The figures show a hypothetical planetary system at two different times. The system has a star...

Transcribed Image Text:

The figures show a hypothetical planetary system at two different times. The system has a star S and three planets, labeled A, B, and C. The table provides the mass of each body in the system, as well as their spatial coordinates (x, y) in their initial and final positions. The spatial coordinates of the bodies are given in Astronomical Units (AU). Final Position Initital Position (0,0) (0.1581,0) (xs.ys) (0,-0.2803) (-1.7873,0) (-0.7599,-0.6035) Body S A B с Mass (kg) mg = 2.5085 x 100 MA=2.6845 x 1028 mg = 6.2841 x 102 me = 7.1397 x 107 The initial velocity of the center of mass of the system is zero. Find the magnitude de of the star's displacement from the origin in its final position. $ (0,0) (0.6239, 1.5929) (0, 1.4245) Initial Position B AU ? Final Position The figures show a hypothetical planetary system at two different times. The system has a star S and three planets, labeled A, B, and C. The table provides the mass of each body in the system, as well as their spatial coordinates (x, y) in their initial and final positions. The spatial coordinates of the bodies are given in Astronomical Units (AU). Final Position Initital Position (0,0) (0.1581,0) (xs.ys) (0,-0.2803) (-1.7873,0) (-0.7599,-0.6035) Body S A B с Mass (kg) mg = 2.5085 x 100 MA=2.6845 x 1028 mg = 6.2841 x 102 me = 7.1397 x 107 The initial velocity of the center of mass of the system is zero. Find the magnitude de of the star's displacement from the origin in its final position. $ (0,0) (0.6239, 1.5929) (0, 1.4245) Initial Position B AU ? Final Position

Answer rating: 100% (QA)

To find the magnitude of the stars displacement from the origin in its final position we n... View the full answer