PLUTON ROOFS IN ARCS AND EMPLACEMENT MECHANISMS: INSIGHTS FROM THE BLACK PEAK INTRUSIVE COMPLEX, NORTH CASCADES
The BPIC is more heterogeneous near the extensively altered and mineralized roof than elsewhere. Texturally variable diorite, local tonalite, and minor hornblendite are cut by porphyritic diorite and tonalite bodies, at least some of which are coeval with the Stiletto Mtn. phase. Sheets and irregularly shaped porphyritic bodies extensively intrude the roof rocks for distances of up to 500 m upward from the roof contact. In some 100s of m2 areas, intrusive rocks are more abundant than host rocks, which form xenoliths and screens. Xenoliths are generally rare within the BPIC, but are present within 500 m of the roof, ranging from <1 cm to 10s of m wide, and in a much narrower zone next to the wall. Foliation in the roof host rocks is mostly discordant to the pluton contact and in the wall foliation is generally concordant to the contact, and where the clastic rocks are in contact with the pluton, bedding is deflected in a narrow (<100-m wide) aureole.
The absence of syn-emplacement faults in the roof and along the wall, and the discordance of foliation and lack of extension of the roof rocks argue against significant lateral dilation during intrusion. Stoping of the roof was important, and some magma wedging likely occurred, whereas limited ductile flow took place next to the wall. These observations support vertical transport of host rocks, as inferred from a number of other roofs. Many other roof contacts, however, are much sharper and less extensively injected by magmatic sheets.