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(Chapter 6.3) History of the Universe

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卡片总数: 20内容版本: v4公开卡包更新时间: 8/1/2026

卡片预览 (20 张)

#1
正面 (问题)

Define emission spectrum

背面 (解答)

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

#2
正面 (问题)

Define absorption spectrum

背面 (解答)

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

#3
正面 (问题)

Define spectroscopy

背面 (解答)

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

#4
正面 (问题)

Define red shift

背面 (解答)

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

#5
正面 (问题)

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

背面 (解答)

True

#6
正面 (问题)

Identify the correlation between red shift and velocity

背面 (解答)

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

#7
正面 (问题)

Define cosmic microwave background radiation

背面 (解答)

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

#8
正面 (问题)

Identify the elongated term for CMBR

背面 (解答)

The elongated term for CMBR is Cosmic Microwave Background Radiation

#9
正面 (问题)

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

背面 (解答)

• The universe began from a singular point containing large amounts of energy • Space and time are created from the big bang • The energy was converted into matter - atomic nuclei and clusters of protons and neutrons • 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 • Electromagnetic radiation and CMBR entropied throughout the universe. • The universe was cool enough for gravity to clump matter and form celestial bodies

#10
正面 (问题)

Define the Big Bang Theory

背面 (解答)

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

#11
正面 (问题)

Define the Steady State Theory

背面 (解答)

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

#12
正面 (问题)

Define radio source

背面 (解答)

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

#13
正面 (问题)

Recall the alternate term for radio source

背面 (解答)

Radio galaxies is the alternate term for radio source

#14
正面 (问题)

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

背面 (解答)

True

#15
正面 (问题)

Recall the formal term for red shift

背面 (解答)

The formal term for red shift is velocity of recession

#16
正面 (问题)

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

背面 (解答)

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
正面 (问题)

Recall the most common element in space

背面 (解答)

Hydrogen is the most common element in space

#18
正面 (问题)

Recall the formula for energy

背面 (解答)

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

#19
正面 (问题)

Recall the formula for Newton’s universal law of gravitation

背面 (解答)

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
正面 (问题)

Recall the influence of gravity on the formation of the universe

背面 (解答)

Gravity formed celestial bodies