Tag Archives: space time

Close-up of an ornate astronomical clock with zodiac signs and intricate golden details.

Five Facts about Time

Here are some interesting facts to ponder about of time:

  1. There is no widely accepted scientific definition of time as a stand alone entity. The reason for this is that according the Einstein’s theory of relativity, time and space are integrated into space-time.
  2. Some physicists argue that “time” has not always existed. According to the big bang theory, the universe started as an infinitely dense small energy ball that expanded to create the universe we now observe. Since some physicist argue that time is a measure of change, before the big bang, there was no change. Hence, there was no time.
  3. Time as measured by clocks will actually slow down in a reference frame moving close to the speed of light or in a high gravitational field. This has been experimentally proven.
  4. Time on Earth is slowing down. Our human perception of time comes from the rotation of the Earth relative to the Sun. Due to tidal friction from the sun and moon, the solar day is lengthening by 1.7 milliseconds each century as the Earth’s rotation slows down.
  5. Your significant other has their own definition of time. It is called a “jiffy.” The jiffy is an undefined time interval that can mean a faction of second to an hour or more. They generally use it in the phrase, “I’ll be ready in a jiffy.”  🙂
Close-up of a large clock face with Roman numerals illuminated by warm golden light.

The Science of Time – Part 3/3

The Science of Time: This is taken from appendix 5 of my new book, How to Time Travel, which will be available on Amazon in early September 2013.

Approaching a scientific definition of time

How is coordinate time related to proper time? Einstein’s special theory of relativity relates coordinate time and proper time by the following convention. For an observer with a clock in an inertial frame of reference, the coordinate time at the event is equal to proper time at the event when measured by a clock that is stationary relative to the observer and at the same location as the event. This convention assumes synchronization of the clock at the event with the observer’s clock. Unfortunately, there have been numerous methods suggested for accurately synchronizing clocks and defining synchronization. For our purposes in defining coordinate time and proper time, it is only important to assume the hands of both clocks move in unison, independent of the method of synchronization.
Most of the scientific community agrees that the most accurate definition of time requires integration with the three normal spatial dimensions (i.e., height, width, and length). Therefore, the scientific community talks in terms of spacetime, especially in the context of relativity, where the event or observer may be moving near the speed of light relative to each another.

Let us consider an example. A clock moving close to the speed of light will appear to run slower to an observer at rest (one frame of reference) relative to the moving clock (another frame of reference). In simple terms, time is not an absolute, but is dependent on the relative motion of the event and observer. It may sound like science fiction that a clock moving at high velocity runs slower, but it is a widely verified science fact. Even the clock on a jet plane flying over an airport will run slightly slower than the clock at rest in the airport terminal. Einstein predicted this time dilation effect in his special theory of relativity, and he derived an equation to calculate the time difference.

Other physical factors affect time. For example, another scientific fact is that a clock in a strong gravitational field will run slower than a clock in a weak gravitational field. Einstein predicted this time dilation effect in his general theory of relativity.
Lastly, the time dilation effects of high velocity and strong gravitational fields are additive. That means a clock moving near the speed of light will move slower if it enters a strong gravitational field.
I termed this section “Approaching a scientific definition of time” for a reason. There is no consensus on the scientific definition of time. However, we can help ourselves conceptualize time by summarizing the salient points discussed above:

  • In our everyday existence, time appears to be an absolute. Time is the same for everyone. When an event occurs, we believe it to occur simultaneously regardless of its relative position or velocity to us, or our relative position or velocity to the event. This is our everyday reality. We typically do not worry about accurately synchronizing our watches, since a minute one way or the other does not matter for most real-life applications. The simple fact is that treating time as an absolute works in most real-life applications. However, it is an illusion and breaks down as the relative velocity of any constituent approaches the speed of light, or when the distances from the event become extremely large and different for the observers. On this last point, regarding relative distances, consider the following example. An observer close to an event will record its occurrence a thousand years sooner than an observer a thousand light-years from the event. The reason for this is that it takes the light a thousand years to reach the furthest observer. This means that the stars we view at night may no longer exist. The light has traveled thousands to millions of light-years to reach our eyes. The stars may have died long ago, but we will not know it for thousands to millions of years.
  • In the world of relativity, where frames of reference can move near the speed of light or gravitational fields can play a factor, time becomes relative. Here are four examples.

1. A clock moving near the speed of light will appear to run slower to an observer at rest, relative to the clock.

2. A clock in a strong gravitational field will appear to run slower to an observer a distance (as little as one meter) farther away from the gravitational field.

