Thursday, November 25, 2010

Our Sun The Basics


Our Sun A Yellow Dwarf/Photo Astronomy for armatures

Our Sun is not unique in the universe. It is a common middle-sized yellow star which scientists have named Sol. This is why our system of planets is called the Solar System. There are trillions of other stars in the Universe just like it. Many of these stars have their own systems of planets, moons, asteroids, and comets.
The Sun was born in a vast cloud of gas and dust around 5 billion years ago. Indeed these vast nebulae are the birth places of all stars. Over a period of many millions of years, this gas and dust began to fall into a common center under the force of its own gravity.

At the center, an ever growing body of mass was forming. As matter falls inward, it generates a tremendous amount of heat and pressure. As it grew, the baby Sun became hotter and hotter. Eventually when it reached a temperature of around 1 million degrees, its core ignited, causing it to begin nuclear fusion
When this happened, the Sun began producing its own light, heat, and energy.

Nuclear fusion is how stars produce their light, heat, and energy. Through this process, they “burn” a fuel known as hydrogen. The result is that they create another type of matter known as helium. However, stars do not burn in the same way that a fire does, because stars are not on fire.
Heat rises, while cooler gas falls. Have you ever noticed that your basement is always much cooler than upstairs. The same laws of physics apply within stars. Because heat rises, while cooler gases fall, the gas within stars is constantly rising and falling. This creates massive streams of circular motion within the star. This is called convection.

As the gases near the core of the Sun are heated, they begin to rise towards the surface. As they do so, they cool somewhat. Eventually, they become cool enough that they begin to sink back down towards the core. It can take an atom millions of years to complete one complete cycle around a convection stream.

On a side note in a recent poll conducted by a leading astronomy magazine found that 55% of adults in the United States don't know that the sun is a typical star, the Sun is known as a yellow dwarf star. This group of stars are relatively small, containing between 80% and 100% the mass of the sun. So the Sun is at the higher end of this group. The official designation is as a G V star.

We will continue the current topic of exploring our sun in the next post, hope you enjoyed today's post and learnt something new.

Friday, November 19, 2010

A Series on the Sun

OUR SUN/PHOTO SPACESTATIONINFO.COM
OK m friends I'm sorry it has been exactly a month since I last posted here, so I am going to get myself motivated and start out a series of posts regarding the sun, not sure how many entries there may be in this series I guess all of us will stand by and see.

The sun is a star which is very closer to earth than any other star and appears very large and bright. Without the Sun's light and heat, there would be no life on Earth. The Sun is a ball of plasma with a mass of about 2×1030 kg. The sun is mainly composed of hydrogen and helium; it contains about 70% of hydrogen, 28% of helium and less than 2% of other metals. The outer atmosphere of sun has a temperature of over 106 K when its visible surface (the photosphere) has a temperature of just 6,000 K. Solar energy is transformed by plants into chemical energy, which is the first step in the food chain for all living things. The Sun has been around for about 4.6 billion years and is expected to keep burning bright for another 5 billion years.

COMPOSITION OF OUR SUN

  1. HYDROGEN-73.46%                                                                 6.  NEON-12%
  2. HELIUM-24.85%                                                                        7.  NITROGEN-0.09%
  3. OXYGEN-0.77%                                                                        8.  SILICON -0.07%
  4. CARBON-0.29%                                                                        9.  MAGNESIUM-0.05%
  5. IRON-0.16%                                                                             10.  SULFUR-0.04%
Something I found that I thought was interesting was that you always hear astronomers talking about the solar "surface," the Sun is actually s hot that it neither liquid or solid matter anywhere inside it. Moving down through the Sun, one continually encounters ever denser and hotter gases.

The Sun only appears to have a surface because most of it's visible light comes from one specific gas layer. This region which is only about 249 miles thick is called the photosphere. The photosphere is the innermost of the three layers comprising the Sun's atmosphere. Because the upper two layers are transparent to most wavelengths of visible light, we see through them down to the down to the photosphere. We cannot, however, see through the shimmering gases of the photosphere, so everything below the photosphere is called the Sun's interior.

Next entry we will continue with The Sun Part II