Atmospheric physicist Nick Gorkavyi missed witnessing an event of the century last winter when a meteor exploded over his hometown of Chelyabinsk, Russia.
From Greenbelt, Md., however, NASA’s Gorkavyi and colleagues witnessed the atmospheric aftermath. The explosion created a never-before-seen belt of “meteor dust” that circulated through the stratosphere for at least three months.
Shortly after dawn on Feb. 15, 2013, the meteor, or bolide, measuring 18 meters across and weighing 11,000 metric tons, screamed into Earth’s atmosphere at 41,600 miles per hour.
Burning from the friction with Earth’s thin air, the space rock exploded 23 km above Chelyabinsk, releasing more than 30 times the energy from the atom bomb that destroyed Hiroshima.
Some of the surviving pieces of the Chelyabinsk bolide fell to the ground. But the explosion also deposited hundreds of tons of dust up in the stratosphere, allowing the NASA-NOAA Suomi National Polar-orbiting Partnership satellite to make unprecedented measurements of how the material formed a thin but cohesive and persistent stratospheric dust belt.
“We wanted to know if our satellite could detect the meteor dust,” said Gorkavyi, of NASA’s Goddard Space Flight Center in Greenbelt, Md., who led the study, which has been accepted for publication in the journal Geophysical Research Letters. “Indeed, we saw the formation of a new dust belt in Earth’s stratosphere, and achieved the first space-based observation of the long-term evolution of a bolide plume.”
Gorkavyi and colleagues combined a series of satellite measurements with atmospheric models to simulate how the plume from the bolide explosion evolved as the stratospheric jet stream carried it around the Northern Hemisphere.
About three and a half hours after the initial explosion, the Ozone Mapping Profiling Suite instrument’s Limb Profiler on Suomi detected the plume high in the atmosphere at an altitude of about 40 km, quickly moving east at about 190 miles per hour.
The day after the explosion, the satellite detected the plume continuing its eastward flow in the jet and reaching the Aleutian Islands.
Larger, heavier particles began to lose altitude and speed, while their smaller, lighter counterparts stayed aloft and retained speed – consistent with wind speed variations at the different altitudes.
By Feb. 19, four days after the explosion, the faster, higher portion of the plume had snaked its way entirely around the Northern Hemisphere and back to Chelyabinsk. But the plume’s evolution continued: At least three months later, a detectable belt of bolide dust persisted around the planet.
The scientists’ model simulations, based on the initial Suomi NPP observations and knowledge about stratospheric circulation, confirmed the observed evolution of the plume, showing agreement in location and vertical structure.
“Thirty years ago, we could only state that the plume was embedded in the stratospheric jet stream,” said Paul Newman, chief scientist for Goddard’s Atmospheric Science Lab. “Today, our models allow us to precisely trace [the dust from] the bolide and understand its evolution as it moves around the globe.”
The full implications of the study remain to be seen.
Every day, tens of metric tons of small material from space encounters Earth and is suspended high in the atmosphere.
Even with the addition of the Chelyabinsk debris, the environment there remains relatively clean. Particles are small and sparse, in contrast to a stratospheric layer just below where abundant natural aerosols from volcanoes and other sources collect.
Still, with satellite technology now capable of more precisely measuring tiny atmospheric particles, scientists can embark on new studies in high-altitude atmospheric physics.
How common are previously unobservable bolide events? How might this debris influence stratospheric and mesospheric clouds?
Scientists previously knew that debris from an exploded bolide could make it high into the atmosphere. In 2004, scientists on the ground in Antarctica made a single lidar observation of the plume from a 1,000-ton bolide.
“But now in the space age, with all of this technology, we can achieve a very different level of understanding of injection and evolution of meteor dust in atmosphere,” Gorkavyi said. “Of course, the Chelyabinsk bolide is much smaller than the ‘dinosaurs killer,’ and this is good: We have the unique opportunity to safely study a potentially very dangerous type of event.”
Dr. Tony Phillips works for the National Aeronautics and Space Administration.