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  1. www.nasa.gov › image-article › layers-of-sunLayers of the Sun - NASA

    10 paź 2012 · The outer layers are the Photosphere, the Chromosphere, the Transition Region and the Corona. IRIS will focus its investigation on the Chromosphere and Transition Region. More detail on the outer layers follows: Photosphere – The photosphere is the deepest layer of the Sun that we can observe directly.

  2. 3 lut 2024 · The four layers of the Sun are the core, radiative zone, convective zone, and atmosphere. The Sun is a colossal nuclear reactor at the heart of our solar system. Our favorite star is about 109 times the diameter of Earth and over 330,000 times its mass.

  3. 2 lut 2023 · The sun has seven different layers, which are further divided into three inner and four outer layers. The names of these layers, in order of their presence from the core of the sun are as follows: Inner Layers. 1) Core. 2) Radiative Zone. 3) Convection Zone. Outer Layers. 1) Photosphere. 2) Chromosphere. 3) Transition Region. 4) Corona

  4. www.nasa.gov › image-article › anatomy-of-sunAnatomy of the Sun - NASA

    23 sty 2013 · Coronal Streamers – The outward flowing plasma of the corona is shaped by magnetic field lines into tapered forms called coronal streamers, which extend millions of miles into space. This image is featured on the Mysteries of the Sun website and companion book. Credit: NASA/Jenny Mottar

  5. The Sun’s outer gases extend far beyond the photosphere (Figure 15.7). Because they are transparent to most visible radiation and emit only a small amount of light, these outer layers are difficult to observe. The region of the Sun’s atmosphere that lies immediately above the photosphere is called the chromosphere.

  6. The layers of the Sun are divided into two larger groups, the outer and the inner layers. The outer layers are the Corona, the Transition Region, the Chromosphere, and the Photosphere, while the inner layers are the Core, the Radiative Zone, and the Convection Zone.

  7. Sun to the outer regions, hence the name “radiative zone”. Through this area of the solar interior, the energy (in the form of radiation) is transmitted by its interaction with the particles in the surrounding.

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