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Middle Miocene vertebrates from the Amazonian Madre
de Dios Subandean Zone, Perú
Pierre-Olivier Antoine, Martin Roddaz, Stéphanie Brichau, Julia Tejada-Lara,
Rodolfo Salas-Gismondi, Ali Altamirano, Mélanie Louterbach, Luc Lambs,
Thierry Otto, Stéphane Brusset
To cite this version:
Pierre-Olivier Antoine, Martin Roddaz, Stéphanie Brichau, Julia Tejada-Lara, Rodolfo Salas-
Gismondi, et al.. Middle Miocene vertebrates from the Amazonian Madre de Dios Subandean
Zone, Perú. Journal of South American Earth Sciences, Elsevier, 2013, vol. 42, pp. 91-102.
￿10.1016/j.jsames.2012.07.008￿. ￿hal-00956894￿
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To link to this article
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http://dx.doi.org/10.1016/j.jsames.2012.07.008
To cite this version
: Antoine, Pierre-Olivier and Roddaz, Martin and
Brichau, Stéphanie and Tejada-Lara, Julia and Salas
-Gismondi,
Rodolfo and Altamirano, Ali and Louterbach, Mélanie
and Lambs, Luc
and Otto, Thierry and Brusset, Stéphane Middle Mioc
ene vertebrates
from the Amazonian Madre de Dios Subandean Zone, Pe
rú. (2013)
Journal of South American Earth Sciences, vol. 42 .
pp. 91-102. ISSN
08959811
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Middle Miocene vertebrates from the Amazonian Madre de Dios Subandean Zone,
Perú
Pierre-Olivier Antoine
a
,
*
, Martin Roddaz
b
, Stéphanie Brichau
b
, Julia Tejada-Lara
c
,
d
,
Rodolfo Salas-Gismondi
c
, Ali Altamirano
c
, Mélanie Louterbach
b
,
e
, Luc Lambs
f
, Thierry Otto
f
,
Stéphane Brusset
b
a
Institut des Sciences de l
Évolution, UMR-CNRS 5554, CC064, Université Montpellier 2, Place Eugène Bataillon, F-34095 Montpellier, France
b
Géosciences-Environnement Toulouse, Université de Toulouse, UPS (SVT-OMP), LMTG, CNRS, IRD, 14 Avenue Édouard Belin, F-31400 Toulouse, France
c
Museo de Historia Natural-Universidad Nacional Mayor San Marcos, Departamento de Paleontología de Vertebrados, Avenida Arenales 1256, Lima 11, Perú
d
Institut Français d
Etudes Andines, Avenida Arequipa 4500, Lima 18, Perú
e
Institut Polytechnique Lasalle Beauvais, Département Géosciences, 19 rue Pierre Waguet, F-60026 Beauvais Cedex, France
f
EcoLab, UMR 5245 CNRS-UPS-INPT, Université de Toulouse, 118 Route de Narbonne, F-31062 Toulouse Cedex 9, France
Keywords:
Colloncuran-early Laventan
Marsupialia
Rodentia
Biochronology
Fission track age
Biogeography
abstract
A new middle Miocene vertebrate fauna from Peruvian Amazonia is described. It yields the marsupials
Sipalocyon
sp. (Hathliacynidae) and
Marmosa
(
Micoureus
) cf.
laventica
(Didelphidae), as well as an
unidenti
fi
ed glyptodontine xenarthran and the rodents
Guiomys
sp. (Caviidae),
ª
Scleromys
º
sp., cf.
quadrangulatus-schurmanni-colombianus
(Dinomyidae), an unidenti
fi
ed acaremyid, and cf.
Micro-
steiromys
sp. (Erethizontidae). Apatite Fission Track provides a detrital age (17.1
2.4 Ma) for the locality,
slightly older than its inferred biochronological age (Colloncuran-early Laventan South American Land
Mammal Ages:
w
15.6
e
13.0 Ma). Put together, both the mammalian assemblage and lithology of the
fossil-bearing level point to a mixture of tropical rainforest environment and more open habitats under
a monsoonal-like tropical climate. The fully
fl
uvial origin of the concerned sedimentary sequence
suggests that the Amazonian Madre de Dios Subandean Zone was not part of the Pebas mega-wetland
System by middle Miocene times. This new assemblage seems to reveal a previously undocumented
ª
spatiotemporal transition
º
between the late early Miocene assemblages from high latitudes (Patagonia
and Southern Chile) and the late middle Miocene faunas of low latitudes (Colombia, Perú, Venezuela, and
?Brazil).
1. Introduction
The middle Miocene period is characterised by the last climatic
optimum (MMCO, for Middle Miocene Climatic Optimum) before
a sustainable deterioration culminating with Pliocene
e
Pleistocene
ice ages (
Zachos et al., 2001
,
2008
). In Northern South America, this
MMCO coincides with the emergence of the
ª
Pebas system
º
, a large
wetland with marine in
fl
uence partly engul
fi
ng what is lowland
Amazonia today (for review, see
Hoorn et al., 2010a
,
b
).
This environment was particularly favourable to biodiversity
and it allowed a wide array of organisms, such as molluscs,
arthropods, and plants to be fossilised (e.g.,
Hoorn, 1993
;
Antoine
et al., 2006
;
Pons and De Franceschi, 2007
;
Jaramillo et al., 2010
;
Wesselingh and Ramos, 2010
). By contrast, and with the notable
exceptions of La Venta (late middle Miocene, Colombia;
Kay et al.,
1997
) and Fitzcarrald local fauna (eastern Perú;
Antoine et al.,
2007
;
Goillot et al., 2011
;
Pujos et al., in press
), middle Miocene
mammals are virtually unknown in tropical-equatorial South
America (e.g.,
Negri et al., 2010
).
The present work aims to report a new vertebrate locality from
the Subandean Zone of Southwestern Peru, designated MD-67
(S12
!
38.683
0
; W71
!
19.284
0
;
w
428 m Above Sea Level) and doc-
umenting the concerned interval. MD-67 was discovered by one of
us (MR) nearby Pilcopata (Cusco) in 2007 (
Fig. 1
). The corre-
sponding results are exposed hereunder in systematic, bio-
stratigraphical, and biogeographical perspectives.
1.1. Geological context
The western Amazon drainage basin extends today from
southern Colombia to northern Bolivia (
Hoorn et al., 2010a
). Since
Pliocene times (
Espurt et al., 2007
,
2010
), the Amazonian foreland
*
Corresponding author. Tel.:
þ
33 467 143 251; fax:
þ
33 467 143 640.
E-mail address:
pierre-olivier.antoine@univ-montp2.fr
(P.-O. Antoine).
http://dx.doi.org/10.1016/j.jsames.2012.07.008
basin has been divided into two foreland basin systems (
sensu
DeCelles and Giles, 1996
): the North Amazonian foreland basin
system and the South Amazonian foreland basin, separated by the
Fitzcarrald Arch (
Roddaz et al., 2005
). The South Amazonian fore-
land basin system comprises the Southern Peruvian and Northern
Bolivian foreland basins. The Subandean Zone is part of the Madre
de Dios foreland basin (
Fig. 1
). The southernmost part of the Sub-
andean Zone is structured by a syncline (Salvación Syncline) fol-
lowed by a thrust-related anticline (Pantiacolla Anticline) and the
Madre de Dios blind thrust front (
Fig. 1
).
The fossiliferous outcrop dips 35
!
SW with a N130 strike (
Fig. 2
).
