Wikipedia - Stellar classification:
|
|
- Anabel Chase
- 5 years ago
- Views:
Transcription
1 Stars and Hertzprung-Russell Diagram Introductory Astronomy laboratory exercise with Stellarium Mike Chu Name Stellarium is an open source and cross-platform application from A star is mainly categorized by its spectral class and absolute magnitude. The spectral type also is referred to as color and it is an indication of the surfacetemperature of the star. Absolute magnitude tells information about the luminosity, or the rate of energy output, of a star. The term spectral type originally pertains to the method of observation in which the spectra of a star is recorded and then the star type is categorized according to the pattern shown in the spectra. Now astronomers have a solid understanding of the physical mechanism to and connection between spectral patterns and surface temperature. There are seven major spectral classes, from hotter classes to colder classes, denoted by the letters O, B, A, F, G, K, M. Each spectral class is furthered subdivided into 10 smaller subclasses indicated by a number from 0 to 9. For example: an A5 star is colder than A0 but hotter than A9 furthermore A9 is hotter than the first subclass of next spectral class F0, and so on. Below is an excerpt from Wikipedia listing the common information about each spectral class. There are additional spectral classes not shown below and are not needed for this work. Wikipedia - Stellar classification: 1
2 The Hertzsprung-Russell (HR) diagram is simply a scatter plot of Absolute Magnitude versus the Spectral Type that exhibits very tell-tale patterns about stars and stellar evolution. The plot is easily constructed from a sufficiently large set of data of absolute magnitude and spectral type of stars. In this lab, the application Stellarium will be used to obtain data from the built-in stellar data. Suggestion for instructor: 1) This exercise may be conducted as an individual exercise where each student is asked to map out the diagram with enough selected star information. 2) The exercise can also be conducted in collaboration where each student is to focus on a particular constellation 3) As this exercise is simple and that Stellarium is highly flexible, creativity is encouraged to make this lab fun and illuminating. Stellarium Instruction: 1) Open up Stellarium, and toggle off Atmosphere, Ground and Nebulae on the bottom menu. 2) Click the search button on the left icon bar (or F3, or ctrl-f3) and search for a common bright star such as Sirius, Betelgeuse, or Rigel or simply find any bright named star on the screen and right-click on the star - the star information will be displayed on the top left corner which will include Absolute Magnitude and Spectral Type. 3) In Stellarium, the spectral class of a star typically is given by more than three letters or characters, such as F0lb. The extra characters or numbers beyond the first 2 places provide additional information such as luminosity class but will not be needed. Make sure that the stars of higher magnitude, or lower visibility, are turned on. This gives a better representation of the available stars, and not just the bright ones, and a more correct look of the HR diagram. Go to Sky View and options, select Sky tab, and find relative scale. Set relative scale from 1.0 to about 0.5. You can turn off all labels of planets, stars and other unnecessary markings for a cleaner visual. If later you find yourself not able to obtain enough faint stars then lower the relative further to see more even fainter stars. (To be improved) 2
3 Examples of stars and their corresponding spectral type: Betelgeuse M2lb Sirius A0M Rigel B8la HIP GIV 4) a. If necessary to show constellations and boundaries, go to Sky and viewing option window [F4] on the left menu, select the Markings tab: Check Show lines, Show labels and Show Boundaries b. Zoom into the constellation of your choice by using mouse or touch pad scroll. 