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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