It crops out in the southern
fl
ank of the Pantiacolla anticline and
was originally mapped as part of the Paleocene
e
Eocene Yahuar-
ango Formation, based on sedimentary facies, but without any
biostratigraphic constraint (
Vargas and Hipólito, 1998
). The
Yahuarango Formation (northern Perú) is poorly dated and it
consists mainly of red siltstones and mudstones forming distal
fl
uvial deposits (see
Roddaz et al., 2010
for a review).
The fossiliferous level corresponds to a 1 m-thick sand-and-
gravel channel of
fl
uvial origin, with iron-rich pisolites and top-
ped by a ferruginous duricrust (
Fig. 2
A). These features coincide
with a lateritic pro
fi
le (e.g.,
Tardy, 1992
). The fossiliferous channel
developed over paleosol mudstones (
Fig. 2
A and B).
2. Material and methods
2.1. Paleontology
All the vertebrate fossil remains described here were recovered
either by hand-picking on the ferruginous crust topping the MD-67
locality during the exploratory 2007
fi
eld trip, or by excavating and
by screen-washing of the corresponding sediment during the 2009
fi
eld season. In 2009, ca. 200 kg of rough sediment were screen-
washed, using a 1 mm mesh. A new survey in 2011 unfortunately
showed the fossil-yielding outcrop had been washed away by the
Madre de Dios River in the meantime (
Fig. 2
C).
F
ragments of turtle plates and crocodile teeth were also recov-
ered in MD-67. As they do not display diagnostic features, they will
not be described here. By contrast, neither
fi
sh nor plant remains
were unearthed in MD-67.
Among mammalian remains, a mesio-labial fragment of a hyp-
selodont upper tooth referable to a toxodontid notoungulate was
recognised in MD-67. This specimen, of poor biochronological and
environmental use, is the only remain unambiguously assignable to
native ungulates in the concerned locality.
The nomenclature used for marsupial dentition is adapted from
that of
Goin and Candela (2004)
. Morphological features of the
cavioid rodent are described and diagnosed following the termi-
nology and phylogenetic characters proposed by
Pérez (2010)
. For
dental features of the dinomyid, octodontoid, and erethizontid
rodents, we follow the nomenclature of
Wood and Wilson (1936)
,
as modi
fi
ed by
Antoine et al. (2012)
.
Except when mentioned, dimensions are given in mm.
2.2. Apatite
fi
ssion track analysis (AFTA)
Apatite grains were mounted and polished for etching to several
the natural spontaneous
fi
ssion tracks. Apatites were etched using
5 N HNO
3
at 20
!
C for 20 s. Etched grain mounts were packed with
mica external detectors and corning glass (CN5) dosimeters and
irradiated in the FRM 11 thermal neutron facility at the University
of Munich in Germany. Following irradiation the external detectors
were etched using 48% HF at 20
!
C for 25 min. Analyses were
carried out on a Zeiss Axioplan microscope at a magni
fi
cation
of
$
1250, using a dry (
$
100) objective. Con
fi
ned track length
measurements were made using a drawing tube and digitising
tablet, calibrated against a stage micrometre. Single-grain AFT ages
were calculated using the external detector method and the zeta
calibration approach, as recommended by the I.U.G.S. Subcom-
mission on Geochronology (
Hurford, 1990
). Track length
measur
ements were restricted to con
fi
ned tracks parallel to the c-
crystallographic axis.
2.3. Institutional abbreviations
AMNH, American Museum of Natural History, New York, USA;
IGM, Ingeominas (Instituto Nacional de Investigaciones en Geo-
ciencias, Minería y Química, Museo Geológico, Bogotá, Colombia;
ISE-M, Institut des Sciences de l
Évolution, Montpellier, France;
MACN, Museo Argentino de Ciencias Naturales Bernardino Riva-
davia, Buenos Aires, Argentina; MLP, Museo de Ciencias Naturales
de La Plata, La Plata, Argentina; MNHN, Muséum National d
Histoire
Naturelle, Paris; MUSM, Museo de Historia Natural de la Uni-
versidad Nacional Mayor San Marcos, Lima, Perú; UCMP, University
of California Museum of Paleontology, Berkeley, USA; UFAC, Labo-
ratório de Pesquisas Paleontológicas, Universidade Federal do Acre,
Rio Branco, Brazil.
Fig. 1.
Location and geological map of the studied area, in the Amazonian Madre de
Dios Subandean Zone, Perú; modi
fi
ed after
Vargas and Hipólito (1998)
.
2.4. Other abbreviations
dist., distal; est., estimated; FAD, First Appearance Datum;
H
,
height; HI, Hypsodonty Index (
¼
H
/MDL);
L
, length; max, maximal;
LLO, Last Local Occurrence; MDL, mesio-distal length; mes, mesial;
SALMA, South American Land Mammal Age;
W
, width.
3. Systematic Paleontology
Class MAMMALIA Linnaeus, 1758
Cohort MARSUPIALIA Illiger, 1811
Order DIDELPHIMORPHIA Gill, 1872
Suborder SPARASSODONTA Ameghino, 1894
Superfamily BORHYAENOIDEA Ameghino, 1894
Subfamily HATHLIACYNIDAE Ameghino, 1894
Sipalocyon
Ameghino, 1887
Sipalocyon
sp.
MUSM 1967 is a much worn and eroded tooth, with a tribos-
phenic bunodont pattern and three broken roots (one lingual and
two labial ones). Following the work of
Forasiepi et al. (2006)
, this
tooth is interpreted as a right M3 of a carnivorous marsupial. It is
roughly triangular in occlusal view, with a straight mesial side (mes
W
¼
5.10), a long and bilobed distolingual border (max
L
¼
6.69),
and a concave labial side (MDL
¼
4.67). Crown height equals
3.24 mm. The paracone and the metacone have their bases twin-
ned, thus determining a very short premetacrista. Even if its tip is
broken away and eroded, the paracone was low, with a faint pre-
paracrista; the most prominent cusp is the metacone, which
occupies a central position in occlusal view (
Fig. 3
A and B). The
paraconule and the metaconule are equally developed, and closely
appressed to the paracone and metacone, respectively (
Fig. 3
A and
B). The protocone is bulbous, much lower than the latter cusps, and
widely remote from them, which further determines a wide
triangular basin which is bordered by a faint preprotocrista and
a low postprotocrista. The postmetacrista is strongly developed and
distally convex, with a
fl
at and high vertical wear facet but without
carnassial notch (
Fig. 3
B). The stylar shelf is smooth and reduced,
with faint or absent cusps. Yet, a rounded crest surrounds the
mesiolabial corner of the tooth, which was either interpreted as an
ectocingulum or a
ª
Cusp B
º
(
Marshall, 1978
;
Forasiepi et al., 2006
).
