612C contains 6 protons and 6 neutrons, while 613C contains 6 protons and 7 neutrons. Both are stable, with 612C accounting for 98.89% of the natural carbon in the environment, and with 613C accounting for 1.11% of the natural carbon in the environment.
There are 13 protons in the nuclei of aluminum.
Carbon-14 contains more neutrons compared to carbon-12. Carbon-12 has 6 neutrons, while carbon-14 has 8 neutrons. The number of protons and electrons in both carbon isotopes remains the same, at 6 each.
3
The stable nuclei that are not radioactive include, for example, carbon-12, oxygen-16, and neon-20. These nuclei have a balanced composition of protons and neutrons that do not undergo radioactive decay.
Nuclear fusion occurs when two nuclei fuse together. This is frequently nuclei of deuterium and tritium (both hydrogen isotopes), which form a helium nucleus plus a neutron.
6.023 x 1023
Carbon's atomic number is 6, therefore it's atoms have 6 protons is their nuclei. If the carbon atom is neutral, it will also have 6 electrons, no matter which isotope of carbon it is.
There are 13 protons in the nuclei of aluminum.
It will take practically forever. Carbon-12 is not radioactive.
No, carbon-13 and nitrogen-14 are not the same element. They are different elements with different atomic numbers, which are the number of protons in their nuclei. Carbon-13 has 6 protons, while nitrogen-14 has 7 protons.
Scientists know that the isotopes Carbon-12 and Carbon-14 are both forms of carbon, but they differ in the number of neutrons they contain. Carbon-12 is the most common form of carbon and is stable, while Carbon-14 is radioactive and is used in radiocarbon dating to determine the age of organic materials.
isotopes of carbon
carbon
Carbon-14 contains more neutrons compared to carbon-12. Carbon-12 has 6 neutrons, while carbon-14 has 8 neutrons. The number of protons and electrons in both carbon isotopes remains the same, at 6 each.
it is the nuclei
3
Three helium nuclei, also known as alpha particles, fuse together to form a carbon atom in the process of stellar nucleosynthesis.