Hello my little starlets,
Today is your day to SHINE! But will you be a BROWN DWARF? Or perhaps a GIGANTIC NUCLEAR FURNACE? Try not to be NEBULOUS!
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Light-years
S.r. solar radius
Kilometers
Parsecs
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Light
White
Energy
Color
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Oxygen and Nitrogen
Nitrogen and Helium
Oxygen and Hydrogen
Hydrogen and Helium
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Multiple systems
Nebulae
Stellar nurseries
Constellations
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The temperatures reaches 6000 C
The electrons in the core elements are lost
Nuclear fusion begins
Stars have planets orbiting it
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The star is hotter than most stars in our galaxy
The star and the sun have similar surface temperatures and sizes
The star will end its life as a neutron star
The star is a white dwarf
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Red, yellow, white, blue
White, blue, yellow, red
Blue, white, yellow, red
Yellow, red, blue, white
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A supergiant
A neutron star
A black hole
A black dwarf
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A supergiant
A neutron star
A low-mass star
A high-mass star
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Matter ejection
Gas concentration
Heavy core formation
Nuclear fusion
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Electrons
Protons
Neutrons
Negitrons
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Novae
Pulsars
Protostars
Red giants
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Main sequence stars
Supergiants
Giants
White dwarfs
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Stars on the upper left end are less massive.
Stars on the upper left end are more massive.
Stars on the upper left end tend to be red in color.
Stars on the upper left end are near the end of their life cycle.
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True
False
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True
False
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True
False
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True
False
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True
False
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True
False
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True
False
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True
False
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True
False
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True
False
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Polaris
Hikianalia
Rigel
Hokul'ea
Polaris
Casseopeia
Hokule'a
Hikianalia
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Cygnus the swan
Leo the lion
Ursa major the bear
Casseopiea the quessn
True
False
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What is wrong with this spreadsheet formula for the average of the values entered into cells B2 through B23? =averageB2-B23
=(average)B2:B23
=B2-B23/22
=average(B2:B23)
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The stars on the main sequence
Those that were actively fusing Hydrogen
Those that were closest
Those with the smallest solar radii
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Plumenia + 2.8
Cartha Minor -1.2
Astronium + 5.4
Alpha Megulus - 0.5
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