The binding energy per nucleon of deuterium and helium nuclei are 1.1 MeV and 7.0 MeV respectively. When two deuterium nuclei fuse to form a helium nucleus the energy released in the fusion is

The binding energy per nucleon of deuterium and helium atom is 1.1 MeV and 7.0 MeV . If two deuterium nuclei fuse to form helium atom, the energy released is.

The binding energy per nucleon of deuterium and helium atom is 1.1 MeV and 7.0 MeV . If two deuterium nuclei fuse to form helium atom, the energy released is.

The binding energy per nucleon of deuterium and helium atom is 1.1 MeV and 7.0 MeV . If two deuterium nuclei fuse to form helium atom, the energy released is.

The source of energy of stars is nuclear fusion. Fusion reaction occurs at very high temperature, about 10^(7) . Energy released in the process of fusion is due to mass defect. It is also called Q -value. Q = Delta mc^(2), Delta m = mass defect. The binding energy per nucleon of ._(1)H^(2) and ._(2)He^(4) are 1.1 MeV and 7 MeV , respectively. If two deuteron nuclei react to form a single helium nucleus, then the energy released is

The source of energy of stars is nuclear fusion. Fusion reaction occurs at very high temperature, about 10^(7) . Energy released in the process of fusion is due to mass defect. It is also called Q -value. Q = Delta mc^(2), Delta m = mass defect. The binding energy per nucleon of ._(1)H^(2) and ._(2)He^(4) are 1.1 MeV and 7 MeV , respectively. If two deuteron nuclei react to form a single helium nucleus, then the energy released is

The binding energy per nucleon for deuteron (""_(1)H^(2)) and helium (""_(2)He^4) are 1.1 MeV and 7.0 MeV respectively. The energy released when two deuterons fuse to form a helium nucleus is