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Unit 8: Space Physics (Physics Only)
8.1 The Solar System
8.1.2 Life Cycle of a Star
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The formation of a star begins with a
nebula
Steps in the formation of a star from a nebula
1️⃣ Nebula undergoes gravitational collapse
2️⃣ A protostar forms at the center
3️⃣ Temperature and pressure in the core increase
4️⃣ Nuclear fusion initiates
5️⃣ A new star is born
During the Main Sequence Stage, a star converts hydrogen into
helium
Match the stage with its characteristics:
Main Sequence ↔️ Hydrogen to Helium, Stable, Yes
Pre-Main Sequence ↔️ None, Increasing, No
Post-Main Sequence ↔️ Heavier elements, Unstable, No
When a star exhausts its hydrogen fuel in the core, it enters the
Red Giant
The surface temperature of a Red Giant is lower than that of a Main Sequence star.
True
The process that powers a star is called
nuclear fusion
A Red Giant is significantly larger than a star in the
Main Sequence Stage
.
True
How does the luminosity of a Red Giant compare to a star in the Main Sequence Stage?
Higher
A Red Giant forms when a star exhausts its hydrogen fuel in the core during the
Main Sequence Stage
.
True
What does the core of a Red Giant eventually initiate fusion into?
Carbon
Helium fusion in a Red Giant produces carbon, while
hydrogen fusion
in the Main Sequence Stage produces helium.
True
After the Main Sequence Stage, a star undergoes significant changes in its
structure
and energy generation.
Steps in the formation of a star
1️⃣ Nebula
2️⃣ Gravitational Collapse
3️⃣ Protostar
4️⃣ Nuclear Fusion
The
Main Sequence Stage
is the longest and most stable period in a star's life cycle.
True
What stage does a star enter after it exhausts its hydrogen fuel in the core during the Main Sequence Stage?
Red Giant Phase
In the Red Giant Phase, the star's surface temperature decreases, giving it a
red
color.
What heavier element is formed during helium fusion in the Red Giant Phase?
Carbon
Match the stage with the type of nuclear fusion occurring:
Main Sequence ↔️ Hydrogen to Helium
Red Giant ↔️ Helium to Carbon
Order the steps in the formation of a Planetary Nebula:
1️⃣ Red Giant Phase
2️⃣ Pulsations
3️⃣ Stellar Winds
4️⃣ Ionization
What remains at the center of a Planetary Nebula?
White Dwarf
White Dwarfs produce energy through nuclear fusion.
False
After a supernova, the star's core collapses to form either a neutron star or a black
hole
.
What is a neutron star composed almost entirely of?
Neutrons
Black holes have infinite density at their core.
True
What is a nebula composed mainly of?
Hydrogen and helium
What is the longest and most stable phase of a star's life cycle?
Main Sequence Stage
The Main Sequence Stage can last for
billions
of years.
True
Match the stage of a star's life with its characteristic:
Main Sequence ↔️ Hydrogen to Helium fusion ||| Stable hydrostatic equilibrium
Red Giant ↔️ Helium to Carbon fusion ||| Lower surface temperature
In the Red Giant Phase, helium fuses into
carbon
What type of remnant is left behind after a star ejects its outer layers as a planetary nebula?
White Dwarf
What is the central star of a Planetary Nebula called?
White Dwarf
Steps in the formation of a Planetary Nebula
1️⃣ Red Giant Phase
2️⃣ Pulsations
3️⃣ Stellar Winds
4️⃣ Ionization
A Planetary Nebula has ongoing nuclear fusion in its core
False
Match the stellar characteristic with the correct stage in a star's life cycle:
Nuclear Fusion of Hydrogen to Helium ↔️ Main Sequence
Extremely High Density ↔️ White Dwarf
Significantly Larger Size ↔️ Red Giant
Steps in the formation of a Supernova
1️⃣ Massive Star Life Cycle
2️⃣ Nuclear Fusion
3️⃣ Red Supergiant Phase
4️⃣ Core Collapse
5️⃣ Supernova Explosion
6️⃣ Remnant
Supernovae are essential for distributing heavy
elements
What is the process called where a nebula contracts under its own gravity?
Gravitational collapse
The Main Sequence Stage is the longest and most stable stage of a star's life cycle.
True
What is the term for the balance between outward pressure and inward gravity in a star?
Hydrostatic equilibrium
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