- Carl Sagan
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So we were undoubtedly all thrilled by the long-awaited James Webb Space Telescope's flawless Christmas morning launch. As a hardcore space fan, when I heard that liftoff from French Guiana would occur around 6am my time, I dutifully set my alarm for the early morning countdown. Unfortunately, the timing was such that I'd gotten my COVID-19 vaccine booster the day before; I hadn't thought much of it since my first two shots produced minimal side-effects, but man alive did I feel horrendous by the time that 6am alarm went off! As JWST took flight, the nausea and full-body soreness combined with my sleep deprivation had me almost ready to hurl. But in the end, both boosters - Ariane 5 and Moderna - were more than worth it! (heh heh see what I did there??)
The Ariane 5 carrying JWST, moments after liftoff |
My unfortunate timing notwithstanding, I've actually had this article idea in mind for months now, ever since NASA Earth Observatory published this great article about where the beryllium for those 18 super-shiny gold hexagonal mirrors on JWST came from. As it turns out, the vast majority of the world's beryllium comes from Spor Mountain in Utah, locked away in minerals that formed 25 million years ago from the lava of a volcanic eruption. NASA has long used beryllium from Spor Mountain for its missions; for JWST, beryllium was perfect because it's 1/3 lighter than aluminum and 6 times stiffer than steel, even under extreme temperatures, so the mirrors can withstand any collisions with micrometeoroids
From mine to mirror, the beryllium in JWST's mirrors has undergone quite a transformation! |
But I wanted to go one level deeper: how did all the beryllium at Spor Mountain get there in the first place, or any of the beryllium on Earth for that matter? During my elective astronomy classes in college, I really enjoyed the unit on nucleosynthesis (how all the various elements get produced in the Universe), and I remembered that beryllium is a pretty strange edge case…
If you were to take a look at the periodic table of elements and make a wild guess as to the relative abundance of each element in the Universe, you'd probably end up with a result that has lighter elements being way more abundant than those weird heavy elements like bismuth or molybdenum. And you'd basically be right, especially if you knew that hydrogen and helium were the two elements largely produced by default from the Big Bang, and that stars are almost entirely made up of! Looking at the figure below plotting relative abundance in the Universe as a function of atomic number, it's a pretty clear trend… EXCEPT for three elements: lithium, beryllium, and boron. Why is that??
Diagram of the triple-alpha process. In the moment the Be-8 nucleus is formed, another He-4 nucleus better come along and slam into it immediately! Otherwise it'll decay right back to He-4 |
Simple diagram of boron spallation forming lithium and helium |
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