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Element Family Tree (Hydrogen (H) (Carbon (C) (Aluminium (Al) (Uranium (U)…
Element Family Tree
Hydrogen (H)
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Hydrogen was formed within the first few minutes of the Big Bang through the combination of one proton and one electron.
Carbon (C)
Aluminium (Al)
Uranium (U)
The core of a supermassive star rapidly collapses from tens of thousands of kilometers to only 20 kilometers in diameter. The process is so violent that the protons and electrons fuse into neutrons in the core. The more massive of the massive stars will rebound so hard that the core collapses further and becomes a black hole. The less massive will leave behind a ball of neutrons, forming a neutron star. During this process of contraction, collision, and rebound, the outer layers mix with one another, colliding violently and forming atoms larger than iron.
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Protons: 92
Neutrons: 146
Electrons: 92
Uranium is weakly radioactive.
Uranium has the highest atomic weight of the primordially occurring elements.
Its density is about 70% higher than that of lead.
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Protons: 13
Neutrons: 14
Electrons: 13
Aluminum is part of the post-transition metals column.
Aluminum is a silvery-white, soft, nonmagnetic and ductile metal in the
boron group.
Aluminum has a boiling point of 2,470 °C
Stars that are three times the mass of the Sun or greater have a greater gravitational pull that leads to greater temperatures and the ability to fuse carbon, oxygen, and nitrogen further. The final fusion processes last only about 12 hours in the most massive stars until the fusion into iron begins.
As the star is in its Main Sequence Stage, the hydrogen fuel source continues to run out. This causes temperatures to increase and giving the right conditions for helium fusion to occur. Helium then fuses into Carbon.
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Protons: 6
Neutrons: 6
Electrons: 6
Carbon has several allotropes, or different forms in which it can exist.
It is highly unreactive under normal conditions.
It has an exceptional ability to bind with a wide variety of other elements.
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Protons: 1
Neutrons: 0
Electrons: 0
Hydrogen is a colorless, odorless, tasteless, non-toxic, nonmetallic gas.
It burns in air or oxygen to produce water.
It is highly flammable.
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Helium (He)
Instantaneous, right after the Big Bang,
Very hot and dense conditions provided a place for nuclear fusion to begin. With the force of gravity and very strong pressure squeezing in, hydrogen nuclei combined to form helium.
Helium was formed within the first few minutes of the big bang through the combination of protons, neutrons and electrons.
Oxygen (O)
Magnesium (Mg)
Gold (Au)
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Protons: 79
Neutrons: 118
Electrons: 79
Gold has one of the higher atomic numbers for natural elements.
It is one of the least reactive chemical elements.
Gold is solid under standard conditions.
The core of a supermassive star rapidly collapses from tens of thousands of kilometers to only 20 kilometers in diameter. The process is so violent that the protons and electrons fuse into neutrons in the core. The more massive of the massive stars will rebound so hard that the core collapses further and becomes a black hole. The less massive will leave behind a ball of neutrons, forming a neutron star. During this process of contraction, collision, and rebound, the outer layers mix with one another, colliding violently and forming atoms larger than iron.
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Stars that are three times the mass of the Sun or greater have a greater gravitational pull that leads to greater temperatures and the ability to fuse carbon, oxygen, and nitrogen further. The final fusion processes last only about 12 hours in the most massive stars until the fusion into iron begins.
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Protons: 12
Neutrons: 12
Electrons: 12
Magnesium is a metal, more specifically, an alkaline earth metal.
It is a shiny gray solid which bears a close physical resemblance to the other five elements in the second column.
Magnesium is the ninth most abundant element in the universe.
As the star is in its Main Sequence Stage, the hydrogen fuel source continues to run out. This causes temperatures to increase and giving the right conditions for helium fusion to occur. Helium then fuses into Oxygen.
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Protons: 8
Neutrons: 8
Electrons: 6
Oxygen is extremely reactive and forms oxides with nearly all other elements except noble gases.
Plants create oxygen.
Plants and animals rely on oxygen for respiration. Oxygen is frequently used to help breathing in patients with respiratory ailments.
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Protons: 2
Neutrons: 2
Electrons: 0
Helium is a light, odorless, colorless, inert, monatomic gas.
It has a low-boiling point, low density and low solubility.
Helium is the gas used to fill balloons to float in the air.
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