πŸ“‘ Astronomy · Cosmology

Astronomy tricks that make the cosmos click

Big Bang, expansion, dark energy, and the CMB β€” mastered.

🌌 Cosmology

Memory tricks

Proven mnemonics — fast to learn, hard to forget.

Hubble's Law
Hubble's Law: v = Hβ‚€ Γ— d β€” farther galaxies recede faster. Hβ‚€ β‰ˆ 70 km/s/Mpc.
Hubble's Law
The expanding universe β€” recession velocity proportional to distance
Hubble (1929): distant galaxies show redshift proportional to distance. v = Hβ‚€ Γ— d. Key insight: galaxies aren't moving through space β€” space itself is expanding. No center of expansion (raisins in rising bread). Hβ‚€ β‰ˆ 70 km/s/Mpc β€” the 'Hubble tension': CMB measurement vs distance ladder give slightly different values. An unresolved discrepancy that may point to new physics.
Cosmic Microwave Background
CMB: 2.7K afterglow of the Big Bang at 380,000 years old. Tiny fluctuations are seeds of all galaxies.
Cosmic Microwave Background
The oldest light in the universe β€” a snapshot of the infant cosmos
At 380,000 years: universe cooled enough for electrons + protons β†’ hydrogen (recombination). Photons decoupled β†’ CMB. Discovered by Penzias and Wilson (1965, Nobel 1978). Temperature 2.725K. COBE, WMAP, Planck mapped tiny anisotropies (1 part in 100,000) β€” quantum fluctuations stretched by inflation β†’ became large-scale structure. CMB is the most direct evidence for the Big Bang.
Cosmic Inflation
Inflation: exponential expansion at 10⁻³⁢ to 10⁻³² seconds β€” solves horizon, flatness, and monopole problems.
Cosmic Inflation
Why the universe looks the same in all directions β€” and why it's so geometrically flat
Alan Guth (1980). Horizon problem: distant regions of CMB were never in causal contact β€” inflation stretched one connected patch to cosmic scales. Flatness problem: inflation drove curvature toward zero. Monopole problem: inflation diluted exotic particles. Quantum fluctuations during inflation β†’ CMB anisotropies β†’ galaxy seeds. Evidence: primordial gravitational waves in CMB B-modes (not yet confirmed). Inflation is the leading explanation but not yet proven.
Dark Energy
Dark energy: ~68% of universe β€” causes accelerating expansion. Nature unknown. Discovered 1998.
Dark Energy
The mysterious energy causing the universe to expand faster and faster
Perlmutter, Schmidt, Riess (1998, Nobel 2011): Type Ia supernovae (standard candles) showed universe expanding faster than expected β€” acceleration. Dark energy: 68% of total energy content. Simplest model: cosmological constant Ξ› (energy of empty space), w = βˆ’1. Alternatives: quintessence (evolving field). Ultimate fate depends on nature: Big Freeze (likely), Big Rip (if w < βˆ’1). Biggest mystery in modern cosmology.
Dark Matter
Dark matter: ~27% of universe β€” detected only by gravity. Never directly seen. Not ordinary matter.
Dark Matter
The invisible mass holding galaxies and galaxy clusters together
Zwicky (1933): Coma cluster too fast β€” missing mass. Vera Rubin (1970s): galaxy rotation curves flat at edges β†’ dark matter halo. Evidence: gravitational lensing (Bullet Cluster), CMB, large-scale structure. Not: ordinary matter, black holes, neutrinos. Candidates: WIMPs, axions, sterile neutrinos. Direct detection experiments (XENON, LUX): no confirmed detection. Constitutes 27% of universe. Modified gravity (MOND) proposed as alternative β€” disfavored by Bullet Cluster.
Olbers' Paradox
Olbers' paradox: infinite eternal universe β†’ bright night sky. Sky is dark because universe is finite in age.
Olbers' Paradox
A simple observation about the night sky that reveals profound cosmological truth
In an infinite, eternal, static universe: every line of sight eventually hits a star β†’ sky uniformly bright as solar surface. Resolution: (1) universe has finite age β€” light from distant stars hasn't arrived yet. (2) Expansion redshifts distant starlight out of visible range. Named after Olbers (1823) but raised by Kepler and Halley. The dark night sky is direct evidence the universe is not infinitely old. Profound cosmological conclusion from everyday observation.
