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Florence University of Art - Planetarium Key Points for the lessons on 26th november 2008 Piero Ranfagni [email protected] 1. Celestial sphere The stars seem numberless and there are actually more than 2 billions of stars in the system we live in (Milky Way), but only 3000 stars are visible at naked eye What we see is NOT what it is actually, the response of our eye is logarithmic not linear All celestial objects seem at the same distance from us, hence we think to be at the center of an huge sphere Constellations exist because of celestial sphere and because pattern recognition is a natural feature for living beeings Constellation shape changes with epoch and their visibility changes with epoch and observer position; shape is not for ever because of star’s proper motion, but no detectable change is observable during human life, at naked eye Constellations and asterisms; we use structures invented by assirian priests in XII century BC: Orion, Ursa Major, Ursa Minor, Scorpion, Gemini, Taurus, the Summer Triangle..... Using a motionless sphere we can define a great circle, the horizon, and its poles, zenith and nadir 2. The daily motion of the sphere All the sky moves from Est to West around an axis that seems fixed on the sphere (for short periods of time as human life) The motion and the sphere define two poles and an equator, we can use some stars to find them; Polaris for NCP and Southern Cross and Centaurus for SCP, Orion Belt for the equator Geographic Latitude is the elevation of the visible pole and, roughly, of Polaris The motion of the sphere seems uniform, for this reason it was the source for time telling, but the time scale that comes from is NOT uniform: rotation is slowing down, the day is longer and longer at the rate of 2 ms a century From the motion we can distinguish circumpolar, rising and setting, not visible stars; their definition depends on the observer’s latitude, so the same stars become visible, circumpolar or invisible at different latitudes At our latitude polar axis is oblique in respect of the horizon and the paths of each object in its daily motion is likewise oblique; at the Geographic North Pole the polar axis is vertical, the celestial equator overlap the horizon and star paths are horizontal; at the Geographical equator the polar axis is on the horizon, the equator passes through the zenith and the star paths are vertical 3. Fixed and wandering stars All celestial object are carried from the daily motion of the sphere at the rate of 15 degree an hour, 1 deg every 4 minutes Fixed stars seem to be engraved on the surface of celestial sphere Mobile stars move along the ecliptic line from West to Est, that is their direct motion; all of them sometime move in retrograde motion from Est to West Also the Sun seems to move along the ecliptic line, its apparent path among the stars was completely described by Mesopotamian People three thousands of years ago and Greek People learnt from them. Perhaps eliacal rising of a star was used The Moon moves actually around us at the variable rate of around 14 degree a day The motions of the Sun and the Moon along the ecliptic are the base of calendars The Sun rising and setting points, Sun elevation at noon and the lenght of its daily arc depend on the date and latitude The annual Sun trip defines seasons, solstices and equinoxes 4. Eclipses The geometrical conditions Types of eclipses The eclipse year and the Saros The cliptic limits Historical value of eclipses 5. The precession of equinoxes Since most of the members of the solar system orbit in the same plane, close to the ecliptic, they tend to pull the equatorial bullge of the Earth towards it and most of this “flattening torque” is caused by the Moon and the Sun. But the Earth is rotating and therefore the torque cannot change the inclination of the equator relative to ecliptic, the rotation axis turns in a direction orthogonal to the axis and to the torque, thus describing a cone once in roughly 26000 years Polaris is not the same star and some time there is no star close to Celestial Poles; Vega is nowadays far away from NCP, but it will be very close in 13000 years The equinoxes seem to reach western horizon before stars, from this, the word precession The position of equinoxes and solstices among the stars change continously and change likewise the stars you observe in the same seasons in different epochs. 6. Some Tools and readings: 1. Arcetri Almanac http://www.arcetri.astro.it/pubblicazioni/Annuario/ 2. Arcetri Sky Maps http://www.arcetri.astro.it/Italiano/EduPage/sky_maps/maps. html 3. Planetario Program http://www.arcetri.astro.it/Italiano/EduPage/software/planetario.html 4. The Electric Astrolabe http://www.astrolabes.org/electric.htm 5. Ancient cosmological models http://www.csit.fsu.edu/~dduke/models.htm 6. NASA Eclipse home page http://sunearth.gsfc.nasa.gov/eclipse/eclipse.html 7. A celestial appointment: on 01 december 2008 The Moon will cover Venus at 17:14 here in Florence. Observe the sky if clear! 8. Art and Astronomy: visit S.Lorenzo Church in Florence; read this article to prepare your visit http://www.arcetri.astro.it/~ranfagni/slorenzo/