SUMMARY
Gravitational lensing is a phenomenon where light from a distant quasar is bent by the gravitational field of an intervening galaxy, resulting in the formation of an Einstein ring. This effect occurs because light travels slower near massive objects, similar to how light behaves when passing through a convex glass lens. The first observation of gravitational lensing was made during a solar eclipse, allowing astronomers to see distorted constellations behind the sun. For further understanding, refer to the Wikipedia article on gravitational lensing and explore related concepts such as gravitational microlensing.
PREREQUISITES
- Understanding of basic astrophysics concepts
- Familiarity with the principles of light propagation
- Knowledge of gravitational effects on light
- Awareness of astronomical observation techniques
NEXT STEPS
- Read the Wikipedia article on gravitational lensing
- Explore gravitational microlensing and its applications in extrasolar planet detection
- Investigate the historical observations of gravitational lensing during solar eclipses
- Examine simulations of gravitational lensing effects
USEFUL FOR
Astronomy enthusiasts, astrophysicists, and students interested in the effects of gravity on light and the study of distant celestial objects.