carbon
The nuclear process that converts helium and hydrogen into heavier elements is nuclear fusion. In this process, the nuclei of lighter elements combine to form the nuclei of heavier elements, releasing large amounts of energy in the process. This is the process that powers stars like our Sun.
Option 'a' is correct.
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.
The process that converts hydrogen into helium within stars, resulting in the release of large amounts of energy, is called nuclear fusion. In the core of stars, hydrogen nuclei fuse under extreme temperature and pressure conditions, producing helium and releasing energy in the form of light and heat. This energy is what powers stars and enables them to shine for billions of years.
Nuclear fusion, converting hydrogen nuclei into helium nuclei.
Nuclear fusion converts hydrogen atoms into helium atoms. In the fusion process, hydrogen nuclei combine to form helium nuclei, releasing a large amount of energy in the form of heat and light.
The nuclear process that converts helium and hydrogen into heavier elements is nuclear fusion. In this process, the nuclei of lighter elements combine to form the nuclei of heavier elements, releasing large amounts of energy in the process. This is the process that powers stars like our Sun.
B- particles are electrons. They are not Helium nuclei.
Option 'a' is correct.
- hydrogen nuclei waiting to be fused into helium and - helium which has been fused from hydrogen nuclei
The main difference is that hydrogen nuclei have 1 proton whereas helium nuclei have 2 protons. The number of neutrons depends on the "isotope". Usually, a hydrogen nucleus does not have neutrons and is simply a proton. The helium nucleus usually has 2 neutrons.
fusion Josh White apex 2009
The sun's energy is released when nuclear fusion converts hydrogen atoms into energy. This process involves the fusion of hydrogen nuclei to form helium nuclei, releasing large amounts of energy in the form of light and heat.
In the Sun's interior, nuclear reactions primarily involve the fusion of hydrogen nuclei (protons) to form helium nuclei. This process, known as nuclear fusion, releases energy in the form of light and heat. This energy is what powers the Sun and sustains life on Earth.
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.
Nuclear fusion, the source of all the energy so generously radiated by the Sun, does two things: it converts hydrogen into helium (or rather, makes helium nuclei from protons) and it converts mass to energy. ... If the fusion reactions in the core become too weak, a star can and does collapse.
Hydrogen Nuclei