When an atomic nucleus splits into two or more pieces, the masses of
the pieces doesn't add up to the mass of the original nucleus. There's
always some mass missing, and some energy is always radiated from
the process.
How much energy ? Exactly what you get when you multiply
(the amount of mass that's missing) times ( c2 ) .
Work gives us energy in Joules, which can be subbed back into the first equation to solve for power.
The sun produces energy by the fusion of nuclei of small elements into those of larger elements: for example hydrogen into oxygen. This process involves a loss of mass and that mass is converted into solar energy - in line with Einstein's equation.
This just means to list values of x and then plug them into the equation to find the value of y for that x. so in (x,y) form:(1,8) (2,16) (3,24) and so on.
They fit the equation t = 0 exactly.
When a single heavy nucleus splits into two or more lighter nuclei (fission), the sum of their masses is less than the mass of the original nucleus. Some mass is missing, and some energy is released. When two light nuclei fuse into a single heavier nucleus (fusion), the mass of the heavier one is less than the sum of the masses of the two light ones. Some mass is missing, and some energy is released. In both events, the missing mass has been converted to energy. If the amount of missing mass is 'm', and you multiply 'm' by the square of the speed of light 'c2' , the answer you get is the amount of energy that was released 'e'. e = mc2
a large amount
The mass-energy equation (E=mc^2) relates the energy released in nuclear fission reactions to the small amount of mass that is converted into energy. In nuclear fission, heavy nuclei split into lighter fragments, releasing energy in the process. This energy is a result of the mass defect, where the total mass of the products is less than the original mass of the nucleus, and this mass is converted into energy according to Einstein's equation.
The equation states that energy is directly proportional to mass and that the constant of proportionality is equal to the square of the velocity of light (in vacuum).
The force to energy equation is work force x distance. This equation shows that work is done when a force is applied to an object and causes it to move a certain distance. Work is the transfer of energy from one object to another, and the force to energy equation helps us understand how this transfer occurs.
The flow energy equation is a mathematical expression that describes the energy balance in a fluid flow system. It relates the energy input, output, and losses in the system. This equation helps us understand how energy is transferred and transformed within the system, highlighting the importance of energy conservation and efficiency in the flow process.
The energy loss equation states that the total energy input into a system is equal to the energy output plus any energy lost as heat or other forms. This equation relates to the conservation of energy principle, which states that energy cannot be created or destroyed, only transferred or transformed. By accounting for energy losses, we can ensure that the total energy in a system remains constant, in line with the conservation of energy principle.
Work gives us energy in Joules, which can be subbed back into the first equation to solve for power.
The Fermi energy equation calculates the energy level at which electrons in a material have a 50 probability of being occupied. It is a key factor in determining the behavior of electrons in a material, as it influences properties such as electrical conductivity and thermal conductivity.
The equation Emc2, also known as the "sexed equation," shows that energy (E) and mass (m) are equivalent and can be converted into each other. This means that a small amount of mass can be converted into a large amount of energy, as demonstrated in nuclear reactions like atomic bombs and nuclear power plants.
The sun produces energy by the fusion of nuclei of small elements into those of larger elements: for example hydrogen into oxygen. This process involves a loss of mass and that mass is converted into solar energy - in line with Einstein's equation.
The first law of thermodynamics equation is: U Q - W. This equation states that the change in internal energy of a system is equal to the heat added to the system minus the work done by the system. This equation relates to the conservation of energy in a thermodynamic system because it shows that energy cannot be created or destroyed, only transferred between different forms (heat and work) within the system.
This just means to list values of x and then plug them into the equation to find the value of y for that x. so in (x,y) form:(1,8) (2,16) (3,24) and so on.