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The convection zone in a star like the Sun is located just beneath the photosphere. It is the layer where energy generated in the star's core is transported to the surface via convection currents, providing the energy needed for the star to shine.
It takes about 100,000 years for a photon to move from the core of the sun to the convection zone. Photons created in the core of the sun have to undergo a random walk through the dense radiative zone before finally reaching the less dense convection zone.
The interior layers of a star, from innermost to outermost, are the core, radiative zone, and convective zone. The core is where nuclear fusion occurs, generating the star's energy. The radiative zone is where energy is transported through radiation, while the convective zone is where energy is transported through the movement of gas.
The radioactive zone in the Sun is the region where nuclear fusion occurs, specifically the conversion of hydrogen into helium. This process releases energy in the form of light and heat, which ultimately powers the Sun and allows it to shine.
The convection zone in the Sun extends from about 200,000 kilometers below the surface to about 200,000 kilometers above the surface, for a total thickness of around 400,000 kilometers.
The convection zone of the sun surrounds the radiative zone, which is the region where energy generated by nuclear fusion in the core is transported outwards through the slow process of radiative diffusion. In the convection zone, energy is transported by the movement of hot plasma, creating convection currents.
The Sun's fusion takes place in the core. The Convective zone brings heat to the surface by thermal convection, which is basically hot plasma coming up to the surface, then cooling and sinking.
The sun is composed of three main regions: the core, where nuclear fusion occurs; the radiative zone, where energy moves by radiation; and the convection zone, where energy moves by convection. The visible surface of the sun is called the photosphere.
The sun has three main layers: the core, where nuclear fusion occurs; the radiative zone, where energy is transported by electromagnetic radiation; and the convective zone, where energy is transported by convection. The sun's atmosphere includes the photosphere, chromosphere, and corona.
The three main parts of the Sun are the core, radiative zone, and convective zone. The core is where nuclear fusion occurs, producing the Sun's energy. The radiative zone is where energy is transported by electromagnetic radiation, and the convective zone is where energy is transported by convection currents.
From outermost layer to innermost layer: corona, chromosphere, photosphere, subsurface flows, convection zone, radiative zone, inner core.
The convection zone.
The three main layers of the sun are the core, the radiative zone, and the convective zone. The core is where nuclear fusion occurs, converting hydrogen into helium. The radiative zone is where energy is transported by photons, while the convective zone is where energy is transferred by gas moving in convection currents.
AnswerCoreCoronaChromospherePhotosphereAnswerThe sun has more than three layers. They are: CoreRadiation zoneConvection zonePhotosphere-sunspotsChromosphereTransition regionCoronaAnswerInterior consists of three layers: CoreThe Radiation ZoneThe Convection ZoneCore: The central region of the sun, where nuclear fusion takes place.Radiation Zone: A region of very tightly packed gas in Sun's interior where energy is transferred mainly in the form of light.Convection Zone: The outer most layer of the sun's interior.There are approximately 3 layers to the sun. They are the core, radiative zone, and convection zone.
The core is the innermost region where nuclear fusion occurs, generating the sun's energy. The radiative zone is a layer of the sun where energy from the core is transported through radiation. The convective zone is the outermost layer where heat is carried through convection currents.
The four main parts of the Sun are the core, radiative zone, convective zone, and the photosphere. The core is where nuclear fusion occurs, producing energy. The radiative zone and convective zone are layers where energy is transported outward through radiation and convection. The photosphere is the visible surface of the Sun.
Energy is generated in the core of the sun through nuclear fusion where hydrogen atoms are converted into helium. This energy then moves through the radiative zone via photons, which are energy particles that bounce around and slowly make their way to the photosphere. The energy eventually reaches the photosphere where it is released as sunlight.