**Formation and Characteristics of Neutron Stars:**When a massive star reaches the end of its life, it is possible for a supernova to occur. This may result in the formation of a very small, but very dense, neutron star, the density of which is about the same as a neutron. - **Neutron Properties:** - Mass: \(1.7 \times 10^{-27}\) kg - Approximate Radius: \(1.2 \times 10^{-15}\) m- **Sun Properties:** - Mass: \(2.0 \times 10^{30}\) kg**Problem Statement:**Determine the radius \( R \) of a neutron star that has three times the mass of our Sun and the same density as a neutron.**Calculation Attempt:**- Result: \( R = 1.27 \times 10^{4} \) m- Status: IncorrectThis calculation box features an interactive field where students can input their results to verify accuracy.

Given Mass of neuron m = 1.7×10-27 kg Radius of neuron r = 1.2×10-15 m Mass of sun (M) =…

When a massive star reaches the end of its life, it is possible for a supernova to occur. This may result in the formation of a very small, but very dense, neutron star, the density of which is about the same as a neutron. A neutron has a mass of 1.7 x 10-27 kg and an approximate radius of 1.2 x 10-15 m. The mass of the sun is 2.0 x 1030 kg. Determine the radius R of a neutron star that has three times the mass of our Sun and the same density as a neutron. 1.27 x104 R = m Incorrect

When a massive star reaches the end of its life, it is possible for a supernova to occur. This may result in the formation of a very small, but very dense, neutron star, the density of which is about the same as a neutron. A neutron has a mass of 1.7 x 10-27 kg and an approximate radius of 1.2 x 10-15 m. The mass of the sun is 2.0 x 1030 kg. Determine the radius R of a neutron star that has three times the mass of our Sun and the same density as a neutron. 1.27 x104 R = m Incorrect