by Mary Hrovat

When I was 17, I took an introductory course in physical geology at a community college. I was enchanted by the descriptions of the physical processes that created land forms, and also by the vocabulary: eskers and drumlins, barchan dunes, columnar basalt. I like to know how things form and what they’re called. My strongest memory of this class, though, centers on the final lecture. The professor put Earth and its landforms and minerals in a larger context. He told us about the life cycles of stars, which have produced most of the elements on Earth.
The central fact of the lecture was that the mass of a star is a key characteristic determining how long it exists and what happens as it ages. Stars are formed when gravity causes a portion of a gas cloud to collapse until its internal pressure, and thus its temperature, are high enough for nuclear fusion to begin. The energy released when, for example, two hydrogen nuclei fuse to form helium supports the mass of the star against the pull of gravity. A star’s life unfolds as a story of the equilibrium (or loss of equilibrium) between these two forces pulling inward and pushing outward. As one fuel source is depleted (for example, as hydrogen is converted to helium) other types of fusion occur in the core of the star using the new fuel source (and creating increasingly heavier elements). At the same time, hydrogen continues to fuse in a shell surrounding the core. Mature stars may have shells dominated by various elements undergoing different fusion reactions, although the available reactions depend on the mass of the star.
The professor probably described stars according to their type. I don’t remember if he mentioned the Hertzsprung–Russell diagram, although it seems likely that he would have. The HR diagram plots the luminosity of stars (the amount of light they emit) versus their temperature. When stars are plotted this way, most of them fall on a curve called the Main Sequence, which runs from hot blue stars to cool red stars along the sequence O-B-A-F-G-K-M. (In some HR diagrams, the stellar type or color is plotted on the horizontal axis as a proxy for temperature.) Stars remain on the Main Sequence as long as the gravitational and thermal forces are in equilibrium. The larger and hotter a star is, the shorter its time on the Main Sequence, because hotter stars consume their fuel more rapidly.
As they age and leave the Main Sequence, stars undergo different processes depending on their size. The universe is still too young for the very smallest stars to have exhausted their fuel, so they’re still on the Main Sequence. Stars with masses ranging from slightly less than that of the sun to 10 times the mass of the sun go through a red giant phase, ultimately undergoing core collapse and forming dense white dwarfs. Larger stars have more complicated end-of-life scenarios, typically exploding in supernovae and leaving behind superdense neutron stars or black holes. Some elements are created only in supernova explosions. Read more »


Risham Syed. The Heavy Weights, 2008.
Despite the fact that Newcomb’s paradox was discovered in 1960, I’ve been prompted to discuss it now for three reasons, the first being its inherent interest and counterintuitive conclusions. The two other factors are topical. One is a scheme put forth by Elon Musk in which he offered a small prize to people who publicly approved of the free speech and gun rights clauses in the Constitution. Doing so, he announced, would register them and make them eligible for a daily giveaway of a million dollars provided by him (an almost homeopathic fraction of his 400 billion dollar fortune). The other topic is the rapid rise in AI’s abilities, especially in AGI (Artificial General Intelligence). Soon enough it will be able, somewhat reliably, to predict our behaviors, at least in some contexts.




My 2024 ends with a ceremony of sorts. On December 31st, I’m sitting in a hotel in Salt Lake City an hour before midnight. I’m looking at my phone and I have it opened to Tinder.
I read the opening of Peter Handke’s A Sorrow Beyond Dreams and immediately thought of Camus’ The Stranger. Here is how Handke begins:

Many environmentalists find the climate change policy problem baffling. The core mechanism of how certain molecules create a greenhouse warming effect on the earth is extremely clear (and has been known for
Since 2010
Philip Graham: 
When I think about AI, I think about poor Queen Elizabeth.
Sughra Raza. Self Portrait, Kigali, January 17, 2016.