Neon belongs to the group of elements known as noble gases. Noble gases are colorless, odorless, and generally inert gases that rarely react with other elements or compounds. Neon, specifically, is known for its bright orange-red glow when electrically charged, which is why it is used in neon signs and lighting. Noble gases have full outer electron shells, making them stable and unreactive under normal conditions. This stability makes neon and other noble gases valuable in various applications, such as in lighting, electronics, and as a shielding gas in welding.

The atomic weight of copper is approximately 63.546 atomic mass units (u). This value represents the average mass of copper atoms, taking into account the isotopic composition of naturally occurring copper. Copper has two stable isotopes, copper-63 and copper-65, with copper-63 being the more abundant. The atomic weight is crucial in various scientific applications, including chemistry, physics, and materials science, as it influences calculations involving stoichiometry and the properties of compounds containing copper.

The atomic mass for Nitrogen is 14. This is because the atomic mass of an element is the weighted average mass of all its isotopes, taking into account the abundance of each isotope. Nitrogen has two main isotopes: Nitrogen-14 and Nitrogen-15. Nitrogen-14 is the most abundant isotope, making up about 99.6% of natural nitrogen. Nitrogen-15 is less abundant. By calculating the weighted average of these isotopes, we arrive at an atomic mass of 14 for Nitrogen.

The atomic number of an element is the number of protons in its nucleus. Nitrogen has an atomic number of 7, meaning each nitrogen atom contains seven protons. This places nitrogen in group 15 and period 2 of the periodic table. Nitrogen is a non-metal and makes up about 78% of the Earth's atmosphere. It is essential for all living organisms as it is a key component of amino acids, proteins, and nucleic acids. Understanding atomic numbers is crucial for identifying elements and predicting their chemical properties and behavior based on their position in the periodic table.

Hydrogen is the most abundant element in the universe. It makes up about 75% of the elemental mass of the universe. Hydrogen is a colorless, odorless gas and the simplest element, consisting of just one proton and one electron. It is found in stars, gas giant planets like Jupiter and Saturn, and in vast interstellar clouds of gas and dust. In stars, hydrogen undergoes nuclear fusion to form helium, releasing energy in the process. This abundant presence of hydrogen in the universe is fundamental to our understanding of stellar evolution, cosmology, and the formation of galaxies and solar systems.