Low Mass Stars: Crash Course Astronomy #29
CrashCourse・12 minutes read
Stars are violent thermonuclear generators that sustain themselves and our existence, with low mass stars like red dwarfs lasting for trillions of years by slowly fusing hydrogen into helium. High mass stars, on the other hand, fuse hydrogen more quickly and will eventually expand into red giants before cooling off and fading over billions of years.
Insights
- Stars, despite their beauty, are actually violent thermonuclear generators sustaining themselves and our existence through energy creation.
- The categorization of stars into low mass and high mass groups, determined by the mass of around eight solar masses, dictates their fusion rates, lifespans, and eventual evolution into red giants or white dwarfs.
Get key ideas from YouTube videos. It’s free
Recent questions
What sustains stars like the Sun?
Fusion of hydrogen into helium generates energy.
Related videos
Free School
All About Stars for Kids: Astronomy and Space for Children - FreeSchool
Cognito
GCSE Physics - The Life Cycle Of Stars / How Stars are Formed and Destroyed #84
Institute of Physics
The Life Cycle of Stars
StarTalk
Why Neil deGrasse Tyson and Emily Rice Think You Should Pay Attention to Low-Mass Stars
Professor Dave Explains
The Life and Death of Stars: White Dwarfs, Supernovae, Neutron Stars, and Black Holes
Summary
00:00
Stellar Evolution: From Fusion to White Dwarfs
- Stars in the sky are beautiful but are actually violent thermonuclear generators that create energy to sustain themselves and our existence.
- Stars can be categorized into low mass and high mass groups, with the dividing line around eight times the mass of the Sun.
- Low mass stars like red dwarfs fuse hydrogen into helium in their cores, generating energy that sustains them for trillions of years.
- Red dwarfs have slow fusion rates, allowing them to shine for a long time as hydrogen mixes throughout the star.
- High mass stars fuse hydrogen more quickly due to higher pressure in their cores, leading to a faster depletion of fuel.
- Stars like the Sun will eventually expand, becoming red giants as they run out of hydrogen and start fusing helium into carbon.
- Red giants lose mass, cool off, and eventually turn into white dwarfs, cooling and fading over billions of years.
- Planetary nebulae form from stars with more mass than the Sun before they die, showcasing a different phase of stellar evolution.
- The Earth will not survive the Sun's expansion into a red giant, likely getting cooked and eventually engulfed by the Sun.
- The Sun's evolution into a red giant will not occur for billions of years, providing ample time for humanity to potentially explore other planets.
11:49
"Team behind project: Thaller, Jenkins, Sweeney, Aranda"
- Michelle Thaller is the director
- Nicholas Jenkins directed the project
- Nicole Sweeney handled the editing
- Michael Aranda is the sound designer
- Thought Café is responsible for the graphics
