Physics Lab #4: Citizen Science - The Milky Way Project
|
|
- Sara Preston
- 6 years ago
- Views:
Transcription
1 Physics Lab #4: Citizen Science - The Milky Way Project Introduction This lab is the first of several Citizen Science labs we will do together this semester as part of the zooniverse.org project family. The concept of Citizen Science is that some Astronomical databases are so large and the data so complex that computer algorithms cannot accurately or reliably sort through all of the data to find the kinds of interesting things that astronomers are looking for. In this lab, we will be exploring the structure and interesting features within our Milky Way galaxy. Part 1 Using a web browser, navigate to and from there, select About and read through the short introduction, answering the associated questions on your worksheet. Part 2 For helpful background information about what astronomers are hoping to learn by studying bubbles, star forming regions, clusters and other structures in the Milky Way, please read through the February 2010 Scientific American article, Cloudy with a Chance of Stars. In order to access this article 1) You will need to go to the TCU library s website at 2) Once there, click on the Library Catalog button directly beneath the tculibrary logo. 3) Next, type Scientific American into the search box, and also change the drop-down menu from Words Anywhere to Journal name begins with 4) Click on the Search button. 5) On the Search results page, click on the first linked entry that simply says Scientific American. 6) On the next results page, in the first record, click on the 2nd or 3rd entry in the list that reads Full text available to the TCU community from Nature Journals Online: 1993 to present.!27
2 7) This will open a new window that gives you access to the complete archive of Scientific American. In the search box there, type in the name of the article we are looking for: Cloudy with a Chance of Stars. 8) On the search results page, the first entry should be the article we are looking for. Click on the PDF link to open up a PDF copy of the article. Ask your TA if you need help with any of the steps in this process. Once you have the article loaded, read through it and answer the questions on your worksheet, which are arranged in the same order that they are covered within the article. Part 3 Next, sign in to the Zooniverse website if you haven t already. You may need to create an account. Be sure to use a username/password that you can remember since we will do more Citizen Science projects later. This will enable the site to keep a record of your work so that we know how many data sets you have completed. Now click on the Classify button to start the tutorial on how to classify objects. Read through the tutorial. Now proceed to classify 90 images. If you have some uncertainty after looking at a few images, go through the tutorial carefully again. Also, click the Need some help with this task? button for some examples of things commonly marked. Many frames (maybe half) have nothing obvious to mark, and that s fine. Just inspect the image for a few seconds to be sure, then move on to the next. Once you have completed your contribution to the project, show your TA your profile page (click your username on the top right, then select Home ). The little ring around the circular icon can be hovered over to indicate how many data sets you have completed for any given project.!28
3 Lab #4 Worksheet Name: Home TA: Part 1 From the About section under the first tab ( Research ), explain what Astronomers hope to learn by studying the dust located on the outer edges of interstellar bubbles. From the About section under the fourth tab ( FAQ ), explain why the project needs many people to classify the same image.!29
4 Part 2 From the article, Cloudy with a Chance of Stars, what four questions about star formation does the author seek to answer with his research? When collapsing interstellar clouds reach a density of about 1000 atoms per cubic centimeter, we call them molecular clouds. Why can molecules survive in these clouds and not in other parts of interstellar space?!30
5 Describe two leading ideas that may explain what upsets the balance of pressure and gravity in order to initiate the formation of a star from an interstellar cloud Explain the evidence from the W5 region (described in the photograph on page 39) that radiation pressure from massive stars has triggered the collapse of surrounding dust clouds and subsequent star formation at the rim of the bubble. Describe the competitive accretion model for the formation of star clusters.!31
6 Describe the evidence in the Christmas Tree cluster that seems to support competitive accretion as a major influence, at least for some stars. Explain how recent theoretical simulations solve the problem of super-massive star formation, allowing stars to form with masses larger than 20 solar masses despite the enormous radiation they emit (which should disperse surrounding gas and dust, limiting further growth). Part 3 Once you have classified 90 images, show your TA your profile for verification. Don t forget to explore what others have also done with the same images using the advice I ve given you in the lab instructions for this part. TA Initials:!32
Physics Lab #6: Citizen Science - Variable Star Zoo
Physics 10263 Lab #6: Citizen Science - Variable Star Zoo Introduction This lab is the another Citizen Science lab we will do together this semester as part of the zooniverse.org project family. This time,
More informationPhysics Lab #1: Scale Models
Physics 10263 Lab #1: Scale Models Introduction The Universe is a big place. But what does that statement really tell you? One of the goals of this course is to have each of you develop some sense for
More informationPhysics Lab #10: Citizen Science - The Galaxy Zoo
Physics 10263 Lab #10: Citizen Science - The Galaxy Zoo Introduction Astronomy over the last two decades has been dominated by large sky survey projects. The Sloan Digital Sky Survey was one of the first
More information4 HOW DID THE EARTH FORM?