6) Find 5 to 10 stars of each of 7 spectral types, and fill up a table or spreadsheet with enough star information. Anywhere between 45 to 75 stars may be sufficient to illuminate the main features of the HR diagram (you will need to determine the diagram quality visually). Be sure to include some of the very faint stars not easily visible on the screen or the resulting HR diagram may not correctly demonstrate some features. For each star, obtain the following information: Absolute magnitude Spectral type Constellation (for plotting purpose spectral type represented by numbers. See below) 7) Complete your spreadsheet. An example spreadsheet with only 3 stars is shown below: Illustration 1: Example spreadsheet with star information including Absolute Magnitude, Spectral Type, Constellation and the ad-hoc Converted Spectral Type The Converted Spectral Type is an ad-hoc creation for the purpose of plotting Absolute Magnitude versus Spectral Type. The spreadsheet plotting-function will not be able to recognize characters (such as M2 or K1 of spectral type) as numerical input, thus for plotting purpose the ad-hoc conversion is made to convert spectral 3
4 types into numbers but following the same order. This ad-hoc conversion is done by replacing the character O-B-A-F-G-K-M with the number : O 1 B 2 A 3 F 4 G 5 K 6 M 7 In the example spreadsheet, M2 is turned into 72 by replacing M with 7, B0 is converted into 20 by replacing B with 2, and K1 is changed to 61 by replacing K with 6. With both Absolute Magnitude and Spectral Type represented by numbers, a scattered plot then can be generated using the spreadsheet plotting function. 7) Plot Absolute Magnitude on the y-axis versus Spectral Type* Converted on the x-axis. (Instruction for Libre Office is to be given in Spring, 2015) Here is a quick and dirty instruction for Excel plot. Simply use your mouse and select all your input on the spreadsheet. Then go to Insert on the top menu bar (next to Home ) select Chart select Scatter Choose Marked Scattered (Scatter with only Markers) type, which is the first choice. You will see a plot but do not worry about the first appearance. It will be fixed via some adjustments. Under Design (make sure you click on the plot first), click Select Data icon in the icon bar (not the Data tab on top). (You will need to remove Series 1, which we do not want). Under Legend Entrees (Series) click Add. Here you will select the data for x-axis and y-axis. Click inside the entry row of Series X values: to make sure the cursor is active within (a flash vertical bar). Now you are ready to select x-axis. Use your mouse to select all data under the Converted Spectral Type. Then hit Enter. (The simple idea is to use Converted Spectral Type for x-axis). For Series Y values:, click on the entry row and then select all data under Absolute Magnitude. Hit Enter. 4
5 Now that you see a plot and think you are done. Not quite! Your nice looking HR diagram may still look nothing like ones shown in text or online resources. Do recall that the magnitude scale, for seemingly strange but sound historical development, is one scale in which the brighter the star the more negative the number. That means the Absolute Magnitude as labeled on the y-axis that you are seeing, is plotted in reverse. So let's revers it. Right click (or maybe just click) on y-axis area > select Format Axis then finally under Axis Options, check the box of Values in reverse order. You should now see a correct HR digram representation of your work. Do check to see if your dataset is sufficient to display the main features of the HR diagram. Consult any reputable online resource. See below link with Excel plotting function: 8) (Per Instruction) your spreadsheet to your instructor. Be sure to include your name, the selected constellation and other important information. A follow up exercise can be built from the overall class result. List of Constellation (Wikipedia): You will be assigned a constellation region. 5
Introduction to Astronomy Laboratory Exercise #1. Intro to the Sky
Introduction to Astronomy Laboratory Exercise #1 Partners Intro to the Sky Date Section Purpose: To develop familiarity with the daytime and nighttime sky through the use of Stellarium. Equipment: Computer
More informationStudents will explore Stellarium, an open-source planetarium and astronomical visualization software.
page 22 STELLARIUM* OBJECTIVE: Students will explore, an open-source planetarium and astronomical visualization software. BACKGROUND & ACKNOWLEDGEMENTS This lab was generously provided by the Red Rocks
More informationLab 3: Stars, Stars, Stars!
Lab 3: Stars, Stars, Stars! The Hertzsprung-Russell Diagram Today we will learn about the different types of stars and how they are different form one another. Go to http://astro.unl.edu/naap/hr/hr.html.
