The Mysterious Case of the Missing Sulfur
In 2010, scientists studying asteroid 433 Eros made a puzzling discovery: its surface showed dramatic sulfur depletion compared to its interior. This finding was later confirmed by analysis of samples from asteroid Itokawa, where Fe-rich whiskers protruded from sulfide grains like microscopic stalagmites 1 . These discoveries revealed a fundamental gap in our understanding of space weatheringâparticularly how sulfur behaves on airless bodies bombarded by cosmic forces.
For decades, planetary scientists assumed solar wind radiation was the primary driver of surface alteration. But when laboratory simulations failed to fully replicate the mysterious sulfur depletion and whisker formation, researchers realized another cosmic sculptor must be at work: micrometeoroid bombardment. This article explores the revolutionary discovery of metal-sulfide agglutinatesâspace-forged composites that rewrite our understanding of asteroid surface evolution.

Cosmic Alchemy: Space Weathering's Secret Recipe
The Birth of Agglutinates
Asteroid surfaces are constantly reshaped by space weatheringâa combination of solar wind irradiation, cosmic rays, and micrometeoroid impacts. When microscopic impactors strike at hypersonic speeds (up to 20 km/s), they generate instantaneous temperatures exceeding 1,100°C. This flash-melts surface minerals, creating glassy composites called agglutinates that cement surrounding particles together 1 .
Unlike lunar agglutinates (iron-dominated), asteroidal varieties contain abundant sulfide minerals like pentlandite ([Fe,Ni]âSâ) and pyrrhotite (FeâââS). These sulfur-rich compounds behave dramatically differently when heated:
Mineral | Composition | Reactivity | Abundance |
---|---|---|---|
Pentlandite | (Fe,Ni)âSâ | Moderate | Common in LL chondrites |
Pyrrhotite | FeâââS | High | Dominant in carbonaceous asteroids |
Pyrite | FeSâ | Low | Rare on weathered surfaces |
Table 1: Key Sulfide Minerals in Space Weathering
The Whisker Enigma
Hayabusa's return of Itokawa samples revealed S-depleted rims on sulfide grains adorned with filamentous Fe-Ni structures up to 3 µm long. Initially attributed to solar wind, their origin remained unexplained until 2025, when transmission electron microscope (TEM) experiments uncovered a startling formation mechanism 1 .
The Smoking Gun Experiment: Simulating Cosmic Impacts
Methodology: Inside the Space Weathering Simulator
Researchers designed a groundbreaking experiment to recreate micrometeoroid strikes:
- Sample Preparation: Natural pentlandite grains were crushed into micron-sized particles mimicking asteroidal regolith 1 .
- Vacuum Chamber: Particles were loaded into a TEM equipped with a laser heating system replicating impact conditions (10â»â¶ mbar pressure).
- Thermal Pulses: Samples received millisecond-scale laser pulses reaching 1,100°Câmatching micrometeoroid impact temperatures.
- Progressive Bombardment: Each sample endured up to three heating cycles to simulate repeated impacts.
- In Situ Analysis: High-resolution imaging and spectroscopy tracked real-time changes in chemistry and microstructure 1 .
Revolutionary Findings
After the first thermal pulse:
- Grains developed rounded morphologies indicating partial melting
- Curved Fe-Ni whiskers sprouted from surfaces (Fig. 1b)
- Whiskers were entirely sulfur-free despite originating from S-rich pentlandite
Impact Cycle | Whisker Length | Composition | Key Features |
---|---|---|---|
1st | Up to 3 µm | Fe + 26-35% Ni | Needle-like, striated surfaces |
2nd | <0.5 µm | Fe + 65-75% Ni | Blunted, coalesced into ridges |
3rd | Absent | â | Fully integrated into Ni-rich rims |
Table 2: Whisker Characteristics After Experimental Impacts
Chemical mapping revealed a zoning phenomenon: sulfur decreased sharply at grain edges while nickel concentrated in whisker bases. Crystallographic analysis showed the whiskers were composed of awaruite (NiâFe)âan iron-nickel alloy absent in the original mineral 1 .
"The whiskers we produced were identical to those on Itokawa samplesâfinally confirming impacts, not just solar wind, drive asteroidal space weathering"
Cosmic Implications: Rewriting Asteroid History
Solving the Sulfur Depletion Mystery
This experiment demonstrated that micrometeoroid impacts:
Vaporization during flash heating releases sulfur from surface minerals
Fractional melting causes nickel to accumulate in specific zones
Heteroepitaxial growth on sulfide substrates creates metal filaments
Ryugu's Organic-Sulfur Connection
Analysis of Hayabusa2 samples revealed even more complexity:
- Thiol organosulfurs coat sulfate grains in Ryugu particles
- Calcium thiosulfate grains show anomalous δ³â´S values (+12â°)
- Isotopic signatures point to presolar photochemistry in molecular clouds 9
This suggests sulfur participates in both mineralogical and organic space weathering cyclesâa revelation for understanding prebiotic chemistry.
The Psyche Mission Connection
NASA's upcoming mission to metal-rich asteroid Psyche will directly observe these processes. As Dr. Bose explains: "Sulfides record both the early solar system environment and active processes on airless bodies today" 1 9 . Instruments will map surface sulfides to test models of impact-driven sulfur loss.
The Scientist's Toolkit: Decoding Sulfur Signatures
Tool | Function | Key Insight |
---|---|---|
FIB-SEM | Cross-sectioning grains | Reveals S-depleted rims beneath surfaces |
Synchrotron XANES | Mapping sulfur speciation | Detects organic vs. inorganic sulfur |
NanoSIMS | Isotopic microanalysis | Identifies presolar sulfur anomalies |
Laser Heated TEM | Simulating impacts | Replicates whisker formation in situ |
Selective Acid Etching | Quantifying sulfides | Distinguishes pyrrhotite vs. pyrite 8 |
Table 3: Essential Tools for Space Sulfur Research
Conclusion: Sulfur's Double Life in Cosmic Evolution
Sulfur's role in solar system evolution is now revealed as a tale of two environments:
Impact-driven sulfide decomposition creates metal agglutinates that dominate optical properties of asteroids like Itokawa and Ryugu
As the Crossley experiment showed, molten sulfides can percolate through solid rock to form planetary cores before full mantle meltingâespecially in sulfur-rich bodies like Mars 3
This dual narrative transforms sulfur from a mere mineral component to a central player in both surface weathering and deep planetary evolution. As sample return missions from Bennu and Ryugu continue to yield surprises, and Psyche launches toward its metal world, we stand poised to decode sulfur's cosmic diaryâone whisker at a time.
"These tiny metal filaments are nature's recordersâthey've witnessed every impact, every solar flare, every collision that shaped our cosmic neighborhood."