Chapter 20 cosmic perspective – Flashcards

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About how many galaxies in observable universe?
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over 100 billion galaxies
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Age of most galaxies around us?
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10 billion years
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How to study young galaxies?
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looking at rgeat distances
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Cosmology
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study of overall structure and evolution of the universe
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Three major types of galaxies
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Spiral, Elliptical, irregular
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Spiral Galaxy
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flat white disks with yellowish bulges at their centers - usually display beautiful spiral arms
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Elliptical Galaxy
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Redder, more rounded , elongated like football - contain very little cool gas and dust, contain very hot, ionized gas
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Irregular Galaxy
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appear neither dislike or rounded - blobby star systems - contain young massive stars - megellanic clouds are examples
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Why do the colors of galaxies differ?
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spiral/irregular galaxies appear white because they ave stars of all different colors and ages, elliptical galaxies have old, reddish stars that produce most their light
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Dwarf Galaxies
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have as few as 100 million stars
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Giant galaxies
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more than 1 trillion stars
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disk component
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flat disk where stars follow orderly, nearly circular orbits around center - contains interstellar medium
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How may disk components differ?
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molecular, atomic, and ionized gases in the interstellar medium may differ from one to the next
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Spheroidal Component
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The bulge and Halo - orbits with many inclinations and contain little cool gas or dust
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Bulges tend to extend how far?
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10,000 Light years
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Barred spiral galaxies
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spiral galaxies that appear to have a straight bar of stars cutting across the center with spiral arms curling away from the ends of the bar
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What do astronomers think our galaxy is?
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Barred spiral galaxies because our bulge appears somewhat elongated
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Lenticular galaxies
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intermediate class between spirals and elliptical (they lack arms) tend to have less cool gas than normal spirals but more than ellipticals
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Among large galaxies what percent are spiral or lenticular?
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75-85%
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elliptical galaxies are sometimes known as?
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spheroidal galaxies
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Elliptical galaxies lack a significant _______ component.
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Disk
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Giant Elliptical galaxies
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relatively rare and are among the most massive galaxies in the universe
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Dwarf Elliptical Galaxies
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fewer than a billion stars - often found new larger spiral galaxies
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Gas in a giant elliptical galaxy:
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Low density, x ray emitting much like the gas in hot bubbles created by supernovae
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Lack of cool gas in elliptical galaxy means:
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They have little to no star formation (like our own halo)
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When were irregular galaxies more common?
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when the universe was younger
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Hubbles Galaxy Classes
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organizes galaxy types into a diagram shaped like a tuning fork
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E0 Galaxy
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Sphere
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Hubble Galaxy Class Elliptical
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Designated by E and a number - Elliptical are on the handle at left - larger number/flatter disk
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Hubble Galaxy Class Spiral
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S for ordinary spiral, SB for barred spirals followed by lowercase a, b, or c - bulge decreases size a-c
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S0 (hubble class)
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Lenticular Galaxies
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Irr (hubble Class)
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Irreglar Galaxes
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Quantitative galaxy classification
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similar to H-R diagram for Stars - measures galaxy luminosity and galaxy color
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Blue Cloud
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Major group - consists of spiral or irregular galaxies with active star formation
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Red Sequence
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Consists galaxies that lack active star formation and are redder in color because they have few blue or white stars - most elliptical in shape
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Groups
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spiral galaxies found in loose collections of up to a few dozen falaxies
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Clusters of galaxies
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contain hundreds and sometimes thousands of galaxies extending over more than 10 million light years - elliptical
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radar ranging
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how astronomers measure AU - radio waves are transmited from Earth and bounced of Venus
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Standard Candle
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light source of a known, standard luminosity
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Main-sequence fitting
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method of determining distances to different star clusters by comparing brightness to their main sequence stars
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Cepheid Variable stars
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extremely luminous variable star
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Henrietta Leavitt
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1912 - discovered Cepheid are closely related to their luminosity (longer the period, more luminous the star)
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Period Luminosity Relation
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the longer the period, the more luminous the star
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Cepheid vary in luminosity because:
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they pulsate in size, growing brighter as they grow larger and dimmer as they shrink -
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The Great debate
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Held in Washington dc April 26 1960 - Shapley ( spiral nebulae were gas clouds internal to milky way) Vs Curtis (Kants island of stars)
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What did Hubble discover about Andromeda?
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Using the 100 inch telescope at Mt Wilson he saw individual stars - he used Cepheid stars to calculate distance
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redshifted
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object emitting radiation is moving away from us
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Hubble's Law
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the formula that expresses the idea that distant galaxies move away from us faster
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Hubble's constant
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H-naught
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Two important difficulties when using hubble's law to measure galactic distances
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1 - galaxies do not object the law perfectly - nearly all galaxies experience gravitational tugs from other galaxies 2 - distance as only as accurate as best measurement of hubble's constant
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Does hubble's law work for galaxies in the local group?
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No
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Cosmological principle
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the idea that the matter in the universe is evenly distributed without a center or edge
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Balloon analogy
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as the balloon expands, the dogs move apart in the same way galaxies move apart in our expanding universe
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lookback time
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difference between current age of the universe and the age of the universe when light left the object
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spacetime diagram
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a way to visualize the relationship bet ween distance, expansion and lookback time
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cosmological redshift
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as the universe expands photo wavelengths shift to longer, redder wavelengths
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cosmological horizon
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marks the limits of the observable universe (a boundary in time not space)
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