Lipid Hydrogen Stable Isotope Probing Reveals Decadal-Scale Generation Times for Archaea in Hot Spring Sediments

Quantifying the lipid biosynthesis rate of archaea in hot spring sediments is necessary to interpret the abundance, isotopic patterns, and environmental significance of archaeal lipid biosignatures, with implications for modern biogeochemical cycling and astrobiology. Here, we performed lipid hydrogen stable isotope probing (LH-SIP) experiments on whole sediments collected from two high-temperature, suboxic, circumneutral hot springs in Yellowstone National Park (USA) and El Tatio Geyserfield (Chile). We determined the incorporation of 2H2O into intact polar lipids (IPLs) which provides a taxon- and metabolism-agnostic quantification of biosynthesis under near-natural conditions. We targeted isoprenoid glycerol dialkyl glycerol tetraether lipids (IPL iGDGTs) and recovered structures with 0 to 7 cyclopentyl rings from both springs. We observed minor 2H-uptake into archaeal IPLs in spring sediments in Yellowstone, corresponding to decadal-scale apparent generation times (16 {+/-} 7 years), and no uptake in El Tatio sediments (consistent with minimum generation times of 35 {+/-} 5 years). We infer that net production of sedimentary IPL-iGDGTs is very slow, consistent with a combination of slow archaeal growth, persistence of older IPLs, lipid recycling, and/or contributions from recently sedimented planktonic biomass. These are the first direct, ex situ estimates of archaeal lipid production rates in terrestrial hydrothermal systems using LH-SIP incubations and provide critical constraints for interpreting archaeal lipids in ancient hot spring deposits. This research establishes a framework for assessing activity by slow-growing extremophilic archaea in hydrothermal environments and provides support for targeting hydrothermal deposits on Mars for biosignature detection efforts. Plain Language SummaryHot springs on Earth are important natural laboratories for understanding how signs of life might form and be preserved in hydrothermal environments on early Earth or Mars. In this study, we examine the rate of archaeal lipid biosignature production in sediments from two hot springs in Yellowstone National Park and the El Tatio Geyserfield in Chile. We used a method that measures new microbial production by tracing heavy hydrogen from labeled water as microbes incorporate that hydrogen into newly made lipids in their cell membranes. We found that archaeal lipids in hot spring sediments are produced very slowly, on timescales of decades. This result, along with the chemical stability of lipids and the rapid mineralization rate in hot springs, may allow these molecular biosignatures to be entombed and preserved in hot spring mineral deposits. These results help us better interpret ancient hydrothermal deposits on Earth and support the idea that slowly growing microbial communities could still leave detectable molecular traces in similar environments on Mars and other rocky planets. Key PointsO_LILipid hydrogen stable isotope probing is applied to high temperature hot spring sediments for the first time C_LIO_LIIn hot spring sediments, archaeal lipid production occurs on decadal timescales comparable to some marine sediments, but are much faster than the century- to millennia-scale rates observed in the deep subsurface C_LIO_LIConfirmation of archaeal lipid synthesis in hot spring sediments adds additional support for targeting Martian hydrothermal deposits for biosignature detection efforts C_LI