STAGE 2-3. Stellar Formation Evolution Flashcards

1
Q

A celestial luminous body in the sky.
They are primarily made up of mostly
hydrogen, with some helium and small
amounts of other elements.

A

STAR

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2
Q

The process by which elements are formed
within stars as a result of nuclear fusion.

A

STELLAR NUCLEOSYNTHESIS

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3
Q

The process by which multiple nuclei joined together to
form a heavier nucleus.

A

NUCLEAR FUSION

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4
Q

_____________ are vast clouds
of dust and gas.

A

NEBULAE

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5
Q
  • Predominantly composed
    of hydrogen and helium.
  • They are also known as
    star nurseries as new
    stars form within them.
A

STELLAR NEBULAE

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6
Q

Though the dust and gas
within nebulae are spread
out, gravitational forces
cause them to clump
together, forming what is
known protostar.

A

STELLAR NEBULAE

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7
Q
  • it is a hot core
    at the heart of the
    collapsing cloud that will
    one day become star
A

PROTOSTAR

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8
Q

In a main sequence star, the
inward pressure of its gravity is
balanced by the outward pressure
of nuclear fusion, where the star
produces energy by converting
hydrogen atoms to helium atoms.

A

MAIN SEQUENCE

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9
Q

Eventually, the hydrogen which
powers the nuclear reactions
inside a star begins to run out. All
stars will expand, cool and change
color.

A

RED GIANT

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10
Q

A smaller star or the average star,
will gradually cool down and stop
glowing.

A

PLANETARY NEBULAE & SUPERNOVA

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11
Q

a region of cosmic gas and dust formed from
the cast-off outer layers of a dying star.

A

PLANETARY NEBULAE

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12
Q

is what happens when
a star has reached the end of its
life and explodes in a brilliant burst
of light.

A

SUPERNOVA

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13
Q

Eventually, red giant stars become
too unstable and expel their outer
gaseous layers, leaving a small,
extremely dense, solid core, known
as a ________________.

A

WHITE DWARF

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14
Q

Without enough energy to emit
light, the white dwarf becomes a _________________.

A

BLACK DWARF

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15
Q

Less massive red super giants
condense into ___________ after
undergoing a supernova.

A

NEUTRON STARS

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16
Q

_____________ are incredibly dense, with a single teaspoon of neutron star weighing a billion tons.

A

NEUTRON STAR

17
Q

If the star was of an extremely
high mass then, after a supernova,
it could collapse into itself,
forming a ________________, in which
gravity is so strong that even light
cannot escape it.

A

BLACK HOLE

18
Q

is one of the ways by
which stars fuse hydrogen into helium

A

PROTON-PROTON CHAIN REACTION

19
Q

is a catalytic process that requires the
presence of some initial carbon, nitrogen, and
oxygen abundance in the stellar material.

20
Q

stars fuse together three
alpha particles, creating a
new particle with six
protons and six neutrons

A

TRIPLE ALPHA PROCESS

21
Q

More and more alpha
particles are fused to
create heavier elements
all the way to iron.

A

ALPHA LADDER

22
Q

slow-neutron-capture-process is a
nucleosynthesis process that occurs at
relatively low neutron density and
intermediate temperature conditions in
stars.

23
Q

a rapid neutron-capture process is a set of
nuclear reactions that in nuclear astrophysics
is responsible for the creation of approximately
half of the atomic nuclei heavier than iron. It is
done in a rapid process.