Kepler's laws of planetary motion 2026-10-13
Kepler's laws describe three connected features of an elliptic orbit: its shape, how fast it is traversed, and how its size determines its orbital period. Kepler's first law gives an ellipse with the attracting centre at one focus of a conic; Kepler's second law gives equal swept areas in equal times; Kepler's third law relates the squared orbital period to the cubed semi-major axis. Together they turn a drawing of a Kepler orbit into a prediction of where the bodies will be and when they will return. [ref]
Here the mathematical model is an isolated two-body problem in Newtonian gravity, with point masses and a bound, noncolliding elliptic orbit. Let be the relative displacement, the separation, and the gravitational parameter, where is the gravitational constant. Newton's law of universal gravitation then givesThe relative Kepler orbit has semi-major axis and orbital eccentricity . Both bodies move around their shared astronomical barycenter, the system's centre of mass. In its rest frame their displacements are and . Their individual semi-major axes therefore add to ; the relative ellipse's attracting focus of a conic represents zero separation, rather than a body fixed in space.
One example will connect all three laws. After nondimensionalization, choose , and . The semi-minor axis is , while the periapsis distance and apoapsis distance areThus measures the ellipse's size even though the separation changes fourfold. The specific angular momentum will be , the two endpoint speeds and , and the orbital period . These are values in the chosen scaled units, not measurements of a particular planet.
Johannes Kepler published Kepler's first law and Kepler's second law in Astronomia Nova in 1609 and Kepler's third law in Harmonices Mundi in 1619. These publication dates are documented by [ref]. Their appeal is that three short statements organize both geometry and timing; Newtonian gravity supplies a common dynamical explanation.
Lorentz force Created 2026-09-24 Updated 2026-10-14
The Lorentz force is the force exerted by an electric field and a magnetic field on a body with electric charge and velocity . In SI units its form in nonrelativistic classical mechanics, using mass and Newton's second law, isBoth fields are evaluated at the body's position at the current time. The electric field contributes even at rest, whereas the magnetic force depends on velocity through a cross product. [ref]
https://openstax.org/books/university-physics-volume-2/pages/5-4-electric-field. OpenStax, electric force and field
; [ref]https://openstax.org/books/university-physics-volume-2/pages/11-2-magnetic-fields-and-lines. OpenStax, magnetic force on moving charge
.For a concrete charged particle in a uniform magnetic field, use nondimensionalization to stipulate , magnetic field , zero electric field, initial position , and initial velocity . These are rescaled quantities, not an assertion that the mass, electric charge, and magnetic field have the same physical units. At the start, , so the magnetic acceleration points toward . The resulting circular motion isAt the position is and the velocity is ; at the position is and the velocity is . Thus the circle has center and radius one. Viewed from toward the plane, the motion is clockwise. Changing only the electric charge to gives position and reverses the bending to counterclockwise.
Adding initial velocity leaves the transverse circular motion unchanged and givesThis is a helix of transverse radius one, cyclotron frequency , and transverse period ; the advance along in one turn is . The parallel component of velocity stays constant because the magnetic force has no parallel component: there is no magnetic acceleration along the magnetic field. If the initial velocity were entirely parallel to the magnetic field, the magnetic force would vanish and the path would be straight. [ref].
More generally, with zero electric field, no other forces, and a uniform constant magnetic field of magnitude , decompose velocity into perpendicular and parallel components. For nonzero electric charge , the perpendicular speed determines the gyroradius, while the cyclotron frequency is an angular frequency:These are nonrelativistic formulas; see the relativistic cyclotron orbit for the correction. The beauty is that increasing perpendicular speed increases the radius in exactly the proportion needed to leave the period unchanged. Conversely, known magnetic field, perpendicular speed, and measured radius determine the magnitude of the electric charge divided by mass. This makes the same geometry useful for comparing bodies with different electric charge and mass.
Two short checks explain the result. First, the cross product gives for both stipulated positive-electric charge paths, exactly their acceleration. Second, the transverse magnetic force supplies the centripetal acceleration, so ; for this gives the gyroradius, and gives the cyclotron frequency.
Magnetic forces do no work: the instantaneous power of the magnetic part of the Lorentz force vanishes because a cross product is perpendicular to its first argument. The work-energy theorem therefore givesThe dot product is zero at every instant, rather than only after a full turn. With zero electric field and no other forces, the kinetic energy and speed remain constant; the electric field can increase or decrease kinetic energy according to the sign of . In the two stipulated examples the constant kinetic energy is respectively and in rescaled units. The extra parallel velocity raises kinetic energy without changing the gyroradius or the cyclotron frequency.
