Spectral Star Analysis

Slides:



Advertisements
Similar presentations
Chapter 11: Characterizing Stars
Advertisements

ASTR 1200 Announcements Website HW #1 along back walkway Lecture Notes going up on the website First.
Stars Flux and Luminosity Brightness of stars and the magnitude scale Absolute magnitude and luminosity Distance modulus Temperature vs heat Temperature.
STARS  Stars are the pieces of our universe.  Each star is fixed in a certain spot in its Galaxy.  Planets and other things orbit in a solar system.
Announcements Observing on the roof of Van Allen Hall has started and will run Tuesday to Thursday from 9-11 pm this week. The first hour exam will be.
Stellar Temperatures Wien’s law works perfectly for objects with Planck spectra. Stars don’t quite have Planck-like spectra. UV Blue Green Red Infrared.
Survey of the Universe Tom Burbine
ASTR100 (Spring 2008) Introduction to Astronomy Properties of Stars Prof. D.C. Richardson Sections
Guiding Questions How far away are the stars?
Properties of Stars How do we measure stellar luminosities?
Properties of Stars. Distance Luminosity (intrinsic brightness) Temperature (at the surface) Radius Mass.
Surveying the Stars.
Susan CartwrightOur Evolving Universe1 Atoms and Starlight n Why do the stars shine? l l planets shine by reflected sunlight—but what generates the Sun’s.
Telescopes (continued). Basic Properties of Stars.
Stellar Spectra AST 112 Lecture 7.
How Do Astronomers Measure the Brightness of a Star?  Stars vary greatly in brightness  Early peoples observed bright stars and grouped them into constellations.
Surveying the Stars Insert TCP 5e Chapter 15 Opener.
Chapter 10 Measuring the Stars. Units of Chapter 10 The Solar Neighborhood Luminosity and Apparent Brightness Stellar Temperatures Stellar Sizes The Hertzsprung-Russell.
Units to cover: 53, 26, 27, 55, 56. The Solar Cycle The number of sunspots seen increases and decreases periodically. Every 11 years or so, the sunspot.
HR Diagram. Characteristics of Stars  Temperature/Color  Mass  Luminosity Absolute Magnitude Apparent Magnitude.
Stellar Spectra Colors/spectra of stars Classifying stars Photons Atomic structure Elements in stars Masses of stars Mass-luminosity relation Reading:
Spectroscopy – the study of the colors of light (the spectrum) given off by luminous objects. Stars have absorption lines at different wavelengths where.
Properties of Stars.
Chapter 11 Surveying the Stars Properties of Stars Our Goals for Learning How luminous are stars? How hot are stars? How massive are stars?
Charles Hakes Fort Lewis College1. Charles Hakes Fort Lewis College2.
Atoms & Light (Spectroscopy). Blackbody Radiation A. Blackbody = a hot solid, hot liquid, or hot high density gas that emits light over a range of frequencies.
Main Classes of Stars Astrophysics Lesson 10. Homework  None, you have exams next week! Good Luck!
Stellar Characteristics. Temperature Temp. is measured in Kelvins Blue stars are hot, above 30,000 K Yellow stars are warm Red stars are cool, below 3,000.
Chapter 11 Surveying the Stars The brightness of a star depends on both distance and luminosity How luminous are stars?
StarsStars. A Star…. Heats and lights the planets in a solar system Is a ball of plasma (4 th state of matter consisting of ionized particles) held together.
Classification of Stars – HR diagram Objectives: understand the differences between near and bright visible stars learn how to use the HR-diagram to classify.
ASTR 1200 Announcements Exam #1 in class, next Tuesday, October 7
Chapter 10 The Nature of Stars. What do you think? What color are stars? Are most stars isolated from other stars, like the Sun?
Astrophysics of Life : Stars. 2 Wave Characteristics: Wavelength - Distance between successive wave peaks Period – Time between passing wave peaks Frequency.
Stars Luminous gaseous celestial body – spherical in shape held by its own gravity.
Chapter 3 Stars: Radiation  Nick Devereux 2006 Revised 2007.
Eclipsing Binaries. If the binary stars are eclipsing, then it is guaranteed that we are in the orbital plane. This means that the maximum radial velocity.
Intro to Astrophysics Dr. Bill Pezzaglia 1 Updated: Nov 2007.
Chapter 10 Measuring the Stars. Star Cluster NGC ,000 light-years away.
How Do Astronomers Measure the Brightness of a Star? Stars vary greatly in brightness Stars vary greatly in brightness Early peoples observed bright stars.
Investigating Astronomy
© 2011 Pearson Education, Inc. Chapter 17 Measuring the Stars.
© 2010 Pearson Education, Inc. Most luminous stars: 10 6 L Sun Least luminous stars: 10 –4 L Sun (L Sun is luminosity of Sun)
CHAPTER 10: THE STARS. S&T P Why do astronomers need to know the apparent brightness and luminosity of stars? The relationship between AB and.
CSI661/ASTR530 Spring, 2011 Chap. 2 An Overview of Stellar Evolution Feb. 02, 2011 Jie Zhang Copyright ©
© 2017 Pearson Education, Inc.
STARS.
Stars Luminous gaseous celestial body – spherical in shape held by its own gravity.
Chapter 10: The Stars.
Stars! How do we know what we know about stars?
CH2. An Overview of Stellar Evolution
Star Characteristics.
Questions 1 – 24: Due Wednesday, February 29, 5:00 pm.
Wien’s Law The Color and Temperature of Stars.
Star Classification.
Wien’s Law The Color and Temperature of Stars.
Characteristics of Stars Chapter 3 Section 4 ISN p. 33
Chapter 11: Characterizing Stars
ASTR 1020 – February 16 { } O B A F G K M .
Black body radiation Why do objects have colour? Would this effect the light they emit if they were hot? What colour would a cold star be?
“Beyond the solar system where no man
HR Diagram.
Characteristics of Stars
To help understand the HR Diagram 
Distance to the Stars How can the distance to a star be measured?
Stellar Classification
The HR diagram.
The Temperature of a Star
Goals Explain how we measure stellar distances Explain the difference between apparent and absolute brightness Explain how we classify stars Describe the.
The Temperature of a Star
Presentation transcript:

Spectral Star Analysis Astrophysics Spectral Star Analysis

Diagram Placements Spectral Analysis ? How do we place them? The process of determining stellar types from observed spectral absorption lines.

Obtaining a Stellar Spectrum

Spectral Key

Spectral Key

Spectral Types “Oh, Be A Fine Guy/Girl, Kiss Me” O B A F G K M Each class is subdivided 0-9 i.e. B0, B1, … B9, A0, … Then further sub divided by Roman Numerals (I – V) And additionally divided alphabetically (a, b, c, d, etc…)

Spectral Types Temperature Variations Color Variations O: hottest, M: coolest Color Variations O, B: Blue A, F, G: Yellow/Orange K, M: Red

Spectral Types O >16 B 2.1 – 16 A 1.4 – 2.1 F 1.04 – 1.4 G Spectral Class Mass (in multiples of the Sun’s mass) O >16 B 2.1 – 16 A 1.4 – 2.1 F 1.04 – 1.4 G 0.8 – 1.04 K 0.45 – 0.8 M 0.08 – 0.45

d Leo b Leo 15_Monocerous

s Leo HD-27808 Rho Auriga

Wein’s Law

Temperature from Wavelength Wien’s Law lmax*T = 0.290 cm K