">
">
">
">
The sun is a star that were located closest to the Earth in both clusters in the Milky Way galaxy and andromeda galaxy. The sun is a star because the sun emits its own light produced. The sun emits light and heat can be a very, very large amount of energy because it is produced from nuclear fusion of hydrogen nuclei merge.
A. Distance of the Sun to the Earth
The sun is a star that looks great compared to most other stars are scattered in space because it is very close, which is about 150 million km. 150 million kilo meters also called unit astronomi.Jarak position nearest the Sun to the Earth is 147 million km away called Perihelium (January 1). While the farthest distance the sun to the Earth is approximately 152 million kilometers called Aphelium (1 July). Of course, there is currently no person involved directly between the sun to the earth as it is very hot and the glare.
B. Temperature Sun
The hot sun on the surface is about 6 thousand degrees Celsius. While in the sun's core temperature reaches 150 million degrees Celsius. From time to time the sun would be predicted temperature gets colder and eventually died with the other planets, including Earth.
C. Authors Solar-Hydrogen : 70%
A. Distance of the Sun to the Earth
The sun is a star that looks great compared to most other stars are scattered in space because it is very close, which is about 150 million km. 150 million kilo meters also called unit astronomi.Jarak position nearest the Sun to the Earth is 147 million km away called Perihelium (January 1). While the farthest distance the sun to the Earth is approximately 152 million kilometers called Aphelium (1 July). Of course, there is currently no person involved directly between the sun to the earth as it is very hot and the glare.
B. Temperature Sun
The hot sun on the surface is about 6 thousand degrees Celsius. While in the sun's core temperature reaches 150 million degrees Celsius. From time to time the sun would be predicted temperature gets colder and eventually died with the other planets, including Earth.
C. Authors Solar-Hydrogen : 70%
- Helium: 25%
- Other elements: 5%
D. Constants And Solar Energy
The amount of heat received by each 1 cm square in the upper atmosphere of the sun per minute is 2 calories per minute per square cm. Solar energy is due to the incorporation of hydrogen nuclei fusiatau form a helium nucleus and two positrons and energy 24.7 MeV.E. Composition Parts of the Sun-photosphere is part surface layer that emits intense light and glare. - Kormosfer is a very thick layer of gas. - Corona is the outermost layer of the solar atmosphere
D. Constants And Solar Energy
The amount of heat received by each 1 cm square in the upper atmosphere of the sun per minute is 2 calories per minute per square cm. Solar energy is due to the incorporation of hydrogen nuclei fusiatau form a helium nucleus and two positrons and energy 24.7 MeV.E. Composition Parts of the Sun-photosphere is part surface layer that emits intense light and glare. - Kormosfer is a very thick layer of gas. - Corona is the outermost layer of the solar atmosphere
Source From : http://www.scribd.com/doc/47580397/Penjelasan-Dan-Pengertian-Matahari-dan-planet-di-tata-surya
0 komentar:
Posting Komentar