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Jon Larsen - In Search of Stardust: Amazing Micrometeorites and Their Terrestrial Imposters

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In Search of Stardust: Amazing Micrometeorites and Their Terrestrial Imposters: summary, description and annotation

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Tiny pieces of space rock called micrometeorites are everywhere on Earth. In Search of Stardust shows you how to find them!

The solar system is a dusty place. Every day approximately 100 metric tons of cosmic dust collides with Earth, mainly in the form of micrometeorites. Most of these mineral particles (iron, nickel, etc.) are smaller than grains of sand, and they are falling down on us all the time and all over the globe. Still, little is known about these exotic extraterrestrials.

In Search of Stardust is the first comprehensive popular science book about micrometeorites. Its also a photo documentary comprising more than 1,500 previously unpublished images: the first atlas of micrometeorites, hundreds of which are depicted here in high-resolution color microscopic photography and in scanning electron microscope imagery.

Author Jon Larsen shows readers how and where to look for micrometeorites, explains the history of micrometeoritics, and offers chapters about micrometeorite formation, classification, and analysis. Thanks to Larsens work, for the first time it is now possible for anyone to find these amazing tiny stones from space.

For more than a century it was believed these incredible space objects could be found only in pristine, unsullied environs like Antarctica and ocean floors. Larsen became the first to break the code and find micrometeorites in populated areas -- in fact, they can be found in the nearest rain gutter. In the book Larsen explains how anyone with a bit of inexpensive equipment can find their own micrometeorites.

It was recently discovered that King Tuts dagger was forged from a chunk of a meteorite. What else is made of extraterrestrial rock? Join the hunt!

Jon Larsen: author's other books


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A fine-grained turtleback micrometeorite - photo 1
A fine-grained turtleback micrometeorite with a nickeliron core in the front - photo 2
A fine-grained turtleback micrometeorite with a nickeliron core in the front - photo 3
A fine-grained turtleback micrometeorite with a nickeliron core in the front - photo 4

A fine-grained turtleback micrometeorite with a nickel/iron core in the front, revealed by the ablation during the atmospheric flight.

Preface

Is it possible to find micrometeorites in populated areas?

The question has been raised for nearly a century, and despite numerous attempts to find them, the answer up to this day has been a very short no. This was confirmed by the top researchers in the field when my project started up.

Meanwhile our knowledge about these amazing stones has gradually increased. There is a continuous evolutionary line in the research on micrometeorites, from the early pioneers John Murray and Adolf Erik Nordenskild to Lucien Rudaux and Harvey H. Nininger. With Donald E. Brownlee and Michel Maurette in the 60s micrometeoritics became real science. During the past two decades this research has accelerated, thanks to, among others, Susan Taylor who extracted micrometeorites from the South Pole water well, and Matthew Genge who figured out the splendid classificiation. Today there is a growing literature about micrometeorites, but still the answer to the initial question has been no.

Micrometeorites have mainly been found in the Antarctic, but also to some extent in prehistoric sediments, remote deserts, and in glaciersplaces that are clear of the confusing anthropogenic influence. In populated areas a wall of contamination has been considered insurmountable.

It is therefore with pride and joy I can report here about a project of systematic examination of all sorts of anthropogenic and naturally occurring spherules in an empirical search for micrometeorites in populated areas. This research has resulted in a new collection of pristine cosmic spherules. The findings have been analysed at several different institutions including electron microprobe verification at the Natural History Museum in London. This new collection of urban micrometeorites is presented here for the first time.

Without knowing what micro-meteorites really look like, it would not have been possible to find them, and it is a pleasure also to present here for the very first time a morphological study of micrometeorites in high-resolution color photography. This has become possible thanks to new micro photo techniques developed together with my brilliant colleague Jan Braly Kihlesine qua non!

Furthermore, this research would have been unsuccessful if not for the invaluable support from the Laboratory for Electron Microscopy in Bergen (UiB), Egil Severin Erichsen, Irene Heggstad, and Gunnar Slen, the SEM lab at the University in Oslo (UiO) Berit Lken Berg and Henning Dypvik and the Natural History Museum (NHM) in Oslo, Rune Selbekk and Harald Folvikwarm thanks to these splendid fellow researchers. But above all very special thanks to Matthew Genge at Imperial College, London, who not only verified my first micro-meteorites but also has been my mentor pro bono, and who initiated the crucial electron microprobe analysis of the micrometeorites at the NHM in London.

Jon Larsen

SEM images shown have a catalog number with a hyphen These are from the South - photo 5

SEM images shown have a catalog number with a hyphen. These are from the South Pole Water Well (SPWW), the Antarctic reference collection of micrometeorites, SEM images by Emily Schaller, published with kind permission from Susan Taylor (US Army Cold Regions Research, CRR).

The Stardust Project

Micrometeorites belong to the oldest matter there is: mineral remnants from before the planets were formed. They may even contain stardust older than the sun, particles which have traveled farther than anything else on Earth. We are just beginning to explore these alien stones, yet they are everywhere around us.

After an incident in 2009 when a micrometeorite literally landed on my table, I wanted to find out more about them, and became intrigued by the contradiction between the global influx rate (see in this book, human tools and activities create spherules not unlike micrometeorites.

To pick out one extraterrestrial particle among billions of others requires - photo 6

To pick out one extraterrestrial particle among billions of others requires knowledge both about what to look for and what to disregard, and initially I was in the dark. The published images of micrometeorites from the Antarctic were mainly black/white SEM sections (shown ), which are poor representations of what micrometeorites look like. And with regard to the confusing contaminants there was a plentitude of speculation, but very little empirical data. There has been research in this field earlier, from NASAs comparative analysis of cosmic and industrial spherules in the 1960s to contemporary studies of road dust in India and Hungary, but these have been fragmentary, and concluded that separation of micrometeorites in populated areas is not possible. On the other hand there have been several physics-at-home experiments searching for micrometeorites at downspouts from roofs gutters, but none of these have yet resulted in verification of extraterrestrial particles.

In the spring of 2010 I started my systematic research on dust samples from populated areas. I initially looked at skywards-facing hard surfaces where particles could accumulate over time, like roads, roofs, parking lots, and industrial areas, and then graduated to look in other cities, countries, mountains, beach sand, desertseverywhere. Now, six years later, I can look back upon nearly 1,000 field searches in nearly 50 countries, all continents represented. The samples were examined in a Zeiss binocular microscope, and interesting particles were picked out, photographed with a USB microscope, and stored in the archive. I established a photo database (now containing photos of more than 40,000 individual objects), kept an illustrated journal, and tried to look for patterns (factor analysis) while I put my complete trust in pure empiricism. The Facebook page Project Stardust was established to share the results.

To begin with the different types of anthropogenic and naturally occurring terrestrial spherules seemed infinite and chaotic, but with time I gradually started to recognise the most common ones. There are surprisingly small variations in the types of spherules found in comparable environments around the globe, and the 25 types presented in this book represent the most of all the spherules found anywhere. The micrometeorites are rare and evenly distributed, so an abundance of one type of particles found locally is one of the indications of terrestrial origin.

The breakthrough in my research came February 4, 2015, when Matthew Genge verified the first micrometeorite, a barred olivine beauty with dendritic magnetite crystals sprinkled all over the surface. The stone was only 0.27 mm, and was found at Brevik in Frogn, Akershus, Norway.

At last I knew what to look for, started immediately to search for similar stones, and found them. Within the first season I had a collection of more than 500 pristine micrometeorites, all the most common types from the classification represented.

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