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The star at the center of our solar system is called the Sun.
The Sun is a white star, although it looks yellow from Earth.
Astronauts who have viewed the Sun from outside of Earth's atmosphere
have all reported the Sun look white. The reason why its looks
yellow to us is because the blue spectrum of light is scattered in our
atmosphere, hence a blue sky. The Earth lies approximately 93
million miles from the Sun. The sun provides the warmth that the
Earth needs to be hospitable to life. It creates the light that
Earth-bound plants need for photosynthesis, it provides the warmth that
causes water to exist in liquid form, but not too much such that the
oceans boil away.
The Sun is huge and comprises 99.86 of all the matter
in our solar system. The Sun is a giant ball of gas that
is held together by its own gravity. This causes
tremendous pressure, and thus tremendous heat. The sun's
core reaches 15 million degrees Celsius (about 27 million
degrees Fahrenheit). The Sun is comprised of hydrogen gas
that undergoes thermonuclear fusion and fuses into Helium.
The outermost layer of the Sun is called the
photosphere. This is where the Sun's radiation escapes.
It takes light 8 minutes to reach the Earth from the Sun.
The photosphere's temperature reaches 5,500º
Celsius (10,000º Fahrenheit)
and is the area in which sunspots form. The areas above
the photosphere are called the chromosphere and the corona.
Oddly enough, the temperature increases to 2 million degrees
Celsius (3.5 million degrees Fahrenheit). The Sun emits a
solar wind of charged particles that extend to the outer limit
of the solar system. The solar wind blows at an incredible
rate of 400 km/s (about 1 million miles per hour).
| Mass (kg)
| 1024 |
| Diameter (km)
| 1.4 million |
| Mean density (kg/m3)
| 1408 |
| Escape velocity (km/s)
| 617.7 |
| Average distance from Earth
| 39.48 AU (5,906,376,200 km)
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| Surface Gravity (eq.) (m/s2) | 274 |
| Absolute Magnitude | +4.83 |
| Luminosity (1024 J/s) | 384.6 |
| Mass conversion rate (106 kg/s) | 4300 |
| Mean energy production (10-3 J/kg) | 0.1937 |
| Surface emission (106 J/m2s) | 63.29 |
| Spectral type | G2V |
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Image of
Our Star, the Sun

Picture of the Sun in
Ultraviolet Light

Photograph of
Coronal Mass Ejection |