Wednesday, March 21, 2007

Happy Spring


The start of the spring season is far less romantic than the first bloom, the larking robin, or the shortening of sleeves and pant legs, exposing skin and luring your fancy.

Instead, the vernal equinox (Latin for spring equal night) happened for only a minute or two, just 7 minutes past midnight today. That marked the moment the sun was directly over the equator, working its way back to the northern hemisphere. Sexy!

Tuesday, February 13, 2007

You Will Never See the Dark Side of the Moon


Well, technically nobody will ever see the dark side of the moon, because no such thing exists. All sides of the moon receive sunlight, but there's still a side you will never see first-hand...unless you're an astronaut on a lunar mission.

It's the farside, not the dark side. The concepts are similar; the names are different.

From Earth, we only ever see one hemisphere of the moon. The farside is always out of our sight, facing off into space. The moon rotates just like the earth, but it rotates for once for every revolution around Earth: 28.5 days. That is roughly equal to a month, or the amount of time it takes to complete a revolution, a synchronous rotation. Therefore, we only see one side.


The farside is riddled with craters, since it intercepts many earth-bound meteors. This image was taken by Apollo 16.

Oh well, I guess one side is better than no sides.



A grammar note: Earth is only capitalized when referring to the celestial body without the use of a definite article, namely the.

The Number of Galaxies in Nothing

Great if you have 6 minutes. Always one of my favorites, the image was my desktop background for a while. I understood where it had come from, but not what it meant until this video.

Monday, February 12, 2007

Finding North

North. It's the "never" in the mneumonic device "never eat spider webs," which translates as North East South West, or the compass directions in a clockwise motion. But where is it?

North is north--yes, that's easy. It's where Canada is when you're stateside or the North Pole is when you're anywhere else. It's where birds migrate during the spring and summer and where chill winds from in the bleaker months.

During the day, you can find it by the sun's position. It rises in the east and sets in the west... Moss grows on the south side of trees, contrary to popular belief, so the clear side of the trunk must point north. And it's where the closest magnetic pole is located, so compass needles, or statically charged paperclips, will point there.

But let's suppose you're trapped in a harrowing novel. You're at sea. Darkness surrounds you, save what twinkles and glows in the sky. How do you orient yourself then? Where is north according to the sky?

Well, the North Star, Polaris, may be positioned in accordance with its eponymous namesake. And it is, of course. It's the brightest star in the sky some say, but this isn't the case, even though it is quite bright. And how do you know it's a star and not a planet?

Well, first off, planets do not twinkle. Pockets of air moving across our field of vision cause stars to twinkle (sorry, they're not really pulsating visibly). The air pockets are larger than the stars as they appear in our field of vision. The planets, however, appear larger than the air pockets, so their reflected light is not refracted by air molecules. Second, there are only five of them visible to the naked eye: Mercury, Venus, Mars, Jupiter, and Saturn. So given the vastness of our sky, you have a small chance of mistaking one for Polaris.


Polaris is very easy to find, even if it weren't so bright. Take the most recognizable constellation: The Big Dipper (Ursa Major). If you imagine it as the ladel it represents, then take the lip of the concave and imagine the two stars that make it up point off into space. If you take the distance between these two stars and multiply it by 5 or 6, you'll hit Polaris.

More easily, though, is that Polaris is the end star of the handle on The Little Dipper (Ursa Minor).

Too many stars to concentrate on just one? Try using the moon...as long as it's not full. Whatever phase the moon is in--quarter, half, waxing, waning--if you draw a line from the tip of one bright point to the tip of the other, then it should point north.

Sunday, February 11, 2007

The Northern Lights

I had seen the Northern Lights (Aurora Borealis) only once before college. I remember laying in the driveway on a blanket next to a field of corn. They were distant, but frantic in their billowing curtain display of ivory shades.

Then I went to the Upper Peninsula and saw them with a frequency I may never again have the opportunity to experience. Reds, greens, whites, and even tints of purple appeared almost monthly above the cresting valley ridge on the other side of the canal.



But what causes these sporadic displays of electrical art? Well, it took me a long time to understand...so here goes:

The earth is surrounded by a magnetic field, originating from deep within its core. The field is strongest at its magnetic poles and weakest around the equator. The sun has a much larger magnetic field, which extends through the orbit of the earth. This field combined with fusion particles and radiation constitute solar wind.

Solar wind acts upon the earth's magnetic field in much the same way normal wind would act upon a pile of sand: the windward side is stretched and extended into the leeward side to create a tail like a melting comet.

The pressure exerted on the earth's magnetic field excites existing particles in the earth's atmosphere and actual creates a voltage gradient between the magnetic poles and the solar-blown "tail" of the earth's magnetic field.

