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When the planets of our solar system aggregated from the primordial dust and ice swirling in a disc around the sun, some crazy things happened. We are used to the relatively stable result, 4.6 billion years later, but in the early days, some planetoids collided cataclysmically; others were flung out of our solar system entirely, to the lifeless void of deep space.

These dense iron meteorites contain the molten metal cores of some planetary body that ended in a mighty kaboom. We know it was big because a molten iron core appears when a planetoid is big enough to have enough gravity to fractionate the elements of the periodic table, with the heavier iron-loving elements migrating to the core and a different subset of the periodic table (e.g., Si, Al, Ca, Na, Mg) constituting the outer mantle and crust. We have never drilled to the molten core of Earth, or even deep into our mantle, but these remnants of planets past are representative of what we would expect to find in the Earth’s core and mantle.

Two big iron meteorites arrived this week, this 45 lb Sericho Pallasite from Kenya and a 127 lb heavy metal barbell from Argentina (Campo del Cielo). Pallasites are an incredible potpourri of shattered mantle in a dollop of molten metal core. They can only form in space where the absence of gravity allows the lighter gemstones to remain scattered throughout the heavy metal matrix (on Earth, they would segregate by density). Those crystal gems are olivine (peridot) and this example shows an array of colors from honey to burnt orange to dark green.

The Campo from Argentina is a deeper core sample, so to speak, of pure molten core of a destroyed planetoid. If we were to look at the metal crystalline patterns inside, we would see something beautiful, an interwoven 3D nest of interlocking shards, a metal crystallization that also could not be made on Earth, but for a different reason: they have to cool very, very slowly, over 10 million years! In the insulating vacuum of space, the motel metal cools slowly as it radiates heat (no conduction or convection).

If this all sounds like a rare event, it is. 2% of meteorites in the Met Bull are irons, and only 0.2% are Pallasites, the most visually beautiful of space rocks, IMHO.

When an iron meteorite is forged into a tool or weapon, the extraterrestrial crystal patterns remain, but become stretched and distorted. The patterns usually cannot be fully eliminated by blacksmithing, even through extensive working. When a knife or tool is forged from meteoric iron and then polished, the patterns appear in the surface of the metal. In ancient times before the invention of steel, these iron-nickel alloys were like advanced alien technology, and probably were the origin of folkloric beliefs about magic swords and vorpal blades. Even King Tut was buried with his meteorite dagger.

There is much going on in this Sericho Pallasite — a meteoritic medley. Transluscent olivine gems across the color spectrum. And the metal matrix has large Farringtonite inclusions (beige) and Chromite (flat black, bottom center). Rounded upper lip is shaped from oriented entry through the Earth’s atmosphere. 45 lbs, 31x25x15cm.

Based on isotope analysis at ETH Zürich, this meteorite spent the last 130-160 million years free floating in space before intersecting Earth’s orbit.

5 responses to “Big Iron from Outer Space — The Sericho Pallasite”

  1. Kenyan recovery digFrom the Met Bull for Sericho: “In 2016, two brothers were searching for their camels and came across several large, dense stones south of Sericho, Kenya. There are no rocks in this area, so they decided they were meteorites. They spent several weeks collecting them with engine hoists and moving them to their homes in Habaswein. The masses had been known to camel-herders for decades prior. One village elder said that as a child, he and his brothers would play on top of the stones. In early January 2017, Michael Farmer received an email showing a photo of a ‘giant pallasite’. He traveled to Nairobi and purchased this stone.”

    Exterior photosSericho Meteorite Exterior 2For a sense of scale… ^ baby Luna as a hand model! 😉

    Closeups… Big Farringtonite inclusions in beige
    Chromite in flat blackThe metal crystal pattern insideA Huge Russian Meteorite“Did we lose a planet? Our Solar System looks to have had a 5th giant planet 10-30x the size of Earth that was ejected. Our giant planets did not form in their current locations but instead arrived on their current orbits as a result of planetary migration. During migration, several tens of Earth masses of material were likely gravitationally scattered around the solar system, with most of that mass being ultimately ejected into interstellar space.” — Kat Volk (U. of Arizona)

