The temperature of the core of a neutron star can range from around 1 million to several billion degrees Kelvin, making it incredibly hot. This high temperature is a result of the extreme density and strong gravitational forces present in the core.
The temperature at which hydrogen fuses is 10,000,000 degrees Kelvin. This is the minimum temperature the core of a proto star has to have to become a true star.
The factor that determines whether a neutron star or a black hole forms after a supernova explosion is the mass of the collapsing core of the star. If the core's mass is between about 1.4 and 3 times the mass of the sun, a neutron star is formed. If the core's mass exceeds about 3 solar masses, a black hole is likely to form.
The temperature of a star increases when nuclear fusion reactions in its core release energy. As more hydrogen is converted into helium through fusion, the core becomes hotter due to the increased energy released. This increase in temperature leads to the star shining brighter and hotter.
It's Mass
The star's mass determines the temperature in its core. A stars mass will also determined it size and the amount of gravitational pull it will have.
The temperature determines the color of the star!:)
A star becomes a star - "is born" - when the process of nuclear fusion begins in the core of the star.
Mainly its temperature.
Temperatures in the star's core can reach 3x109 K.
The temperature of the core of a star can reach millions of degrees Kelvin due to nuclear fusion reactions that generate immense heat and light. This intense heat and pressure in the core are what sustain a star's energy output.
The temperature of the core of a neutron star can range from around 1 million to several billion degrees Kelvin, making it incredibly hot. This high temperature is a result of the extreme density and strong gravitational forces present in the core.
The temperature in the core of a star depends, to a great extent, on:* The star's mass. The general tendency is that high-mass stars are hotter. * Where the star is in its life cycle. The star's core temperature will vary over time. On the other hand, the star's surface temperature also depends on its size. Thus, it is possible that PRECISELY because a star is hotter in the core, it gets bigger, and the surface temperature DECREASES (though its total energy output increases).
The core.
If the core temperature of a star decreases, it will contract, causing the core to become denser. This contraction may lead to an increase in temperature in the outer layers, causing the star to expand its radius to re-establish equilibrium.
The temperature at which hydrogen fuses is 10,000,000 degrees Kelvin. This is the minimum temperature the core of a proto star has to have to become a true star.
The star with a surface temperature closest to the boundary between Earth's mantle and core would be the Sun, with a surface temperature of about 5,500 degrees Celsius. The temperature at the boundary between Earth's mantle and core is estimated to be around 3,000-4,000 degrees Celsius.