- comprises all space and time, and all matter & energy in it - made up of 4.6% baryonic matter, 24% cold matter, and 71.4% dark energy - it is 13.8 billion years old
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Hydrogen, helium and Lithium
The three most abundant elements in the universe
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Baryonic Matter ? 4.6%
- “ordinary” matter consisting of protons, electrons and neutrons that comprises atoms, planets, stars, galaxies and other bodies - How much of it is in the universe?
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Dark Matter ? 24%
- matter that has gravity but does not emit light - How much of it is in the universe?
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Dark Energy ? 71.4%
- a source of anti-gravity; a force that counteracts gravity and causes the universe to expand - How much of it is in the universe?
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The Steady State Model
- proposed in 1948 by Bondi and Gould and by Hoyle - pertains that new matter is created as the universe expands thereby maintaining its density - implies that universe have NO BEGINNING and END
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The Big Bang Theory
- states that one time, the entire universe was confined to a dense, hot, supermassive ball. Then, about 13.8 billion years ago, a violent EXPLOSION occurred, hurling this material in all directions
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1. General Relativity 2. Cosmological principle
• what are the 2 ideas the Big Bang Theory rests on? (1) Gravity is a distortion of space and time (2) Assumes that the universe is homogeneous and isotropic; means every observer SHOULD see the universe with the same physical properties wherever you like and the same structure whatever direction you see it
• The tests for expansion the Big Bang Theory has withstood
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Redshift
- the shifting of absorption lines from the light spectrum towards larger wavelength(red light) - happens when a light source is moving away(receding) towards the observer - discovered by Edwin Hubble when he noticed that most galaxies have spectral shifts toward the red end of the spectrum
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Hubble’s Law
- states that galaxies recede at speeds proportional to their distances from the observer
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Cosmic Microwave Background
- a faint glow of light that fills the universe, falling on Earth from every direction with nearly uniform intensity - can be observed as a striking uniform glow in the microwave band coming from all directions-blackbody radiation with an average temp of about 2.7 degrees above absolute zero
- formed when gravity cause matter to accumulate into large “clumps” and “strands” of interstellar matter known as NEBULAE - first developed approximately after 400,000 millions years after the Big Bang
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All stars, regardless of their size, run out of fuel and collapse due to gravity
• How do stars die?
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Hertzprung-Rusell Diagram
- a graphical representation of the relationship between the true brightness(absolute magnitude) of stars and their respective temperatures
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H-R Diagram and Stellar Evolution
- useful for illustrating the changes that take place in an individual star during its life span
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Galaxies
- collections of interstellar matter, stars and stellar remnants that are gravitationally bound - the first of them were small and composed mainly of massive stars and abundant interstellar matter - have 3 basic types
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Spiral Galaxies
- flat, disk-shaped objects that range from 20,000 to about 125,000 light-years in diameter - have a greater concentration of stars near their centers, but there are numerous variations - makes up 30% of the universe
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Milky Way
- a large SPIRAL GALAXY whose disk is about 100,000 light years wide and about 10,000 light years thick at the nucleus - has at least 3 distinct spiral arms, with some splintering - part of the so called Local Group of Galaxies, which in turn is part of the Virgo supercluster of galaxies
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Barred Spiral Galaxy • Andromeda Galaxy
• what kind of spiral galaxy is this? • give an example
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Elliptical Galaxy • Cygnus A
- have an ellipsoidal shape that can be nearly spherical and they LACK SPIRAL ARMS - some of the largest and smallest galaxies are classified as this - makes up 60% of the universe • give an example
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Irregular Galaxy • Small & Large Magellanic Clouds
- have no symmetry - some were once spiral or elliptical galaxies that were subsequently distorted by the gravity of a large neighbor • give an example
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Galactic Clusters • Fornax Galaxy Cluster
- galaxies that are grouped intro gravitationally bound clusters • give an example
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Galactic Collisions
- interactions between galaxies, often driven by one GALAXY’S GRAVITY disturbing another - common within galactic cluster
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Solar System
- located in the Milky Way galaxy - comprises the Sun, eight planets, dwarf planets suck as Pluto, satellites, asteroids, comets, other minor bodies suck as those in the Kuiper belt and interplanetary dust
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• Orbits of the planets are ELLIPTICAL and are on the same plane • the periods of revolution of the planets increase with increasing distance from the Sun
• the solar system in Macroscale
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• Most planets rotate prograde(west to east) • Planets fall into 2 groups based on location size and density; terrestrial and Jovian
