Astronomy 3

 

Transcript

Under a dark sky, you can see thousands of stars. If you watch for a few hours, you can

see them rise and set as the Earth rotates once a day.

And if you go outside the next night at the same time, you’ll see that things’ll look

pretty much the same as they did the night before. The stars rise and set, Polaris hangs

to the north, and so on.

One day hardly makes any difference to the sky’s appearance.

But what if you wait for another night? Or a week? If you’re that patient, and observant,

you can spot subtle changes in the sky.

Let’s say a couple of weeks have passed. Remember that star that was just over a tree

in the east when the Sun set -- the one that made you first notice the stars are rising

and setting? Go look at it again.

If you happen to be out at the same time, you’d expect that star to be in the same

place. But it’s not. It’s actually a bit higher above the tree. And if you look west,

stars that were well off the horizon just after sunset last week are now lower.

If you wait a month, this effect is even more pronounced; all new constellations will be

visible in the sky after sunset. This is because the Earth is going around the Sun, literally

changing our viewpoint on the sky.

The Earth takes a year to orbit the Sun once. Every day, it moves a little bit along its

orbit. And as it does, from Earth’s perspective, distant stars appear to move their positions

relative to the sun. So, one day we might see a star very near the Sun, but the next

day the angle is a bit bigger.

At some point, about six months after we first saw it, the star is directly opposite the

Sun in the sky. Then the angle starts to shrink again as the star approaches the Sun from

the opposite side, until, after a full year, the cycle repeats.

What this means to you, the naked eye observer, is that the stars appear to rise and set at

different times over the course of the year. Stars in the east rise about four minutes

earlier every night, and stars in the west set four minutes earlier. A constellation

that was entirely below the eastern horizon at sunset one month might be completely visible

after sunset the next month.

Another way to think about it is that the stars appear to be fixed, and as the Earth

circles the Sun, the Sun moves through the stars over the course of the year, making

a complete circle around the sky once per year.

The path it takes is a reflection of the Earth’s path around the Sun, a line in the sky. We

call that line the ecliptic.

That means the Sun passes through the same constellations in the sky every year. We give

those constellations a special name: the zodiac. Every year, during a given month, the Sun

will appear to be in a certain zodiacal constellation, from Sagittarius through Scorpius, Libra,

Virgo, Leo, Cancer, and the rest.

Eventually, over a year, the Sun returns to Sagittarius, and the cycle starts again. But

even though we talk about this process in terms of the sun’s movement, it’s really

the path traveled by the Earth that creates this effect, as our perspective moves with it.

And of course, the planets move in the sky as well. Mercury, Venus, Mars… they orbit

the Sun, too, and they do so in approximately the same plane the Earth does. If you could

see the solar system from the side, it would look flat!

So to us, on Earth, the planets go around the sky over the course of a year, and they

also appear to change their positions relative to the Sun and the stars.

The inner planets, Mercury and Venus, move so rapidly you can see their motion after

a single night. The outer planets are more leisurely, but wait long enough and they too

will be seen to move, sliding through the constellations.

By the way, the word “planet” is Greek for “wanderer."

There’s another aspect of all this you might notice over time.

You’ve probably seen a globe, and noticed that the axis of it is tilted; that is,

it’s not straight up-and-down, perpendicular to how it sits. That’s because a globe is

modeling the Earth and the Earth is tilted.

The Earth spins on its axis once per day, and orbits the Sun once per year. But the

Earth’s axis is tilted with respect to its orbital plane by 23.5 degrees. And this has

a profound effect on our planet.

Imagine for a moment that the Earth’s axis were exactly perpendicular to its orbit, straight

up and down. If that were the case, every day, the Sun would take the same path across

the sky. If you were on the equator the Sun would rise, go exactly overhead, and then

set. If you’re on the pole, the Sun will appear to go around the horizon every day,

neither rising nor setting — it would always be twilight.

But that’s not the case. The Earth is tilted. In the months of June and July, the Earth’s

north pole is tipped toward the Sun. Six months later it’s pointed away. This affects the

path the Sun takes across our sky.

Instead of it taking the same path every day, in the northern summer, when we’re tipped

toward the Sun, the Sun takes a higher path in the sky. Because that path is longer,

the days are longer, too.

