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United States Naval Observatory
The Naval Observatory Flagstaff Station
The Ron Stone 0.2-meter telescope
Home
Our Commands
United States Naval Observatory
The Naval Observatory Flagstaff Station
The Ron Stone 0.2-meter telescope
ABOUT US
Mission & Vision
History
Naval Oceanography One Pager
End of Year Graphic 2022
LEADERSHIP
Commander
Technical Director
Command Master Chief
All Leadership
OUR COMMANDS
Naval Oceanographic Office
Fleet Numerical Meteorology & Oceanography Center
United States Naval Observatory
News from the Naval Observatory
Earth Orientation Department
Precise Time Department
The USNO Master Clock
The USNO Master Clock
Time Dissemination at the USNO
USNO Alternate Master Clock (AMC)
Cesium Atomic Clocks
Hydrogen Masers at the USNO
Rubidium Fountain Clocks
USNO Time Scales
International Time Scales and the BIPM
Definitions of Systems of Time
Global Positioning System
Global Positioning System Overview
USNO GPS Data Categories Explanation
CGGTTS Data Format
USNO GPS Time Transfer
Leap Seconds
GPS Information: SA, DGPS, Leap Seconds, etc.
GPS Week Number Rollover
GPS Timing Data and Information
USNO Format Explanation
USNO Computer Display Clocks
Two-Way Satellite Time Transfer (TWSTT)
Telephone Time
Network Time Protocol (NTP)
US Eastern Time Zone NTP Servers
US Mountain Time Zone Servers
DoD Customer Servers
Astronomical Applications Department
Celestial Reference Frame Department
Senior Enlisted Advisor
Careers at the USNO
Naval Oceanography Operations Command
Fleet Weather Center - Norfolk
National Ice Center
Fleet Weather Center - San Diego
Joint Typhoon Warning Center
Naval Oceanography Anti-Submarine Warfare Center
Navy DoD Supercomputing Resource Center
PRESS ROOM
News Stories
Photo Gallery
Video Gallery
Public Use of Limitations
CONTACT US
The Ron Stone
A
strometric
S
canning
T
ransit
T
elescope is a completely automated transit telescope utilizing scan-mode CCD cameras to measure the positions of hundreds of thousands of stars to fainter than 17th magnitude. It has been used in studies of the relationship between optical and radio reference frames, since it can detect and accurately measure positions of both the bright stars used to define the optical reference frame and faint quasars and radio galaxies that define the radio frame.
Telescope Data
Construction
Optics: Farrand Optical Company
Mounting: Farrand Optical Company
Date Completed: 1981
Optical Design: Achromat
Overall Focal Ratio: f/10.4
Focal Plane Scale: 99 arcsec/mm
Objective Lens
Diameter: 20-cm (8-inches)
Material: Crown & Flint Glass
Focal Ratio: f/10.4
Total Weight (Optics, Tube and Mount): 1,910 kg (2.1 tons)
Current Research Programs
Sloan Digital Sky Survey
astrometric calibration
Near Earth Object astrometry - in collaboration with
Lowell Observatory
Astrometry to support NASA spacecraft missions - in collaboration with
Jet Propulsion Laboratory
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