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Author Topic: NASA Attacks the Moon  (Read 802 times)
Rhonda
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« Reply #15 on: October 09, 2009, 08:19:46 AM »

Great post 2aggies, I just saw you put it on Danny's as well...Smiley
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walleye
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« Reply #16 on: October 09, 2009, 09:06:19 AM »

See that NASA wasn't able to see the crash as planned for some odd reason, and they were expecting to see a 6 mile plume of dust.  And the Liberals want the government to run our health care.......give me a break!!!
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deadserious
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« Reply #17 on: October 09, 2009, 09:43:36 AM »

I think this whole bomb the moon thing is just a payoff to the corporate fat-cats at Cheese-Its
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Now back to your regularly scheduled drivel...
Otteralum
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« Reply #18 on: October 09, 2009, 11:36:17 AM »

lol! how much greenhouse gas did the rocket + moondust put into earth's atmosphere??  We may not find water, but I guarantee you they found CO2 -- it's everywhere!!!
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"Life is Relationships"
Otteralum
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« Reply #19 on: October 09, 2009, 11:42:00 AM »

oooo. Rush just told me that the "water" mission is really a ruse and that Obama is preparing the site for a new FEMA camp.  I knew it!
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"Life is Relationships"
walleye
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« Reply #20 on: October 09, 2009, 11:49:30 AM »

lol! how much greenhouse gas did the rocket + moondust put into earth's atmosphere??  We may not find water, but I guarantee you they found CO2 -- it's everywhere!!!

Otter, I agree.  I couldn't find the exact numbers on today's mission, but maybe you could break this down for me, my "Geek" friend...

Results of radiometer measurements of infrared Hydroxyl (OH) emissions from five rocket flights are presented. Two of the rocket payloads were flown from Poker Flat Rocket Range, Alaska and three were flown from White Sands Missile Range, Nex Mexico. Four of the flights were flown during night-time conditions and one (at WSMR) was flown during twilight (CHI _ 99 deg). Each rocket payload was instrumented with liquid nitrogen cooled dual-channel radiometers to measure infrared OH emissions from the vibration-rotation bands 2-0 through 5-3 (1.56 micrometer channel) and the 7-5 through 9-7 (1.99 micrometer channel). The rocket data shows that the principle OH emissions in the bands cited occurs in a thin layer 8 to 10 km thick with peak emission near an altitude of 89 km. The ratio of night-time 1.56 micrometer to 1.99 micrometer radiance is constant, at a value of 1.4, up to an altitude of 80 km regardless of latitude. At twilight, this ratio is larger at low altitudes (60 km) and diminishes with increasing altitude. Estimated night-time peak volume emission rates at WSMR are 1 megaphotons per cm per sec per micrometer in the 1.56 micrometer band and 0.7 megaphotons per cu cm per sec per micrometer in the 1.99 micrometer band.
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