Newtonian Physics


Contents:
  1. Introduction to Newtonian Physics
  2. Newton 3 Laws of Motion
  3. Mass
  4. Center of Mass
  5. Finding Center of Mass
  6. Acceleration and Force
  7. Newton's Law of Universal Gravitation
  8. Why Do We Need the Physics for Orbits?

  1. Introduction to Newtonian Physics:

    Newtonian physics was, of course, discovered by Isaac Newton (1643--1727) (see the figure below (local link / general link: newton_principia_2.html) and it continues to be regarded as a true emergent theory in the classical limit where the effects of relativistic physics (combined special relativity (1905) general relativity (1915)) and quantum mechanics become vanishingly small.

    Some Qualifications are needed:

    1. One aspect of Newtonian physics has been corrected from Newton's original version. His understanding of inertial frames has been replaced by a modern understanting based on general relativity (1915) (see Mechanics file: frame_basics.html).

    2. Newton's presentation of Newtonian physics did NOT include the concept of energy though some people in his day were vaguely thinking about it and it is implicit in Newtonian physics. The energy concept was developed extended beyond Newtonian physics in the 19th century. In this file, we largely avoid energy. Energy is explicated in IAL 5: Physics, Gravity, Orbits, Thermodynamics, Tides: Energy.

    3. The mathematical formalism of Newtonian physics used by Newton himself is excruciatingly difficult and it was obsolete almost immediately. This makes his book Principia (1687) extremely difficult for a modern person to understand even if you can read Latin. In fact, the "translation" into a mathematical formalism much closer to modern mathematical formalism was begun by Pierre Varignon (1654--1722) soon after the publicaition of the Principia (1687).


  2. Newton 3 Laws of Motion:

    Newtonian physics is primarily based on Newton's 3 laws of motion and Newton's law of universal gravitation which we discuss below in section Newton's Law of Universal Gravitation.

    There is whole lot of Newtonian physics formalism developed on the basis of the primary bases.

    Newton's 3 laws of motion are:

    1. Newton's 1st law of motion: The center of mass (CM) of a body will stay in uniform motion (i.e., unaccelerated motion) relative to all LOCAL inertial frames (see above subsection The Basics of Reference Frames Relevant to Physics, unless acted on by a NET EXTERNAL force.

      LOCAL means in the same place or nearly the same place. Context as usual determines the exact meaning. Here the meaning is "in the same place".

    2. Newton's 2nd law of motion: A net acceleration of the CM relative to all LOCAL inertial frames is caused by (and only caused by) a NET EXTERNAL force. As formula, the 2nd law is

        (vec F_net_ext) = m(vec a_CM)
       
        or 
      
        (vec a_CM) = (vec F_net_ext)/m  , 
      where "vec" means vector (a quantity with a magnitude and a direction), vec F_net_ext is a NET EXTERNAL a href="http://en.wikipedia.org/wiki/Force">force, vec a_CM is CM acceleration, and m is mass (i.e., the body's resistance to acceleration).

      The Newton's 2nd law of motion is often just referred to as F=ma.

    3. Newton's 3rd law of motion: For every force, there is an equal and opposite force. This pair of forces do NOT have to be on the same body. Counterfactually if they did, NO body CM would ever accelerate at all.

      In fact, the internal forces on a body do cancel out pairwise and this is why they do NOT affect the motion of the CM though they certainly affect the motion of the body parts.

    Newtonian physics is strongly believed to hold (exactly) asymptotically in the classical limit and to be an emergent theory from TOE-Plus.

    Note that Newton's 3 laws of motion are referenced to inertial frames. It is just part of their statements just as we gave them above. However, inertial frames are often omitted in initial presentations of the Newton's 3 laws of motion to students. They should NOT be omitted.

    Now most of everyday life and most astro-bodies from interstellar medium (ISM) to large-scale structure of the universe are close enough to the classical limit that they obey Newtonian physics to a high accuracy/precision.

    More general theories can be applied when Newtonian physics fails: e.g., for atoms and molecules, black holes, and the observable universe.

    We give explication of the some of the keywords of Newtonian physics in subsections below: mass, center of mass (CM), acceleration, force, etc.

  3. Mass:

    Formally mass is just defined as the resistance of a body to acceleration relative to an inertial frame and the body's gravitational "charge" (i.e., the strength parameter of its gravitational effects). That the two aspects of mass are the same is just a coincidence in Newtonian physics, but general relativity shows that is a fundmental fact.

    Now in the classical limit, the mass of a body equals the sum of the rest mass of baryonic matter particles (i.e., protons, neutrons, and electrons) that make it up. Because of this statement, mass is often defined as the quantity of matter as a shorthand.

