Hi! It's 13 Million* Fahrenheit to 3.6* Fahrenheit.
The temperature in the radiative zone of the sun averages around 27 million degrees Fahrenheit.
The radiative zone in the sun can reach temperatures of several million degrees Celsius. Energy from nuclear fusion reactions in the core is transported through this region via photons before reaching the convective zone.
The three main layers of the sun's interior are the core, radiative zone, and convective zone. The core is where nuclear fusion reactions occur, producing the sun's energy. The radiative zone is where energy moves outward through radiation. The convective zone is where heat is carried to the surface through the movement of hot gas.
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 can be divided into three main regions: the core, the radiative zone, and the convective zone. The core is where nuclear fusion reactions occur, producing the sun's energy. The radiative zone is where energy is transported primarily through electromagnetic radiation. The convective zone is the outermost layer where energy is transferred through the motion of hot gas bubbles.
The two main parts of the Sun's core are the radiative zone and the convective zone. In the radiative zone, energy is transferred through radiation as photons bounce around and slowly move toward the surface. In the convective zone, energy is transported through the movement of hot plasma creating convection currents.
The radiative zone is hotter than the convection zone. In the radiative zone, energy is transferred through electromagnetic radiation, while in the convection zone, energy is transferred through the movement of hot gas or plasma.
In the radiative zone of a star, energy is transferred through electromagnetic radiation (photons) as it travels from the core to the convective zone. In contrast, in the convective zone, energy is transferred by the physical movement of hot gas or plasma through convection currents.
The radiative zone in the sun can reach temperatures of several million degrees Celsius. Energy from nuclear fusion reactions in the core is transported through this region via photons before reaching the convective zone.
In the radiative zone, energy is transferred by electromagnetic radiation as photons travel through the dense plasma. In the convective zone, energy is transferred through the physical movement of hot plasma carrying heat to the surface which causes convection currents.
By hot zone, I assume you mean out of the habitable or Goldilocks zone. Estimates vary, but in all likely hood changes will become noticeable in about a billion years, and severe in three billion years.
The danger zone is between 41-140 Fahrenheit, but around 165 Fahrenheit is the best
The convection zone of the sun contains hot gas moving up toward the surface and cooler gas moving down toward the center. This zone is located above the radiative zone and is responsible for transporting heat from the sun's core to its surface through the motion of plasma currents.
Corona, Chromosphere, Photosphere, Subsurface Flows, Internal Structure (convection zone, radiative zone, inner zone)
hot hot hot
the suns terrain is hot rock jessica ford
hot hot hot
The answer depends on what you are used to. Most people from the temperate zone will consider it hot but people from tropical regions will consider is cold.