Lightyear Distance: Understand Its Impact

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Discussion Overview

The discussion revolves around the concept of measuring astronomical distances in light-years, particularly in the context of how gravity affects light and the implications for distance measurement in cosmology. Participants explore the definitions and standards of light-years and meters, as well as the practicalities and theoretical considerations involved in these measurements.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Some participants question the consistency of light being affected by gravity and its implications for measuring distances in light-years.
  • Others argue that space is flat between galaxies, making light-years a sensible unit for measuring vast distances in the observable universe.
  • A participant suggests that while stacking metersticks is impractical, light-years and meters ultimately represent the same distance due to the definition of the meter in terms of the speed of light.
  • Another participant clarifies that a light-year is defined as the distance light travels in one Julian year in a vacuum, emphasizing that it does not imply that light took that exact time to reach us from distant objects.
  • Some participants note that while the Shapiro time delay is a consideration, it occurs infrequently in the context of the Milky Way.
  • There is a discussion about the convenience of using light as a standard for distance measurement, given its constant speed, and how this relates to the definition of the meter.
  • One participant highlights that for large distances, the effects of curvature in spacetime become significant, similar to how navigation on Earth requires different considerations at large scales.
  • Another point raised is that using light-years provides immediate information about how far away an object was at the time of emission, which is particularly relevant for receding galaxies.
  • Some participants express concern that the phrasing regarding distance could be misunderstood, advocating for clarity in communication about distances in the context of cosmic expansion.

Areas of Agreement / Disagreement

Participants express a range of views on the implications of using light-years as a measurement unit, with some agreeing on the convenience of this standard while others raise concerns about its consistency and the effects of gravity on light. The discussion remains unresolved, with multiple competing perspectives present.

Contextual Notes

Limitations include the dependence on definitions of distance and the unresolved nature of how gravity affects light over vast distances. Participants acknowledge that the effects of spacetime curvature may vary significantly depending on the scale of measurement.

Mickeydee
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if light is affected by gravity (ie. bend, stretch, curve) inconsistent.
why do we measure distance in lightyear?
 
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Mickeydee said:
if light is affected by gravity (ie. bend, stretch, curve) inconsistent.
why do we measure distance in lightyear?
Space is flat between galaxies and overall (mainly) in the observable universe so it makes sense to measure this way given the enormous distances.
 
Furthermore, what is your alternative? Even if stacking metersticks were practical, they would have the same issues.
 
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Mickeydee said:
if light is affected by gravity (ie. bend, stretch, curve) inconsistent.
why do we measure distance in lightyear?
In modern physics the second has a definition and light speed is defined to be ##299,792 km/s##.

So, the metre is in fact defined in terms of the speed of light.

It doesn't matter, therefore, whether we quote a distance in light years or in metres. It means exactly the same thing.

Your question could be rephrased by asking what we really mean when we say, for example, that a star is 25 light years away (or whatever the equivalent is in metres)? And what sort of measurement process are we assuming?

One answer is that you might as well use the path that light takes. As spacetime is curved, no other path makes any more sense and, indeed, the light path might seem the most natural.
 
The "light year" is a standard. It is the distance light would travel in one Julian year (365.25 days) in a vacuum through flat space. So when we say something is 1 million light years away, we mean that it is 1 million multiples of that distance away, not that the light leaving it took exactly 1 million Julian years to reach us, taking into account any bending of the light path along the way.

Similarly we have the parsec. Which the distance at which an object would exhibit 1 arc sec of parallax. Again, if we say a galaxy is 1 billion parsecs away, we mean that it is 1 billion multiples of these units of distance away, not that we measured its parallax and came up with this distance from that measurement, as parallaxes at this distance are just too small to measure. The fact that we can't directly measure the parallax of this galaxy doesn't preclude us from giving its distance in parsecs.
 
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Mickeydee said:
if light is affected by gravity (ie. bend, stretch, curve) inconsistent.
why do we measure distance in lightyear?
you seem to think of the Shapiro time delay. But if light crosses the whole milky way thereby passing near stars happens extremely seldom presumably.
 
Mickeydee said:
if light is affected by gravity (ie. bend, stretch, curve) inconsistent.
why do we measure distance in lightyear?

We can measure distances in any units we like - meters, light-years, inches, furlongs.

The constancy of the speed of light makes it a convenient way to standardized our distance measurements, in fact, the definition of the meter used to be the distance that light traveled in 1/299,792,458 of a second . Nowadays this definition is worded a bit more abstractly, but it boils down to the same thing.

If you'd like to ask why, how, or when we settled on using light as the basis for our definition, we can attempt to discuss that, but it's not clear if that's what you're asking.

This standard definition of the meter alone does not account for the stretching, bending, etc. of space-time. The definition applies for small distances, where these effects are negligible. For small distances, the bending, stretching et al doesn't matter, similarly to the way one can draw local maps of the Earth's surface on a flat sheet of paper without difficutlies.

For large distance it does matters, just as for large distances on the Earth one needs to use a globe to get accurate visualizations of navigation and long distances.

The units still don't really matter - if you have a long distance, you have the same issues with regard to curvature, whether or not you call that distance 9.461e+15 meters or if you call it instead 1 light year.
 
Ignoring the recent measurements of gravity waves, the only thing we get from those distances is light (electromagnetic waves), so it is very natural and convenient to use lightyears as units of distance. It immediately tells us how far away it is was at the time of emission and how long ago that was.
 
Last edited:
FactChecker said:
It immediately tells us how far away it is and how long ago it was.
This could be misunderstood by the OP. I'd prefer to say how far it was away at the time of emission, if we talk about galaxies which recede with the Hubble flow.
 
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timmdeeg said:
This could be misunderstood by the OP. I'd prefer to say how far it was away at the time of emission, if we talk about galaxies which recede with the Hubble flow.
Good point. I edited it to be clearer.
 

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