SUMMARY
Photons from stars, such as the sun, do exert a radiation pressure that can theoretically influence the flight paths of nearby celestial bodies, including asteroids. However, the impact of these photons on the orbits of other stars is negligible due to the immense mass of stars and the low intensity of light they emit. Dark matter and dark energy do not factor into these interactions, as they operate on vastly larger cosmic scales. Historical discussions, such as those by physicist Leonard Susskind, highlight that while radiation pressure was significant in the early universe, its effects have diminished considerably since then.
PREREQUISITES
- Understanding of radiation pressure in astrophysics
- Familiarity with dark matter and dark energy concepts
- Basic knowledge of stellar dynamics
- Awareness of cosmological expansion theories
NEXT STEPS
- Research the effects of radiation pressure on celestial bodies
- Study the role of dark matter and dark energy in cosmology
- Explore stellar dynamics and their influence on star systems
- Watch Leonard Susskind's lectures on cosmological expansion and radiation pressure
USEFUL FOR
Astronomers, astrophysicists, students of cosmology, and anyone interested in the interactions between stars and the fundamental forces of the universe.