Scientists debated the origin of microscopic magnetite () crystals found within carbonate globules in the Martian meteorite ALH84001.
Hypothesis 1
The magnetite crystals are biogenic, meaning they were formed by ancient Martian magnetotactic bacteria. Magnetotactic bacteria produce magnetite intracellularly under low-temperature (less than ), aqueous conditions. These biogenic crystals are characterized by extreme chemical purity, a distinct narrow size range ( to ), and a lack of structural defects (such as screw dislocations), which optimizes their magnetic properties. The proponents argue these properties cannot be replicated simultaneously by abiotic processes.
Hypothesis 2
The magnetite crystals are abiogenic, formed during a high-temperature (greater than ), short-duration shock event on Mars. A meteoroid impact caused the thermal decomposition of iron-bearing carbonate minerals. Proponents of this view argue that such shock-induced decomposition typically yields magnetite crystals containing chemical impurities (such as magnesium or manganese ions substituting for iron) and high densities of structural defects, distributed across a wide range of sizes.
New Evidence
Researchers simulated Martian shock events in a laboratory by subjecting natural iron-bearing carbonates to rapid heating at using a high-energy laser for less than . Analysis of the resulting magnetite crystals revealed that they were chemically pure, lacked any detectable screw dislocations, and of them had diameters between and .
Which of the following statements best describes how this new evidence impacts the two hypotheses?
- It weakens Hypothesis 1 by showing that the specific physical characteristics of the meteorite's magnetite are not unique to bacterial synthesis, and it supports the viability of Hypothesis 2 by demonstrating that thermal decomposition can produce these characteristics.Cevap
- BIt supports Hypothesis 1 by demonstrating that magnetite crystals can be synthesized within a narrow size range, and it weakens Hypothesis 2 because the simulated shock event did not produce the expected chemical impurities and structural defects.
- CIt weakens Hypothesis 1 because the experimental temperature of is too high for magnetotactic bacteria to survive, but it has no effect on Hypothesis 2 because the laboratory shock simulation did not occur on Mars.
- DIt supports both Hypothesis 1 and Hypothesis 2 because it shows that magnetite crystals can be formed under both low-temperature aqueous conditions and high-temperature shock conditions.