Module 1A Flashcards

1
Q

Astronomy

A

the scientific investigation of the Universe.

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2
Q

The Universe

A

All that exists

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3
Q

laws and principles of science,

A

the relationships between matter and force particles,

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4
Q

big G,

A

the universal gravity constant, a measure of the strength of the gravity
force,

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5
Q

little k,

A

Coulomb’s constant, a measure of the strength of the electromagnetic
force,

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6
Q

multiverse

A

(multiple universes),

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7
Q

physics

A

what is happening here on Earth,

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8
Q

What is astronomy about?

A

whereas astronomy is
mostly about what is happening “out there”

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9
Q

cosmology

A

the study of the evolution of the Universe, past, present and future.

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10
Q

13.8 billion years ago.

A

The universe began

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11
Q

the average mass-energy density of the Universe

A

ultimately determines the geometry of the Universe, and whether it is finite or
infinite in extent.

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12
Q

Flat geometry

A

The geometry of the universe

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13
Q

The universe is expanding into

A

it’s infinite self

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14
Q

The striking uniformity of the CMB temperature implies

A

an immense and rapid “blowing up” or “inflation” for less than a trillionth of a second after the Big Bang, with the observable Universe growing from the size of a proton to the size of a grapefruit (about 26 orders of magnitude enlargement).

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15
Q

CMB temperature

A

3000°

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16
Q

“cosmic inflation,”

A

slight increases in matter density were “seeded” into the then grapefruit
sized observable Universe.

17
Q

the force of gravity started to dominate the fledgling Universe, and

A

matter naturally started to clump together around these “seed” points of slightly higher density put into the Universe during the “cosmic inflation” period. These “seed” points grew into the stars and galaxies we see today.

18
Q

The expansion rate of the universe

A

is speeding up

19
Q

three kinds of matter or energy:

A

ordinary matter, dark matter, and dark
energy.

20
Q

The universe is 4.6%

21
Q

The universe is 71.4%

A

Dark energy

22
Q

The universe is 24%

A

dark matter

23
Q

ordinary matter

A

the regular matter we encounter every
day, matter composed of protons,
neutrons and electrons.

24
Q

Dark matter

A

dark matter is more than 5 times more abundant than ordinary matter in the visible Universe.

25
Q

dark energy.

A

energy that permeates all of space and causes space to expand as if there were a repulsive gravitational force present.

26
Q

the more space that is added by space expansion,

A

the more dark energy there is.