The main morphological features of this tooth (tribospheny,
reduced protocone, paracone and metacone closely appressed, and
reduced stylar shelf and cusps) point to a carnivorous marsupial, as
de
fi
ned by
Muizon (1999: 502)
. The presence of a thick and low
protocone, and of equally developed paraconule and metaconule
allow referring it as to a medium-sized hathliacynid borhyaenoid
(
Forasiepi et al., 2006
). Accordingly, comparison was made with
Cladosictis
Ameghino, 1887 (early Miocene of Argentina and Chile;
Flynn et al., 2002
)
Sipalocyon
Ameghino, 1887 (Colhuehuapian-San-
tacrucian of Patagonia;
Marshall, 1981
),
Acyon
Ameghino, 1887
(middle Miocene of Southern Bolivia;
Forasiepi et al., 2006
), and
Notogale
Loomis, 1914 (Deseadan of Bolivia and Argentina;
Muizon,
1999
). A similar large-sized lingual basin is only observed in
Noto-
gale mitis
(Ameghino,1897), as illustrated by
Marshall (1981: Figs. 54
and 55)
. Based oncompatible proportions/size and onthe presence of
an ectocingulum, MUSM 1967 shows the closest af
fi
nities with the
M3 of
Sipalocyon gracilis
Ameghino, 1887 (AMNH 107401-001; FM
9254-001; Santacrucian) and
Sipalocyon externa
(Ameghino, 1902)
(Colhuehuapian;
Marshall, 1981
). It differs from
S. externa
in having
a lower and smoother protocone, a very wide lingual basin, labially-
displaced paracone and metacone, and in showing a more developed
paraconule and metaconule (
Marshall, 1981
), but closely resembles
the M3 of
S. gracilis
from
ª
Río Coyle
º
(maxilla MNHN SCZ 122,
Fig. 2.
Middle Miocene vertebrate locality MD-67, in the Amazonian Madre de Dios Subandean Zone, Perú. A. Detail of the fossil-yielding red sand-and-gravel channel, developing
over red clays (paleosol), as discovered in October 2007. Note the dipping of the topping surface (ferruginous duricrust). Picture by Patrice Baby. B. Detail of the transition between
the underlying red clays (top) and the gravel channel, with iron-rich pisolites (black balls, at the bottom). Picture by Patrice Baby (same day as in
Fig. 2
A). C. The same area in August
2011. The fossil-yielding channel (denoted by the white dotted line) had been washed away by the Madre de Dios River in the meantime. Picture by Laurent Marivaux. (For
interpretation of the references to colour in this
fi
gure legend, the reader is referred to the web version of this article.)
Tournouër Collection; Santa Cruz Formation, Patagonia) in all these
aspects.
Sipalocyon
has a Colhuehuapian
e
Friasian range, so far
restricted to middle and high latitudes (37.5
e
48
!
S;
Marshall, 1981
;
Flynn et al., 2008
). Recognition of a hathliacynid closely allied to
Sipalocyon
, here referred as to
Sipalocyon
sp., widely extends north-
ward the geographical range of the genus.
Superfamily DIDELPHOIDEA Gray, 1821
Family DIDELPHIDAE Gray, 1821
Subfamily DIDELPHINAE Gray, 1821
Tribe MARMOSINI Reig, Kirsch and Marshall in Reig, 1981
Genus
Marmosa
Gray, 1821
Fig. 3.
Fossil mammal remains from the MD-67 locality, middle Miocene of the Amazonian Madre de Dios Subandean Zone, Perú. A
e
B.
Sipalocyon
sp., right M3 (MUSM 1967) in
labial (A) and occlusal views (B). C.
Marmosa
(
Micoureus
) cf.
laventica
, left M3 lacking the protocone (MUSM 1968). Reconstructed areas appear in grey (reconstruction based on
Marshall, 1976
: text-Fig. 2). D
e
E. Glyptodontinae indet., isolated osteoderms in external view. D, MUSM 1720; E, MUSM 1585. F
e
H,
Guiomys
sp., left M1/2 (MUSM 1970) in occlusal
(F), labial (G), and mesial views (H). I
e
K,
ª
Scleromys
º
sp., gr.
quadrangulatus-schurmanni-colombianus
. Left d4 (MUSM 1971) in occlusal view (I). Left m1 (MUSM 1972) in occlusal (J)
and labial views (K). L, Acaremyidae indet., left m1/2 (MUSM 1973) in occlusal view. M
e
N, cf.
Microsteiromys
sp. Left P4 (MUSM 1974) in occlusal view (M). Right ?M3 (MUSM 1975)
in occlusal view (N). Scale bar
¼
2 mm (A
e
B, F
e
K), 5 mm (
D
e
E), or 1 mm (C, L
e
N).
Subgenus
Micoureus
Lesson, 1842
sensu
Voss, and Jansa, 2009
:
101
Marmosa
(
Micoureus
) cf.
laventica
Marshall, 1976
MUSM 1968 is a left upper molariform tooth, the protocone of
which was broken away. This tooth has a dilambdodont tribos-
phenic pattern, a large stylar shelf, and four stylar cusps (termed A
e
D). It bears one lingual and two labial roots. The tooth is almost
unworn and its dimensions are very small (MDL
¼
1.75; est
W
¼
1.8). The metacone is much larger and higher than the para-
cone. There was neither paraconule nor metaconule. All these
features point to a marmosine didelphid rather than to a micro-
biothere (
Marshall, 1976
). MUSM 1968 was compared to the M1
e
M3 series UCMP 108563 of
ª
M
.
laventica
Marshall, 1976
º
from the
middle Miocene of La Venta, Colombia, described and illustrated by
Marshall (1976: text-Fig. 2)
, as well as to the isolated M1 IGM
251011 and M3 IGM 250278 of the same species and area, as
described and
fi
gured under the name
ª
M
.
laventicus
º
by
Goin
(1997: Fig. 11.2)
. Its isometric proportions, moderate dissymmetry
(with a lingual part slightly mesially displaced), and concave labial
border in occlusal view allow identifying it as an M3. The missing
part of the tooth was virtually reconstructed, based on available
illustrations of
M.
(
Mi
.)
laventica
(
Fig. 3
C). There was neither junc-
tion between the preprotocrista and the paracone nor between the
postprotocrista and the metacone. The stylar cusp A is disconnected
from the paracone and from the preparacrista. The stylar cusp B
appears as the strongest cusp, as it does in fresh teeth of most
marmosines (
Rossi et al., 2010
: 22). There is a deep mesiolabial
notch for the metastyle of M2, but neither labial, nor distal
cingulum, as in
M.
(
Mi
.)
laventica
(
Marshall, 1976
) and the living
species
M.
(
Mi
.)
demerarae
Thomas, 1905 (ISE-M V-1590). A thick
cingulum, running along the labial half of the mesial side, was
connecting the stylar cusp A and the protocone through the pre-
protocrista, as in the isolated M3 IGM 250278 of
M.
(
Mi
.)
laventica
(
Goin, 1997
). This cingulum is much stronger and the tooth ca. 30%
smaller than in
M.
(
Mi
.)
demerarae
. Even if their overall size is
comparable, the stylar cusps are much stronger and the notch for
the metastyle of M2 is much deeper in MUSM 1968 than in the M3s
of the living
Marmosa
(
Marmosa
)
murina
Linnaeus,1758 (Linnaeus
s
Mouse Opossum; ISE-M V-1109).
Basically, the size, proportions, and morphological features of
MUSM 1968 closely match those of the M3 of
M.
(
Mi
.)
laventica
from
La Venta area, Colombia, i.e., the only fossil species described and
named for this genus so far (
Goin, 1997
). The stratigraphical range
of
M.
(
Mi
.)
laventica
spans the La Victoria Fm. and the base of the
Baraya Mb. of the overlying Villavieja Fm. in La Venta region,
Colombia (
w
13.5
e
13.0 Ma;
Goin, 1997
;
Madden et al., 1997
: 511;
Gradstein et al., 2005
). If the close af
fi
nities of MUSM 1968 with
Marmosa
(
Micoureus
) are con
fi
rmed, this would be the second fossil
occurrence of this living (sub-) genus (
Goin, 1997
).
Infraclass EUTHERIA Gill, 1872
Order XENARTHRA Cope, 1889
Suborder CINGULATA Illiger, 1911
Superfamily GLYPTODONTOIDEA Gray, 1869
Family GLYPTODONTIDAE Gray, 1869
Subfamily GLYPTODONTINAE Gray, 1869
Genus and species indet.
