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Physics and Inertial Frames (Mostly Only Reading)


In order to understand orbits, we need to understand a little physics including the part about inertial frames.

It all gets a bit hairy, but we'll do best to make sense of it.

We'll look at motion and orbits again when we do a further discussion of Newtonian physics and gravity in IAL 5: Newtonian Physics, Gravity, Orbits, Energy, Tides.

  1. Reference Frames:

    A reference frame is just a coordinate system (or some simpler kind of reference system if you want to think that way) that one lays on all space or some subset of all space.

    It allows you to locate objects in space and describe their motion (in physics jargon, their kinematics).

    Usually, there is a specified origin for the reference frame.

    There are infinitely many reference frames that one can use: they can have different origins, different kinds of coordinates (e.g., Cartesian coordinates, spherical coordinates), and be in any kind of motion.

    See the figure below for an example reference frame which includes a time coordinate.


    Reference frames can be just geometrical descriptions or they can be attached to some physical object, and/or have a definite physical nature which is the case for inertial frames most imporantly of all.

  2. Inertial Frames:

    The modern inertial frame is defined in general relativity discovered by Albert Einstein (1879--1955). General relativity is our best theory of gravity and the main theory ingredient of cosmology.

    To be specific, the modern inertial frame (as defined and described below) depends on the strong equivalence principle of general relativity which has been verified to a degree, but NOT as much as people would like.

    Definition: An inertial frame is reference frame defined inside a region of space with a uniform external gravitational field and that is unaccelerated with respect to the free-fall trajectory in that uniform external gravitational field.

    Some explication is needed.

    1. Inertial frames are, in fact, free-fall frames, but we don't call them that. Perhaps we should.

    2. The gravitational field is the cause of the gravitational force. It is a vector field. At every point in space it has a magnitude and a direction.

      The common symbol is "g" put in vector notation: e.g., boldface vector notation g or, as yours truly often writes it in HTML, the vector notation vec g.

      The gravitational force on a body in a small compared to variations in vec g is just m(vec g), where m is the body's mass.

    3. The uniform external gravitational field inside the inertial frame has NO effect on internal motions.

      This is because the uniform external gravitational field pulls on every bit of a system equally.

    4. Perfectly uniform gravitational fields are an idealization.

      The external gravitational field of the definition just has to be uniform enough for your purposes or the non-uniformities have to be correctable in your calculations.

      So, in fact, exact inertial frames are also idealizations, but in many cases approached to high accuracy/precision.

      Some reference frames are more inertial than others: there are varying degrees of approximation to exact inertiality.

      If a reference frame is inertial enough for your purposes, it is an inertial frame. If NOT, it's a non-inertial frame. There is NO hard line.

    5. There are often internal gravitational fields that you just treat as forces for internal motions.

    6. The natural origin for a reference inertial frame is the center of mass of the system embedded in the inertial frame.

      The center of mass is a mass-weighted average position for a system. We explicate center of mass further below in subsection Center of Mass.

      The center of mass follows the exact free fall trajectory.

      The reference frame with this origin cannot be taken to rotate with respect to the free-fall trajectory because that would be an acceleration.

      An acceleration is change in speed and/or direction.

      We explicate acceleration further below in subsection Acceleration, Force, and Inertial Frames.

      Let's call the inertial frame with the origin at the center of mass, the center-of-mass inertial frame.

    7. Any other reference frame local to the region of uniform external gravitational field that is UNACCELERATED relative to the center-of-mass inertial frame is also an inertial frame for the region.

    8. Any other reference frame local to the region of uniform external gravitational field that is ACCELERATED relative to the center-of-mass inertial frame is NOT an inertial frame for the region.

      It is an non-inertial frame for that region.

    9. Note that a rotating frame actually consists of a continuum of non-inertial frames, each of which is accelerating relative to the reference frame of the free fall trajectory which defines basic local inertial frame.

