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When you combine an electron with a proton you make a neutron. Therefore you make a "neutron" star.
An isotope can be produced if a nucleus gains a neutron or if one of the protons in its nucleus decays into a neutron and positron.
A Neutron.
A neutron star no longer produces energy - it is a dead star. It will gradually get colder, until it stops emitting any significant amount of heat. Any heat the neutron star radiates is residual heat - heat that was produced earlier, either through fusion, or through the tremendous gravitational collaps that produced the neutron star.
You left out part of this statement. One neutron has a mass of 1.67495x10^-24g.
When you combine an electron with a proton you make a neutron. Therefore you make a "neutron" star.
An isotope can be produced if a nucleus gains a neutron or if one of the protons in its nucleus decays into a neutron and positron.
An isotope can be produced if a nucleus gains a neutron or if one of the protons in its nucleus decays into a neutron and positron.
a neutron has no charge
You have half answered this question for yoiurself ( produced) ; the answer is 'PRODUCTS'.
phermones
A Neutron.
A neutron star no longer produces energy - it is a dead star. It will gradually get colder, until it stops emitting any significant amount of heat. Any heat the neutron star radiates is residual heat - heat that was produced earlier, either through fusion, or through the tremendous gravitational collaps that produced the neutron star.
You left out part of this statement. One neutron has a mass of 1.67495x10^-24g.
Each proton and neutron is made up of three quarks.
When a neutron star is formed, protons and electrons are crushed, they collide and become neutrons.
During electron capture, an electron and proton combine and are converted to a neutron.