Moon and Tides Lab teaching notes

For middle school Earth science teachers, co-op leaders and parents. Phases in one period, a period each for eclipses and tides, what students get wrong and where the app answers it, what the model leaves out, and the sheet and the setup.

Using this with a class? Make a free class and add your students yourself: each gets a username and password, with no email or Google account needed. Or give them one join code. Using Google Classroom? Post the link there; with a free class, the link also puts each student in your class, so you see their work. mytekDev is also available from the Google Workspace Marketplace, so your school's Google admin can install it for everyone.A first lesson: One period for phases: predict what makes the Moon change shape, drag it round, test the Earth's-shadow idea, and predict again. A second period for eclipses, and a third for tides where your state teaches them.

Set up a free class Share to Google Classroom
Put this on your class site

Students can use Moon and Tides Lab right on your page, with no account. What they make stays on that page; to keep their work, they make a free account.

Google Sites: Insert, then Embed, then By URL, and paste this address.

https://mytekdev.com/try/moontideslab?embed=1

Canvas, a blog, or any page that takes HTML: paste this code where you edit the page as HTML.

<iframe src="https://mytekdev.com/try/moontideslab?embed=1" width="100%" height="640" style="border:0" allow="fullscreen" title="Moon and Tides Lab demo from mytekDev"></iframe>

About these notes

Moon and Tides Lab shows one moment two ways: the Earth and Moon from far above the North Pole, and the sky from a beach where a small person on the Earth is standing. Drag the Moon and the Moon over the beach changes shape; drag the person and the clock turns. Three chapters, Phases, Eclipses and Tides, each open with a prediction that is saved and asked again at the end.

It is written for MS-ESS1-1: develop and use a model of the Earth-sun-moon system to describe the cyclic patterns of lunar phases, eclipses of the sun and moon, and seasons. Its evidence statement asks students to predict the phase from the positions, the positions from a phase, and whether an eclipse will be seen from a place, and to name the model's scale limits. Those are the app's puzzles, and every view says what is not to scale. Seasons are not in this version.

Phases in one period

  1. Predict (3 minutes) Everyone picks what they think makes the Moon change shape: Earth's shadow, something covering it, or how much of its lit half we see. About half of people pick the shadow. Do not correct anyone yet.
  2. Drag to the half Moon (7 minutes) The guide sends them to drag the Moon a quarter of the way round. The crescent over the beach grows into a half Moon, high in the sky at sunset. The yellow and blue arcs mark the half lit by the Sun and the half facing Earth; the overlap is what we see.
  3. Test the shadow idea (10 minutes) On to full Moon, then Earth's shadow on. It points straight away from the Sun. Drag back to a crescent: the shadow is nowhere near it, and the Moon still has a shape. Everyone answers the question again.
  4. Turn the Earth (10 minutes) Drag the person round. The phase does not change in a night; where it is does. Try the Moon in the daytime and the same night in Sydney.
  5. Puzzles (10 minutes) Name the phase from above, place the Moon to make a picture, and set the clock to the moment a full Moon rises.
  6. Exit question (5 minutes) Why is it not Earth's shadow that makes the Moon change shape?

Eclipses, a second period

Open the Eclipses tab. The picture from above gets a side view under it, with heights to scale and distances squeezed (it says how many times). The guide asks whether there is an eclipse of the Moon every month, sends them to press Next full Moon three times, then to lay the orbit flat (every full Moon is now an eclipse) and back. The year strip shades the eclipse seasons. Things to try find a total eclipse of the Moon and an eclipse of the Sun seen from your place.

Every solar eclipse card in the app carries the safety lines: eclipse glasses made to ISO 12312-2, never sunglasses, a pinhole viewer with your back to the Sun, bare eyes only during totality, and never a camera, binoculars or a telescope without its own solar filter on the front.

Tides, a third period where your state teaches them

Tides are not in NGSS MS-ESS1-1, but Texas (TEKS 6.9B), Virginia (SOL 6.3), Florida and New York teach them with the Moon. The Tides chapter starts on an ocean planet: arrows show the Moon's pull at each place less its pull on the Earth's middle, the ocean stretches into two bulges, and a beach turning through a day gets two high tides. The Sun's pull and a month on the graph show spring and neap tides. Then Real coast picks a NOAA station: Boston's two equal tides, San Francisco's two unequal ones, Pensacola's one a day, Eastport's five meters.

The tide on an ocean planet is about half a meter at most. Real coasts are often much bigger and their timing is set by the shape of the ocean, so the Real coast curve comes from NOAA's measured numbers, not from the bulges. On once-a-day coasts like Pensacola the biggest tides follow the Moon's distance north or south of the equator rather than its phase, and the app says so there.

What students get wrong, and where the app answers it

What students sayWhere the app answers it
Phases are Earth's shadowThe shadow switch points away from a crescent and a half Moon; the prediction is asked before and after
Phases and eclipses are the same thingPhases first, then the Eclipses chapter: the shadow only matters at the crossing points
Australia sees a different phase tonightThe same night in Sydney: the same phase, turned over
The far side of the Moon is darkA marked crater always faces Earth; the far side is lit at new Moon
The Moon is only out at nightA half Moon in the afternoon sky, a third quarter Moon in the morning
There should be an eclipse every monthThe side view, eclipse seasons, and the flat orbit switch
Everyone sees a solar eclipseEarth seen from the Sun: a small dark spot of totality inside a wider partial shadow
One high tide a day, under the MoonThe far bulge and the arrows; the beach turns through two highs
Tides are the wind and the wavesA month of a real station's tide lined up with the Moon's phases
The Moon is close to the EarthReal distance: 30 Earth-widths away

What the app simplifies, on purpose

Middle school and high school

Middle schoolHigh school
PhasesPhase names, percent lit, low or high in the sky, rise and set timesThe angle from the Sun, the phase angle, the lit-fraction formula, altitude and azimuth
EclipsesAbove or below the shadow, who can see itThe Moon's height in degrees, how far the shadow misses Earth's middle, the umbra's size
TidesMeters above or below average, spring and neapOne over distance cubed, the Sun's share, a station's tide constituents and its form factor

The sheet, the puzzles and the setup

The Sheet in the app's header is the student's write-up: a picture, their predictions before and after in each chapter, the puzzles solved, their Moon log, and questions with the standard each serves. They hand it in and it saves with the project; Print makes a paper copy. The eight Puzzles are checked by the app itself, never by a typed answer.

Setup is for you: the level, which chapters students can open (Phases is always on), whether the guide is on, one place for the whole class, whether real dates are allowed, the sheet's questions and up to ten of your own. Print answer key gives every puzzle's answer and what a good answer to each question says. Press Done, save, and hand the project out as the starter.

Standards

More help

Is something on this page wrong or not clear? Write to us.

Page last reviewed November 2026.
Google, Google Classroom and Chromebook are trademarks of Google LLC.