{{asɛmtiNe Ɔkyerɛwfo}} | Nhomakorabea | Nneɛma a ɛma wotumi yɛ ade

Objectives of the Formative:

Students will be able to show knowledge and understanding of the sun and it's energy transfer to Earth.

Standards tested:

HS-ESS1-1.Develop a model based on evidence to illustrate the life span of the sun and the role of nuclear fusion in the sun’s core to release energy that eventually reaches Earth in the form of radiation.

1

Using the relative proportions of hydrogen and helium in a star we can predict it's age.

Nokorɛ

Ɛnyɛ ampa

1

What fuels the sun's energy?

Hydrogen

Helium

Oxygen

Carbon

HS-ESS1-1

1

In complete sentances, explain why the sun's radiation changes over time?

HS-ESS1-1

1

Draw a model showing the relationship between stars, their fuel source, and their byproducts,.

HS-ESS1-1

1

What is the expected lifespan of the sun?

10 Years

1 million years

1 billion years

10 billion years

HS-ESS1-1

Unit 1 Test

Unit 1 Test

Using the relative proportions of hydrogen and helium in a star we can predict it's age.

What fuels the sun's energy?

In complete sentances, explain why the sun's radiation changes over time?

Draw a model showing the relationship between stars, their fuel source, and their byproducts,.

What is the expected lifespan of the sun?

Using the relative proportions of hydrogen and helium in a star we can predict it's age.

What fuels the sun's energy?

In complete sentances, explain why the sun's radiation changes over time?

Draw a model showing the relationship between stars, their fuel source, and their byproducts,.

What is the expected lifespan of the sun?