Effect of fission products on tensile strength of UO<sub>2</sub> Σ3 (111)/[1<math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg" class="math"><mover accent="true"><mn>1</mn><mo stretchy="true">¯</mo></mover></math>0] and UO<sub>2</sub> Σ11 (1<math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg" class="math"><mover accent="true"><mn>1</mn><mo stretchy="true">¯</mo></mover></math>3)/[110] grain boundaries from first-principles study

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As with crypto-currency, records of who owns what are stored on a ledger that is maintained by thousands of computers around the world. These records can’t be forged because the whole system operates on an open-source network.

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The atmosphere is a ruthless incinerator, and, no matter how the ISS comes down, most of it would be vaporized. But there’s still that chunk of station that could survive reentry. In the best case, where we’re prepared, air traffic controllers and maritime authorities can issue alerts. The station will shed pieces into the sky, and Australians might get a nice view before things kerplunk into the sea. Then the remains of this historic feat of human engineering will sink to the ocean floor, another carcass left to the algae and the microplastics.