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Seasons on Saturn | ||||
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My Video Hello 1.8Mb mpg |
Creating a model to
Predict Hubble’s View of Saturn With Keith Noll
Saturn's equator is tilted relative to its orbit by 27 degrees, very similar to the 23-degree tilt of the Earth. As Saturn moves along its orbit, first one hemisphere, then the other is tilted towards the Sun. This cyclical change causes seasons on Saturn, just as the changing orientation of Earth's tilt causes seasons on our planet. These Hubble Space Telescope images, captured from 1996 to 2000, show Saturn's rings opening up from just past edge-on to nearly fully as it moves from autumn towards winter in its Northern Hemisphere . The first image in this sequence, on
the lower left, was taken soon after the autumnal equinox in Saturn's Northern
Hemisphere. By the time of the final image in the sequence, on the upper right,
the tilt is nearing its extreme, or winter solstice in the Northern Hemisphere
Your challenge is to use each of the images of Saturn
below to find out when Hubble will next view Saturn across the plane of the
rings (like looking side-on to a CD).
To do this, follow the procedure below:
1.
Use the linked images above and our recommended program ‘WaveJ’ to
measure the width and the apparent height [OPU1]of the rings for each
image.
Click
here
for a guide to using WaveJ.
2.
Use trigonometry to find the angle below the plane of the rings
from which Hubble viewed the images in each case. To find out why this angle is
helpful and for help with this click
here.
3.
Input your angles into the MS Excel program
here
and transform the sin curve to fit your data by
shifting and stretching the basic shape up and down.
Now you can read from your graph when the angle
was last 0° and when it will next be 0°.
If you’ve got this right then your prediction for
the next view of Saturn across the plane of the rings will be correct.
Congratulations
– you are now prepared for this rare astronomical event!
Click
here
for a zipped folder of the essential files in this pack (1.7mb) |
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