<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Angular Momentum on gdpark.blog</title><link>https://gdpark.blog/tags/angular-momentum/</link><description>Recent content in Angular Momentum on gdpark.blog</description><generator>Hugo</generator><language>en</language><lastBuildDate>Thu, 25 Jun 2015 00:00:00 +0000</lastBuildDate><atom:link href="https://gdpark.blog/tags/angular-momentum/index.xml" rel="self" type="application/rss+xml"/><item><title>The Orbit Equation via Energy Methods [Classical Mechanics I Studied #10]</title><link>https://gdpark.blog/posts/classical-mechanics-10-the-orbit-equation-via-energy-methods/</link><pubDate>Thu, 25 Jun 2015 00:00:00 +0000</pubDate><guid>https://gdpark.blog/posts/classical-mechanics-10-the-orbit-equation-via-energy-methods/</guid><description>We re-derive the orbital equation using energy conservation instead of angular momentum — plus a quick vibe check on why gravitational potential energy is negative.</description></item><item><title>Orbital Stability [Classical Mechanics I Studied #11]</title><link>https://gdpark.blog/posts/classical-mechanics-11-orbital-stability/</link><pubDate>Thu, 25 Jun 2015 00:00:00 +0000</pubDate><guid>https://gdpark.blog/posts/classical-mechanics-11-orbital-stability/</guid><description>Why does Earth just keep cruising in its orbit without getting knocked off track? Turns out there&amp;rsquo;s a sneaky spring constant hiding in the radial equation of motion!</description></item><item><title>Angular Momentum of a System of Particles [Classical Mechanics I Studied #15]</title><link>https://gdpark.blog/posts/classical-mechanics-15-angular-momentum-of-a-system-of-particles/</link><pubDate>Sat, 17 Jan 2015 00:00:00 +0000</pubDate><guid>https://gdpark.blog/posts/classical-mechanics-15-angular-momentum-of-a-system-of-particles/</guid><description>We decompose total angular momentum into an orbital piece (system as one lump at the CM) and a spin piece (particles wiggling around it) — and show why those cross terms vanish.</description></item><item><title>Rigid Body in Planar Motion [Classical Mechanics I Studied #20]</title><link>https://gdpark.blog/posts/classical-mechanics-20-rigid-body-in-planar-motion/</link><pubDate>Mon, 19 Jan 2015 00:00:00 +0000</pubDate><guid>https://gdpark.blog/posts/classical-mechanics-20-rigid-body-in-planar-motion/</guid><description>Fixed-axis rotation is so last chapter — now the axis itself moves, and we figure out exactly when that messy extra torque term thankfully drops to zero.</description></item><item><title>Euler's Equations of Motion for a Rigid Body [Classical Mechanics I Studied #24]</title><link>https://gdpark.blog/posts/classical-mechanics-24-euler-s-equations-of-motion-for-a-rigid-body/</link><pubDate>Thu, 22 Jan 2015 00:00:00 +0000</pubDate><guid>https://gdpark.blog/posts/classical-mechanics-24-euler-s-equations-of-motion-for-a-rigid-body/</guid><description>We finally dig into full-on 3D rigid body rotation — inertial frames, rotating frames, and how Euler&amp;rsquo;s equations of motion fall out of it all. lol.</description></item></channel></rss>