Tag Archives: seasons

170. Middle School Astronomy

We learn our astronomy from books, but that isn’t how the science started. The ancient Greeks learned about the stars by looking at the stars. Their understanding was a mixture of observation and myth, with myth sometimes predominating.

When we are young, we also learn astronomy from casual statements we hear from adults. I’ll give you an example. Mars has recently been at a close approach; every evening lately, when I step out my front door (miles from the nearest city) to look at the sky before bed, there it is, red and bright, about halfway to zenith in the south-eastern sky. Now imagine that I say to a child, “Mars is really getting close.” Just that, with no other comment. What images might pop into that child’s mind?

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“The seasons change because of changes in the Earth’s tilt.” You might find a statement like that in an old middle school science textbook along with an illustration like this:

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Not true. Not a lie, but an oversimplification that may be fine for the average student, but does not do justice to the brightest kid in the room. A better statement would be, “The seasons change because of apparent I changes in the Earth’s tilt”, coupled with an illustration like this:

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Now we are more accurate but we’ve confused 90% of the students.

It should be obvious by now that this is a bit of a how-to based on long experience. Even if you aren’t a teacher, you will probably someday have to explain this kind of thing to your own kids.

Let me suggest a third option. First explain things in your best lecture voice with reference to the textbook and with drawings on the board. Then pick a student sitting in the middle of the classroom; out of kindness, choose someone who likes attention. Say, “Helen, don’t move. For the next few minutes, your head is going to be the sun.” Then establish where Polaris lies, for the sake of the demonstration. Your classroom may not allow you to use real north. If some bright, smart-mouth kid catches you out, don’t get mad. Rejoice that someone is paying that much attention and make it a teachable moment.

Now walk around the classroom with the classroom globe tilted toward your Polaris and talk them through the seasons, pointing out that the tilt never changes in relationship to Polaris, but it appears to change in relationship to Helen, our sun. Pat your worst troublemaker on the shoulder as you pass him, wink at the shy girl in the back corner who never volunteers, and say, “Excuse me, Earth coming through,” when you have to dodge around desks.

There is a rule of thumb for teaching science (which probably doesn’t work for algebra). If you enjoy teaching, and you let your students enjoy learning, they probably will.

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That exercise was for letting students visualize things they can’t see for themselves. You can also help them see things that happen in their everyday world, but normally go unnoticed.

Observing the path of the sun through the seasons is an Earth’s-eye-view version of the tilted globe carried through the classroom. How do you compress a year’s worth of observation into one 40 minute session, using the real sun instead of charts and graphs? It can be done, but it takes nine observations on your part, spread over three days, with those three days spread over half a year. It also takes a small can of paint and a paintbrush.

When I set this up, I picked a solid, upright, eight foot steel pole which was set up away from the shadows of structures and which I knew would not be disturbed for years to come — a volleyball net pole out on the playground. At 10 AM, noon, and 2 PM (sun time, not daylight savings time) one summer solstice I painted three inch circles (same diameter as the pole) at the pole shadow’s tip.

I repeated those actions during the fall equinox, which was intriguing for my students. I had a paint can and small brush at the ready during my ten and two classes, and on the stroke of the hour, I ran out of the classroom, painted the circle, and ran back in while they watched from the windows. The noon painting had an even bigger audience because of noon recess. As you might guess, I told those who asked questions, “You’ll find out what this is all about — some day.” On Christmas break I painted the last three circles during the winter solstice.

That spring, and for years afterward, I arranged to teach solar motion as near as possible to the spring equinox. The solstices fall outside school days, and the fall equinox is often cloudy in California. I explained everything with lectures, and reading, and drawings on the board, but then we all went out to those nine circles on the playground. As I talked them through the lesson, we all watched the pole’s shadow move. It is fascinating in our mile-a-minute world to take the time to watch a shadow inch its way across the ground. Even if it wasn’t 10 or noon or 2, everyone could see that the shadow’s tip either had or would touch all three of the middle circles.

I explained how I had placed the circles and invited students to lie down with their head on a circle and look past the tip of the pole to see where the sun would be (or would have been) at noon or 10 or 2 on the first day of summer or the first day of winter.

They paid attention. On days they pay attention, learning happens. It isn’t easy, but it works.

169. North Light at Solstice

Some years ago, I had an epiphany at solstice time, all about north light.

North light is one of those concepts we accept without thinking it through. Artists prefer north light for their studios – we learn this young if we are thinking about being painters. Most of us never become artists and never have a studio, so the notion falls into the category of unexamined concepts.

