Universal Reference Point question

In summary, the conversation discusses the idea of using a universal reference point on Earth to measure relativistic effects for potential time travel in the future. However, it is pointed out that it is difficult to define an inertial reference frame on Earth due to its constant movement and the effects of gravity on a larger scale. This may make the concept of a universal reference point impractical.
  • #1
Chaos' lil bro Order
683
2
If in the future humans master time travel, might it be valuable to know a Universal Reference point that is common to both the present and past coordinates in space and time. For example, say we designated a single point on Earth from which all other relativistic effects are to be measured against. We could set this point as a microdot in a NIST building, sitting on a pedestal and when we created it we'd stamp the exact time, position to the sun and moon and all sorts of other data beside it. Everyone in the world who thought time travel may be possible in their life times invests in an atomic watch with GPS and the watch always calculates your relative position in time and space versus the NIST dot and it takes into the relativistic effects of you moving about in your life 1000s of miles away from the dot. The watch also downloads and tracks the movements of the Earth in the solar system, the solar system in the galaxy, and the galaxy in the cluster? with the goal of making the dot an inertial reference point in time. Who knows what form of time travel if any will be available in the future, this universal reference point may be useful or never, I am not sure.
 
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  • #2
I just got one of these watches yesterday. Best thing is, it also has a built in mp3 player.
 
  • #3
Al68 said:
I just got one of these watches yesterday. Best thing is, it also has a built in mp3 player.

Why should I care, read this again.
 
  • #4
Chaos' lil bro Order said:
If in the future humans master time travel, might it be valuable to know a Universal Reference point that is common to both the present and past coordinates in space and time. For example, say we designated a single point on Earth from which all other relativistic effects are to be measured against. We could set this point as a microdot in a NIST building, sitting on a pedestal and when we created it we'd stamp the exact time, position to the sun and moon and all sorts of other data beside it. Everyone in the world who thought time travel may be possible in their life times invests in an atomic watch with GPS and the watch always calculates your relative position in time and space versus the NIST dot and it takes into the relativistic effects of you moving about in your life 1000s of miles away from the dot. The watch also downloads and tracks the movements of the Earth in the solar system, the solar system in the galaxy, and the galaxy in the cluster? with the goal of making the dot an inertial reference point in time. Who knows what form of time travel if any will be available in the future, this universal reference point may be useful or never, I am not sure.

You can't use a point (and set of axes) on the Earth to define an inertial reference frame, because it's not inertial. (Earth rotates on its axis once a day, and moves around its center of mass with the moon, and orbits the sun, and the sun moves around the galaxy, and the galaxies move relative to each other, and so on). You can't use a non-inertial reference point because it doesn't uniquely define times and locations elsewhere, because changing velocity leads to changing simultaneity.

If you ask where you are "now" relative to a reference point, you need to define the frame in which "now" is calculated. If it is the subjective frame, that means the same event would have different coordinates depending on the velocity of the observer. If it is the frame of the "reference point", that has to be inertial, otherwise it cannot uniquely label distant events.

In general, you can't define an inertial frame which is useful both locally and at the galactic scale, because of gravity. A frame which "feels" inertial locally is one which is actually in free fall, so is being affected by gravity, which varies with location. You can at least detect and eliminate rotation locally relative to the fixed stars to a high accuracy, but it is not practical to calculate the linear gravitational acceleration due to all stars, galaxies and so on and define an "inertial" frame in that way, especially as on a larger scale you would find that the expansion of the universe would also affect it.
 
  • #5
Jonathan Scott said:
You can't use a point (and set of axes) on the Earth to define an inertial reference frame, because it's not inertial. (Earth rotates on its axis once a day, and moves around its center of mass with the moon, and orbits the sun, and the sun moves around the galaxy, and the galaxies move relative to each other, and so on). You can't use a non-inertial reference point because it doesn't uniquely define times and locations elsewhere, because changing velocity leads to changing simultaneity.

If you ask where you are "now" relative to a reference point, you need to define the frame in which "now" is calculated. If it is the subjective frame, that means the same event would have different coordinates depending on the velocity of the observer. If it is the frame of the "reference point", that has to be inertial, otherwise it cannot uniquely label distant events.

In general, you can't define an inertial frame which is useful both locally and at the galactic scale, because of gravity. A frame which "feels" inertial locally is one which is actually in free fall, so is being affected by gravity, which varies with location. You can at least detect and eliminate rotation locally relative to the fixed stars to a high accuracy, but it is not practical to calculate the linear gravitational acceleration due to all stars, galaxies and so on and define an "inertial" frame in that way, especially as on a larger scale you would find that the expansion of the universe would also affect it.

Excellent post, thank you for your reply.
 

What is a Universal Reference Point?

A Universal Reference Point is a fixed location or object that is used as a standard for measuring or comparing other things. It serves as a reliable and consistent point of reference for scientific or mathematical calculations.

Why is a Universal Reference Point important in science?

A Universal Reference Point is crucial in science because it allows for accurate and precise measurements. By having a standardized point of reference, scientists can ensure that their data is consistent and comparable, making it easier to draw conclusions and make predictions.

What are some examples of Universal Reference Points?

Some common examples of Universal Reference Points include the Sun, the North Star, and the equator. These are all fixed points that can be used to measure time, direction, and location, respectively.

Can Universal Reference Points change over time?

Yes, Universal Reference Points can change over time. This can be due to shifts in the Earth's axis or changes in the natural cycles of celestial bodies. In order to maintain accuracy, scientists constantly monitor and adjust their measurements to account for any changes.

How do scientists determine the accuracy of a Universal Reference Point?

Scientists use multiple methods to determine the accuracy of a Universal Reference Point. This can include comparing it to other established reference points, conducting experiments and calculations, and using advanced technology such as GPS satellites. Through these processes, scientists can ensure that their chosen reference point is reliable and consistent.

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