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8/9/2019 01 Naked-eye Observations of Sun & Moon
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Lecture 1
Naked-eyeObservations:Sun & Moon
Total Solar Eclipse, 212 Nov 1!,"ustralia
http://apod.nasa.gov/apod/image/1211/tse2012C3shadowbands_StephenMudge.jpghttp://apod.nasa.gov/apod/image/1211/tse2012C3shadowbands_StephenMudge.jpg8/9/2019 01 Naked-eye Observations of Sun & Moon
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Sunrise
Te direction o( terisin' Sun can'estrou'out te
year) Only on te
e*uino+es are terisin' point dueeast)
"rny & Scneider, ./0E 1)1!"
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an'in' irection
Te Sun 3ill al3ays rise and set (urtest tote sout durin' te day o( 4interSolstice, and (urtest to te nort durin'
Su%%er Solstice)
.reece
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Eart5s 0otation &0evolution
Te period (ro% one noon to te ne+tis te 26-our solar day) Te dailypro'ress o( te Sun across te sky is
a conse*uence o( Eart5s rotation)
Eart rotates on its central a+is 3ileat te sa%e ti%e resolvin' around
te Sun) Eart takes !78 days to orbit te Sun)
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nclination o( 0otation "+is
Eart5s rotation a+is is inclined at an an'le o(2!)8to te plane o( its orbit)
Te su%%er solstice represents te locationin Eart5s orbit 3ere our planet5s Nort pole
co%es closest to pointin' in te direction o(te Sun) Tis occurs on or near 9une 21)
Si+ %onts later, te Nort #ole points(arter (ro% te Sun) 4e ave reaced te
3inter solstice) Te vernal autu%nal; e*uino+ occurs innortern sprin' (all;, on or near Marc 21Septe%ber 21;)
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Stoneen'e
#eraps te best-kno3narcaeoastrono%icalsite)
t dates (ro% te Stone"'e)
0esearcers tink it 3asan early astrono%icalobservatory o( sorts%a'ic> %o%ent)
http://www.english-heritage.org.uk/stonehengehttp://news.yahoo.com/michael-johnson-takes-olympic-flame-stonehenge-112314022--oly.html?_esi=1http://antwrp.gsfc.nasa.gov/apod/image/1006/stonehengesun_alexander_big.jpghttp://news.yahoo.com/michael-johnson-takes-olympic-flame-stonehenge-112314022--oly.html?_esi=1http://www.english-heritage.org.uk/stonehenge8/9/2019 01 Naked-eye Observations of Sun & Moon
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@eel Stone
On su%%er solstice, as seen(ro% te center o( te stonecircle, te Sun rose directly overte eel stone)
http://viewfinder.english-heritage.org.uk/search/reference.aspx?uid=76018&index=12&mainQuery=stonehenge&searchType=all&form=homehttp://viewfinder.english-heritage.org.uk/search/reference.aspx?uid=76018&index=12&mainQuery=stonehenge&searchType=all&form=home8/9/2019 01 Naked-eye Observations of Sun & Moon
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"pparent Motion o( te Sun
On te e*uator, 3e3ill observe tat teSun is (artest nortdurin' su%%er
solstice and (artestsout durin' 3intersolstice)
Solar altitude is te
sa%e durin' botsu%%er and 3intersolstice)
http://mydarksky.org/2009/12/22/solstices-and-equinoxeshttp://mydarksky.org/2009/12/22/solstices-and-equinoxes8/9/2019 01 Naked-eye Observations of Sun & Moon
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Nortern @e%ispere
On te norternand souterne%ispere, te
noonti%e Sun isi'est in te skydurin' su%%ersolstice and lo3est
in te sky durin'3inter solstice)
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"pparent Motion o( te Sun
Te picture is a co%posite o( ourly i%a'estaken o( te Sun above ?ursa, Turkey)
2A ec,4interSolstice
2$9une,Su%%erSolstice
2$Marc,BernalE*uino+
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Seasons
Te tilt o( Eart5s rotation a+is isresponsible (or te seasons)
T3o (actors co%bine to cause te
seasons)1) Tere are %ore ours o( dayli't durin'
te su%%er tan in 3inter)
2) 4en te Sun is i' in te sky in su%%er,rays o( sunli't strikin' Eart5s sur(ace are%ore concentrated tan in 3inter) "s aresult, te Sun (eels otter)
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@ours o( ayli't
"t te e*uino+es,e+actly al( o( tesunCs circular patlies above te
oriDon) n 9une, considerably
%ore tan al( o( tecircle is above te
oriDon) n ece%ber, %uc
less tan al( tecircle is visible)
http://physics.weber.edu/schroeder/ua/SunAndSeasons.htmlhttp://physics.weber.edu/schroeder/ua/SunAndSeasons.html8/9/2019 01 Naked-eye Observations of Sun & Moon
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Solar @ei'ts
( you took a picture o(te Sun at te sa%e
ti%e eac day, teSun 3ould trace outan anale%%aF overte course o( a year)
3int
er
su%%er
" co%posite o( 67 separate Sunpoto'raps taken durin' 2! in
http://abyss.uoregon.edu/~js/ast122/lectures/lec02.htmlhttp://abyss.uoregon.edu/~js/ast122/lectures/lec02.html8/9/2019 01 Naked-eye Observations of Sun & Moon
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Eart5s Elliptical Orbit
Tis co%posite neatly co%pares t3opictures o( te Sun taken 3it te
sa%e telescope and ca%era on tedates o( #erielion closest