3. A clock will run even slower when moving near the speed of light when it enters a strong gravitational field (i.e., the affects are additive).

4. An event will appear to occur first to the observer closest to the event. The farther away an observer is from an event, the longer it will take the light to travel to the observer, and for the observer to become aware of the event.

Notice that all our attempts to define time fail. Instead, we describe how time behaves during an interval, a change in time. We are unable to point to an entity and say “that is time.” The reason for this is that time is not a single entity, but scientifically an interval. We cannot slice time down to a shadow-like sliver, a dimensionless interval. In fact, scientifically speaking, the smallest interval of time that science can theoretically define, based on the fundamental invariant aspects of the universe, is Planck time.

Planck time is the smallest interval of time that science is able to define. The theoretical formulation of Planck time comes from dimensional analysis, which studies units of measurement, physical constants, and the relationship between units of measurement and physical constants. In simpler terms, one Planck interval is approximately equal to 10^-44 seconds (i.e., 1 divided by 1 with 44 zeros after it). As far as the science community is concerned, there is a consensus that we would not be able to measure anything smaller than a Planck interval. In fact, the smallest interval science is able to measure as of this writing is trillions of times larger than a Planck interval. It is also widely believed that we would not be able to measure a change smaller than a Planck interval. From this standpoint, we can assert that time is only reducible to an interval, not a dimensionless sliver, and that interval is the Planck interval. Therefore, our scientific definition of time forces us to acknowledge that time is only definable as an interval, the Planck interval.

Close-up of an ornate clock face with Roman numerals illuminated by a warm golden light.

The Science of Time – Part 2/3

The Science of Time: This is taken from appendix 5 of my new book, How to Time Travel, which will be available on Amazon in early September 2013.

What happens as the frames of reference move at velocities close to the speed of light? To address this question, we need to discuss the Lorenz transformation.

Time is relative (Lorenz transformation)

To transfer the time coordinates between frames moving close to the speed of light, an entirely new transformation methodology needed to be developed. Einstein became painfully aware of this during the development of his famous special theory of relativity. As a result, he utilized the Lorenz transformation. Some authors give Einstein credit as having developed the Lorenz transformation. This is not historically correct. The Lorenz transformation was in existence prior to Einstein’s publication of the special theory of relativity in 1905. In fact, numerous physicists, including Voigt (1887), Lorentz (1895), Larmor (1897), and Poincaré (1905), contributed to its formulation. It was Poincaré, in 1905, who brought it into its final modern form and named it the Lorenz transformation. It is fair, though, to say that Einstein rederived the Lorenz transformation in the context of special relativity.

Just what is the Lorenz transformation, and how does it treat the time coordinate between frames moving at a constant rate close to the speed of light? It takes into account that light travels at a finite speed (approximately 186,000 miles/second), and that speed is a constant in any frame of reference moving at a constant velocity, typically referred to as an inertial frame of reference. As a result, according to the Lorenz transformation, different observers moving at different velocities or at rest will not measure time in the same way. Indeed, they may measure different elapsed times, and even a different orderings of events.

Time as a coordinate

At this point, it may appear obvious that time is a coordinate. Both the Galilean and Lorenz transformations view time as a coordinate, and they only differ in how they translate the time coordinate between initial frames of reference. Intuitively, when you think of time as a coordinate, it makes sense. For example, when you set a meeting, you not only set the place (i.e., the spatial coordinates), but the time (i.e., the temporal coordinate). In this context, time is a coordinate (i.e., also known as “coordinate time”). This terminology distinguishes it from “proper time,” which is not a coordinate, but rather a process. In Einstein’s special theory of relativity, “proper time” (also known as “clock time”) is a measure of change, such as the number of rotations of a simple mechanical clock’s hands. It is arbitrary. For example, proper time may refer to the time it takes a candle to burn down to a specific point. Before we go further, let us be perfectly clear on the distinction of time as a coordinate (“coordinate time”) and proper time (“clock time”). If you specify that you will meet someone at a specific time, you are using “coordinate time.” If you say it takes the second hand of your watch one minute to make a compete revolution, you are talking about proper time (“clock time”). You may wonder if coordinate time and proper time are related. It turns out they are. Einstein’s special theory of relativity relates coordinate time, proper time, and space to each other via spacetime, which we will discuss next. Stay tuned for The Science of Time – Part 3/3