How Radioactive Tracers Are Unlocking Earth's Atmospheric Secrets
Sulfur—the tenth most abundant element in the universe—powers biogeochemical cycles that shape Earth's climate, air quality, and even the evolution of life. Yet its radioactive variant, cosmogenic radiosulfur (³⁵S), has long eluded scientists due to its fleeting half-life (87 days) and vanishingly low natural concentrations. Recent breakthroughs in detection techniques are now turning ³⁵S into a "cosmic clock," revealing secrets from the rapid transport of stratospheric air to the chemical chaos of our planet's earliest atmosphere 1 3 . By decoding the whispers of radioactive sulfur in ice, aerosols, and ancient rocks, researchers are rewriting the story of Earth's past and present.
Cosmic rays interacting with Earth's atmosphere create radioactive isotopes like ³⁵S that serve as tracers for atmospheric processes.
Sulfur cycles through land, sea, and air in a complex dance driven by:
Volcanic emissions, oceanic plankton (producing dimethyl sulfide), and weathering.
Fossil fuel combustion and industrial activity.
Oxidation of SO₂ to sulfate aerosols, which scatter sunlight and seed clouds.
In the oxygen-rich modern atmosphere, these processes erase isotopic "fingerprints." But in the oxygen-poor Archean eon (4–2.5 billion years ago), unique sulfur isotope signatures were preserved in rocks—clues to atmospheric chemistry before complex life 4 6 .
Sulfur has four stable isotopes (³²S, ³³S, ³⁴S, ³⁶S) and one radioactive isotope (³⁵S). Mass-independent fractionation (MIF) occurs when isotopic ratios deviate from predictable mass-dependent patterns, signaling photochemical reactions in an ozone-free atmosphere. For decades, MIF in Archean sediments pointed to an alien world bathed in ultraviolet (UV) light 6 . Yet measuring ³⁵S—the "missing piece"—proved impossible until now.
The ratio of sulfur isotopes can reveal whether a sample was formed in an oxygen-rich or oxygen-poor atmosphere, making them powerful tools for studying Earth's history.
Mass-independent fractionation (MIF): When isotopes fractionate in ways that don't depend strictly on their mass differences, indicating unusual atmospheric chemistry.
In May 2014, an air pollution crisis hit Southern California. Ground-level ozone spiked mysteriously, breaching U.S. air quality standards. Suspecting a stratospheric intrusion, Mang Lin's team deployed a novel ³⁵S-tracking protocol:
High-volume air collectors captured SO₂ and sulfate aerosols at Scripps Pier (La Jolla, CA) for 3–10 days.
SO₂ was trapped on potassium hydroxide (KOH)-impregnated filters; aerosols were dissolved and purified.
An ultra-low-background liquid scintillation spectrometer quantified ³⁵S atoms 3 .
| Tool/Reagent | Function |
|---|---|
| KOH-impregnated filters | Traps SO₂ gas from air samples |
| Liquid scintillation counter | Detects beta decay from ³⁵S in purified samples (sensitivity: 1 atom/10¹⁸ S) |
| High-volume aerosol sampler | Collects large air volumes (∼1 m³/min) for rare ³⁵S capture |
| Isotope purification columns | Isolates sulfate from interfering ions (e.g., sea salt, organics) |
On May 3, 2014, ³⁵S concentrations in fine aerosols skyrocketed to 7,390 atoms/m³—16 times above baseline. Simultaneously, ozone peaked at >70 ppb across 43 monitoring stations. Satellite data and wind models confirmed the culprit: a deep stratospheric intrusion, funneled by a mid-latitude cyclone and Santa Ana winds 3 .
| Parameter | Background Level | Event Peak (May 3, 2014) |
|---|---|---|
| ³⁵S in aerosols | ~460 atoms/m³ | 7,390 atoms/m³ |
| Ground-level O₃ | <60 ppb | >70 ppb |
| Air mass origin | Marine boundary layer | Stratosphere (15–20 km altitude) |
Air quality monitoring stations like this one helped track the stratospheric intrusion event.
This study proved ³⁵S's power as a stratospheric tracer. Unlike stable isotopes, ³⁵S's production peaks in the upper atmosphere, making it unambiguous evidence of vertical air transport. The findings revealed how weather systems can "puncture" the tropopause, flooding the surface with ozone—a revelation for climate and air quality models 3 .
Lin's team later analyzed all five sulfur isotopes (³²S, ³³S, ³⁴S, ³⁵S, ³⁶S) in modern sulfate aerosols. They discovered two distinct MIF effects:
Tied to stratospheric SO₂ photolysis.
Linked to combustion—likely from recombination reactions in flames 3 .
| Era | Sample Type | Δ³³S Range (‰) | Key Insight |
|---|---|---|---|
| Archean (~2.7 Ga) | Hamersley Basin rocks | −1.9 to +6.9 6 | UV photolysis dominated an O₂-free atmosphere |
| Present day | Tibetan Plateau aerosols | +0.1 to +0.5 3 | Reflects residual stratospheric influence |
This duality was revolutionary. Modern combustion MIF mirrors isotopic oddities in 2.7-billion-year-old rocks, suggesting that both UV photolysis and thermal reactions (e.g., volcanic or wildfire-driven) shaped the Archean sulfur cycle 3 6 .
Archean MIF records—once attributed solely to UV photolysis—now demand reconsideration. Lin's work on Himalayan lake sediments showed that dust and weathering can overprint isotopic signals, complicating climate reconstructions. Simultaneously, ³⁵S-based models confirm that the Archean atmosphere had <0.0001% of today's oxygen, allowing MIF to endure 3 4 .
Artist's conception of Archean Earth with a vastly different atmosphere than today.
"Simultaneous analysis of all five sulfur isotopes lets us see the invisible threads tying Earth's earliest atmosphere to today's climate challenges."
From the toxic haze of ancient volcanoes to the contrails of jet engines, radiosulfur has emerged as a Rosetta Stone for atmospheric science. By fusing cutting-edge detection with the fossilized chemistry of deep time, researchers are not just peering into Earth's past—they're forecasting its future. As this cosmic clock ticks on, it promises to unravel how sulfur shaped, and will continue to shape, the air we breathe.
Understanding atmospheric chemistry helps us protect Earth's future.
Researchers continue to unlock secrets of Earth's atmosphere through isotopic analysis.