4 HOW DID THE EARTH FORM? New stars and space debris spinning like pizza dough are a couple of the things that explain the formation of solar systems like ours. In this three-part lecture, David Christian
More informationThe Secrets of Galaxies. Student s Guide Advanced Level CESAR s Science Case
The Secrets of Galaxies Student s Guide Advanced Level Introduction Galaxies are fundamental building blocks of the Universe. Some are simple, while others are very complex in structure; some have enormous
More informationGalaxy Zoo. Materials Computer Internet connection
Name: Date: Galaxy Zoo Objectives: Distinguish between different types of galaxies Identify the various features of each subclass Contribute data that will be used by astronomers in their work Learn to
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 informationGalaxies and The Milky Way
Galaxies and The Milky Way Attendance Quiz Are you here today? Here! (a) yes (b) no (c) To infinity and beyond! Next Tuesday, 5/30, I will be away at a meeting. There will be a guest lecture by Dr. Jorge
More informationReview: HR Diagram. Label A, B, C respectively
Stellar Evolution Review: HR Diagram Label A, B, C respectively A C B a) A: White dwarfs, B: Giants, C: Main sequence b) A: Main sequence, B: Giants, C: White dwarfs c) A: Main sequence, B: White Dwarfs,
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 informationD.T.M: TRANSFER TEXTBOOKS FROM ONE SCHOOL TO ANOTHER
Destiny Textbook Manager allows users with full access to transfer Textbooks from one school site to another and receive transfers from the warehouse In this tutorial you will learn how to: Requirements:
More informationMATH 137 : Calculus 1 for Honours Mathematics. Online Assignment #2. Introduction to Sequences
1 MATH 137 : Calculus 1 for Honours Mathematics Online Assignment #2 Introduction to Sequences Due by 9:00 pm on WEDNESDAY, September 19, 2018 Instructions: Weight: 2% This assignment covers the topics
More informationPROJECT GLOBULAR CLUSTERS
PROJECT 5 GLOBULAR CLUSTERS Objective: The objective of this exercise is the calculation of the core and tidal radius of a globular cluster in the Milky Way. Measure the tidal radius of a globular cluster
More informationMeasurement: Length, Area and Volume Part I
IDS 101 Name Measurement: Length, Area and Volume Part I If we ask someone the size of a common object, such as a dime or penny, most people come pretty close to the actual size. However, objects that
More informationREPLACE DAMAGED OR MISSING TEXTBOOK BARCODE LABEL
Destiny Textbook Manager allows users to create and print replacement barcode labels for textbooks. In this tutorial you will learn how to: Replace damaged textbook barcode label(s) Replace missing textbook
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 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 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 informationHomework on Properties of Galaxies in the Hubble Deep Field Name: Due: Friday, April 8 30 points Prof. Rieke & TA Melissa Halford
Homework on Properties of Galaxies in the Hubble Deep Field Name: Due: Friday, April 8 30 points Prof. Rieke & TA Melissa Halford You are going to work with some famous astronomical data in this homework.