    Note the rest mass is the mass-energy of existence for massive particles (i.e., those particles with rest mass).

    Note also that by the dictate of quantum mechanics, subatomic particles and unperturbed atoms and molecules of a given type are absolutely identical---they have NO freedom to be different. So each such particle of a given type has exactly the same rest mass.

    Note also again, there are massless particles: the photon being the best known. But actually, massless particles have mass since they have energy as implied by mass-energy equivalence E=mc2. They do NOT have rest mass since they do NOT exist at rest in inertial frames. Relative to any inertial frames, they always move at the vacuum light speed c = 2.99792458*10**8 m/s (exact by definition) ≅ 3*10**8 m/s = 3*10**5 km/s ≅ 1 ft/ns in vacuum and more slowly in a media-dependent way in media.

  4. Center of Mass:

    What the heck is center of mass and why do we need it?

    Short answer: To clear the bar (see the figure below (local link / general link: center_of_mass_fosbury_flop.html).


    Somewhat longer answer: a
    center of mass is the mass-weighted average position of a body and we need it since Newton's 2nd law of motion (AKA F=ma) controls the motion of the center of mass of a body via the NET EXTERNAL force on the body.

    What about the parts of a body?

    The parts of the body are their own bodies with their own centers of mass and their own NET EXTERNAL forces which include those forces due to other parts of the whole body.

    In the astrophysical realm, there is hierarchy of systems of astro-bodies. Each systems has its own centers of mass which moves under the net EXTERNAL of a larger system of astro-bodies. A system can be analyzed in a celestial frame which name can be used as a synonym for the system itself. Top of the hierarchy are comoving frames. For further explication on the hierarchy, celestial frames, and comoving frames, see file: Mechanics file: frame_hierarchy_astro.html.

  5. Finding Center of Mass:

    Don't panic, we'll NEVER calculate a center of mass---we just need to understand the concept center of mass and learn how to find it without calculating it in some simple cases.

    Since a center of mass is a mass-weighted average position, for bodies of sufficiently high symmetry, centers of mass must be at the obvious centers of symmetry.

    There is NO place else centers of mass could be given that they are mass-weighted average positions.

    So one can find the centers of mass by inspection in the figure below (local link / general link: center_of_mass_2d.html).


    What if a
    center of mass CANNOT be found by inspection.

    Something which everyone knows (even if they don't know they know it) is to balance body, the center of mass must be above the balance point. A balance is, of course, an unstable equilibrium.

    A stable equilibrium is when a body is hanging and at rest. The center of mass must be below the hanging point. Remember bodies always hang the same way from a given hanging point.

    We will NOT prove the above statements.

    However, there is a simple empirical method for finding the center of mass for rigid objects. The method is illustrated in the figure below (local link / general link: center_of_mass_hanging.html).


    The
    center of mass can be located deceptively as shown in the figure below (local link / general link: center_of_mass_balancing_bird.html).


    Of course, you can calculate the
    center of mass. How this is done in general is illustrated in the figure below (local link / general link: center_of_mass_illustrated.html).


  6. Acceleration and Force:

    To further explicate Newtonian physics we need to define what we mean by acceleration and force.

    An acceleration of a body is a change in speed AND/OR a change in direction relative to an inertial frame caused by a net force acting on the body.

    These two kinds of change included in the definition of acceleration are illustrated in the two figures just below (local link / general link: gravity_acceleration_little_g.html; local link / general link: newton_2nd_law.html).



    Now as to
    force:

    1. An ORDINARY force or force without qualification is a physical relationship between bodies or between a body and force field (e.g., the gravitational field and electromagnetic field) that can an acceleration of a body relative to an inertial frame.

      By physical relationship, one means that the force depends on the nature of the bodies and the states of the bodies.

      A force can depend on mass (gravity), electric charge (the electromagnetic force), relative position (gravity, the electromagnetic force), velocity (the magnetic force), and other things.

    2. An inertial force is a relationship between a body and convert-to inertial frame. But in that convert-to inertial frame, it acts just like an ordinary force. In fact, in general relativity, inertial forces and gravity are regarded as fundamentally the same thing.

    If you know the forces acting on a body from known force laws, then physical law will predict the acceleration relative to the inertial frame you are using. The physical law in the classical limit is Newton's 2nd law of motion (AKA F=ma).

    If you are NOT in the classical limit, you have to use relativistic mechanics and/or quantum mechanics.





