Author Archives: nirng

You Who Came From The Stars

You may know that your body is made of 65% oxygen, 19% hydrogen, and other heavier elements. But do you know where did all these elements come from and how they were generated?

An artist drawing of Big Bang. (via Google)

We know that the current theory states that the universe began with the Big Bang, an event that initially started at an extremely hot and dense point and that point expanded over nearly 14 billion to form the current universe. Right after the Big Bang, the universe contained only free floating subatomic particles such as protons, neutrons, and electrons. When the universe continued to expand, its temperature cooled off. Once the temperature was cool enough for the protons to catch the running electrons in this colder than before, yet still boiling universe, the first hydrogen atom formed. Similarly, helium and lithium were generated by the collision of protons and neutron. By that time the universe was made of mostly hydrogen, helium and trace amount of lithium.

After another long period of time, the region of the universe that was slightly higher in density started to attract any mass to form gas cloud by the force of gravity. As this cloud of mass got denser, it attracted even more mass. Eventually, the core became dense and hot enough for hydrogen atoms fusing together to form helium atoms and generating enormous amount of energy. Nowadays, we call this cloud of gas a star. As a star grows, more fusion reaction happened and more helium were generated. When there was enough helium accumulated in the core, all these helium started to fuse together and form carbon. After that, when there was enough carbon, oxygen started to form. This process continued until iron was formed.

An Image of Our Sun ( via Wikipedia)

An image of our Sun ( via Wikipedia)

Unfortunately, the stars can’t generate any heavier element than iron. This is because the nature of iron fusion does not produce energy  but consume energy. Hence, when a star started to fuse iron, its core lost the pressure-gradient force against its gravity and the core collapsed. The result was a supernova: a stellar explosion.

An Image of Our Sun ( via Wikipedia)

Kepler’s Supernova ( via Wikipedia)

That was the moment the rest of the period table elements were filled!

During supernova, atoms were exposed in more extreme temperature and pressure, allowing the formation of elements beyond iron in just a few second. Then, the star exploded into a cloud of gas: nebula.

 

Eagle Nebula (via Wikipedia)

This newly formed nebula can now give the raise of another star or stars and the debris that rotate around the newly formed star would become a planet and elements that you find on a planet, including yourself.

Now you can tell your friends that your body was once the core of stars.

By William Yang

Pluto 1930 – 2006

In 2006, thousands of astronomers around the world gathered in Praha to vote for the fate of the ninth planets in our solar system, Pluto. 76 years after its discovery, the planet was removed from the list of the nine planets in our solar system. This may not be new to you, but do you know why was Pluto demoted?

Prior to the discovery of Pluto, astronomers had mathematically predicted the existence of a ninth planet based on the perturbed orbital motions of Neptune and Uranus. After tracing the shadows of the planets for several decades, in 1930, astronomers finally confirmed that they had found the ninth planet, Pluto. It is only approximately 0.21 percent of Earth’s mass and it has five known moons. Pluto seems to share all the properties of the other eight planets, except for one: it has a very eccentric orbit.

Pluto under a 14” telescope from Earth. Photo credit : via Google

Over the span of half a century, telescopes are starting to get more advanced. As a result of that, astronomers have accomplished observing more than 10,000 of the small asteroids or icy bodies with a radius over 100km around the orbits of Pluto. The radius of the largest asteroids discovered, Eris, is 27 percent greater than that of Pluto. Astronomers began having problems classifying these huge asteroids. Hence, they decided to vote on the definition of a planet on the 26th General Assembly for the International Astronomical Union in 2006.

The new definition of a planet is given that

  1. The celestial body must orbits around the Sun
  2. It must have enough gravity to pull itself into a spherical shape
  3. It must have cleared all other celestial bodies on its orbit
  4. Any non-satellite body that meet the first two requirements but not the third one is classified as a dwarf planet.

What would happened if the definition of a planets is unclear. Photo credit: Flickr user Wesley Fryer via Flickr

Now let’s see if Pluto meets the above requirements.

We know that it orbits around the Sun and maintains itself in a spherical shape. Although the first two requirements are met, it does not meet the last one as it has over thousands of asteroids on its orbit. Soon after the approval of the new definition of a planet, Pluto was crossed out from the list of planets in our solar system. However, this dwarf planet, Pluto, will still be orbiting in our solar system for a long time.

To learn more about classification of Pluto, here is a short video.

YouTube Preview Image

 

Written by: William Yang