How does a Sun-like star become a white dwarf?
A Sun-like star sheds its outer layers, leaving a hot, compact core that gradually cools and fades without sustained fusion.
Study 07 Stellar Endings and Cosmic Recycling with 12 free online flashcards. Review key terms, definitions, and concepts with this interactive flashcard deck.
How does a Sun-like star become a white dwarf?
A Sun-like star sheds its outer layers, leaving a hot, compact core that gradually cools and fades without sustained fusion.
What supports a white dwarf, and what is its approximate mass limit?
Electron degeneracy pressure supports a white dwarf against gravity. It cannot remain stable above about 1.4 solar masses, the Chandrasekhar limit.
What happens to a white dwarf during a nova?
A nova is a surface eruption on a white dwarf that ejects material but leaves the white dwarf intact.
What is the defining outcome of a Type Ia supernova?
A Type Ia supernova is a thermonuclear explosion that destroys a white dwarf in a binary system.
Why can an iron-rich stellar core collapse?
Iron fusion does not release energy to support the core, so an iron-rich core in a sufficiently massive star can collapse rapidly.
What makes a neutron star extraordinarily dense?
A neutron star packs more mass than the Sun into a sphere about 20 kilometers across, made mostly of neutron-rich matter.
What produces the repeating signals of a pulsar?
A pulsar is a rotating neutron star whose beams of radiation sweep across Earth like a lighthouse.
What defines a black hole's event horizon?
A black hole is so compact that nothing, not even light, can escape from inside its event horizon.
How can astronomers detect a stellar-mass black hole indirectly?
Astronomers infer stellar-mass black holes from gravitational effects, such as a companion star's motion, or from radiation emitted by hot gas in an accretion disk.
What happens in a core-collapse supernova?
A core-collapse supernova follows the collapse of a massive star's core, expelling outer layers; the remnant may be a neutron star or black hole.
How does fusion build elements inside massive stars?
During a massive star's life, fusion builds elements from lighter nuclei through the iron group.
Where does the s-process build some heavy elements?
The slow neutron-capture process, or s-process, builds some heavy elements in evolved stars.