black hole and neutron star
The possible final states of a star depend on its initial mass. Low to medium-mass stars, like our Sun, typically end their lives as white dwarfs after shedding their outer layers and forming planetary nebulae. Massive stars can explode in supernovae, leaving behind neutron stars or, if their mass is sufficient, collapsing into black holes. Each final state represents a different evolutionary path influenced by the star's mass and internal processes.
The plan to kill all Jews was called the Final Solution, in which means that the mass murdering of Jews, in 1942 after the Final solution was decided, 3 million jews were murdered in a single year, 8,000+ dying daily.
The "Final Solution" was genocide, mass murder of an entire people.
It was an evil idea. The Final Solution refers to 'The final solution to the Jewish question', ie. what to do with the Jews under German control. This invariably meant mass murder or genocide.
Land, Labor and Capitol
Mass murder, the 'Final Solution' was to kill them, until then other outcomes were explored.
No. If the variable is continuous, for example, height or mass of something, or time interval, then the set of possible outcomes is infinite.
The outcomes of each of the mass extinctions is that animal and/or bacteria die.
High, typically 10 to 70 times (or more) the mass of our own sun.
The possible final states of a star depend on its initial mass. Low to medium-mass stars, like our Sun, typically end their lives as white dwarfs after shedding their outer layers and forming planetary nebulae. Massive stars can explode in supernovae, leaving behind neutron stars or, if their mass is sufficient, collapsing into black holes. Each final state represents a different evolutionary path influenced by the star's mass and internal processes.
7.48
To calculate the initial and final mass in a radioactive decay equation, you would typically use the equation: final mass = initial mass * (1 - decay constant)^time. The initial mass is the quantity of the radioactive substance at the beginning, while the final mass is the amount after a specified amount of time has passed.
For HIGH mass stars- 1. the hydrogen in the core burns until only helium is left. 2. Then the core contracts, while the outer layers expand. 3. It expands into the red-giant stage and 4. then to the super-giant stage. 5. It will finally die in a supernova explosion, 6. leaving behind a white dwarf (if its final mass is less than 1.4 solar masses), a neutron star (if the final mass is between 1.4 and 3 solar masses) or a black hole (if the final mass is more than 3 times that of the Sun).
No, it is not possible for an object's mass to be zero.
The final mass of anhydrous cupric sulfate will be less than the initial mass of hydrated cupric sulfate due to the loss of water during the dehydration process. The final mass can be determined by subtracting the mass of the water lost from the initial mass of the hydrated salt.
High mass.
High mass.