Sun Statistics
太阳参数 |
| 质量 (kg) |
1.989e+30 |
| 质量 (地球 = 1) |
332,830 |
| 赤道半径 (km) |
695,000 |
| 迟到半径 (地球 = 1) |
108.97 |
| 密度 (mg/cm^3) |
1.410 |
| 自转周期 (天) |
25-36* |
| 逃逸速度 (km/sec) |
618.02 |
| 亮度 (ergs/sec) |
3.827e33 |
| 星等 (Vo) |
-26.8 |
| 表面温度 |
6,000°C |
| 年龄 (十亿年) |
4.5 |
化学成分
氢Hydrogen
氦Helium
氧Oxygen
碳Carbon
镍Nitrogen
氖Neon
铁Iron
硅Silicon
镁Magnesium
硫Sulfur
其它All others
|
92.1%
7.8%
0.061%
0.030%
0.0084%
0.0076%
0.0037%
0.0031%
0.0024%
0.0015%
0.0015% |
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English Material:
The Sun is the most prominent feature in our solar system. It is the largest object and contains approximately 98% of the total solar system mass. One hundred and nine Earths would be required to fit across the Sun's disk, and its interior could hold over 1.3 million Earths. The Sun's outer visible layer is called the photosphere and has a temperature of 6,000°C (11,000°F). This layer has a mottled appearance due to the turbulent eruptions of energy at the surface.
Solar energy is created deep within the core of the Sun. It is here that the temperature (15,000,000° C; 27,000,000° F) and pressure (340 billion times Earth's air pressure at sea level) is so intense that nuclear reactions take place. This reaction causes four protons or hydrogen nuclei to fuse together to form one alpha particle or helium nucleus. The alpha particle is about .7 percent less massive than the four protons. The difference in mass is expelled as energy and is carried to the surface of the Sun, through a process known as convection, where it is released as light and heat. Energy generated in the Sun's core takes a million years to reach its surface. Every second 700 million tons of hydrogen are converted into helium ashes. In the process 5 million tons of pure energy is released; therefore, as time goes on the Sun is becoming lighter.
The chromosphere is above the photosphere. Solar energy passes through this region on its way out from the center of the Sun. Faculae and flares arise in the chromosphere. Faculae are bright luminous hydrogen clouds which form above regions where sunspots are about to form. Flares are bright filaments of hot gas emerging from sunspot regions. Sunspots are dark depressions on the photosphere with a typical temperature of 4,000°C (7,000°F).
From: http://www.solarviews.com |
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