Two isolated carapace osteoderms were found. They are small
(MUSM 1720:
W
¼
16, preserved
L
¼
22; MUSM 1585:
W
¼
13,
L
¼
17),
quadrangular to pentagonal in shape, with large round principal
fi
gures near the posterior edge. In both osteoderms, the principal
fi
gure is completely surrounded by peripheral ones
e
eight in MUSM
1720 (
Fig. 3
D) and six in MUSM 1585 (
Fig. 3
E)
e
,
although medial,
lateral, and posterior
fi
gures are reduced in size. The principal
fi
gure
is slightly convex on MUSM 1720, while it is
fl
at on MUSM 1585.
Osteoderms are thin (MUSM 1720: 3.5 mm; MUSM 1585: 4.8 mm),
with a punctuated surface, and serrated edges. The principal and
radial sulci are wide and shallow. Piliferous pits are large and located
in some intersections of the principal sulcus and the radial sulci
(
Fig. 3
D
e
E).
The concerned osteoderms cannot be con
fi
dently identi
fi
ed at
genus or species level because their characteristics are widely
distributed in several clades. However, they are likely to document
a single small and unknown taxon within the Glyptodontinae
(smaller than the oldest glyptodontine genus known so far,
Bor-
eostemma
from Laventan SALMA), because of the combination of
the following characters: (i) osteoderms
fl
at or smoothly convex,
(ii) surface punctuated, (iii) principal
fi
gure completely surrounded
by peripheral
fi
gures, and (iv) quadrangular
ª
U
º
-shaped cross
section of the sulci. The latter feature has been suggested as
a noncranial character that differentiates Glyptodontinae from
Propalaehoplophorinae within Glyptodontidae (
Carlini et al., 2008
).
As
a consequence, a reduced size
e
almost twice smaller than the
corresponding osteoderms in
Boreostemma
e
and the presence of
thin osteoderms might represent a plesiomorphic condition for the
Glyptodontinae. On the other hand, the posteriorly displaced
position of the principal
fi
gure, as well as the reduction in size of
posterior, medial, and lateral peripheral
fi
gures, appear as tied to
the location of the osteoderms in the carapace (i.e., submarginal),
instead of representing a plesiomorphic trait (i.e., principal
fi
gure
close to the posterior margin), as seen on glyptatelines and
Para-
propalaehoplophorus
(see
Croft et al., 2007
).
Order RODENTIA Bowdich, 1821
Infraorder HYSTRICOGNATHI Tullberg, 1899
Parvorder CAVIOMORPHA Wood, 1955
Superfamily CAVIOIDEA Fischer de Waldheim, 1817
Family CAVIIDAE Fischer de Waldheim, 1817
Guiomys
sp.
MUSM 1970 is a very small tooth (
L
¼
2.93;
W
¼
2.61), hyp-
selodont (i.e.,
ª
euhypsodont
º
following
Pérez, 2010
), preserving the
occlusal surface, but the basal most part of which crown is broken
away (
Fig. 3
G
e
H). This tooth is interpreted as a left M1 or M2. It is
bilobed, with lozenge-shaped lobes connected by a thick labial
bridge; the mesial lobe is slightly smaller than the distal one
(
Fig. 3
F). The occlusal surface of both lobes lacks any fossette and
the apex of each lobe is not constricted at the current wear stage.
The hypo
fl
exus is transversely developed (reaching c. 80% of the
transverse width of the crown) and funnel-shaped; cement is
fi
lling
the bottom of the hypo
fl
exus, which is pointing distally and labially.
A shallow furrow faces the tip of the hypo
fl
exus. There is no
transverse dentine crest crossing each lobe (
Fig. 3
F). Enamel is
present all around the crown but interrupted on the labial most
part of each lobe.
The bilobed pattern of this molar is characteristic of cavioid
caviomorph rodents (
Pérez, 2010
;
Croft et al., 2011
). Among Cav-
ioidea, the hypselodont pattern of this tooth impedes its referral to
Asteromys
,
Luantus
,
Chubutomys
, and
Phanomys
(
Pérez, 2010
). The
funnel-shaped hypo
fl
exus points to the clade including
Eocardia
robusta
,
Guiomys unica
, and crown cavioids (
Pérez, 2010
). The
absence of transverse dentine crest on each lobe discards referring
this tooth as to
Prodolichotis pridiana
or
Orthomyctera chapadma-
lense
, while the funnel-shaped hypo
fl
exus further distinguishes
MUSM 1970 from
P. pridiana
(
Walton, 1997
;
Pérez, 2010
). The
presence of a single labial furrow makes it distinct from upper
molars of
E
.
robusta
. To sum up, the morphology of this specimen
points to a stem cavioid and, together with its small size, it is only
consistent with
Guiomys
Pérez, 2010
, the smallest and earliest
caviid known so far, from the middle Miocene of Patagonia (?Col-
loncuran and Laventan SALMAs;
Pérez, 2010
;
Pérez and Vucetich,
20
11
) and the Laventan of Quebrada Honda, Bolivia (
Croft et al.,
2011
). This left molar is provisionally referred to as
Guiomys
sp.,
as it is 15
e
20% smaller than the teeth of the type and only species of
the latter genus (
Pérez, 2010
;
Croft et al., 2011
).
Superfamily CHINCHILLOIDEA Kraglievich, 1940
Family DINOMYIDAE Peters, 1873
Subfamily POTAMARCHINAE Kraglievich, 1926
ª
Scleromys
º
sp., gr. quadrangulatus-schurmanni-colombianus
MUSM 1971 is a left d4. It is low-crowned and elongate mesio-
distally, with a trapezoid occlusal outline, widening distally
(MDL
¼
5.04;
W
¼
2.81;
H
¼
3.10; HI
¼
0.62). It has an
ª
F-
G
-I-I
º
lophid
pattern, with distinctive features such as taeniodonty (see
Antoine
et al., 2012
), elongate cristids connected distolingually to the ante-
rolophid and the metalophid, a circular supernumerary cuspid
mediodistal to the anterolophid, and a short transverse supernu-
merary lingual lophid distal to the metalophid (
Fig. 3
I). The hypo-
lophid and the posterolophid are straight, oblique, distinct, and
parallel one to another. The hypolophid displays a small mesiolabial
spur. The enamel band is crenulated on the mesial side of the
posterolophid. Such crenulations occur frequently in potamarchine
teeth (especially in
Potamarchus murinus
;
Sant
Anna Filho, 1994
).
This tooth is twice smaller than d4s of
ª
Olenopsis
º
/Drytomomys
from
the Middle Miocene of La Venta (Colombia;
Fields,1957
: 330, Fig.18;
Candela and Nasif, 2006
) and of Fitzcarrald (Perú;
Antoine et al.,
2007
). In addition, MUSM 1971 is quite distinct from the d4 of
P
.
murinus
from the middle to late Miocene of the Upper Juruá, Brazil
(AMNH58535;
Sant
Anna Filho,1994
), in having a trapezoid occlusal
outline and in being tetralophodont, instead of being quadrangular
and pentalophodont, respectively. MUSM 1971 is tetralophodont,
half the size of, and much less hypsodont (HI
¼
0.62) than the
pentalophodont p4s referred to
Simplimus indivisus
(MLP 15-244a:
HI
w
2.92; Laguna Blanca/Río Fénix, Friasian SALMA, Patagonia;
Vucetich, 1984
) and to
Simplimus
sp. (UFAC DGM 533M: HI
w
2.88;
Upper Juruá, middle-late Miocene, Brazil;
Sant
Anna Filho,1994
). On
the other hand, its size and proportions recall those of d4s of
ª
S
.
