Phosphorus (P) is the ultimate limiting nutrient for marine photosynthesis (Tyrrell, 1999). Earth historians have thus spent decades trying to reconstruct the evolution of the marine P reservoir. In lieu of multiple stable isotopes, most efforts use the P concentration of marine sediments-or specific sedimentary P phases (Ruttenberg, 1992;Thompson et al., 2019)-to gain insights into P burial during transient perturbations (e.g., OAE's;Handoh & Lenton, 2003;Mort et al., 2007;Kraal et al., 2010) or long-term secular evolution (e.g., Precambrian;Reinhard et al., 2017). A key observation emerging from this work is that Precambrian siliciclastic marine sediments have lower P contents than Phanerozoic equivalents (Reinhard et al., 2017). While this signal clearly represents low P burial, authors disagree as to why. Some contend that the Precambrian marine P reservoir was smaller, due to either P scavenging by Fe minerals in an Fe-rich ocean (