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Discovery's debut
In our continuing look back at the classic days of the space shuttle program, today we show the STS-41D post-flight presentation by the mission's astronauts. The crew narrates this film of home movies and mission highlights from space shuttle Discovery's maiden voyage in August 1984. STS-41D deployed a remarkable three communications satellites -- a new record high -- from Discovery's payload bay, extended and tested a 100-foot solar array wing and even knocked free an icicle from the shuttle's side using the robot arm.

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"Ride of Your Life"
As the title aptly describes, this movie straps you aboard the flight deck for the thunderous liftoff, the re-entry and safe landing of a space shuttle mission. The movie features the rarely heard intercom communications between the crewmembers, including pilot Jim Halsell assisting commander Bob Cabana during the landing.

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Message from Apollo 8
On Christmas Eve in 1968, a live television broadcast from Apollo 8 offered this message of hope to the people of Earth. The famous transmission occurred as the astronauts orbited the Moon.

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ISS receives supply ship
The International Space Station receives its 20th Russian Progress cargo ship, bringing the outpost's two-man Expedition 12 crew a delivery of fresh food, clothes, equipment and special holiday gifts just in time for Christmas.

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Rendezvous with ISS
This movie features highlights of the December 23 rendezvous between the Russian Progress 20P vessel and the International Space Station. The footage comes from a camera mounted on the supply ship's nose.

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Stardust return preview
NASA's Stardust spacecraft encountered Comet Wild 2 two years ago, gathering samples of cometary dust for return to Earth. In this Dec. 21 news conference, mission officials and scientists detail the probe's homecoming and planned landing in Utah scheduled for January 15, 2006.

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Science of New Horizons
The first robotic space mission to visit the distant planet Pluto and frozen objects in the Kuiper Belt is explained by the project's managers and scientists in this NASA news conference from the agency's Washington headquarters on Dec. 19.

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Hubble Space Telescope
Scientists marvel at the achievements made by the orbiting Hubble Space Telescope in this produced movie looking at the crown jewel observatory that has served as our window on the universe.

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U.S. Naval Observatory to add leap second to clocks
Posted: December 30, 2005

On December 31, 2005 a "leap second" will be added to the world's clocks at 23 hours, 59 minutes and 59 seconds Coordinated Universal Time (UTC). This corresponds to 6:59:59 pm Eastern Standard Time, when the extra second will be inserted at the U.S. Naval Observatory. This marks the 23rd leap second to be added to UTC, a uniform time-scale kept by atomic clocks around the world. Although you normally don't think about it, for most conventional uses the "civil" time you use is based on UTC. At the U.S. Naval Observatory, UTC is determined by averaging the time signals from cesium beam atomic clocks and hydrogen masers (the last being an improvement over the tried and true cesium clocks for measuring short periods of time).

Man's oldest clock has always been the Earth. We know it's morning when the Sun rises, noon when the Sun is overhead, and evening when the Sun sets. The Earth's accuracy as a clock is good to about one thousandth of a second per day - more than enough accuracy for most people. However, the invention of "atomic" clocks, which operate by measuring the resonant frequency of a given atom - (currently Cesium, Hydrogen or Mercury) - greatly increased that accuracy, and has now led to the capability at the U.S. Naval Observatory of measuring time to accuracies exceeding a billionth of a second per day.

Time measured by the rotation of the Earth is not uniform when compared to the time kept by atomic clocks. In fact, radio telescopes now observe the most distant objects in the universe, known as quasars, to determine the irregularities in the Earth's rotation, an important function performed by the Naval Observatory in our Very Long Baseline Interferometry (VLBI) program. As a result of these irregularities, atomic clocks gradually get out of sync with the Earth.

In 1972, by international agreement, it was decided to let atomic clocks run independently of the Earth, keep two separate time-scales, and then coordinate the two. In order to keep the difference between Earth time and atomic time within nine-tenths of a second as the two time-scales get out of sync, leap seconds are factored into the atomic time-scale. The International Earth Rotation and Reference System Service (for which the U.S. Naval Observatory provides the Rapid Service and Prediction Product Center) is the organization which monitors the differences in the two time scales and calls for leap seconds to be inserted when necessary. Since 1972 leap seconds have been added at intervals varying from six months to two years. This leap second is occuring seven years since the last one. Leap seconds are added because the Earth's rotation tends to slow down relative to atomic time. If the Earth were to speed up, a leap second could be removed.

The U.S. Naval Observatory is charged with the responsibility for precise determination and management of time dissemination, and as such provides the Master Clock for the Department of Defense. USNO, together with the National Institutes for Standards and Technology (NIST), determines time for the entire nation. Modern electronic systems, such as electronic navigation or communication systems, depend increasingly on precise time and time interval (PTTI). Examples are the ground-based LORAN-C navigation system and the satellite-based Global Positioning System (GPS).

These systems are all based on the travel time of electromagnetic signals: an accuracy of 10 nanoseconds (ten billionths of a second) corresponds to a positional accuracy of about three meters or 10 feet. In fast communications, time synchronization is equally important. All of these systems are referenced to the U.S. Naval Observatory Master Clock.

The present Master Clock is required by the Department of Defense to be accurate to better than a billionth of a second per day. It is based on an ensemble of 60 independently operating cesium-beam atomic clocks and 15 hydrogen maser atomic clocks. These clocks operate in environmentally controlled vaults to ensure their stability. By automatic inter-comparison of all of the clocks every 100 seconds, a time-scale can be computed which is not only reliable but also extremely stable. Its rate does not change by more than about 100 picoseconds (0.000 000 000 1 seconds) per day from day to day. On the basis of this computed time-scale, a clock reference system is steered to produce clock signals which serve as the U.S. Naval Observatory Master Clock.

The U.S. Naval Observatory's success in its time standard function is evident in the fact that it is the largest single contributor to the international time scale (UTC), which is computed in Paris, France, at the International Bureau of Weights and Measures. Moreover, its principal role in keeping track of the change in the "Earth clock" (i.e., Earth rotation) and its dissemination of this information as the Rapid Service Bureau and Predictions Product Center for the International Earth Rotation and Reference System Service attests to the fact that globally, as well as nationally, the U.S. Naval Observatory remains the leader in precise time.