High School Lightyear Distance: Understand Its Impact

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SUMMARY

The discussion centers on the concept of lightyears as a unit of distance in astronomy, emphasizing its practicality given the vastness of space. Light travels at a constant speed of 299,792 km/s, and the lightyear is defined as the distance light travels in one Julian year (365.25 days) in a vacuum. The conversation highlights that while light may be affected by gravity, the use of lightyears provides a standardized method for measuring astronomical distances, which remains consistent despite the complexities of spacetime curvature. Additionally, the parsec is introduced as another unit of measurement, defined by parallax, further illustrating the challenges of measuring vast distances in the universe.

PREREQUISITES
  • Understanding of the speed of light (299,792 km/s)
  • Familiarity with the concept of a Julian year (365.25 days)
  • Basic knowledge of spacetime curvature and its effects on light
  • Awareness of astronomical distance units such as lightyears and parsecs
NEXT STEPS
  • Research the implications of spacetime curvature on light propagation
  • Learn about the measurement techniques for astronomical distances, including parallax
  • Explore the historical development of distance measurement standards in astronomy
  • Investigate the concept of the Hubble flow and its impact on distance measurements
USEFUL FOR

Astronomers, astrophysicists, and students of physics who seek to deepen their understanding of distance measurement in the universe and the implications of light's behavior in curved spacetime.

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.
 
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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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