SUMMARY
The standard gravitational parameter (G*M) is measured with greater accuracy than the gravitational constant (G). Observations of planetary orbits around the Sun have established the Sun's standard gravitational parameter to 11 significant digits, while Earth's parameter is known to 9 or 10 significant digits. The challenge lies in isolating G from G*M, as G is only known to 4 or 5 significant digits, primarily due to limitations in measuring the Earth's mass accurately. Remote sensing projects, such as those conducted by NASA's GRACE mission, provide insights into the Earth's dimensions and composition but are limited to measuring G*Me.
PREREQUISITES
- Understanding of gravitational parameters and constants
- Familiarity with celestial mechanics and orbital dynamics
- Knowledge of remote sensing techniques in geophysics
- Basic principles of mass measurement and uncertainty analysis
NEXT STEPS
- Research the methods used in remote sensing projects like NASA's GRACE mission
- Study the implications of gravitational constant measurements on astrophysics
- Explore the relationship between G, M, and the standard gravitational parameter in detail
- Investigate the historical development of gravitational measurements and their accuracy
USEFUL FOR
Astronomers, geophysicists, and students of physics interested in gravitational measurements and their implications in celestial mechanics.