Understanding the Changing Density of the Sun's Core

In summary, the density of the core of the sun is approximately 150 g/cm³. It is calculated by dividing the mass of the core by its volume and is affected by factors such as temperature, pressure, and composition. The density of the core is much higher than that of other celestial bodies due to intense gravitational forces. It remains relatively constant over time due to the balance between inward gravitational forces and outward pressure forces caused by nuclear fusion reactions.
  • #1
Rameesh
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why density of core of the sun is changing ?
please give me brief explain with calculation
 
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Thank you
 

FAQ: Understanding the Changing Density of the Sun's Core

What is the density of the core of the sun?

The density of the core of the sun is approximately 150 g/cm³.

How is the density of the core of the sun measured?

The density of the core of the sun is calculated by dividing the mass of the core by its volume.

What factors affect the density of the core of the sun?

The density of the core of the sun is affected by the temperature, pressure, and composition of the materials present in the core.

How does the density of the core of the sun compare to other celestial bodies?

The density of the core of the sun is much higher than that of other celestial bodies, such as planets or stars, due to the intense gravitational forces present in the core.

How does the density of the core of the sun change over time?

The density of the core of the sun remains relatively constant over time, as the nuclear fusion reactions in the core maintain a balance between the inward gravitational forces and the outward pressure forces.

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