What is it about?

Brazil's Santos Basin today is one of the world's most prolific with super-giant reserves but in 2005, it was still considered a minor gas-prone province. The analysis we presented as a poster at AAPG-ACE in Calgary laid out evidence for an oil-prone pre-salt source that must have charged every pre-salt structure from basin center across the Santos Outer Basin High. Eighteen months later, the first of eleven consecutive giant pre-salt discoveries was announced, more than validating our reasoning as presented in this look-back case study.

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Why is it important?

As combined in multi-disciplinary studies, weak indicators from varied, scant but validated individual samples can provide powerful geologic insights. Although Brazil's Santos Basin was, in 2005, considered a gas-prone disappointment, the authors' interpretation then saw potential for large volumes of liquid hydrocarbons sourced from a lacustrine Guaratiba interval of Aptian age and trapped below a regional salt layer; subsequently dramatically verified by super-giant discoveries from late 2006. The lesson? Joint efforts across disciplines provide insights from scattered measurements that even the most complete single data sets cannot offer.

Perspectives

This paper represents joint efforts by three key consultancies plus inputs from others. Our concepts, as they were refined and our data sets developed from 1998 - 2005, spurred us to continue building studies by cross-fertilizing our efforts. Looking back nearly 15 years since the poster abstract was submitted, we can see what was missed because of data gaps and inadequate understanding of crustal processes. However, the key insight stands up and we wanted to provide a case history of our petroleum systems detective work.

William Dickson
DIGs (Dickson International Geosciences)

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This page is a summary of: Defining a supergiant petroleum system in Brazil’s Santos Basin with multi-disciplinary methods: one template for exploration success, Interpretation, August 2019, Society of Exploration Geophysicists,
DOI: 10.1190/int-2018-0204.1.
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