Measuring the Stars pages 813-820. Groups of stars – the big ideas 1.Social significance of constellations 2.Why stars move 3.Star clusters 4.Binary systems,

Slides:



Advertisements
Similar presentations
Constellations By Jaclyn Schmitz.
Advertisements

Brightnesses, sizes and motions of stars. Recap Canvas assignment due Friday Project: due Friday 11/21 Campus observatory Emission and absorption lines.
Stars.
Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 10 Measuring the Stars.
Constellations.
Stars: Constellations
Question 1 Constellations appear to move across the sky at night because 1) the Earth orbits the Sun. 2) the Moon orbits the Earth. 3) stars are in constant.
CHAPTER 28 STARS AND GALAXIES
Earth Motions and the Heavens
Chapter 21 Stars and galaxies. Chapter 21 Stars and their Characteristics Kinds of Stars Formation of Stars Galaxies and the Universe.
Section 3 Constellations  Sections of sky with recognizable star patterns  Used by ancient people for navigation  Also used to keep track of time.
Star Properties studied so far… Period Mass Eccentricity Red shift Velocity Temperature (Wiens Law) Composition – which elements and how much of each Color.
The Electromagnetic Spectrum
* Celestial Sphere: * a sphere surrounding, and rotating around, Earth on which the stars and constellations were once thought to be firmly embedded *
Stars and galaxies. Constellations  Ancient Greeks, Romans and other cultures saw patterns of stars in the sky called constellations  They imagined.
PG. 127 Measuring the Stars. Groups of stars Long ago, people grouped bright stars and named them after animals, mythological characters or every day.
Bell Ringer 9/29 What are stars made of? Stars.
Earth’s Rotation and Revolution
Chapter 29 Notes Stars. The Sun: Solar Atmosphere Photoshere: visible surface, 5800 K Chromosphere: 30,000 K Corona: 1 to 2 million K, solar wind.
Stars.
Why does Earth seem to be standing still?
Concept 3: Longitude and earth’s rotation I. Rotation is the spinning of an object on its axis (imaginary.
Stars 2-1; part 2 How Bright is that Star?. What can you say about the brightness of the street lights as they appear in this picture? Can we use the.
Astronomical distances The SI unit for length, the metre, is a very small unit to measure astronomical distances. There units usually used is astronomy:
Astronomy Day Three Radiation, E-M Spectrum, Black Body Radiation, Doppler Effect.
Brightnesses, sizes and motions of stars Recap Project: due Friday 11/21 Campus observatory Information from brightnesses of stars – Brightness depends.
Stars, Galaxies, and the Universe Section 1 Section 1: Characteristics of Stars Preview Key Ideas Analyzing Starlight Stellar Motion Distances to Stars.
Chapter 30.1: Characteristics of Stars. At the center of the most violent starburst region in the local universe lies a cluster of brilliant, massive.
Astronomy Day Three Radiation, E-M Spectrum, Black Body Radiation, Doppler Effect.
Measuring the Stars Chapter Grouping of Stars Groups of stars named after animals, mythological characters, or everyday objects are called constellations.
Objectives Determine how distances between stars are measured. Distinguish between brightness and luminosity. Identify the properties used to classify.
Astronomy Day Three Radiation, E-M Spectrum, Black Body Radiation, Doppler Effect.
Measuring the Stars pages Groups of stars – the big ideas 1.Social significance of constellations 2.Why stars move 3.Star clusters 4.Binary systems,
EARTH & SPACE SCIENCE Chapter 30 Stars, Galaxies, and the Universe
Ch. 27 Stars and Galaxies Ch Characteristics of Stars.
 Students will be able to determine how distances between stars are measured.  Students will be able to distinguish between brightness and luminosity.
Chapter 30 Section 1 Handout Characteristics of Stars.
Monday, November Warm-Up: Grade Content Frame 2. Astronomy Intro.
Stars, Galaxies, and the Universe Section 1 Section 1: Characteristics of Stars Preview Key Ideas Analyzing Starlight Stellar Motion Distances to Stars.
Stars. Constellations -Patterns of stars in the sky A constellation looks like spots of light arranged in a particular shape against the dark night.
Chapter 30 Section 1 Handout Characteristics of Stars.
STARS & GALAXIES Constellations, the Sun, Milky Way.
Ch Stars Part 1 Chapter 19, Section 1. Stars Stars are huge, hot, brilliant balls of gas. To learn about stars, scientists study starlight.
Measuring Stars. Visible Spectrum & Wavelengths Spectral Types Continuous spectrum: Produced when white light passes through a prism Emission spectra:
Chapter 30.1: Characteristics of Stars. Characteristics of Stars A star is a _________________________ _______________________________ ____. Size varies.
Mapping the Stars Section 1-3 Summary. Patterns in the sky Constellations: sections of the sky that contain recognizable star patterns – Today scientists.
Constellations An group of stars the ancients originally named after mythical characters.
Astronomy Basic Properties of Stars. Kirchhoff’s Three Kinds of Spectra.
 .
1.1 Some space objects are visible to the human eye
DO NOW: Write it down  1. Most of the galaxies in the universe are moving __________ from us. 2. Our evidence to support this is ___ ___________________________.
Earth Science Ms. Cordaro San Marcos High School
Rotation and Revolution
28-1 A Closer Look at Light A. What is Light?
University of Scouting March 24, 2012 Gary G. Smith
Characteristics of STars
Section 2: Measuring the Stars
The Properties of Stars
Stars and HR Diagrams.
Stars.
Characteristics of Stars Chapter 3 Section 4 ISN p. 33
Stars.
Section 2: Measuring the Stars
Unit 5 Review.
Section 1: Characteristics of Stars
Ch Stars Chapter 19, Section 1 Part 1.
DO NOW: Write it down  1. Most of the galaxies in the universe are moving __________ from us. 2. Our evidence to support this is ___ ___________________________.
Ch Stars Chapter 19, Section 1 Part 1.
Section 1: Characteristics of Stars
The Properties of Stars
Presentation transcript:

