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Integrative Studies 410 Our Place in the Universe
Integrative Studies 410 Our Place in the Universe

... • Named after δ Cephei • Period-Luminosity Relations • Two types of Cepheids: – Type I: higher luminosity, metal-rich, Pop. 1 – Type II: lower lum., metal-poor, Population 2 ...
What constitutes the dark matter?
What constitutes the dark matter?

... formed out of frozen gas balls that are already present. • Dwarf galaxy problem (10.000 stars, much dark matter) solved: Jeans cluster with still many frozen gas balls. ...
Chapter 7 Worksheet November 1
Chapter 7 Worksheet November 1

... C. The amount of energy contained in an electromagnetic wave D. The speed of light 3. (#40 from the text) Place the following types of radiation in order of increasing wavelength and increasing energy per photon: Gamma Rays // Radio Waves // Microwaves // Visible Light ...
Constellation Information
Constellation Information

... The spring constellation most prominent is Leo, the Lion. Leo really does resemble the outline of a lion. His front part is formed by the hook of stars extending north from the bright star Regulus in his forefoot. This hook of stars- usually called the Sickle- represents Leos chest, mane and head. ...
insert - Athens
insert - Athens

... more than a thousand billion billion stars in our universe! However, almost all of them are too far away for you to see with your naked eyes. From our perspective on earth, stars appear as tiny points of light, but of course, they are much, much larger than they seem. A medium-sized star like our su ...
fact packet spring 2014
fact packet spring 2014

ASTR101 Unit 14 Assessment Answer Key 1. It is believed that the
ASTR101 Unit 14 Assessment Answer Key 1. It is believed that the

... factors and multiplying them is the number of communicating civilizations in the galaxy at the present time. 3. The principle argument for the nonexistence of extraterrestrial life is the Fermi paradox. If other technological civilizations exist, they would tend to spread out and colonize the galaxy ...
NOVA COLLEGE-WIDE COURSE CONTENT SUMMARY PHY 150
NOVA COLLEGE-WIDE COURSE CONTENT SUMMARY PHY 150

... The history & development of astronomy and related laws of physics The nature & physics of light. Optics, telescopes and spectroscopy The Earth as a planet and its nearest neighbor, the Moon Atmospheric and geological characteristics of planets, moons and minor bodies of the solar system. The atmosp ...
Celestial Motion - Boris Boguslavsky
Celestial Motion - Boris Boguslavsky

... they leave the body’s atmosphere and escape its gravitational field, they climb out of the well. The deeper the well, the more energy it takes to escape. ...
What Stellar Properties would we like to know and Measure?
What Stellar Properties would we like to know and Measure?

Quick and Easy Activities and Demonstrations for Astronomy
Quick and Easy Activities and Demonstrations for Astronomy

... 1- using a lamp or other light source, have a student sit on a swivel chair a few m in front of the light.(have the room light off) have another student or teacher, walk around student with a ball(the bigger the better) cutting in front of the light. Stop at various points and get the student to des ...
Project 9: Stellar Spectra: Temperature
Project 9: Stellar Spectra: Temperature

... strengths  of  the  absorption  lines  and  therefore  calculate  the chemical composition of the  outer part of a star. Relative absorption line strengths can also be used to find temperatures  and densities.   Absorption lines occur when an electron absorbs energy from the spectrum to move up the  ...
Sample Assessment Items
Sample Assessment Items

... b. Mars is moving much faster than the stars. c. The stars are much farther away than Mars, so they appear not to move. d. Earth and the stars move in one direction, and Mars moves in the other. Answer: The stars in the night sky look as if they are slowly moving because _______________. a. the Eart ...
Testing - Elon University
Testing - Elon University

... What is the galaxy made of? Matter inside stars: ~ 0.6% Matter outside stars: ~ 3.8% ...
Space Science Unit - World of Teaching
Space Science Unit - World of Teaching

Chapter105.ppt
Chapter105.ppt

... • The church hierarchy adopted this view as dogma because it confirmed their own view that the Earth was the most important place in the Universe and human beings the Universe’s most important creatures. (Also, at the time, most people believe the Earth was flat, not spherical, and that if you sail ...
New ultra faint dwarf galaxy candidates discovered with the Dark
New ultra faint dwarf galaxy candidates discovered with the Dark

... KEY UNSOLVED PROBLEM in basic physics today**, Just the sort of problem a fundamental science lab like Fermilab is interested in exploring. The LHC/CMS experiment is looking for it in the form of SUSY particles. DES is looking for how it affects the motions of stars and galaxies, as part of its main ...
The Life Cycle of Stars Webquest
The Life Cycle of Stars Webquest

... Task #4: Types of Stars Continue to read on to the section “Types of Stars” on the same webpage http://www.seasky.org/cosmic/sky7a01.html and answer the following questions: 1. What does the main ...
The Life Cycle of Stars Webquest
The Life Cycle of Stars Webquest

... Task #4: Types of Stars Continue to read on to the section “Types of Stars” on the same webpage http://www.seasky.org/cosmic/sky7a01.html and answer the following questions: 1. What does the main ...
Unit E: SPACE EXPLORATION
Unit E: SPACE EXPLORATION

... the centre with the Earth and planets revolving around it • Proposed by Polish astronomer Nicholas Copernicus in 1530 • Could not accurately predict planetary motion ...
Space Science Unit
Space Science Unit

... slide we will demonstrate the concept of parallax, which is the apparent change of a stars position in the sky. • The stars are not really moving, rather the Earth is and therefore we see ...
Average absolute magnitude
Average absolute magnitude

... Hubble’s law states that v =H0d, where v is the relative recessional speed between galaxies, d is their separation and H0 is the Hubble constant. Recent measurements place the value of H0 in the range 60 to 90 km s–1 Mpc–1. Estimate, in seconds, the maximum known age of the universe. ...
News Analysis - Learning Space
News Analysis - Learning Space

... It simplified large number of physical theories It is not rigid, it is flexible. It can be distorted and warped as large masses move through it. ...
The Milky Way - Houston Community College System
The Milky Way - Houston Community College System

... Temp. ~ 25,000 K Luminosity ~ 0.01 Lsun ...
March 2016 star chart
March 2016 star chart

... Golden Jupiter appears in the east at dusk, the brightest 'star' in the sky. At midnight it is due north. By dawn it is low in the west. Bright stars are overhead and down into the southeast evening sky. Jupiter is the biggest planet by far. Its mass is greater than all the other planets put togethe ...
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Astronomical spectroscopy



Astronomical spectroscopy is the study of astronomy using the techniques of spectroscopy to measure the spectrum of electromagnetic radiation, including visible light, which radiates from stars and other hot celestial objects. Spectroscopy can be used to derive many properties of distant stars and galaxies, such as their chemical composition, temperature, density, mass, distance, luminosity, and relative motion using Doppler shift measurements.
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