(Chapter 6.3) History of the Universe Flashcards

1
Q

Define emission spectrum

A

The spectrum of frequencies of electromagnetic radiation emitted when an electron makes a transition from a high energy state to a lower energy state. As the name suggests, atoms emit energy

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

Define absorption spectrum

A

The spectrum of frequencies of electromagnetic radiation transmitted when an electron makes a transition from a lower energy state to a higher energy state. As the name suggests, atoms absorb energy

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

Define spectroscopy

A

The study of the absorption and emission of light and other radiation by matter

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

Define red shift

A

A shift in the ‘red’ of the electromagnetic spectrum and indicates the galaxy is moving away from the Earth

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

True or False. “Hubble correctly discovered that most galaxies tended to have a red shift.”

A

True

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

Identify the correlation between red shift and velocity

A

The more severe a red shift is, the higher the velocity of a galaxy

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

Define cosmic microwave background radiation

A

A faint glow of light that fills the universe, falling on Earth from every direction with nearly uniform intensity

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

Identify the elongated term for CMBR

A

The elongated term for CMBR is Cosmic Microwave Background Radiation

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

Outline the accepted proposed history of the Universe by the majority of society

A
  1. The universe began from a singular point containing large amounts of energy
  2. Space and time are created from the big bang
  3. The energy was converted into matter - atomic nuclei and clusters of protons and neutrons
  4. Within 400 00 years, the universe began to cool until the point where it was possible for electrons to combine with the atomic nuclei to form neutral atoms
  5. Electromagnetic radiation and CMBR entropied throughout the universe.
  6. The universe was cool enough for gravity to clump matter and form celestial bodies
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

Define the Big Bang Theory

A

A theory that states the universe and life started from a singular hot and dense particle that expanded into the universe

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

Define the Steady State Theory

A

A theory that states the universe has always existed and always will; that the universe had no beginning and has no end. Furthermore, the expansion of the universe is caused by the constant creation of matter at an enormous rate

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

Define radio source

A

Any of various objects in the universe that emit relatively large amounts of radio waves

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

Recall the alternate term for radio source

A

Radio galaxies is the alternate term for radio source

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

True or False: “Each element has unique spectra lines”

A

True

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

Recall the formal term for red shift

A

The formal term for red shift is velocity of recession

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

Explain why the occurrence of red shifts supports the theory that the universe is expanding

A

Red shifts show that galaxies are moving away from the Milky Way; hence, the distance between galaxies is expanding, which can only be explained by the expansion of the Universe

17
Q

Recall the most common element in space

A

Hydrogen is the most common element in space

18
Q

Recall the formula for energy

A

E = mc^2
where:
E = energy (Joules)
m = mass (kg)
c = speed of light (m/s)

19
Q

Recall the formula for Newton’s universal law of gravitation

A

F = G * (m_1 * m_2)/d^2
where:
F = Force of attraction (N)
G = Gravitational constant (6.67*10^-11)
m_1 = Mass of Object 1 (kg)
m_2 = Mass of Object 2 (kg)
d^2 = Distance between objects (m)

20
Q

Recall the influence of gravity on the formation of the universe

A

Gravity formed celestial bodies