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|    Message 141,912 of 143,102    |
|    Bill Sloman to Martin Brown    |
|    Re: noi siamo noi    |
|    01 Jan 26 04:01:16    |
      From: bill.sloman@ieee.org              On 1/01/2026 12:31 am, Martin Brown wrote:       > On 31/12/2025 11:32, Jeroen Belleman wrote:       >> On 12/31/25 12:01, Martin Brown wrote:       >>> On 29/12/2025 16:04, john larkin wrote:       >>>>       >>>> Oh, I've worked with TOF atom probe spectroscopy and backscatter       >>>> analysis and analytical NMR and all sorts of exotic physics.       >>>> Physiscists need help with circuits.       >>>>       >>>> But a lot of the solar system has rocks with similar isotopic content.       >>>> Declaring a meteorite to be a chunk knocked of Mars is a real       >>>> hand-waver.       >>>       >>> Not really. The oxygen isotopic signature on Mars is different enough       >>> to recognise Mars rocks. Although that doesn't stop charlatans on       >>> eBay selling Mars meteorites that are just similar looking Earth rocks.       >>>       >>> Anyone with a stable isotope MS or a noble gas MS would be able to       >>> test the gasses in inclusions and see old Martian atmosphere if it is       >>> real.       >>       >> I suppose analysis methods are more refined these days, but in 1974 I       >> simulated a meteorite hit in a class mate's garden as a hoax. What I       >> did not anticipate is that everyone took this seriously. It was just a       >> piece of steel furnace slag, but even the Max Planck institute in       >> Germany refused to admit they'd been fooled.       >       > Back then they wouldn't have any easy way of testing it. That all       > changed in about 1990 when TOF ion probes and laser ablation mass       > spectrometry came of age. Before that you had to pound it to dust and       > dissolve in HF (not nice) then do some very fancy wet chemistry.              Not true. Back when I was an undergraduate I had to check out an X-ray       fluorescence scheme for detecting low levels of alumina (Al2O3) in       titanium dioxide (TiO2) for my summer job, in 1961. As a graduate       student I met Alan Walsh (in 1968) who pretty much invented atomic       absorbtion spectroscopy, where you sprayed the solution into a flame and       detected the absorbtion lines of specific elements in the flame.              Australia's plastic banknotes have holograms as a side effect his       efforts to make cheap plastic diffraction gratings to disperse the light       that had been through the flame.              Inorganic chemists took to physical methods early.              > I worked on software for the mass spectrometric rare earth element       > analysis of meteorites at one time (and on dating ancient rocks).              Mass spectrometers work, but you need big expensive precise machines to       sort out the isotopes of heavier elements (and I didn't work on them       until 1992, and then only briefly).              > The geologists get very excited about the Europium anomaly in them. That       > one species is a marker that varies enormously with the type of rock and       > the chemical environment when and where it was formed.       >       > https://en.wikipedia.org/wiki/Europium_anomaly       >       > I understand that it occurs when Europium is in an unusual oxidation       > state and is commonly seen in stony chondrites and moon rocks. I have       > seen a few close up in a glove box. I never had the chance to smell any.       > Keeping them clean under an inert dry atmosphere was a priority.       >       > Cute demo with a modern Nd magnet you can collect micrometeorites from       > the black gunge that accumulates in PVC gutters. Too small for the naked       > eye to see but obvious with even a basic toy microscope.       >       > https://www.quekett.org/resources/article-archive/bsw-2017/bsw       7-micrometeorites       >       > Some nice almost safe for modern H&S rules science demos on that site.              --       Bill Sloman, Sydney              --- SoupGate-DOS v1.05        * Origin: you cannot sedate... all the things you hate (1:229/2)    |
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