The formation of our solar system was triggered by the collapse of a giant molecular cloud, leading to the creation of the Sun and its surrounding planets.
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Star formation requires a triggering event because the gas and dust in space need a disturbance, such as a shockwave or gravitational collapse, to overcome their natural tendency to remain diffuse and form into dense clumps that can eventually collapse and form stars.
The keyword density of a black hole is significant in understanding its gravitational pull and impact on surrounding objects because it indicates the concentration of mass within the black hole. A higher keyword density implies a stronger gravitational pull, which can have a greater impact on nearby objects by bending light, distorting space-time, and potentially pulling objects into the black hole's event horizon.
In a chain reaction, a series of events occur where each event triggers the next event, leading to a self-sustaining reaction. This propagation through a system happens as each event releases energy or particles that cause subsequent events to occur, creating a domino effect. This can result in a rapid and exponential increase in the reaction, potentially leading to a large-scale impact on the system.
When momentum is conserved, it means that the total momentum of a system before an event is equal to the total momentum after the event, as long as there are no external forces acting on the system. This principle is based on the law of conservation of momentum, which states that in a closed system, momentum remains constant before and after a collision or interaction.
Linear momentum is conserved in a closed system when there are no external forces acting on it. This means that the total linear momentum of the system before an event is equal to the total linear momentum after the event.