December 7, 2016 report
Cosmic dust found in city rooftop gutters
Up till now, researchers looking for space dust have usually had to travel to the Antarctic—it was thought the tiny particles, believed to be left over remnants of the formation of the solar system, would be too difficult to find in places where there is a proliferation of other dust types, particularly in areas where people live. John Larson, an amateur space scientist with Project Stardust, came to researchers at Imperial College suggesting that maybe space dust could be found on rooftops. Despite a high degree of skepticism regarding the prospects, the team traveled to Oslo, Berlin and Paris and obtained 300 kilograms of dirt samples from rain gutters on rooftops. Back in the lab, they used magnets to pull possible cosmic dust grains from within the muck. They report that they found and identified approximately 500 samples.
The team also report that the dust grains they found were larger than those typically found in Antarctica—they measured approximately 0.3 millimeters as opposed to the customary average of 0.01 millimeters. They also noted the grains had fewer feather-like crystals than those found in Antarctica. They suggest the differences are likely due to age—those from Antarctica are typically much older, which would mean the planets would have been aligned slightly differently when they fell to Earth. That differences indicate dust particles falling through the atmosphere would have been traveling much faster in more recent times due to a difference in trajectory—up to 12 kilometers per second—the fastest ever recorded for space dust. Those differences, the researchers note, may illuminate the movement of the planets relative to one another over time, helping to understand the history of the solar system.
We report the discovery of significant numbers (500) of large micrometeorites (>100 μm) from rooftops in urban areas. The identification of particles as micrometeorites is achieved on the basis of their compositions, mineralogies, and textures. All particles are silicate-dominated (S type) cosmic spherules with subspherical shapes that form by melting during atmospheric entry and consist of quench crystals of magnesian olivine, relict crystals of forsterite, and iron-bearing olivine within glass. Four particles also contain Ni-rich metal-sulfide beads. Bulk compositions are chondritic apart from depletions in the volatile, moderately volatile, and siderophile elements, as observed in micrometeorites from other sources. The reported particles are likely to have fallen on Earth in the past 6 yr and thus represent the youngest large micrometeorites collected to date. The relative abundance ratio of barred olivine to cryptocrystalline spherule types in the urban particles of 1.45 is shown to be higher than a Quaternary average of ~0.9, suggesting variations in the extraterrestrial dust flux over the past 800 k.y. Changes in the entry velocities of dust caused by quasi-periodic gravitational perturbation during transport to Earth are suggested to be responsible. Variations in cosmic spherule abundance within the geologic column are thus unavoidable and can be a consequence of dust transport as well as major dust production events.
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