Earth Sci Chapter 1 Flashcards

1
Q

What observations led to the acceptance of the Big Bang theory?

A

Three Pillars of Proof
o Recession of stars/galaxies (Hubble’s Law)
o Characteristics of microwave background radiation
o Abundance of light elements

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2
Q

What are the steps of the scientific method?

A

Hypothesis, Theory, Law

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3
Q

What is hypothesis?

A

an educated guess based upon observation (sometimes only one observation)

cannot be supported or rejected
cannot be proven to be true

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4
Q

What is theory

A

the foundation of science, and summarizes a hypothesis (or group of hypotheses) that is supported by repeated testing and observation

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5
Q

what is law

A

explains a body of observations. no exceptions found

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6
Q

What is a singularity

A
  • No readily understood definition
  • An area in space-time where gravitational force is so high that all known laws of
    physics break down and do not apply
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7
Q

What is the Big Bang theory? What does it describe?

A
  • The theory of how the universe was created

- It describes a gigantic expansion that was the beginning of space and time

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8
Q

What are the three main lines of observation that support the Big Bang theory?

A

doppler effect, cosmic microwave background, abundance of light elements

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9
Q

What is the big bang theory

A

an effort to explain exactly what happened at the beginning of the Universe

At the birth of the universe, time and space were created in a gigantic expansion that emanated from a ‘singularity’

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10
Q

what is a gigantic expansion?

A

Think of an infinitesimally small balloon, which in the tiniest fraction of time, suddenly expands and keeps on expanding. In that tiny instant, time and space had a finite beginning inside the balloon

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11
Q

Doppler effect

A

An object coming towards you making sound will have compressed sound
waves (louder)

­An object moving away making sound will have extended sound waves (lower)

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12
Q

Cosmic Microwave Background (CMB)

A

The hot light photons from the big bang have lost energy and dropped into
microwave wavelength (out of visible light)
­
Appears as static noise when played by a sensitive microwave radio
receiver

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13
Q

Abundance of light elements

A

Hydrogen (75%), Helium (25%), Lithium (trace)

can be explained only if they originated from one single ratio of the first subatomic particles of matter that can be formed from a super-hot environment

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14
Q

What are the possible shapes of the universe?

A

Sphere, saddle shaped, and flat

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15
Q

Sphere universe

A
  • ­Positive curvature
  • ­Closed universe
  • Finite size but without boundary
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16
Q

saddle shaped universe

A
  • Negative curvature

- ­Infinite and unbound

17
Q

Flat universe

A
  • Infinite and boundless
18
Q

What makes up the most matter in the universe, dark matter or stars?

A

Dark matter > stars

Dark matter: 27%
Stars, etc: 5%

19
Q

What is the difference between dark matter and dark energy?

A

Dark matter is unable to be seen, gives off no electromagnetic energy, has gravitational attraction

Dark energy is opposite of gravity, it repels matter, controls expansion of space

20
Q

What is the difference between dark matter and dark energy?

A

Dark matter is unable to be seen, gives off no electromagnetic energy, has gravitational attraction

Dark energy is opposite of gravity, it repels matter, controls expansion of space

21
Q

How can we know the age of the universe? (3 ways)

A

Radioactivity, Hubble’s Expansion Constant, Cosmic Microwave Background Radiation

22
Q

Radioactivity

A
  • Radioactive elements that break down into other components are tracked
  • Measure how long the process took based on which radioactive process produces said gasses from the first elements
  • Between 11.5 and 17.5 billion years, at least 13.2 billion
23
Q

Hubble’s Expansion Constant,

A
  • Using Hubble’s constant equation, there is a t variable
    ­- Possible to determine age of the most distant light sources
    ­- Between 13 and 4 billion years
24
Q

Cosmic Microwave Background Radiation

A
  • Offer most accurate view of conditions in early Universe
    ­- A model based on the CMB signal map when first photons were produced
    by Big Bang
    ­- 13.80 +/- 0.04 billion years