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oemBiology oemBiology
wrote...
Posts: 1247
5 years ago
I would like to know on how to determine the brigthness of different planets.

1) any data source to find on what the brightness intensity is for different planets?
2) What formula to determine the brightness of different planets viewing from Earth?

Does anyone have any suggestions?
Thanks in advance for any suggestions
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wrote...
Educator
5 years ago
Planet luminosity depends on the planet's atmosphere, generally its chemical makeup.

I think the relative brightness is measured in \(\frac{mag}{\operatorname{arcsec}^2}\)

Take for example, Jupiter:

https://www.calsky.com/?Jupiterviewer=
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oemBiology Author
wrote...
5 years ago
Planet luminosity depends on the planet's atmosphere, generally its chemical makeup. I think the relative brightness is measured in \(\frac{mag}{\operatorname{arcsec}^2}\) Take for example, Jupiter: https://www.calsky.com/?Jupiterviewer=

That is what I look for and would like to know on any data source to retrieve those historical data.
Do you have any suggestions?
Thank you very much for any suggestions (^v^)
wrote...
Educator
5 years ago
This number is calculated mathematically with the help of telescopes.

I found some documents that make reference to the number 5.4 mag [see attachment]. They mention Near-Infrared Coronagraphic Imager

Additional information: http://iopscience.iop.org/article/10.1086/300553/fulltext/

I'll need to research this more to give you a precise document as to when it was first document (it'll be hard), but I'll keep you posted by tomorrow




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oemBiology Author
wrote...
5 years ago
I look forward to your reply
Thank you very much for any suggestions (^v^)
wrote...
Educator
5 years ago
Hi again oem7110

I strongly recommend you read this article: https://en.wikipedia.org/wiki/Apparent_magnitude

The article states:

The apparent magnitude \((m)\) of an astronomical object is a number that is a measure of its brightness as seen by an observer on Earth. The magnitude scale is logarithmic. A difference of 1 in magnitude corresponds to a change in brightness by a factor of \(\sqrt[5]{100}\), or about \(2.512\). The brighter an object appears, the lower its magnitude value (i.e. inverse relation), with the brightest astronomical objects having negative apparent magnitudes: for example Sirius at \(−1.46\). The measurement of apparent magnitudes or brightnesses of celestial objects is known as photometry.

You might also be interested in Surface brightness. For that, I recommend this article: https://en.wikipedia.org/wiki/Surface_brightness


I did more searching and found this journal article from the year 1899: http://adsabs.harvard.edu/full/1899ApJ....10..225H

It discusses in detail how it's calculated (beyond my scope of knowledge)



Hopefully this helps!
oemBiology Author
wrote...
5 years ago
Thank you very much for suggestions (^v^)
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