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Module 5: Newtonian World and Astrophysics
5.5 Astrophysics and Cosmology
5.5.1 Stellar Evolution
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During the collapse stage of star formation, gravity increases the density and
temperature
Main sequence stars are in hydrostatic
equilibrium
Match the characteristics with the type of star
Pre-Main Sequence Star ↔️ Kelvin-Helmholtz contraction
Main Sequence Star ↔️ Nuclear fusion
Stages in the formation of a star within a molecular cloud
1️⃣ Collapse
2️⃣ Protostar Formation
3️⃣ Nuclear Fusion
What type of energy source powers a pre-main sequence star?
Kelvin-Helmholtz contraction
Main sequence stars produce energy through the fusion of hydrogen into
helium
in their core.
True
What is the most common and stable stage of a star's life cycle?
Main sequence
Stages in the post-main sequence evolution of low mass stars
1️⃣ Red Giant
2️⃣ Planetary Nebula
3️⃣ White Dwarf
A pre-main sequence star has not yet begun nuclear
fusion
Red giants begin fusing
helium
in their core as hydrogen is depleted.
In the core of a red giant, hydrogen is depleted, and the core begins to
contract
What drives the expansion of a red giant's outer layers?
Hydrogen depletion
A white dwarf eventually collapses into a black hole
False
Match the stage of stellar evolution with the corresponding event:
Red Giant ↔️ Core contracts as hydrogen is depleted
Supernova ↔️ Catastrophic core collapse
White Dwarf ↔️ Dense, cooling core
Planetary Nebula ↔️ Outer layers are ejected
What triggers a supernova explosion in a high mass star?
Core collapse
As a star's core runs out of hydrogen, it begins to contract under its own
gravity
What is the composition of neutron stars?
Neutron-degenerate matter
Nuclear fusion marks the birth of a main sequence star when hydrogen is fused into helium.
True
A pre-main sequence star's luminosity is derived from nuclear reactions.
False
Pre-main sequence stars have core temperatures high enough for nuclear fusion.
False
Main sequence stars maintain hydrostatic equilibrium due to
nuclear fusion
.
True
Stars form within giant molecular
clouds
Main sequence stars have core temperatures hot enough for nuclear fusion of hydrogen into
helium
The luminosity of a red giant is lower than that of a main sequence star
False
Order the stages in the post-main sequence evolution of low mass stars:
1️⃣ Red Giant
2️⃣ Planetary Nebula
3️⃣ White Dwarf
How does the post-main sequence evolution of high mass stars differ from that of low mass stars?
High mass stars undergo supernovae
A black hole can form from the remnant of a high
mass
star
True
Order the stages in the process leading to a supernova explosion:
1️⃣ Core Collapse
2️⃣ Fusion Reactions
3️⃣ Supernova Explosion
4️⃣ Remnant Formation
What happens to the outer layers of a star during a supernova explosion?
They are blown off
The gravity of a neutron star is strong enough to trap light
False
The transition of a star into the red giant phase is driven by the depletion of hydrogen fuel in its
core
.
True
During protostar formation, heat is generated by Kelvin-Helmholtz
contraction
The higher luminosity of main sequence stars is derived from nuclear reactions in their core.
True
What happens to the core of a star as it transitions into a red giant phase?
It contracts
What is the primary energy source of a red giant?
Helium fusion
When a low mass star ejects its outer layers, it forms a colorful, glowing shell called a
planetary nebula
A high mass star ends its life in a violent explosion called a
supernova
Supernovae are crucial for distributing heavy elements throughout the cosmos
True
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