More informationColor-Magnitude Diagram Lab Manual
Color-Magnitude Diagram Lab Manual Due Oct. 21, 2011 1 Pre-Lab 1.1 Photometry and the Magnitude Scale The brightness of stars is represented by its value on the magnitude scale. The ancient Greek astronomer
More informationASTRO 1050 The Seven Sisters, and Lives of the Stars
ASTRO 1050 The Seven Sisters, and Lives of the Stars ABSTRACT There is a conspicuous nest of stars, or star cluster, in the winter and spring sky called the Pleiades, or Seven Sisters. By plotting a luminosity-temperature
More informationStar Cluster Photometry and the H-R Diagram
Star Cluster Photometry and the H-R Diagram Contents Introduction Star Cluster Photometry... 1 Downloads... 1 Part 1: Measuring Star Magnitudes... 2 Part 2: Plotting the Stars on a Colour-Magnitude (H-R)
More informationStellarium Walk-through for First Time Users
Stellarium Walk-through for First Time Users Stellarium is the computer program often demonstrated during our planetarium shows at The MOST, Syracuse s science museum. It is our hope that visitors to our
More informationAstronomy 101 Lab: Stellarium Tutorial
Name: Astronomy 101 Lab: Stellarium Tutorial Please install the Stellarium software on your computer using the instructions in the procedure. If you own a laptop, please bring it to class. You will submit
More informationAstron 104 Laboratory #8 The H-R Diagram
Name: Date: Section: Astron 104 Laboratory #8 The H-R Diagram Section 10.1, 10.5 Introduction The Hertzsprung-Russell diagram, or H-R diagram for short, relates two fundamental properties of stars and
More informationAssignment #0 Using Stellarium
Name: Class: Date: Assignment #0 Using Stellarium The purpose of this exercise is to familiarize yourself with the Stellarium program and its many capabilities and features. Stellarium is a visually beautiful
More informationLab 8: Stellar Classification and the H-R Diagram
Name: Section: Date: Lab 8: Stellar Classification and the H-R Diagram 1 Introduction Stellar Classification As early as the beginning of the 19th century, scientists have studied absorption spectra in
More informationAstro 101 Lab #1. To advance time forward and backward, click on the arrow toolbar. From left to right, the buttons will
Name: Astro 101 Lab #1 Lab objectives 1) Learn how to use the Stellarium planetarium program, by becoming familiar with the user interface and configuring the planetarium to your present location on Earth.
More informationThe Hertzsprung-Russell Diagram
The Hertzsprung-Russell Diagram Our Objectives To determine the physical properties of the stars; to learn how they differ; and to understand why those differences arise We can now get around the problem
More informationTHE STARS. Information and contacts: -
THE STARS G. Iafrate (a), M. Ramella (a) and V. Bologna (b) (a) INAF - Astronomical Observatory of Trieste (b) Istituto Comprensivo S. Giovanni Sc. Sec. di primo grado M. Codermatz" - Trieste Information
More informationMaking an H-R diagram Earth & Sky
Making an H-R diagram Earth & Sky Name: Introduction Astronomers have discovered relationships between the surface temperatures and luminosities (brightnesses) of stars. These relationships are often presented
More informationPhysics Lab #6:! Mercury!
Physics 10293 Lab #6: Mercury Introduction Today we will explore the motions in the sky of the innermost planet in our solar system: Mercury. Both Mercury and Venus were easily visible to the naked eye
More informationThe Hertzsprung-Russell Diagram
The Hertzsprung-Russell Diagram Name: Date: 1 Introduction As you may have learned in class, the Hertzsprung-Russell Diagram, or the HR diagram, is one of the most important tools used by astronomers:
More informationA1101, Lab 5: The Hertzsprung- Russell Diagram Laboratory Worksheet
Student Name: Lab TA Name: A1101, Lab 5: The Hertzsprung- Russell Diagram Laboratory Worksheet One of the most basic physical properties of a star is its luminosity, the rate at which it radiates energy
More informationCOLOR MAGNITUDE DIAGRAMS
COLOR MAGNITUDE DIAGRAMS What will you learn in this Lab? This lab will introduce you to Color-Magnitude, or Hertzsprung-Russell, Diagrams: one of the most useful diagnostic tools developed in 20 th century
More informationHR Diagram Student Guide
Name: HR Diagram Student Guide Pretest Score: Background Information Work through the background sections on Spectral Classification, Luminosity, and the Hertzsprung-Russell Diagram. Then complete the
More informationSkyGlobe Planetarium
SkyGlobe Planetarium Introduction: This exercise will simulate the night sky and demonstrate a number of principles of the celestial sphere and the motions of the Earth and planets. Getting Started: 1.
