Cepheid Variables and Their Role in Astronomy

Cepheid Variables and Their Role in Astronomy

Assessment

Interactive Video

Physics

9th - 10th Grade

Hard

Created by

Nancy Jackson

FREE Resource

10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What characteristic of Cepheid variables allows them to be used for measuring distances in space?

Their proximity to Earth

Their small size

Their periodic changes in luminosity

Their constant brightness

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Why were Cepheid variables crucial in expanding our understanding of the universe?

They are the closest stars to Earth

They emit the most energy

They allowed measurement of distances beyond the parallax limit

They are the largest stars in the universe

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What was the limitation of the parallax method before the discovery of Cepheid variables?

It could only measure distances within 10 light years

It was only applicable to planets

It was limited to 100 light years

It could not measure distances at all

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What was Henrietta Leavitt's significant contribution to astronomy?

She discovered a new planet

She mapped the entire Milky Way

She invented the telescope

She found a relationship between the period and luminosity of Cepheid variables

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How did Henrietta Leavitt determine the relative luminosity of stars?

By comparing stars in the Magellanic Clouds

By observing their color

By using a telescope

By measuring their temperature

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What did Henrietta Leavitt use to observe the stars, given the restrictions of her time?

A telescope

Data recorded by other scientists

Her own observations

A microscope

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the role of the brightness equation in measuring distances using Cepheid variables?

It calculates the temperature of stars

It determines the color of stars

It relates observed brightness to luminosity and distance

It measures the size of stars

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