º
schurmanni
from La Venta, Colombia, as illustrated by
Fields (1957:
285, Fig. 5)
. The pattern is quite similar, especially for the distal
lophids. Yet, the occlusal pattern of mesial lophids and cuspids
observed in MUSM 1971 prevents from referring it to
ª
S
.
º
schur-
manni
. Teeth of
ª
S.
º
colombianus
(La Venta;
Fields, 1957
;
Walton,
1997
) are ca. 20% larger than both
ª
S.
º
schurmanni
and MUSM 1971.
MUSM 1972 is a left lower molariform and hypsodont tooth,
with a quadrangulate occlusal contour and a straight anterior
border (
Fig. 3
J). It is high, elongate mesiodistally and at an early
stage of wear (MDL
¼
4.14;
W
¼
3.72;
H
¼
8.4; HI
¼
2.03). The
mesiodistal and labiolingual lengths of the tooth diminish and
increase strongly with wear, respectively, which allows interpret-
ing it as an m1 at
ª
stage of wear n
!
2
º
, by comparison with serial
sections of molariform teeth of
ª
S
.
º
colombianus
as proposed by
Fields (1957: 318
e
319, Fig. 14)
. Roots are still developed and the
neck is well-marked (
Fig. 3
K). This tooth is tetralophodont and
taeniodont, with oblique and large lophids. The short metalophulid
I and the longer metalophulid II are connected at both lingual and
labial ends. The hypolophid and the posterolophid (damaged in its
distolingual part) are not connected lingually at the current stage of
wear, but they would join in later stages. Contrary to other lophids,
the posterolophid is curved and concave mesiolingually in occlusal
view, joining a thick and mesially-displaced hypoconid.
These two lower teeth have a typical dinomyid occlusal pattern
(i.e., high-crowned, tetralophodont, taeniodont, with oblique
lophids, and a posterolophid isolated before wear). By their
dimensionsand pattern,theyare provisionallythought to document
a single taxon.
Scleromys
Ameghino, 1887 is the earliest represen-
tative of Dinomyidae (
Horovitz et al., 2006
). The high crown,
mesiodistal elongation, quadrangular contour, large and persistent
fossettids, and straight aspect of the mesial border of MUSM 1972
discard any referral to the typical Santacrucian species of
Scleromys
,
i.e., the type species
Scleromys angustus
Ameghino, 1887 and
Scle-
romys osbornianus
Ameghino 1894 (Argentinian Patagonia). The
present specimen seems to be somewhat closer to
S. quadrangulatus
(pre-Santacrucian
ª
Pinturan
º
age, Patagonia, Argentina;
Kramarz,
2006
) and to
Scleromys
sp. (Mariño Formation, ?early Santa-
crucian, Mendoza, Argentina;
Cerdeño and Vucetich, 2007
) in
sharing both a small size and a quadrangular contour. MUSM 1972
further resembles
S. quadrangulatus
in having a straight mesial
border, and a mesiodistal elongation. However, the lower molars
referred to
S. quadrangulatus
are lower-crowned than MUSM 1972
and they lack persistent fossettids. The latter feature is so far only
observedin
S
.sp.fromtheMariñoFormation(
CerdeñoandVucetich,
2007
),
ª
S
.
º
schurmanni
Stehlin, 1940 and
ª
S.
º
colombianus
Fields,
1957
, from the Laventan of Colombia and Peru (
Fields, 1957
;
Walton, 1997
;
Antoine et al., 2007
). Similarly, in the Patagonian
species of
Scleromys
, the metalophulid II is typically reduced, being
shorter than the metalophulid I. In that aspect, MUSM 1972 seems to
be closer to the Laventan species from Colombia in having a larger
metalophulid II. Nevertheless, in the latter taxa (the generic
assignment of which is challenged by most authors; e.g.,
Patterson
and Wood, 1982
;
Walton, 1997
), teeth are noticeably larger,
higher-crowned and wider labiolingually than in MD-67. Regardless
of thelingualhypolophid
e
posterolophidjunction (notyetoccurring
in MUSM 1972), the MD-67 specimen matches an m3 referred to
ª
Scleromys
cf.
S. schurmanni
º
from the Laventan Fitzcarrald local
fauna of Peruvian Amazonia (MUSM 1566;
Antoine et al., 2007
;
Negri et al., 2010
), being only narrower labiolingually and lower-
crowned. In addition, this lower molar has similar proportions and
lophid pattern as an m2 from the middle to late Miocene of the
Upper Juruá, Brazil (UFAC DGM 582M;
Sant
Anna Filho, 1994
)
referred to
ª
S
.
º
colombianus
, by reference to specimens from La
Venta, Colombia. However, the tooth from MD-67 is distinctly
smaller, lower-crowned, and less prismatic.
To sum up, the dental pattern and the occlusal contour of MUSM
1972 match those of several species referred to
Scleromys sensu lato
,
either of pre-Santacrucian (
S. quadrangulatus
) or of Laventan ages
(
ª
S.
º
colombianus
and
ª
S.
º
schurmanni
;
Fields, 1957
). These taxa are
likely to form a
ª
lineage
º
distinctive from the typical Santacrucian
Scleromys
cluster, as hypothesised by
Kramarz (2006: 59)
. Following
that scheme, the crown height, proportions, and fossettid develop-
ment of MUSM 1972 shall coincide with a
ª
transitional evolutionary
stage
º
between
S
.
quadrangulatus
from the early Miocene of
Argentina and the representatives of
ª
Scleromys
º
from the late
middle Miocene of Northern South America (
Fields,1957
;
Sant
Anna
Filho, 1994
;
Walton, 1997
;
Kramarz, 2006
;
Antoine et al., 2007
;
Cerdeño and Vucetich, 2007
). As such, these specimens, provision-
ally referred to as
ª
Scleromys
º
sp., may document a
ª
Friasian
º
to
Colloncuran morphological grade for potamarchine dinomyids.
Superfamily OCTODONTOIDEA Waterhouse, 1839
Family ACAREMYIDAE Ameghino, 1902
Genus and species indet.
MUSM 1973 is a diminutive lower molar (MDL
¼
1.72;
W
¼
2.10),
roughly square in occlusal view, and with a rather high crown
(
ª
mesodont
º
sensu
Vucetich and Kramarz, 2003
). It is interpreted as
a left m1 or m2. This tooth has a tetralophodont pattern, with bulky
lophids and no cuspid well individualised (
Fig. 3
L). Enamel is thick,
especially on the labial half of the molar. In occlusal view, the mesial
margin is straight and the distal one convex. The lophids are thick,
transversely oriented, and separate by deep and wide
fl
exids. The
hypo
fl
exid is deep (it almost reaches the lingual half of the tooth),
nearly transverse, and
ª
U-shaped
º
in occlusal view. The talonid is
narrower than the
ª
trigonid
º
, due to the weak lingual development
of the posterolophid, thus providing a trapezoid shape to the
occlusal contour of the tooth. The metalophulid I is complete and
straight, with a thick mesiolabial projection, pointing linguodistally
and joining the metalophulid II. The metalophulid II is long, and it
also joins the metalophulid I at the lingual margin of the tooth,
determining a mesial fossettid, oval and elongate transversely
(closed antero
fl
exid). The junction between both metalophulids is
somewhat constricted lingually, mesial to the mesostylid. The
ectolophid is distinct and oblique. The hypolophid is transverse,
and it connects lingually a smoothly constricted entoconid. The
meso
fl
exid is open lingually until a late stage of wear. The meta-
fl
exid is also open lingually, and it would not get closed even with
heavy wear. The posterolophid is curved, with a strong hypoconid
and a short lingual arm (getting longer with wear).
