Stellar Properties and Measurements

Stellar Properties and Measurements

Assessment

Interactive Video

Physics, Science, Mathematics

9th - 12th Grade

Hard

Created by

Patricia Brown

FREE Resource

The video tutorial explains the process of measuring the distances to stars, focusing on Sirius. It covers the use of color filters to determine the color index, which helps identify the star type and calculate its temperature. The tutorial also discusses using the HR diagram and Stefan-Boltzmann law to find the star's luminosity. It explains how to calculate the absolute magnitude and convert it to distance in parsecs and lightyears, highlighting the inherent inaccuracies in astronomical measurements.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the primary purpose of using color filters in measuring stellar distances?

To determine the color index

To enhance the brightness of stars

To calculate the star's age

To measure the star's size

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How is the type of star determined using the color index?

By comparing it to a standard star chart

By using a telescope

By referencing a table of color indices

By consulting a star catalog

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the approximate temperature of Sirius calculated using the color index?

11,000 Kelvin

10,000 Kelvin

12,000 Kelvin

9,000 Kelvin

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which law is used to calculate the luminosity of a star?

Hubble's Law

Kepler's Law

Stefan-Boltzmann's Law

Newton's Law

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the luminosity ratio of Sirius to the Sun?

10

25-26

20

15

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How is the absolute magnitude of a star calculated?

By comparing it to the Sun

Using the formula -2.5 times the log of the luminosity ratio

By observing its color

By measuring its brightness directly

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the apparent magnitude of Sirius?

-1.46 to -1.44

2.50

0.00

1.24

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