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NOTICE TO OUR USERS

Under direction from the Chief of Naval Operations, the U.S. Naval Observatory's web site is changing from its traditional appearance to a web "portal" which will combine all of the Navy Oceanography Community's products and services.

As of 15 January 2009, the U.S. Naval Observatory's publicly-accessible products and services will continue to be available at http://www.usno.navy.mil, but will be part of a larger portal.

DoD customers are directed to our NIPRNet site at https://oceanography.navy.mil (CAC required).

Questions or comments regarding the new "portal" architecture may be submitted here.

Please direct any non-portal related general questions or comments to our Webmaster.

The U.S. Naval Observatory is one of the oldest scientific agencies in the country. Established in 1830 as the Depot of Charts and Instruments, its primary mission was to care for the U.S. Navy's chronometers, charts, and other navigational equipment. Today, USNO is the preeminent authority in the areas of Precise Time and Astrometry, and distributes Earth Orientation parameters and other Astronomical Data required for accurate navigation and fundamental astronomy. USNO headquarters in Washington, DC is the administrative and scientific hub of Observatory operations and is home to the James M. Gilliss Library, one of the most complete collections of astronomical literature in the world. USNO operates a remote observing station at Flagstaff, AZ and an Alternate Master Clock Facility at Schriever AFB, CO.

The Moon, Venus, & Jupiter gather over USNO, 2008 December 1

The USNO CCD Astrograph Catalog is an astrometric observational program which started in February 1998 at CTIO. All sky observations were completed in May 2004. The final catalog is expected to be released by early 2009. The second data release (UCAC2) became public in 2003. Positions accurate to 20 mas for stars in the 10 to 14 magnitude range are obtained. At the limiting magnitude of R=16 the catalog positions have a standard error of 70 mas. Proper motions are provided using various earlier epoch data. Photometry is poor, with errors on the order 0.1 to 0.3 magnitudes in a single, non-standard color.

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