Command Module

Sections:

FACTS ABOUT SPACE

1. Moon craters            2. Cosmic Rays          3. Messier's list
4. Meteors                   5. Parsecs                6. Stars from the moon
7. Billions and billions      8. Lunar eclipses       9. How long is a day?
10. Moon rotation          11. Earth's rotation   12. Earth's revolution


1.
Did you ever wonder why there are so many craters on the moon, but so few on earth?

In the early solar system the earth was bombarded with just as many asteroids as the moon was. The difference is that the earth has water and an atmosphere. Over the years the wind and water gradually weathered away any signs of those original craters. The moon has no atmosphere and no water, so once a crater forms there, it lasts forever.

2. Cosmic rays from space are always hitting the earth! But what are cosmic rays?

Cosmic rays come mainly from exploding stars, known as supernovas. When these stars explode they eject pieces of atoms that travel through space at the speed of light. Fortunately, our atmosphere shields us from most of these deadly rays. But next time you go into space, watch out!

3. Did you ever hear of galaxies and other space objects described as M1 or M86 and wonder what the "M" stands for?

The "M" stands for Messier, who was a French astronomer in the 1700's. He prepared a list of faint astronomical objects known as "Messier's list". The objects on the list were galaxies, nebulas, and globular clusters, but Messier didn't know that at the time. He didn't know what they were. So he just numbered them (M1, M2, etc.). Now we know that M1 is the Crab nebula and M86 is a galaxy in Ursis major. However, many objects on the list are still referred to by their "M" number.

4. Rocks from space are sometimes called meteors and sometimes called meteorites. Which is correct?

It depends on where the rock is. If it's burning up in the atmosphere, like during a "meteor" shower, it's called a meteor. But if it survives its journey through the atmosphere and is found on the ground, it's a meteorite. What if it's flying through space? That would be a called a meteoroid.

5. On Star Trek they're always talking about distance in "parsecs". What is a parsec?

A parsec is 3.26 light years (the distance light would travel in 3.26 years). The word parsec stands for "parallax second". Parallax is a method of estimating the distance of a star from earth by viewing it from two different spots in the earth's orbit and measuring the difference in the angle to the star. A star is one parsec away if the difference in the angle is one "second" of arc, which is equal to less than one-millionth of a circle.

6. Would the star constellations look different if you were on the moon?

The answer is both yes and no. All the stars that can be seen from earth would be visible from the moon, but since the moon has no atmosphere you would see twice as many stars. The major features of the constellations could still be made out, but the finer details would be completely obscured by all of the additional visible stars. So the night sky would look very different.

7. As Carl Sagan liked to say, there are billions and billions of stars in a galaxy, and billions and billions of galaxies in the universe. But exactly how many is a billion?

The answer seems obvious. A billion is a thousand millions, or a 1 followed by 9 zeroes (1,000,000,000). But someone from England or Germany would disagree. In those countries a billion is a million millions, or a 1 followed by 12 zeroes (1,000,000,000,000). If you're like most people and find this hard to believe, just look up the word "billion" in the encyclopedia and see for yourself!

8. A lunar eclipse occurs when the moon, in its orbit around the earth comes between the sun and the earth, casting a shadow on the earth. If this is true, then why isn't there a lunar eclipse every month?

There would be an eclipse every month if the moon orbited around the earth in the same plane that the earth orbits the sun. But it doesn't. The moon's orbit is tilted by a little over 5 degrees relative to the earth's orbit. Therefore, an eclipse only occurs when the intersection of the orbital planes (the "nodes") happen to be in the earth-sun line.

9. Everyone knows that a day is 24 hours, right? But that depends on what you mean by a day.

The "solar" day, the time from when the sun appears in the same spot overhead, averages 24 hours. But since the earth's orbit is elliptical, the day is slightly shorter when the earth is closer to the sun (and is consequently moving faster) and is slightly more than 24 hours when the earth is at its farthest point. However, the day can also be measured by the position in the sky of a particular star. This is called the "sidereal" day, and it's only 23 hours, 56 minutes long. Why is the sidereal day shorter than the solar day? Because in the time it takes for the earth to rotate, the earth has moved a little in its orbit around the sun.

10. Why do we only see one side of the moon?

A long time ago the moon did rotate, and although there were no humans to see it, all sides of the moon were visible. However, over time the pull of the earth's gravity gradually slowed down the moon's rotation until finally only one side faced the earth. The reason this happens is that the earth's gravitational pull on the near side of the moon is greater than on the far side. This uneven pull slightly distorts the moon's shape and causes friction as it rotates. These "tidal forces" are what cause the rotation to slow down.

11. Are days getting longer?

Surprisingly, the answer is yes! But it's not noticable. Scientists estimate that the Earth's rotation is slowing down at a rate of only 2.2 seconds every 100,000 years.
The gravity of the moon, the same force that causes the tides, is gradually slowing the earth's rotation. Eventually it will stop, for the same reason that the moon's rotation long ago ceased. Interestingly, at the same time, due to something known as the "Law of Conservation of Angular Momentum", the earth and moon are also getting farther apart.

12. Why does the earth revolve around the sun instead of vice versa?

It has to do with the fact that the mass of the sun is greater than the mass of the earth. To be technical, the earth does not actually revolve around the sun. Both the earth and the sun revolve around the center of gravity of the earth-sun system. It appears that the earth revolves around the sun because the sun is so much more massive. Consequently, the center of gravity is actually inside the sphere of the sun (but not at its center). The sun revolves around this point, tracing out a small circle. When this type of "wobble" is detected when observing other stars, it is an indication that the star has a planet revolving around it.


 
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