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			 November 2005
 
			from
			
			Etheric Website
 
				
					
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						Please note that the 
						following discussion builds on concepts set forth in
						
						The Talk of the Galaxy 
						and therefore is best understood if you have already 
						read the book. Alternatively, see the essay "The 
						Forgotten Challenge: Pulsars" for an overview 
						of some of the book's ideas. |  
			  
			
			
 Further Evidence for an ETI Origin
 
				
				
				The map charting the sky locations of pulsars (figures 9 and 13 
			in the first edition of The Talk of the Galaxy) has now been revised 
			and no longer shows a clump or pulsars positioned adjacent to the 
			Galactic one-radian point. When The Talk of the Galaxy was first 
			published in 2000, a total of 1100 pulsars had been cataloged. 
				   
				As of 
			the end of 2007, this number has risen to 1775. Most of the new 
			pulsar additions have southern hemisphere locations, having been 
			located in the Parkes Multibeam Pulsar Survey. With the new data 
			set, a galactic longitude histogram that shows the distribution of 
			pulsars along the galactic equator no longer shows a decline in 
			pulsar population extending from the one-radian longitude (l ~ 
			57.3°) toward the Galactic center.    
				This is because most of the newly 
			discovered pulsars lie in the central part of the Galaxy and hence 
			the profile showing their distribution as a function of galactic 
			longitude now absorbs this former clump. However, the sharp cut off 
			in pulsar population just beyond the one-radian longitude is still 
			present and, as before, is not easily explained as being due to any 
			natural cause or selection effect.
				
				In September 2005 Dr. LaViolette made several new discoveries 
			which along with other findings described in The Talk of the Galaxy 
			strongly support the interpretation that pulsar beacons have an 
			extraterrestrial intelligence origin.    
					
					
					The two fastest pulsars in the sky, the 
					Millisecond Pulsar and 
			the Eclipsing Binary Millisecond (EBM) Pulsar, not only are among 
			the closest pulsars to the one-radian longitude (as pointed out in 
			2000), but their longitude positions accurately portray the 1-to-2p 
			relation. That is, if one takes the angular deviation of the 
			Millisecond Pulsar longitude from the Galactic one-radian longitude 
			and divides by the deviation in longitude between the Millisecond 
			Pulsar and the EBM Pulsar, the ratio so obtained is within 0.1% of 
			being exactly equal to 1/2p. In other words, through their sky 
			positions, these two pulsars express the one-radian concept -- 
			portraying the fraction of a circle's circumference that is 
			represented by a one-radian arc.
					
					If one takes the longitudinal deviation of the Millisecond Pulsar 
			from the Galactic one-radian longitude, bisects this arc and adds 
			the result to the angular deviation between the longitudes of these 
			two millisecond pulsars, then divides the sum by 57.2958° to express 
			the angle in radians, one obtains 3.1809%. This is within 0.09% of 
			equaling 3.1837%, the fractional amount that the period of the EBM 
			Pulsar deviates from the period of the Millisecond Pulsar. (It is 
			logical to use the Millisecond Pulsar period as the base reference 
			since it is not only the second fastest pulsar in the sky but also 
			the closest to the Galaxy's equatorial one-radian longitude point.
					
					The ratios described in both a) and b) would have been exact if 
			the pulsar positions were observed between 1750 and 1800 AD. The 
			ratios are less exact today since the longitude sky position of the EBM Pulsar is gradually changing due to the pulsar's proper motion 
			toward the Galactic center.
					
					Since 2000, a new eclipsing binary pulsar has been discovered 
			(J1953+1846A), which lies in the vicinity of the one-radian 
			longitude. It has almost the same angular separation from the Gamma Sagittae pointer star as the EBM Pulsar. Its close sky position 
			proximity to both the EBM pulsar and to Gamma Sagittae is quite 
			surprising since only 14 eclipsing binary pulsars are known to 
			exist, less than one percent of the pulsar population. 
			Interestingly, if one takes the period of this pulsar (4.8883 
			milliseconds) and divides by that of the Millisecond Pulsar 
			(1.5578), one obtains 3.1380, which is within 0.1% of being exactly 
			equal to p. 
			All of the above is best understood within the context of the 
			arguments and perspective carefully set forth in The Talk of the 
			Galaxy. Needless to say, the apparent sky positions of these pulsars 
			which exhibit these pi ratios can be seen as such only from our 
			particular viewing perspective.  
			  
			We are led to conclude that this 
			one-radian message is intentionally targeted toward our solar 
			system.
 
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