More informationNotifications and Accretions: Facility Role
Notifications and Accretions: Facility Role Goal: Learn to view and resolve notification and accretion discrepancies in CROWNWeb. Estimated Time: 25 to 30 minutes PDF: Download a screen reader compatible
More informationThe Interstellar Medium (ch. 18)
The Interstellar Medium (ch. 18) The interstellar medium (ISM) is all the gas (and about 1% dust) that fills our Galaxy and others. It is the raw material from which stars form, and into which stars eject
More informationSpeeds of a Chemical Reaction
Speeds of a Chemical Reaction Name Lab Section Log on to the Internet. Type the following address into the location-input line of your browser: http://cheminfo.chem.ou.edu/~mra/ccli2004/k2rm.htm This will
More informationCHEMICAL INVENTORY ENTRY GUIDE
CHEMICAL INVENTORY ENTRY GUIDE Version Date Comments 1 October 2013 Initial A. SUMMARY All chemicals located in research and instructional laboratories at George Mason University are required to be input
More informationACTIVITIES for Grades 9-12
ACTIVITIES for Grades 9-12 BEFORE YOUR VISIT Online Video: Journey to the Stars Trailer and Prelude To prepare for your Museum visit, watch the trailer and the prelude with your students. Class Discussion:
More informationDear Teacher, Overview Page 1
Dear Teacher, You are about to involve your students in one of the most exciting frontiers of science the search for other worlds and life in solar systems beyond our own! Using the MicroObservatory telescopes,
More informationThe Galaxy Zoo Project
Astronomy 201: Cosmology Fall 2009 Prof. Bechtold NAME: The Galaxy Zoo Project 200 points Due: Nov. 23, 2010, in class Professional astronomers often have to search through enormous quantities of data
More informationPhysics Lab #3:! Starry Night! Observations of the Sun and Moon!
Physics 10293 Lab #3: 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 informationPOC via CHEMnetBASE for Identifying Unknowns
Table of Contents A red arrow is used to identify where buttons and functions are located in CHEMnetBASE. Figure Description Page Entering the Properties of Organic Compounds (POC) Database 1 CHEMnetBASE
More informationUNST 232 Mentor Section Assignment 5 Historical Climate Data
UNST 232 Mentor Section Assignment 5 Historical Climate Data 1 introduction Informally, we can define climate as the typical weather experienced in a particular region. More rigorously, it is the statistical
More informationDISCRETE RANDOM VARIABLES EXCEL LAB #3
DISCRETE RANDOM VARIABLES EXCEL LAB #3 ECON/BUSN 180: Quantitative Methods for Economics and Business Department of Economics and Business Lake Forest College Lake Forest, IL 60045 Copyright, 2011 Overview
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 informationa computer running the CLEA activity The Large Scale Structure of the Universe. a computer running a spreadsheet program
TAP 704-5: Red shift The CLEA software enables you to simulate controlling a telescope so that it points at a selected galaxy, and then using a spectrometer to record the light received over a range of
More informationPhysics Lab #2: Spectroscopy
Physics 10263 Lab #2: Spectroscopy Introduction This lab is meant to serve as an introduction to the science of spectroscopy. In this lab, we ll learn about how emission and absorption works, and we ll
More informationLab 2 Astronomical Coordinates, Time, Focal Length, Messier List and Open Clusters
Lab 2 Astronomical Coordinates, Time, Focal Length, Messier List and Open Clusters Name: Partner(s): Boxes contain questions that you are expected to answer (in the box). You will also be asked to put
More informationQuality Measures (QM) Report. Self Guided Tutorial
Quality Measures (QM) Report Self Guided Tutorial 1 Tutorial Contents Overview of the QM Online Report Facility Summary Report Resident Drill down Monthly Trend Report Resident Roster Report Printing Reports/Export
More informationInteracting Galaxies
Interacting Galaxies Contents Introduction... 1 Downloads... 1 Selecting Interacting Galaxies to Observe... 2 Measuring the sizes of the Galaxies... 5 Making a Colour Image in IRIS... 8 External Resources...