Both the tetralophodont pattern and small size of MUSM 1973
allow attributing it to an early diverging octodontoid. The absence of
an eight-shaped-pattern due to the lingual opening of the meta
fl
exid
discards referring this tooth to the Octodontidae (
Vucetich and
Kr
amarz, 2003
). Among Echimyidae, the transverse orientation of
the lophids impedes any referral to Adelphomyinae, while tetralo-
phodonty distinguishes it from Echimyinae (
Vucetich et al., 1993
;
Kramarz, 2001
). MUSM 1973 resembles
Protacaremys
(Colhuehua-
pian-Colloncuran SALMAs of Patagonia and Chile;
Flynn et al., 2008
)
in having deep, transversely elongate and persistent fossettids/
fl
ex-
ids (notably the antero-fossettid/-
fl
exid), but differs from it in the
absence of pinched and cuspidate lophids, in the U-shaped, trans-
versely oriented and smooth hypo
fl
exid, in the complete and early
lingual junction between the metalophulids I and II (anterolophid
and mesolophid
sensu
Vucetich and Kramarz, 2003
), and in lacking
a
fi
gure-eight occlusal pattern (
Kramarz, 2001
).
On the other hand, the dental pattern of MUSM 1973 is strongly
reminiscent of Acaremyidae (
Acaremys
,
Sciamys
, and
Galileomys
;
Vucetich and Kramarz, 2003
). It differs from the m1s and m2s of
Galileomys
in a marked mesodonty, the presence of transverse
lophids,
fl
exids, and fossettids, a stronger transverse development
of the U-shaped hypo
fl
exid, and in the lingual connection between
the two mesial lophids (
Vucetich and Kramarz, 2003
;
Kramarz,
2004
). It resembles more
Sciamys
and
Acaremys
. Nevertheless, it
can be distinguished from
Sciamys
, as illustrated by
Arnal and
Vucetich (2011)
, by the quadrangular occlusal contour (more elon-
gate mesiodistally in
Sciamys
), by a shorter labial arm of the post-
erolophid, and by smaller dimensions. It differs from known species
of
Acaremys
in having a mesolophid reaching the lingual wall and
determining a transversely elongate anterofossettid persistent until
late stages of wear, two features which are only observed in
Sciamys
among acaremyids (
Vucetich and Kramarz, 2003
). It further differs
from
Acaremys
in having a much smaller metaconid, a narrower and
transversally longer meso
fl
exid, a less penetrating hypo
fl
exid, and
a posterolophid narrower mesiodistally. As a result, MUSM 1973 is
likely to document a late representative of Acaremyidae with closer
af
fi
nities to
Sciamys
and
Acaremys
than to
Galileomys
, provisionally
identi
fi
ed as
ª
Acaremyidae indet
º
.
Superfamily ERETHIZONTOIDEA Thomas, 1897
Family ERETHIZONTIDAE Thomas, 1897
cf.
Microsteiromys
sp.
Two upper molariform teeth are assigned to a small
erethizontid.
MUSM 1974 is a left P4 with a circular occlusal outline
(
L
¼
2.14;
W
¼
2.20). It is preserved at a very early stage of wear
(just erupted). Accordingly, there is no wear facet due to the
contact with a mesial or a distal tooth (
Fig. 3
M). The crown is
much higher lingually than labially. The tooth was biradiculate,
with lingual and labial roots mesiodistally elongate. The occlusal
pattern is restricted to the apical-most part of the crown, with
distinct cusps. The tooth is tetralophodont, with a thin but
complete anteroloph, curved distolingually, with a prominent
protocone. The para
fl
exus is triangular in occlusal view, and open
both lingually and labially at the current stage of wear. The pro-
toloph is oblique, short lingually, and independent from adjacent
lophs at both ends; the lingual protoloph is a low and constricted
crest. The paracone is distinct and bulky. The hypo
fl
exus is deep
and wide (i.e., there is no endoloph). The lingual cusps, still
distinct at the current stage of wear, would be coalescent after
a smooth wear. The meso
fl
exus is open lingually and medially;
the mure is low and constricted, interrupted at the current stage
of wear. The third loph is very short, restricted to the centro-
distal part of the crown, and interpreted as a mesolophule; it is
connected lingually to the anterior arm of the hypocone and
labially, to the mesoloph. The posteroloph is thin, with a hypo-
cone and a metacone distinct and bulky. It extends mesiolabially
to the metacone until a faint cusp, interpreted as a mesostyle and
facing the paracone. The postero
fl
exus, still open mesiolabially,
would be quadrate at later stages of wear.
A right pentalophodont molar (MUSM 1975;
L
¼
2.44 mm;
W
¼
2.11 mm) has three broken roots, with two labial roots
(circular cross section) and a mesiodistally elongate lingual one,
which point to an upper molar (
Fig. 3
N). A contact facet is visible
on the mesial side of the crown, but not on the distal side. Given
the stage of occlusal wear, it allows identifying this tooth as
a probable M3, even if the tooth is only slightly tapering distally (as
in M2s) and if the hypocone is also located as in an M2, i.e.,
lingually displaced with respect to what is generally observed in
M3s. The occlusal pattern is longer than wide, with a
ª
EUJ
º
-shaped
occlusal design. All the lophs are moderately worn, with slight
constrictions, and a low obliquity. The anteroloph is the most
developed loph, and it connects a labiolingually compressed and
oblique paracone. The para
fl
exus is oval, elongate transversely,
open labially but closed lingually by a low and constricted lingual
protoloph. The protoloph is straight, slightly oblique, and it
connects a strong paracone, labially. It joins the mesolophule
lingually, through a strong but very short mure, oriented sagittally.
The mesostyle and the paracone are remote and the meso
fl
exus is
wide and U-shaped in occlusal view (open labially). The meso-
lophule is transversely oriented and S-shaped, with a labiodistally-
oriented mesostyle. The meta
fl
exus is wide, comma-shaped, still
labially open at this stage of wear, and closed lingually by a labio-
lingually compressed hypocone and its strong anterior arm. The
posteroloph is short, but it extends mesiolabially until the meta-
cone, thus forming a distolabial wall. The posteroloph is somewhat
constricted labially to the hypocone and lingually to the metaloph.
The latter is short, oriented mesiolabially, connected to the mid-
posteroloph and disconnected to both the distolabial wall and
the metacone, thus forming a small posterofossette joined labially
to the meta
fl
exus.
The pentalophodont pattern of the upper molar, the low loph-
obliquity, and the circular occlusal outline of the P4, as well as the
low crown and thick enamel of both teeth, point to erethizontids.
