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Par Galaksiju

Authored by ketija Petrova

Science

9th - 12th Grade

Par Galaksiju
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12 questions

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1.

MULTIPLE CHOICE QUESTION

30 sec • 2 pts

What are the three main types of galaxies?

Lenticular, spiral, dwarf

Spiral, elliptical, irregular

Barred spiral, elliptical, spiral

Irregular, barred spiral, lenticular

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which type of galaxy is characterized by a flat disk and spiral arms?

Elliptical galaxy

Spiral galaxy

Lenticular galaxy

Irregular galaxy

3.

MULTIPLE CHOICE QUESTION

45 sec • 2 pts

What is the primary difference between elliptical and spiral galaxies?

Elliptical galaxies have more gas and dust than spiral galaxies.

Spiral galaxies are older than elliptical galaxies.

Elliptical galaxies are more luminous than spiral galaxies.

Elliptical galaxies lack structure and have older stars, while spiral galaxies have distinct arms and ongoing star formation.

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How do astronomers detect black holes in galaxies?

By observing gravitational effects and X-ray emissions.

By tracking the movement of comets

By analyzing the color of nearby planets

By measuring the temperature of stars

5.

MULTIPLE CHOICE QUESTION

30 sec • 2 pts

What is the role of supermassive black holes in galaxy formation?

Supermassive black holes help regulate star formation and influence galaxy dynamics.

Supermassive black holes only exist in small galaxies.

Supermassive black holes are formed from dying stars.

Supermassive black holes have no impact on galaxy structure.

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Can black holes be found in all types of galaxies?

Black holes cannot exist in elliptical galaxies.

Only supermassive black holes exist in galaxies.

Yes, black holes can be found in all types of galaxies.

Black holes are only found in spiral galaxies.

7.

MULTIPLE CHOICE QUESTION

45 sec • 3 pts

What evidence supports the existence of dark matter in galaxies?

Evidence includes galaxy rotation curves, gravitational lensing, cosmic microwave background fluctuations, and galaxy cluster dynamics.

The presence of supernova remnants

Observations of black holes in galaxies

Variations in star brightness over time

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