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The core of a star collapses during a supernova, fanning a neutron star.
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University Physics Volume 3
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- C6M.9 Astar with mass M and radius R collides with another star of massM and radius R, and coalesce to form a new star at rest whose radius is R. Assume that initially the colliding stars had angular velocities with opposite direc- tions but the same magnitude | What is the magnitude and direction of the final star's angular velocity? (Express the magnitude as a fraction of )arrow_forwardThe Sun’s mass is 2.0 × 1030 kg, its radius is 7.0 × 105 km, and it has a rotational period of approximately 28 days. If the Sun should collapse into a white dwarf of radius 3.5 × 103 km, what would its period be if no mass were ejected and a sphere of uniform density can model the Sun both before and after?arrow_forwardA star with a of mass of 3.0x1032 kg and radius 7.0x108 m is initially rotating at a rate of once every 30 days. The star collapses into a neutron star with the same mass but a new radius of 18,000 m. What is the new angular speed of the star? (Give your answer in rotations per second.) Assume the star is a solid sphere: Isphere = 2/5 MR2.arrow_forward
- A star has a mass of 1.23 x 1030 kg and is moving in a circular orbit about the center of its galaxy. The radius of the orbit is 1.0 x 104light-years (1 light-year = 9.5 x 1015 m), and the angular speed of the star is 1.7 x 10-15 rad/s. (a) Determine the tangential speed of the star. (b) What is the magnitude of the net force that acts on the star to keep it moving around the center of the galaxy?arrow_forwardWhen a star collapses it significantly shrinks in size and spins up. Consider a star with a mass of M = 2.2×1030 kg and an initial radius of R₁ = 6.8×105 km. If the initial period of rotation of the star is T₁ = 28.9 days, find the new rotational period after it collapses to a final radius of Rf = 6.8×10³ km. Treat the star before and after the collapse as a solid sphere with uniform mass distribution (which is not true, of course, but good enough for an estimation). The new rotational period of the star, Tf = Find the ratio between the final and initial rotational kinetic energies of the star. The factor by which the kinetic energy of the star increases, KE₁/KE₁ Units km = Units Select an answer ✓ Units N X The increase in the rotational kinetic energy of the star comes from gravity. How much work is done by the gravity force while collapsing the star? The work done by gravity, W = ||arrow_forwardA star has a mass of 1.5 x 10^30 kg and is moving in a circular orbit about the center of its galaxy. The radius of the orbit is 2.2 x 10 ^ 4 light years( 1 lightyear = 9.5 x 10 ^15 m ) , and the angular speed of the star is 2.2 x 10 ^ -15 rad/s. a) Determine the tangential speed of the star. b) What is the magnitude of the net force that acts on the star to keep moving around the center of the galaxy?arrow_forward
- A star has a mass of 1.03 x 1030 kg and is moving in a circular orbit about the center of its galaxy. The radius of the orbit is 2.4 x 104 light-years (1 light-year = 9.5 x 1015 m), and the angular speed of the star is 1.0 x 10-15 rad/s. (a) Determine the tangential speed of the star. (b) What is the magnitude of the net force that acts on the star to keep it moving around the center of the galaxy?arrow_forwardPulsars. When a star with a mass at least ten times that of the Sun explodes outward in a supernova, its core can be collapsed into a pulsar, which is a spinning star that emits electromagnetic radiation (radio waves or light) in two tight bears in opposite directions. If a beam sweeps across Earth during the rotation, we can detect repeated pulses of the radiation, one per revolution. (a) The first pulsar was discovered by Jocelyn Bell Burnell and Antony Hewish in 1967; its pulses are separated by 1.3373 s. What is its angular speed in revolutions per second? (b) To date, the fastest spinning pulsar has an angular speed of 716 rev/s. What is the separation of its detected pulses in milliseconds? (a) Number (b) Number Hint 1345.98 eTextbook and Media Save for Later 2510 Units Units revis ms Attempts: 1 of 5 used Submit Answerarrow_forwardA star has a mass of 2.42 x 1030 kg and is moving in a circular orbit about the center of its galaxy. The radius of the orbit is 1.5 x 104 light-years (1 light-year = 9.5 x 1015 m), and the angular speed of the star is 1.8 x 10-15 rad/s. (a) Determine the tangential speed of the star. (b) What is the magnitude of the net force that acts on the star to keep it moving around the center of the galaxy?arrow_forward
- A star has a mass of 1.87 x 1030 kg and is moving in a circular orbit about the center of its galaxy. The radius of the orbit is 2.3 x 104 light-years (1 light-year = 9.5 x 1015 m), and the angular speed of the star is 1.9 x 10-15 rad/s. (a) Determine the tangential speed of the star. (b) What is the magnitude of the net force that acts on the star to keep it moving around the center of the galaxy? (a) Number Units (b) Number Unitsarrow_forwardA star has a mass of 2.62 x 10³0 kg and is moving in a circular orbit about the center of its galaxy. The radius of the orbit is 3.0 x 104 light-years (1 light-year = 9.5 x 1015 m), and the angular speed of the star is 1.6 x 10-15 rad/s. (a) Determine the tangential speed of the star. (b) What is the magnitude of the net force that acts on the star to keep it moving around the center of the galaxy? (a) Number i (b) Number i Units Unitsarrow_forwardHunting a black hole. Observations of the light from a certain star indicate that it is part of a binary (two- star) system. This visible star has orbital speed v = 270 km/s, orbital period T = 23.1 days, and approximate mass m₁ = 5.7M², where Ms is the Sun's mass, 1.99 x 10³0 kg. Assume that the visible star and its companion star, which is dark and unseen, are both in circular orbits (see the figure). Find the ratio of the approximate mass m2 of the dark star to Ms. Number IN m₁ 11 Units m₂arrow_forward
- University Physics Volume 1PhysicsISBN:9781938168277Author:William Moebs, Samuel J. Ling, Jeff SannyPublisher:OpenStax - Rice University