Icy Moons Collection: 1. Europa

The Icy Moons Collection: 1. Europa

In this lesson, we will be focusing on Jupiter’s moon Europa, the ocean that lies beneath its icy surface and its potential as a habitat for life.

Reminder: Teachers’ notes, presentations and all content can be downloaded for adaptation and use in your classroom. Just don’t forget to credit us (see ‘Using the Resources‘).

Overview

Activity Outline: Understand geological processes that occur on Europa and how these affect the potential for life in this environment.

Age Range:

10-14

Equipment Needed:

  • Computer
  • Projector

Lesson Time:

45 Minutes (including 1 videos)

Topics Covered:

  • Chemistry
  • Geological processes
  • Biology (Life in extremes)
  • Astronomy

Learning Outcomes

After completing this activity, pupils will:

  • Understand the composition of Europa.
  • Explain the formation of the cracks on Europa’s surface.
  • Describe the nature of Europa’s subsurface oceans.
  • Understand extremophiles and life in space.

Introduction to Europa

Jupiter has at least 92 moons, some of which have diameters of less than 1 kilometre. Europa is the smallest of the four largest moons of Jupiter, known as the Galilean moons because they were discovered by Galileo Galilei in 1610. You see the four Galilean moons if you look through binoculars or a small telescope. 

Europa is the sixth largest moon in our Solar System, and is about the same size as Earth’s Moon. It has the smoothest known surface of any moon, with very few craters. In fact, Europa has the smoothest surface of any known object in our Solar System.

Uncovering Europa’s ice-covered secrets

Because, to date, we have limited data about Europa gathered by space missions, there are still many things we don’t know about this moon of Jupiter. The European Space Agency (ESA) mission, the Jupiter Icy Moons Explorer (JUICE), and NASA’s Europa Clipper mission will help change that. JUICE, which launched in April 2023, will arrive at Jupiter in 2031 and will make two flybys of Europa before going into orbit around Ganymede. Europa Clipper, which will launch in 2024 and reach Jupiter in 2030, will make over 50 flybys of Europa.

The internal structure of Europa is thought to be a metallic core, surrounded by silicate rock, which together account for the majority of the moon’s mass. This is covered by a global, liquid water ocean, beneath a thick icy crust. The temperatures on Europa are extremely cold (- 220 degrees Celsius to – 160 degrees Celsius).

Europa’s surface

Despite its unusual smoothness, the surface ice of Europa is marked with long, thin, parallel streaks or stripes. These stripes are actually cracks, referred to as lineae. The lineae are caused by tidal heating. Europa’s orbit of Jupiter is not perfectly circular, so there are times when the two bodies are closer or further away from each other. In the same way as the gravitational pull of the Moon causes Earth’s oceans to bulge out on either side, the intensity of Jupiter’s gravitational pull on Europa stretches and compresses the entire moon at different points during its orbit. This deformation cracks the icy crust, forming the lineae.

Clues from the lineae

Material from the ocean below and within the icy crust can seep out through the lineae to the moon’s surface. This is important because it indicates that there is transfer of material between the ocean and the crust. Therefore, although space missions to date (including JUICE and Europa Clipper) can’t access the ocean directly, analysis of the material seeping through the lineae can give us a very good indication of the ocean’s composition and density.  

Chaos terrain

Regions of Europa’s surface that are particularly cracked are known as ‘chaos terrain’. These areas are particularly interesting for studying material that has seeped through from the sub-surface ocean. The blue-white terrains indicate relatively pure water ice, whereas the reddish areas contain water ice mixed with hydrated salts, potentially magnesium sulphate or sulfuric acid. Jupiter’s huge magnetic field traps high energy particles, creating powerful radiation that constantly bombards the surface of Europa. The interaction of high energy particles ‘weathers’ the moon’s surface by driving chemical reactions and altering the physical properties of the ice, such as grain size.

Subsurface ocean

Europa is unique and interesting as a moon. Past missions have shown that Europa has a magnetic field that is generated by some kind of conductive fluid beneath the icy crust. Measurements of Europa’s magnetic field, the moon’s density (derived from its size and gravitational field), and analysis of the properties of its surface ice indicates that Europa has a subsurface ocean of salty water that is more acidic than terrestrial seawater. Although temperatures at Europa are very cold, an ocean of liquid water could be sustained because salt lowers the freezing point of water. The salty ocean is in contact with the rocky shell around Europa’s core. This is interesting to scientists as the interaction between salty water and rock in the ocean is similar to that suggested by the “primordial soup” concept for the emergence of life on Earth, whereby organic molecules were mixed in ancient bodies of water, assembling to form living organisms. 

Extremophiles

Extremophiles are organisms that can survive in extreme climates. Any organisms on Europa would probably need to be able to survive in extremely cold temperatures. However, hydrothermal vents in the ocean could also create microcosms that could support life, just like on Earth. Around vents, the temperatures could be significantly higher than in the surrounding ocean – these environments could be very hot! Thus, although the surface of Europa is very cold, within the moon’s oceans it could be fairly temperate.

Potential for life

In small groups, discuss whether you think there is life on Europa and if so what sort of adaptations and features would you expect it to have. 

  • Would life just be microorganisms, or could larger forms of life might have evolved?
  • What kind of metabolic processes might they have?

Remember, we need to wait for JUICE and Europa Clipper to arrive at Jupiter to find out more about Europa, and may still need to send future missions to definitively answer the question of whether there is life beneath the icy surface. For now, there are no right or wrong answers!

Additional Activities

Ask your class to write an essay arguing the case as to whether we might find life (giving sources of information) or draw what they think life might look like on Europa – we’d love to see their ideas.


Sources

For more information, see the following sources:

Europa in Depth (NASA): https://solarsystem.nasa.gov/moons/jupiter-moons/europa/in-depth/

Juice Mission (ESA): https://www.esa.int/Science_Exploration/Space_Science/Juice

Europa Clipper (NASA): https://europa.nasa.gov

Europa’s core, mantle and water shell (Geo Girl): https://www.youtube.com/watch?v=dJ-biPZG8Jw

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Новости Омутнинск Любовь и семья Общество Люди и события Красота и здоровье Дети Диета Кулинария Полезные советы Шоу-бизнес Огород Гороскопы Авто Интерьер Домашние животные Технологии Рекорды и антирекорды