More informationLab #8. The Moons of the Outer Planets
Lab #8 The Moons of the Outer Planets Introduction In this lab, we will explore the outer planets and their fascinating moons using the latest information on the Web. There are several processes at work
More informationPhysics E-1ax, Fall 2014 Experiment 3. Experiment 3: Force. 2. Find your center of mass by balancing yourself on two force plates.
Learning Goals Experiment 3: Force After you finish this lab, you will be able to: 1. Use Logger Pro to analyze video and calculate position, velocity, and acceleration. 2. Find your center of mass by
More informationEOS 102: Dynamic Oceans Exercise 1: Navigating Planet Earth
EOS 102: Dynamic Oceans Exercise 1: Navigating Planet Earth YOU MUST READ THROUGH THIS CAREFULLY! This exercise is designed to familiarize yourself with Google Earth and some of its basic functions while
More informationBig Bang, Black Holes, No Math
ASTR/PHYS 109 Dr. David Toback Lectures 2 & 3 1 Prep For Today (is now due) L3 Reading (If you haven t already): Required: BBBHNM: Chapter 1-4 Recommended: (BHOT: Chap. 1-3, SHU: Chap. 1-2, TOE: Chap.
More information( ) = 5log pc NAME: OPEN CLUSTER PRELAB
NAME: OPEN CLUSTER PRELAB 1. Read over the material in the lab script that discusses the background of colormagnitude (CM) diagrams (these can also be called H-R diagrams). Explain the CM diagram: What
More informationDesigning a Quilt with GIMP 2011
Planning your quilt and want to see what it will look like in the fabric you just got from your LQS? You don t need to purchase a super expensive program. Try this and the best part it s FREE!!! *** Please
More informationMeasurements of a Table
Measurements of a Table OBJECTIVES to practice the concepts of significant figures, the mean value, the standard deviation of the mean and the normal distribution by making multiple measurements of length
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 informationAstronomy 9 Concepts of the Cosmos
Astronomy 9 Concepts of the Cosmos Monday/Wednesday, 1:30-2:45 pm, Cabot Auditorium LECTURE 2: I.Our Place in the Universe Lecture on Mon., Feb. 1 st Pre-course Test - REQUIRED! (if you want the attendance
More informationDefense Acquisition University
STEP 1 STEP 2 STEP 3 STEP 4 STEP 5 STEP 6 Search For Training Take DAU Orientation Take Online Training Take Instructor-Led Training Edit Your User Record View Your Course Completions Defense Acquisition
More informationLab 1: Measurement Errors Adapted from Holtzman's Intro Lab for Astr110
Lab 1: Measurement Errors Adapted from Holtzman's Intro Lab for Astr110 Purpose: to give students practice making measurements and estimating error, as an introduction to understanding measurements in
More information1m 100cm=1m =1 100cm 1m 89cm = 0.89m 100cm
Units and Measurement Physics 40 Lab 1: Introduction to Measurement One of the most important steps in applying the scientific method is experiment: testing the prediction of a hypothesis. Typically we
More informationEOSC 110 Reading Week Activity, February Visible Geology: Building structural geology skills by exploring 3D models online
EOSC 110 Reading Week Activity, February 2015. Visible Geology: Building structural geology skills by exploring 3D models online Geological maps show where rocks of different ages occur on the Earth s
More informationLearning ArcGIS: Introduction to ArcCatalog 10.1
Learning ArcGIS: Introduction to ArcCatalog 10.1 Estimated Time: 1 Hour Information systems help us to manage what we know by making it easier to organize, access, manipulate, and apply knowledge to the
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 informationWHAT DOES A GAME HAVE TO DO WITH ASTRONOMY? AST MESA COMMUNITY COLLEGE
NAME: DATE: INTRODUCTION This lab exercise introduces the concepts of scientific inquiry. LEARNING GOALS Identify patterns in data. Propose scientific hypotheses. Test predictions using observations. EQUIPMENT
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 informationPHYS1021 Stars and Galaxies Summer 2015