For an electric example in rescaled units, stipulate , zero magnetic field, constant electric field , no other forces, and rest at . The Lorentz force gives acceleration and velocity , hence kinetic energy and power . At , the kinetic energy has risen from zero to two: the electric field has done positive work.
The existing electromagnetic field tensor formulation expresses the same interaction covariantly. For four-momentum and four-velocity , using proper time , the Lorentz force law isIts spatial and temporal components are
Newtonian gravitational field Created 2026-09-24 Updated 2026-10-14
The Newtonian gravitational field is the gravitational force per unit mass of a test particle. For a point mass at the origin,The test particle's mass cancels: different small masses have the same gravitational acceleration at the same position. In SI, the Newtonian gravitational field has units . The same exterior expression holds for a spherically symmetric source, by the spherical shell theorem.
Choose a reference radius , set , and use nondimensionalization with . Then : at , the magnitudes are . This makes the spatial variation visible without specifying a planet. [ref]
https://openstax.org/books/university-physics-volume-1/pages/13-1-newtons-law-of-universal-gravitation. OpenStax: inverse-square attraction and spherical sources
Normalized Newtonian gravitational field and point-mass potential
. Doubling the radius quarters the magnitude of the Newtonian gravitational field, but halves the magnitude of the negative Newtonian gravitational potential. Both curves approach zero as radius increases; the inward gravitational acceleration is minus the gradient of the Newtonian gravitational potential. Details. Past exam of the mathematics course of the University of Cambridge 2005 ii Paper 2 13E a Solution Created 2026-09-24 Updated 2026-09-24
Past exam of the mathematics course of the University of Cambridge 2008 ii Paper 3 6B Solution Created 2026-09-24 Updated 2026-09-24
Physics Created 2026-09-24 Updated 2026-10-13
Physics investigates matter, motion, and interactions by building mathematical models and testing their consequences against observations. A physical law supplies a relation; a model specifies the objects, conditions, and approximations used to apply it. Classical mechanics, electromagnetism, thermodynamics, and quantum mechanics organize different aspects of these investigations. Their usefulness comes from turning measurements into predictions that can be checked and refined.
Consider a simple pendulum: how does its oscillation period change when its length changes? For small amplitude, the ideal model gives , where is gravitational acceleration. Taking as the model parameter, a one-metre pendulum has predicted period . Increasing its length to four metres gives : quadrupling the length doubles the period. The point mass cancels from the equation, so changing it alone does not change this model's answer.
The prediction identifies a mechanism and a way to challenge it. The small-angle approximation replaces by ; the full ideal equation predicts a longer period at large amplitude. At , its period is about , already a change. Measurements at such amplitudes can reveal the limit of the approximation, while appreciable drag requires a damped pendulum. These distinctions are developed in simple pendulum and dimensional analysis. The small-amplitude model is also derived in Ling, Sanny and Moebs, University Physics, pendulums.
Several different experiments can become one calculation. Nondimensionalization rewrites the pendulum equation using , leaving . All lengths share that dimensionless equation; the amplitude remains a parameter. Similarly, conservation laws and symmetry reveal features that many models share. This is one source of the subject's beauty: a compact relation can organize a large range of phenomena.
The connection to evidence remains essential when a model is elegant. In his introductory lectures, Richard Feynman emphasizes testing proposed relations by experiment and using idealizations whose accuracy depends on the conditions. [ref]
https://www.feynmanlectures.caltech.edu/I_01.html. Feynman, Leighton and Sands, Atoms in motion, section 1–1
A discrepancy can motivate a better measurement, a better approximation, or a different physical model; the mathematical calculation and the empirical assessment are both part of the explanation. Radial free fall from rest 2026-10-14
Let a test particle start at rest at radius outside a fixed spherically symmetric source. The spherical shell theorem gives the exterior Newtonian gravitational potential , where is the source's standard gravitational parameter. Zero initial transverse velocity makes the motion radial. Conservation of mechanical energy per unit mass givesThe minus sign selects inward motion; the positive square root is its speed. For a fall from to the surface , that speed is . In the limit of release from rest infinitely far away, the familiar free-fall speed is , equal in magnitude to the local escape velocity. A finite starting radius gives a smaller speed.
The arrival time follows from the same first integral. Set . ThenFor arrival at this is finite, and the field formula is used only outside the source. For , givesKeeping the smaller initial gravitational magnitude constant would predict , about longer. The actual acceleration increases during the fall.
The curves compare a shallow fall, , with a fall from , so . Each comparison holds the release height and initial gravitational magnitude fixed. The constant-gravity model is close for the shallow fall and increasingly inaccurate for the larger one. This is also a practical use of nondimensionalization: the normalized trajectories depend on , while supplies the dimensional time scale.