  7. Newton's Law of Universal Gravitation:

    Newton's law of universal gravitation for 2 point masses:

             G * M_1 * M_2
      F =   ---------------   ,
                 r**2 
    where F is size of the pulling gravitational force each point mass exerts on the other, gravitational constant G=6.67430(15)*10**(-11) (MKS units), (M_1 * M_2) is the product of the point mass masses, and r is their separation.

    Explication:

    1. If you have finite bodies,, then the gravitational force between them can be found by summing the gravitational force between all their infinitesimal bits (i.e., their point masses parts). Because this can be done, the gravitiational law is a universal law: it applies to all bodies.

    2. If 2 bodies are spherically symmetric (and they are NOT overlapping), the gravitiational law applies directly to them with r being their center-to-center separation. This result was proven by Isaac Newton (1643--1727) himself and was a vital ingredient in understanding systems made of (nearly) spherically symmetric astro-bodies: e.g., the Solar System.

    3. The gravitational force is actually weak in a sense. The whole Earth pulls on you (you being effectively a point mass), but you can still stand up with just your INTERNAL body pressure force.

    4. The gravitational force between 2 human scale bodies is NOT noticeable. This is why students in a classroom do NOT clump together in one big clump.

      However, the gravitational force between kilogram masses can be measured in high sensitivity experiments.

    5. But despite being weak, the gravitational force is a key ingredient in determining astrophysical structures. It CANNOT canceled since there is only one "gravitational charge" which is mass and likes attract. This is unlike the Coulomb's law force (AKA electric force), where unlikes attract and cancel mostly overall at the macroscopic scale since the amount of positive charge and negative charge in the observable universe is seemingly exactly equal. At the microscopic scale, quantum mechanics forbids exact cancellation.

    6. How are astrophysical structures determined? The short answers:

      1. Compact astro-bodies (above the scale of small asteroids) are determined by a combination of self-gravity and the pressure force. These astro-bodies are, e.g., large asteroids, large moons, planets, stars, white dwarfs, and neutron stars. Black holes require general relativity as do neutron stars to a degree. Astro-bodies of the scale of small asteroids or smaller also have rigid-body forces (i.e., chemical bonds) determining their structure.

      2. Systems of astro-bodies like planet-moon systems, planetary systems, star clusters, galaxies, galaxy clusters, galaxy superclusters, the large-scale structure of the universe and the observable universe, as whole are determined by gravity and kinetic energy. At the scale of the large-scale structure, and the observable universe the cosmological constant force (or its dark energy equivalent) are also important.

    7. To explicated the dependencies of the gravitiational law, note that the gravitational force of attraction is proportional to the product of the masses of the bodies:

        M_1 * M_2 .

      It is also inversely proportional to the square of the distance between the bodies:

        1/r**2

        and so is grows small as r increases.

        The 1/r**2 behavior is an inverse-square law.

      The fall-off of the gravitational attraction with distance---the inverse-square law behavior---in one sense is rapid.

      Double the distance and the force decreases by a factor of 4; triple the distance and the force decreases by a factor of 9; etc.

      But formally the gravitational force does NOT go to zero until r → ∞. So, in fact, gravity is a long-range force.

      The inverse-square law behavior is illustrated in the figure below (local link / general link: function_behaviors_plot.html).


  8. Why Do We Need the Physics for Orbits?

    The short answer is to understand all the astrophysical structures, in particular gravitationally bound systems which are full of gravitationally bound orbits: i.e., more or less revolving motions relative to the center of mass of center-of-mass inertial frames constituted by the gravitationally bound systems.

    For a sufficiently isolated gravitationally-bound system, all the astro-bodies orbit gravitationally-bound system center of mass unaffected by the rest of observable universe to high accuracy/precision, except that the center of mass is in free-fall in the EXTERNAL gravitational field due to the rest of observable universe. For a NOT sufficiently isolated gravitationally-bound system, the EXTERNAL gravitational field will exert a tidal force on a gravitationally-bound system that will effect the INTERNAL motions (i.e., motions relative to the center of mass).

    There is a whole hierarchy of such isolated gravitationally-bound systems. To give an example of gravitationally-bound systems in the hierarchy consider the following cases:
    1. Low-Earth-orbit artificial satellites orbit the Earth's center of mass.
    2. The Earth's center of mass orbits the Earth-Moon system center of mass.
    3. The Earth-Moon system center of mass orbits the Solar System center of mass.
    4. The Solar System center of mass orbits the Milky Way center of mass.
    5. The Milky Way center of mass orbits the Local Group of Galaxies center of mass.

    A fairly general explication of orbits is given in the figure below (local link / general link: orbit_defined.html).

Local file: local link: frame_basics.html.
File:
Mechanics file: newtonian_physics.html.