More informationThe Hertzsprung-Russell Diagram and Stellar Evolution
The Hertzsprung-Russell Diagram and Stellar Evolution Names: The H-R Diagram and Stellar Properties Activity 1. In which corner of the diagram (upper right, upper left, lower right, or lower left) would
More informationLAB: Photometry of the Pleiades Cluster
LAB: Photometry of the Pleiades Cluster ASTR 203 - Instructors Olszewski & Rigby Due IN CLASS on Oct. 30 You may work with 1 partner. If you do, only turn in 1 assignment with both your names on it! You
More informationComputer simulation of radioactive decay
Computer simulation of radioactive decay y now you should have worked your way through the introduction to Maple, as well as the introduction to data analysis using Excel Now we will explore radioactive
More informationHOMEWORK 4: H-R DIAGRAM
NAME(S) SECTION DAY/TIME ASTRONOMY25 (LLOYD) SPRING 2012 Purpose HOMEWORK 4: H-R DIAGRAM To plot the H-R diagram of a star cluster and estimate its age and distance. Background Magnitude is a measure of
More informationFor instance, for a particular star cluster, these data were derived:
Astronomy 100 Name(s): Exercise 5: The H-R diagram and spectroscopy A very basic correlation using the color index By the 1920 s, various astronomers had evidence that the temperature of a star was also
More informationAssignment #12 The Milky Way
Name Date Class Assignment #12 The Milky Way For thousands of years people assumed that the stars they saw at night were the entire universe. Even after telescopes had been invented, the concept of a galaxy
More informationWrite It! Students should be encouraged to do the Research and Explore station before attempting this one.
Kesler Science Station Lab H-R Diagram Teacher Directions Explore It! I will spend much of my time at this station making sure that the students are doing the Celebrity H-R diagram correctly and not wasting
More informationThe Mass of Jupiter Student Guide
The Mass of Jupiter Student Guide Introduction: In this lab, you will use astronomical observations of Jupiter and its satellites to measure the mass of Jupiter. We will use the program Stellarium to simulate
More informationPhotometry of Messier 34
Photometry of Messier 34 J. Kielkopf November 12, 2012 1 Messier 34 The open cluster Messier 34 (M34) is in the solar neighborhood, lying roughly in the plane of the Milky Way galaxy in the direction of
More informationAstronomy 102 Lab: Stellar Parallax and Proper Motion
Name: Astronomy 102 Lab: Stellar Parallax and Proper Motion If you own a laptop, please bring it to class. You will use Stellarium again. The Stellarium shortcuts you used in the first lab are on the inside
More informationASTR-1020: Astronomy II Course Lecture Notes Section III
ASTR-1020: Astronomy II Course Lecture Notes Section III Dr. Donald G. Luttermoser East Tennessee State University Edition 4.0 Abstract These class notes are designed for use of the instructor and students
More informationFree Fall. v gt (Eq. 4) Goals and Introduction
Free Fall Goals and Introduction When an object is subjected to only a gravitational force, the object is said to be in free fall. This is a special case of a constant-acceleration motion, and one that
More informationPhotometry of Supernovae with Makali i
Photometry of Supernovae with Makali i How to perform photometry specifically on supernovae targets using the free image processing software, Makali i This worksheet describes how to use photometry to
More informationPhotoelectric Photometry of the Pleiades
Photoelectric Photometry of the Pleiades Student Manual A Manual to Accompany Software for the Introductory Astronomy Lab Exercise Document SM 2: Version 1 Department of Physics Gettysburg College Gettysburg,
More informationObjectives: (a) To understand how to display a spectral image both as an image and graphically.
