The Delaware Gazette

The Pole Star

I’ve been doing some infor­mal polling dur­ing our day­time field trips to Perkins, and I’d like to share the results with you. Ask your aver­age fifth grader to iden­tify the bright­est star, and most of them will reply, “Polaris,” the North Star.

A quick trip out­side demon­strates that your aver­age fifth grader is wrong. Polaris is the end star in the tail of Ursa Minor, the Lit­tle Bear, also known as the Lit­tle Dip­per. Polaris is easy enough to find if you can see it at all. It is, after all the NORTH star. Just look directly north about half way up from the hori­zon. Sadly, Polaris is not par­tic­u­larly bright. It’s dif­fi­cult to see from sub­ur­ban skies because of all the street­light pol­lu­tion, and you won’t see it at all from down­town Columbus.

What makes Polaris spe­cial is that every other star you see changes its posi­tion over the course of a night. Polaris just seems to sit there. Of course, the stars are so far away that from the per­spec­tive of a fixed point in space, they don’t seem to be mov­ing at all. We’re the ones who are mov­ing. Earth rotates once every day. At 40 degrees lat­i­tude, where we’re located, we are hurtling around the spin­ning ter­res­trial orb at 680 miles per hour. And that would knock your hat right off if your hat weren’t also trav­el­ing at the same velocity.

In a sense, Polaris isn’t fixed at all. Where it is in the sky depends on where you hap­pen­ing to be stand­ing on Earth, as early sailors try­ing to find there way around soon learned. To the south of Earth’s equa­tor, the North Star is invis­i­ble below the north­ern hori­zon. Directly above the equa­tor, the Pole Star sits just above the north­ern horizon.

At 40 degrees lat­i­tude, it hov­ers 40 degrees above the hori­zon, about half way from the hori­zon to the top of the sky. At 20 degrees lat­i­tude, Polaris is 20 degrees above the hori­zon, and so on.

Since Earth is spin­ning from west to east, the sun, moon, plan­ets, and most of the stars seem to move from east to west.

From our Delaware van­tage, they cir­cle around Polaris, ris­ing above the hori­zon and even­tu­ally setting.

The odd­est place to observe Polaris would be from the North Pole. If you were stand­ing right next to Santa’s work­shop, Polaris would be straight over­head, and the other stars would spin around it like horses on a merry-go-round. That’s some­thing I’ve always wanted to do. I have a bone to pick with Santa about that tele­scope I didn’t get when I was eight years old.

Another way of think­ing about Polaris is that it is directly above the imag­i­nary line that passes through Earth’s north and south poles. Extend that line 820 light years (or 5 quadrillion miles) into space and you’ll run into the Pole Star. Well, almost, any­way. Polaris isn’t directly north. It actu­ally scribes a cir­cle, albeit a small one, over the course of a day and night, just like all the other stars.

And there’s another prob­lem. Earth wob­bles a lit­tle as it spins on its axis. Over the course of 26,000 years, the posi­tion of the pole in the sky changes. Right now, it’s near Polaris. To the ancient Egyp­tians in 3,000 BCE, the North Star was the star Thuban in the con­stel­la­tion Draco, the Dragon. Our cave-dwelling ances­tors 18,000 years ago looked toward Alderamin, the bright­est star in Cepheus, when they wanted to find their way.

The pole will never be pointed directly at Polaris, but it reached its clos­est point in 2005. Every sec­ond that passes, the pole moves a bit far­ther away from Polaris and toward the star Vega in the con­stel­la­tion Lyra. In 50,000 years or so Vega will be the clos­est star to the pole. Don’t for­get to mark it on your calendar.

Astron­omy Fair

Start­ing at 4 p.m. This Sat­ur­day, Sept. 10, the Colum­bus Astro­nom­i­cal Soci­ety will hold its annual Astron­omy Fair at Perkins Obser­va­tory. They’re charg­ing $5 per car admis­sion and will donate the pro­ceeds to Perkins Obser­va­tory. If you want to get a great intro­duc­tion to stargaz­ing and a day­time tour of the obser­va­tory as well come on down.

Tom Burns is the direc­tor of Ohio Wes­leyan University’s Perkins Obser­va­tory. Con­tact him at tlburns@owu.edu.

Posted by on Sep 4 2011. You can follow any responses to this entry through the RSS Feed. Comments can be made below.

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