Measuring the Stars pages

Groups of stars – the big ideas 1.Social significance of constellations 2.Why stars move 3.Star clusters 4.Binary systems, and multiple systems

Social significance of constellations 1.Constellations do not look like animals. The ancient peoples used to pick out a piece of the sky, and dedicate it to a deity, concept or person. If you connect the dots, you do not get a picture. 2.The twelve houses of the zodiac correspond to the constellation that is just behind the Sun on the day you were born. 3.The age, like the age of Aquarius is the house that the axis of the Earth is pointing to for about the next 2,000 years. The Earth has a wobble, and the axis will only point at Polaris for a few hundred years, then, another star will be north. The ancient Egyptians could not have used Polaris as a compass.

Why stars move 1.Stars move rapidly across the sky, each night, because of the rotation of the Earth on its axis. 2.Each star, at exactly 7:00 p.m., will be a bit farther west, because of the revolution of the Earth around the Sun.

Why stars move 1.Stars move rapidly across the sky, each night, because of the rotation of the Earth on its axis. 2.Each star, at exactly 7:00 p.m., will be a bit farther west, because of the revolution of the Earth around the Sun. 3.Some stars are visible in the summer, and others in the winter, because they are on the ether side of the sun. 4.If a star is visible year round, it must be very far north or south, and it would be called circumpolar, because it circled the pole.

Northern Star

Star clusters 1. Most of the stars in the sky are not just single stars. a.The point of light might be a binary, multiple or even a galaxy. b.The stars are too far away for out eyes to make out the separation.

What stars look like, the big ideas. Parallax Magnitude Light emitted by stars H-R diagram Parallax 1.This is the apparent shift in position of something, because of the movement of the observer. You can see this by putting your thumb up in front of your face, and closing one eye and then the other. 2.For finding the distance to stars, the change in position of the observer is the movement of the Earth around the Sun.

