Dubrovnik: A Lumberjack Meteorite from the land of Oak Forests

Updated: Martin Horejsi’s Meteorite Books Website 

A February 1951 Witnessed Fall: Dubrovnik, Croatia

Dubrovnik: A Lumberjack Meteorite

from the land of Oak Forests

Dubrovnnik meteoirte

Resting on a one centimeter cube, it is easy to see this sample of Dubrovnik is not large. But according to the distribution listed in the Catalogue of Meteorites, this piece is the seventh largest in any collection anywhere. However, depending on the numbers you trust, approximately 94% of the Dubrovnik stone is still intact as the main mass.

Until most of the trees were cut down and used to build ships, the city of Dubrovnik was not only surrounded by ancient fortified walls, but also surrounded by trees. Even the name Dubrovnik is the Proto-Slavic word for oak forests. Yet there had to be at least one tree still standing February 20, 1951 when an L3-6 polymict brecciated chondrite fell from space at about 2:00 in the afternoon because it hit a tree. The single 1.9kg stone was recovered after burying itself “several feet” in the ground.

According to Yokoyama and others, Meteorites of regolith breccia preserve the records of formation and evolution of surface material on the asteroids. With longer residence time, the surface material changes its textural and mineralogical properties, so called “space weathering”, mainly due to cosmic dust bombardment and solar-wind implantation.

In addition, cosmogenic nuclides are produced via spallation reactions between in-coming cosmic rays and the surface material. Therefore, it is expected that the meteorites that have experienced heavier space weathering contain higher concentrations of implanted solar winds and cosmogenic nuclides.”


Dubrovnnik meteoirte

Loads of activity in here! As you’ll read below, there is so much going on inside Dubrovnik that a soap opera of events transpired to bring together the eye candy others call an L3-6 polymict breccia.

Croatia claims only four meteorites recovered from within its borders. All are falls, but in an interesting twist of synchronicity, exactly 200 years after the first known Croatian meteorite named Hraschina fell, the most recent Croatian meteorite fell and christened Dubrovnik.
Immediately preceding the Dubrovnik meteorite’s arrival to earth, “a noise like a thunderclap was heard.” I can only imagine the wondrous sound the compression waves made as they roiled around inside the walled city of Dubrovnik. However, the combination of the historical turmoil of the region and the recently deceased World War 2 might have made a meteorite fall not the first thing the citizens of the area thought of upon hearing the boom.


Dubrovnnik meteoirte

Sometimes small specimens completely misrepresent the overall nature of a whole meteorite. In this case, my sample provides just enough tasty snippets of geologic activity to provide loads of enticing hints about how beautiful a large piece would be. 

Colors, regions, shapes, lines, darks, lights; the story is endless. In this view alone, I can see the type-three chondrules on the left bumping up against the jagged fragmentation of the type-six breccia on the right. And the upper portion of the center, its anyone’s guess. The tides of matrix flow light and dark, the grain size sifts between the microscopic and not.

In the inverted and brightened picture below, the wild west nature of this stone is obvious.

Dubrovnnik meteoirte


In an article titled Petrology, Mineralogy, And Noble Gas Composition Of The Dubrovnik L Chondrite Breccia by Yokoyama, et. al., a detailed inspection of the cosmochemistry of Dubrovnik is presented resulting in a telling story of Dubrovnik’s cosmic history. Without adding much embellishment, the story could read better than a dime store novel complete with car chases and love stories. Enough talk. Here’s the text…
“Based on the results of a series of analysis, we infer the formation and evolution history of the surface of Dubrovnik parent asteroid. First, the whites formed in the interior of the parent body during prolonged thermal metamorphism at around 900. Then a large impact destroyed the parent body which excavated the deeper-seated white to the asteroid surface and, at the same time, might have disturbed the composition of Fe-Ni metals due to impact heating.

