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Material Type: Notes; Class: Stellar & Galactic Astronomy; Subject: Astronomy; University: North Georgia College & State University; Term: Unknown 1989;
Typology: Study notes
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Chapter 2 page Column Keywords 27 right constellation official borders of constellations set by IAU 88 constellations 28 left constellations visible from southern hemisphere named by seventeenth-century European explorers celestial sphere right north celestial pole south celestial pole celestial equator ecliptic whitish band of light – Milky Way Galaxy 29 left traces galactic plane as viewed from our location shape of Milky Way Galaxy right we see half the celestial sphere at any one time local sky horizon many ancient peoples – flat Earth zenith meridian direction and altitude 30 angular size angular distance rough estimates of angular size using hand right arcminutes arcseconds 1 = 60 arcminutes = 3600 arcseconds angular unit abbreviations The Circling Sky stars rising and setting really Earth moving 31 left paths of stars – orange dots 33 left latitude, longitude, prime meridian right locations with same latitude see the same constellations 34 left at north pole only circumpolar stars can be seen Sun visible for 6 months out of the year northern hemisphere – altitude of Polaris is your latitude 35 left Seasonal Changes in the Night Sky constellations visible depend on time of year Earth orbits Sun in counter-clockwise direction ecliptic zodiac Sun’s apparent location among the zodiac constellations 36 tilt of Earth’s axis causes seasons 37 left seasons only caused by axis tilt, not by variation of distance from Sun right solstices and equinoxes – stuff with orange dots
38 left equinoxes – Sun rises due east, sets due west solstices – Sun rises and sets furthest north or furthest south first days of seasons – why? right seasons in southern hemisphere 39 explanation of why distance from the Sun doesn’t affect the seasons 40 left precession - cycle of Earth’s precession right why does precession occur? – conservation of angular momentum and gravity 41 left Earth not a perfect sphere – equatorial bulge right The Moon period of Moon’s orbit – 27 1/3 days average distance from Earth – about 380,000 km Moon moves across sky one Moon diameter per hour 42 left Whys do we see phases of the Moon? lunar phases – figure 2. right 1. and 2. complete cycle of phases – 29 ½ days half of moon always lit – phase depends on where Moon is in its orbit 43 left waxing and waning new, first quarter, full, third quarter crescent, gibbous right synchronous rotation phases of Earth from Moon – opposite Moon phases 44 left Earthshine eclipses – stuff with orange dots right conditions for eclipses – 1. and 2. at bottom of column 45 left umbra and penumbra right total lunar eclipse, partial lunar eclipse, penumbral lunar eclipse 46 left totality right total solar eclipse 47 left partial solar eclipse annular eclipse predicting eclipses ( continued on 48) 48 left Thales eclipse season saros cycle – 18 years 11 1/3 days 49 left planets – five planets easy to see planets do not twinkle planet – wandering star – wander through zodiac 50 left apparent retrograde motion Earth-centered universe – greeks – hard to explain apparent retrograde motion - wrong Sun-centered – easy to explain apparent retrograde motion - correct right why did the greeks reject heliocentric universe? 51 stellar parallax 52 left 1. and 2. – 1. correct - you have to have a telescope