UMD ASTR 120 - Class 9 Celestial coordinates and navigation

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1Class 9Celestial coordinates and navigation Celestial coordinates Basic principles of navigation The longitude problem2I : Celestial coordinates Astronomers need to be able to describe theposition of an object in the sky… need acoordinate system for the sky Most common choice is the RA/Dec system…the celestial version of latitude and longitude Declination : Angle from the celestial equator tothe object (measured in degrees). Right Ascension (RA) : Consider a line runningfrom the north to south celestial poles through thevernal equinox. The RA is the angular distance fromthis line to the object (typically measured in terms ofhours).3 Examples… Jupiter (today) RA : 18h 58m 2s Dec : -23o 5.8’ Center of Andromeda galaxy RA : 00h 42m 44s Dec : +41o 16’ 09”4 Why do all objects change their RA and Dec over time?5Another common choice… “Galactic Latitude and Longitude”II : Basics of navigation Astronomy and navigation have close ties… Imagine you are on a ship in the middle of theocean (without GPS!)… how do you figure outwhere you are? A good topic for discussion…67GoogleThe Longitude Problem 1675 : Royal Observatory at Greenwichestablished by Charles II in order to solve theproblem of finding longitude at sea 1714 : British Government established the“Longitude Prize”… 20,000 pounds! (~ 7 million dollars today) Winner must devise method for finding longitude towithin half a degree during a journey from Britain toNew World Board of prominent scientists established to overseaprize8John


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