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Abdul Ahad - Bestselling Author

Abdul Ahad


Last Updated: 11/18/2009

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Gender: Male
Status: Married
Age: 40
Sign: Sagittarius

City: Luton
Country: UK
Signup Date: 3/30/2006

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Thursday, January 11, 2007 

Current mood:  accomplished
Search the internet for "Ahad's constant" and you'll get an inordinate amount of discussion and yet an equal amount of contention about how this number ought to be calculated and what it should be called. Two years ago, when I first calculated a one number solution for the universe's total background illumination, it never occurred to me that the net value of such a logarithmic series could become the subject of so much controversy even to this day. It is understandable, however, on the grounds that in reaching the exact value one comes up against many unanswered questions about the size and scale of the universe and how we've come to define the number of emitting sources of light within it to be *finite* as opposed to being *infinite*... After all, there are more stars in the observable universe than all the grains of sand on all the shores of every single ocean across the world added together...
What is "Ahad's constant"?
If we exclude all light coming directly and indirectly from the nearby Sun, the rest of the universe collectively supplies us with a mere 1/300th of a Full Moon's worth of illumination. That's "Ahad's constant"
A key thing to stress here is this all about "ILLUMINATION" provided by visible starlight, in the same sense as "sunshine" and "moonlight". The two questions: "How bright is the night sky?" and "How much light illumination does the night sky provide?" are not the same things! The latter is what this whole concept is about. 

Astronomers measure the brightnesses of stars across the night sky using something called the magnitude scale, first introduced by the Greek astronomer Hipparchus in the second century B.C. The scale in itself can be somewhat confusing, since a first magnitude star is actually brighter than a second magnitude star...opposite to what you'd expect going purely by every day common sense. You can learn more by searching Google for  'magnitude scale for star brightnesses' Here's one site that goes into much elaborate detail.
Back to the definition of "Ahad's constant".
Suppose we have two stars of apparent magnitudes m1 and m2. Then their luminosities L1 and L2 are related by the formula:-

L2/L1 = 10^[0.4*(m1-m2)]

The luminosity of the pair of stars is L1 + L2 = L1(1 + L2/L1), and their combined magnitude is then given by:-

Mc = m1 - 2.5*log10 (1 + L2/L1)

For the general case, where the magnitudes of "n" stars need to be aggregated, we can generalise this by computing all the ratios:-

Li/L1 = 10^[0.4*(m1-mi)]   ...............................................equation (1)

for all stars i from 2 through n. The combined magnitude is then:-

Mc = m1 - 2.5*log10 (1 + L2/L1 + L3/L1 + ... + Ln/L1)   ..........equation (2)

"Ahad's constant" is simply defined to be the sum of all the individual magnitudes of every single star across the entire night sky, right down to the faintest star that could ever be seen with the most powerful telescope ever invented or is likely to be invented in the future.
In other words, the value of "n" in the above formulae (i.e. the star count) will tend to infinity. Based on my own numerical integrations, I have found that as n tends to infinity, the variable Mc in the above equation tends to a net figure of -6.5 magnitudes (1/300th of a full moon equivalent worth of light). That is what some are calling "Ahad's constant".





It can be appreciated by someone sailing more than a couple of light years beyond the neighborhood of the Sun in any direction. When you're that far out, you'd want certain physical barometers to pinpoint your overall "existence". One of them might be knowing whether the environment your ship is sailing through is a complete vacuum. Another might be knowing your distance from the next nearest planet or star. Yet another might be to know how much net starlight illumination the sky is providing (i.e. "Ahad's constant").
It will not be a true celestial constant, but vary slightly, to a traveller located in deep interstellar space within several hundreds - if not thousands - of light years from here. All that humanity can ever hope to physically experience or meaningfully contemplate over within the foreseeable future of our species...
Stars in the neighborhood of the Sun are extremely feeble in their intrinsic brilliance - most of them being tiny red dwarves of  < 0.1 x Sun power - and the average spacing between them is approximately 5 light years. Hence, 99.9% of the time during an interstellar voyage between any two stars in this part of the galaxy, you will be travelling under the feeble illumination quantified by "Ahad's constant":



Above: Stars in the neighborhood of our Solar System, going 20-light years out in all directions. If you place your finger randomly anywhere on this map, 99.9% of the time when you're physically there, you are going to be surrounded by a perpetual cosmic night. The net illumination from all the pinpricks of starry light in the 360-degree celestial sphere around you will then equate to "Ahad's constant". FACT, not fiction!
To make my work somewhat "official", preliminary results of the above integrations were published in Journal of the British Astronomical Association, Volume 115, No. 5, October 2005 edition, page 297.
Ahad's constant has significance to Einstein's Special Theory of Relativity and relativistic interstellar travel. See this page for more details.

(Note: "Ahad's constant" is not to be confused with something called "Olbers Paradox")
Please leave your comments on this blog below. Thanks!!!
Abdul Ahad

Abe
Abe F. March

 

Abdul,

what you have written is most impressive.  I must admit that I don't comprehend all of it, especially the calculaltions.  I want to re-read it however. 

