DOC PREVIEW
GSU ASTR 1020 - ASTR Notes

This preview shows page 1-2-3-18-19-37-38-39 out of 39 pages.

Save
View full document
View full document
Premium Document
Do you want full access? Go Premium and unlock all 39 pages.
Access to all documents
Download any document
Ad free experience
View full document
Premium Document
Do you want full access? Go Premium and unlock all 39 pages.
Access to all documents
Download any document
Ad free experience
View full document
Premium Document
Do you want full access? Go Premium and unlock all 39 pages.
Access to all documents
Download any document
Ad free experience
View full document
Premium Document
Do you want full access? Go Premium and unlock all 39 pages.
Access to all documents
Download any document
Ad free experience
View full document
Premium Document
Do you want full access? Go Premium and unlock all 39 pages.
Access to all documents
Download any document
Ad free experience
View full document
Premium Document
Do you want full access? Go Premium and unlock all 39 pages.
Access to all documents
Download any document
Ad free experience
View full document
Premium Document
Do you want full access? Go Premium and unlock all 39 pages.
Access to all documents
Download any document
Ad free experience
View full document
Premium Document
Do you want full access? Go Premium and unlock all 39 pages.
Access to all documents
Download any document
Ad free experience
Premium Document
Do you want full access? Go Premium and unlock all 39 pages.
Access to all documents
Download any document
Ad free experience

Unformatted text preview:

