When Left Alone
![[url=https://pixabay.com/en/background-wallpaper-blue-1430009/]"Asteroid in Space"[/url] by Frantisek_Krejci, [url=http://pixabay.com/]pixabay is in the [/url][url=http://creativecommons.org/publicdomain/zero/1.0/]Public Domain, CC0[/url]](https://www.geogebra.org/resource/VDzjTA4s/O1VdQC4m2tvyxHPP/material-VDzjTA4s.png)
I gave this chapter a somewhat silly title for a good reason. I want to start our physics discussions with a discussion of what an object's behavior looks like when nothing else is around. The object can be anything you'd like it to be, except that I don't want you to think of moving parts. Picture something like a rock or a ball or a planet seen from space.. We don't want to think of a complex object with movable parts because the added complexity will draw focus away from the point I want to make right now.
Let's say our object is a rock - maybe the asteroid in the picture above. The question I want to pose is this: What will the rock's motion look like if the rock is all alone in the universe? Of course nothing can ever be truly alone, so what I mean by this is that the rock is far away from anything with which it would interact.
The reason this is a question that's worth asking is that if we understand its answer, we will more clearly recognize and be able to describe the rock's motion when other things are around and the rock is not alone.
So picture a rock (asteroid) floating in interstellar space that is far from any planet or star. Consider these questions for a moment:
- Do you suppose the rock could speed up or slow down on its own?
- Do you suppose it could turn?
- If the rock is at first observed to be in motion, what do we expect the properties of this motion to be? Pause and consider these questions before reading on.
Deeper Implications
Having had this brief discussion about inertia, even without getting into any equations we can make a profound statement about nature and physics. The law of intertia was instrumental for Einstein's relativity theories 250 years later. One deeper implication about the law of interia is that there is no difference in the behavior of an object at rest from that of one in motion. What I mean is that whether going what we call quickly or slowly, the behavior is identical. Both continue moving at constant speed in a straight line. There is nothing about going faster that makes the behavior different.
At first glance this argument may seemed flawed. After all, sticking your head or hand out a car window while traveling 30mph versus 120mph is a very different experience. But what you are doing is moving your head or hand relative to the air. Relative velocities are easy to measure and often have real effects associated with them as in the example above. But what if there was no atmosphere? Now could you feel or measure anything different in the car at 30mph versus 120mph when you stick your head out? No!
It is not possible to define a state of absolute rest, only relative rest. We can only ever say that an object is at rest with respect to some other object. You might be thinking that you are at rest right now, but you're only at rest with respect to earth while earth is traveling very rapidly through space in a galaxy that also is moving with respect to other neighboring galaxies. Yet we don't feel like we're moving at hundreds of kilometers per second. That's precisely because there is no difference in how it feels to move rapidly than to not move at all. Motion can only be defined relative to another object. There is no experiment that can be performed to determine whether you are moving or are at rest in an absolute sense. So how quickly is earth moving right now? It depends on who is measuring! The fact that the answer is relative to the observer is at the core of Einstein's relativity theory.
In order to get more sophisticated in discussions of motion we will need to develop some definitions and as you'll see, mathematics will enter our discussions, since it is a much more elegant language than English to discuss natural laws. A more careful discussion of motion will be the focus of the next section.