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Ch 14: Periodic Motion
Chapter 14, Problem 13

Astronomers have observed a small, massive object at the center of our Milky Way galaxy. A ring of material orbits this massive object; the ring has a diameter of about 15 light-years and an orbital speed of about 200 km/s. (b) Observations of stars, as well as theories of the structure of stars, suggest that it is impossible for a single star to have a mass of more than about 50 solar masses. Can this massive object be a single, ordinary star?

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Identify the given information: The diameter of the ring is 15 light-years and the orbital speed of the ring is 200 km/s.
Convert the diameter of the ring from light-years to meters for consistency in units. Recall that 1 light-year is approximately 9.461 x 10^15 meters.
Calculate the circumference of the ring using the formula for the circumference of a circle, C = \\(\pi \\cdot d\\), where \\(d\\) is the diameter.
Determine the orbital period of the ring using the formula \\(T = \frac{C}{v}\\), where \\(C\\) is the circumference and \\(v\\) is the orbital speed.
Use Kepler's third law in the form \\(M = \frac{v^2 \\cdot r}{G}\\) to estimate the mass of the central object, where \\(v\\) is the orbital speed, \\(r\\) is the radius of the orbit (half of the diameter), and \\(G\\) is the gravitational constant. Compare this mass to the maximum mass of a single star (50 solar masses) to determine if the central object could be a single, ordinary star.

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Key Concepts

Here are the essential concepts you must grasp in order to answer the question correctly.

Mass of Stars

The mass of a star is a critical factor in determining its lifecycle and characteristics. Ordinary stars, like our Sun, have mass limits, with the most massive stars reaching around 50 solar masses. Beyond this limit, stars cannot maintain stable fusion processes, leading to different evolutionary paths, such as becoming supernovae or black holes.
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Orbital Mechanics

Orbital mechanics describes the motion of objects in space under the influence of gravitational forces. The speed and distance of an orbiting object can be analyzed using Kepler's laws and Newton's law of gravitation. In this case, the observed orbital speed of 200 km/s and the size of the ring provide insights into the mass of the central object, suggesting it is significantly more massive than a single star.
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Supermassive Black Holes

Supermassive black holes are astronomical objects with masses ranging from millions to billions of solar masses, typically found at the centers of galaxies. They exert strong gravitational forces that can influence the motion of nearby stars and gas. The presence of a massive object at the center of the Milky Way, along with the observed orbital dynamics, strongly indicates that this object is likely a supermassive black hole rather than a single star.
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