Solving for Magnitude of Sirius (-1.5) Through Triple Window

  • Thread starter Thread starter Jussi Lundahl
  • Start date Start date
  • Tags Tags
    Magnitude
Click For Summary

Homework Help Overview

The problem involves calculating the apparent magnitude of the star Sirius as observed through a triple window, where each surface reflects away 15% of the incident light. The original poster mentions the magnitude of Sirius as -1.5 and seeks to understand how this changes after passing through the windows.

Discussion Character

  • Exploratory, Assumption checking

Approaches and Questions Raised

  • Participants discuss the definitions of variables in the magnitude equation and the impact of light reflection on intensity. There is an exploration of how to calculate the effective intensity after reflection and its relation to apparent magnitude.

Discussion Status

Some participants have provided calculations and interpretations regarding the effect of light reflection on the apparent magnitude. However, there are reminders about adhering to forum rules against providing complete answers, indicating an ongoing exploration of the topic.

Contextual Notes

There is a mention of the need to clarify the definitions of flux density and luminosity, as well as the implications of the reflection percentages on the calculations. The discussion also highlights the importance of not providing full solutions in the forum.

Jussi Lundahl
Messages
6
Reaction score
0

Homework Statement


Stars are observed through a triple window.
Each surface reflects away 15% of the incident light.
a) What is the magnitude of Sirius (m = -1.5) seen
through the window?

And I know that the solution is -0,97.

Homework Equations


m1-m2=-2,5*log10*(F1/F2)

The Attempt at a Solution


I have no idea what to do...
 
Physics news on Phys.org
Ok, start by telling us what are the F1 and F2 in the equation.
 
If 15% is deflected each time, then sirius's intensity, which let's say is 1 becomes 0.614 since (0.85)^3=0.614

Then, log(1/0.614)*2.5=0.5295

0.5295 is hence the difference between the apparnt magnitudes of the star after it has passed through the three windows. -1.5+0.5295=-0.9704

There's the answer.
 
  • Like
Likes   Reactions: Jussi Lundahl
Bandersnatch said:
Ok, start by telling us what are the F1 and F2 in the equation.

I think those are called flux density in English. $$F=\frac{L}{4 \pi r^2}$$, where the L is luminosity and r is radius. $$ L= \omega r^2$$ where $$\omega$$ is solid angle?? and r is radius.
 
Voltageisntreal said:
If 15% is deflected each time, then sirius's intensity, which let's say is 1 becomes 0.614 since (0.85)^3=0.614

Then, log(1/0.614)*2.5=0.5295

0.5295 is hence the difference between the apparnt magnitudes of the star after it has passed through the three windows. -1.5+0.5295=0.9704

There's the answer.

Thank you! You saved my day :)
 
Voltageisntreal said:
There's the answer.
Please, do not provide full answers to questions posted in the homework forum. Spoon-feeding is against the rules.
 
Member warned not to use text-speak in posts.
Bandersnatch said:
Please, do not provide full answers to questions posted in the homework forum. Spoon-feeding is against the rules.

;o, mb didn't kno rip
 
Voltageisntreal said:
;o, mb didn't kno rip
Text speak is also not permitted!
 

Similar threads

Replies
4
Views
2K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 1 ·
Replies
1
Views
4K
  • · Replies 3 ·
Replies
3
Views
5K
  • · Replies 5 ·
Replies
5
Views
8K
  • · Replies 21 ·
Replies
21
Views
8K
  • · Replies 16 ·
Replies
16
Views
4K
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 5 ·
Replies
5
Views
5K
  • · Replies 1 ·
Replies
1
Views
5K