Describe the changes in temperature and density one would hypothetically encounter if they could travel through the Sun’s convection zone and radiative zone, ending up in the core.
The interior and exterior of the Sun have layers that vary in terms of temperature, pressure, and density. Additionally, the processes involved for the transference of energy/light differ amongst them. Below, you see several statements describing different layers. In each of the blanks next to them, put one letter that identifies the name of the […]