Texas Tech University Department of Physics & Astronomy Astronomy 2401 Observational Astronomy Lab 8:- CCD Image Analysis:- Spectroscopy Objectives: There are two principle objectives for this laboratory
More informationLAB B. The Local Stellar Population
KEELE UNIVERSITY SCHOOL OF PHYSICAL AND GEOGRAPHICAL SCIENCES Year 1 ASTROPHYSICS LAB LAB B. The Local Stellar Population R. D. Jeffries version January 2010 D. E. McLaughlin Throughout this experiment
More informationOrganizing the Family of Stars:
Organizing the Family of Stars: We know: Stars have different temperatures, different luminosities, and different sizes. To bring some order into that zoo of different types of stars: organize them in
More informationSpectral Classification of Stars
Department of Physics and Geology Spectral Classification of Stars Astronomy 1402 Part 1: Background Spectral Classification of Stars 1.1 Spectral Types: O, B, A, F, G, K, M On a dark, clear night far
More informationHertzsprung-Russel Diagrams and Distance to Stars
Chapter 10 Hertzsprung-Russel Diagrams and Distance to Stars 10.1 Purpose In this lab, we will explore how astronomer classify stars. This classificatin one way that can be used to determine the distance
More informationPhotoelectric Photometry of the Pleiades Student Manual
Name: Lab Partner: Photoelectric Photometry of the Pleiades Student Manual A Manual to Accompany Software for the Introductory Astronomy Lab Exercise Edited by Lucy Kulbago, John Carroll University 11/24/2008
More information5E Lesson Plan Template
Handout Authors: Ashley Thornburg Austin Ross Title of Lesson: The Life Cycle of Stars Date of Lesson: Wednesday March 14, 2012 Length of Lesson: 40-45 minutes Name/Level of Course: Science 8 th Source
More informationEXCELLING WITH BIOLOGICAL MODELS FROM THE CLASSROOM T0 RESEARCH
EXCELLING WITH BIOLOGICAL MODELS FROM THE CLASSROOM T0 RESEARCH Timothy D. Comar Benedictine University Department of Mathematics 5700 College Road Lisle, IL 60532 tcomar@ben.edu Introduction Computer
More informationProperties of Stars & H-R Diagram
Properties of Stars & H-R Diagram What is a star? A cloud of gas, mainly hydrogen and helium The core is so hot/dense that nuclear fusion can occur. The fusion converts light nuclei (elements) into heavier
More informationStudying Topography, Orographic Rainfall, and Ecosystems (STORE)
Studying Topography, Orographic Rainfall, and Ecosystems (STORE) Introduction Basic Lesson 3: Using Microsoft Excel to Analyze Weather Data: Topography and Temperature This lesson uses NCDC data to compare
More informationMeasuring stellar distances.
Measuring stellar distances This method can be used to measure distances up to 100pc Some new technology allows measuring distances up to 200pc using this method p= 1/d Stellar Parallax.htm This method
More informationUsing Microsoft Excel
Using Microsoft Excel Objective: Students will gain familiarity with using Excel to record data, display data properly, use built-in formulae to do calculations, and plot and fit data with linear functions.
More informationMolecular Modeling and Conformational Analysis with PC Spartan
Molecular Modeling and Conformational Analysis with PC Spartan Introduction Molecular modeling can be done in a variety of ways, from using simple hand-held models to doing sophisticated calculations on
More informationIntroduction to Computer Tools and Uncertainties
Experiment 1 Introduction to Computer Tools and Uncertainties 1.1 Objectives To become familiar with the computer programs and utilities that will be used throughout the semester. To become familiar with
More informationStudent Exploration: H-R Diagram
Name: Date: Student Exploration: H-R Diagram Vocabulary: giant, H-R diagram, luminosity, main sequence, star, supergiant, white dwarf Prior Knowledge Questions (Do these BEFORE using the Gizmo.) 1. The
More informationLife Cycle of Stars. Photometry of star clusters with SalsaJ. Authors: Daniel Duggan & Sarah Roberts
Photometry of star clusters with SalsaJ Authors: Daniel Duggan & Sarah Roberts Photometry of star clusters with SalsaJ Introduction Photometry is the measurement of the intensity or brightness of an astronomical
More informationExperiment 0 ~ Introduction to Statistics and Excel Tutorial. Introduction to Statistics, Error and Measurement
Experiment 0 ~ Introduction to Statistics and Excel Tutorial Many of you already went through the introduction to laboratory practice and excel tutorial in Physics 1011. For that reason, we aren t going
More informationStar Magnitudes & Distances with Stellarium (Stellarium Exercise #2)
Name Date Star Magnitudes & Distances with Stellarium (Stellarium Exercise #2) Millions of stars are scattered across the sky. Astronomers want to study these stars as carefully as possible. This means
More informationPhotoelectric Photometry of the Pleiades
Photoelectric Photometry of the Pleiades Student Manual A Manual to Accompany Software for the Introductory Astronomy Lab Exercise Document SM 2: Version 0.96lab Department of Physics Gettysburg College
More informationCLEA/VIREO PHOTOMETRY OF THE PLEIADES
CLEA/VIREO PHOTOMETRY OF THE PLEIADES Starting up the program The computer program you will use is a realistic simulation of a UBV photometer attached to a small (diameter=0.4 meters) research telescope.
