Ch 26 & 27 Astronomy Test

Ch 26 & 27 Astronomy Test

9th - 12th Grade

24 Qs

quiz-placeholder

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Ch 26 & 27 Astronomy Test

Ch 26 & 27 Astronomy Test

Assessment

Quiz

Physics

9th - 12th Grade

Medium

Created by

Ann Beemer

Used 8+ times

FREE Resource

24 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the meaning of isotropic?

the same density everywhere

the same in all directions

the same at all times

the same temperature everywhere

the same in every way throughout space

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

________ is the concept that all large samples of the universe are alike in appearance anywhere in the universe.

Confromity

Isotropy

Universality

Homogeneity

Cosmology

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Because almost all of the galaxies are redshifted, we know that:

there was no beginning to time.

we are at or close to the center of the universe.

the universe is expanding.

the sky is dark at night.

All of the above are correct.

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

The darkness of the night sky in a seemingly infinite universe is addressed in:

the Doppler shift

parallax shift

Stefan's Law

Olbers' Paradox

the Cosmological Principle.

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

The redshift of galaxies in the universe is correctly interpreted as:

 a Doppler shift due to the motions of the galaxies through space.

an "aging" of the light.

the effect of intergalactic dust.

space itself is expanding with time; the wavelengths of photon are stretched while they travel through space.

the difference in temperatures of distant and nearby galaxies.

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

While a variety of factors can produce red shifts in the spectrum, the one associated with the expansion of the universe is called:

universal

cosmological

olberian

relativistic

the Zeeman Effect

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

If the density of the universe is less than critical, then:

the universe will "survive" to expand forever.

 the universe on average must be less than 2.73K in temperature.

the universal expansion must stop within about twenty billion years.

 the universe must be static, and the red shifts are not cosmological.

the universe will begin contracting immediately into the "Big Crunch."

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