Origins of the Universe

Origins of the Universe

Assessment

Flashcard

Science

8th Grade

Hard

NGSS
HS-ESS1-2, HS-ESS1-4, HS-PS2-1

Standards-aligned

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15 questions

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1.

FLASHCARD QUESTION

Front

What is the significance of the light we see from celestial objects?

Back

The light we see from celestial objects is from the past, as it takes time for light to travel from these objects to Earth.

2.

FLASHCARD QUESTION

Front

What theory explains the origin of the universe and its initial expansion?

Back

The Big Bang Theory explains that the universe began a tremendous expansion approximately 13-15 billion years ago.

Tags

NGSS.HS-ESS1-2

3.

FLASHCARD QUESTION

Front

How does the density of the universe change over time according to the Big Bang Theory?

Back

According to the Big Bang Theory, the universe changes from more dense to less dense over time.

Tags

NGSS.HS-ESS1-2

4.

FLASHCARD QUESTION

Front

Who was the first scientist to provide observational evidence for the expansion of the universe?

Back

Edwin Hubble was the first scientist to present observational evidence that supported the expansion of the universe, known as redshift.

Tags

NGSS.HS-ESS1-2

5.

FLASHCARD QUESTION

Front

What is Cosmic Microwave Background Radiation (CMBR) and its significance?

Back

CMBR is the residual microwave radiation observed everywhere in the universe, believed to be radiation left over from the rapid expansion of matter during the Big Bang, serving as evidence for the Big Bang Theory.

Tags

NGSS.HS-ESS1-2

6.

FLASHCARD QUESTION

Front

What does the term 'redshift' refer to in the context of the universe?

Back

Redshift refers to the phenomenon where light from distant galaxies is shifted towards the red end of the spectrum, indicating that those galaxies are moving away from us, supporting the idea of an expanding universe.

Tags

NGSS.HS-ESS1-2

7.

FLASHCARD QUESTION

Front

What evidence supports the Big Bang Theory besides CMBR?

Back

Other evidence supporting the Big Bang Theory includes the abundance of light elements (hydrogen, helium, and lithium) and the observed large-scale structure of the universe.

Tags

NGSS.HS-ESS1-2

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