Star Properties Part 2

Star Properties Part 2

11th - 12th Grade

12 Qs

quiz-placeholder

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Star Properties Part 2

Star Properties Part 2

Assessment

Quiz

Science

11th - 12th Grade

Medium

Created by

Glen Cline

Used 56+ times

FREE Resource

12 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

2 mins • 1 pt

What is meant by the term luminosity?

Luminosity is the amount of energy generated in the star as electromagnetic radiation.

Luminosity is how bright a star seems to an observer far away.

Luminosity is the color at which a star burns.

Luminosity is the determinant of whether a star is approaching an observer or receding,

2.

MULTIPLE CHOICE QUESTION

2 mins • 1 pt

How do we calculate the luminosity of the Sun?

use the inverse square law

use Einstein's law of mass -energy conversion

use the quadratic equation

use the accekeration formula a = f/m

3.

MULTIPLE CHOICE QUESTION

2 mins • 1 pt

At the Earth's surface, how much energy do we receive from the Sun?

1,400,000 ergs/square cm/second

9.8 meters/second2

3.1416 joules/second

1x10^3 kilowatts/minute

4.

MULTIPLE CHOICE QUESTION

2 mins • 1 pt

Stellar diameters can be measured for some nearby giant and supergiant stars by using a technique called stellar:

triangulation.

calculus.

binomial quadratics.

interferometry.

5.

MULTIPLE CHOICE QUESTION

2 mins • 1 pt

What is the unit for measuring the linear diameters of stars?

miles

millions of kilometers

light years

solar radii

6.

MULTIPLE CHOICE QUESTION

2 mins • 1 pt

Which of the following is but the most reliable method for measuring distances to stars?

algebraic formulation

geometric parallel

trigonometric parallax

applying Newton's second law

7.

MULTIPLE CHOICE QUESTION

2 mins • 1 pt

Which of the following is the best description of the parallax effect?

The parallax effect is the square root of the diameter of the star.

The parallax effect is the apparent motion of a nearby object compared to distance background objects because the change in viewing angle.

The parallax effect is calculated by dividing the star's mass by its volume.

The parallax effect is the distance to a star divided by its intrinsic luminosity.

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