Estimates of the change rate of solar mass and gravitational constant based on the dynamics of the Solar System
arXiv:2201.09804 · doi:10.1051/0004-6361/202039893
Abstract
The estimate of the change rate of the solar gravitational parameter is obtained from processing modern positional observations of planets and spacecraft. Observations were processed and parameters were determined basing on the numerical planetary ephemeris EPM2019. The obtained annual decrease in solar mass accounts for the loss through radiation , through the outgoing solar wind , and for the material falling on the Sun . The estimated relative value is within per year. The following range for the change rate of the gravitational constant was obtained: per year ). The new result reduces the interval for the change in and narrows the limits of possible deviations for alternative gravitational theories from general relativity.
References in corpus (10)
- The Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere
- Electrons in the Young Solar Wind: First Results from the Parker Solar Probe
- The Near-Sun Dust Environment: Initial Observations from Parker Solar Probe
- A Statistical Study of CME Properties and of the Correlation Between Flares and CMEs over Solar Cycles 23 and 24
- Relating streamer flows to density and magnetic structures at the Parker Solar Probe
- Mass Loss via Solar Wind and Coronal Mass Ejections During Solar Cycle 23 and 24
- Strong Erosion-Driven Nongravitational Effects in Orbital Motions of the Kreutz Sungrazing System's Dwarf Comets
- Readdressing the UV solar variability with SATIRE-S: non-LTE effects
- Comet C/2017 S3 (PanSTARRS): Outbursts and Disintegration
- Preperihelion Outbursts and Disintegration of Comet C/2017 S3 (Pan-STARRS)