More informationLines of Hydrogen. Most prominent lines in many astronomical objects: Balmer lines of hydrogen
The Family of Stars Lines of Hydrogen Most prominent lines in many astronomical objects: Balmer lines of hydrogen The Balmer Thermometer Balmer line strength is sensitive to temperature: Most hydrogen
More informationH-R Diagram Lab. Vocabulary:
H-R Diagram Lab Vocabulary: luminosity: brightness dependent on a star s size; temperature and distance spectral class: classification of stars by their spectrum and luminosity magnitude: measure of the
More informationI. Introduction. II. An Introduction to Starry Night NAME: ORBITAL MOTION
NAME: ORBITAL MOTION What will you learn in this Lab? You will be using some special software to simulate the motion of planets in our Solar System and across the night sky. You will be asked to try and
More informationDAY LABORATORY EXERCISE: SPECTROSCOPY
AS101 - Day Laboratory: Spectroscopy Page 1 DAY LABORATORY EXERCISE: SPECTROSCOPY Goals: To see light dispersed into its constituent colors To study how temperature, light intensity, and light color are
More informationBackground and Theory
Homework 4. Cluster HR Diagrams and the Age of Stars NAME: Due: Thursday, October 7, 2010 In Class Astro 201: Cosmology Prof. Bechtold In this assignment, we are going to measure the age of stars in star
More informationPOC via CHEMnetBASE for Identifying Unknowns
Table of Contents A red arrow was used to identify where buttons and functions are located in CHEMnetBASE. Figure Description Page Entering the Properties of Organic Compounds (POC) Database 1 Swain Home
More informationOkay now go back to your pyraf window
PHYS 391 Astronomical Image Data: Measuring the Distance and Age of a Stellar Cluster Goals This lab is designed to demonstrate basic astronomy data analysis and how extracting stellar population information
More informationHow to Make or Plot a Graph or Chart in Excel
This is a complete video tutorial on How to Make or Plot a Graph or Chart in Excel. To make complex chart like Gantt Chart, you have know the basic principles of making a chart. Though I have used Excel
More informationPhotoelectric Photometry of the Pleiades Student Manual
Photoelectric Photometry of the Pleiades Student Manual A Manual to Accompany Software for the Introductory Astronomy Lab Exercise Document SM 2: Version 1.1.1 lab Department of Physics Gettysburg College
More informationAstron 104 Laboratory #9 The H-R Diagram
Name: Date: Section: Astron 104 Laboratory #9 The H-R Diagram Section 10.1, 10.5 If we know the temperature of a star (or its Spectral Type) and the stars intrinsic brightness (or luminosity), a great
More informationOUTSIDE LAB 1: Observing the Heavens
OUTSIDE LAB 1: Observing the Heavens OBJECTIVE: To become familiar with some of the more conspicuous constellations and to observe the motions of stars in the night sky. DISCUSSION: Most people are unfamiliar
More informationMotion II. Goals and Introduction
Motion II Goals and Introduction As you have probably already seen in lecture or homework, and if you ve performed the experiment Motion I, it is important to develop a strong understanding of how to model
More informationAstronomy 102 Lab: Distance to the Pleiades
Name: Astronomy 102 Lab: Distance to the Pleiades Please bring your textbook to class. Use a pencil when plotting the points on the graphs. Pre-Lab Assignment: From the planetarium, you know the Pleiades
More informationExperiment: Oscillations of a Mass on a Spring
Physics NYC F17 Objective: Theory: Experiment: Oscillations of a Mass on a Spring A: to verify Hooke s law for a spring and measure its elasticity constant. B: to check the relationship between the period
More informationExperiment 13. Dilutions and Data Handling in a Spreadsheet rev 1/2013
Absorbance Experiment 13 Dilutions and Data Handling in a Spreadsheet rev 1/2013 GOAL: This lab experiment will provide practice in making dilutions using pipets and introduce basic spreadsheet skills
More informationAstronomy 201: Cosmology, Fall Professor Edward Olszewski and Charles Kilpatrick
Astronomy 201: Cosmology, Fall 2013 Professor Edward Olszewski and Charles Kilpatrick Lab 3, Cluster Hertzsprung-Russell Diagrams and the Age of Stars Due October 22, Worth 32 points You may work in groups
More informationLab 6: The Planets and Kepler
Lab 6: The Planets and Kepler The Motion of the Planets part I 1. Morning and Evening Stars. Start up Stellarium, and check to see if you have the Angle Tool installed it looks like a sideways A ( ) in
More information5. A particular star has an angle of parallax of 0.2 arcsecond. What is the distance to this star? A) 50 pc B) 2 pc C) 5 pc D) 0.