You are to be congratulated on what you have already accomplished.  I forsee you becoming a prominent name in the space science field.


 
Posted by Abe on Friday, January 12, 2007 - 8:09 AM
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Abdul Ahad - Bestselling Author
Abdul Ahad

 

Here’s how you can visualise this "constant" from your own backyard without going into outer space 

Let’s say it’s midday now, right at this minute, and you’re standing out in the garden at the back of your house admiring all the beautiful plants around you.

Now if someone were to switch off the Sun right at this minute, as if it were just an ordinary light bulb, the sky up above would go dark, right? And the stars would come out, as if nightfall had suddenly descended across the land? Sure thing! It’s how things are for us after sunset each and every single evening.

Now imagine the earth beneath your feet gradually crumbled away and disappeared into nothingness. If you now look down beneath your feet, way down into the distance, you’ll see stars much as you would when you looked up. You would have stars all around you, way up above your head, across over to your right, over to your left and going way into the distance beneath your feet... You’d be surrounded by a 360-degree sphere of starry pinpricks of light from all across the universe. In this imaginary scenario, you have entered a perpetual interstellar night that one would encounter on every single journey going outward from our Solar System in any direction... in a rocket ship sailing toward the immensely distant stars.

If now you held out the palm of your hand in front of you, could you see it solely by the naked light from all those tiny pinpricks of stars? To answer this question, you have to evaluate "Ahad’s constant"!


 
Posted by Abdul Ahad - Bestselling Author on Friday, January 12, 2007 - 9:40 AM
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Anubis

 
In my opinion, you have hit the nail on the head.  I don't think there should be any debate!
 
Posted by Anubis on Friday, January 12, 2007 - 8:11 AM
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Ex Cigarette Addict

 
My friend Abdul, Does NASA know about you? If not, they should!
 
Posted by Ex Cigarette Addict on Friday, January 12, 2007 - 8:19 AM
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I agree with your friend call NASA. This is very interesting, they would want to hear about this. 
 
Posted by on Monday, January 15, 2007 - 8:43 PM
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Just2Write

 

Now if someone were to switch off the Sun right at this minute, as if it were just an ordinary light bulb, the sky up above would go dark, right? And the stars would come out, as if nightfall had suddenly descended across the land? Sure thing! It’s how things are for us after sunset each and every single evening.

If  I were to occupy a particular place in space where the sun were switched off like a light bulb, the immediate reflective objects would not display themselves because they are not being illuminated by the Sun any longer, thus creating a whole different view than if we left the sun "on". The position of the planets are contantly changing and thus creating a slightly different lighting as well. Also you are assuming that the person occupying the space without sun is not carrying a pocket flashlight which throws the whole thing off once used.  Hmmm...... The constant we know for sure is that there is no constant. Hmmmm..........I like you, you make my brain work. This is fun. What else you got?!

J.

 

 


 
Posted by Just2Write on Thursday, January 18, 2007 - 4:41 PM
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Abdul Ahad - Bestselling Author
Abdul Ahad

 

This is a fun brain teaser!!!

Here are the twenty closest stars to the Sun, as they are positioned in 3D space relative to one another:-

Consider the brighter and more luminous ones amongst them on this chart: Sol (which is our Sun), Procyon, Sirius and Alpha Centauri.

Now, ask an astronomer: what is the net amount of natural light the sky is going to produce when I'm sailing about mid-way between: (a) Sol and Alpha Centauri, (b) Sirius and Procyon, (c) Alpha Centauri and Sirius, (d) Alpha Centauri and Procyon, etc...?

Whatever answer he/she will give you will be exactly the same for each of those four interstellar journeys (a), (b), (c) and (d),... That is indeed a "constant". Does the confusion stop here - lol...?

 


 
Posted by Abdul Ahad - Bestselling Author on Thursday, January 18, 2007 - 9:37 PM
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Pierre Girard
Pierre Girard

 

Isn't there a constant already in use by astronomers which is for a patch a sky devoid of visible stars and galaxies  and expressed in magnitudes per unit of square area?  In photometry, it is essential to know your sky background brightness before assessing small scale variations in variable objects.  This might only apply though for objects seen through our atmosphere from observatory Earth.  I have no idea whether observations carried out in space are treated similarly.

Time to do some research.

Pierre


 
Posted by Pierre Girard on Saturday, January 20, 2007 - 5:47 PM
[Reply to this
Monique
Monique Osier

 
WOW Abdul, this is so over my head I needed consultation with God.

My guy, however, is a physics geek and I can't wait to show him this!

I have to say, that even though I can't understand your calculations, you present this in such a way that even a layman such as myself, can jibe meaning from the hypothesis and with the links; comprehend your content.

You are shining star, Abdul...a great and creative mind! I am glad you made this available on my page...thank you for including me.

