AST 309-TIME
Telling Time by the Stars


Using the Big Dipper and Polaris as a clock


The following idea is also due to John Conway. You can determine the local time at night by looking at the Big Dipper and Polaris, and doing a simple calculation.

The first thing is to look at the line joining Polaris to the two pointer stars of the Big Dipper. Here's a picture that shows what you might see:

Conway suggests looking at the line from the Big Dipper to Polaris as if it were the hour hand of a clock centered on Polaris. You read off the time in the sky from this hour hand. In the drawing, the time in the sky is about 1:25 (you have to do the best you can). This can be a little tricky, see below.

Write the time in the sky as hh:mm, in this case, 1:25.

Now write down what Conway calls the time in the year. This is gotten from the date by writing it as if it were a time, as follows: Suppose the date is the d'th day of month m. Then write the time in the year as m:2d. For example, on January 20, the time in the year would be 1:40.

To get the local time (on a 24-hour clock), calculate

local time = 06:30 - 2 (sky-time + year-time).

In the above example, we would have

local time = 06:30 - 2 (1:25 + 1:40) = 06:30 - 2 (3:05) = 06:30 - 06:10 = 00:20,

which corresponds to 20 minutes after local midnight. If you get a negative number, just add 24 hours.

The result is local time. It doesn't take into account Daylight Savings Time (so you have to add an hour if you are on Daylight Savings Time), and it doesn't take into account your longitude away from the center of your time zone. The correction for longitude is 4 minutes for each degree you are away from the center of the time zone. In Austin, TX, since we are 31 minutes west of the center of our time zone, you have to add 30 minutes to the result to correct for this effect (because if you are west of center, the sky will read earlier than a standard clock). In January we are on Standard Time, so the only correction would be for the longitude effect, and our final result in the example would be

Central Standard Time = 00:50 (approximately).

Conway points out one caution: Near 3:00 and 9:00 sky-time, it is somewhat difficult to read the clock. The picture shows it correctly: You should draw the line from Polaris to the pointers, and see what angle that makes with the vertical. If it is a 90 degree angle, then it is 3:00 (or 9:00 on the other side). Because of the curvature of the sky, it can appear that the sky-time is closer to 00:00 (12:00) than it actually is, so be careful! One way to judge this is to compare the angle to the corner of a small card, or to use your hands to mark off a 90 degree angle, placing the corner on Polaris with one side of the card (or your hand) pointing straight up.


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