Happy 1st Anniversary Chelyabinsk! The Fireball that Woke Up the World

by Bob King on February 15, 2014

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Chelyabinsk fireball recorded by a dashcam from Kamensk-Uralsky north of Chelyabinsk where it was still dawn.

Frame grab of the Chelyabinsk fireball recorded by a dashcam from Kamensk-Uralsky north of Chelyabinsk at dawn. No one knew the asteroid was headed our way because for the previous few weeks it was in the same direction in the sky as the sun and impossible to observe. Click to see full video.

Wonder and terror. Every time I watch the dashcam videos of the Chelyabinsk fireball it sends chills down my spine. One year ago today, February 15, 2013, the good citizens of Chelyabinsk, Russia and surrounding towns collectively experienced these two powerful emotions as they witnessed the largest meteorite fall in over 100 years. 


Incredible compilation of dashcam and security camera videos of the fireball

The Chelyabinsk fall, the largest witnessed meteorite fall since the Tunguska event in 1908, exploded with 20-30 times the force of the atomic bomb over Hiroshima at an altitude of just 14.5 miles (23 km). Before it detonated into thousands of mostly gravel-sized meteorites and dust,  it’s estimate the incoming meteoroid was some 66 feet (20-meters) end to end, as tall as a five-story building. The shock wave from the explosion shattered windows up and down the city, injuring nearly 1,500 people.

Friction and enormous pressures placed upon the Chelyabinsk meteoroid by the atmosphere caused it to explode to pieces and send a shock wave across the cities below. This is a selection of typical small, fusion-crust covered Chelyabinsk meteorites. The U.S. penny is 9mm in diameter. Credit: Bob King

Atmospheric friction pressure on the Chelyabinsk meteoroid caused it to explode to pieces and send a shock wave across the land below. Pictured is a selection of typical small, fusion-crust covered Chelyabinsk meteorites recovered shortly after the fall. The U.S. penny is 9mm in diameter. Credit: Bob King

For nearby observers it briefly appeared brighter than the sun.  NASA Meteorite researcher Peter Jenniskens conducted an Internet survey of eyewitnesses and found that eye pain and temporary blindness were the most common complaints from those who looked directly at the fireball.  20 people also reported sunburns including one person burned so badly that his skin peeled:

Trajectory projection and strewnfield map showing the main fireball (and two additional explosions) at top and the elliptical shaped area where the densest concentration of meteorites were found. Credit: Svend  Buhl and K. Wimmer

Map showing the trajectory of the main fireball in yellow (and two additional explosions at top left). The pink oval, called the strewnfield, is where the densest concentration of meteorites were found. Click to see additional maps. Credit: Svend Buhl and K. Wimmer

“We calculated how much UV light came down and we think it’s possible,” Jenniskens said. Perhaps surprisingly, most of the meteoroid’s mass – an estimated 76% – burned up and was converted to dust during atmospheric entry. It’s estimated that only 0.05% of the original meteoroid or 9,000 to 13,000 pounds of meteorites fell to the ground.


No video I’ve seen better captures the both the explosion of the fireball and ensuring confusion and chaos better than this one.

The largest fragment, weighing 1,442 lbs. (654 kg), punched a hole in the ice of Lake Chebarkul. Divers raised it from the bottom muck on Oct. 16 last year and rafted it ashore, where scientists and excited onlookers watched as the massive space rock was hoisted onto a scale and promptly broke into three pieces. Moments later the scale itself broke from the weight.

The 26-foot-wide (8-meter) hole punched in the ice of Chebarkul Lake by the largest fragment of the Chelyabinsk meteorite. Credit: Eduard Kalinin

The 26-foot-wide (8-meter) hole punched in the ice of Chebarkul Lake by the largest fragment of the Chelyabinsk meteorite. Credit: Eduard Kalinin

There were plenty of meteorite to go around as local residents tracked down thousands of fragments by looking for holes pierced in the snow cover by the hail of space rocks. Working with hands and trowels, they dug out mostly small, rounded rocks covered in fresh black fusion crust, a 1-2 mm thick layer of rock blackened and melted rock from frictional heating by the atmosphere. According to the Meteoritical Bulletin Database entry,  the total mass of the recovered meteorites to date comes to 1,000 kg (2,204 lbs.) with locals finding up to more than half of that total.


