To this day we don't have a picture of our home galaxy, from the outside. This is because it is so large that sending a probe far enough to grab the selfie would take far too long. If we can't see it from the outside then how do we know its size and our location within it?⬇️1/6
Harlow Shapley, an American astronomer (1885-1972), began by studying the distribution of globular clusters (dense collections of ancient stars) in the sky. He noted that these clusters were not uniformly distributed, but instead were more concentrated in one part of the sky⬇️2/
Shapley used variable stars within these clusters to estimate their distances. These variable stars have an intrinsic (actual) brightness and apparent (what we see) brightness. By comparing the intrinsic and apparent brightness, Shapley estimated how far away they were.⬇️3/6
Shapley found that the clusters were distributed roughly in a sphere whose center lay in the direction of Sagittarius, far from the Sun's location. Shapley inferred this to be the center of the galaxy.⬇️4/6
This was a revolutionary finding, as it contradicted the long-standing belief that our Sun was at the center of the Milky Way. Instead, Shapley's measurements placed the Sun about 50,000 light years from the galactic center, or about two-thirds of the way out from the center⬇️5/
Today, with more precise measurements, the accepted distance from the Sun to the center of the Milky Way is about 26,000 light-years. His estimate was a little off, but his conclusion that the Sun was not at the center of the galaxy was groundbreaking and fundamentally correct.
Be sure to check out my previous tweet on how long it would take to travel to the center of the galaxy and back if traveling near the speed of light!
This Physicist Friday goes to Lise Meitner. Meitner (1878-1968) was an Austrian-Swedish physicist known for her role in the discovery of nuclear fission. Working with chemist Otto Hahn, they bombarded uranium atoms with neutrons, splitting the nucleus and detecting barium. ⬇️1/4
Meitner, along with her nephew Otto Frisch, interpreted the results using Einstein's E=mc^2 to explain the observed energy release. They realized that the splitting of the atomic nucleus into smaller nuclei released a significant amount of energy.⬇️2/4
This insight was crucial in understanding the potential applications of nuclear fission, such as nuclear power generation and atomic weapons.⬇️3/4
Snake venoms are complex mixtures of proteins, peptides, and other molecules that have evolved for various purposes, such as prey immobilization and digestion. This video demonstrates how procoagulants in some snake venom promote blood clotting. How does this work? See Next⬇️1/3
These procoagulants directly interact with proteins involved in the blood clotting process. Often these are proteases (cleave proteins) which ultimately lead to the rapid formation of fibrin, the protein mesh that stabilizes blood clots. ⬇️2/3
Retrograde motion is the apparent backwards motion that planets make as they travel across the sky.
Prior to the sun-centered model of the solar system, it was believed planets made loopty loops as they circled the earth.
The Copernican model explains this motion w/o loops. (1/2)