Star Formation and Evolution Quiz
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Questions and Answers

What marks the transformation of a protostar into a main-sequence star?

  • Formation of an accretion disk
  • Collapse under gravity
  • Initiation of nuclear fusion (correct)
  • Explosion into a supernova

All stars last the same amount of time on the main sequence.

False (B)

What occurs when the hydrogen in a star's core is depleted?

The star leaves the main sequence.

A core with a mass exceeding 3 times that of the Sun will collapse into a __________.

<p>black hole</p> Signup and view all the answers

Match the outcomes of a star's core collapse with their conditions:

<p>Neutron Star = Core mass between 1.4 and 3 times the mass of the Sun Black Hole = Core mass exceeds 3 times the mass of the Sun Supernova = Result of rapid core collapse Main-sequence Star = Star after becoming a protostar</p> Signup and view all the answers

Flashcards

Star formation

Stars are born from collapsing clouds of gas and dust called nebulae.

Main Sequence Star

A star that fuses hydrogen in its core, being a stable phase.

Supernova

Powerful explosion marking a massive star's demise.

Neutron Star

Denser star formed after the supernova of a huge star if its core mass is 1.4-3 times of the Sun.

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Black Hole

An extremely dense remnant of an exploding star whose gravity is so strong that nothing, not even light, can escape.

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Study Notes

Star Formation and Evolution

  • Stars form in nebulae, vast clouds of gas and dust.
  • Gravity causes these clouds to collapse, creating a protostar.
  • Nuclear fusion ignites in the protostar's core, transforming it into a main sequence star.

Main Sequence Star Lifespan

  • Star lifespan depends on mass; larger stars burn faster.
  • Hydrogen fuel eventually depletes, causing the star to leave the main sequence.

Massive Star Evolution

  • Massive stars fuse successively heavier elements (like helium, carbon, and oxygen).
  • Fusion progresses to iron, where energy production stops.
  • Core collapse triggers a supernova explosion.

Stellar Remnants

  • Neutron Star: A core between 1.4 and 3 times the Sun's mass collapses into a neutron star.
  • Black Hole: A core exceeding this mass collapses into a black hole, an incredibly dense region with immense gravitational pull. Light cannot escape its gravity.

Black Holes in Detail

  • Black holes warp spacetime around them.
  • Accretion disks form when black holes draw in matter, heating and glowing.
  • Black holes' presence is understood through the effects they have on their surroundings.

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Test your knowledge on the processes involved in star formation and evolution. Explore concepts like the life cycle of stars, from protostars to black holes, and understand how gravity and nuclear fusion play crucial roles in their development.

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