dv said:
Technetium and promethium have no isotopes that are long-lived on a geological timescale. When I were a lad they were considered purely synthetic, in an earthly context. (It has long been known that they can be produced in stars.)
In 1999, David Curtis of LANL used X-ray emissions from a uranium sample to determine that Tc-99 exists in association with uranium in amounts of around 1 in a trillion, as a product of natural fission. (Some have taken this as confirmation of results reported by a German team of Tacke, Noddack and Berg in 1925, which were not widely accepted at the time. Technetium is usually said to have been discovered in 1936 by the Italian researchers Perrier and Segre.) This would mean there are several tonnes of technetium in the crust, and hundreds of tonnes in the Earth altogether.
Promethium is also now known to exist naturally in the crust, again as a product of natural fission of uranium. It is much rarer than technetium, and it is thought there is about half a kilogram in the crust, and a few dozen kilograms in the Earth as a whole.
Nice, I hadn’t heard that. I had heard that plutonium and neptunium, once thought to be purely synthetic, are now known to exist is significant quantities in the Earth’s crust.
From memory, technetium is a natural product of nuclear fission, yes, you’ve said that. It is even be a bit more than that, because with a mass of 98 it’s actually one of the most commonly produced elements from the spontaneous fission of 235U and 238U. On the other hand, it’s not the most commonly produced element by the fission of 232Th and 233U whose (lower mass) products peak at a mass of 91-93. According to wikipedia, the half-life of 238U with respect to spontaneous fission is 8.4×10^15 years.
I had thought that promethium was common on Earth. I hadn’t even known that all its isotopes were radioactive. Let me check: “The most stable isotope of the element is promethium-145, which has a half-life of 17.7 years via electron capture”. Compare that with “Technetium-99 has a radioactive half-life of 212,000 years”. isotopes with mass 145 are almost the most common (higher mass) fission product of 239Pu, which is itself rare. Promethium is not the most common isotope produced by the spontaneous fission of 238U, but still, isotopes with a mass of 145 are produced in about 4% of fissions of 238U.
Aha, now I know why I thought promethium was common on Earth. According to wikipedia it had been thought that promethium was a decay product of natural niobium, which is common. This was only disproved in the year 2003.