The Sulfur Enigma

How Space Dust Forges Metal Whiskers on Asteroids

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 weathering—particularly 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 agglutinates—space-forged composites that rewrite our understanding of asteroid surface evolution.

Asteroid 433 Eros
Asteroid 433 Eros, where sulfur depletion was first observed (Credit: NASA)

Cosmic Alchemy: Space Weathering's Secret Recipe

The Birth of Agglutinates

Asteroid surfaces are constantly reshaped by space weathering—a 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]₉S₈) and pyrrhotite (Fe₁₋ₓS). These sulfur-rich compounds behave dramatically differently when heated:

Mineral Composition Reactivity Abundance
Pentlandite (Fe,Ni)₉S₈ Moderate Common in LL chondrites
Pyrrhotite Fe₁₋ₓS 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 .

Itokawa samples
Itokawa samples showing metal whiskers (Credit: JAXA)

The Smoking Gun Experiment: Simulating Cosmic Impacts

Methodology: Inside the Space Weathering Simulator

Researchers designed a groundbreaking experiment to recreate micrometeoroid strikes:

  1. Sample Preparation: Natural pentlandite grains were crushed into micron-sized particles mimicking asteroidal regolith 1 .
  2. Vacuum Chamber: Particles were loaded into a TEM equipped with a laser heating system replicating impact conditions (10⁻⁶ mbar pressure).
  3. Thermal Pulses: Samples received millisecond-scale laser pulses reaching 1,100°C—matching micrometeoroid impact temperatures.
  4. Progressive Bombardment: Each sample endured up to three heating cycles to simulate repeated impacts.
  5. 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 — 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 (Ni₃Fe)—an iron-nickel alloy absent in the original mineral 1 .

"The whiskers we produced were identical to those on Itokawa samples—finally confirming impacts, not just solar wind, drive asteroidal space weathering"

Dr. Thompson

Cosmic Implications: Rewriting Asteroid History

Solving the Sulfur Depletion Mystery

This experiment demonstrated that micrometeoroid impacts:

Sulfur Liberation

Vaporization during flash heating releases sulfur from surface minerals

Nickel Concentration

Fractional melting causes nickel to accumulate in specific zones

Whisker Growth

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 δ³⁴S values (+12‰)
  • Isotopic signatures point to presolar photochemistry in molecular clouds 9

This suggests sulfur participates in both mineralogical and organic space weathering cycles—a 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:

Surface Sculptor

Impact-driven sulfide decomposition creates metal agglutinates that dominate optical properties of asteroids like Itokawa and Ryugu

Planet Builder

As the Crossley experiment showed, molten sulfides can percolate through solid rock to form planetary cores before full mantle melting—especially 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 diary—one whisker at a time.

"These tiny metal filaments are nature's recorders—they've witnessed every impact, every solar flare, every collision that shaped our cosmic neighborhood."

Dr. Michelle Thompson, ARES Division, NASA Johnson Space Center 1

References