Stellar Mid-Life and Old Age

0.0(0)
studied byStudied by 0 people
0.0(0)
linked notesView linked note
full-widthCall Kai
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
GameKnowt Play
Card Sorting

1/15

flashcard set

Earn XP

Description and Tags

These flashcards cover essential vocabulary and concepts related to stellar evolution, specifically focusing on life stages, fusion processes, and end-of-life outcomes for stars.

Study Analytics
Name
Mastery
Learn
Test
Matching
Spaced

No study sessions yet.

16 Terms

1
New cards

Stellar Mid-Life

The phase in a star's life cycle where it faces a balance between outward pressure and the inward pull of gravity.

2
New cards

Core Fusion

The process of nuclear fusion at the core of a star, which creates energy that counteracts gravitational collapse.

3
New cards

Luminosity

The total amount of energy radiated by a star per unit time.

4
New cards

Main Sequence Star

A stage in stellar evolution where stars spend most of their lives fusing hydrogen into helium.

5
New cards

Post-Main Sequence

The phase after a star exhausts hydrogen in its core, leading to changes in temperature and luminosity.

6
New cards

Triple-alpha Process

A set of nuclear fusion reactions by which helium is converted into carbon in the cores of stars.

7
New cards

Asymptotic-Giant Branch

A late phase in the life cycle of a star where helium fusion ceases and the star becomes a red supergiant.

8
New cards

Neutron Star

A compact star composed primarily of neutrons, formed from the remnants of massive stars after a supernova.

9
New cards

Supernova

An astronomical explosion that occurs at the end of a massive star's life cycle, resulting in the ejection of the outer layers.

10
New cards

Planetary Nebula

A shell of gas expelled from a star during the late stages of stellar evolution, leading to the formation of a white dwarf.

11
New cards

Iron Core

The final stage of nuclear reactions in massive stars, marking the end of fusion processes as it has no more nuclear energy.

12
New cards

Horizontal Branch

A phase in the stellar evolution when a star burns helium in its core after hydrogen fusion has ended.

13
New cards

Red Giant Branch

The region of the Hertzsprung-Russell diagram where stars expand and cool after exhausting hydrogen in their cores.

14
New cards

Chemical Composition of Star Clusters

The common elements and isotopes found in stars within the same cluster, indicating their similar formation history.

15
New cards

Shell Fusion

Nuclear fusion that occurs in a shell surrounding the stellar core, often after the core's fusion has ended.

16
New cards

Main-Sequence Life Span

The duration a star spends in the main-sequence phase, dependent on its mass and fuel consumption.