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        IGNITE the night sky electronically!
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1.   Demonstrate the phases of the moon by showing the alignment of the earth  moon  and sun   b  Explain the alignment of the earth  moon  and sun during solar and lunar eclipses   c  Relate the tilt of the earth to the distribution of sunlight throughout the year and its effect on  climate     Getting Started    When you open Stellarium  it might figure out where you are and what time it is from your computer   If it does not  or if you want to change locations     do the following   Use F6 to access the Location Window  Or on a Macintosh OS X  go to left side and hover over  compass needle image to access the Location Window   Use F5 to access the Date Time Window to set the time to a different time     e By default  you are pointing South with a 60 degree field of view  FOV   To change where you  are pointing you can    e Click and drag with the mouse    e Use the arrow keys    e To zoom in and out or to select an object you can    e Page up page down to zoom   e Use mouse wheel to zoom in out    e Select an object with left mouse click and unselect with right mouse click    e Use the forwardslash     to zoom in to selected object   Very cool on the planets       e Use the backslash     to return to original default field of view     Move time forward faster     click the double forward arrow at the bottom of the screen  If you click  again  you can make time go even faster  And faster still  You can make it go fast enough to make  yourself a bit ill  Use the  L  key to spee
2. IGNITE the night sky electronically     Using Stellarium to present Astronomy concepts in your classroom     A planetarium software like Stellarium is very useful as it is always clear weather in the computer and  you can speed up time to show days and months in a class period  You can also translocate yourself to  other parts of the planet to view the sky from other places     Stellarium is a freely downloadable program for Windows and Mac  It is provided on this disk for you  but you can download the newest version from http   stellarium org  A user s manual is provided at  http   stellartum org wiki index php Category User 27s_ Guide and a copy is included on this disk     Some of the  sky  standards in the GPS   S4E1  Students will compare and contrast the physical attributes of stars  star patterns  and  planets  b  Compare the similarities and differences of planets to the stars in appearance   position  and number in the night sky   c  Explain why the pattern of stars in a constellation stays the same  but a planet can be seen in different  locations at different times   S4E2  Students will model the position and motion of the earth in the solar system and will  explain the role of relative position and motion in determining sequence of the phases of the moon   a  Explain the day night cycle of the earth using a model   b  Explain the sequence of the phases of the moon   S6E2  Students will understand the effects of the relative positions of the earth  moon and sun   a
3. both in the view at once  What do you think  the Moon will look like  Zoom in to check      Teacher note     many students may not realize that the Moon is visible during the daytime for so many  days of the month  The reason may be that the Moon is not in the same spot in the sky at the same time  of day       Go the the gond of February  This is what is known as i    quarter moon  Note that the Moon is  rising right around noon time  Run time forward to see a full day  How does the relative  position of the Moon and Sun change during the day   You may want to turn on the  constellation name and patterns using c  and v to help since you can t get both the Sun and  Moon in the same 60 degree field of view     When the Sun is setting  where is the Moon in relation to the Sun    After sunset  can you still see the Moon  Is the same side of the Moon lit up  How many hours  after the Sun set did the Moon set    Make a prediction  what will be the relative position in the sky of the Sun and Moon when the  Moon is in the full moon phase   Feb  27  go to a time just before sunset to check your answer   Go to March 3  2010 around 23 00  Look to the East and zoom in on the Moon  Do you think  the Moon will set before the Sun rises  What should the relative position of the Moon and Sun  in the sky be to make this phase    Zoom back out     and let the night progress  Does the Sun rise first  or does the Moon set first     I hope you can see how using Stellarium  or other planetarium so
4. d up     There are MANY more features     but let s look at how to use Stellarium to show the altitude of the Sun  changes during the day and that the Sun is highest in the sky when it is due South in the Northern  hemisphere  Azimuth is a way of numerically specifying NSEW  Azimth   0 for North  90 for East  180  for South  ad 270 for West   e Set date to March 21  Set time to around 7 30 am   7 52 AM works well for Columbus   You  should see the Sun rising near the East  You may need to scroll over to the East to see it   e Click fast forward 3 times   or hit J three times   You may have to scroll around on the screen to  follow the Sun   e Click on the Sun so you can see its vital statistics on the screen  What is the azimuth when the  altitude is the highest   click  K  to slow time down to normal speed again   e Return to around sunrise on March 21   e Use the     key to advance time by about a week  Keep advancing time until you are near the  beginning of May   e Run time through a day and find the azimuth when the Sun is highest  You should find it is  again 180 degrees     or due South     for observers in the Northern hemisphere   Depending on your students  you may need to reinforce this with more than two examples     Day Length  amp  Seasonal Climate Variations    Once you have mastered following the Sun and observing its position at its highest point  you can start  to relate seasonal climate variations to the length of day  which in turn is related to the tilt o
