# Urutan Lapisan Matahari dari Inti hingga Lapisan Terluar adalah
The sun is a magnificent celestial body that provides us with warmth and light. It is composed of several layers, each with its own characteristics and importance. Let’s explore the layers of the sun, starting from its core and moving towards the outermost layer.
## 1. Inti
At the very heart of the sun lies its core, the center of all the action. This is where nuclear fusion takes place, converting hydrogen atoms into helium and releasing an enormous amount of energy in the process. The temperature in the core reaches a staggering 15 million degrees Celsius, making it the hottest part of the sun. The intense heat and pressure create the conditions necessary for the sun to shine brightly.
## 2. Radiasi
Moving outwards from the core, we come to the radiative zone. This layer is primarily responsible for the transport of energy generated in the core to the sun’s surface. Photons, which are particles of light, are constantly absorbed and re-emitted as they make their way through this zone. It can take up to thousands of years for a photon to travel through the radiative zone, as it has to navigate through the dense plasma of the sun. Despite the slow progress, the radiative zone ensures that the sun’s energy reaches all the other layers.
## 3. Konveksi
Beyond the radiative zone lies the convective zone. This layer is characterized by the movement of plasma in large convection currents. The energy generated in the core is transported to the surface through these currents, as hot plasma rises and cooler plasma sinks. This process is similar to how boiling water creates bubbles that rise to the top. The convective zone plays a crucial role in mixing the sun’s material, distributing heat, and generating the sun’s magnetic field.
As we journeyed from the core to the outer layers of the sun, we witnessed the incredible processes that occur within each layer. The sun’s core is the powerhouse that sustains its existence, while the radiative and convective zones work together to transport energy and maintain its equilibrium. Understanding the structure of the sun helps us appreciate the immense power and beauty that it radiates.
In conclusion, the sun’s layers, from the core to the outermost layer, showcase the complexity and elegance of our star. Each layer plays a vital role in the sun’s existence and the continuous provision of light and heat to our planet. So, the next time you bask in the warm rays of the sun, remember the intricate journey those photons took from the core to reach your skin.