Professor: Dr. Mark W. Plano Clark Office: Geo/Phys 435 Telephone: (513) 556-0546 Email: Office Hours: Text: Course Description mark.planoclark@uc.edu PHYS1021 Stars and Galaxies Summer 2015 MTWR: 10:00-11:00
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 informationLife of a Star. Lesson development
Lesson development InstructIonal objectives Students will compare various life cycles; interpret charts and diagrams depicting the life cycle of stars; use a variety of Internet sources to research stages
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 information[FILE] MILKY WAY AT HOME EBOOK
29 May, 2018 [FILE] MILKY WAY AT HOME EBOOK Document Filetype: PDF 244.76 KB 0 [FILE] MILKY WAY AT HOME EBOOK The galaxy contains about 400 billion stars, with a 4-billion-solar-mass black hole at its
More informationIntroduction to the College of DuPage NEXLAB Website
Introduction to the College of DuPage NEXLAB Website The purpose of this lab is to familiarize yourself with our website so that you will have an easier time following along in class and will be able to
More informationChapter 19 Reading Quiz Clickers. The Cosmic Perspective Seventh Edition. Our Galaxy Pearson Education, Inc.
Reading Quiz Clickers The Cosmic Perspective Seventh Edition Our Galaxy 19.1 The Milky Way Revealed What does our galaxy look like? How do stars orbit in our galaxy? Where are globular clusters located
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 informationFireFamilyPlus Version 5.0
FireFamilyPlus Version 5.0 Working with the new 2016 NFDRS model Objectives During this presentation, we will discuss Changes to FireFamilyPlus Data requirements for NFDRS2016 Quality control for data
More informationLogistics. Test 3 will be 4/24 MRS 2 due Thursday 4/17
Stellar Evolution Logistics Test 3 will be 4/24 MRS 2 due Thursday 4/17 GTA Award The Graduate Teaching Assistant Excellence Award is an internal initiative which is intended to promote, recognize, and
More informationAstronomy 102: Stars and Galaxies Examination 3 Review Problems
Astronomy 102: Stars and Galaxies Examination 3 Review Problems Multiple Choice Questions: The first eight questions are multiple choice. Except where explicitly noted, only one answer is correct for each
More informationThe data for this lab comes from McDonald Forest. We will be working with spatial data representing the forest boundary, streams, roads, and stands.
GIS LAB 6 Using the Projection Utility. Converting Data to Oregon s Approved Lambert Projection. Determining Stand Size, Stand Types, Road Length, and Stream Length. This lab will ask you to work with
More informationHubble Deep Field Activity
National Aeronautics and Space Administration Hubble Deep Field Activity This booklet contains activities that appear on the back of the HDF poster. The Amazing Space Web site contains an online version
More informationJr. Meteorologist Club
Vintage Math, Science and Technology Magnet School Jr. Meteorologist Club Hey, you 5 th Grade WeatherBugs Complete the four required activities plus two activities of your choice in this Jr. Meteorologist
More informationPART 3 Galaxies. Gas, Stars and stellar motion in the Milky Way
PART 3 Galaxies Gas, Stars and stellar motion in the Milky Way The Interstellar Medium The Sombrero Galaxy Space is far from empty! Clouds of cold gas Clouds of dust In a galaxy, gravity pulls the dust
More informationWikipedia - Stellar classification:
Stars and Hertzprung-Russell Diagram Introductory Astronomy laboratory exercise with Stellarium Mike Chu Name Stellarium is an open source and cross-platform application from www.stellarium.org. A star
More informationPS 101: Introductory Astronomy Fall 2014
PS 101: Introductory Astronomy Fall 2014 Lecture: Lab: Tues./Thurs. 12:00 pm - 1:15 pm, S166 Tues. 4:00 pm - 5:50 pm, S166 Instructor: Dr. Jon M. Saken Office: S178 (Science Bldg.) Phone: 696-2753 E-mail:
More informationAS102 -The Astronomical Universe. The boring details. AS102 - Major Topics. Day Labs - Rooms B4 & 606. Where are we (earth, sun) in the universe?
