Back Bones Are Forever Save as PDF
Chapters (41)
  1. Acknowledgments
  2. Chapter 1
  3. Chapter 2
  4. Chapter 3
  5. Chapter 4
  6. Chapter 5
  7. Chapter 6
  8. Chapter 7
  9. Chapter 8
  10. Chapter 9
  11. Chapter 10
  12. Chapter 11
  13. Chapter 12
  14. Chapter 13
  15. Chapter 14
  16. Chapter 15
  17. Chapter 16
  18. Chapter 17
  19. Chapter 18
  20. Chapter 19
  21. Chapter 20
  22. Chapter 21
  23. Chapter 22
  24. Chapter 23
  25. Chapter 24
  26. Chapter 25
  27. Chapter 26
  28. Chapter 27
  29. Chapter 28
  30. Chapter 29
  31. Chapter 30
  32. Chapter 31
  33. Chapter 32
  34. Chapter 33
  35. Chapter 34
  36. Chapter 35
  37. Chapter 36
  38. Chapter 37
  39. Chapter 38
  40. Chapter 39
  41. Chapter 40

Before booting my laptop, I knew that diamonds are carbon transformed by extreme heat and pressure into the hardest, clearest mineral on earth. That because of their rigid tetrahedral molecular structure—a triangular pyramid with four faces—a diamond can be cut only by another diamond or a laser.

I knew that the sparkly little rocks are pricey as hell. And that they create an eyeful of bling.

That was about it.

Every thirty minutes I’d interrupt my research to phone Katy. Each time her phone would roll to voice mail. Uneasy, I’d dive back onto the Internet.

In between dialing, I learned the following.

It takes forty-four to fifty kilobars of pressure at a minimum of a thousand degrees Celsius to change carbon into diamond. I understood the temperature but wasn’t sure the exact nature of a kilobar.

The appropriate combo of heating and crushing existed a few billion years ago at depths of eighty to a hundred and twenty-five miles in rock formations called cratons, dense old slabs of continental plate.

Later, underground volcanoes sent magma—or molten rock—minerals, rock fragments, and occasionally diamonds bubbling up through the cratons. The mixture expanded and cooled along the way to form either carrot-shaped pipes to the surface, or wide flat underground structures called dikes. It then solidified into rock called kimberlite.

Most diamondiferous kimberlites are associated with cratons from the Archean era, an early part of the Precambrian, when the earth was much hotter than today. Much hotter. Many kimberlite pipes lie underneath shallow lakes formed in inactive volcanic craters called calderas.

So. To score diamonds, you locate a pipe rising from a really old craton. Piece of cake, right? Wrong. The buggers are incredibly hard to find.

That’s where Chuck Fipke and Stu Blusson came in. Both knew that the Slave craton, which underlies the Northwest Territories from Great Slave Lake in the south to Coronation Gulf on the Arctic Ocean, is one of the oldest rock formations on earth. And they developed an effective technique to explore it.

Fipke understood the significance of indicator minerals, the traveling companions of diamonds. Those in kimberlite include calcium carbonate, olivine, garnet, phlogopite, pyroxene, serpentine, upper mantle rock, and a variety of trace minerals. Fipke focused on the trifecta of chromite, ilmenite, and high-chrome, low-calcium G10 garnets.

Blusson understood the significance of glacial movement during the last ice age. He reasoned that, after eroding a kimberlite pipe, a retreating glacier would leave a debris path containing diamond indicator minerals. Track the path to its source, he argued, and you’ll find the pipe.

Fipke and Blusson spent a decade scouring the tundra, mapping, surveying, coring, and collecting when temperatures were bearable, analyzing samples in their lab when the weather was too harsh. Everyone in the mining world thought they were nuts.