shape and
venation: e.g. the hindwing is short and broad, c. 0.4 of
forewing length, with rounded apex and reduced venation
in Allopterus, and relatively narrow, without tornus, 0.6–
0.8 of forewing length, with different venation (in partic-
ular, Rs inclined at a more acute angle to R1, with Rs1
originating more distally) in Karenina (Makarkin and
Menon 2005; Nel et al. 2005).
According to Nel et al. (2005), Triangulochrysopa (with
Allopterus, Karenina and Armandochrysopa Nel et al.,
2005) belongs to the family Allopteridae in the superfam-
ily Chrysopoidea. They proposed the following phyloge-
netic relationship: (Cratochrysa Martins-Neto, 1994 +
(Liassochrysidae + (Paralembochrysa Nel et al., 2005 +
((Allopteridae + Mesochrysopidae + Tachinymphidae +
Mesotermes Haase, 1890) + (Limaiidae + Chrysopi-
dae))))). We have previously regarded Mesotermes and
the genera of Allopteridae, Mesochrysopidae and Tachi-
nymphidae as forming the single, monophyletic family
Mesochrysopidae (Makarkin and Menon 2005). We are
still of the opinion that the elevation of these groups
(and Limaiidae) to family rank is unjustified.
Triangulochrysopa formosa sp. nov.
Text-figures 5–6
2001 Unnamed neuropteran; Bechly et al. p. 55, fig. 45.
Derivation of name. Latin adjective, formosus, graceful, beautiful,
with reference to the appearance of the holotype.
Holotype. SMNS 66000 ⁄ 271. A complete well-preserved speci-
men exposed in ventral aspect, with all wings wide open; disar-
ticulated fragments of legs are visible along the abdomen in the
matrix.
Type locality and horizon. As for Nuddsia longiantennata above.
Diagnosis. Triangulochrysopa formosa may be distin-
guished from T. sanzi by the following forewing charac-
ters: forewing more elongate, length ⁄ width ratio 4.0 [3.3
in the holotype of T. sanzi], pterostigma distinct [absent
(or not detectable) in T. sanzi], MP touching CuA [con-
nected by short crossvein in T. sanzi], 1A with two
branches [one in T. sanzi].
Description. Head oval, wider than long, 4.5 mm long, 2.6 mm
wide with large compound eyes, each 1 mm in diameter. Anten-
nae incomplete, 13 mm long (estimated), filiform; scape not pre-
served, flagellum composed of at least 40 equal segments.
Prothorax elongate, 3.5 mm long, 2.3 mm wide; mesothorax and
metathorax oval, robust, 8 mm long, 4 mm wide. Legs only
partly preserved: fragmentary coxae on all three pairs of legs;
right foreleg: femur rather stout, 3.5 mm long, tibiae 3.7 mm
long; disarticulated tarsus (belonging probably to left midleg)
with five cup-shaped segments (total length 3 mm), bearing two
distinct claws. Abdomen composed of nine segments, 22 mm
long.
Forewing: elongate with sub-acute apex, 44 mm long, 11 mm
wide (length ⁄ width ratio 4.0). Costal space narrow, slightly
dilated towards pterostigma. Subcostal veinlets proximal to
pterostigma simple (one forked, obviously an anomaly), 36 in
number, perpendicular to Sc or inclined to apex, becoming
increasingly inclined, closely spaced to pterostigmal region; ante-
rior tip of most basal subcostal (humeral) veinlet inclined
towards base. Veinlets of Sc, Sc+R1 distal to pterostigma mostly
forked, connected by 1–2 crossveins, forming 2–3 rows of cells
between C, Sc+R1. Pterostigma dark coloured, 3.5 mm long,
covering seven cells. No crossveins in subcostal space detected.
Sc, R1 fused distal to pterostigma. Sc+R1 entering wing margin
at apex. Stem of Rs straight, zigzagged distally; its origin 4.5 mm
from wing base. R1 space dilated at origin of Rs1, 1.3 mm
(wider than width of costal space), narrowed towards apex, with
28 crossveins; Rs with 20 zigzagged branches not forked before
marginal forks, each with 1–2 crossveins connected to branches
of fork. Venation in radial space highly reticulated, not forming
distinct gradate series. In radial space two longitudinal conver-
gent folds present. No crossvein between stem of Rs, M. Origin
of M at 3 mm from wing base. M moderately convex, divided
into MA, MP at 8 mm from wing base and at relatively acute
angle (c. 45 degrees). MA smooth, slightly convex, entering mar-
gin well before wing mid-point, with marginal fork. MP zig-
zagged, without marginal fork, with two long zigzagged
branches. Crossveins in medial space not arranged in regular ser-
ies. Basal crossvein m-cu located slightly distal to origin of M,
oblique, long. Cu not fused with R basally, divided into CuA,
CuP distal to crossvein m-cu. CuA strongly convex, straight,
only slightly bent at MP touching, ending in very shallow mar-
ginal fork and with single short branch (it is difficult to identify
these with certainty as the venation in medial and cubical spaces
is highly reticulated; CuA could be also strongly zigzagged in
distal half, with two branches having each wide marginal fork).
