Body A has a mass of 1027 kilogram. The central star has a mass of 1030...
Body A has a mass of 1027 kilogram. The central star has a mass of 1030 kilogram. The average distance between the central star and Body A is 5.2 AU (Astronomical Unit). The Solar Luminosity of the central star is 1026 W. In this hypothetical universe, the Stefan-Boltzman constant is 10-8 W m-2 K-4. (this is all the information I was given)
What is the minimum velocity of an object hitting Body A? A spherical asteroid with a radius of 50 km and a density of 5000 kg m-3 just struck Body A with this minimum velocity. How much energy is delivered to Body A?
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Body A has a mass of 1027 kilogram. The central star
has a mass of 1030...
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 (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 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 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...
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...
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 PositionFinal Position s l ms = 2.1419 × 1030 | A | mA = 1.9513 ×...
Please use the formulate sheet and show all steps to make sure the question is worth...
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...
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 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 (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 PositionFinal Position s l ms = 2.1419 × 1030 | A | mA = 1.9513 ×...
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...
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