The figures show a hypothetical planetary system at two different times. The system has a star...
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). Body Mass (kg) Initital Position Final Position Sms- 1.6531 x 1030 A MA 2.4401 x 1028 Bİmg_7.0129x1026| (0.7483,1.5507) |...
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). Body Mass (kg) Initital Position Final Position S ms - 2.5085 x 1090 (0,0) (xs, ys) A m...
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 (2x, y) in their initial and final positions. The spatial coordinates of the bodies are given in Astronomical Units (AU). Body Mass (kg) Initital Position Final Position S ms = 2.6307 x 1030 (0,0) (as, ys) A ma...
The figures show a hypothetical planetary system at two different times. The spatial coordinates (x, y) of the bodies are given in Astronomical Units (AU). In the first picture, the velocity of the center of mass of the system is zero. Find the magnitude, ds, of the star's displacement. ms-1.8975 x 1030 kg mA-2.3179 x1028 kg mg-68307x 1026 kg mc 8.0285 x107 kg Number (0, 1.2601) (0.6239, 1.6351) (0.2967, 0) (-1.6007, 0) (0, 0) (0, -0.2803) (-0.6333,-0.8927)
Please use the formulate sheet and show all steps to make sure the question is worth any points a) The initial ratio of deuterium (D) to hydrogen (H) in a planet's atmosphere was 175000; however, the present ratio is 1/1500 and the initial and final abundances of D are 5 x 10° atoms per m3 and 9 x 106 atoms per m2, respectively. What fraction of deuterium has been lost, and what fraction of hydrogen has been lost in this...