11-16-2025, 07:15 PM
⭐ How Stars & Galaxies Evolve Over Billions of Years
Stellar & Galactic Dynamics — The Lumin Archive
? Overview
Stars and galaxies are not static objects — they are living systems constantly
changing over cosmic time.
This thread explains:
• How stars evolve from birth → death
• How galaxies form, grow, merge, and reshape
• Why the universe looks the way it does today
Clear diagrams and simple explanations included.
? 1. The Lifecycle of a Star — The Quick Map
A star's path depends mainly on ONE number:
Its mass.
Diagram:
Key idea:
Bigger stars burn hotter, faster, and die violently.
? 2. How Galaxies Evolve
Galaxies grow through:
✔ Gas accretion
✔ Star formation
✔ Mergers (small & large)
✔ Supermassive black hole feedback
ASCII Diagram:
Major mergers destroy spirals and create giant elliptical galaxies.
? 3. Star Formation Rate Over Time
The universe had a “Golden Age” of star formation.
• Peak: 10 billion years ago
• Now: only ~5–10% of that rate
• Future: slow decline until star formation stops completely
Graph (conceptual):
? 4. Galactic Rotation & Dark Matter
Stars orbit the galactic center too fast for the visible mass alone.
This requires:
Dark matter.
Rotation curve diagram:
? Summary
• Stars evolve based on mass — small stars live long, big stars die fast
• Galaxies constantly grow, merge, and reshape
• Dark matter is required to explain galaxy rotation
• The universe is slowing down in star formation but still evolving
If you want deeper sections (supernova types, galaxy clusters, mergers),
just reply and I’ll expand this into a multipart series.
Written for The Lumin Archive — Clear, accessible science for all.
Stellar & Galactic Dynamics — The Lumin Archive
? Overview
Stars and galaxies are not static objects — they are living systems constantly
changing over cosmic time.
This thread explains:
• How stars evolve from birth → death
• How galaxies form, grow, merge, and reshape
• Why the universe looks the way it does today
Clear diagrams and simple explanations included.
? 1. The Lifecycle of a Star — The Quick Map
A star's path depends mainly on ONE number:
Its mass.
Diagram:
Code:
Mass < 8 Suns Mass > 8 Suns
-------------------- -------------------------
Protostar Protostar
↓ ↓
Main Sequence Main Sequence (very short)
↓ ↓
Red Giant Red Supergiant
↓ ↓
Planetary Nebula Supernova
↓ ↓
White Dwarf Neutron Star / Black HoleKey idea:
Bigger stars burn hotter, faster, and die violently.
? 2. How Galaxies Evolve
Galaxies grow through:
✔ Gas accretion
✔ Star formation
✔ Mergers (small & large)
✔ Supermassive black hole feedback
ASCII Diagram:
Code:
Gas Cloud → Proto-Galaxy
↓
Spiral Galaxy
↙ ↘
Minor Merger Major Merger
↓ ↓
Thick Disk Elliptical GalaxyMajor mergers destroy spirals and create giant elliptical galaxies.
? 3. Star Formation Rate Over Time
The universe had a “Golden Age” of star formation.
• Peak: 10 billion years ago
• Now: only ~5–10% of that rate
• Future: slow decline until star formation stops completely
Graph (conceptual):
Code:
Star Formation Rate
|
| peak
| /''''''\
| / \___
|____/ \____ time →? 4. Galactic Rotation & Dark Matter
Stars orbit the galactic center too fast for the visible mass alone.
This requires:
Dark matter.
Rotation curve diagram:
Code:
Velocity ↑
Observed ────────────
\
\_Visible matter only
Distance →? Summary
• Stars evolve based on mass — small stars live long, big stars die fast
• Galaxies constantly grow, merge, and reshape
• Dark matter is required to explain galaxy rotation
• The universe is slowing down in star formation but still evolving
If you want deeper sections (supernova types, galaxy clusters, mergers),
just reply and I’ll expand this into a multipart series.
Written for The Lumin Archive — Clear, accessible science for all.