The Abo Formation consists of fluvial
redbed mudstones and
sandstones, including river channel deposits in its lower beds (Scholle Member) and distinctive sandstone sheets in its upper beds (Cañon de Espinoso Member.) Its depositional environment was typical of the "wet red beds" of tropical
Pangaea. It is extensively exposed in the mountains and other uplifts bordering the
Rio Grande Rift, with a thickness of at the type section. It is also present in the subsurface in the
Raton Basin. The base of the Abo is gradational with the
Madera Group, and is usually placed at the first massive marine limestone bed below the fluvial sediments of the Abo. It is overlain by the
Yeso Formation, with the base of the Yeso placed at the first massive sandstone bed showing frosted grains and other
eolian features. The transition zone between the Madera Group and the Abo Formation is distinctive enough in many locations that it is broken out into its own formation, the
Bursum Formation. Sandstone in the exposures towards the north, at Abo Pass and in the Jemez Mountains, tends to be
arkosic, with detrital
feldspars dominated by potassium feldspar including
microcline. The feldspar is locally
albitized, possibly by brines in
evaporite basins or due to high heat flow in the crust.
Granitic rock fragments are much more common than
metamorphic. Cementing is usually by
calcite, but
quartz cementing is often present.
Carbonate grains are likely reworked
caliche. The formation fines to the south. The composition and southward fining indicate a granitic source to the north. The Abo Formation was deposited in a time of rapid global warming. Carbon and oxygen isotope ratios in
caliches within the formation indicate a rise in temperature from 15-30 °C during the eighteen million years in which the formation was deposited. This was accompanied by increased aridity. Deposition took place on a low-gradient, broad, well-oxidized alluvial plain in which rivers flowed to the Hueco seaway in southern New Mexico. There are indications in the strata of strong seasonality typical of the megamonsoonal climate of early Permian Pangaea. The Abo transitions seamlessly to the
Cutler Formation in the northern
Jemez Mountains. With both names deeply entrenched in the geological literature, the convention is to use the name "Cutler Formation" north of 36 degrees north latitude and "Abo Formation" south of that latitude. Paleontological data and regional correlations suggest that the age of the Abo Formation is middle
Wolfcampian to early
Leonardian.
Members The Abo Formation is divided into the lower Scholle Member and the upper Cañon de Espinoso Member. The
Scholle Member is dominated by mudstone (87% of the type section), with some trough-crossbedded, coarse-grained, conglomeratic sandstones (11% of the type section) interpreted as channel deposits. The remaining 2% is calcrete ledges. The member is thick at the type section and is a slope-forming member. It reflect relatively rapid tectonic subsidence. The
Cañon de Espinoso Member is thick at the type section, of which 70% is mudstone, 21% is thin ledges of laminated climbing-rippled sandstone, and 9% is siltstone beds. The sandstones form distinctive sheet-like bodies. This member was deposited as tectonic subsidence slowed, with an episodically stable base level. ==Fossils==