Final Units of Astronomy

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160 Terms

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Components of our Galaxy

Disk, bulge, and halo

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Disk

flat, contains spiral arms which are home to bright/young stars

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Bulge

Bright, central, thicker region, older stars, cigar shape

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Halo

Spherical region around disk, very few stars, globular clusters

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Interstellar medium

dusty gas clouds that obscure our view of the galaxy because they absorb so much light

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Does dust hide most of galaxy

Yes

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How big is Milky Way and is there anything similar

Milky Way is very large, closest galaxy to that size is Andromeda

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Do several small galaxies orbit our galaxy?

Yes, large and small magellanic clouds

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Disk star orbits

move in a nearly circular orbit around the center

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Why do disk stars bob up and down

gravity

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What does the bobbing cause

disk thickness

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Halo Star orbits

randomly oriented, elongated orbits

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Do halo stars pass through disk very fast?

Yes, the disk gravity barely changes their path

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Does the randomness cause puffiness in the halo?

yes

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Bulge star orbits

Some are like halo orbits and some are like disk orbits; it's very hard to measure

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What shape do the stars orbiting the bulge give it

a cigar shape

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How to find mass within an orbit

Use Newton's version of Kepler's Third Law. Need the orbital speed and radius of the star

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Does the halo contain visible stars or gas?

Almost none

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Galactic Recycling

Milky Way constantly recycles gas between stars and the interstellar medium

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Stages of Galactic Recycling

Atomic clouds, molecular clouds, star formation, nuclear fusion in stars, returning gas in supernovae, hot bubbles

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Atomic clouds

Most iSM gas is cool atomic hydrogen

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What do atomic clouds emit

radio waves, these help astronomers map them

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What do atomic clouds contain

dust grains which absorb visible light and is the reason we can't see across the disk

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When do atomic clouds form

They form as hit gas cools, allowing electrons to join with protons

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Molecular clouds

Come about when atomic clouds cool/contract

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How do you detect molecular clouds?

Via the CO emission lines

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What are molecular clouds mostly made of

H2

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Are moiecular clouds dense

yes, very

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Star formation

Gravity collapses molecular clouds and forms a star cluster in the cloud

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What do massive newborn stars emit

UV rays, those rays also erode the cloud

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How much of a cloud of gas becomes stars

Just a fraction

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Nuclear Fusion in Stars

Nuclear fusion happens in stars and they're stars

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Gas returned by a low mass star

Returns gas to interstellar space through winds and planetary nebulae

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How strong are the winds of a low-mass star during life

Weak winds; strong winds as a red giant though

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Gas returned by High-mass stars

explode as supernovae and eject huge amounts of gas and heavy elements

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How strong are winds from a high-mass star

Very strong

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Supernovae and Stellar winds create

Hot bubble of ionized gas and shock fronts (wall of gas moving faster than sound)

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Hot bubbles

Help mix heavy elements across the galaxy and enrich our galaxy

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Many supernovae in one region merge their bubbles and make

giant bubbles that burst out of the disk

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Where are molecular clouds

central plane of disk

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Where is atomic hydrogen

fills the disk

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Where are hot bubbles

in disk/halo

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Where do stars form

only in molecular clouds

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Regions with newborn hot stars show

ionization nebulae, reflection nebulae, and dark dust clouds

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Spiral Arms

Full of massive stars, ionization nebulae, gas/dust,

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What are spiral arms in galaxies?

Density waves

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What is one result of the density waves in spiral arms?

Compression of gas leading to star formation

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Why do blue stars remain near the spiral arms?

They die fast

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Why do low mass stars spread around the disk of a galaxy?