AS102 - Major Topics Where are we (earth, sun) in the universe? What are stars? AS102 -The Astronomical Universe Instructor: Professor Tereasa Brainerd TAs: Ren Cashman & Katie Garcia How are stars born,
More informationConformational Analysis of n-butane
Conformational Analysis of n-butane In this exercise you will calculate the Molecular Mechanics (MM) single point energy of butane in various conformations with respect to internal rotation around the
More informationLab Exploration #4: Solar Radiation & Temperature Part II: A More Complex Computer Model
METR 104: Our Dynamic Weather (w/lab) Lab Exploration #4: Solar Radiation & Temperature Part II: A More Complex Computer Model Dr. Dave Dempsey, Department of Earth & Climate Sciences, SFSU, Spring 2014
More informationAstronomy 142 Recitation #7
Astronomy 14 Recitation #7 1 March 01 Formulas to remember Reddening and extinction Magnitude reminder: U = mu, B= mb, = m (apparent magnitudes); B = mb m (color index). isual extinction toward a star:
More informationAstron 104 Laboratory #5 The Size of the Solar System
Name: Date: Section: Astron 104 Laboratory #5 The Size of the Solar System Section 1.3 In this exercise, we will use actual images of the planet Venus passing in front of the Sun (known as a transit of
More informationRelative Photometry with data from the Peter van de Kamp Observatory D. Cohen and E. Jensen (v.1.0 October 19, 2014)
Relative Photometry with data from the Peter van de Kamp Observatory D. Cohen and E. Jensen (v.1.0 October 19, 2014) Context This document assumes familiarity with Image reduction and analysis at the Peter
More informationclass 21 Astro 16: Astrophysics: Stars, ISM, Galaxies November 20, 2018
Topics: Post-main-sequence stellar evolution, degeneracy pressure, and white dwarfs Summary of reading: Review section 2 of Ch. 17. Read the beginning and first section of Ch. 18 (up through the middle
More informationPython Tutorial on Reading in & Manipulating Fits Images and Creating Image Masks (with brief introduction on DS9)
1 Tyler James Metivier Professor Whitaker Undergrad. Research February 26, 2017 Python Tutorial on Reading in & Manipulating Fits Images and Creating Image Masks (with brief introduction on DS9) Abstract:
More informationLecture Outlines. Chapter 23. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.
Lecture Outlines Chapter 23 Astronomy Today 8th Edition Chaisson/McMillan Chapter 23 The Milky Way Galaxy Units of Chapter 23 23.1 Our Parent Galaxy 23.2 Measuring the Milky Way Discovery 23-1 Early Computers
More informationDark Energy and Dark Matter
Dark Energy and Dark Matter Attendance Quiz Are you here today? (a) yes (b) no Here! (c) The Dark Lord wants his ring back! Final Exam The final exam is Thursday, 6/8, from 11:30am to 1:30pm (2 hours),
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 informationIntroduction to Simple Harmonic Motion
Introduction to Prelab Prelab 1: Write the objective of your experiment. Prelab 2: Write the relevant theory of this experiment. Prelab 3: List your apparatus and sketch your setup.! Have these ready to
More informationPDF-2 Tools and Searches
PDF-2 Tools and Searches PDF-2 2019 The PDF-2 2019 database is powered by our integrated search display software. PDF-2 2019 boasts 69 search selections coupled with 53 display fields resulting in a nearly
More informationData Mining with the PDF-4 Databases. FeO Non-stoichiometric Oxides
Data Mining with the PDF-4 Databases FeO Non-stoichiometric Oxides This is one of three example-based tutorials for using the data mining capabilities of the PDF-4+ database and it covers the following
More informationStructures in the Magnetosphere 2. Hover the curser over a point on the image. The coordinates and value at that point should appear.
