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CH2Cl2, or dichloromethane has a distorted tetrahedral shape caused by the larger masses of the chlorine atoms compared to the hydrogen atoms. The bond angles between the hydrogen atoms is 112 degrees and 108 degrees between the chlorine atoms.
Approximately 100,000,000. This assumes the atoms are one Angstrom apart, which is actually a little closer than you can pack most of them; for larger atoms, half of that would be a reasonable number.
meter
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It is estimated that there are 10^12 galaxies in the universe, each with about 10^12 stars. Each star has an average of 10^57 hydrogen atoms; using these estimates, the number of particles in the universe would be about 10^82.
they have a big gland in the middle and it makes more atom
Helium atoms
Gemini is not a single star but a constellation. Each of the stars in Gemini "lives" through thermonuclear fusion. Atoms of small nucleii are fused together to produce atoms of larger nucleii while releasing energy.
In nuclear fusion, atoms of hydrogen isotopes such as deuterium and tritium are used to produce helium atoms with larger masses. The fusion reaction involves the combination of these hydrogen isotopes to form helium, releasing a significant amount of energy in the process.
Yes. The sun is one of many stars, and there are even larger stars than the sun. Our sun is just an average star.
Hydrogen atoms are used to produce helium atoms with larger masses in nuclear fusion. During the fusion process, hydrogen isotopes (such as deuterium and tritium) combine to form helium, releasing vast amounts of energy in the process. Oxygen atoms are not typically involved in nuclear fusion reactions to produce helium.
The process at the center of stars is called nuclear fusion. This is the process where hydrogen nuclei fuse together to form helium, releasing a lot of energy in the form of heat and light.
The enormous heat and pressure at the center of a star causes atoms to fuse together, releasing enormous amounts of energy. Most stars fuse hydrogen, but larger stars that have exhausted the hydrogen in their cores may fuse heavy elements.
The sun's energy comes from nuclear fusion, where hydrogen atoms combine to form helium and release energy in the form of light and heat. Gravity within the sun's core keeps the immense pressure and temperature required for fusion to occur, sustaining the sun's fiery state.
The combination of the nuclei of atoms to produce a heavier element is called nuclear fusion. This process releases a large amount of energy and is the main source of power in stars like our sun.
Stars produce nuclear energy by fusion Stars form when contracting dust in a planetary nebula contract and get so hot that nuclear fusion occurs. It explodes, forming a porotostar. Nuclear fusion of hydrogen atoms combining to form helium atoms is what keeps the star glowing.
Atomic fussion, which takes place inside stars and fused Hydrogen atoms together to form Helium atoms. Nuclear fusion