Name: Date: 1. How far away is the nearest star beyond the Sun, in parsecs? A) between 1 and 2 pc B) about 12 pc C) about 4 pc D) between 1/2 and 1 pc 2. Parallax of a nearby star is used to estimate its
More informationLarge Scale Structure of the Universe Lab
Large Scale Structure of the Universe Lab Introduction: Since the mid-1980 s astronomers have gathered data allowing, for the first time, a view of the structure of the Universe in three-dimensions. You
More information5-Sep-15 PHYS101-2 GRAPHING
GRAPHING Objectives 1- To plot and analyze a graph manually and using Microsoft Excel. 2- To find constants from a nonlinear relation. Exercise 1 - Using Excel to plot a graph Suppose you have measured
More informationClassifying the stars: from dwarfs to supergiants
Classifying the stars: from dwarfs to supergiants By SAO Encyclopedia of Astronomy, Big History Project, adapted by Newsela staff on 08.22.17 Word Count 697 Level 1170L Artist s depiction of the life cycle
More informationTHE MOON. G. Iafrate (a), M. Ramella (a) e V. Bologna (b) (a) INAF - Osservatorio Astronomico di Trieste (b)
THE MOON G. Iafrate (a), M. Ramella (a) e V. Bologna (b) (a) INAF - Osservatorio Astronomico di Trieste (b) Istituto Comprensivo S. Giovanni Sc. Sec. di primo grado M. Codermatz" - Trieste Information
More informationCHARTING THE HEAVENS USING A VIRTUAL PLANETARIUM
Name Partner(s) Section Date CHARTING THE HEAVENS USING A VIRTUAL PLANETARIUM You have had the opportunity to look at two different tools to display the night sky, the celestial sphere and the star chart.
More informationQuestion: How do we use a Hertzsprung-Russell Diagram to explain star characteristics?
The Hertzsprung-Russell Diagram Assignment Introduction: The development of the H-R Diagram began with Danish astronomer Ejnar Hertzsprung who began plotting the stars around 1911. American astronomer
More informationTHE PLEIADES OPEN CLUSTER
THE PLEIADES OPEN CLUSTER G. Iafrate (a), M. Ramella (a) and P. Padovani (b) (a) INAF - Astronomical Observatory of Trieste (b) ESO - European Southern Observatory 1 Introduction Open star clusters are
More informationOPEN CLUSTERS LAB. I. Introduction: II. HR Diagram NAME:
NAME: OPEN CLUSTERS LAB What will you learn in this Lab? An open cluster is a group of stars that were born at the same time and can be studied to determine both the distance and age of the member stars
More informationMass-Luminosity and Stellar Lifetimes WS
Name Mass-Luminosity and Stellar Lifetimes WS The graph shows the Mass-Luminosity Relationship for main sequence stars. Use it to answer questions 1-3. 1) A star with a mass of 0.5 solar masses would be
More informationCharacteristics of Stars
Characteristics of Stars This section explains how astronomers measure distances to stars. It also describes how stars are classified. Use Target Reading Skills As you read about stars, stop and write
More informationLocation Latitude Longitude Durham, NH
Name: Date: Weather to Climate Investigation: Snow **These are example answers using the Durham, NH dataset. Answers from students using Boise and Little Rock datasets will differ. Guiding Questions: What
More informationAstron 104 Laboratory #12 Hubble s Law
Name: Date: Section: Astron 104 Laboratory #12 Hubble s Law Section 15.3 In this lab, you investigate Hubble s Law, an empirical law which relates the speed with which galaxies recede from us to their
More informationPhysics Lab #5: Starry Night Observations of the Sun and Moon
Physics 10293 Lab #5: Starry Night Observations of the Sun and Moon Introduction Today, we are going to use the Starry Night software to learn about motion of the stars, sun and moon on the celestial sphere.
