Free Online Flashcard Deck

07 Stellar Endings and Cosmic Recycling Free Online FlashCards

Study 07 Stellar Endings and Cosmic Recycling with 12 free online flashcards. Review key terms, definitions, and concepts with this interactive flashcard deck.

12 cards
01
Front

How does a Sun-like star become a white dwarf?

Back

A Sun-like star sheds its outer layers, leaving a hot, compact core that gradually cools and fades without sustained fusion.

02
Front

What supports a white dwarf, and what is its approximate mass limit?

Back

Electron degeneracy pressure supports a white dwarf against gravity. It cannot remain stable above about 1.4 solar masses, the Chandrasekhar limit.

03
Front

What happens to a white dwarf during a nova?

Back

A nova is a surface eruption on a white dwarf that ejects material but leaves the white dwarf intact.

04
Front

What is the defining outcome of a Type Ia supernova?

Back

A Type Ia supernova is a thermonuclear explosion that destroys a white dwarf in a binary system.

05
Front

Why can an iron-rich stellar core collapse?

Back

Iron fusion does not release energy to support the core, so an iron-rich core in a sufficiently massive star can collapse rapidly.

06
Front

What makes a neutron star extraordinarily dense?

Back

A neutron star packs more mass than the Sun into a sphere about 20 kilometers across, made mostly of neutron-rich matter.

07
Front

What produces the repeating signals of a pulsar?

Back

A pulsar is a rotating neutron star whose beams of radiation sweep across Earth like a lighthouse.

08
Front

What defines a black hole's event horizon?

Back

A black hole is so compact that nothing, not even light, can escape from inside its event horizon.

09
Front

How can astronomers detect a stellar-mass black hole indirectly?

Back

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.

10
Front

What happens in a core-collapse supernova?

Back

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.

11
Front

How does fusion build elements inside massive stars?

Back

During a massive star's life, fusion builds elements from lighter nuclei through the iron group.

12
Front

Where does the s-process build some heavy elements?

Back

The slow neutron-capture process, or s-process, builds some heavy elements in evolved stars.