Class: ______Period: _____
Date: ______ / TutorUse Only:
Essential Question:
Chapter 28 Stars and Galaxies
28.1 Closer look at Light
- Light is a form of ______, which is energy that travels in waves.
- Waves of energy travel at 300,000 km/sec (speed of light
- Ex: radio waves and x-rays
- Electromagnetic waves do not need a ______to travel, they travel through ______
- Electromagnetic waves emitted by an object indicated what ______are present and its motion
- Electromagnetic radiation waves are arranged into a continuum call the ______.
- Wide range of wavelengths
- ______wavelengths with ______frequencies at one end, ______wavelengths with ______frequencies at the other end
- ______ measured crest to crest/trough to trough
- ______ the number of that crests of the same wavelength that pass a point in one second.
- Scientists study the visible light portion of the electromagnetic spectrum.
- ______of stars allow for astronomers to learn about the star’s elements and motion.
- Spectra studied using a ______
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- Three types of visible spectra
- ______spectrum: unbroken band of colors, emitting all colors of visible light
- glowing solids, such as a light bulb filament
- glowing liquids, molten iron
- hot, compressed gases inside a star
- ______spectrum: unevenly spaced lines of different colors, emitting light of only some wavelengths
- glowing thin gases
- every element has its own unique emission spectrum, element’s finger print
- ______spectrum: dark lines that cross a continuous spectrum.
- forms when light from a glowing object pass through a cooler gas which absorbs some wavelengths
- can determine what is present in the cooler gas by comparing emission and absorption spectrum
- ______Effect is the apparent change in the wavelength of radiation or sound due to relative motion between the object and the receiver.
- Doppler effect applies to ______as well as sound.
- Shift of the ______spectra can indicate if the object is moving towards or away from Earth
- Shift towards the red end of the visible light spectrum, object moving away Earth – ______
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- Shift towards the blue end of the visible light spectrum, object moving towards Earth - ______
- Doppler effect determined that the universe is ______
- ______Telescopes – gather far more light than an unaided eye and magnify imagers
- ______
- Uses one lens at back to gather and focus light
- Image reflected on to a small mirror and then the eye piece
- ______
- Uses two lenses
- Lens at the front gathers light
- Eyepiece magnifies image
- ______Telescopes
- Technical term for really big satellite dishes
- Use to detect energy waves at frequencies lower than visible light
- Other
- Detects energy waves at frequencies higher than visible light
- Usually satellites in space
- Gamma ray
- Background radiation
- X-ray
- Hubble (infrared)
- Observation of stars has been going on for over ______years
- The grouping of stars are called ______
- Constellations
- ______grouping of stars
- only appear together as viewed from ______from a different angle they do not look like the constellation
- Grouped together due to ______like they all have the same brightness (______magnitude)
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- Constellations will change shape over ______of years due to the universe expanding
- Some constellations have been around for thousands of years other were recently conceived
- Move across the sky from ______to ______(though Earth rotates west to east)
- Big Dipper and Little Dipper two of the best know constellations point to the ______
- North Star
- Current north star is called ______
- Sits directly over the ______pole
- Does not ______to the naked eye
- Very powerful tool for ______
- Due to ______, Polaris will not always be the “North Star”
- Circumpolar Constellations – constellations around the north star
- Create star trails evidence for Earth’s ______
- North star appears ______in the sky as Earth rotates
- star trails from circumpolar constellations rotate ______around the north star
- Circumpolar constellations seem to ______set from some northern hemisphere latitude
- Distances to stars and other objects in space
- Unit of measurements on Earth are ______sufficient for space measurements
- ______ (AU) is used for the distance from Earth to the Sun (150 million kilometers)
- ______ is the distance light travels in one year (9.5 trillion kilometers)
- It is a ______measurement
- Example - 4.2 light-years means that the light we see has been traveling for 4.2 years before we can see it (4.2 X 9.5 trillion km)
- ______change in an object’s direction due to a change in the observer’s position
- Parsec short for “parallax second” equal to 3.258 light-years.
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- Stars
- Elements
- ______~69%
- ______~29%
- Heavier elements ~2%
- No two stars have the same proportions of elements
- light that radiates is dependent on composition and temperature, this differs in every star
- Star spectrum is its fingerprint
- Mass, Size and Temperature
- Stars vary greatly in ______, ______, and ______
- Cannot observe directly so we are estimating what the mass might be
- ______effect on bodies around the star help with estimating its mass
- Star ______is expressed as multiples of the mass of our Sun (which has a stellar mass of 1)
- ______varies more than mass
- Smallest stars are ______than Earth
- Largest have diameters more than ______times that of our Sun
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Essential Question:
- Stars differ even more in ______
- Betelguese is about one ten-millionth of our Sun
- One star is so dense that one ______would weight more than a ______on Earth
- ______of stars vary
- Stars have ______colors which indicate different temperatures
- Cool stars are ______in color
- Mid-temp are ______in color
- Hot stars are ______in color
- Astronomers group stars by ______and color into spectral classes.
- Star Brightness
- Actual brightness of a star is ______
- Dependent on ______and ______
- ______from Earth is not a factor
- If two stars are the same size the ______star would be more luminous
- ______magnitude is how bright a star appears to an observe on Earth
- Does not factor in ______
- ______magnitude is the measure of how bright a star would be is all stars were the same distance from Earth (10 parsec)
See foldable for Star life cycle and HR Diagram
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28.4 Galaxies and the Universe
Galaxies:
- The ______ is everything that exists.
- The ______is everything we can observe.
- Astronomers have are not sure how old the universe is since the light from the beginning has not yet reach us. The estimate is between 10-20 billion years
- Galaxies are hard to separate from stars without ______.
- Hazy patches of light which when viewed through a telescope reveals thousands to billions of stars.
- Astronomers estimate there are 50- 100 billion galaxies in the observable universe.
- No two galaxies are the ______, however, they are classified based on ______.
- There are ______classifications
- ______(ex. Milky Way)
- ______are near spherical to lens-shape
- ______(ex. The two Magellanic Clouds )
- ______ – explains history of the universe from a tiny fraction of a second after it came into being up to the present
- ______explanation for how the universe came to being
- Developed due to ______of stars, galaxies and other objects with telescopes and experimenting with matter on Earth
- Approximately 10-20 billion years ago all matter in the universe existed in an incredibly hot and dense state, from which it expanded and cooled slowly condensing into stars and galaxies.
- It is ______at a very slow rate and is still expanding today
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- ______for the Big Bang Model:
- The universes apparent ______, distance between galaxies and groups of galaxies seems to be increasing with time.
- Edwin Hubble’s discovery of the ______in the spectra of galaxies supports the expansion of the universe
- Discovery of radiation called ______background radiation apparently left over from the universe’s beginning.
- Continues to be tested and examined to seek further evidence to support it
- Some astronomers are considering alternative ways the universe has reached its present state.
- It is ______to know for certain how the universe began
- as long as the Big Bang Model ______crucial tests, it remains the best ______for the origin of the universe
- If it were to ever fail a test, then astronomers will have to look for a new theory/model
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