Sunday, August 06, 2006

Space the Final Frontier, Spaceman

Apollo 11, Credit: NASA Johnson Space Center (NASA-JSC)
Date: 07.11.1969m Title: Artists concept of Apollo 11 Astronaut Neil Armstrong on the moon. Description: A Grumman Aircraft Engineering Corporation artist's concept depicting mankind's first walk on another celestianl body. Here, Astronaut Neil Armstrong, Apollo 11 commander, is making his first step onto the surface of the moon. BestAudioCodes.com
In the background is the Earth, some 240,000 miles away. Armstrong. They are continuing their postflight debriefings. The three astronauts will be released from quarantine on August 11, 1969. Donald K. Slayton (right), MSC Director of Flight Crew Operations; and Lloyd Reeder, training coordinator. ID: S69-38662. Credit: NASA Johnson Space Center (NASA-JSC)

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Saturday, August 05, 2006

Space the Final Frontier, CTA-102

U.S. Naval Observatory Radio Reference Frame Image Database Movies
Image Information: All information presented on these pages (THIS IMAGE) is considered public domain and may be distributed or copied unless otherwise specified. Use of appropriate byline, photo, image credits is requested. "U.S. Naval Observatory Radio Reference Frame Image Database Movies" the U.S. Naval Observatory (USNO). is responsible for the determination
of the positions and motions of stars and solar system objects and the establishment of celestial reference frames. BestAudioCodes.com

Quasar, source of radio waves, first observed in the early 1960s by CALTEC, and proposed, in 1963, by N. S. Kardashev in the Astronomical Journal of the USSR as evidence of a Type Two or Three Kardashev civilization. A worldwide sensation followed CTA-102

The quasar CTA 102 (QSO 2230+114) was observed four times in 1991-1992 by the EGRET high-energy gamma ray telescope on the Compton Gamma Ray Observatory satellite. In the 1992 January 23 -- February 6 observation, emission was detected at the level (2:4 \Sigma 0:5) \Theta 10 \Gamma7 photons cm \Gamma2 s \Gamma1 (E ? 100 MeV). Observation of High-Energy Gamma Rays from the QSO CTA 102

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