Toggle Navigation
Games
Blog
Class PIN
Join for Free
Sign in
Toggle Navigation
Games
PIN
Join for Free
Blog
Pricing
Contact us
Help center
Sign in
Study
Duplicate of The Sun + Duplicate of Layers of th ...
0
%
0
0
0
Back
Restart
The asteroid belt is between
Earth and the Moon
Earth and Venus
Earth and Mars
Mars and Jupiter
Oops!
Okay!
comets have ______________ when they get close to a star
tail
face
leg
arm
Oops!
Okay!
HUGE loops of gas on the suns surface.
Core
Prominences
Solar Flare
Sunspots
Oops!
Okay!
Stream of energy that leaves the sun in all directions. Our magnetic field protects us.
Solar Wind
Prominence
Sunspot
Flare
Oops!
Okay!
How old is the sun?
Billions of years
Trillions of Years
Thousands of Years
Millions of Years
Oops!
Okay!
The light that comes to Earth comes from this layer of the sun.
Photosphere
Corona
Chromosphere
Convection Zone
Oops!
Okay!
His model was geocentric for our solar system.
Copernicus
Mr. Wizard
Aristarchus
Ptolemy
Oops!
Okay!
This philosopher created a model that said this (see picture).
Aristotle
Columbus
Copernicus
Ptolemy
Oops!
Okay!
Where Hydrogen is converted into Helium
Corona
Chromosphere
Core
Photosphere
Oops!
Okay!
This zone takes energy 170,000 years to reach the next layer.
Chromosphere
Radiation Zone
Photosphere
Convection Zone
Oops!
Okay!
When TWO prominences connect...Huge Explosion of Energy.
Sunspot
Solar Wind
Prominence
Solar Flare
Oops!
Okay!
This layer produces the solar wind.
Chromosphere
Photosphere
Convection Zone
Corona
Oops!
Okay!
Helio- means this.
Star
Moon
Hello
Sun
Oops!
Okay!
When a meteroid hits the ground it is called an
meteoroid
meteorite
rock
Asteroid
Oops!
Okay!
This process occurs in the core of the Sun.
Nucleic Acid
Nucleus
Nuclear Fission
Nuclear Fusion
Oops!
Okay!
He identified that Venus has phases similar to our moon because of sunlight reflection angles.
Ptolemy
Copernicus
Kepler
Galileo
Oops!
Okay!
Outer most layer. The Crown
chromosphere
corona
photosphere
core
Oops!
Okay!
This is the outermost layer of the Sun's atmosphere...
Chromosphere
Photosphere
Exosphere
Corona
Oops!
Okay!
The Layer that produces LIGHT
Photosphere
Chromosphere
Corona
Sunspots
Oops!
Okay!
These two elements fuse together to produce energy in the Sun's core.
Helium and Honey
Helium and Oxygen
Hydrogen and Helium
Hydrogen and Oxygen
Oops!
Okay!
This the outermost layer of the sun.
Corona
Convection Zone
Chromosphere
Photosphere
Oops!
Okay!
This zone is the layer of the sun where energy is transferred away from the core.
Radiator
Radiation
Convection
Conduction
Oops!
Okay!
Solar flares shoot out of this layer
Convection zone
Corona
Photosphere
Chromosphere
Oops!
Okay!
Hot gases rise and cool gases sink in this layer.
Corona
Photosphere
Chromosphere
Convection Zone
Oops!
Okay!
The sun is 10%
Oxygen
Carbon
Hydrogen
Helium
Oops!
Okay!
Areas on the sun that appear darker because they are cooler.
Prominences
Sunspots
Flare
Solar Wind
Oops!
Okay!
This is the dense center which is around 15 million degrees Celsius. Nuclear Fusion occurs.
Photosphere
Core
Corona
Cornea
Oops!
Okay!
The layer that gives the Sun COLOR
Chromosphere
Photosphere
Prominence
Corona
Oops!
Okay!
Sunspots appear on this layer.
Chromosphere
Photosphere
Convection Zone
Corona
Oops!
Okay!
This is the visible surface of the sun where energy escapes.
Corona
Exosphere
Core
Photosphere
Oops!
Okay!
This layer can only be seen during an eclipse.
Chromosphere
Photosphere
Corona
Convection Zone
Oops!
Okay!
In this layer, energy travels from the radiative zone to the photosphere.
Convection Zone
Danger Zone
Conduction Zone
Radiative Zone
Oops!
Okay!
This is the middle layer of the Sun's atmosphere it appears as red ring during a solar eclipse.
Chromosphere
Corona
Photosphere
Core
Oops!
Okay!
Meteroids are chunks of asteroids or
planets
comets
people
moons
Oops!
Okay!
Nuclear fusion occurs in which layer of the sun?
Core
Corona
Convection one
Radiation Zone
Oops!
Okay!
This is the part of the sun that we see.
Photosphere
Chromosphere
Convection Zone
Corona
Oops!
Okay!
The sun is 90%
Hydrogen
Oxygen
Carbon
Helium
Oops!
Okay!
Your experience on this site will be improved by allowing cookies.
Allow cookies