High School Variation of Apparent Luminosity with Distance

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SUMMARY

The discussion focuses on the relationship between true luminosity and apparent luminosity of celestial objects, specifically object X and object Y. It establishes that apparent luminosity is inversely proportional to the square of the distance from the observer, represented by the formula ##A_X = \frac{T_X}{D_X^2}##. The conversation also highlights that true luminosity can be calculated using the formula ##T_X = A_X \times D_X^2##. Additionally, it emphasizes that distance measurements, such as parallax, do not rely on luminosity.

PREREQUISITES
  • Understanding of true luminosity and apparent luminosity concepts
  • Familiarity with the formula for luminosity and distance relationships
  • Knowledge of parallax as a distance measurement technique
  • Basic grasp of the physics of light propagation and energy distribution
NEXT STEPS
  • Study the Cosmic Distance Ladder to understand distance measurement techniques
  • Learn about the inverse square law of light and its implications in astronomy
  • Explore advanced concepts in photometry and luminosity calculations
  • Investigate the role of parallax in measuring astronomical distances
USEFUL FOR

Astronomers, astrophysics students, and anyone interested in understanding the principles of luminosity and distance in celestial observations.

Agent Smith
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True luminosity of object X = ##T_X##
Apparent luminosity object X = ##A_X##
Distance of object X from observer = ##D_X##
True luminosity of object Y = ##T_Y##
Apparent luminosity of object Y = ##A_Y##
Distance of object Y from observer = ##D_Y##

Apparent luminosity is something measurable I suppose. Distance is measured by means that don't depend on luminosity (parallax?)

Assuming ##A_X = \frac{T_X}{D_X}## and ##A_Y = \frac{T_Y}{D_Y}##

So we can find ...
1. True luminosity: ##T_X = A_X \times D_X## and ##T_Y = A_Y \times D_Y##
2. The relative distance of luminous objects: Assuming ##A_X = A_Y##, we have ##\frac{D_X}{D_Y} = \frac{T_X}{T_Y}##
 
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Agent Smith said:
Distance is measured by means that don't depend on luminosity (parallax?)
https://en.wikipedia.org/wiki/Cosmic_distance_ladder
Agent Smith said:
Assuming ##A_X = \frac{T_X}{D_X}## and ##A_Y = \frac{T_Y}{D_Y}##
No, the measured luminosity drops with the square of distance. The light emitted in a short time period forms an expanding sphere around the source. The total energy of the light is constant, but spread over the area of the sphere which grows with the square of distance.
 
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So ##A_X = \frac{T_X}{D_X {^2}}##. So I'd be underestimating the true luminosity.
 
https://en.wikipedia.org/wiki/MoM-z14 Any photon with energy above 24.6 eV is going to ionize any atom. K, L X-rays would certainly ionize atoms. https://www.scientificamerican.com/article/whats-the-most-distant-galaxy/ The James Webb Space Telescope has found the most distant galaxy ever seen, at the dawn of the cosmos. Again. https://www.skyatnightmagazine.com/news/webb-mom-z14 A Cosmic Miracle: A Remarkably Luminous Galaxy at zspec = 14.44 Confirmed with JWST...

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