    Actually, inertial frame is NOT a good name in yours truly's opinion: it's NOT descriptive, it's hard for yours truly to pronounce, and yours truly when speaking is always confusing it with its opposite the non-inertial frame.

    One might suggest:

    1. inertial frame → physical frame since physical laws are referenced to this kind of frame, except for general relativity itself.
    2. non-inertial framegeometrical frame since physical laws are NOT referenced to this kind of reference frame but, of course, they are "physical frames" in another sense.

    But the dead hand of tradition has stuck us with inertial frames and non-inertial frames.

  3. Important Examples of Inertial Frames:

    To make concrete all that explication of inertial frames given above in subsection Inertial Frames, let's consider a few important examples of inertial frames

    1. The center-of-mass inertial frame of the Earth which is at the center of the Earth.

      The center of mass does follow a free-fall trajectory in the external gravitational field mainly due to the Sun and Moon.

      Actually, this external gravitational field is NOT perfectly uniform across the Earth.

      The variation in the external gravitational field causes a slight time-varying stretching of the Earth.

      We call the effective stretching force the tidal force which, among other things, causes the tides.

      It has vanishingly small effect on objects much smaller than the Earth like us.

    2. The ground.

      The ground is actually a rotating frame relative to the center-of-mass inertial frame of the Earth.

      However, the acceleration of the ground is only about 5/1000 at most of the acceleration due to gravity near the Earth's surface (see Wikipedia: Gravity of Earth: Latitude).

      So for most purposes, the ground is suffiicently inertial to be considered an inertial frame.

      Not all purposes. It's NOT for long-range artillery nor atmospheric circulation. Non-inertial-frame effects are important for those phenomena.

      The effects can be treated by using inertial forces which are NOT real forces, but they act like body forces pulling on every bit of an object like gravity.

      The best known inertial force for rotating frames is the centrifugal force which tries to throw you off playground merry-go-rounds and carnival centrifuges. Real forces have to be exerted to keep you moving with the rotating frame.

      The centrifugal force of the Earth just acts as small correction to gravity and is easily treated.

      The Coriolis force is another inertial force for rotating frames. The Coriolis force for the Earth is the inertial force needed for long-range artillery and atmospheric circulation. The Coriolis force acts when you have a velocity relative to a rotating frame.

    3. Spacecraft in free fall.

      Since the internal gravitational field is negligible, there is weightlessness.

    4. The center-of-mass inertial frame of the Earth-Moon system.

      Actually, this reference frame is NOT inertial enough to be used as an inertial frame for accurate calculations.

      To calculate the orbit of the Moon adequately, you have to take into account the variations in the gravitational field of the Sun.

    5. The inertial frame of the fixed stars---which are, in fact, nearby stars.

      This reference frame is very inertial because the fixed stars in their orbits around the center of the Milky Way are pretty much all in the same free-fall region (i.e., region of approximately uniform external gravitational field due to the whole Milky Way).

      For much of Solar-System astronomy, the inertial frame of the fixed stars is adequate for describing motion.

      Actually, the center-of-mass inertial frame of the Solar System which is virtually the same as that of the fixed stars, but it's much easier to locate the fixed stars than that center of mass of Solar System directly.

      By the by, the center of mass of an orbital system has the special name barycenter.

    6. The center-of-mass inertial frames of most isolated galaxies.

    7. Frames of reference that participate in the mean expansion of the universe.

      These are the most fundamental free-fall frames and can be called the comoving frames of the expanding universe. We explicate them further below in subsection Comoving Frames.

  4. Acceleration, Force, and Inertial Frames:

    To further explicate inertial frames, we need to define what we mean by acceleration and force.

    An acceleration is a change in speed AND/OR a change in direction.

    These two kinds of change are illustrated in the two figures just below.

    Now a force is a physical relationship between bodies or between a body and force field (e.g., the gravitational field and electromagnetic field) that causes an acceleration of a body relative to all inertial frames.