Animation of the orbit Chelyabinsk meteoroid via Ferrin and Zuluaga. Meteoroid is the name given a meteor while still orbiting the sun before it enters Earth’s atmosphere.

Thanks to the unprecedented number of observations of the fireball recorded by dashcams, security cameras and eyewitness accounts, astronomers were able to determine an orbit for  Although some uncertainties remain, the object is (was) a member of the Apollo family of asteroids, named for 1862 Apollo, discovered in 1932. Apollos cross Earth’s orbit on a routine basis when they’re nearest the sun. Chelyabink’s most recent crossing was of course its last.

Chelyabinsk meteorites exhibit many signs of  shock created during an asteroid impact long ago. Many specimens show a typical pale white color with small chondrules typical of LL5 chondrite. A closer look shows fine, dark shock veins of melted glass. Other fragments are made of impact melt, rock shocked-heated and blackened by impact. Credit: Bob King

Chelyabinsk meteorites tell the tale of an earlier impact with another asteroid 4.452 billion years ago. Many specimens are pale white with small chondrules typical of LL5 chondrites. A closer look shows fine, dark shock veins of melted glass. Other fragments are made of pure impact melt, rock shocked-heated, melted and blackened by impact. Credit: Bob King

Chelyabinsk belongs to a class of meteorites called ordinary chondrites, a broad category that includes most stony meteorite types. The chondrites formed from dust and metals whirling about the newborn sun some 4.5 billion years ago; they later served as the building blocks for the planets, asteroids and comets that populate our solar system. Chondrites are further subdivided into many categories. Chelyabinsk belongs to the scarce LL5 class — a low iron, low metal stony meteorite composed of silicate materials like olivine and plagioclase along with small amounts of iron-nickel metal.

 

Most of the Chelyabinsk meteorites were shattered and broken during the explosion / shock blast, revealing brecciation, metal and shock veins in their interiors. Credit: Bob King

Most of the Chelyabinsk meteorites were shattered and broken during the explosion / shock blast, revealing brecciation, metal and shock veins in their interiors. Credit: Bob King

A thin slice of Chelyabinsk impact melt breccia. Flows of once-molten rock (gray) surround islands of less altered material. A small iron nickel nodule is seen at lower left. Credit: Bob King

A thin slice of Chelyabinsk impact melt breccia. Flows of once-molten rock (paler gray) surround islands of less altered material. A small iron nickel nodule is seen at lower left. Credit: Bob King

 

A closer look at Chelyabinsk meteorites reveals a fascinating story of ancient impact. Remarkably, the seeds of the meteoroid’s atmospheric destruction were sown 115 million years after the solar system’s formation when ur-Chelyabinsk was struck by another asteroid, suffering a powerful shock event that heated, fragmented and partially melted its interior. Look inside a specimen and the signs are everywhere – flows of melted rock, spider webby shock veins of melted silicates and peculiar, shiny cleavages called “slickensides” where meteorites broke along  pre-existing fracture planes.

Slickensides on a Chelyabinsk meteorite fragment where the fragment broke along a pre-existing fracture plane. Credit: Bob King

Slickensides on a Chelyabinsk meteorite fragment where the fragment broke along a pre-existing fracture plane. Credit: Bob King

Jenniskens calculated that the object may have come from the Flora family of S-type or stony asteroids in the belt between Mars and Jupiter. Somehow Chelyabinsk held together after the impact until nearly the time it met its fate with Earth’s atmosphere. Researchers at University of Tokyo and Waseda University in Japan discovered that the meteorite had only been exposed to cosmic rays for an unusually brief time for a Flora member – just 1.2 million years. Typical exposures are much longer and indicate that the Chelyabinsk parent asteroid only recently broke apart. Jenniskens speculates it was likely part of a loosely-bound, rubble pile asteroid that may have broken apart during a previous close encounter with Earth in the last 1.2 million years. The rest of the rubble pile might still be orbiting relatively nearby as part of the larger population of near-Earth asteroids.