Because of parallax, it seems that the star moved, when compared to far away stars, but it did not actually do so. The smaller the parallax, the farther away the star is.

Magnitude ~ This is how bright something appears. 1.Apparent magnitude ~ this is how bright something appears from Earth. 2.Absolute magnitude ~ this is how bright something actually is, from 32.6 light years away, or 10 parsecs. A parsec is a parallax of 1second of arc, or 1/3,600 th of a degree. 3.Luminosity ~ is the basis of magnitudes. Luminosity is the energy output from the surface of the body.

The light shown by stars are based upon what they are made of, and if the star is moving. 1.Lines of absorption show what elements are in a star, because of dark patches on the rainbow. 2.Lines of emission show what elements are in a star, because of bright patches.

The light shown by stars are based upon what they are made of, and if the star is moving. 1.Lines of absorption show what elements are in a star, because of dark patches on the rainbow. 2.Lines of emission show what elements are in a star, because of bright patches. 3.If a star is moving away, light is stretched out the Doppler effect, and it will appear redder. 4.If a star is moving towards an observer, the Doppler effect compresses light, and it will appear bluer.

The Doppler effect is when the wavelength or speed of an energy source is apparently changing, based upon the changing location of source or the observer. 45 mph Sound of engine will seem lower Sound of engine will seem higher

Show Doppler effect animation here

Airplane is flying at 400 m/s, and bullet shoots ahead at 400 m/s. What is the speed and direction of the bullet relative to the airplane?

400 meters per second straight ahead

Airplane is flying at 400 m/s, and bullet shoots ahead at 400 m/s. What is the speed and direction of the bullet relative to the ground?

800 meters per second horizontally

Both airplanes are flying at 400 m/s, and the lead airplane shoots straight back, with a bullet that has a speed of 400 m/s. What is the speed and direction of the bullet relative to the first airplane?

400 meters per second straight backwards

Both airplanes are flying at 400 m/s, and the lead airplane shoots straight back, with a bullet that has a speed of 400 m/s. What is the speed and direction of the bullet relative to the following airplane?

400 meters per second, straight at him!!!!!!!!

Both airplanes are flying at 400 m/s, and the lead airplane shoots straight back, with a bullet that has a speed of 400 m/s. What is the speed and direction of the bullet relative to the ground?

It will fall straight down.

Actually, I made all these cases a bit more simplistic, because gravity will have an effect in all of these cases. It will make all of these bullets accelerate towards the Earth with a change in velocity of 9.8 meters per second per second.

Both airplanes are flying at 400 m/s. Will the sound of plane "a" be higher, lower, or the same as plane "b", to the pilot of plane "b"? ab

ab It would be the same, because the relative speed between the two is zero meters per second. There is no Doppler effect.

Both airplanes are flying at 400 m/s. Will the sound of plane "a" be higher, lower, or the same as plane "b", to the person on the ground? ab

ab

ab Plane “a” would be higher, because it is “pushing” the sound ahead of it ~ because of its higher relative speed than plane “b”

Both airplanes are flying at 400 m/s. Will the sound of plane "a" be higher, lower, or the same as plane "b", to the person on the ground? ab Plane “b” would be lower to Albert, because it is stretching out the sound waves.. But to each other, they are the same.

a b Spaceship "b" shoots a "photon torpedo" at "a". What will be the speed of the "photon torpedo" when it reaches "a"? “c” is the speed of light, or 300,000,000 m/s Speed is 1/3 c, 100,000,000 m/s Speed is 0 c

a b Spaceship "b" shoots a "photon torpedo" at "a". What will be the speed of the "photon torpedo" when it reaches "a"? Speed is 1/3 cSpeed is 0 c It MUST be 300,000,000 meters per second. ALWAYS. It will, however, be REDSHIFTED, because the wavelengths are stretched out.

H-R Diagram 1.The H-R diagram shows a relationship between the absolute magnitude / the temperature of a star, and the size of a star. 2.Stars move around on the H-R diagram. Ours is a main sequence star (most are), but not all.