Six months later, in December and January, the Earth’s pole is tipped away. The Sun

takes a lower path in the sky, and because the path is shorter days are shorter too.

That’s why we have seasons! When the Sun is up high in the sky it shines straight down

on the ground, heating it better, and days are longer so it has more time to heat us

up. It gets hot.

In the winter, it’s the reverse: The Sun is lower so it can’t warm us up as efficiently,

and it has less time to do so. It gets cold.

There you go: seasons. The Earth’s axis is tipped. If it weren’t, the seasons wouldn’t

occur, and the temperature of the Earth wouldn’t change month to month.

There’s a common misconception that the Earth has seasons because it orbits the Sun

on an ellipse, and so it’s closer to the Sun in summer and farther in winter. While

it’s true the orbit is elliptical, Earth is closer to the sun in January -- on the

order of 5 million kilometers or so -- than it is in July. It’s the angle of the sun’s

rays that makes winter cold and summer hot, not our distance from the sun.

Also, you may know that when it’s summer in the northern hemisphere, it’s winter

in the southern. When the north pole is tipped toward the Sun, the south pole is tipped away,

so northern and southern hemisphere seasons are opposite each other.

But nothing in astronomy is permanent. The north pole’s not always going to point toward

the sun in June, and Polaris is not always going to be the North Star.

That’s because our planet’s axis is actually moving.

Have you ever seen a spinning top start to wobble, its axis moving in a slow circle even

as the top itself spins? This is called precession, and the Earth does it too! Our planet spins

on its axis once per day, but the axis wobbles, making a very slow circle that takes

This affects a lot of what we see in the sky. For example, Polaris won’t always be the

pole star! Every year, the pole points a little farther from that star, making a big circle

about 11,000 years that position will be held by the bright star Vega.

Also, the date the Sun is in a particular zodiac constellation changes slowly due to

precession as well. When the ancients first thought up this idea, the Sun was in Aries

on March 22, the vernal equinox (what some people call the first day of spring). But

due to precession, it’s now in Pisces! That’s why your astrological sign doesn’t match

where the Sun actually is in the sky; 2000 years of precession has changed them…one

of the many reasons astrology is silly.

It’s incredible to think about: The Earth, the Sun, the stars: they allow us to tell

the time and time of year just by looking up and paying attention. This is why the stars

were so important to ancient humans. The stars were like a clock and a calendar in the sky,

long before we had invented either.

We’ve actually learned a lot about the sky just by looking at it. Of course, some of

the stuff I’ve explained we’ve learned through other means – the Earth is spinning,

stars have different intrinsic brightnesses, and so on. But all of that knowledge, and

far more, got its start by people who went outside and looked up. Later, as we applied

math and physics to what we observed we learned even more, and could then go back

and explain what we saw.

So don’t discount naked eye astronomy; it’s all we had for thousands of years.

In fact, I think we lost something when we started using clocks and calendars, and moving

to cities with bright lights that washed away the stars from the sky. Those folks long ago

were tied to the sky; they knew it like you know the streets in your neighborhood. They

could see the stars rise and set, they knew the glory of the Milky Way sprawled across

the heavens, even if they didn’t know exactly what it was.

We do know, now, with our knowledge gained over the centuries. But it comes at the cost

of losing touch with the sky, not living under it as much as we once did. I’ve spent thousands

of hours over my life at night just simply looking up, watching the stars, appreciating

the Universe as I can see it. The things I have witnessed have shaped my life, and instilled

in me a permanent and endless sense of wonder and joy.

The Universe belongs to everyone. Go outside and, if you can, soak up your share.

Today we talked about cycles: As the Earth goes around the Sun we see stars rising and

setting at different times, the Sun moves along a line in the sky called the ecliptic,

through a set of constellations called the zodiac — really a reflection of the Earth’s

motion around the Sun — that the planets move more or less along the ecliptic as well,

and that seasons are caused by the tilt of the Earth’s axis together with its annual

orbit around the Sun.

Crash Course is produced in association with PBS Digital Studios. This episode was written

by me, Phil Plait. The script was edited by Blake de Pastino, and our consultant is Dr.

Michelle Thaller. It was co-directed by Nicholas Jenkins and Michael Aranda,

and the graphics team is Thought Café.