  2. the Earth’s mantle and core in hand
    thank you! for sharing precursor world-building meteorite with the Earth Science Teaching Resource group

  3. [https://www.flickr.com/photos/31856336@N03] you’re welcome. It’s quite fascinating. And where did this heavy metal come from? Long ago, after the Big Bang, we had 200 million years of ¾ H and ¼ He. The first planets were gas (like Jupiter). There were just 2 elements on periodic table. Heavier and heavier elements form each time a solar core stalls and reignites, populating most of the periodic table. Then the supernova: igniting with the brightness of 100 billion suns for a week and outshining entire galaxies. “Draped like glowing tapestries, the ejecta from a supernova explosion decorate the ocean of interstellar space.” (quotes from the book Meteorite, p.161) Consider the radioactive heating from Aluminum-26 “our nebula was seeded with stellar fallout right before it collapsed.”

    When an atom has an excess of neutrons, the neutron decomposes to a proton, changing the element. Solar alchemy is the slow process of element formation.

    Two merging neutron stars are the rapid-process synthesis path, creating 15,000 Earth’s of matter in a flash. 10 Earth’s of gold alone! Half of the elements heavier than iron come from this fast path. P.S. only Beryllium & Boron are not from stars.

    Some of the diamond and silicon carbide grains in our early solar disk “crystallized around other stars. They are pieces of bona fide stardust.” (177)

    “Some pre-date the solar system by over three billion years! Tiny pieces of rock that are seven billion years old! The mind boggles. We call these most remarkable motes of cosmic sediment ‘pre-solar’ grains.” (179)

    And here is the rough distribution of meteorite types…

  4. 1) incredible Sericho pallasite.

    2) Super-geek-out:

    "The origin and evolution of Lithium-Beryllium-Boron is a crossing point between different astrophysical fields : optical and gamma spectroscopy, non thermal nucleosynthesis, Big Bang and stellar nucleosynthesis and finally galactic
    evolution. We describe the production and the evolution of Lithium-BerylliumBoron from Big Bang up to now through the interaction of the Standard Galactic Cosmic Rays with the interstellar medium, supernova neutrino spallation and a low energy component related to supernova explosions in galactic superbubbles." –

    cds.cern.ch/record/393331/files/9907171.pdf

    3) "The cosmochemical behavior of beryllium and boron"
    Dante S. Lauretta, Katharina Lodders => http://www.sciencedirect.com/science/article/abs/pii/S0012821X96...

    Abstract
    "The chemistry of Be and B in the solar nebula is reinvestigated using thermodynamic equilibrium calculations. The dominant Be gases are monatomic Be at high temperatures and the hydroxides BeOH and Be(OH)2 at lower temperatures. Beryllium condenses as gugiaite (Ca2BeSi2O7) in solid solution with melilite with a 50% condensation temperature of 1490 K. If an ideal solid solution of chrysoberyl (BeAl2O4) into spinel is assumed, most of the Be condenses into spinel, yielding a 50% condensation temperature of 1501 K. However, the difference in the crystal structures of spinel and chrysoberyl indicates that their solid solution may be non-ideal. At high temperatures the dominant B gases are BO, HBO, and HBO2, while NaBO2, KBO2, and LiBO2 are dominant at lower temperatures. Boron is less refractory than Be and is calculated to condense into solid solution with feldspar. The majority of B condenses as danburite (CaB2Si2O8) in solid solution with anorthite. At lower temperatures, when the feldspar composition is more albitic, the remaining B condenses as reedmergnerite (NaBSi3O8). The 50% condensation temperature of B is 964 K. The 50% condensation temperature of B is similar to that of Na and much higher than that of S. Therefore, normalized B abundances in chondrites are expected to correlate with Na abundances. Be is predicted to be concentrated in melilite, a conclusion which is consistent with the few measurements of Be concentrations in calcium aluminum-rich inclusions (CAIs). Boron is predicted to be concentrated in feldspar, but no analytical data are available to test this prediction."

  5. thanks! We love a good geek out.

    P.S. Christie’s auctioned off a 3×4" Sericho nugget last year. It looks like a space pineapple inside 🙂(note: they mistakenly call it an Admire nugget. The seller informed me that it’s actually a Sericho)

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