Category Archives: Daily Asteroid

Meteorites are fragments of asteroids or comets that have survived their passage through the Earth’s atmosphere and have impacted the Earth’s surface. These extraterrestrial rocks have fascinated humans for centuries and have provided valuable insights into the formation and evolution of our Solar System, approximately 4.6 billion years ago.

According to current scientific understanding, the Solar System formed from a cloud of gas and dust that collapsed under its own gravity. As this cloud collapsed, it began to spin and flatten into a disk. The Sun formed at the center of this disk, and the remaining gas and dust eventually formed into the planets, moons, asteroids, and comets that we see today.

Meteorites are believed to originate from two main sources: asteroids and comets. Asteroids are rocky and metallic objects that orbit the Sun in the asteroid belt between Mars and Jupiter. They are remnants from the early Solar System that never accreted into a planet. Comets, on the other hand, are icy objects that originate from the Kuiper Belt and the Oort Cloud beyond the orbit of Neptune.

When asteroids or comets collide with each other, fragments can be ejected into space. These fragments can travel through the Solar System and eventually collide with a planet, such as Earth, where they become meteorites. Most meteorites that are found on Earth are believed to be from asteroids, while cometary meteorites are rare.

It’s believed that cometary meteorites could be carbonaceous chondrites. They are a type of stony meteorite that contain a high amount of carbon compounds and volatile elements, which are thought to be characteristic of comets.

Carbonaceous chondrites are believed to originate from the outer regions of the Solar System, beyond the orbit of Jupiter. They are thought to be remnants from the early Solar System that have remained relatively unchanged since their formation, providing valuable information about the conditions that existed in the early Solar System.

Some carbonaceous chondrites have been found to contain organic compounds, including amino acids, which are the building blocks of life. This has led some scientists to speculate that these meteorites could have played a role in the origin of life on Earth.

One famous example of a carbonaceous chondrite is the Murchison meteorite, which fell in Australia in 1969. It is one of the most studied meteorites in history and has provided valuable insights into the chemical and isotopic composition of the early Solar System.

The study of meteorites has provided valuable insights into the formation and evolution of our Solar System. By analyzing the chemical and isotopic composition of meteorites, scientists have been able to determine the age of the Solar System, the processes that led to the formation of planets, and the conditions that existed in the early Solar System.

In conclusion, meteorites are extraterrestrial rocks that have impacted the Earth’s surface. They originate from asteroids and comets and provide valuable insights into the formation and evolution of our Solar System. The study of meteorites has helped scientists to better understand our place in the universe and the processes that have shaped our planet and the objects that surround us.

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WHAT ARE TEKTITES?

The idea that continents on Earth today had once constituted a “supercontinent” was prevalent in geologic studies. Pangea was the supercontinent that existed in the late Paleozoic era and was centered on the Equator, surrounded by a vast “superocean” called Panthalassa. Scientists estimate that Pangea was assembled approximately 335 million years ago and began breaking apart about 175 million years ago.

Further studies posit that before Pangea, another supercontinent existed in the Neoproterozoic era, about 550 million years ago, called Gondwana. According to some theories, Gondwana and Euramerica (another continent), merged to form Pangea. The supercontinent was named by Austrian scientist Eduard Suess, who proposed its existence in 1861. Suess’s son, Franz Eduard Suess, walked a similar path to his father’s and would go on to study geology. The younger Suess would coin a term familiar to meteorite collectors and those studying the metaphysical properties of minerals: tektite.

The word “tektite” comes from the Greek word for “molten.” Tektites come in a vast array of shapes and sizes. Moldavites, for example, are a gem-like green while Libyan Desert Glass pieces are honey-colored. Tektites form in a manner similar to terrestrial volcanic glasses, obsidians; they’re ejected during meteorite impacts. However, unlike volcanic glasses, tektites contain virtually no water, and their silica and isotope composition are quite different from obsidians. They also contain bands or particles of lechatelierite, a mineraloid that forms from quartz at very high temperatures. Lechatelierite is not found in obsidians and is common to tektites.