• the solar system in Microscale
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Terrestrial Planets • Mercury, Venus, Earth, Mars
- a planet that is composed primarily of silicate rocks or metals, • give the 4 examples in the Solar System
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Jovian Planets • Jupiter, Saturn, Uranus, Neptune
- massive gaseous planets(gas giants) that extent far from the sun - planets that do not have solid surfaces, have many moons and rings • give the 4 examples in the Solar System
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Nebular Hypothesis
- hypothesis for the origin of the Solar System - thought of rotating gaseous cloud that cools and contracts in the middles to form the Sun and the rest into a disc - in this theory, the whole Solar System starts as a large cloud of gas that contracts under self gravity
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Encounter Hypothesis
- hypothesis for the origin of the Solar System - a “near miss” encounter occurs between the Sun and a passing star. Material is pulled from the stellar surfaces by tidal forces then cools and condenses to form planetary bodies • Problems: (1)hot gas expands not contracts and would not form planets. (2) encounter between stars are extremely rare
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Protoplanet Hypothesis
- hypothesis for the origin of the Solar System - incorporates many of the components of the nebular hypothesis, but adds some new aspects from modern knowledge of fluids ands states of matter - In the Orion arm of the Milky Way galaxy, a slowly-rotating gas and dust cloud dominated by hydrogen and helium starts to contract due to gravity - as most of the mass move to the center to eventually become a proto-Sun, the remaining materials form a disc that will eventually become the planets and momentum is transferred outwards
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Temperature • -15ºC to 115ºC
• factors that make a planet habitable - influences how quickly atoms and molecules move • acceptable range in Celsius where liquid water can still exist under certain conditions
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Atmosphere • 100 miles thick
• factors that make a planet habitable - keep the surface warm & protects it from radiation and small to medium sized meteorites • acceptable thickness in miles
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Energy
• factors that make a planet habitable - can either be light or chemical - with it, cells can run the chemical reactions necessary for life
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Nutrients
• factors that make a planet habitable - used to build and maintain an organism’s body
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Energy from the sun
• factor on Earth that Sustains Life; Energy - drives EXTERNAL PROCESSES such as weather, ocean, circulation and erosional processes, PHOTOSYNTHESIS
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Energy from the Earth’s interior
• factor on Earth that Sustains Life; Energy - drives INTERNAL PROCESSES including volcanoes, earthquakes and mountain building
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Water
• factor on Earth that Sustains Life - one of the most important prerequisites of life4 - important part in regulating temperature, chemical reactions to matter, to aquatic habitat
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Gases
• factor on Earth that Sustains Life - makes up the atmosphere; greenhouse gases helps maintain the heat on Earth - essential to photosynthesis and other biochemical reactions
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Resources
• factor on Earth that Sustains Life - include water, soil, minerals and energy - have 2 broad categories: renewable and nonrenewable
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• In the ‘Habitable Zone” where you have just the right distance away from a star like the Sun • Made of Rocks • Big enough to have a molten core • Have a protective atmosphere
• Characteristics of a Habitable Planet
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System
- any size group of interacting parts that form a unified and complex whole
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Open System
• type of system - allows energy and matter to flow in and out of the system
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Closed System
• type of system - allows energy to flow in and out of the system while matter cannot
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Atmosphere • through atmospheric circulation
• Earth’s Subsystem - the thin gaseous layer that envelopes the Earth - composed of 78% nitrogen(N), 21% oxygen(O), 0.9% argon(Ar), and trace number of other gases - along with hydrosphere, where the exchange of heat and moisture occur • How is the heat of Earth’s surface redistributed
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Geosphere
• Earth’s Subsystem - associated with solid portion of the Earth - includes the rocks of the crust and mantle, metallic liquid outer core and the solid metallic inner core - the physical structure of the surface of the Earth is shaped through process of plate tectonics[a process for this subsystem]
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Hydrosphere • through ocean circulation
• Earth’s Subsystem - the total amount of water on a planet; including water on the Earth’s surface, underground and in the air • How is heat reabsorbed and redistributed on the surface of the Earth?
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Hypsographic Curve
- a graphical representation of the proportion of land at various elevations(meters above or below sea level)
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Biosphere
• Earth’s Subsystem - areas or regions of the Earth that possess life; comprised of living organisms and nonliving factors from which organisms derive energy and nutrients - the set of all life forms on Earth - covers all ecosystems