Appendix A: Longitudes and Latitudes of Cities Around the World
Appendix A: Longitudes and Latitudes of Cities Around the World City Longitude Latitude Anchorage 149540W61130N Athens 23430E37580N Auckland, NZ 174440E36500S Beijing 116240E39550N Berlin 13230E52310N Buenos Aires 58230W34360S Cairo 31140E30030N Colombo 79510E6560N Dakar 17270W14420N Hong Kong 114100E22170N Honolulu 157500W21190N Istanbul 28570E41010N Jerusalem 35130E31470N Johannesburg 28030E26120S Lima 77020W12030S London 0080W51300N Los Angeles 118150W34030N Mexico City 99080W19260N Moscow 37370E55450N New Delhi 77130E28370N New York 73560W40400N Paris 2210E48510N Rio de Janeiro 43120W22550S Santiago, Chile 70400W33270S Singapore 103500E1170N Sydney 151130E33520S Tehran 51250E35420N Tokyo 139420E35410N © Springer International Publishing AG 2017 217 S. Kwok, Our Place in the Universe, DOI 10.1007/978-3-319-54172-3 Appendix B: Astronomical Measurements Ancient astronomers typically made two types of measurements: position and brightness. Position refers to the angular position of a celestial object on the celestial sphere. Since our view of the sky is two-dimensional, we use the unit of angles to assign the positions of stars. The Babylonian concept of a degree is based on the fact that 1 year has 365 days. Since 365 is close to the nice number 360 which can be divided by 2, 3, 4, 5, 6, 8, 9, 10, 12, 15, etc., astronomers adopted 360 degrees as a full circle and this Babylonian unit is still in use today. Again, since 60 is a good number, we divide a degree into 60 arc minutes, and an arc minute into 60 arc seconds. To get an idea of how large these units are, a one-centimeter coin placed at a distance of 1 km will have an angular size of 2 arc seconds, so one arc second is a very small separation indeed.
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