Age of Light: How is it Estimated?

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SUMMARY

The age of light from astronomical objects is estimated using standard candles such as Type IA Supernovae and Cepheid variables, which allow astronomers to calculate distances based on their known brightness. This distance is then calibrated using redshift, a phenomenon observed through the Doppler effect, where light waves elongate due to the speed of the source and the expansion of the universe. The age of the light is directly correlated to the distance of the emitting object; for instance, light from an object 10 billion light years away is considered to be 10 billion years old by the time it reaches Earth. The process of determining these distances is often referred to as the "distance ladder."

PREREQUISITES
  • Understanding of standard candles in astronomy
  • Familiarity with redshift and the Doppler effect
  • Knowledge of light propagation and inverse square law
  • Basic concepts of cosmic distance ladder
NEXT STEPS
  • Research the mechanics of Type IA Supernovae and their role in distance measurement
  • Study the principles of redshift and its calculation methods
  • Explore the concept of the cosmic distance ladder in detail
  • Investigate the implications of light travel time on our understanding of the universe
USEFUL FOR

Astronomers, astrophysics students, and anyone interested in understanding the methods used to estimate the age of light and the distances of celestial objects.

fugg
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Hello. I was recently reading up on the furthest start found so far to have been dated to approximately 13.7 billion years ago if I remember correctly.
I'm curious though, how is the "age" of this light approximated? Photons themselves are radiation right soo...? Thanks in advance.
 
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This is how I [a regular Joe] understand it:

There's objects in the universe that serve as http://en.wikipedia.org/wiki/Standard_candle" . Two are the most common used to calibrate astronomical distances: Type IA Supernovae and Cepheid variables. If you know how bright something is, you can estimate it's distance using an inverse square law of light propagation. Then.. you have to calibrate your measurement using something called "redshift".

Light propagates as a wave (as well as discrete packages of energy: photons). Being a wave, it has a measurable frequency and this frequency can vary for a variety of reasons. In this particular case, Astronomers measure what's called "redshift". Redshift is equivalent to a frequency elongation which can be estimated using the Doppler effect for light.

Analogous to the Doppler effect for sound, light waves can elongate (redshift) or compress (blueshift). The elongation in light from deep deep outer space is caused by 2 things: the speed of source and the expansion of the universe itself.

If you're not familiar with the Doppler effect, think of it as what you hear when you're standing still on the side of the highway and big loud truck passes by [the sound pitch will increase as the osingbject gets closer].

EDIT: Added first paragraph. It didn't pass the first time I posted
 
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To sum it up simply: the age of the light is determined by finding the distance to the object emitting it. If an object is 10 billion light years away, we say the light it emitted is 10 billion years old by the time it gets to us. As JRPB explained, the distance can be determined using the brightness of standard candles, or by measuring redshift. (Hopefully the two measurements should roughly agree with each other)
 
google "distance ladder" But be warned, you might regret learning just how tenuous are our ideas of the size of the universe :smile:
 
Diazona isn't that just begging the question?
Seems a bit tough to chew but interesting nonetheless. Thanks for the responses.
 

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