    To explicate:

    1. Recall all local reference frames NOT accelerating relative to a local inertial frame are also local inertial frames. But there is usually one inertial frame that is most convenient for analysis of a physical system.

      Often the center-of-mass inertial frame.

    2. 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.

    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.

    Note that Newton's laws of motion are referenced to inertial frames. It is just part of their statements---though this part is often omitted in initial presentations of the laws to students.

    Actually, almost all physical laws are referenced to inertial frames.

    What referenced to means is that the laws do NOT work if NOT applied relative to inertial frames.

    This does NOT mean the physical laws are wrong somehow since they are explicity or implicitly formulated as referenced to inertial frames.

    General relativity is a great exception to the rule that physical laws are referenced to inertial frames. General relativity is the other way around. It tells us what inertial frames are and where they are. See subsection Inertial Frames above.

  5. Inertial Frames and Everyday Life:

    The expression inertial frame does NOT come up much in everyday speech, but inertial frames are actually really well known.

    They are the reference frames we use for understanding most ordinary motion both in the ordinary everyday empirical way used by everyone and all biota and in applying Newtonian physics as discussed above in subsection Acceleration, Force, and Inertial Frames.

    So there is nothing mysterious about inertial frames in everyday life, except the name.

    They are just the reference frames in which your empirical sense of how things move is right.

    Examples of inertial frames (sufficiently inertial for most purposes) are the ground (as discussed above), unaccelerating planes, trains, and automobiles, and the frames of unaccelerating elevators.

    See figure of a nice ground inertial frame below.

    Non-inertial frames are reference frames that are in acceleration with respect to inertial frames as discussed above in subsection Inertial Frames.

    If you are in acceleration relative to one local inertial frame, you are in acceleration relative to them all since they are NOT in acceleration relative to each other.

    Non-inertial frames are common too, but we tend to avoid being in them with our bodies because they are tricky relative to our empirical sense of how things move.

    But we have to be in them when we accelerate in a vehicle of any kind since the vehicle interior defines an non-inertial frame.

    Sometimes we like being in non-inertial frames for fun like playground merry-go-rounds---see the figure below.

    In non-inertial frames, there can be accelerations without forces just due to the motion of the non-inertial frames.

    There will be no accelerations relative to any inertial frame if there are no net forces acting on a body.

    The funny effects in non-inertial frames can be accounted for by inertial forces which we discussed above in subsection Important Examples of Inertial Frames.

    In non-inertial frames, you feel inertial forces that try to throw you around relative to the non-inertial frames.

    If there were no real forces acting on you, Newton's 1st law of motion would just keep you at a constant velocity relative to inertial frames.

    You have to exert real forces to counteract the inertial forces in order to keep moving with the non-inertial frames and be accelerating with them relative to inertial frames.

    Rotating reference frames are particularly difficult to understand because they are actually a continuum of different non-inertial frames.

    See the animation below that dynamically illustrates motion in a rotating reference frame.

  6. Important Examples of Non-inertial Frames:

    Well:

    1. Almost all rotating frames are non-inertial frames.

      We discussed the odd effects in rotating frames above in subsection Inertial Frames and Everyday Life

    2. An example of a very much non-inertial frame (one with only a geometrical nature), consider the geocentric reference frame for the universe.

      The geocentric reference frame is attached to the Earth's surface and has the Earth's center as the origin and extend to the whole universe which rotates around the Earth once per day in this reference frame. See the Earth and the geocentric reference frame in the figure below

      The universe it is overwhelmingly NOT in an uniform external gravitational field with the center of the Earth at its center of mass. No physical law determines the rotational motion of the universe around the Earth in any direct sense.

      However, for astronomical measurement purposes (i.e., astrometry), we often do use the geocentric reference frame for the whole universe as we will discuss in IAL: The Sky.

      Why? Well after all:

      The Earth is our platform for observing the whole universe, and for locating things in the sky, and so for these purposes, the geocentric reference frame is a convenient or natural reference frame.