Investigating the Magnetosphere Introduction In this investigation, you will explore the properties of the regions of the magnetosphere using simulation results from the BATS-R-US model from the magnetosphere
More informationGalactic Rotation Activity*
Galactic Rotation Activity* Neutral hydrogen atoms (H I) consist of a single proton and a single electron. The electron and proton can spin in the same direction (parallel) or in the opposite direction
More informationPDF-4+ Tools and Searches
PDF-4+ Tools and Searches PDF-4+ 2019 The PDF-4+ 2019 database is powered by our integrated search display software. PDF-4+ 2019 boasts 74 search selections coupled with 126 display fields resulting in
More informationThe Hubble Law & The Structure of the Universe
Name: Lab Meeting Date/Time: The Hubble Law & The Structure of the Universe The Hubble Law is a relationship between two quantities the speed of and distance to a galaxy. In order to determine the Hubble
More informationHomework #7: Properties of Galaxies in the Hubble Deep Field Name: Due: Friday, October points Profs. Rieke
Homework #7: Properties of Galaxies in the Hubble Deep Field Name: Due: Friday, October 31 30 points Profs. Rieke You are going to work with some famous astronomical data in this homework. The image data
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 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 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 informationHow big is the Milky Way? Introduction. by Toby O'Neil. How big is the Milky Way? about Plus support Plus subscribe to Plus terms of use
about Plus support Plus subscribe to Plus terms of use search plus with google home latest issue explore the archive careers library news 1997 2004, Millennium Mathematics Project, University of Cambridge.
More informationMAS156: Mathematics (Electrical and Aerospace)
MAS156: Mathematics (Electrical and Aerospace) Dr Sam Marsh mas-engineering@sheffield.ac.uk Tuesday 17th October 2017, 1pm Diamond LT4 Course matters Online tests Some people had problems in the early
More informationAstro 32 - Galactic and Extragalactic Astrophysics/Spring 2016
Astro 32 - Galactic and Extragalactic Astrophysics/Spring 2016 The class meets Monday and Wednesday 10:30-11:45am (Block E+) in 574 Boston Ave, room 401 Instructor: Professor Anna Sajina email: Anna.Sajina@tufts.edu
More informationGeneral Chemistry Lab Molecular Modeling
PURPOSE The objectives of this experiment are PROCEDURE General Chemistry Lab Molecular Modeling To learn how to use molecular modeling software, a commonly used tool in chemical research and industry.
More informationA galaxy is a self-gravitating system composed of an interstellar medium, stars, and dark matter.
Chapter 1 Introduction 1.1 What is a Galaxy? It s surprisingly difficult to answer the question what is a galaxy? Many astronomers seem content to say I know one when I see one. But one possible definition
More informationBig Bang, Black Holes, No Math
ASTR/PHYS 109 Dr. David Toback Lectures 10, 11 & 12 1 Prep For Today (is now due) L12 Reading: (BBBHNM Unit 2) Pre-Lecture Reading Questions: If you were misgraded, need help or an extension let me know
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 informationCONFIRMATION OF A SUPERNOVA IN THE GALAXY NGC6946
CONFIRMATION OF A SUPERNOVA IN THE GALAXY NGC6946 G. Iafrate and M. Ramella INAF - Astronomical Observatory of Trieste 1 Introduction Suddenly a star runs out its nuclear fuel. Its life as a normal star
More information