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2016-02-27 09:21:42

This is your ●●●●●●ment ●●●●●●ct order ●●●●●●idone ●●●●●● pdf What you hear in Tuvan ●●●●●● ●●●●●●g is a deft ●●●●●●●●●●●● of the ●●●●●●x ●●●●●●ties of sound waves. When ●●●●●● ●●●●●●es a sound, the ●●●●●●ion of the vocal cords ●●●●●●s a sound wave that is ●●●●●●ved as pitch. Slower ●●●●●●ion=●●●●●● sound wave=lower pitch. Faster ●●●●●●ion=●●●●●● sound wave=●●●●●● pitch. But in ●●●●●●on to the main sound wave — what we ●●●●●●ve as the note — there are ●●●●●●ics, ●●●●●●r sound waves ●●●●●●ed at 2, 3, 4, 5 times the speed of the main one. Since they are ●●●●●●y ●●●●●●d with the main wave, we don't hear them as ●●●●●●ent notes, but they do add to our ●●●●●●tion of the ●●●●●●l ●●●●●●y of a voice. ●●●●●●x ●●●●●●●●●●●● aetna A●●●●●●mers have known for about a ●●●●●● ●●●●●●iolet and X-ray ●●●●●●ion from the main star in HD 189733 are ●●●●●●ating the ●●●●●●here of HD 189733b over time. The ●●●●●●s ●●●●●●te it is ●●●●●● 100 ●●●●●●n to 600 ●●●●●●n ●●●●●●ams of mass per ●●●●●●. HD 189733b’s ●●●●●●here ●●●●●●s to be ●●●●●●ng 25 ●●●●●●t to 65 ●●●●●●t ●●●●●● than it would be if the ●●●●●●’s ●●●●●●here were ●●●●●●r.