### 第1段

1 .<-NARRATOR:->Listen to part of a lecture in an astronomy class. You will not need to remember the numbers the professor mentions.

### 第2段

1 .<-MALE PROFESSOR:->OK. Let's get going. Today I'm going to talk about how the asteroid belt was discovered. And... I'm going to start by writing some numbers on the board.

2 .Here they are; We'll start with zero, then 3, ... 6, ... 12. Uh, tell me what I'm doing.

### 第3段

1 .<-FEMALE STUDENT:->Multiplying by 2?

2 .<-MALE PROFESSOR:->Right, I'm doubling the numbers, so 2 times 12 is 24, and the next one I'm going to write after 24 would be...

### 第4段

1 .<-FEMALE STUDENT:->48

### 第5段

1 .<-MALE PROFESSOR:->48 [slowly, as if just being calculated and written on the board]. Then 96 [slowly, as if just being calculated]. We'll stop there for now. Uh, now I'll write another row of numbers under that. Tell me what I'm doing.

2 .4, 7, 10... How am I getting the second row?

4,7,10……第二组数字我是怎么得到的？

### 第6段

1 .<-MALE STUDENT:->Adding 4 to the numbers in the first row.

### 第7段

1 .<-MALE PROFESSOR:->I'm adding 4 to each number in the first row to give you a second row. So the last two will be 52, 100, and now tell me what I'm doing.

### 第8段

1 .<-FEMALE STUDENT:->Putting in a decimal?

### 第9段

1 .<-MALE PROFESSOR:->Yes, I divided all those numbers by 10 by putting in a decimal point.

2 .Now I'm going to write the names of the planets under the numbers. Mercury... Venus... Earth... Mars.

3 .So, what do the numbers mean? Do you remember from the reading?

### 第10段

1 .<-MALE STUDENT:->Is it the distance of the planets from the Sun?

### 第11段

1 .<-MALE PROFESSOR:->Right. In astronomical units - not perfect, but tantalizingly close.

2 .The value for Mars is off by... 6 or 7 percent or so. It's... but it's within 10 percent of the average distance to Mars from the Sun.

3 .But I kind of have to skip the one after Mars for now.

4 .Then Jupiter's right there at 5-point something, and then Saturn is about 10 astronomical units from the Sun.

5 .Um, well, this pattern is known as Bode's Law.

### 第12段

1 .Um, it isn't really a scientific law, not in the sense of predicting gravitation mathematically or something, but it's attempting a pattern in the spacing of the planets, and it was noticed by Bode hundreds of years ago.

2 .Well, you can imagine that there was some interest in why the 2.8 spot in the pattern was skipped, and um... but there wasn't anything obvious there, in the early telescopes.

3 .Then what happened in the late 1700s? The discovery of...?

### 第13段

1 .<-FEMALE STUDENT:->Another planet?

### 第14段

1 .<-MALE PROFESSOR:->The next planet out, Uranus - after Saturn. And look, Uranus fits in the next spot in the pattern pretty nicely, um, not perfectly, but close.

### 第15段

1 .And so then people got really excited about the validity of this thing and finding the missing object between Mars and Jupiter.

2 .And telescopes, remember, were getting better. So people went to work on finding objects that would be at that missing distance from the Sun, and then in 1801, the object Ceres [SI-reez] was discovered.

### 第16段

1 .And Ceres was in the right place - the missing spot.

2 .Uh, but it was way too faint to be a planet. It looked like a little star. Uh, and because of its star-like appearance, um, it was called an "asteroid".

3 .OK? "Aster" is Greek for "star", as in "astronomy".

4 .Um, and so, Ceres was the first and is the largest of what became many objects discovered at that same distance.

5 .Not just one thing, but all the objects found at that distance form the asteroid belt.

6 .So the asteroid belt is the most famous success of this Bode's Law.

7 .That's how the asteroid belt was discovered.