I learned to paint and draw, but my skill level never rose above adequate. I didn’t become an artist, or any of another double-dozen fleeting ambitions, but I did become a writer and later a teacher. As I was nearing retirement, I bought a three acre parcel with house in the foothills of the Sierras.

For the first time, I had the chance to build something bigger than furniture or musical instruments. I was wandering around the back yard on blistering summer afternoon, thinking about north light and about building a shop with big widows pulling in masses of lovely natural light, when I looked at the north wall of my new house and saw that it was in full, hot, withering sunlight.

That’s not supposed to happen. But it does.

I live at latitude 37, roughly in line with San Francisco, Tulsa, and Washington, D. C. Here the sun is so far north (apparently) by mid-summer that it rises well north of east and sets well north of west, traversing a curved path so that at noon it is still south of zenith. The result is that the north sides of structures receive cool morning sunlight, shade during most of the day, and blistering sunlight in late afternoon.

I should have known, but in the cities where I had spent my life there were always trees and the shadows of multiple buildings to hide the effect. I had studied astronomy, but that is about the big picture, not about what is happening in your own backyard. I should have known from a youth spent outdoors, but then I was always on a tractor and in motion, concentrating on the windrow of hay I was creating, not on how sunlight fell on structures.

As a childI was aware of the motion of sunsets across the western horizon as the seasons progress, because every evening I was in the dairy barn looking out its west facing windows. I still love that phenomenon. There is a place near my foothill home where my wife and I go to watch the sunset. The spot faces west, on the western side of the westernmost hill in our area, so the vista carries all the way across the San Joaquin Valley to the coast range, and to the the buildup of clouds beyond where the cold waters of the Pacific spill fog over San Francisco. Mount Diablo, the highest peak in this section of the coast range, lies directly west of our lookout. Every spring and autumn equinox, the sun sets directly behind it. As summer progresses, each sunset is further north until we reach the summer solstice. Then they drift back, pass Mount Diablo, and head south until the winter solstice turns them back north again.

This is how astronomy began, with observations of visible phenomena. There were no ideas of orbiting bodies; that came later. Today, however, we know too much. We learn our astronomy from textbooks, not from our own observations. And then the reality in our own back yard catches us by surprise. more tomorrow and Wednesday

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For the record, I scratched the itch to build a building. My wife and I rebuilt a sagging 11 x 24 tool shed, put in big windows and a fancy facade. It is our quilting studio, where I also write. I’m sitting in in it now, watching the sun rise through the east window.

65. Winter Solstice

DSCN1841The calendar says “first day of winter”. The astronomically inclined say “winter solstice”. Since this is the day that the sun appears to be as far south as it ever gets, it bothers me sometimes that the first day of winter (speaking with a northern hemispheric bias) comes when, by the sun, winter should be half over. That feeling comes of having a certain kind of over-picky mind; pure experience, of the shivering kind, recognizes that there is a delay effect in seasonal changes. Meterologically speaking, the phrase “first day of winter” fits pretty well. It’s going to get a lot colder before it gets warmer again.

What if it didn’t get colder, or warmer? What if we had no seasons? What would that do to your heating and cooling bills? What would it do to your wardrobe? Would you even wear clothing?

It’s easy enough to arrange; just choose a planet with no axial tilt. Like Cyan.

Late in the novel Cyan, while some of the scouts are on a rescue mission to save a group of Cyl (non-human natives) by transferring them to the southern hemisphere, we get a detailed picture of what Cyan looks like.

In the cockpit, Debra was alone with her thoughts while Tasmeen attended to piloting the landing craft.  The sky outside was black with stars. She had never expected to see the stars from space again. Beneath them, Cyan spun lazily. Clouds blanketed various portions of the temperate zone where humans lived, and only a bit of the torrid zone which was the domain of the Cyl. Further north than that, where Keir and the children were, clouds massed high and storms raged.

The lower latitudes passed beneath them. This was the band of eternal desert, where every island and fragment of a continent was dry lifeless rock studding a lifeless sea. There were few clouds here, but ahead of them now was the equatorial cloud band. The heart of the great heat engine that was Cyan, where the water steamed in the relentless light of Procyon A, pumping moisture into the atmosphere and sending it northward and southward, over the lifeless bands too hot for coalescence and on up toward the dry Cyl lands and the wet human lands and the great snowcapped poles.

They passed the clouded equator, the southern dead zone, spiraling down toward the southern torrid, the zone where neither Cyl nor man had ever set foot, and where the Cyl could live secure from the depredations of man.

Aside: Cyan was originally scheduled for publication in January, but has been pushed back to April or May.