    3. Most astronomical objects in the observable universe are in an overall sense rotating frames, and so are non-inertial frames.

      See the figure below for examples of rotating astronomical objects.

  7. Comoving Frames

    Are there fundamental inertial frames?

    Isaac Newton (1643--1727) postulated that the average frame of rest of the fixed stars defined the fundamental inertial frame which he called absolute space.

    See the fixed stars in the figure below.

    But, of course, we now know that the fixed stars are all very nearby in the Milky Way and do NOT represent the observable universe.

    So Newton's idea was wrong, but the inertial frame of the fixed stars is a very good inertial frame for many purposes.

    In fact, we do NOT now believe in absolute space in Newton's sense.

    There is no single fundamental inertial frame.

    The expanding universe gives us a different picture.

    Note the expanding universe is the observable universe and probably a lot more, but NOT necessarily the whole universe whatever that is. Maybe the whole universe is the multiverse. Yours truly has invented the expression pan-universe for the whole universe, but yours truly doesn't think it will catch on.

    Note that systems like you, me, moons, planets, stars, galaxies, and probably most galaxy clusters are NOT expanding. But the space between them is. In general relativity, space is a sort of stuff and it can literally grow.

    The two figures below illustrate the expanding universe which is a general scaling up of UNBOUND systems.

    Nowadays from general relativity, we do NOT believe in a single fundamental inertial frame (i.e., a fundamental fundamental inertial frame).

    We believe there are an infinite continuum of fundamental inertial frames. Each one attached to a point participating in the mean expansion of the universe.

    These can be called the comoving frames of the expanding universe. These reference frames are actually in free fall, and so are consistent with our discussion of inertial frames given above in subsection Inertial Frames.

    The region of space up to about the scale of a galaxy cluster or maybe a galaxy supercluster can be approximated to some adequacy as a single local basic comoving frame.

    That single big comoving frame can be used for structures bigger than in the smaller local inertial frames such as those described in subsection Important Examples of Inertial Frames.

    For the observable universe as whole, we are beyond the realm of validity of the concept of inertial frame and use general relativity in a more direct sense.

  8. Center of Mass:

    What the heck is center of mass and why do WE (i.e., YOU) need to know about it for a discussion of inertial frames?---don't panic, we'll NEVER calculate a center of mass---we just need to grok the concept.

    The figure below illustrates and explicates center of mass.

    Below is a figure illustrating a gravitationally-bound system of astronomical objects orbiting the system barycenter (i.e., center of mass).

    The centers of mass for objects of sufficiently high symmetry are the obvious centers of symmetry as the figure below illustrates.

    One can find these centers of mass by inspection.

    For objects where center of mass CANNOT be found by by inspection, one can do a calculation from the formula for center of mass displayed in the figure shown somewhere above.

    However, there is a simple empirical method for finding the center of mass for rigid systems. The method is illustrated in the figure below.

    The center of mass can located deceptively as shown in the figure below.

    ????

  9. The Sun Barycenter Inertial Frame:

    The Sun's mass is 99.86 % of the Solar System mass (see Wikipedia: Solar System: Structure and composition).

    This overwhelming dominance of the Sun's mass means that to good approximation the Sun's center is approximately the barycenter (i.e., orbital system center of mass) of Solar System and can be used to define an approximate inertial frame which is good enough for many purposes.

    However, the inertial frame of fixed stars is more inertial and is easier to use in general.

    Note that the gravitational force the Sun is the main determinant of the structure of the Solar System.

    It pulls the planets into their orbits---which means the planets are in states of acceleration.

    If you recall Newton's 3rd law, you know that for every force there is an equal and opposite force---but note these two forces do NOT have to be on the same body, and so just don't cancel out all the time.

    Thus the planets exert equal gravitational forces on the Sun to what the Sun exerts on them.

    So the Sun should also be accelerated in the frame of fixed stars.