Points – 538.27 – 69.01 – 6 (12)9.15 – 14 (26)10.08 – 2 (28)10.15 – 6 (34)10.20 – 9 (43)10.29 – 3 (46)11.05 – 1 (47)11.10 – 4 (51)11.12 – 2 (53)11.24 – 3 (56)Lecture #9Light MatterToday1. Nature of Light2. Properties of MatterReadings Chapter 5 (sections 1-3)How do we experience Light?- Warmth (sun)- ColorColors is Light- Light is made up of many different colorso Very hot material emits visible light (sun, wire in light bulb)o Cool light (from a chair) doesn’t emit visible light by itself Absorbs and reflects it- i.e. Red Chair = absorbs blue light, reflects red lightHow do light and matter interact?- Emission - Absorptiono Materials that absorb = opaque- Transmission (allow some to pass through)o Materials that transmit = transparent- Reflection (or redirecting or scattering)o Reflection = bouncing in same general directiono Scattering = more randomRecap- How do we experience light?o Light is a form of energyo Light comes in many colors that combine to form white light- How does light interact with matter?o Matter can emit, absorb, transmit, and reflect (redirect/scatter) lighto Interactions between light and matter determine the appearance of everything we see around us Part 2 What is light?- Light can act either like a wave or like a particle- Particles of light are called photonsWaves- Pebble in the pond analogyo Waves ripple in the pond Consists of trough (water lower than average) and peaks (water higher than average)o Leaf in pond will rise and fall with peaks and troughs but won’t move  waves carry energy outward but do not carry matter along with them- Particle = thing- Wave = pattern revealed by interactions with particlesProperties of Waves- 3 basic properties of waves: wavelength, frequency, and speed- Wavelength o Distance from one peak to the next- Frequencyo Number of times (per sec) that a wave vibrates up and down “cycles per second” often called Hertz (Hz)- Wave Speedo Wave Speed = Wavelength x Frequency Tells us how fast their peaks travel Light: Electromagnetic Waves- A light wave is a vibration of electric and magnetic fieldso Light is an electromagnetic wave Causes electrons to bob up and down – wriggle as a snake as light passed byo A field is used to describe the force an object would feel when in a certain space- Light interacts with charged particles through these electric and magnetic fieldso Light always travels at the speed of light (about 300,000 km per sec) Wavelength x Frequency = Speed of Light (c)o So there is an inverse relationship between Frequency and Wavelength Longer Wavelength = Shorter Frequency Examples- If W is 1cm, F must be 30 GHz- Therefore, if W = .5cm  F would double to 60 GHz- W = .25cm  F = 120 GHzParticles of Light- Particles of Light are called photonso Has properties of both particles and waves- Each photon has a wavelength and a frequency- The energy of a photon depends of its frequency o Directly proportional to its frequencyo E = h x f H is called “Planck’s Constant”Electromagnetic Spectrum- Light we can see = Visible Lighto 400nm – 700nm (Blue  Red)- In order of Short  Long Wavelengthso Gamma rays, X-Rays, UV rays, Visible, Infrared, Radioo High frequency  low frequency (inversely proportional to wavelength)o Large energy per photon  small energy per photon- Infrared Lighto Wavelengths somewhat longer than red lights Lies beyond red in the spectrum I.E. Jupiter- Radio Waveso We hear sound waves from the car radio, not electromagnetic waveso Sometimes given the name microwaves Radar, Microwave ovens Cosmic microwave background  Radio images of Galaxies (Centaurus A)- Ultraviolet (UV) Lighto Just to the left of visible light (violet) Example: The Suno Mostly absorbed by the ozone in the atmosphere o Can cause skin cancer- X-Rayso Very short, very energetic wavelengths (left of UV, right of Gamma)o Can penetrate through tissues, but not bones- Gamma Rayso Most energetic, shortest wavelengthso Extremely Violent eventsRecap: Properties of Light- What is light?o Can behave either like a wave or a particleo A light wave is a vibration of electric and magnetic fieldso Light waves have a wavelength and a frequencyo Photons are particle of light- What is the electromagnetic spectrum?o Human eyes cannot see most forms of lighto The entire range of wavelengths of light is known as the electromagnetic spectrumProperties of MatterWhat to know- What is the structure of matter?- What are the phases of matter?What is the Structure of Matter- Electron (Negative), Protons (Positive – Red), and Neutrons (Neutral – Grey)- Atomic Termso Atomic Number – number of protons in nucleus Number of electrons = number of protonso Atomic Mass – number of protons and neutronso Molecules – consist of two or more atomso Isotopes – Atoms with same number of protons, but different number of neutronsPhases of Matter- Solid, liquid, gas o Phases depend primarily on temperature but are also affected by pressureTemperature- Measures how fast particles (atoms or molecules) moveTemp. Scales- Water Boils around 100 C- Freezes at 0 C- Absolute Zero = -273.15 C- Room Temp = 0 C or 300KPhase Changes- Melting: Breaking of rigid lattice; solid  liquid- Evaporation: Breaking of chemical bonds; liquid  gas- Dissociation: Breaking of molecules into atoms- Ionization: Stripping of electrons, changing atoms into plasma o Free elections and ions- Often more than one phase is presentLecture #10Matter and ShitToday1. Matter (Cont., recap)2. Inferring properties of matter from light3. Inferring motions of objects from lightReadings Chapter 5 (sections 4 and 5)Energy Levels in Atoms- Electrons in an atom are held in orbit around nucleus by electrical forceo Kind of like a planet around a sun- Can occupy many discrete orbitso Each orbit is an energy level (like the rungs on a latter  specific heights)Recap- What is the structure of mattero Matter is made of atoms, which consist of a nucleus of protons and neutrons surrounded by a cloud of electrons- What are the phases of mattero As temperature rises, a substance transforms from a solid to a liquid to a gas, then the molecules can dissociate into atoms (more than one can co-exist, thought)o Stripping of electrons from atoms (ionization) turns the substance into a plasms- How is energy stored in atoms?o The energies of electrons in atoms correspond to discrete energy levelsLearning From Light-


View Full Document

GSU ASTR 1020 - ASTR Notes

Download ASTR Notes
Our administrator received your request to download this document. We will send you the file to your email shortly.
Loading Unlocking...
Login

Join to view ASTR Notes and access 3M+ class-specific study document.

or
We will never post anything without your permission.
Don't have an account?
Sign Up

Join to view ASTR Notes 2 2 and access 3M+ class-specific study document.

or

By creating an account you agree to our Privacy Policy and Terms Of Use

Already a member?