Chemical characterization of C <sub>31</sub> sterols from sponges and Neoproterozoic fossil sterane counterparts

L Lubna Shawar (Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology) G Gordon D. Love (Department of Earth and Planetary Sciences, University of California) B Benjamin T. Uveges (Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology) J J. Alex Zumberge (GeoMark Research) P Paco Cárdenas (Pharmacognosy, Department of Medicinal Chemistry, Uppsala University) J José-Luis Giner (Department of Chemistry, State University of New York College of Environmental Science and Forestry) R Roger E. Summons (Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology)

Abstract

Putative metazoan body fossils from the Precambrian are curiously lacking morphological characteristics that link them unambiguously to extant animal phyla, including sponges. Chemical fossils such as the rare C 30 hydrocarbons 24- iso -propylcholestane (24- i pc) and 26-methylstigmastane (26-mes), however, have been proposed as evidence for the Neoproterozoic emergence of the Demospongiae (Porifera) due to their prevalence in rocks of this age and the occurrence of their sterol precursors in contemporary demosponges. However, there are alternative hypotheses which posit that diagenetic alteration products of algal sterols, or those from Rhizaria or other protists, account for the enigmatic steroid distributions observed in these ancient sedimentary rocks. Here, we report additional support for the Neoproterozoic rise of demosponges through the chemical characterization of two previously unrecognized C 31 hydrocarbons—24- n -butylcholestane (24- n bc) and 24- sec -butylcholestane (24- sec bc). Precursor C 31 sterols from contemporary demosponges, as well as a suite of synthesized C 31 sterol standards were reduced to their sterane counterparts. Gas chromatography-tandem mass spectrometry analysis and collisionally activated dissociation mass spectra confirmed the presence of 24- n bc and 24- sec bc in well-preserved early Ediacaran rocks, and the coelution of these compounds with synthetic standards enhances the robustness of these findings. Co-occurrence of abundant 24- i pc and 24- sec bc was found for numerous Neoproterozoic-Cambrian rock/oil samples, closely mimicking the abundance patterns and high structural selectivity of major C 30 and C 31 sterols detected in numerous species of modern demosponges. These findings support the hypothesized first emergence of sponges during the Neoproterozoic Era.

Article Details

Volume / Issue Vol. 122, Issue 41
Published October 14, 2025
ISSN 0027-8424
Publisher National Academy of Sciences

Authors (7)

L

Lubna Shawar

Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology

G

Gordon D. Love

Department of Earth and Planetary Sciences, University of California

B

Benjamin T. Uveges

Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology

J

J. Alex Zumberge

GeoMark Research

P

Paco Cárdenas

Pharmacognosy, Department of Medicinal Chemistry, Uppsala University

J

José-Luis Giner

Department of Chemistry, State University of New York College of Environmental Science and Forestry

R

Roger E. Summons

Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology