Fiveable

🪐Intro to Astronomy Unit 24 Review

QR code for Intro to Astronomy practice questions

24.1 Introducing General Relativity

🪐Intro to Astronomy
Unit 24 Review

24.1 Introducing General Relativity

Written by the Fiveable Content Team • Last updated September 2025
Written by the Fiveable Content Team • Last updated September 2025
🪐Intro to Astronomy
Unit & Topic Study Guides

Einstein's theory of general relativity revolutionized our understanding of gravity. It describes gravity as a result of spacetime curvature caused by mass and energy, rather than a force between objects. This groundbreaking idea transformed physics and astronomy.

General relativity explains phenomena that Newtonian physics couldn't, like Mercury's orbit. It predicts mind-bending concepts like black holes, gravitational waves, and time dilation. These ideas continue to shape our view of the universe and inspire new discoveries.

Principles and Implications of General Relativity

Principles of general relativity

  • General relativity is Einstein's theory of gravity that extends special relativity to include gravitational effects
  • Describes gravity as a consequence of the curvature of spacetime caused by the presence of mass and energy
  • Principle of equivalence states that gravitational and inertial mass are equivalent
    • Objects in freefall follow geodesics (shortest paths) in curved spacetime (astronauts in orbit)
  • Principle of general covariance states that the laws of physics are the same in all reference frames
    • Effects of gravity can be described by the curvature of spacetime (Earth orbiting the Sun)

Newtonian vs Einsteinian gravity

  • Newtonian gravity describes gravity as an instantaneous force between objects with mass using Newton's law of universal gravitation $F = G \frac{m_1 m_2}{r^2}$
    • Space and time are absolute and independent (falling apple)
  • Einsteinian gravity (general relativity) describes gravity as a consequence of the curvature of spacetime caused by mass and energy
    • Spacetime is a four-dimensional continuum of three spatial dimensions and one time dimension (fabric of the universe)
    • Massive objects curve spacetime, and objects follow the straightest possible path (geodesic) in this curved spacetime (planets orbiting the Sun)
  • Newtonian gravity is an approximation that works well for weak fields and low velocities, while general relativity is more accurate in strong fields and high velocities (Mercury's orbit)

Equivalence of gravity and acceleration

  • Principle of equivalence states that gravitational and inertial mass are equivalent
    • Inertial mass measures an object's resistance to acceleration (pushing a car)
    • Gravitational mass measures an object's response to a gravitational field (weight on Earth)
  • An observer in a closed elevator cannot distinguish between being at rest in a gravitational field and being accelerated in the absence of gravity (Einstein's "elevator thought experiment")
  • Gravity and acceleration are indistinguishable within a local reference frame
    1. A person in freefall experiences weightlessness as if there were no gravity (skydiving)
    2. An accelerating observer experiences a force indistinguishable from gravity (rocket launch)

General relativity in black holes

  • Black holes are regions of spacetime where the gravitational pull is so strong that nothing, not even light, can escape once it crosses the event horizon
    • Event horizon is the boundary of a black hole beyond which the escape velocity exceeds the speed of light (point of no return)
  • Black holes form when massive stars (> 8 solar masses) exhaust their nuclear fuel and collapse under their own gravity until a singularity forms with infinite density and zero volume
  • Black holes are characterized by mass, charge, and angular momentum
    • Schwarzschild radius is the event horizon radius for a non-rotating, uncharged black hole, given by $R_s = \frac{2GM}{c^2}$
  • Gravitational time dilation causes time to pass more slowly near a black hole due to the intense gravitational field (Interstellar movie)
  • Hawking radiation is predicted to be emitted from black holes due to quantum effects near the event horizon, causing them to slowly evaporate over time (smaller ones evaporate faster)

Mathematical foundations and predictions of general relativity

  • Albert Einstein developed general relativity using tensor mathematics to describe the relationship between spacetime curvature and the distribution of matter and energy
  • The theory predicts the existence of gravitational waves, which are ripples in spacetime caused by accelerating massive objects
  • Spacetime curvature explains how gravity affects the path of light and massive objects, leading to phenomena such as gravitational lensing and time dilation