What is Dark Matter?
Welcome! I am glad you are curious about dark matter. Before we dive into what it is and how we know it is there, I would love to learn a bit more about your background.
What brings you to study dark matter today, and how comfortable are you with physics or astrophysics concepts?
I have a solid science background, looking for a deep dive.
Awesome! Having a strong background in science means we can really get under the hood of astrophysics and particle physics.
Continue to galaxy rotation curves and Vera Rubin's work
Let's dive straight into the crucial observational evidence that convinced the astronomy community dark matter had to exist: galaxy rotation curves.
Based on classical Newtonian mechanics, orbital speed at distance from a centralized mass follows a simple gravitational balance:
Beyond the visible edge of a galaxy where almost all luminous matter is concentrated, stops growing and becomes roughly constant. Consequently, speed should follow a Keplerian decline where .
Instead, Rubin found that orbital velocities remain almost completely flat even far out into the sparse fringes of galaxies.
Comparison of expected Keplerian galaxy rotation velocity versus observed flat rotation velocity across galactic radius.
I've kicked off a diagram showing the exact discrepancy Vera Rubin uncovered between theoretical expectations and observational data.
For to stay constant at large radii, the mass contained within radius must scale linearly with distance (). This implies galaxies live inside massive, extended dark matter halos that reach far beyond their visible stars.
Continue to galaxy clusters and Fritz Zwicky's work
xcpybr
| Component | Percentage | Description |
|---|---|---|
| Dark Energy | ~68% | Repulsive force driving cosmic acceleration |
| Dark Matter | ~27% | Non-baryonic, non-luminous matter holding structures together |
| Baryonic Matter | ~5% | Normal matter (stars, planets, gas, and us) |