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Title: Site U1591
Prior to arrival on site, a decision was made to replace the original primary site (proposed Site CSK-13A) by an alternate site (proposed Site CSK-20A); hence, the latter became Site U1591. This was done to pass through a slightly more complete suite of reflectors in the 800–900 ms two-way traveltime (TWT) interval. Site U1591 is located ~8 km northwest of Christiani Island and ~20 km southwest of Santorini (Figure F1) at 514 meters below sea level (mbsl). It was drilled in three holes (U1591A–U1591C) to a maximum recovery depth of 902.7 meters below seafloor (mbsf) (all depths below seafloor are given using the core depth below seafloor, Method A [CSF-A], scale, except in Operations where the drilling depth below seafloor [DSF] scale is used). Average core recovery was similar in all three holes (U1591A= 66%; U1591B= 43%; U1591C= 58%). The drill site targeted the volcano-sedimentary fill of the Christiana Basin. This basin was believed to have formed by subsidence along an ENE–WSW fault system before the changing tectonic regime activated the current northeast–southwest rift system in which the Christiana-Santorini-Kolumbo (CSK) volcanic field lies (Tsampouraki-Kraounaki and Sakellariou, 2018; Preine et al., 2022a, 2022b). Christiana Basin is deeper than the Anhydros and Anafi Basins; its volcano-sedimentary fill potentially recorded the earlier volcanic history of the CSK volcanic field (including the products of Christiana and early Santorini), as well as younger Santorini and possibly Milos Volcano to the west along the Hellenic volcanic arc. The now-extinct Christiana Volcano produced lavas and tuffs of unknown ages (Aarburg and Frechen, 1999). An ignimbrite found on Christiani Island (one of the two small islands of Christiana Volcano), Santorini, and the nonvolcanic island of Anaphi, called the Christiani Ignimbrite, was identified (Keller et al., 2010). Six seismic units were previously recognized in the Christiana Basin (Preine et al., 2022a, 2022b; Figure F2). Site U1591 was chosen to pass through Seismic Units U1–U6, including volcaniclastics from Santorini and Christiana, and to target the top few meters of the prevolcanic basement below Unit U1. We received permission from the International Ocean Discovery Program (IODP) Environmental Protection and Safety Panel to drill to the Alpine basement at this site in an advanced piston corer/extended core barrel/rotary core barrel (APC/XCB/RCB) drilling strategy involving three holes. The aims of Site U1591 were (1) to better date the volcanic activity of Christiana using biostratigraphic and magnetostratigraphic means and determine whether the CSK volcanic field had Pliocene volcanism similar to the Milos Volcano farther west; (2) to relate the Christiana volcanism to subsidence along the ENE–WSW fault sets and to the activation of the northeast–southwest fault sets; and (3) to seek the submarine equivalent of the Christiani Ignimbrite. By using deeper coring (and seismic profiles) to reconstruct the volcanic, sedimentary, and tectonic histories of the Christiana Volcano, and possibly the Milos Volcano, we aimed to complement the Santorini and Kolumbo volcanic records of Sites U1589 and U1592 and therefore access a near-continuous time series of volcanism of the CSK volcanic field since rift inception. Site U1591 addressed scientific Objectives 1–4 and 6 of the Expedition 398 Scientific Prospectus (Druitt et al., 2022).  more » « less
Award ID(s):
1326927
PAR ID:
10528191
Author(s) / Creator(s):
; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; more » ; ; ; ; ; ; ; ; ; ; ; « less
Publisher / Repository:
International Ocean Discovery Program
Date Published:
Journal Name:
Proceedings of the International Ocean Discovery Program Expedition reports
Volume:
398
Issue:
105
ISSN:
2377-3189
Format(s):
Medium: X
Sponsoring Org:
National Science Foundation
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