CuA touching MP. CuP short, with two short branches. Basal
158 P A L A E O N T O L O G Y , V O L U M E 5 1
crossvein cua-cup oblique, long, situated slightly proximal to
meeting point of MP, CuA; distal crossvein cua-cup oblique,
rather short, situated far distal to meeting point of MP and
CuA. At least one distal crossvein between CuP, 1A. 1A, 2A
nearly parallel to hind margin; 1A with one branch; 2A not
branched. 3A not detected.
Hindwing: subtriangular in shape with somewhat pointed
apex, 28 mm long, 8.5 mm maximum width. Costal space
equally narrow throughout length (0.5 mm). Subcostal veinlets
simple, forming 31 cells proximal to pterostigma. Pterostigma
short (1 mm long), covering three cells, dark coloured. Sc and
R1 fused distal to pterostigma. No crossveins in subcostal space
detected. Origin of Rs at 5.7 mm from wing base. R1 space
1 mm at its widest point, with 17 crossveins; hypostigmal cells
short. Stem of Rs zigzagged, with 12 zigzagged branches, simple
(distal branches) or with shallow, wide marginal fork (proximal
branches). Crossveins in radial space numerous, not forming
distinct gradate series. M dividing into MA, MP at 4 mm from
wing base; MP appears to be a continuation of M, MA arising
from M nearly at right angle. MA smooth, only slightly arched,
with marginal fork entering wing margin at mid-point (15 mm
from wing base). MP zigzagged, divided into two long branches.
CuA strongly convex basally, touching MP at nearly half of its
length, strongly zigzagged distally, with seven short branches.
Venation between MA, CuA strongly reticulated (especially dis-
tally, making it impossible to discriminate with certainty longi-
tudinal veins from crossveins). CuP, anal veins not detected.
Remarks. Both species of the genus, T. sanzi and T. for-
mosa, are very similar to each other. T. sanzi was
described from five specimens from the Barremian of Las
Hoyas, Spain, which differ somewhat in size (forewing
length ranges from 27.5 to 39.2 mm) and venation. Nel
A
B
TEXT -F IG . 5 . Triangulochrysopa formosa sp. nov. A, photograph, and B line drawing of the holotype, SMNS 66000 ⁄ 271. Scale bar
represents 10 mm.
M E N O N A N D M A K A R K I N : C R E T A C E O U S F O S S I L L A C E W I N G S A N D A N T L I O N S F R O M B R A Z I L 159
et al. (2005) considered these differences insufficient to
separate them; however, some may be significant at a spe-
cific level. For example, the hindwing venation of the
specimens 92 ⁄ 2 ⁄ 3 (Nel et al. 2005, fig. 7.5) and LH-18572
(Nel et al. 2005, fig. 7.4) of T. sanzi is very different; they
are 19.2 mm and 21.6 mm long respectively, whereas the
hindwing of the holotype is 31.6 mm long (unfortunately,
this wing was not figured). The hindwing ⁄ forewing length
ratio ranges from 0.55 to 0.66 in these paratypes, and is
0.95 in the holotype. The photograph of the holotype
does not reveal such long hindwings; the measurement
should probably be 21.6, not 31.6 mm. In any case, after
this discovery of another very similar species from a
South American locality distant from southern Europe, all
material previously identified as T. sanzi should be
revised.
Acknowledgements. We thank Dr Gunter Bechly and Dr Gerd
Dietl (SMNS) for allowing us to study the material we have
described; Dr Andre Nel (Museum national d’Histoire naturelle,
Paris) and Prof. Dr Rafael Martins-Neto (Universidade Federal
de Juiz de Fora, Brazil) for providing us with advance copies of
their papers in press; Prof. Dr Ulrike Aspock and Dr Harald
Schillhammer (Naturhistorisches Museum Wien) for providing
the photograph of the holotype of Gumilla adspersa; Jean
Dougherty (Geological Survey of Canada, Ottawa, Canada), and
Bruce Archibald (Museum of Comparative Zoology, Harvard
University) for providing the photograph of the holotype of Pal-
aeoleon ferrogeneticus; Mr Robert Loveridge (University of Ports-
mouth) for providing the photograph of the holotype of
Baisopardus chryptohymen; Bruce Archibald for helpful com-
ments and for suggestions on the English; James Jepson (Univer-
sity of Manchester) for correcting our English; Dr Gunter Bechly
and Dr Rafael Giois Martins-Neto for reviewing the manuscript;
and Prof. David Batten (University of Manchester) for editorial
work. The visit to Stuttgart by FM was funded by the Deutscher
Akademischer Austausch Dienst (DAAD).
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