Hi Call, my comments about WDS expanded 3D maybe misguuded. PCL have stated that its all in relation to the full extent of Saturn complex and surrounding area.
I am curious about the deepwater side of PEL87 though.
Does the Saturn ponding, volcanic high, reservoir qualities etc.. prevent sediment forming in a possible a basin floor fan in the western side of PEL87 in water depths of 2000 - 3000m. In other words another Venus?
I'm trying to learn from OldGeo like everyone else!
PCL Price at posting:
2.0¢ Sentiment: Hold Disclosure: Held
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