The temperature of the sun is the coolest on the surface at 6000 degrees C or 10882 degrees F. In the middle layer of the sun, the temperature is 1,500,000 degrees C or 2,700,032 degrees F. In the center or core of the sun the temperature is 15,000,000 degrees C or 27,000,000 degrees F. Sunspots on the surface have an average temperature of 4,000 degrees C or 7,000 degrees F.
The third layer of the sun is the convective zone, where heat from the core is transported through the movement of plasma. In this layer, hot material rises towards the surface, cools down, and then descends back towards the core in a continuous cycle. The convective zone is responsible for the sun's complex magnetic field and sunspots.
The convective layer of the sun is responsible for moving heat from the radiative layer to the photosphere. In this layer, heat is transferred through the movement of hot plasma in large convection currents, which helps to transport energy outward to the surface of the sun.
The surface of the sun is known as the photosphere, which appears as a bright, granular layer due to the convective motion of hot gases. It is where the sun's energy is released in the form of light and heat, making it the visible layer of the sun.
The photosphere is the outermost layer of the Sun, followed by the chromosphere, and then the corona. The photosphere is the visible surface of the Sun, while the chromosphere is a layer of hot, ionized gas above it. The corona is the outermost layer of the Sun's atmosphere, extending millions of kilometers into space.
The outermost layer of the Sun's atmosphere is the corona. It is visible during a solar eclipse as a faint, pearly white ring around the Sun. The corona is extremely hot and extends millions of kilometers into space.
The third layer of the sun is the convective zone, where heat from the core is transported through the movement of plasma. In this layer, hot material rises towards the surface, cools down, and then descends back towards the core in a continuous cycle. The convective zone is responsible for the sun's complex magnetic field and sunspots.
5500 Celsius
The convective layer of the sun is responsible for moving heat from the radiative layer to the photosphere. In this layer, heat is transferred through the movement of hot plasma in large convection currents, which helps to transport energy outward to the surface of the sun.
The surface of the sun is known as the photosphere, which appears as a bright, granular layer due to the convective motion of hot gases. It is where the sun's energy is released in the form of light and heat, making it the visible layer of the sun.
The photosphere is the outermost layer of the Sun, followed by the chromosphere, and then the corona. The photosphere is the visible surface of the Sun, while the chromosphere is a layer of hot, ionized gas above it. The corona is the outermost layer of the Sun's atmosphere, extending millions of kilometers into space.
you don't burn because of the ozone layer of the earth. the ozone layer is a layer on earth that observes solar ultraviolet radiation.
The outermost layer of the Sun's atmosphere is the corona. It is visible during a solar eclipse as a faint, pearly white ring around the Sun. The corona is extremely hot and extends millions of kilometers into space.
The sun is like a ball of hot gases with no hard surfaces. Astronomers have found that there are layers in the sun. The part of the sun that gives off th light energy we see is called the photoshere. It is the innermost layer of the of the Sun's atomosphere. The layer above the photoshpere is the chromosphere. The outermost layer is called the corona.
the outermost layer of the sun's atmosphere is the corona.
The sun does not have a solid surface. The visible surface of the Sun is the photosphere, it is the layer below which the Sun becomes opaque to visible light. this layer is hundreds of km thick.
The radiation zone is the sun's thickest layer.
photosphere is the lowes layer of the sun