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Parallax
Parallax

... distance directly. Instead, astronomers must be very clever and measure the distance indirectly. One of the ways they do this is by the method of Parallax. ...
ART. VULCAN/05
ART. VULCAN/05

... and magnetic resonance of past events. ...
Astronomy Quiz 12 “Stars
Astronomy Quiz 12 “Stars

... D. relative _____2. 80% of all stars in the galaxy are __ while only 1 in 10,000 is a __. A. white dwarfs / red giant C. red giants / blue dwarfs B. yellow dwarfs / red supergiant D. red dwarfs / blue supergiant _____3. The actual 3D motion of stars relative to each other in a rotating and swirling ...
Quiz  # 5 – 11/15/2011
Quiz # 5 – 11/15/2011

... 3. To calculate a star radius you must know its A. chemical composition and temperature. B. color and chemical compositions. C. surface gravity and temperature. D. temperature and luminosity. E. chemical composition and luminosity. 4. If the size of an object doubles, but its temperature stays the s ...
DTU9ePPTChap13 - Faculty Lounge : Astronomy
DTU9ePPTChap13 - Faculty Lounge : Astronomy

... from one of the first pulsars to be discovered, PSR 0329 + 54. Note that some of the pulses are weak and others are strong. Nevertheless, the spacing between pulses is so regular (0.714 s) that it is more precise than most clocks on Earth. ...
The Scale of the Cosmos
The Scale of the Cosmos

... at every full moon. • The Moon's orbit is tipped about 5 degrees to the ...
Stars…Giants, Supergiants, Dwarfs….
Stars…Giants, Supergiants, Dwarfs….

... neighbors” and have identity crises. The atomic energy levels, instead of being crisp and unique, get “fuzzed out”. “Fuzzed out” is technical terminology for a change in the energy which depends on how close the neighbors are, how many of them there are, what direction they are,…… ...
Exercise 5
Exercise 5

... Of interest to us are the apparently light vertical “lines” that appear at irregular intervals throughout each spectrum. These spectra are actually negatives — that is, most of the spectrum should be light-colored, and the lines should appear ...
Chapter 4 Study Guide
Chapter 4 Study Guide

... Chapter 4: Making Sense of the Universe Scott Hildreth – Chabot College ...
Document
Document

... When astronomers look through their telescopes, they see billions of stars. What can they learn fromThe goal of this problem set is for you to understand that astronomers classify stars on the basis of two different criteria: (1) the intensity of one of the H absorption lines (called H), and (2) on ...
Spectrum Analysis Activity File
Spectrum Analysis Activity File

... Our modern understanding of light began when Newton passed a beam of white light through a prism and found that the light was broken up into the colors of the rainbow. This rainbow of colors ranges from violet at 400nm to red at 700nm and is called the visible spectrum. Scientists designed and const ...
Measuring the distance to Galaxies
Measuring the distance to Galaxies

key - Scioly.org
key - Scioly.org

... a) 321.5 seconds (5.4 minutes); It is the shortest orbital period of any binary system discovered. b) Xray c) The observation of such systems pushes to the limit of current technology because they are so dim that only the largest telescopes can sense them. d) Approximately one ton (~.5 solar masses ...
script (powerpoint)
script (powerpoint)

... The 2009-2010 orbital motions of the four planets are shown in the larger plot. A square symbol denotes the first 2009 epoch. The upper-right small panel shows a zoomed version of e's astrometry including the expected motion (curved line) if it is an unrelated background object. Planet e is confirm ...
supplemental educational materials PDF
supplemental educational materials PDF

... a “guest observer” at the MicroObservatory Web site and request that a telescope snap a picture of the star-forming region. Then you can view the image on the Web site. To become a guest observer, go to: http://mo-www.harvard.edu/MicroObservatory/ ...
Announcements
Announcements

... Clicker question l  A planet is discovered in another solar system which has the same diameter for its orbit around its star as the Earth does around the Sun. Their star, however, has a mass of four times that of our Sun. How long does it take this new planet to travel around its star? ...
Stellar and Atomic Spectra
Stellar and Atomic Spectra

Chapter 10: The Stars
Chapter 10: The Stars

More on Cluster HR diagrams - University of Texas Astronomy
More on Cluster HR diagrams - University of Texas Astronomy

... This reaction requires T~100 million degrees K, which the core has attained by its contraction and heating. But for low mass stars (less than about 2 Mo), when the He gets hot enough to ignite, the core is so dense that the gas is degenerate. (This is an important concept, and will recur when we des ...
Homework # 1
Homework # 1

... to questions do not need to be written in complete sentences and you should show your work where ever it is appropriate. Partial credit may be given for showing your work even if your result is incorrect. You will also be graded on the use of significant figures, proper units of measure and proper s ...
Observations of the Sky
Observations of the Sky

... Did you know?  Polaris is really *3* stars;  Brightest is yellow “giant” ~ 5 x more massive than our Sun  Pulsates & changes in brightness (“Cepheid”)  Distance 300-433 ly away! ...
The Characteristics of Stars
The Characteristics of Stars

... problem, astronomers have developed an absolute magnitude scale. The absolute magnitude of a celestial object equals the apparent magnitude the object would have if it were 33 ly from the observer. If the Sun were 33 ly from Earth, it would have an apparent magnitude of 4.8. Therefore, the Sun’s abs ...
Star Finder
Star Finder

... ECLIPTIC CIRCLE: This is the daily path of the sun (due to the earth going around the sun) through the constellations known as the band of animals or Zodiac. The Planets and our Moon are also are found in the constellations along this path. The ECLIPTIC is indicated by a dashed circle on the dial. F ...
UNIT 2 - Orange Public Schools
UNIT 2 - Orange Public Schools

July - Rose City Astronomers
July - Rose City Astronomers

... This is a pretty simple process requiring only the filling out of a registration form (no fees involved) and then waiting a few days for your observer initials to be emailed to you: Therefore, for the most part, the Astrophysicist's are pretty much dependent upon world wide amateur contributors to r ...
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Timeline of astronomy

Timeline of astronomy around 2300 BC.
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