Monique

 
Posted by Monique on Tuesday, January 23, 2007 - 10:14 PM
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Boris

 

Most impressive. The calculations went a bit over my head but I can see were you are going =). ..:namespace prefix = o ns = "urn:schemas-microsoft-com:office:office" />


 
Posted by Boris on Saturday, January 27, 2007 - 8:58 AM
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Abdul Ahad - Bestselling Author
Abdul Ahad

 

Okay, here is a worked example

Consider these three bright stars, which twinkle prominently in our evening skies during early summer each year:-

Vega, Altair and Deneb

Their apparent visual magnitudes are:-

Vega = 0.03, Altair = 0.77, Deneb = 1.25

The combined brightnesses of these three stars could be worked out as follows.

Let m1=0.03, m2=0.77, m3=1.25

Now, by equation (1) above, Li/L1 = 10^[0.4*(M1-Mi)], we have:-

L2/L1 = 10^[0.4*(m1-m2)] = 10^[0.4*(0.03-0.77)] = 0.5058 (to 4 decimal places)

Similarly, L3/L1 = 10^[0.4*(m1-m3)] = 10^[0.4*(0.03-1.25)] = 0.3251

Finally, by equation (2) above, Mc = m1 - 2.5*Log10(1+L2/L1+L3/L1) = 0.03 - 2.5*Log10(1+0.5058+0.3251) = -0.63

Hence, the combined magnitude of all three stars comes to a net value of -0.63.

Now suppose we placed ourselves a couple of light years beyond the neighborhood of our Solar System, into deep interstellar space. From that vantage point, if we continued adding the magnitudes of every single star visible across the entire cosmic sky in this manner, the total luminosity would eventually tend "asymptotically" towards a final figure of circa -6.5 magnitudes.

Comparing this brightness with that of the Full Moon (which shines at approximately magnitude -12.7 in the night skies of planet Earth), the magnitude difference is (-6.5) - (-12.7) = 6.2. This equates to a brightness ratio of 10^(0.4*6.2) = 302. Hence, the total luminosity of the interstellar night sky amounts to circa 1/300th of a Full Moon’s worth ("Ahad’s constant") .


 
Posted by Abdul Ahad - Bestselling Author on Tuesday, January 30, 2007 - 8:28 AM
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Boris

 

That actually makes sense. I’m starting to understand the idea of Ahad’s constant. ..:namespace prefix = o ns = "urn:schemas-microsoft-com:office:office" />

 

I’m doing another night shift so I got lots of time to study these things


 
Posted by Boris on Thursday, February 01, 2007 - 9:22 PM
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Abdul Ahad - Bestselling Author
Abdul Ahad

 

The apparent magnitude of the Sun as seen from Earth is -26.7. As we head outward from our Solar System, the Sun’s apparent brightness will fall off according to the inverse square law. The absolute magnitude of a star is its apparent magnitude when viewed from a standard distance of 10 parsecs (32.616 light years). We know from direct measurements, the Sun has an absolute magnitude of +4.76.

The formula for working out the apparent visual magnitude 'm' of a star whose absolute magnitude is 'M', as seen from a distance of 'd' light years is given by:-

m = M - [5 - 5 * log10(d / 3.2616)] ............. Equation (3)

Using the above equation, it is possible to chart the fall off in apparent magnitude of the Sun with increasing distance, a bit like this:-

The average distance of the Earth from the Sun is 149.6 million kilometers. This yardstick distance is referred to by astronomers as an ‘astronomical unit’ (AU). Light from the Sun takes 8 minutes and 18 seconds to cross 149.6 million km of space to reach us here on Earth. In other words, that’s how long it takes to cross 1 AU. Hence, by simple arithmetic, there are 63,240 AUs in 1 light year. At a distance of some 11,500 AUs (0.182 light-year) from the Sun, its apparent magnitude would be (by equation 3 above):

m = +4.76 - [5 - 5*log10(0.182/3.2616)] = -6.5

Therefore, that is the distance where the Sun’s light output exactly matches that of the surrounding cosmic night sky’s total integrated magnitude of -6.5 ("Ahad’s constant").

It is thus possible to draw an imaginary sphere around the Sun, within which the Sun would remain the most supreme source of light, relative to the universe’s total background illumination:

Beyond the outer fringes of this theoretical sphere, our Sun would become overpowered by the collective light from the rest of the universe... Where the Sun would no longer be the most supreme source of light and heat to an interstellar traveller. It marks the edge of the Sun’s effective light dominion.


 
Posted by Abdul Ahad - Bestselling Author on Thursday, February 08, 2007 - 11:17 PM
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Emdad

 

Please leave your valuable comments after reading.

http://www.openmindsblogspot.com/HOME/tabid/36/Default.aspx 


 
Posted by Emdad on Wednesday, February 07, 2007 - 9:09 AM
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Abdul Ahad - Bestselling Author
Abdul Ahad

 

Flux equations for Ahad's constant derivation, their result and the light dominion sphere whose radius is the famous "Ahad radius"  were published in the Mathaba News Network here. Comments from a wide cross-section of the world public were collated and posted here.


 
Posted by Abdul Ahad - Bestselling Author on Sunday, February 18, 2007 - 11:39 AM
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