 

The dark material was produced with time on the surface by space weathering. The whites and the dark were mixed due to repeated impacts. Mg-rich pyroxene in the dark would have incorporated from least metamorphosed portions of the surface, or as in-coming meteoroids during the impact-induced mixing processes, and the black melt pocket was also produced due to local shock heating. During impacts, the dark and the whites consolidated together to form a chondritic regolith breccia. After consolidation, there is no heating enough to degas noble gases.”


Dubrovnnik meteoirte

The scars of a childhood filled with abuse are visible as cemented fragments; the shattered attempts at normalcy. 

Although I feel bad that Dubrovnik likely lived in fear of more abuse, I hope our excitement over its torrid past helps, even in some small way, to alleviate some of the pain it experienced in the cold, dark, loneliness of space.


The collection distribution of the Dubrovnik according to the Catalogue of Meteorites provides a different picture on the small total known weight of this locality. Of the 1900 grams recovered from the fall, 1790 grams are in the Dubrovnik Museum in the form of a single main mass. After the 204g in the Vienna Museum (ignoring the discrepancy in TKW), it goes downhill rapidly from there. 39.3g are listed as in the AMNH in New York; 23.5g in the Field Museum in Chicago; another 23.5g in London; 22g in the collection of the University of New Mexico; five grams in Moscow; and 3.8g in the DuPont collection.

 

Although many of the specimens of Dubrovnik listed in other collections are small, I suspect that many samples have a sizable helping of crust just as mine does.

Dubrovnnik meteoirte

Since Dubrovnik fell as a single stone, most of the pieces initially removed from the main mass will be heavily crusted. The lack of cut surfaces supports the contention that this specimen was broken off either the main stone, or a fragment from a larger sample. 

Since corners and protrusions are the easiest to forcibly remove, two things happen. First, the remaining main mass becomes more spherical with Ensisheim being the prime example. And second, the removed pieces often hold the corners and other interesting undulations from the initial form of the meteorite.

A number of years ago, as I was negotiating an exchange with another collector, a Dubrovnik blip started moving on the radar screen. Although not terribly old, this youngster’s earth age was easily overshadowed by the desirable collection qualities including the low total weight and low distribution of Dubrovnik, the interesting fall location and circumstances, the museum and collection documentation, the excellent crust, and, of course, its coveted classification.


Dubrovnnik meteoirte

Dubrovnnik meteoirte

Eugene and Sharon Cisneros who run the Mineralogical Research Company in San Jose, California. I’ve bought from them over the years and always enjoyed their old-school (in a very good way) professionalism. None of the flash and bloated showmanship so common today. Just quality, service, and honesty. 

I’ve known Jim Schwade for years so it feels odd to consider a card from his collection as treasured piece of meteorite collection history. But it is.


The specimen label that came with this piece Dubrovnik is from the Natural History Museum in Zagreb, Croatia. Back in 1989 I spent some time in Zagreb. What a wonderful place filled with kind people. I have not been back since the Croatian War of Independence, but that region of the world has moved back up on my list of places to visit again.

 

And when I again visit Croatia, I’ll be sure and stop by to say hello to the main mass of Dubrovnik.

Until next time….


The Accretion Desk welcomes all comments and feedback. accretiondesk@gmail.com


Tags:

About the Author

Martin Horejsi
Dr. Martin Horejsi is a Professor of Instructional Technology and Science Education at The University of Montana. A long-time meteorite collector and writer, before publishing his column The Accretion Desk in The Meteorite Times, he contributed often and wrote the column From The Strewnfields in Meteorite Magazine. Horejsi is currently a monthly columnist in The Science Teacher, a journal by the National Science Teachers Association. Horejsi specializes in the collection and study of historic witnessed fall meteorites with the older, smaller, and rarer the better. Although his meteorite collection once numbered over a thousand pieces with near that many different locations, several large trades and sales have streamlined the collection to about 250 locations with all but 10 being important witnessed falls. Many of the significant specimens in Horejsi's collection are historic witnessed falls that once occupied prominence in the meteorite collections of Robert A. Haag, James Schwade, and Michael Farmer. Other important specimens were acquired through institutional trades including those from The Smithsonian Institution, Arizona State University, and other universities.
Top