How Do Scientists Measure Distance Using Standard Candles?

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Discussion Overview

The discussion revolves around the concept of measuring astronomical distances using standard candles, specifically type Ia supernovae. Participants explore the principles behind luminosity and brightness, and how these relate to distance measurements in astronomy.

Discussion Character

  • Exploratory, Conceptual clarification

Main Points Raised

  • One participant expresses confusion about how standard candles work, particularly in relation to measuring distance based on luminosity.
  • Another participant explains that if two objects have the same luminosity, they will appear equally bright at the same distance, but will differ in brightness when viewed from different distances, allowing for distance estimation.
  • A third participant adds that the uniform luminosity of type Ia supernovae is inferred from the physics of their explosions, which occur at a specific mass, leading to similar intensities.
  • One participant acknowledges confusion between the concepts of luminosity and brightness, indicating a need for clarification on these terms.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the understanding of luminosity versus brightness, and some confusion remains regarding the measurement process using standard candles.

Contextual Notes

There are limitations in the discussion regarding the definitions of luminosity and brightness, as well as the assumptions underlying the uniformity of type Ia supernovae luminosity.

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.
 

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