How are Black Holes formed — Reading Comprehension

Supernova explosion, the final stage in the life of a massive star that collapses to form a black hole.

Black holes are one of the most mysterious and extreme objects in the universe. A black hole is not a literal hole, but rather a region in space where gravity is so incredibly strong that nothing, not even light, can escape. This intense gravitational pull is a result of a massive amount of matter being squeezed into an extremely small space. The boundary around a black hole beyond which escape is impossible is called the event horizon. While we cannot see a black hole directly because it absorbs all light, its presence is inferred by observing its powerful effects on surrounding stars and gas.

The most common way for a black hole to form is from the death of a very large star, a process known as stellar collapse. Throughout its life, a star generates energy through nuclear fusion, converting lighter elements like hydrogen into heavier ones. This fusion process creates an outward pressure that perfectly balances the inward pull of gravity. When a massive star, one that is at least ten times the mass of our Sun, runs out of fuel, the fusion process stops. The outward pressure disappears, and gravity takes over, causing the star's core to collapse in on itself at incredible speeds.

This rapid collapse triggers a cataclysmic explosion called a supernova, which blasts the star's outer layers into space. What remains is a super-dense core. If this leftover core is more than three times the mass of our Sun, gravity is so strong that it overcomes all other forces, continuing to compress the matter into an infinitesimally small point called a singularity. This singularity is the heart of the newly formed black hole. The size of the event horizon is directly proportional to the mass of the black hole. The more massive the black hole, the larger its event horizon.

The existence of black holes is supported by Albert Einstein’s theory of general relativity, which describes how mass warps space-time. A black hole’s immense gravity warps space-time so severely that it creates a one-way trip, pulling everything toward the singularity. After formation, black holes can continue to grow by absorbing gas, dust, and even other stars. 
 

Fun Fact: If the Sun were to suddenly become a black hole, its gravity would be the same, and Earth would continue to orbit it just as it does now, though our planet would be plunged into total darkness.

What is the definition of a black hole?

What is the boundary around a black hole called?

What process provides the outward pressure that balances gravity in a star's life?

According to the passage, what type of star can become a black hole?

What event occurs after a massive star's core collapses?

Why can we not see a black hole directly?

Which statement best summarizes the main idea of the passage?

If a star's core after a supernova is less than three times the mass of our Sun, what is a likely outcome, based on the passage?