This all takes place in the magnetosphere and as the voltage pushes the charged particles towards the poles, they amass and are pulled closer into the ionosphere. There, they react with ionosphere gases and the resulting reaction discharges visible electrical energy...light.

The stronger the solar wind, usually indicated by solar flares, or spastic jumps of solar activity beyond the sun's regular corona, the more brilliant the auroras.

Saturday, February 10, 2007

Winter

"No matter what you learn today, nine of you will go back to saying winter is caused by the earth being farther away from the sun," my high school science teacher told us. We were a class of ten.

While the elliptical orbit of the earth around the sun does cause it to be farther in some time periods, it does not fully account for those winter months.

The axis of the earth, the point around which it rotates, is tilted relative to the sun at about 23 degrees. A line drawn through the axis would point to the same position in space even as the earth moves around the sun.

So, as the earth revolves, different hemispheres are leaning either toward or away from the sun.

As a result, the sun's rays strike the earth at different angles. In summer, the angle is more direct, a sort of concentration of heat radiation. In winter, the angle is more obtuse, spreading the summer concentration over a larger area.

Suppose each yellow line represents 20 degrees Fahrenheit of the sun's heat energy. In summer, the small area receives 4 lines, about 80 degrees. In winter, a larger area receives the same energy that would have amounted to 80 degrees in the summer, but, being spread out, each locale is about 20 degrees. But remember, this is a very simplified explanation.

Parallax

One of the earliest arguments against the multi-dimensionality of outer space was parallax. It could've been the ruin of the Copernican Revolution.


To observe parallax on a small scale hold your hands out in front of your face with the left elbow bent at a right angle and the right elbow straight, but try to keep both hands at eye-level. Make certain there is a gap between your hands. Now, move your head to the left and watch the gap close and your right hand disappear. Voila, parallax! (Click pic.)

Parallax is the apparent shift in background (right hand) as the point of observation (head) relative to the observed object (left hand) moves.

Copernicus resurrected the heliocentric (sun-centered) model of our solar system, which was set to replace the geocentric (earth-centered) model. This, however, was difficult to prove given the unnoticeable parallax phenomenon. If the earth were moving, then how come the other planets' positions did not change relative to the stars? It should be mentioned that the stars were considered to be lined up on a single plane of their own, beyond the farthest known planet, Saturn.

Parallax wasn't proven until 300 years after Copernicus's model.

Another popular argument against the movement of planet Earth was the tower argument. Simply put, when a stone is dropped from the top of a tower, why doesn't it land many feet away from the base of the tower? After all, if the earth is moving, the ground beneath the falling rock would shift accordingly, causing it's impact to be a hypotenuse away from the tower's base...

The Gravity of Bended Space


It may not entirely have been gravity we were breaking with our expensive rockets or even our stepping feet. Theory suggests everything moves in a linear motion along a trajectory through space that is bent by mass. Though, physics' calculations requires a reconciliation of the two.

The simplest way to explain bended space is to imagine a large mattress covered in a thick quilt. It can be black if it helps. The surface represents the plane on which our planets revolve around the sun. Let some massive objects, like bowling balls, represent the planets and sun. The dip in the mattress caused by their sheer mass is bended space. The planets move linearly (straight) through space. It's just that the space is now bent, giving the "sense" of elliptical motion.

To prove this, we assume light, with linear motion, can be bent by mass. We know it is subject to some force because of black holes, which are said to be so massive, that not even light can escape it. Anyway, either light has mass (which actually may be the case) or it follows the curve in space, so says Einstein's warped space corollary in his General Theory of Relativity.

Now we can't really observe this in a laboratory test. Nothing we have has enough mass to produce any measurable influence on the path of light. Light may bend slightly around me, but it's nothing any of our instruments can detect.

So to test this theory, astronomer Arthur Eddington used the sun as his massive object and set to observe the stars around its edge. Of course, the sun's own brightness mutes the light from other stars, so Eddington waited for a solar eclipse to run his experiment.

The results showed that the stars appeared out of their usual position, as the light which allows them to be seen was distorted by the sun and made them appear elsewhere.

Gravity, or the attraction of bodies to each other, still can exist, though. Warped space simple is a way to explain gravitation. Well, it's either that or gravitons.

Finding Space

Photo Copyright NOA0 AURA
First, it was an absence of sky. Then, it was a tank of ether. Then, it was a complete void. Now, it may be filled and emptied with quantum byproducts.

Space is the final frontier, though not the only one yet undiscovered. Like withstanding 16,000 psi to reach the sea's bottom, we have generated crafts propelled by 300,000 pounds of thrust (Sputnik I) to reach beyond the edge of blue. And we've only begun to scratch the surface of what's beyond the beyond.

For as constant as space appears to us, it will always be ever-changing, molded by our knowledge and understanding and forever worthy of our attention.