More informationLecture 10: The Hertzsprung-Russell Diagram Reading: Sections
Lecture 10: The Hertzsprung-Russell Diagram Reading: Sections 19.7-19.8 Key Ideas The Hertzsprung-Russell (H-R) Diagram Plot of Luminosity vs. Temperature for stars Features: Main Sequence Giant & Supergiant
More informationZeeman Effect Physics 481
Zeeman Effect Introduction You are familiar with Atomic Spectra, especially the H- atom energy spectrum. Atoms emit or absorb energies in packets, or quanta which are photons. The orbital motion of electrons
More informationLab #10 Atomic Radius Rubric o Missing 1 out of 4 o Missing 2 out of 4 o Missing 3 out of 4
Name: Date: Chemistry ~ Ms. Hart Class: Anions or Cations 4.7 Relationships Among Elements Lab #10 Background Information The periodic table is a wonderful source of information about all of the elements
More informationMeasuring the Stars. The measurement of distances The family of distance-measurement techniques used by astronomers to chart the universe is called
Measuring the Stars How to measure: Distance Stellar motion Luminosity Temperature Size Evolutionary stage (H-R diagram) Cosmic distances Mass The measurement of distances The family of distance-measurement
More information18-Dec-12 PHYS Simple Pendulum. To investigate the fundamental physical properties of a simple pendulum.
Objective Simple Pendulum To investigate the fundamental physical properties of a simple pendulum. Equipment Needed Simple Pendulum Apparatus with Meter Scale and Protractor Bobs 4 (Aluminum, Brass, Lead,
More informationOPEN CLUSTER PRELAB The first place to look for answers is in the lab script!
NAME: 1. Define using complete sentences: Globular Cluster: OPEN CLUSTER PRELAB The first place to look for answers is in the lab script! Open Cluster: Main Sequence: Turnoff point: Answer the following
More informationHubble's Law and the Age of the Universe
Hubble's Law and the Age of the Universe Procedure: Name: 1. Login into the network using your user ID and your password. 2. Double click on the Astronomy shortcuts folder on the desktop. 3. Double click
More informationThe Distance Modulus. Absolute Magnitude. Chapter 9. Family of the Stars
Foundations of Astronomy 13e Seeds Phys1403 Introductory Astronomy Instructor: Dr. Goderya Chapter 9 Family of the Stars Cengage Learning 016 Topics for Today s Class 1. Recap: Intrinsic Brightness a)
More informationHow Do I Create a Hubble Diagram to show the expanding universe?
How Do I Create a Hubble Diagram to show the expanding universe? An extremely important topic in astronomy is the expansion of the universe. Although the expanding universe is nearly always discussed in
More informationElectric Fields and Equipotentials
OBJECTIVE Electric Fields and Equipotentials To study and describe the two-dimensional electric field. To map the location of the equipotential surfaces around charged electrodes. To study the relationship
More informationGravity: How fast do objects fall? Teacher Advanced Version (Grade Level: 8 12)
Gravity: How fast do objects fall? Teacher Advanced Version (Grade Level: 8 12) *** Experiment with Audacity and Excel to be sure you know how to do what s needed for the lab*** Kinematics is the study
More informationAstroBITS: Open Cluster Project
AstroBITS: Open Cluster Project I. Introduction The observational data that astronomers have gathered over many years indicate that all stars form in clusters. In a cloud of hydrogen gas, laced with helium
More informationGalaxy Metallicity: What Oxygen Tells Us About The Lifecycles of Galaxies Designed by Prof Jess Werk, modified by Marie Wingyee Lau
Introduction Galaxy Metallicity: What Oxygen Tells Us About The Lifecycles of Galaxies Designed by Prof Jess Werk, modified by Marie Wingyee Lau Before stars and galaxies came into existence, the very
More informationError Analysis, Statistics and Graphing Workshop
Error Analysis, Statistics and Graphing Workshop Percent error: The error of a measurement is defined as the difference between the experimental and the true value. This is often expressed as percent (%)
More information