5. f the Earth   Longer days   more hours of sunshine   warmer  Stellartum can be used to demonstrate the variations  in the length of day at different times of year  Ask your students to find how long the day is     by  defining the beginning of daylight to be when the Sun is at or above an altitude of 0 degrees  You can  break up your class into groups and ask them to find out the sunrise and sunset times for a few dozen  days and then plot the length of day as a function of year     or you can demonstrate day length using  your own projector and ask students to record the data    The graph will depend on your latitude as shown here  This graph assumes Day 0 is December 21  the  shortest day of the year   http   gandraxa com length of_day aspx     Length of Day             30   Northpole     60             6r     s0      _4  beeen    20               0      0    Equator              Day of Year    The nice thing is that once you click on the Sun  you don t have to follow the Sun in the sky to see its  altitude  The altitude will update even if you can t see the Sun on the screen     Planets vs  Stars    The word planet is originally Greek for wandering star  What does this mean  And how can we  demonstrate this to students who may live in light polluted environments where it is not feasible to  make regular observations of the night sky  Compare and contrast the position of highly recognizable  constellations with that of some planets over a few months or a few years using Ste
6. ftware  might provide another  dimension for teaching various abstract ideas about the sky     Common Key Strokes for These Exercises    K    Return to  normal speed  Go backwards  in time or  slow down  forwards time  Go forward in  time or slow  down  backwards  time   Go Forward  one day   Go Back one  day    Go forward  one week    Go back one  week    Show planet  names    Show  constellation F6  outlines    F5    Show  constellation    names    Show ground          Show NSEW  directions  Show  atmosphere  if  you turn off  the  atmosphere  during the day  time  you will  see the stars  instead of blue  sky      Date Time    Location on  Earth     Zoom in on  object    Zoom back  out    Want to learn more astronomy and how to use real astronomy data in your high school classroom   Apply fora GEARS summer workshop  Applications are available at the GEARS booth at GSTA or by  visiting the website  http   cheller phy georgiasouthern edu gears   and clicking on the Workshops link   Georgians Experience Astronomy Research in Schools  GEARS  is funded by NASA grant NNX09AH83A through the GA  Department of Education  and is supported by Columbus State University and Georgia Southern University     
7. in  Capricorn in the Southwest around 20 00  Dec  10  2009  You can see it for a few weeks at the same  time of night  You may have noticed Jupiter in the Western sky around sunset this winter     Phases of the Moon    Fourth graders are supposed to be able to explain the sequence of the phases and sixth graders are  supposed to relate the phases of the moon to the relative positions of Earth  Moon  and Sun  There are  fabulous 3 D kinesthetic activities related to the phases of the Moon   e g   http   www learner org teacherslab pup act_moonphase html  You can also use Stellarium to show the  relative positions of the Sun and Moon as seen from the Earth observer to help show the progression of  the phases of the Moon  and why certain phases are visible at certain times of day in certain parts of the  sky  High School level      Go to February 10  2010  at noon  Look in the South  You should see the Sun and Moon  Make  a note of the relative position between the Sun and Moon    Click on the Moon    Quick     make a prediction  What do you think the Moon will look like    Zoom in on the Moon using      Does your prediction match the appearance    Zoom back out using       Go forward one day      Make your prediction about what you think the Moon will look like   Make a note of the relative position of the Moon and Sun in the sky     Go forward to about the 2oth of February  Note the relative position of the Moon and Sun in the  sky  You might have to scroll around to get them 
8. in Cancer  Normally the planets will travel Eastward with respect to  the stars  That time interval when Mars  or other planets   reverse  direction and head Westward is  called retrograde motion  It happens when the Earth  in its orbital motion around the Sun  begins to  catch up to the planet in its orbit  See this simulation for a better view   http   www astro illinois edu projects data Retrograde    This year  Mars is undergoing retrograde  motion from December 20  2009 to March 10  2010  So  when we started this activity    Mars was  already undergoing retrograde motion  Retrograde motion is not part of the standards until high school  Astronomy     You may also use Stellarium to address certain aspects of S4E1b   in that some of the planets are  bright and that they may change brightness  note how Mars gets dimmer as Earth and Mars move  farther apart between January and April 2010  What you can t use Stellarium for is the  lack of twinkle     most planets have compared to the stars  The distance of the stars makes them appear very small  so  small that any piece of pollen can block the light for an instant and cause the brightness of the star to  appear to vary     or twinkle  Planets are much closer  by contrast  and have a finite and measurable  disk  Small fluctuations in the atmosphere will affect the overall appearance of the planet much less so  they don t twinkle     If you want another example of planetary motion with respect to the stars     look for Jupiter 
9. llarium  This helps  you get at S4ElIc     e Go to January 27  2010  20 00 or so  You should see Mars rising in the East   check that your  options for show planet labels is on  hit  p  or click planet button on bottom menu   Also turn on  the constellation lines   c   and constellation labels   v    You will see that Mars is in the  constellation Cancer    e Ask your students to sketch the relative position of the stars in Cancer and Mars    e Advance the night sky 6 or 7 hours and continue to follow Mars    e Ask your students to repeat their sketch of the stars of Cancer and Mars    e Are the relative positions the same at the beginning of the night and towards the end of the  night    e Advance to February 12  2010 around 19 00  Look in the southeast  You should again see Mars  in the constellation of Cancer  Is Mars in the same spot relative to the other stars in the  constellation   Teacher note     a careful observer will probably be able to see changes in the  position of the Moon with respect to the stars in one night  but a naked eye observer is not going  to notice a difference for the planets in one night      e You can use the     key to step forward a week at a time and watch the relative position of Mars  change with respect to the stars in the constellation Cancer   You can also see it gets lighter for  the same time of night     If you go far enough into April  you may notice that Mars stops heading Westward and reverses  directions with respect to the stars 
    
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