Rivulets of melted rock line the fusion crust of melted rock on this small Chelyabinsk meteorite. Credit: Bob King

Rivulets of melted rock line the fusion crust of melted rock on this small Chelyabinsk meteorite. Credit: Bob King

Good thing Chelyabinsk arrived pre-fractured. Had it been solid through and through, more of the original asteroid might have survived its fiery descent and wreaked even more havoc in in its wake.

We’re fortunate that Chelyabinsk contains a fantastic diversity of features and that we have so many pieces for study. Surveys have found some 500 near-Earth asteroids. No doubt some are part of the parent body of Chelyabinsk and may grace our skies on some future date. Whatever happens, Feb. 15, 2013 will go down as a very loud “wake-up call” for our species to implement more asteroid-hunting programs both in space and on the ground. Enjoy a few more photos of this incredible gift from space:

This Chelyabinsk "nosecone" or "bullet" weighs just 0.35g. It displays a beautiful streamlined form from its flight through the atmosphere. Credit: Bob King

This Chelyabinsk “nosecone” or “bullet” weighs just 0.35g. It displays a beautiful streamlined form from its flight through the atmosphere. Credit: Bob King

Check out the bubble texture on this one. Heated by friction with the air, this fragment shows bubbly crust from escaping gases. Credit: Bob King

Check out the bubble texture on this one. Heated by friction with the air, this fragment shows bubbly crust from escaping gases. Credit: Bob King

Slice of Chelyabinsk showing relatively unshocked areas (light brown) cut by thick dark veins of shock-darkened material. Credit: Bob King

Slice of Chelyabinsk showing mildy shocked areas (light brown) cut by thick dark veins of shock-darkened material. Credit: Bob King

Some Chelyabinsk individuals show interesting variations in color that have nothing to do with rusting. It's believed that varying amounts of oxygen available to the speeding rocks during the meteorite break up created the brownish-red coloration on some fusion crusts. Credit: Bob King

Some Chelyabinsk individuals show interesting variations in color that have nothing to do with rusting. It’s believed that varying amounts of oxygen available to the speeding rocks during the meteorite break up created the brownish-red coloration on some fusion crusts. Credit: Bob King

OK, I saved the weirdest for last - a smaller Chelyabinsk meteorite appears to have followed closely enough behind the larger for there liquid fusion crusts to have welded them together. Just my speculation. Credit: Bob King

I saved the weirdest for last – a smaller Chelyabinsk meteorite appears to have followed closely enough behind the larger for their still-molten fusion crusts to have welded them together. Just my speculation. Credit: Bob King

About 

I'm a long-time amateur astronomer and member of the American Association of Variable Star Observers (AAVSO). My observing passions include everything from auroras to Z Cam stars. Every day the universe offers up something both beautiful and thought-provoking. I also write a daily astronomy blog called Astro Bob.

2eurocents February 15, 2014 at 3:59 PM

I know it’s all too easy to be facetious and not really think, and believe you’re not responsible for what you spout out online.
But step back and look at this: more than 1,000 people (albeit Russians) were injured and who knows how many traumatized on that day.
Now look at this: “Happy anniversary?”
I hope you’re properly ashamed of yourself.

Bob King February 15, 2014 at 9:05 PM

Dear 2eurocents,
No harm meant by the headline. It’s just an expression. I did mention those injured (as well as the good meteorite science gleaned from Chelyabinsk). If you read the article, you’ll see my point – that the Chelyabinsk fall was a wake-up call for science and the public to do more to potentially prevent a catastrophe.

Manu February 15, 2014 at 5:42 PM

Great article, thanks!
I also found the website from which the map originates highly interesting:
http://www.meteorite-recon.com/en/Meteorite_Chelyabinsk_1.html

Gozlemci February 16, 2014 at 1:18 AM

Thanks Bob… It is a very informative article…

Bob King February 17, 2014 at 6:17 PM

Manu and Gozlemci – thank you very much!

Woody February 19, 2014 at 12:41 PM

Hi Bob,

Thanks for this interesting article. I have a question about specimens from the Chelyabinsk fall. Many of the meteorites offered for sale appear riddled with hairline cracks on the surface, like those seen in one of your photos above (the brownish specimen). Do such cracks penetrate deep, and is such a specimen at risk of falling apart?

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