Tektites are traditionally divided into four groups: microtektites, which are less than 1 mm; splash-form tektites, considered the most “normal”; aerodynamically shaped tektites; and layered tektites. Splash-form tektites are shaped like spheres, teardrops, and other shapes you might expect something molten that solidified to take. Aerodynamically shaped tektites acquire their peculiar shape when they re-enter our atmosphere, like iron meteorites. Layered tektites are usually larger and have distinct blocky, chunky appearances and a “layered” structure.

The most widely accepted theory to explain the origin of tektites is that they came from terrestrial material that was ejected during a meteorite impact event. The debris either melted or vaporized, or both – the exact process they undergo is still poorly understood – and cooled as they fell back to Earth. This theory is supported by mineral inclusions of quartz, zircon, chromite, etc. in tektites and the fact that some tektites can be tied to an impact crater by their age and isotopic composition. However, some scientists debate this origin theory and believe tektites could have come from the Moon, an idea supported by Franz E. Suess.

Such explanations posit that tektites formed from volcanic activity on the Moon, which ejected the glasses into outer space, later landing on Earth. Scientists who support this theory cite tektites’ rare-earth and isotopic composition, physical properties, and other characteristics. There are numerous problems with the extraterrestrial origin theory of tektites, however, and most scientists agree that the characteristics displayed by tektites strongly suggest that they derived from terrestrial rocks. Even still, tektites are a major area of interest for those with an academic interest in meteorites, avid and amateur collectors, and even those interested in their metaphysical qualities.

Darwin Glass, Libyan Desert Glass, Moldavite, and Indochinites are some of the most alluring tektites, and we have several specimens available for purchase on our website. Shop here: aerolite.org/shop/our-impactites/

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Libyan Desert Glass

Libyan Desert Glass (LDG) are mysterious, honey-colored glass fragments that lie on the majestic sand dunes in western Egypt. The region was discovered in 1932 and is relatively inaccessible to human beings. Despite the challenges presented by the jagged desert landscape, the area has seen at least 10 expeditions since 1932.

It’s hard to say when, exactly, human beings discovered Libyan Desert Glass; a jewel-encrusted breastplate recovered from King Tutankhamun’s tomb boasts a beautiful scarab, carved from golden Libyan Desert Glass.

The origin of these glasses was, for a long time, considered a mystery; scientists estimated that they formed approximately 29 million years ago and there were two main formation hypotheses to explain their existence. One was that a massive meteorite impact caused the silica in the sand to melt and another pointed to melting by a large atmospheric airburst, which occurs when meteors explode in the atmosphere.

Research on the origin of these glasses is difficult because little remains of whatever it was that caused the melting in the first place. However, scientists have found evidence of a mineral called reidite, which only forms during a meteorite impact. More importantly, this mineral does not form during airbursts. Zircon grains, which are commonly found on Earth, the Moon, Mars, and various meteorites, were found in LDG specimens. These grains, smaller than the width of a single human hair, are what preserve evidence of former reidite.

The composition of LDG is rather astonishing; it’s almost completely pure silica. In an article titled “The Riddle of the Sands,” Giles Wright says that it’s the purest natural silica glass ever found. Some pieces of LDG display small, opaque, spherical inclusions of a silica polymorph called cristobalite.  Its presence in these curious glasses indicates that at one time, the source rock had been heated to temperatures of at least 2822°F (1550°C). Other inclusions have been found in LDG, and scientists study these to attempt to piece together how, exactly, the glasses formed and under what conditions.

Libyan Desert Glass is now difficult to obtain, due to the inaccessibility of the region where they are found and restrictions imposed by the Egyptian government that, in most cases, prohibit the removal of the material from the site. Aerolite Meteorites is fortunate enough to have pieces of the mystical glasses in stock, obtained legally, that display fascinating inclusions, shapes formed by years have the wind and sand swept over them, and in rare cases, marvelous translucency. View our available catalog here.

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THE SEYMCHAN PALLASITE

The modern Seymchan settlement began in 1940; during World War 2, an airfield was built there to allow aircraft to be delivered there through the Lend-Lease program, whereby the USA would supply the United Kingdom, Free France, the Republic of China, the Soviet Union, and other Allied nations with supplies like food, oil, and weaponry.

