Super Mario Galaxy

Nuclear Fusion and the Remains of a Dead Star Throughout the history of Earth, multicellular organisms rely on one thing, the sun. And throughout the observable universe, there are million of stars out there just like our sun. These stars could be different however, with either more mass, volume, heat, etc. In our high school career, we learn a lot about astronomy, such as the order of the planets in our solar system. We also learn about gravity, rotation of planets, and how long it takes…

In 1964 a physicist by the name of Peter Higgs took some ideas that were floating around at the time, added an insight or two of his own, and proposed that there was an energy field that permeated the entire universe. This energy field is now called the Higgs filed. The reason he proposed this field was that nobody understood why some subatomic particles had a great deal of mass, while others had little and some had none at all. The energy filed that Higgs proposed would interact with the…

Picture you are on Earth 5 billion years into the future. The sun is closing in on Earth and the Earth is burning up. What are you going to do? This is why it is so important to explore space, because humans could go extinct if we don’t find another planet to colonize on before the sun swallows Earth. Also, space has helped us learn about the moon and even Earth. I take the position that we should explore outer space instead of exploring underwater because eventually we will have to evacuate…

William Herschel was not an astronomer when he discovered Uranus. He was actually a musician and teacher. He looked at the stars as a hobby. However, he used a method different than most star gazers of the time. He mapped out the stars in relation to each other, instead of the traditional grid method used at the time (Smith 2013). He started out by studying the Society papers on natural history and matter theory, after he joined the Bath Philosophical Society in 1780. He also reached out to the…

dust in outer space. A primeval is standing for the earliest ages in the history of the world. This means Primeval nebula means a cloud of gas and dust in outer space a long time ago. It was how people think the galaxy was created. This is saying that the universe was always there. The galaxy was created. Then all the stars and planets were created. They were all made from small clouds of dust and gas in space. The nebular hypothesis is the most widely used theory for the formation of the…

HR Diagrams The Hertzsprung-Russell Diagram, otherwise known as HR diagram, is a graph that shows many patterns and properties of stars based on plotting them by their temperature on the surface and their light they emit, or luminosity. Created in 1912, the HR diagram was made by two astronomers, Ejnar Hertzsprung and Henry Russell who found patterns with stars’ properties. The Hertzsprung-Russell Diagram shows how every star goes through different evolutionary stages. These evolutionary stages…

How many things can you see in the night sky? A lot! On a clear night you might see the moon, some planets, and thousands of sparkling stars. You can see even more with a telescope. You might see stars where before you only saw dark space. You might see that many stars look larger than others. You might see that some stars that look white are really red or blue. With bigger and bigger telescopes you can see more and more objects in the sky and you can see those objects in more and more detail.…

William Huggins was an amazing contribution to the rise of astronomy. When Huggins was born in Cornhill, England on February 7, 1824. A bit later in life, Huggins married Margaret Lindsey who also had an affinity for astronomy. She persuaded her husband to continue his work and together they became a dynamic duo of astronomers. Somewhere towards the middle of his life, William Huggins built an observatory on top of the roof of his own house. At this time, he lived in Tulse Hill, England. The…

In the mid 20-ies of the last century the American astronomer E. Hubble found that the distance between galaxies in the observable universe is continuously increasing, like galaxies diverge from each other. At Hubble and his colleagues began to form the impression that the many billions of years ago in our days talking about 15 - 20 billion of the universe matter was concentrated in a very small volume with a fantastically high density, many orders of magnitude superior to the density of matter…

it? The observable universe is about 90 billion light years in diameter. There are at least one hundred billion galaxies, each with one hundred to one thousand billion stars. Recently, we've learned that planets are very common too. And that there are probably trillions and trillions of habitable planets in the universe. This leads…