Rocket sets the big ball on the table and holds the orange on its pencil in front of it. The lamp glows behind.
"Move the Moon between the Sun and Earth," Raven says. Rocket slides the orange in line. A small dark spot appears on the ball.
"Solar eclipse!" he says. "Only the spot sees it."
"Now swing it around behind," Raven says. Rocket does. The orange darkens in the ball's shadow. "Lunar eclipse."
Nova hovers above. "Now lift the Moon a little higher as it passes," she says.
Rocket lifts the orange a thumb's width. The shadow slides off into the air. Nothing is eclipsed.
"That is most months," Raven says. Nova hums. "A small tilt, a big difference."
Today you use last week's model to make a solar eclipse, a lunar eclipse and then a month with no eclipse.
The lamp is the Sun, the big ball is Earth and the small ball or orange on a pencil is the Moon.
Eclipses are modeled indoors in this course. We never watch the real Sun, eclipse or not.
| Moon position | Whose shadow falls where | Eclipse type | How much of Earth could see it |
|---|---|---|---|
| Between lamp and Earth, in line | |||
| Behind Earth, in line | |||
| Between lamp and Earth, lifted | |||
| Behind Earth, lifted |
The Moon's shadow on Earth was a small spot. OpenStax says a total solar eclipse is seen only inside a small area under the shadow's tip.
Earth's shadow swallowed the whole Moon. A lunar eclipse is visible to everyone who can see the Moon.
That is why a given place sees lunar eclipses far more often than solar eclipses, even though they happen about as often.
What the model gets wrong: the real Moon is about 30 Earth widths away. The real tilt is only about 5 degrees.
| What the model shows | True or false? |
|---|---|
| The Moon's shadow covered only a small spot on Earth. | ? |
| Earth's shadow could darken the whole Moon. | ? |
| Lifting the Moon a little made the eclipses bigger. | ? |
| The lunar eclipse happened with the Moon between the lamp and Earth. | ? |
Both eclipses made and missed. Tomorrow you read a table of how often and how long real eclipses happen.