In 1949, and through 1955, a sub-settlement located a few kilometers south housed the Dalstroy prison camp, part of the Gulag camp network. Dalstroy was also called the “Far North Construction Trust” and used prisoners in the mining of gold and tin, as well as some timber production. Dalstroy was disbanded a few years after Joseph Stalin’s death in 1953.

The Seymchan meteorite was found in a dry river bed in the area in 1967 by Russian geologist F. A. Mednikov. The massive space rock was found lying among river stones; it was triangular-shaped and displayed thumbprints its surface. It was originally classified as an IIE iron; these are octahedrites, the term given to iron meteorites with a crystal structure that mimics an octahedron.

When new material was found to contain olivine crystals, Seymchan was reclassified; its designation was changed to pallasite in 2007. As the Seymchan mass was hurtling through the atmosphere, we imagine that chunks of Seymchan were sheared off at the nickel-iron/olivine borders. Because of that, some areas of Seymchan display olivine-rich clusters, and others consist almost entirely of nickel-iron.

Seymchan belongs to the main group of meteorite pallasites, though scientists find that it contains a high percentage of iridium, a  rare, silvery-white chemical element. Iridium is brittle, despite being considered to be one of the densest metals. On Earth, it’s found in ore mined from South Africa, Brazil, Russia, Australia, and Alaska, USA. Iridium is found in much higher abundance in meteorites than on Earth, which makes a case for asteroid mining.

Seymchan meteorites are attractive to collectors for various reasons; it has an interesting back story and slices can have many different appearances; some areas display olivine-rich clusters, while others consist almost entirely of nickel-iron. Worldwide interest in meteorites continues to grow and olivine-rich Seymchan specimens are now extremely difficult to acquire.

To view our available inventory, click here.

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2021 TUCSON GEM SHOW

• Air filtration: although not a requirement, the Main and Showcase Tent will have aggressive air movement via 50-ton HVACS equipped with MERV 13 air filters, which have the most effective air filtration rating and are used in hospitals
• Aisle width: all Tucson gem shows are required to provide 12′ wide aisles to enable and encourage social distancing
• Controlled entries: the Showcase Tent will have one entry and one exit in order to monitor capacity limits. The Main Tent will have controlled entries at each end and three ‘Emergency Only’ exits on the sides
• Staff screening: all show staff and security officers will be subject to daily temperature checks and health evaluation
• Enforcement: uniformed armed security will be onsite to quickly eject anyone who refuses to mask up
• Face masks: 100% required with no exceptions

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The Tsarev Stony Meteorite

Witnessed meteorite falls are some of the most spectacular events that occur in the natural world. That an event so rare is also actually seen to occur by human beings is almost equally as unbelievable, but they do happen. Advances in video technology, and how widely available dashcams and home security cameras are, allow us to witness more and more meteorite events.

Before the ability to record video became widely available to the general population, however, people had other means of reporting fireballs and strange occurrences in the sky. Scientists have found petroglyphs in ancient dwellings which appear to depict fireball-like events; meteorite events have been described in paintings, newspapers, and letters before scientists even knew they actually happened.

In the absence of video footage to confirm the meteorite falls or fireballs, eyewitness accounts become very important and, in some cases, can be tied to later finds. Such is the case, it appears, for a meteorite found in 1968 in Russia.

1968 was already a memorable year, marked by a worldwide escalation of conflict. However, in Volgograd Oblast–the primary site of the Battle of Stalingrad during World War II, one of the largest and bloodiest battles in history–a remarkable discovery was made in the quiet fields near the rural village of Tsarev.

“Tsarev,” which translates to czar, is one of the largest stone meteorites found in Russia (the USSR at the time) that resulted in one of the largest meteorite showers in Russian history. Eyewitness accounts revealed that the meteorite shower happened on December 6, 1922, though the stones were not found until 1968. The mineral composition of Tsarev is consistent with that of ordinary chondrites: olivine, orthopyroxene, clinopyroxene, maskelynite, calcium phosphates, nickel-iron, troilite, chromite, ilmenite, and rutile.

