Harvest Moon

harvestmoon The closest full moon to the autumnal equinox is called the harvest moon. The harvest moon is not necessarily bigger or brighter than a regular full moon. However, the moon’s orbital path is unique at this time of the year, and so it rises earlier than usual. Because of this, there is a shorter than usual time between sunset and the rise of the full moon, which means a nice, bright late evening sky.

Why does it look so big?

This is due to an optical illusion, the reason for which is still debated. Whenever the full moon is closer to the horizon, it appears to be much larger than when it is not. However, you can de-bunk this illusion very easily. Hold up a dime toward the full moon when it is near the horizon, and then a few hours later when it is farther up in the sky. You will notice that even though the moon appears larger when it is near the horizon, the dime will cover up the same amount of the moon in both positions. Another fun thing to try is to bend over and look at the full moon from between your legs. When you look at it from this position, it looks much smaller than when you look at it right side up!

Why is it called the “Harvest” moon?

Historically, the early brightness of this full moon helped farmers to gather their crops, despite the days getting shorter and shorter at this time of year. As the sun begins to set, the full moon rises, illuminating their fields. Save time on academic papers with research papers writer service. Today farmers rely on artificial lights to guide their tractors, but in the times before electricity, the harvest moon was a huge help.

Fall Equinox Activity

Here at Lie Back, Look Up, you will find plenty of stargazing and astronomy activities to do with your family. Many of these activities include free printables, as well as some tutorials and videos. Please let me know in the comments how your family has enjoyed these activities!

The autumnal equinox, occurring this year on September 22nd, is a great opportunity to help your kids explore why we experience seasons. The explanation behind the occurrence of seasons is one of the biggest misconceptions in astronomy. Many children believe that the Earth is closer to the sun in the summer and farther in the winter, thus the seasons. And while some children understand that seasons have to do with the tilt of the Earth, many still have trouble explaining how this results in seasons.

One of the greatest activities that I’ve done with my middle school students to help them understand this concept (as well as seasonal constellations) is “kinesthetic astronomy”. This involves using your bodies to model the objects and movements in the solar system. The original idea and complete lesson plan for this activity can be found here. You can modify this activity to focus only on the “reason for the seasons”, as explained below.

Reason for the Seasons

Begin by explaining that you will be using your bodies to model the Earth. The North Pole is at the top of your head, the South Pole at your tailbone, and the equator would be your waist. Use a basketball or other round object to model the Sun. Position yourselves so that you are facing the sun. Point out where your home would be on your body–  North America would be on your chest, so when you are facing the sun, North America is experiencing daytime. Explain that the Earth rotates on its axis, which would be an imaginary line, going straight up out of your head and straight down out of your tailbone. Model the Earth’s rotation on its axis by spinning counterclockwise. Model the Earth’s orbit (revolution) around the sun by traveling around the sun. Kids can have quite a bit of fun by rotating and orbiting at the same time!

Once your child understands those two basic motions, rotation and revolution, you can begin talking about the tilt of the Earth’s axis. The North Pole of the Earth’s axis is tilted toward the star Polaris, which is 500 light years away. Have your child tilt from their waist approximately 23.5 degrees from vertical. Now you can again practice rotating and revolving, but this time incorporating the tilt of the axis. This can be very tricky but a lot of fun! Remind your child that they must keep their bodies tilted toward Polaris the whole time. The direction of the tilt should not change as you rotate and revolve.

Have your child move through the Earth’s orbit around the sun slowly. Point out that at one point his or her chest is pointed toward the sun and at one point it is tilted away from the sun. Also, there are two in-between points in the orbit. You can also mention that the tilt of the Earth’s axis has not changed (it is always towards Polaris), but their orientation to the sun has changed because of the Earth’s tilt and revolution. When the Earth is tilted toward the sun we experience summer and when we are tilted away from the sun we experience winter. The two in-between points are fall and spring.

To explain why the tilt towards or away from the sun causes seasons, you can remove your object representing the sun and instead use a flashlight to represent the sun. Stand in the middle while your child orbits around you (with the tilt), and shine a flashlight at his chest. Have him stop when he is tilted toward the sun and look at the flashlight beam on his chest. It should be concentrated in a small circle. This shows that in the summer, the sun’s rays are very direct on the Earth. Next have him stop when he is tilted away from the sun and look at the flashlight on his chest. It should be spread out, which shows that in the winter, the sun’s rays aren’t as direct on the Earth. In the fall and spring positions, the Earth is in-between the positions of direct and indirect rays.

Here is a great interactive to test their understanding after the activity!



Why do we have “seasonal” constellations?

If you’ve been visiting Lie Back, Look Up for awhile (or any other stargazing sites), you’ve probably been reading about the different constellations that you can view each season. You might also be wondering why we see different constellations each season. Understanding this explanation involves visualizing the Earth-Sun relationship in our solar system, as well as our solar system’s position in the Milky Way Galaxy.

It is helpful to remember that the stars are always up in the sky, we’re just not able to see them during the day due to the brightness of the sun. Without the sun shining during the day, we would be able to see the winter constellations during the daytime in the summer (and vice versa). Because the Earth changes position around the sun throughout the year, we get a different view of the stars in the Milky Way Galaxy during different times of the year.

Looking at the drawing above, you can see that on December 21st, we are able to see the stars in the constellation Gemini at night. We would not be able to see the stars of Sagittarius on December 21st, because they would be in the daytime sky. If you are looking to explain this to your kids, it is a great idea to “act out” the drawing above. Print out pictures of the constellations in the drawing and place them around the room. Use a basketball to model the sun in the center. They can rotate to experience day and night, and walk around the sun to model the orbit throughout the year. Have them stop in different positions throughout the year, and ask them which constellations they would be able to see at night. They will have to spin around in their position to face away from the sun, in order to view the nighttime constellations.