theories about the formation of the universe and the solar system

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39 Terms

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telescope

used to observe heavenly bodies

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Hans Lippershey

original patent holder of the telescope (1608)

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3x

lippershey telescope magnification

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Galileo Galilei

reinforced the telescope

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what galileo discovered

  • sunspots

  • phases of venus

    • 4 galilean moons of jupiter

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28x

galileo telescope magnification

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james webb space telescope

took 1st deep field photo

  • made in 2021

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  1. stars

  2. galaxies

  3. nebula

main objects in universe

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stars

generated heat via nuclear fusion in core

  • (H+He)

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galaxies

systems of stars/interstellar objects

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nebula

accumulations of space dust/stars

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  1. universe is a finite, closed 4-D sphere

  2. universe is homogenous

what Einstein said about the universe

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Wilkinson Microwave Anisotropy Probe (WMAP)

observes fluctuations and temperature differences in CMB radiation/anisotropes to determine traits of the universe

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  • 4% ordinary matter

  • 73% dark energy

  • 23% dark matter

composition of the universe

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  1. universe is smooth and homogenous

  2. universe is dominated by gravity only

assumptions of the universe

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tiny clumps that grew bigger due to gravity

contradiction to the theory that the universe is smooth and homogenous

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CMB radiation fluctuates; there must be 100x more dark matter than ordinary matter

contradiction to the universe is dominated by gravity theory

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  • both have sufficient mass to become round

  • both orbit the sun

similarities of planets and dwarf planets

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pluto intersects neptune’s orbit

why pluto is not a planet

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  • mercury

  • venus

  • earth

  • mars

aka inner planets

terrestrial planets

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characteristics of a terrestrial planets

  • small size and high density

  • made of rock and metal

  • no rings

    • little to no moons

  • solid and warm surfaces

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  • jupiter

  • saturn

  • uranus

  • neptune

aka outer planets

jovian planets

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characteristics of a jovian planet

  • larger size and mass

  • low density

  • many rings and moons

  • gaseous surfaces with cool temperatures

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elliptical

all planets are in this type of orbit (approximately same ecliptic)

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counter-clockwise (except for venus and uranus)

the direction in which the planet turns

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>3.4Âş

inclination of planetary orbits (except for mercury)

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true

there is a clear demarcation between terrestrial and gaseous planets

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6Âş

sun rotation axis

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sun

most of the solar system mass

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nebular hypothesis

the solar system was developed from a primeval nebula

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conservation of angular momentum

what made a disc (eventually the solar system)

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nuclear fusion

growing core created this because of heating

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centrifugal force

caused a ring to form around the protosun

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protoplanetary disk

ring around the protosun

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lighter gas was swept further from the sun leaving heavier elements

what happened to the lighter and heavier elements

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accretion

mutual gravity created terrestrial planets

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asteroids

what the leftovers from accretion formed

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nebular capture

colder regions made water vapour condense into ice and combined with gas

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comets

what the leftovers from nebular capture formed