Age & Distance of Stars: Clarifying Light Speed Impact

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SUMMARY

The discussion clarifies that the age of stars is generally evenly distributed with respect to their distance from Earth, with no inherent age correlation based solely on distance. It emphasizes that light from distant stars and galaxies acts as a time capsule, revealing their past states due to the finite speed of light. The Hubble constant, approximately 70 km/s/Mpc, plays a crucial role in understanding the relative speeds of these celestial bodies. Additionally, the apparent speed of receding galaxies, measured through redshift, is a fundamental aspect of cosmic expansion, regardless of whether the universe is accelerating or decelerating.

PREREQUISITES
  • Understanding of the Hubble constant (70 km/s/Mpc)
  • Familiarity with redshift and its implications in astronomy
  • Basic knowledge of stellar evolution and age distribution
  • Concept of light travel time in astrophysics
NEXT STEPS
  • Research the implications of the Hubble constant on cosmic expansion
  • Learn about redshift and its measurement techniques in astronomy
  • Explore stellar evolution and the lifecycle of stars
  • Investigate the concept of light travel time and its effects on astronomical observations
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Astronomers, astrophysicists, and students of cosmology who seek to understand the relationship between distance, age, and the observable universe.

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Are stars far away the same age as stars closer, or are they younger or older?

And wouldn't the speed of light make the planets farther away less then estimates say they are?
 
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Light from astronomical bodies just makes them appear younger than they are because photons do not age as they approach us; they are frozen in the moment of time at which they are emitted from their source, traveling at the speed of light, to the moment they impinge on our retina.
 
The age of stars can be assumed to be evenly distributed with respect to distance from us. There are lots of reasons why stars are clumped by age (such as stellar nurseries) but in general, there's no reason why a young star couldn't be right next door.

I think you're talking about telescopes being a sort of time machine looking into the past. This is true. Stars that are 4 ly away are seen as they were 4 years ago. Stars that are 2 million ly away are seen as they were 2My ago.

This fact has not escaped astronomers, and they take it into account.



"And wouldn't the speed of light make the planets farther away less then estimates say they are?"

Yes, our view of the planets is delayed by a few light-minutes to light-hours.

All well-accounted for. Our "estimates" are pretty accurate. We know a LOT about where they are and where they're going. We can predict their positions many, many years, decades, and to some degree, centuries, into the past and future. And we can know their present positions accurately enough to land spacecraft on them.
 
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Dmstifik8ion said:
Light from astronomical bodies just makes them appear younger than they are because photons do not age as they approach us; they are frozen in the moment of time at which they are emitted from their source, traveling at the speed of light, to the moment they impinge on our retina.
With all due respect, this is an odd and rather misleading pseudo-explanation. It seems to suggest that the distance=peering-into-the-past is some sort of illusion, instead of a very real and fundamental part of our universe.
 
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if the universe is expanding and the relative speed from us is v=HR[\tex] where H is hubbell const (around 70 parsec/sec if i recall correctly)<br /> <br /> apart from the fact that light takes time to reach us from distant planets, the stars that are far from us are seem to be slower because of their relative speed, and the ones at the edge (v approaches c) are almost frozen in time as far as were concerned...
 
fargoth said:
if the universe is expanding and the relative speed from us is v=HR[\tex] where H is hubbell const (around 70 parsec/sec if i recall correctly)<br /> <br /> apart from the fact that light takes time to reach us from distant planets, the stars that are far from us are seem to be slower because of their relative speed, and the ones at the edge (v approaches c) are almost frozen in time as far as were concerned...
<br /> I don&#039;t think that relativistic time dilation plays much of a part in this. <br /> <br /> The dilatory factor remains effectively zero until within a few percent of the speed of light. This means that, in the 13.7Gly to the edge of the observable universe, only the last few 100Mly or so (i.e. &lt; the skin on a universe-sized apple) would exhibit any observable time dilation at all.
 
The Hubble flow is negligible until you reach mega-parsec distance scales; at which point it is extremely difficult to resolve individual stars. On the other hand, all photons we observe are time capsules that represent their personal surface of last scattering.
 
Okay, so here was a simple idea that I'm pretty sure is wrong, but who knows?Anyway,

Since stars further away are seen moving faster then stars closer, and those stars are seen as younger, does that mean that as time passes, the expansion slows, answering the question of what's happening to the universe?

Please tell me how I'm wrong in this conjecture, for I am almost sure I am.
 
DaveC426913 said:
The age of stars can be assumed to be evenly distributed with respect to distance from us.

Well, it depends on the scales you're talking about. The average age of the stellar populations tends to decrease with distance above the galactic plane. Within a bubble of 100 pc, the ages should be fairly evenly (though not smoothly) distributed. In a bubble of a kiloparsec, there would definitely be a noticable gradient. On still larger scales, you'll see gradients in the radial direction as well.
 
  • #10
Blahness said:
Since stars further away are seen moving faster then stars closer, and those stars are seen as younger, does that mean that as time passes, the expansion slows, answering the question of what's happening to the universe?

I'll assume you're talking about cosmological scales, on which we observe galaxies and quasars instead of individual stars. It turns out that more distant objects would appear to be moving more quickly (and appear younger) regardless of whether the universe were accelerating or decelerating.

Think of it this way. The apparent speed of the receding galaxies is measured by the redshift of their light. The amount that light becomes redshifted is related to the amount by which the universe has expanded during its journey to us. Light coming from more distant objects will always have to travel further to reach us, so the universe will always have expanded more during its trip. Thus, light from more distant objects will always appear more redshifted and we'll always infer their recession velocities to be higher, as long as the universe is expanding. If the universe were contracting, then the opposite would be the case.
 
  • #11
^That's the kind of perfect explanation I love to see!

Thank you! ^_^'
 

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