Physics · Gravitation and the universe · Grade 9
Scales of the universe
From quarks to the Universe: which laws of physics rule at each scale?
The situation
Imagine a person standing near the Tashkent TV Tower. If the camera moves away 10 times farther with each step, after 7 steps the whole Earth is visible, and after 21 steps the Milky Way galaxy. If the camera goes inwards, we see a cell, DNA, an atom, a nucleus and the quarks inside a proton. Over the whole journey the scale changes by about 10⁴² times. Are the laws of physics the same at every scale, or does each scale have its own “ruling” law?
Topic
Physical picture of the universe: scales. From a quark to a galaxy: a journey through the powers of ten
Key ideas
- Powers of ten
- Fundamental constants
- Branches of physics
Formulas
The Planck length and time — a scale built from three fundamental constants.
Two limits: if a body is smaller than , it is a black hole; at scales smaller than , quantum effects dominate.
Dimensionless numbers: if they are smaller than the required accuracy, classical (Newtonian) physics is enough.
Reference frame: the position vector, its derivative is the velocity, and the integral of the velocity is the distance travelled.
The speed of light is finite: when we look far away, we see the past.
Theory
Powers of ten: space and time
The diameter of a proton is ≈ 1.7·10⁻¹⁵ m, and the diameter of the observable Universe is ≈ 8.8·10²⁶ m. Such numbers are convenient to write with powers of ten: each step is a factor of 10. Time is the same: light crosses a proton in ≈ 6·10⁻²⁴ s, while the age of the Universe is ≈ 4.4·10¹⁷ s (13.8 billion years). Units of length are chosen according to the scale: fm (nuclei), nm (molecules), m, km, AU (Earth–Sun), the light-year and the parsec (stars), Mpc (galaxies). Space and time are the stage of all phenomena; special relativity unites them into a single space-time.
Reference frame and position vector
To say where a body is, you need a reference frame: a reference body, coordinate axes and a clock. In the “Powers of ten” scene, at the scale of 10² m, the origin is at the foot of the TV tower: points east, up, south. The person's position is the position vector m. The derivative of the position vector with respect to time is the velocity, and the integral of the velocity is the distance travelled. Velocity depends on the reference frame: a “stationary” person in Tashkent moves at ≈ 350 m/s with the Earth's rotation, at ≈ 30 km/s with the Earth around the Sun, and at ≈ 230 km/s with the Sun around the centre of the Galaxy.
The four interactions: a single picture of the world
All phenomena are explained by four interactions. The strong one holds quarks in protons and neutrons and nucleons in the nucleus; its range is ≈ 10⁻¹⁵ m. The weak one governs β-decay and the first stage of fusion in the Sun; ≈ 10⁻¹⁸ m. The electromagnetic one gives atoms, molecules, chemistry, biology, friction and elasticity; its range is infinite. Gravity is the weakest (≈ 10³⁶ times weaker than the electric repulsion between two protons), but because matter is usually electrically neutral, it dominates at large scales — planets, stars, galaxies. The history of physics is a history of unification: electricity and magnetism (Maxwell), electromagnetic and weak interactions (electroweak theory), the Standard Model; uniting gravity with quantum physics is still unsolved.
The cube of theories: the limits of classical physics
Each theory can be marked by three constants. In the limit , , — Newtonian mechanics. When approaches the speed of light — special relativity; when the action () is close to — quantum mechanics; both together — quantum field theory; strong gravity and — general relativity. Which theory is needed also depends on the accuracy: for GPS clocks even corrections of matter, while for a football 1 % accuracy is enough. The old theory remains the limiting case of the new one — this is the correspondence principle.
The microworld: milestones of atomism and particle physics
The size of an atom is ≈ 10⁻¹⁰ m (the Bohr radius is 5.29·10⁻¹¹ m), while the nucleus is ≈ 10⁻¹⁵ m — about 100 000 times smaller than the atom, yet it holds more than 99.9 % of the mass. The microworld is governed by fundamental constants: the elementary charge , the electron mass , Planck's constant , and the speed of light . The quantum (wave nature, spin, energy levels) and relativistic (antiparticles, ) properties of particles appear together at this scale. Milestones: the electron (1897, J. J. Thomson), the nucleus (1911, E. Rutherford), the neutron and positron (1932), the quark model (1964), quarks “seen” in experiment (1968–1969, SLAC), W and Z bosons (1983, CERN), the top quark (1995), the Higgs boson (2012, LHC).
Physics, other sciences and society; the model
Physics studies the most general laws of nature through observation, experiment, models and theory; its language is mathematics. It is the foundation of chemistry (the structure of atoms and molecules), biology and medicine (biophysics, X-rays, MRI, PET), geology, astronomy and engineering. Electricity grids, the transistor and computers, lasers, GPS, nuclear power stations and solar panels are products of discoveries in physics; they have transformed society's productive forces. Model: sizes are approximate; the Moon and planets are enlarged to be visible; galaxies and the cosmic web are schematic; the positions of the TV tower and the person are arbitrary.
Did you know?
- The Tashkent TV Tower is 375 m tall. It was put into operation on 15 January 1985 and from 1985 to 1991 was the fourth tallest tower in the world.
- A “stationary” person beside the TV tower moves with the Earth's rotation at about 350 m/s — faster than the speed of sound.
Inside the experiment
The experiment starts from a real-life situation: you predict the result, change the controls, run the experiment and draw a conclusion. Inside are missions, theory, a quiz and a guided tour in which the camera moves and explains the key points.
More experiments in this section
- The Solar System — Grade 7
- Newton's cannon: an artificial satellite — Grade 10
- Special relativity — Grade 10
- Law of universal gravitation — Grade 10
- Relativistic dynamics — Grade 10
- Kepler's laws — Grade 10
- Physics of stars — Year 1
- The expanding universe — Year 1
- Black holes — Year 4