"MIThenge"
MIT Infinite Corridor Astronomy |
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In a tradition going back more than 30 years, people gather on the third floor of the Building 8 end of the Infinite Corridor to view the "MIThenge" effect. In mid-November and in late January every year, the circular path of the sun crosses the axis of the infinite corridor. When this happens the setting sun can be seen from the far end of the corridor. (As viewed from a stationary point on the earth, the path of the sun through the sky is roughly a circle which moves north and south as the seasons go by.) The arrangement of the infinite corridor so as to capture the setting sun at a particular moment is sometimes called MIThenge by analogy with Stonehenge.
Predictions Prepared by Ken Olum
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| The predictions shown above give the times at which the center of the sun will cross the azimuth of the infinite corridor axis, and the observed altitude of the center of the sun above a level reference plane at that time, in minutes of arc. The sun is approximately 30 minutes of arc (half a degree) in diameter, and so extends about 15' in each direction. Because there is a hill in Boston that blocks a level view along the corridor, only parts of the sun that are somewhat above the level plane are visible. What you'll see As the sun becomes better and better aligned with the corridor the amount of floor that is illuminated goes up and up. Since the floor is very reflective this means that the reflected sun can be seen far down the corridor as the event approaches. The orange light reflected onto the ceiling is often striking. This phenomenon is visible for a week or two around the actual sunset days. At some point, some portion of the sun's disk will be visible from the far end of the corridor. Which part of the disk will be seen first depends on whether the sun is crossing above or below the corridor. If the altitude in the table above is high, the sun will cross the upper right edge of the corridor as seen from the lower left. If the altitude is low, the sun will cross from the center left of the corridor and set below the hill. The disk of the sun is larger than the area of sky visible from the end of the corridor. Therefore if your timing is right and you get a good vantage point you will see nothing of the sky except for the interior of the sun's disk. Observing this event depends strongly on atmospheric conditions. I think the best is a very red sunset. This decreases the total light intensity and makes it possible to see the corridor and the sun at the same time. If the sky is brilliantly transparent right down to the horizon then the setting sun will be too bright to look at. When you use a filter to save your eyes (see below) you won't be able to see much of the corridor. I have found that the infinite corridor produces the "moon illusion", in which the setting sun looks gigantic in the sky, even though it is no larger at the horizon than it is at the zenith. The period of time during which the sun can be seen from the corridor end is quite short -- no more than two minutes, and only as long as that under ideal conditions. Some suggestions:
Data and Computations These predictions depend on knowing the azimuth of the infinite corridor to an accuracy of several arc-minutes. The best figure we have found is the accurately surveyed azimuth of MIT's property line along Memorial Drive, which is 245.47391075 degrees true. According to Michael K. Owu '86, the infinite corridor should have been constructed parallel to this line. However, it is possible that they aren't really exactly parallel, which would cause an error in the above tables. Other possible causes of error include computer program bugs and general incompetence on my part. You can help improve the computations by taking sightings during the event. What we need to know is the azimuth of the corridor. The azimuth of the sun in the sky at any given time can be easily computed. So if you observe that the left edge of the sun is visible by sighting along the corridor wall and make a precise note of the time then we can calculate the azimuth. Note that this doesn't help with the top edge, but only the left or right edge. Also note that we need a fixed line in order to know what it is whose azimuth we've computed. It won't help to say "I saw the left edge disappear behind the door" unless you know from what point you observed this.
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