SPACE

Introduction and Chemical Elements in Space

Introduction and Chemical Elements in Space

Introduction to Space

The Universe began about 13 billion years ago after the Big Bang. At first, the Universe was a hot ball of matter and radiation. However, as it expanded it got cooler and now it’s cold and dark, all apart from the stars. When you look out at night the stars that you see are part of our Milky Way. The closest star to Earth is the Sun but there are billions of other stars that make up the Milky Way. There are also billions of other galaxies, all separated by empty space. From these galaxies, it has taken billions of years for light to reach us on Earth.

As the Universe expanded, it also became transparent. Between the empty space of the atoms radiation was able to pass through. This period of time, known as the Dark Age of the Universe, is when background microwave radiation was formed. For a few billion years the Universe was only dark, empty space, filled with helium and hydrogen. After that, the stars and galaxies appeared.

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Chemical elements in space

Light elements were created due to fusion within stars. Hydrogen, helium and sometimes carbon, which contains small nuclei, fuse together. During the red giant stage larger nuclei form due to fusion with helium and other elements with small nuclei. Nuclear fusion then stops once iron is formed as too much energy is required to fuse this element.

Physics GCSE science revision- SpaceHeavy elements are formed from supernovas. The huge amount of pressure which occurs when the white dwarf collapses causes small nuclei to fuse forming large nuclei. These nuclei are bigger than iron. The explosion scatter the star debris throughout space and this debris consists of all the elements, from the lightest to the heaviest. When the debris are brought together again a new star can be born.

Planets are formed in a similar way, from supernova debris being brought together by gravity. This means that planets are also formed from all the known elements. Uranium is the heaviest known element and has a radioactive half-life of 4,500 million years. This is proof that Earth must have been formed from a supernova explosion.

Attempts are being made today to see if there could be, or is, other life in space. Two ways in which this is being done are:

  • Physics GCSE science revision- Spacespace probes have been sent to Mars to try and detect chemicals and microbes in the soil, rocks and atmosphere which might signify life
  • radio telescopes are used in the Search for Extra-Terrestrial Intelligence (SETI) to search for technological signals from other life forms however, for the last four decades, nothing has been picked up yet