Construct Your Own Problem Consider a star moving in a circular orbit at the edge of a galaxy. Construct a problem in which you calculate the mass of that galaxy in kg and in multiples of the solar mass based on the velocity of the star and its distance from the center of the galaxy. Star4 lyEarthSunDiameter of orbitFigure 34.26 Distances to nearby stars are measured usingtriangulation, also called the parallax method. The angle ofline of sight to the star is measured at intervals six monthsapart, and the distance is calculated by using the known

The gravitational force between the two objects is given by: FG=GMGLM*R2…

Star 4 ly Earth Sun Diameter of orbit Figure 34.26 Distances to nearby stars are measured using triangulation, also called the parallax method. The angle of line of sight to the star is measured at intervals six months apart, and the distance is calculated by using the known

Star 4 ly Earth Sun Diameter of orbit Figure 34.26 Distances to nearby stars are measured using triangulation, also called the parallax method. The angle of line of sight to the star is measured at intervals six months apart, and the distance is calculated by using the known

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Question

Construct Your Own Problem Consider a star moving in a circular orbit at the edge of a galaxy. Construct a problem in which you calculate the mass of that galaxy in kg and in multiples of the solar mass based on the velocity of the star and its distance from the center of the galaxy.