A pure substance that represents the species (variety) of a specific atom
Isotopes
Atoms of the same element but with different atomic mass (different number of neutrons)
Element
Identity of an atom
Atom
Shows the variety of an element
Proton
Positively charged particle located in the nucleus along with the neutron
Neutron
Uncharged particle
Electron
Negatively charged particle located around the nucleus
There are many theories to explain the origin of the Universe, but the most sound is the BIG BANG
Big Bang Theory
Postulates that the universe emerged from a state of enormous density and energy. Everything came from a single point and expanded to now what we call the universe.
Georges Lemaitre
Proposed the Big Bang theory
Georges Henri Joseph Édouard Lemaître: 'A French priest and was coined for the idea of the expanding universe.'
Evidences of the Big Bang
Cosmic expansion, discovered by Edwin Hubble
Cosmic Microwave Background, discovered by George Gamow
Primordial or Big Bang Nucleosynthesis
Nucleosynthesis
The formation of atomic nuclei (center of atoms protons and neutrons)
Nucleosynthesis occurred right after the Big Bang
Nucleosynthesis
Started as quarks forming the protons and neutrons
Types of Nucleosynthesis
Big Bang Nucleosynthesis
Stellar Nucleosynthesis
Supernova Nucleosynthesis
Stars
Must have energy to exist for a certain length of time
Energy source of stars
1. Nuclear fusion reactions between light elements
2. Release of a huge amount of energy
3. Keeps the star hot
Atoms collide and alters atomic structures and releases an enormous quantity of energy
The energy release is manifested as the light emitted by the stars
Nuclear fusion in the core of a star
Hydrogen is converted to helium
As stars age they run out of fuel
Massive stars undergo supernova (explosion of a star)
The explosion results in the formation of elements heavier than iron, Fe
Big Bang Nucleosynthesis
Formation of light elements, Hydrogen and Helium by combination of protons and neutrons right after the Big Bang
Lithium was also formed through Big Bang Nucleosynthesis
Stellar Nucleosynthesis
Formation of elements in the stars' interior
Occurs through nuclear fusion and electron capture
Responsible for the formation of elements heavier than Helium, He until Iron, Fe
Two types of Neutron Capture
s-process (slow)
r-process (rapid)
process (slow)
Addition of neutron is so slow that beta decay happened before another neutron is added to the nucleus
r-process
Fast capture of neutron before radioactive decay occurs
Astrochemist
Part Astronomer and part Chemist who intensely studies the periodic table within the context of space rather than of Earth
Astrochemists
Observe stars
Examine, analyze, and dissect stars
Study the different aspects of all the fascinating objects in the universe on a molecular level
Aim to answer questions how they were formed
s-process
Happens when there is slow rate of capturing neutron while there is a faster rate of radioactive decay
Stellar nucleosynthesis
Process by which elements are created within stars
Tri-Alpha process
Conversion of helium nuclei to carbon
Supernova nucleosynthesis
Process by which heavier elements after iron are formed
Proton-proton chain
Nuclear fusion reaction where hydrogen is converted to helium