cosmology Flashcards

1
Q

what is cosmology

A

Study of the structure and evolution of the Universe

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2
Q

what image did ancients used to have of the universe

A
  • geometric image
  • flat earth
  • “Proven” by Ptolemy
    *A rebirth of rational thinking e.g. Heliocentric ideas happened in 15th-century Europe
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3
Q

3 things Newton devised

A
  • The Law of Universal Gravitation
  • The Three Laws of Motion
  • The mathematics of change (calculus)
    < He proved that natural law governs natural events
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4
Q

2 evidence for a spherical Earth

A
  • A curved shadow crossed the Moon during eclipses
  • Only the tops of distant sailing ships were visible
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5
Q

who circumnavigated the spherical earth

A

Magellan, 1520

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6
Q

difference between how a flat earth would receive the sun compared to a round one

A
  • flat Earth - receive light at a right angle at noon everywhere
  • round Earth - receive light at diminishing angles toward the poles
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7
Q

who almost accurately measured the earth

A

Eratosthenes

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8
Q

who proved Earth’s rotation

A

Jean Bernard Léon Foucault’s pendulum (1851)
*Clearly visible in a time-lapse photograph of the night sky

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9
Q

what is wavelength

A

spacing of waves - compress or relax with relative motion

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10
Q

what is frequency

A

waves passing a point in an interval of time

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11
Q

in the visible light spectrum is blue of red higher frequency

A
  • Blue = Higher frequency
  • Red = Lower frequency - more spaced out waves
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12
Q

how does light from an approaching and receding star vary

A
  • Light from an approaching star is compressed - higher frequency
  • Light from a receding star is expanded - lower frequency
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13
Q

what is the Doppler shift / effect and how it relates to the modern universe

A

Hubble concluded galaxies were moving away from us rapidly as Light from distant galaxies appeared “red shifted.” instead of “blue shifted” - evidence for expansion of the universe

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14
Q

explain the Big Bang theory

A

When the expanding Universe began
- All of the mass and energy in the Universe was packed into a single small point
- It exploded ~14 Ga and has been expanding ever since

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15
Q

what are nebulae

A

vast gas clouds that formed from the 1st atoms (hydrogen and helium) of the universe developing soon after the big bang

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16
Q

one strong evidence for the Big Bang

A

Universe Composition
- Started out ~100% Hydrogen and Helium
- NUCLEOSYNTHESIS occurred during the earliest stages of the Big Bang
- Explains present composition:
~90% H
~10% He
«1% heavier elements

17
Q

explain the process of star formation and evolution after the Big Bang

A
  • Post-Big Bang Expansion & Cooling → H₂ formed, fueling future stars
  • Formation of Gaseous Nebulae → Atoms and molecules gathered under gravity
    Gravity-Induced Collapse → Caused:
    Increased temperature & density
    Faster rotation
  • Formation of accretion discs
  • Nuclear Fusion Ignition → Created first-generation stars, consuming hydrogen rapidly
  • Star Death (Supernova) → When hydrogen ran out:
    Stars collapsed & heated
  • Heavy elements were produced
  • Explosive supernova released these elements into space, enriching the universe
  • This cycle of star birth + death eventually led to the formation of galaxies, planets, and life
18
Q

how do stars create elements

A

through nucleosynthesis -> stars are “element factories”

19
Q

what did Stellar Nucleosynthesis form

A

elements up to iron (Fe, atomic #26) inside stars

20
Q

what did Supernova Nucleosynthesis form

A

elements heavier than iron during supernova explosions.

21
Q

what determines the elements that stars produce

A

Star Mass
- Small Stars (e.g., the Sun) → Burn slowly, live longer (10 billion years), create lighter elements up to carbon
- Large Stars (10–100x Sun’s mass) → Burn rapidly, live shorter (millions of years), create heavier elements up to iron

22
Q

planet characteristics

A
  • large solid body orbiting a star (e.g., the Sun)
  • nearly spherical shape
  • cleared its neighborhood of other objects
    *Pluto, previously defined as a planet, is now excluded (belonging to the Kuiper Belt)
23
Q

what is included in our solar system

A
  • 7 other planets
  • The moon - solid body locked in orbit around a planet
  • The Sun – An average star
  • Asteroids – Rocky or metallic fragments
  • Comets – Fragments of ice orbiting the Sun
  • Kuiper Belt and Oort Cloud objects
24
Q

what is the Nebular Theory

A

Explains how the Solar System formed 4.56 billion years ago (Ga) from a 3rd, 4th, or nth generation nebula

25
what is Nebula composed of
- Hydrogen (H) + Helium (He) → Left over from the Big Bang - Heavier elements → Created by stellar fusion and supernovae
26
formation process of the solar system through the Nebular Theory
- Nebula condenses into an accretion disc - The central mass grows dense and hot, igniting nuclear fusion → The Sun is born - Dust in the disc condenses into particles, which coalesce into planetesimals - Planetesimals collide and accumulate, forming a proto-Earth - Earth's interior heats up, softens, and becomes spherical due to gravity - Differentiation occurs: Nickel-iron core forms Silicate mantle surrounds it - A planetoid collides with Earth, forming a debris ring → Moon forms - Volcanic gases create Earth's atmosphere - Cooling allows moisture to condense → Oceans form
27
supporting evidence for the nebular theory
- Planets’ orbits align within 3° of the Sun's equator - All planets orbit in the same direction