SUMMARY
The Galactic Center of the Milky Way is located approximately 25,900 light years from the solar system and has a mass of 4.31 million solar masses. The Sun does not follow a Keplerian orbit around this center due to the significant mass of the galaxy, which totals around 580 billion solar masses. Instead, the Sun's orbit is influenced by the combined gravitational effects of the entire galaxy. Key vectors of interest include the velocity of the Sun and its radius from the singularity, both measured in the reference frame of the supermassive black hole at the Galactic Center.
PREREQUISITES
- Understanding of gravitational dynamics in astrophysics
- Familiarity with orbital mechanics and non-Keplerian orbits
- Knowledge of vector mathematics in a three-dimensional space
- Basic concepts of galactic structure and mass distribution
NEXT STEPS
- Research the dynamics of non-Keplerian orbits in astrophysics
- Study the gravitational effects of mass distribution in galaxies
- Learn about the methods for calculating orbital vectors in a multi-body system
- Explore the implications of the Milky Way's mass on stellar orbits
USEFUL FOR
Astronomers, astrophysicists, and students of celestial mechanics interested in the dynamics of the Milky Way Galaxy and the behavior of stars in its gravitational field.