Gravity Effects General Relativity Quiz: Test Your Knowledge

Concept: time dilation in gravity. In stronger gravity, clocks run more slowly relative to far-away clocks. This is a real effect measured in experiments and technology.

Concept: gravity slows clocks. Gravity affects the rate at which time passes. The difference is small on Earth but measurable with precise clocks.

Concept: lensing. Light follows curved spacetime, so its path can bend near mass. This can create distorted or multiple images of distant objects.

Concept: gravitational waves (intro). GR predicts that accelerating masses can create spacetime ripples. These waves carry energy and can be detected with sensitive instruments.

Concept: orbit as free fall. Orbit can be seen as continuous free fall around a mass. The curved geometry makes the 'straightest path' loop around.

Concept: support force. The sensation of weight comes from the ground preventing free fall. In free fall, that support force disappears, so you feel weightless.

Concept: image distortion. Lensing can stretch, arc, or duplicate images. The amount depends on mass distribution along the line of sight.

Concept: relativity in navigation. GPS needs extremely accurate timing. Relativistic time differences accumulate and must be corrected to prevent location errors.

Concept: free fall as inertial motion. In GR, free fall follows a geodesic, like inertial motion in curved spacetime. You feel weightless because there is no support force.

Concept: equivalence principle. Locally, free fall can mimic an inertial frame with no gravity felt. This idea helped guide Einstein toward a geometric theory.

Concept: photons follow spacetime. Light travels along null geodesics in curved spacetime. Curvature affects the path without needing rest mass.

Concept: einstein ring. When alignment is very good, lensing can produce a ring. It’s a striking sign of gravity bending light.

Concept: geometry connection. GR connects physical content (mass-energy) to geometry. Geometry then influences motion and light paths.

Concept: when GR matters. In strong fields (near massive objects) or precision timing/orbits, GR effects become noticeable. Newton’s model is often an excellent approximation otherwise.

Concept: wave sources. Strong gravitational waves come from huge masses moving rapidly, especially compact binaries. Everyday events are far too weak to detect this way.

Concept: key GR consequences. GR predicts time dilation, lensing, and waves. Temperature can relate to energy, but 'temperature bends space directly' is not the usual simple statement.

Concept: correspondence. A new theory must recover old successful results in the right limit. GR does this for everyday gravitational conditions.

Concept: mass mapping with lensing. Lensing depends on total mass, including mass that doesn’t emit light. That makes it useful for studying invisible matter distributions.

Concept: gravity responds to mass-energy. Lensing reveals how mass is spread out. This works even when the mass is dark or hard to see directly.

Concept: mercury’s perihelion (qualitative). GR predicts a tiny extra precession in mercury’s orbit beyond Newtonian effects. This was a classic early test of the theory.