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Solar Structure

Total questions: 20

Worksheet time: 12mins

Name
Class
Date
1.

Which is NOT a layer of the solar atmosphere?

a)

photosphere

b)

chromosphere

c)

stratosphere

d)

corona

2.

The photosphere has a temperature of about

a)

500,000 K

b)

2 Million K

c)

5,800 K

d)

3,000 K

3.

The temperature of the photosphere is determined precisely by:

a)

measuring the spectrum of sunlight then using Wein's Law

b)

using a thermometer attached to a spacecraft

c)

running algorithms from a computer simulation

d)

estimating the temperature required to burn coal, which is what the sun is made up of

4.

The Sun makes its energy by:

a)

burning fossil fuels

b)

nuclear reactions in the core

c)

shining light

d)

photosynthesis

5.

The Sun's visible surface, the ______, is the layer in the sun from which visible photons most easily escape.

a)

corona

b)

chromosphere

c)

photosphere

d)

entire atmosphere

6.

Which is true?

a)

The sun is gaseous from its outer atmosphere right down to its center

b)

The sun is mainly gaseous but has a solid core

c)

The sun's chromosphere is gaseous, but the photosphere is a solid surface on fire

d)

The sun's atmosphere is gaseous and the surface is a boiling liquid

7.

Much of the light generated below the photosphere...

a)

cannot escape because it is blocked by dense gases

b)

is so bright that we are unable to see the photosphere itself

8.

__________ show that the Sun's photosphere contains atoms of hydrogen, helium, and other gases.

a)

absorption lines

b)

emission lines

c)

granules

d)

magnetic fields

9.

The photosphere's mottled appearance, with regions with dark edges, is called:

a)

limb darkening

b)

granulation

c)

spiculation

d)

color pixelation

10.

The center of a photospheric granule is:

a)

sinking gas because it is hotter than the gas on the edges of the granules

b)

rising gas because it is hotter than the gas on the edges of the granules

c)

sinking because it is cooler than the edges of the granules

d)

sinking because it is hotter than the edges of the granules

11.

The speeds of rising and sinking of gases in the sun's photosphere is measured using:

a)

doppler shifts of spectral lines.

b)

Wein's law.

c)

High speed cameras.

d)

robots that we send to the sun.

12.

granulation is the surface effect of:

a)

conduction

b)

convection

c)

poor visibility

d)

rotating hurricanes

13.

The layer directly above the photosphere is called the _____.

a)

chromosphere

b)

corona

c)

core

d)

radiative zone

14.

How can you see the chromosphere?

a)

Anytime, with binoculars

b)

During a solar eclipse, with an unaided eye

c)

During a solar eclipse, but only with special eclipse goggles

d)

During a lunar eclipse, with a special lense on a telescope

15.

The chromosphere is _____ due to ______.

a)

yellow... sulfur gas

b)

pink... red, blue, and violet Balmer lines.

c)

white... red, yellow, green and blue gases

d)

blue... the high temperature

16.

Filtergrams of the chromosphere reveal _____, which are flame-like structures extending into the lower corona.

a)

granules

b)

spicules

c)

limbs

17.

The ____ is the sun's outermost atmospheric layer that extends many solar radii from the visible sun.

a)

photosphere

b)

corona

c)

exosphere

d)

chronosphere

18.

What is the solar wind?

a)

a breeze of low-density ionized gas streaming from the Sun's corona.

b)

wind generated from rotation of the sun.

c)

a breeze originating from the sun's magnetic fields.

d)

another term for "light"

19.

Which is true about temperature of the solar atmosphere?

a)

Temperature decreases from the photosphere to the corona

b)

Temperature increases from the photosphere to the corona

c)

Temperature stays relatively consistent within the solar atmosphere

d)

Temperature increases then decreases in the corona

20.

The hottest layer of the sun's atmosphere is its:

a)

innermost layer, the photosphere

b)

outermost layer, the corona

c)

middle layer, the chromosphere