How Do Scientists Measure Distance Using Standard Candles?

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SUMMARY

Scientists measure astronomical distances using standard candles, specifically type Ia supernovae, which have a consistent luminosity due to their formation from white dwarf stars reaching a critical mass. When observing these supernovae, if one appears brighter than another, it indicates that it is closer to Earth. The difference in brightness allows astronomers to calculate the distance based on the known luminosity of type Ia supernovae. This method relies on the physics of these stellar explosions, which ensures uniform intensity across different events.

PREREQUISITES
  • Understanding of type Ia supernovae and their characteristics
  • Knowledge of luminosity versus brightness in astrophysics
  • Familiarity with distance measurement techniques in astronomy
  • Basic principles of stellar evolution and white dwarf stars
NEXT STEPS
  • Research the physics behind type Ia supernovae and their formation
  • Learn about the inverse square law of light and its application in distance measurement
  • Explore other standard candles used in astronomy, such as Cepheid variables
  • Investigate the role of supernovae in cosmology and the expansion of the universe
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Astronomers, astrophysics students, and anyone interested in understanding distance measurement techniques in the universe, particularly through the use of standard candles like type Ia supernovae.

hobobobo
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I'm kinda confused about how standard candle works. I know they use type 1 supernovae since their luminosity is the same everywhere but how do scientists know how far a star is if their luminosity is the same everywhere. I don't really get how they measure distance with it. Can someone please explain to me! thanx^^
 
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If the luminosity of two objects are the same they will appear to be equally bright when viewed from a equal distance. They will not appear to be equally bright when viewed from different distances. Thus if we see two type 1 supernovae, and one is brighter than the other, we know that it is closer to us than the other. And by how much brighter we can tell how much nearer it is.
 
I think that scientists can infer that all type I supernova have about the same luminosity because of the physics behind this specific type of supernova. I believe it only occurs with a certain mass of star, so the explosions are relatively the same intensity for all of them. The other half is what Janus said :)
 
hmmmm I see because I was confused of luminosity and brightness like the difference from those two.
 
I always thought it was odd that we know dark energy expands our universe, and that we know it has been increasing over time, yet no one ever expressed a "true" size of the universe (not "observable" universe, the ENTIRE universe) by just reversing the process of expansion based on our understanding of its rate through history, to the point where everything would've been in an extremely small region. The more I've looked into it recently, I've come to find that it is due to that "inflation"...

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