Gravitational Waves
Gravitational waves: ripples in spacetime from accelerating masses. LIGO detected first in 2015 (Nobel 2017).
Gravitational Waves
Einstein's 1916 prediction β€” finally confirmed 100 years later
Einstein (1916): accelerating masses create ripples in spacetime traveling at speed of light. LIGO: arms 4 km long β€” detects length changes of 10⁻¹⁸ m (1/10,000 proton diameter). First detection (Sept 14, 2015): two merging black holes, 1.3 billion light-years. Nobel 2017. GW170817: neutron star merger detected in GW + gamma rays + optical β†’ multi-messenger astronomy. LISA (space-based): will detect supermassive black hole mergers. New window on the universe.
Cosmic Distance Ladder
Distance ladder: parallax β†’ Cepheid variables β†’ Type Ia supernovae. Each rung extends range further.
Cosmic Distance Ladder
How astronomers measure distances across billions of light-years β€” step by step
Parallax: trigonometric, <10,000 ly, Gaia measured 1 billion stars. Cepheid variables: period-luminosity relation (Leavitt) β†’ up to ~100 Mpc. RR Lyrae: similar, older stellar populations. Type Ia supernovae: standard candles (same peak luminosity) β†’ up to 1000+ Mpc. Tully-Fisher (spirals) and Fundamental Plane (ellipticals). Hubble tension: distance ladder gives Hβ‚€ β‰ˆ 73 vs CMB gives Hβ‚€ β‰ˆ 67 β€” unexplained discrepancy.
Parallax
< 10,000 ly β€” direct geometry, Gaia
Cepheids
Up to ~100 Mpc β€” pulsation period
Type Ia SN
Up to ~1000 Mpc β€” standard candle
Hubble tension
CMB vs ladder Hβ‚€ values disagree
Fate of the Universe
Universe fates: Big Freeze (most likely), Big Crunch, Big Rip. Depends on dark energy equation of state w.
Fate of the Universe
Three possible endings for the cosmos β€” all incomprehensibly far in the future
Big Freeze (Heat Death): expansion continues, all stars die (~10¹⁴ yr), black holes evaporate via Hawking radiation (~10¹⁰⁰ yr), maximum entropy β†’ no usable energy. Big Crunch: if dark energy weakens, gravity eventually reverses expansion. Big Rip: if dark energy strengthens (w < βˆ’1), expansion tears apart galaxies, stars, then atoms. Current data (w β‰ˆ βˆ’1) favors Big Freeze. PoincarΓ© recurrence: infinite time β†’ any configuration repeatable β€” but timescale ~10^(10^120) years.
Early Universe Timeline
Planck epoch β†’ inflation β†’ quarks β†’ nucleosynthesis β†’ CMB β†’ first stars. First 380,000 years mapped.
Early Universe Timeline
The first moments of the universe β€” from incomprehensible energy to hydrogen and helium
< 10⁻⁴³ s: Planck epoch β€” quantum gravity unknown. 10⁻³⁢ s: inflation. 10⁻¹² s: electroweak phase transition. 10⁻⁢ s: quarks β†’ protons/neutrons. 1 s: neutrinos decouple, antimatter annihilated (slight matter excess). 3 min: Big Bang nucleosynthesis β€” 75% H, 25% He-4, trace D, He-3, Li. 380,000 yr: recombination, CMB released. ~200 million yr: Population III stars ignite β€” first light after the cosmic Dark Ages.
10⁻⁴³ s
Planck epoch
10⁻³⁢ s
Inflation begins
10⁻⁢ s
Quarks form protons/neutrons
3 min
H and He nucleosynthesis
380k yr
CMB released, universe transparent
Multiverse
Multiverse types: eternal inflation (bubble universes), string landscape (~10⁡⁰⁰ vacua), many-worlds quantum.
Multiverse Hypotheses
Three independent theoretical reasons why our universe may not be unique
Eternal inflation: inflation continues forever in most regions β€” bubble universes nucleate with different physical constants. String landscape: ~10⁡⁰⁰ vacuum states β†’ anthropic principle explains fine-tuning. Many-worlds interpretation: every quantum measurement spawns parallel branches. Common thread: constants in our universe are compatible with life β€” perhaps anthropically selected from vast ensemble. Criticism: untestable by current means. CMB bubble-collision signatures searched β€” not found. Fascinating but controversial.