Given their compatible size and pattern, both teeth are assumed to
document a single diminutive taxon. The fossil record of Erethi-
zontidae ranges from the Late Oligocene up to Recent times
(
Vucetich et al., 1999
;
Candela and Morrone, 2003
). Accordingly
and whenever possible, these teeth were compared to those of
Protosteiromys
(Deseadan, Patagonia;
Wood and Patterson, 1959
),
of
Eosteiromys
Ameghino, 1902,
Hypsosteiromys
Patterson, 1958
,
Parasteiromys
Ameghino, 1903, and
Branisamyopsis
Candela, 2003
(Colhuehuapian, Argentina;
Patterson, 1958
;
Candela, 1999
,
2003
;
Dozo et al., 2004
;
Kramarz, 2004
;
Kramarz and Bellosi,
2005
;
Vucetich et al., 2010
), of
Steiromys
Ameghino, 1887 (Santa-
crucian-?Laventan; Patagonia, ?Colombia;
Fields, 1957
;
Walton,
1997
;
Candela, 1999
), of
Neosteiromys
Rovereto, 1914 (?Collon-
curan-Huayquerian; Northwestern Argentina;
Candela, 1999
,
2004
), of
Microsteiromys
Walton, 1997
(Laventan; Colombia;
Walton, 1997
), and of
Erethizon
Cuvier, 1823 (Recent;
Candela,
1999
).
The teeth from MD-67 are half the size of than those of all
known Recent and fossil Erethizontidae but
Microsteiromys jacobsi
Walton, 1997
, of compatible size (
Walton, 1997
). No P4 is described
from any Deseadan erethizontid. The P4 from MD-67 differs from
all known Recent and fossil Erethizontidae but
Eosteiromys
homogenidens
Ameghino, 1902, in having a labially-displaced
hypocone. A circular occlusal outline is only observed in
E. homogenidens
(holotype MACN A-52-165) and ?
Steiromys
from La
Venta (
Walton, 1997
). Tetralophodonty and low loph obliquity also
characterises the P4 of
Eosteiromys
, ?
Steiromys
, and
Steiromys
detentus
Ameghino, 1887 (MLP 15
e
17). MUSM 1974 further differs
from the dP4 of
Parasteiromys uniformis
(Ameghino,1903) in having
a marked mure, and in bearing
fl
exi labiolingually compressed
(
Candela, 1999
). Its para
fl
exus, which is closed labially, makes it
distinct from the P4 of
Branisamyopsis praesigmoides
Kramarz, 2004
and
S
.
detentus
(
Kramarz, 2004
: 14, Fig. 7). It also differs from the P4
of
Neosteiromys bombifrons
Rovereto,1914 in having no lingual wall
(
Candela, 2004
: 61, Fig. 3).
The upper molar from MD-67 differs from all known erethi-
zontids in its labially-interrupted metaloph and in its mesiodistal
elongation (e.g.,
Candela, 1999
,
2004
;
Vucetich et al., 2010
). Its size
is also very distinctive, as it is twice smaller than in all known
taxa, except
M
.
jacobsi
, of similar dimensions (
Walton, 1997
). The
pentalophodont pattern makes it distinct from
Protosteiromys
medianus
,
Hypsosteiromys axiculus
, and
Steiromys
(
Patterson, 1958
;
Wood and Patterson, 1959
;
Candela, 1999
;
Dozo et al., 2004
). The
presence of a mure and the late labial closure of the para
fl
exus
discard any referral to
Parasteiromys
or
Neosteiromys
(
Candela,
1999
).
The presence of a distal constriction labially to the hypocone and
lingually to the metaloph is only observed in
Parasteiromys friantae
Candela, 1999
(but not in
P. uniformis
;
Candela, 1999
: Fig. 2),
E
.
homogenidens
(type, MACN A-52
e
165) and
E
. cf.
homogenidens
(
Kramarz, 2004
). However, all these taxa are characterised by
lower-crowned teeth, a much larger size, and a complete metaloph,
i.e., reaching the labial side of the tooth.
To sum up, the pattern and morphological features of the P4 and
of the upper molar from MD-67 show certain af
fi
nities with
E
.
homogenidens
(Colhuehuapian), and
Steiromys
(Santacrucian-?
Laventan) to a lesser extent, while size is only compatible with
Microsteiromys
(
Walton, 1997
).
Microsteiromys
Walton, 1997
is the
smallest known representative of New World porcupines, with
a geographic and stratigraphic range thus far restricted to the
Baraya Member of the Villavieja Fm. of Colombia (c. 13
e
12.5 Ma,
middle Laventan;
Madden et al., 1997
;
Candela and Morrone,
2003
). This diminutive monotypic genus is only known by two
mandibles, which makes it impossible to compare with the avail-
able teeth from MD-67 (
Walton, 1997
). However, we assume that
these teeth are likely to document a close ally of
Microsteiromys
Walton, 1997
, here referred to as cf.
Microsteiromys
sp. Given their
morphological af
fi
nities with taxa spanning the early and middle
Miocene interval, these specimens cannot be used with much
con
fi
dence in a biochronological perspective.
4. Discussion
4.1. Biochronological age
Glyptodontid xenarthrans are of poor biochronological interest,
especially when identi
fi
ed above genus level. Caviomorph rodents
are the most diverse group in MD-67, with four taxa encompassing
four superfamilies (Octodontoidea, Erethizontoidea, Cavioidea, and
Chinchilloidea;
Vucetich et al.,1999
). Caviidae have their FAD in the
lat
est (or post-) Colloncuran of Patagonia, with
Guiomys
(
Pérez,
2010
;
Pérez and Vucetich, 2011
), a genus which is recognised at
MD-67 (
Fig. 3
F
e
H;
Table 1
). Acaremyidae had a Colhuehuapian-
Colloncuran stratigraphical range (
Vucetich and Kramarz, 2003
)
while the hathliacynid marsupial
Sipalocyon
had only an early
Miocene record so far (Colhuehuapian-Santacrucian;
Marshall,
1981
). As such, MD-67 might extend upward the known range of
both taxa, and thus represent their Last Local Occurrence (
Table 1
).
On the other hand, the recognition of
Marmosa
(
Micoureus
) and of
a
Microsteiromys
-like dwarf porcupine in MD-67 predates the
previous FAD of both taxa, formerly restricted to the Laventan
Table 1
Stratigraphic range of the middle Miocene vertebrate locality MD-67 as inferred by
mammalian biochronology and
fi
ssion track datings (see
Supplementary Data
). Data
from
Walton (1997)
,
Vucetich et al. (1993
,
2010
),
Vucetich and Kramarz (2003)
,
Kramarz (2004
,
2006)
,
Gradstein et al. (2005)
,
Kramarz and Bellosi (2005)
,
Cerdeño
and Vucetich (2007)
,
Croft et al. (2011)
, and
Pérez and Vucetich (2011)
.
SALMA in the La Venta area of Colombia (
Table 1
;
Marshall, 1976
;
Goin, 1997
;
Madden et al., 1997
;
Walton, 1997
).
At
fi
rst sight, the biochronological age for MD-67 is middle
Miocene, i.e., Colloncuran-Laventan (
w
15.6
e
11.6 Ma;
Kay et al.,
1997
;
Madden et al., 1997
), but the occurrence of a typical early
Miocene genus such as
Sipalocyon
and the potentially
ª
plesiomor-
phic evolutionary stage
º
of
ª
Scleromys
º
with respect to its Laventan
counterparts (
Walton, 1997
) would tend to favour a Colloncuran-
early Laventan age for this new locality (
w
15.6
e
13.0 Ma;
Table 1
).
4.2. Apatite
fi
ssion track age of MD-67: 17.1
2.4 Ma
A
fi
ssion track age was calculated on 11 apatite grains. The
corresponding results are detailed in the
Supplementary Data
. The
c
2
test (
Galbraith, 1981
;
Green, 1981
) is currently used to discrim-
inate between concordant (
P
(
c
2
)
>
5%) and discordant (
P
(
c
2
)
<
5%)
grain-age distributions. The MD 67 sample passes the
c
2
test
(
P
(
c
2
)
>
5%) indicating that the apatite grains display a concordant
population and that they are derived from homogeneous sources
(
Galbraith, 1981
;
Green, 1981
).
