Want to create interactive content? It’s easy in Genially!

Get started free

Formation of the Earth-Moon System

Edward Hasselberg

Created on October 23, 2025

Start designing with a free template

Discover more than 1500 professional designs like these:

Animated Chalkboard Presentation

Genial Storytale Presentation

Blackboard Presentation

Psychedelic Presentation

Chalkboard Presentation

Witchcraft Presentation

Sketchbook Presentation

Transcript

Formation of the Earth-Moon System

Accretion

Small fragments of rocky material called planetesimals stick together = accretion

Accretion

Larger and larger pieces came together to form the terrestrial planets.

Accretion

The leftovers became asteroids and comets. Collisions between the planets and leftover planetesimals were common.

Moon

How did the moon form?An asteroid the size of Mars (Theia) collided with the early fully formed Earth. (Impact-Ejection hypothesis)

Theia colliding with Earth

Occurred 100 million years after the Sun was born.

Impact Ejection Hypothesis

Debris filled the space around the earth and formed a ring of debris

Moon

Ring then went through accretion to form the moon.

This could explain spin of the Earth.

The Moon is gradually moving further and further away

Syzygy

It takes 27.3 days for the Moon to travel completely around the Earth.

However, the Earth and Moon have also moved together around the Sun during that time.

Two more days must pass before the Moon, Earth, and Sun are lined up again.

Sidereal month = 27.3 days Synodic month = 29.5 days (Full moon to Full moon) Syzygy means 3 celestial bodies in a line.

Synchronous Rotation

It revolves around the Earth in the same amount of time

The moon rotates on its axis every 27.3 days

Caused by Earth’sgravity

Synchronous Rotation

It revolves around the Earth in the same amount of time

The moon rotates on its axis every 27.3 days

Caused by Earth’sgravity

Synchronous Rotation

Therefore, the same side of the Moon is always facing the Earth

Due to slight variations 59% of the moon’s surface is visible over time.

Perigee – point of moon being closest to the Earth during its orbit

Apogee – point in its orbit furthest from Earth

moon types

moon illusion

Harvest moon

blue moon

the moon appears larger near the horizon than when it is high in the sky
Full moon nearest the time of the autumnal equinox
when 2 full moons occur in the same calendar month. Occurs every 2.72 years

+info

+info

+info

Formation of the Earth-Moon System

Earth Days

When the earth first formed, each day lasted for about 6 hours.

Earth days are getting longer and longer (fewer days in a year)

The earth is slowing down because of the forces of gravity between the Earth, Moon, and Sun. No evidence to suggest that the time period for one revolution has changed

Moon Phases

Moon Phases

Moon Phases

Moon Phases

Moon Phases

Moon Phases

Moon Phases

Moon Phases

Moon Phases

Tides

The gravitational pull of the moon and sun on the oceans causes the tides.

The water and solid earth are stretched but the water stretches more because it flows more easily.

There are two bulges or tides on the Earth at once. One pointing towards the moon and the other on the opposite side of the earth.

Gravitational pull of the Sun

Much larger mass than the moon, but much further away

Therefore, the sun does not affect the tides as much as the moon.

The moon exerts 2.4 times stronger tide-producing force than the sun

Tides

2 high tides and 2 low tides occur each day.

Moon rises and sets about 50 minutes later each day

Due to fact that the moon is revolving around the Earth

This causes each tide to occur 25 min. later than the previous one

Formation of the Earth-Moon System

Spring Tide

The highest of the high tides.

Low tides are lower than normal

This occurs during the new and full moon phases.

The gravitational pull of the Sun and Moon are parallel to each other.

Neap Tide

The lowest of the high tides.

Low tides are higher than normal

This occurs during the first quarter and third quarter moon phases

The gravitational pull of the Sun and Moon are perpendicular to each other.

Tidal Cycle

The tide is like an ocean wave High and low tides travel around the Earth twice per day

This wave lags behind the Earth’s rotation This causes the time of the high tide to not coincide directly to when the moon is directly overhea

The friction of this lag gradually slows the Earth’s rotation

The tidal bulge also causes the moon to move away from the Earth a few centimeters a year

Tides

Agenda:

1. Earth Moon Warm up 2. Notes - Phases of the Moon 3. Phases activity

Learning Target:I will be able to understand the difference between waning and waxing.

¿Tienes una idea?

Usa este espacio para añadir una interactividad genial. Incluye texto, imágenes, vídeos, tablas, PDFs… ¡incluso preguntas interactivas! Tip premium: Obten información de cómo interacciona tu audiencia:

  • Visita las preferencias de Analytics;
  • Activa el seguimiento de usuarios;
  • ¡Que fluya la comunicación!

Agenda

The Moon

1. EdPuzzle Intro 2. Notes 3. Moon Activity

Agenda:

1. Moon Phases Warm Up 2. Notes - Finish Tides the Moon 3. Phases activity

Learning Target:I will be able to understand the difference between waning and waxing.

Agenda

The Moon

1. EdPuzzle Intro 2. Notes 3. Moon Activity

Agenda

The Moon

1. EdPuzzle Intro 2. Notes 3. Moon Activity

¿Tienes una idea?

Usa este espacio para añadir una interactividad genial. Incluye texto, imágenes, vídeos, tablas, PDFs… ¡incluso preguntas interactivas! Tip premium: Obten información de cómo interacciona tu audiencia:

  • Visita las preferencias de Analytics;
  • Activa el seguimiento de usuarios;
  • ¡Que fluya la comunicación!