    But, as we will discuss IAL 5: Newtonian Physics, Gravity, Orbits, Energy, Tides, acceleration is proportional to the force and INVERSELY proportional to mass.

    So the gravitational forces of the planets on Sun, do NOT affect the motion of the Sun very much.

    This has been a long story, but it explains why we say "the planets orbit the Sun".

    They orbit the Sun in our local-in-the-Milky Way inertial frame: i.e., the inertial frame of the fixed stars.

    The moons also orbit their planets in inertial frame of the fixed stars.

    However, it also true that they orbit their planets in the approximate inertial frames defined by the planet centers of mass---but these inertial frames are NOT as inertial as the frame of the fixed stars.

    To NOT have to say inertial frame all the time, we often just say the planets physically orbit the Sun and the moons physically orbit the planets.

    The adverb "physically" here having the special meaning of "with-reference-to-a-local-approximate inertial-frame".

  10. Is There a Fundamental Inertial Frame?

    Now I know what you are thinking: is there a fundamental reference inertial frame?

    For everyday life, the ground serves as a basic reference inertial frame.

    All reference frames NOT accelerated with respect to the ground also serve pretty well as inertial frames.

    But the ground is only an approximately inertial frame.

    It's actually, a non-inertial frame if looked at a closely.

    In fact, exact inertial frames are elusive---as we will now discuss and as we illustrate in the figure below.

  11. Exact Inertial Frames Are Comoving Frames of the Expanding Universe:

    Nowadays, we believe there is NOT a single fundamental inertial frame like Newton's hypothesized absolute space.

    Rather we believe there is a continuum of fundamental inertial frames which are frames that participate in the mean expansion of the universe.

    These frames can be called the comoving frames of expanding universe

    The comoving frames are everywhere in a sense---one is definable at every point---but virtually no matter is at rest with respect to them, except very rarely by accident. Most matter is rotating with respect to them and also has a translation velocity with respect to its local comoving frames.

    The expansion of the universe is topic of IAL 31: Cosmology, but we can give brief introduction here.

    The expansion of the universe is the growth of space---yes space---between bound systems---but NOT inside them---you and I are NOT expanding, nor is the Milky Way or other galaxies or gravitationally bound galaxy clusters.

    But the space between the bound systems is growing as the universe scales up.

    The figure and animation below illustrate the expansion of the universe.

  12. Identifying Comoving Frames of Universal Expansion:

    We can actually identify the comoving frames of the expanding universe which are fundamental inertial frames.

    The barycenters of most galaxy clusters are approximately comoving frames---this is a hypothesis which is verified by the consistency of all modern cosmology.

    We can also identify very exactly the local-to-us or nearby-to-us comoving frames by observations.

    Cosmologically remote astronomical objects (i.e., galaxies or quasars) should be unrotating relative to the local-to-us comoving frames in modern theory cosmological theory, and so define for us local unrotating frames.

    Now the cosmic microwave background (CMB) is by modern theory cosmological theory NOT Doppler shifted in a comoving frame.

    But we observe Doppler shift which we call the CMB dipole anisotropy. From that observation, we can determine the translations with respect to the local-to-us and nearby-to-us comoving frames.

    1. The Solar System barycenter is moving at 368 ± 2 km/s in some direction relative to the local comoving frame: i.e., the CMB (see Caltech: Description of CMB Anisotropies).

    2. The Milky Way barycenter is moving at 552(6) km/s in the direction 10.5 hours right ascension (RA), 0.24° declination (Dec or δ) in equatorial coordinates with respect to the local comoving frame (see Wikipedia: Milky Way: Velocity).

    3. Local Group of Galaxies center of mass is moving at 627 ± 22 km/s in some direction relative to the local comoving frame: i.e., the CMB (see Caltech: Description of CMB Anisotropies).

    For very exact, modern studies of motions one actually does make use of local comoving frames.

    Fortunately, we do NOT usually have to work that hard.