Physics, 08.08.2019 21:20 chrisraptorofficial
Once again in this chapter, we see the use of kepler’s third law to estimate the mass of supermassive black holes. in the case of ngc 4261, this chapter supplied the result of the calculation of the mass of the black hole in ngc 4261. in order to get this answer, astronomers had to measure the velocity of particles in the ring of dust and gas that surrounds the black hole. how high were these velocities? turn kepler’s third law around and use the information given in this chapter about the galaxy ngc 4261—the mass of the black hole at its center and the diameter of the surrounding ring of dust and gas—to calculate how long it would take a dust particle in the ring to complete a single orbit around the black hole. assume that the only force acting on the dust particle is the gravitational force exerted by the black hole. calculate the velocity of the dust particle in km/s.
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Physics, 21.06.2019 21:30
How many seconds does it take a pebble released from rest off a bridge to fall 29.4 m ? what is the pebble's speed when it has fallen 29.4 m ?
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Physics, 22.06.2019 20:40
Ablock of mass m = 2.5 kg is attached to a spring with spring constant k = 740 n/m. it is initially at rest on an inclined plane that is at an angle of theta= 26 with respect to the horizontal, and the coefficient of kinetic friction between the block and the plane is uk = 0.17. in the initial position, where the spring is compressed by a distance of d = 0.16 m, the mass is at its lowest position and the spring is compressed the maximum amount. take the initial gravitational energy of the block as zero. the block's initial mechanical energy is 9.472 j.b. if the spring pushes the block up the incline, what distance l in meters will the block travel before coming to rest? the spring remains attached to both the block and the fixed wall throughout its motion.
Answers: 3
Physics, 22.06.2019 23:00
During the past 150 years in the united states, how did energy consumption compare to population growth
Answers: 1
Once again in this chapter, we see the use of kepler’s third law to estimate the mass of supermassiv...
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