The central age (17.1
2.4 Ma), pointing to a Burdigalian
e
Langhian age for the concerned grains (
Table 1
), is only partly in
agreement with the faunal content of MD-67, interpreted as doc-
umenting a Colloncuran-early Laventan age (
w
15.6
e
13.0 Ma;
Table 1
).
In other words, Apatite Fission Track provides a detrital age
(17.1
2.4 Ma) for the vertebrate-yielding locality, slightly older
than its inferred biochronological age (Colloncuran-early Laventan
South American Land Mammal Ages:
w
15.6
e
13.0 Ma). Be as it may,
the middle Miocene age of the concerned outcrop is fully contra-
dictory to its original assignment to the Paleocene-Eocene
Yahuarango Formation (
Vargas and Hipólito, 1998
).
4.3. Paleoenvironment
At regional scale, the concerned area mostly yielded terrestrial
habitats of low elevation, with a moist forest assumed as resem-
bling the modern Amazonian rainforest, in terms of composition
and biodiversity (
Hoorn, 1993
;
Antoine et al., 2006
;
Pons and De
Franceschi, 2007
;
Hoorn et al., 2010a
,
b
).
Unfortunately, MD-67 yields no pollen, spores, or plant fossils.
Available proxies (dental morphology and habitat preferences of
living and fossil mammal analogues; depositional environment)
thus provide only indirect information on the environment of the
concerned area by the time fossil mammals accumulated.
Most rodents from the current assemblage, including a meso-
dont acaremyid, a hypsodont dinomyid (
ª
Scleromys
º
sp.), and
a hypselodont caviid (
Guiomys
sp.), can be interpreted as an indi-
cator of open and dusty environments under a quite dry and windy
climate (
Candela and Vucetich, 2002
). Yet, the dwarf
Micro-
steiromys
-like erethizontid of MD-67 was most probably fully
arboreal, like all living New World porcupines and their fossil kin,
as proposed by
Candela and Picasso (2008)
. Accordingly, all living
marmosine marsupials, such as the representatives of the subgenus
Marmosa
(
Micoureus
) are forest dwellers, being either arboreal or
ground foragers, in moist habitats related to tropical evergreen or
mossy forests (
Emmons and Feer, 1997
).
The appendicular skeleton of
Sipalocyon
is poorly known, but
functional anatomy suggests arboreal and potential grasping
capabilities for this carnivorous marsupial (
Argot, 2003
,
2004
). The
Santa Cruz Beds of Patagonia, which yield most remains of
Sipalo-
cyon
, are interpreted as originating from a temperate coastal plain
(
Bown and Fleagle, 1993
), with moderate rainfall and a mixture of
forested habitats/open areas/bushland as suggested by mammals,
pollen, and terrestrial arthropods (
Vizcaíno et al., 2010
).
Lithology of the fossil-bearing beds (i.e., channel-iron deposits,
with Fe-rich pisolite gravels) provides valuable information on the
depositional environment and associated diagenetic processes:
pisolites might have formed in the ground by alteration and
concretion of highly ferruginous groundwater solutions under warm,
humid, and seasonally-contrasted conditions (
Tardy, 1992
). Accord-
in
gly, isotopic analyses performed on coeval mollusc shells from the
Iquitos area (
w
1000 km more to the North) show the region was
experiencing a seasonal water in
fl
ux under a monsoonal-like tropical
climate by that time (
Kaandorp et al., 2006
;
Wesselingh et al., 2006
).
Both proxies are therefore in good agreement.
One of the striking features of the Miocene of Amazonia is the
presence of a large and long-lasting
ª
mega-wetland
º
. The Amazo-
nian mega-wetland reached its maximum extent during the Middle
Miocene (also called
ª
Pebas phase
º
sensu
Hoorn et al., 2010a
,
b
) and
it consisted of a complex mosaic of lakes, embayments, swamps,
rivers, and
fl
uvio-tidal environments (see review in
Hoorn et al.,
2010a
,
b
). Our data suggest the absence of this megawetland in
the Amazonian Madre de Dios Subandean Zone of Perú (
Fig. 4
),
while other coeval localities such as IQ-26 and NA069 (nearby
Iquitos;
Antoine et al., 2006
;
Pujos et al., 2009
) or the Fitzcarrald
Local Fauna (
Antoine et al., 2007
;
Goillot et al., 2011
) were under its
in
fl
uence during the same period (
Fig. 4
). This environmental
contrast might in turn have played some role in the faunal
discrepancies as observed in middle Miocene times between
Northern and Southern South America (
Madden et al., 1997
).
4.4. Biogeography
The earliest undisputable representatives of Glyptodontinae,
referred to
Boreostemma
, originate from middle Miocene Laventan
localities of La Venta and Fitzcarrald (Colombia and Perú, respec-
tively; e.g.,
Antoine et al., 2007
). In southern South America, the
earliest record occurs much later, with
Glyptodontidium tuberifer
from the late Miocene-Pliocene of NW Argentina (e.g.,
Oliva et al.,
2010
), which is most probably tied to environmental reasons
(
Carlini et al., 2008
). If con
fi
rmed, the referral of the osteoderms of
MD-67 to Glyptodontinae would still extend the gap between the
fi
rst local occurrences of the group in low and high latitudes.
The cavioid rodent
Guiomys
Pérez, 2010
was so far restricted to
the middle Miocene of Patagonia and Southern Bolivia, with a ?
Colloncuran (
w
14 Ma; Patagonia)-Laventan (Patagonia
þ
Southern
Bolivia) stratigraphic range (
Fig. 4
;
Pérez, 2010
;
Croft et al., 2011
;
Pérez and Vucetich, 2011
). Accordingly,
Sipalocyon
was so far
restricted to high Southern latitudes, from Patagonia to Southern
Chile (51.5
e
37.5
!
S;
Marshall, 1981
;
Forasiepi et al., 2006
;
Flynn
et al., 2008
). The co-occurrence of this stem caviid and of
Sipalo-
cyon
(37.5
e
48
!
S) in Peruvian Amazonia extends the geographical
range of
w
10
!
and
w
25
!
more to the North, respectively (
Flynn
et al., 2008
;
Croft et al., 2011
). On the other hand, the small mar-
mosine
M
. (
Mi
.)
laventica
and the diminutive erethizontid
Micro-
steiromys
were only known in the Huila Department of Colombia
during a very short Laventan interval (
Fig. 4
;
Goin, 1997
;
Walton,
1997
), i.e., later and
w
15
!
more to the North than in MD-67.
In other words, the MD-67 assemblage both (i) postdates the
formerly known range of taxa of mid- and high latitude af
fi
nities
(
Sipalocyon
; Acaremyidae) and (ii) predates that of taxa of low latitude
af
fi
nities (
Marmosa
(
Micoureus
);
Microsteiromys
; Glyptodontinae).
This phenomenon is summarised by the spatiotemporal range of the
small dinomyid recognised in MD-67 and its kin, if close phylogene
tic
af
fi
nities are con
fi
rmed between the representatives of
Scleromys
sensu stricto (early Miocene of Patagonia and Southern Chile;
Flynn
et al., 2008
) and those of
ª
Scleromys
º
sensu
Walton, 1997
(late
middle Miocene of Colombia and Peru;
Walton, 1997
;
Antoine et al.,
2007
). Such assertion may be an artefact tied to the scarce fossil