Chelyabinsk Meteorite - Classic Riker Box Specimens
Chelyabinsk Meteorite - Classic Riker Box Specimens
The Chelyabinsk meteorite is part of the First Edition collection. We are happy to offer it once again as a stand-alone specimen!
Normally, the Sun is the brightest object you see in the sky, but on the morning of February 15th, 2013, this wasn’t the case. Just minutes after sunrise, over 18 miles up, an object entering the Earth’s atmosphere exploded over the town of Chelyabinsk in Russia. This object, known as the Chelyabinsk meteor, has since become one of the most witnessed entries of an extraterrestrial object.
This specimen is a Chelyabinsk meteorite fragment. The specimen is housed in an acrylic jar that is encased within a glass-topped riker display box. The box measures 4 1/2" x 3 1/2". A small information card is also included, which serves as the certificate of authenticity.
Both small and medium sized fragments are available. You can see the full sizing info further below.
📸 The Chelyabinsk Meteorite Specimen
Chelyabinsk Meteorite (Fall date: 2013)
Normally, the Sun is the brightest object you see in the sky, but on the morning of February 15th, 2013, this wasn’t the case. Just minutes after sunrise, over 18 miles up, an object entering the Earth’s atmosphere exploded over the town of Chelyabinsk in Russia. This object, known as the Chelyabinsk meteor, has since become one of the most witnessed entries of an extraterrestrial object.
The phenomenon was quickly shared all across the globe — the Chelyabinsk meteorite was only of the only impact events to be witness by a large group of people in the 21st century, which means a uniquely large amount of footage is available thanks to cell phones and dashcam footage.
The impressive meteorite reached a top speed of over 40,000 miles per hour and after the explosion, pieces flew across the Russian snowbanks where they were discovered by collectors.
This specimen is a Chelyabinsk meteorite fragment. The specimen is housed in an acrylic jar that is encased within a glass-topped riker display box. The box measures 4 1/2" x 3 1/2". A small information card is also included, which serves as the certificate of authenticity.
Both small and medium sized fragments are currently available. We also have larger "showcase" sized specimens available as stock lasts.
Small - 0.5 cm and smaller
Medium - 0.5 cm to 1 cm
Showcase - Sized individually (see below)
The specimens vary in size and shape, but all will show some measure of the black fusion crust created by the intense heat and speed of the meteorite. This crust is a clear indicator of the fragment's powerful stellar origins.
Showcase Specimens
We have larger showcase Chelyabinsk fragments available while supplies last as well. These items are photographed individually and listed by size. You can see all of them in the collection below!
These pieces are quite large and come in either one of our glass-topped riker display boxes or a hinged jewelry box with a golf tee style stand depending on the size. Both a certificate of authenticity and informational photo card are also included with your fragment.
40,000 Miles Per Hour, 30 times brighter than the sun
MORE ABOUT CHELYABINSK
"Immediately one can start asking questions about whether these are as rare as we thought."~ Dr. Paul Chodas, Manager of the NASA NEO Program Office at JPL
📸 This image of a vapor trail was captured about 125 miles (200 kilometers) from the Chelyabinsk meteor event, about one minute after the house-sized asteroid entered Earth’s atmosphere. (Source: Alex Alishevskikh)
📸 A dashcam image of the meteorite near its brightest point
A fireball in the sky
The Chelyabinsk meteor is referred to as a bolide, a term for objects which appear like fireballs during entry. The light seen over Chelyabinsk peaked with a magnitude of -27.3, 30 times brighter than the Sun itself. Anyone awake in the early morning would have immediately seen the shift in light, with shadows cast from extreme angles that moved with the arc of the meteor.
This meteor had a massive 66-foot diameter and is estimated to have weighed over 13,000 tons. At its fastest, it was moving at over 40,000 miles per hour, almost 60 times the speed of sound.
📸 Damage from the explosion
Shortly after the meteor hit its brightest point, it shattered in a powerful explosion that sent a shockwave of force from the sky. Pieces of the object were flung west of Chelyabinsk, with many meteorites leaving holes in the morning’s snowbanks. Several fragments would eventually be found in Lake Chebarkul, with one weighing up to 1,442 pounds. While it was fortunate that there were no major damages from the impact, the airburst was powerful enough to affect things on the ground.
The shock waves from the explosion damaged over 7000 regional buildings and sent over 1000 people to the hospital, mostly suffering from lacerations from flying glass. The event was so powerful it created a dust belt in the stratosphere that circled the entire planet and lingered for months. Witnesses claimed they had to turn away from the intense heat and light and some even suffered from sunburns. Videos quickly appeared on the Internet where millions around the world viewed the event soon after it occurred.
While the event has had no reported deaths, it has raised some fears over unpreparedness for subsequent meteorites. The space around the planet is filled with objects whose orbits cross with Earth, so many in fact, that it is impossible to track them all. Many of these burn up into nothing in the atmosphere, but obviously not all of them. The Chelyabinsk meteor went undetected until its entry and was the largest meteor to enter the atmosphere since Tunguska in 1908. Before this incident, it was thought that such large strikes were a once-in-centuries event. Now, some think it may be a once-in-decades event.
📸 A macro shot of a piece of the Chelyabinsk meteorite
Creating a fusion crust
The Chelyabinsk meteorite is what's known as a chondrite — a stony meteorite full of round mineral grains. These meteorites are made up of iron oxides and silicates that originated from a larger body in the asteroid belt.
The dark black outer layer of the meteorite is a relatively new addition though; it was created during the entry to Earth's atmosphere. This outer coating is what's known as a fusion crust. When the Chelyabinsk meteorite rocketed to the ground, the high speed and air friction caused its exterior to rapidly heat up. A thin layer of material melted and quickly cooled, turning into a dark and glassy coating.
This fusion crust is a prime indicator of meteorite material, as the conditions to create it are not found in natural places on Earth. Interplanetary travel is the only way for such a feature to appear in a natural stone.
FRONT OF THE SPECIMEN CARD
BACK OF THE SPECIMEN CARD
Further Reading
Grant, Andrew. “Large Meteor Strikes Underestimated.” Science News, vol. 184, no. 11, 2013, pp. 6–6.
Chapman, Clark R. “Calibrating Asteroid Impact.” Science, vol. 342, no. 6162, 2013, pp. 1051–1052.
Popova, Olga P., et al. “Chelyabinsk Airburst, Damage Assessment Meteorite Recovery, and Characterization.” Science, vol. 342, no. 6162, 2013, pp. 1069–1073.
Ozawa, S., Miyahara, M., Ohtani, E. et al. “Jadeite in Chelyabinsk meteorite and the nature of an impact event on its parent body.” Sci Rep vol 4, 5033 (2014).
Yau, Kevin, et al. “Meteorite Falls in China and Some Related Human Casualty Events.” Meteoritics, vol. 29, no. 6, 1994, pp. 864–871.