http://www.uwsp.edu/geo/faculty/ritter/glossary/A_D/Aphelion.htmlhttp://www.uwsp.edu/geo/faculty/ritter/glossary/A_D/Aphelion.html8/9/2019 01 Naked-eye Observations of Sun & Moon
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Sunset
Te Sun appears oran'e and di%%er tan at noon)
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Oran'e & i%
0aylei' (ound tat blue li't is %uc %ore easilyscattered tan red li't, basically because te3avelen't o( blue li't 6 n%; is closer to tesiDe o( air %olecules tan te 3avelen't o( red
li't A n%;
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Near te @oriDon
"t dusk, 3it te Sunnear te oriDon,sunli't %ust passtrou' %uc %ore
at%ospere) Te blue co%ponent o(
te Sun5s li't isal%ost entirely
scattered out o( teline o( si't, and evente red co%ponent is
di%inised in intensity)
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Moon llusion
Te Moon appears tobe very nearly tesa%e siDe no %atterits location on te sky)
ore'round obHects%ake a oriDon Moonsee% (arter in tedistance) Te %ind
interprets %oredistant obHects as3ider)
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Lunar #ases
Te Moon5s appearance under'oes are'ular cycle o( can'es, takin' rou'ly2I)8 days to co%plete)
Te 3ord %ont derives (ro% Moon ;)Te inese and sla%ic calendars in use
today are still based s*uarely on te lunarcycle, eac %ont be'innin' 3it te ne3Moon)
Te %odern 4estern calendar retains %ontsas convenient subdivisions, but tey ave noparticular lunar si'niGcance)
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Moon Orbits Eart
Te Moon e%its no li't o( its o3n)nstead, it sines by re=ected sunli't)
@al( o( te Moon5s sur(ace is
illu%inated by te Sun at any instant)
?ecause te Moon orbits Eart, tevisible (raction o( te lunar sunlit (ace
varies (ro% ni't to ni't) JouTube: Te #ases o( te Moon
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More rescent Moons
rescent Lunar#ase
LunarEclipseK
LunarEclipseK
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#artial Eclipse
212 9une 6
4e see tat te Eart5s sado3on te Moon is curved)
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Eart5s urved Sado32$ "u'ust
Tis co%posite i%a'e uses successive picturesrecorded to trace out a lar'e part o( te u%braCs
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Total Eclipse
211ece%ber N": Sin'aporeans 'ater to
see lunar eclipse
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i+, ./0E I)11
eep 0ed oloration
urin' a total lunar eclipse, te Moon o(tenac*uires an eerie, deep red coloration)
" s%all a%ount o( sunli't is reddened byEart5s at%ospere 0aylei' scatterin'; andre(racted bent; onto te Moon5s sur(ace)
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Solar Eclipses
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Total Eclipse
Te day is brie=yturned into ni't)#lanets and so%e
stars beco%evisible in tedayti%e)
Ti%e-Lapse: " Total
Solar Eclipse
2$ "u'ust, .reat 4all,ina
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ia%ond 0in'
212 Nov1!
"s te total pase te solareclipse ca%e to an end, sunli'tstrea%in' past te ed'e o( teMoon created te =eetin'
appearance o( a 'listenin'dia%ond rin' in te sky)
Sunli't strea%in' trou''aps in te ru''ed proGle o(te lunar li%b creates tebrilliant but =eetin' ?ailyCs
ia%ondsF
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"nnular Eclipse
Te Moon5s orbit isnot e+actly circular)
Te Moon %ay be(ar enou' (ro%Eart tat its disk(ails to cover tedisk o( te Sunco%pletely)
0ou'ly al( o( allsolar eclipses areannular)1II2
9anuary
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uture Eclipses
?ecause 3e kno3 te orbits o( Eartand te Moon to 'reat accuracy, 3ecan predict eclipses (ar into te
(uture)
4eblinks: N"S" Eclipse 4eb Site
Eclipse alculator Solar Eclipses in
Sin'apore
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T3o Eclipse Seasons
Te Moon5s orbit is sli'tly inclined to teecliptic at an an'le o( 8)2;)
n an un(avorable conG'uration, te Moonlies above or belo3 te plane o( te ecliptic)
n a (avorable conG'uration, Eart, Moon,and Sun are precisely ali'ned, and aneclipse occurs)
Tere are t3o periods, kno3n as eclipseseasons, at 3ic an eclipse can occur)
Si%ulation: Eclipses
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Moon5s Orbital nclination
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#recession o( Moon5s Orbit
Te eclipse seasons 'raduallypro'ress back3ard trou' tecalendar, occurrin' about 1I days
earlier eac year) Te 'ravitational tu' o( te Sun
causes te Moon5s orbital orientation
to can'e slo3ly 3it ti%e) "ni%ation: #recession o( Moon5s Orbit
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i+, ./0E I)12
Te Bisibility o( an Eclipse
" total solar eclipsecan be seen (ro%only a s%all
portion o( Eart5sdayti%e side)
" lunar eclipse issi%ultaneously
visible (ro% alllocations onEart5s ni't side)
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Moon5s Sado3
"nnular Solar Eclipse, 212 May 2