They live long

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Where do we find ionization nebulae

In the disk because there's star formation there

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What is a density wave

slow-moving ripple of high-density

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How do stars and gas move through a density wave

Like cars in traffic jam

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What causes spiral arms

Compression waves reproducing around the disk (density waves)

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Spiral arms appear what color compared to bulge

Blue

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Halo stars

Formed first (old), random orbits, no new stars

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Disk stars

all ages, circular orbits, ongoing star formation

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Why are halo stars so old

Halo has hot gas, bad environment for the molecular clouds and it formed before supernovae enriched the galaxy

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Simple version of galaxy forming

1. Giant gas cloud to begin with

2. Halo stars start to form as gravity causes cloud to contract

3. Remaining gas settled into a spinning disk

4. Stars continuously form in the disk as the galaxy grows older

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More realistic version

the galaxy gets assembled from a lot of smaller clumps of gas and stars. Little galaxies get merged together over time. The halo stars are very old, but many come from small galaxies accreted earlier

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Evidence halo stars are from other galaxies

streams of halo stars = remnants of old dwarf galaxies

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Is the halo a smooth sphere of stars?

No many are in "tidal streams"

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Can tidal streams destroy smaller galaxies near Milky Way?

Yes, we can destroy small

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What brought the universe more heavy elements over time?

The star-gas-star cycle

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Black hole at center of Milky Way?

Yes

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How do we know black hole at center of our universe?

Infrared images, radio emissions, x-ray flares, and stars orbiting

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A galaxy's age, distance, and age of the universe are all closely related

Truth

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Disk component

stars of all ages, many gas clouds

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Spheroidal component

bulge and halo, old stars, few gas clouds

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red-yellow color in galaxy

older star population

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blue-white color in galaxy

ongoing star formation

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What shape do elliptical galaxies typically have?

Round or oval

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What type of stars are primarily found in elliptical galaxies?

Red old stars

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Do elliptical galaxies contain a lot of cool gas?

No, they contain little cool gas

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Is there new star formation in elliptical galaxies?

No, there is no new star formation

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What is a characteristic feature of elliptical galaxies regarding their structure?

They have no arms

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Can elliptical galaxies vary in size?

Yes, they can be huge or tiny

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Lenticular Galaxy

has a disk like spiral galaxy but much less dusty gas

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Is lenticular intermediate between spiral and elliptical?

Yes

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What type of galaxy is not spiral or elliptical?

Irregular galaxy

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What is a characteristic shape of an irregular galaxy?

No clear shape

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What is a common size characteristic of irregular galaxies?

Often small

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What color are irregular galaxies typically described as?

White and dusty

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What type of activity is often found in irregular galaxies?

Active star formation

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When were irregular galaxies more common in the universe?

In the early universe

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Barred spirals

Spiral galaxy with straight bar of stars across the center

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The Hubble "Tuning Fork"

Qualitative way of classifying galaxies

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Does The Hubble "Tuning Fork" answer the question of why galaxies have different shapes?

No

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What is the scale of the The Hubble "Tuning Fork"

Spheroidal dominant to disk dominant

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Blue Cloud

spirals and irregulars: lots of cold gas and new star formation

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Red sequence

ellipticals and very luminous at the top

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Where are spiral galaxies often found

in isolation or in groups of galaxies (group being a couple dozen of galaxies)

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Where are elliptical galaxies found

Much more common in huge clusters of galaxies (hundreds to thousands of galaxies packed into a volume not much larger than distance between Andromeda and Milky Way)

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Why distance of galaxies matters

Allows us to determine the size, age, and expansion rate of the universe

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Distance Ladder

a method used in astronomy where greater and greater distances are determined using many different measuring techniques that overlap to establish a sequence of increasing distances.

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standard candle

an easily recognizable astronomical object whose absolute brightness is confidently known

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Cepheid Variables

A variable star that brightens and dims regularly, or pulses, and whose distance can be determined from its period of pulsation (longer period = brighter)

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Hubble's Law

The observation that the farther away a galaxy is, the faster it is moving away. As we look back in time galaxies should be closer together and more dense

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How did Hubble say galaxies are shifting?

Redshifting

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Hubble's constant

tells us the age of the universe because it relates velocities and distances of all galaxies

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How did Galaxies form?

Our best models for galaxy formation assume that gravity made galaxies out of regions in the early universe that were slightly denser than their surroundings.