Astronomy
Galaxies and Hubble
Galaxy shapes, rotation curves, the Hubble–Lemaître law, and a standard-candle sketch.
Basics
Shapes
Hubble’s tuning-fork sketch splits ellipticals, spirals (barred or not), and irregulars. Ellipticals are gas-poor with older stars; spirals form stars in arms. The Milky Way is a barred spiral. Shape is a snapshot, not a path from elliptical into spiral. Mergers can make ellipticals and irregulars.
Rotation curves
In spirals, orbital speed in the disk often stays flat far out instead of falling. Stars and gas we see do not supply enough gravity, so a dark-matter halo is added. Modified gravity is studied too; the standard sketch is a halo. The Milky Way shows the same pattern. Do not count mass by light alone.
Hubble–Lemaître
Nearer galaxies show smaller redshifts. v ≈ H₀ d is the linear sketch. Photometric ladders and the CMB give slightly different H₀ — the “Hubble tension”. In the far universe one reads a changing scale factor, not a simple speed. Recession is expanding space, not galaxies tunnelling through the void.
The distance ladder
Parallax (Gaia) measures nearby stars; Cepheid period–luminosity and the near-standard peak of Type Ia supernovae extend the ruler. Each rung passes calibration error to the next. Gravitational-wave “standard sirens” test another path. Numbers are revised; in class, keep the backbone of the methods.
Formulas
Hubble–Lemaître (nearby)
Low speed and redshift. H₀ in km s⁻¹ Mpc⁻¹.
Symbols
-
vrecession-speed sketch -
H₀Hubble constant (today) -
ddistance (near proper distance)
Redshift
In cosmology, 1+z = 1/a at emission.
Symbols
-
λ_obsobserved wavelength -
λ_ememitted wavelength
Circular speed
A flat curve suggests M(<r) grows with r.
Symbols
-
M(<r)mass interior to r
Key table
| H₀ ballpark | around 70 km s⁻¹ Mpc⁻¹; methods differ by a few km |
|---|---|
| Local Group | Milky Way, Andromeda (M31), Triangulum (M33), … |
| Dark matter | almost no light, gravity only; the particle is still unconfirmed in the lab |
In this field
Solar system
Planets, Kepler, gravity, escape speed.
Stars
HR diagram, fusion, lifetimes, magnitude.
Galaxies and cosmology
Galaxies, Hubble, redshift, black holes.
Observing basics
Celestial sphere, coordinates, telescopes, spectra.
Exoplanets and life
Detection, habitable zone, a SETI sketch.
The Sun and space weather
Solar structure, spots, flares and CMEs.
Moon, tides, and eclipses
Lunar phases, tides, and solar and lunar eclipses.
Magnitudes and spectra
Apparent and absolute magnitude, distance modulus, colour and spectral type, Wien’s law.
Telescopes and light
Aperture, diffraction limit, collecting area, seeing versus space telescopes.
Stellar death
Red giants, supernovae, and sketches of white dwarfs, neutron stars, and black holes.