Academic samples of the Tsarev meteorite reveal large grains of nickel-iron, light grey areas with a well-preserved chondritic texture, and dark areas containing a matrix with olivine grains and relics of chondrules. Though its parent body remains unknown, experts suspect the meteorite may have originated on or near the surface of the body.

These meteorites may have undergone regolith processes and can provide valuable information in the search for parent bodies of these chondrites. Among the many finds scientists made when analyzing the meteorite was the discovery that the isotopic composition of the noble gases found in Tsarev appear to be comparable to that of solar wind, a stream of particles and plasma released from the Sun’s upper atmosphere.

View our available inventory of Tsarev stone meteorites here.

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ODESSA METEORITES

Imagine stumbling across a meteorite crater!

Craters are pretty delicate – like everything else on Earth, they are at the mercy of their environment and many of them have been eroded away by the elements. The Wabar craters, for example, in Saudi Arabia have slowly disappeared over time because the shifting sands have filled them in. Even still, craters are some of the most fascinating geological features on our planet’s surface and new ones are still being discovered today.

In 1892, a rancher looking for a lost calf on horseback had one such experience. He found not only the missing bovine, but he also stumbled upon an odd depression in the landscape, now known to be the Odessa impact crater. Located in West Texas, the crater is now recognized as a National Natural Landmark by the National Park Service. The crater itself is home to species of cactus, sagebrush, and other plants. The rim of the depression is surrounded by fragments of limestone, which stretches for miles in every direction. Beds of brownish sandstone were also found beneath the surface.

As most know, the Odessa crater was verified as a meteorite impact crater when a geologist noticed an odd paperweight sitting on a desk in the office of Odessa’s first mayor, Samuel R. McKinney. The paperweight, McKinney explained, was a rock that had come out of the center of the crater. This rock was later confirmed to be a meteorite by the head curator of the Department of Geology at the United States National Museum, now the National Museum of Natural History at the Smithsonian Institution.

The crater is estimated to be about 63,500 years old. It is no longer as deep as it once was, having been slowly filled by soil and debris eroding its original features. However, the crater remains a popular site and is one of the largest impact craters in the United States. Odessa meteorites are a nickel-iron metal and suspected to have crystallized from a melt. These irons belong to the coarse octahedrite class, which describes the way alloy metals in iron meteorites are structured. Some Odessa meteorites display dark fusion crust, caused by the meteoroid’s flight through the atmosphere.

Odessa meteorites are particularly hard to find; they’re highly collectible and have a fantastic background story. Few, if any, new specimens come out of the craters at Odessa, Texas, which has been all but picked clean by meteorite hunters and their metal detectors. We have not offered Odessa in quite some time, and are more than honored to have such fantastic pieces in our current inventory, which you can view here –> https://aerolite.org/product-category/iron-meteorites/odessa/

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ADMIRE METEORITES
Gemstones from Outer Space

The Admire meteorite was found in 1881 in Kansas by a farmer plowing a field. It’s named after the city of Admire in Lyon County (meteorites are named for the places they were found). You might think Kansas–or more generally, the Midwest–is a hot spot for meteorite falls. Meteorites, however, fall randomly across the surface of our planet, and they could land anywhere. Why, then, do so many meteorite finds happen in Kansas?

It’s a combination of factors; the soil in Kansas contains very few indigenous stones. The Kansas soil is also very fertile, so it’s farmed intensely. Meteorites frequently turn up as a result of this farming and, since Kansas soil contains such few stones, these meteorites are less likely to be mistaken for terrestrial rocks.

Scientists believe, after much study, that the Admire pallasite formed at the core-mantle boundary of an ancient asteroid. Pallasites are the rarest of meteorites; less than 1% of all meteorites are pallasites, and even fewer still contain un-shocked crystals, something which academics were surprised to discover in the Admire pallasite.

About 1 in 100 of these crystals, remarkably, lend themselves to faceting, something that is not possible with shocked crystals. Admire is one of the only meteorites that produces these “space gems.” When sliced and polished, Admire meteorite slices present a wealth of richly-colored, angular crystals of different sizes and shapes.

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Where to Buy Mars Meteorite Dust?

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