Thursday, February 6, 2020

Solar Chemistry

Solar ChemistrySolar Chemistry is quite the advanced science as it examines the behavior of atoms in the solar spectrum. It uses special spectrographs and a solar microscope to capture images of light from the sun's surface.Solar Chemistry first began as a reaction to apply to the study of crystals by Georgius Agrippa who, in 1551, had made many discoveries regarding the structure of water. The system then expanded to include other crystals, plants, animals, and even living things. It can be said that Agrippa was the first to understand that minerals were actually composed of smaller components, each of which were in contact with one another through chemical reactions.The reaction was simple in that the smaller minerals were attracted to each other and caused them to mix with the larger ones to form a crystal. This was done because a major factor in this process was the connection that mineral forms could make with the absorption of light by the grains.There are many phenomena in Sol ar Chemistry that are used in many laboratories and home laboratories. One example of this is the 'Chlorophyll' of plants. This molecule is responsible for the absorption of sunlight by plants.The two types of chlorophyll molecules are named A and B. These A and B molecules can be treated as opposites, A being fixed and B being polar. In normal circumstances, the molecule would absorb energy from the sun.However, when these chlorophyll molecules absorb more energy, the atoms in it move closer together creating the effect of a 'bonding' in this particular molecule. This bond will cause the molecules to vibrate more efficiently and this in turn will cause them to absorb energy in the same manner.All of the atoms, including the nitrogen atom in a hydrogen atom, move in the same direction when these bonds occur. This means that the number of electrons, either positive or negative, will change depending on the amount of absorption in the molecule. All of this results in different types o f atoms and this is the basis of what is called the 'spectrum' of solar chemistry.

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