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PHYSICAL SCIENCE

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PHYSICAL SCIENCE
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  • Good morning, Eli! What do you think will be our lesson for today?
  • Good morning, John! I don't know yet but we'll see.
  • Wait, I remember! Our science teacher mentioned that we're going to discuss about the origin of the elements.
  • There are a lot of theories that revolves around the origin of the elements that might be discussed later.
  • Do you have anything in the origin of the elements that amuses you most?
  • Of course! It is the Stellar Nucleosynthesis.
  • There are still a lot of things about it and I know our teacher will mention it.
  • Stellar Nucleosynthesis is the creation of chemical elements by nuclear fusion reactions within stars. Stellar nucleosynthesis has occurred since the original creation of hydrogen, helium and lithium during the Big Bang.
  • Can I ask what Stellar Nucleosynthesis is all about?
  • The elements created in stellar nucleosynthesis are are hydrogen (H), carbon (C), nitrogen (N), oxygen (O), phosphorous (P), sulfur (S), chlorine (Cl), sodium from natrium (Na), magnesium (Mg), potassium from kalium (K), calcium (Ca), and iron from ferrum (Fe).
  • The phrase "stellar nucleosynthesis" refers to the nuclear events that occur in stars to create the nuclei of heavier elements. Stellar nucleosynthesis is the process by which chemical elements are created within stars through nuclear fusion processes. Stellar nucleosynthesis has happened since the Big Bang's first generation of hydrogen, helium, and lithium.
  • There are still a lot of things to be discussed about Stellar Nucleosynthesis.
  • Thank you, ma'am! I understood the main idea about what Stellar Nucleosynthesis is.
  • I am looking forward to our next discussion, ma'am!
  • But what I recently discussed only cover some of the main parts invovling the topic.
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