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Chapter 1 Seeing the Light: The Art and Science of Astronomy
Chapter 1 Seeing the Light: The Art and Science of Astronomy

22 pm - Starmap
22 pm - Starmap

... Many deep sky objects like galaxies and clusters will be within reach. Jupiter satellites and Saturn’s rings will also be visible. A spectacular experience for beginners in astronomy... Avoid the nights when the Moon is too bright as its light would make the observation of faint objects ...
Luminosity
Luminosity

The Milky Way - University of North Texas
The Milky Way - University of North Texas

... recent maximum can be used to predict the time of a future maximum. Suppose that you calculate the time of future maximum brightness and then make measurements to observe this maximum. After the correction for Earth's orbital position has been made, you find that the maximum occurred a few minutes l ...
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AJAstroProject

key for the HR Diagram Lab Handout
key for the HR Diagram Lab Handout

Planetary Nebulae – White dwarfs
Planetary Nebulae – White dwarfs

Deaths of Stars - Chabot College
Deaths of Stars - Chabot College

Picture: Alnitak is the left-hand star in Orion`s Belt. Image: NASA
Picture: Alnitak is the left-hand star in Orion`s Belt. Image: NASA

Building the Hertzsprung
Building the Hertzsprung

lecture19 - Stony Brook University
lecture19 - Stony Brook University

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... in whole or in sections must include the referral attribution link http://www.ck12.org/saythanks (placed in a visible location) in addition to the following terms. Except as otherwise noted, all CK-12 Content (including CK-12 Curriculum Material) is made available to Users in accordance with the Cre ...
Stars, Galaxies, and the Universe Section 1
Stars, Galaxies, and the Universe Section 1

Part 1: If a 10000 K blackbody has a wavelength of peak emission at
Part 1: If a 10000 K blackbody has a wavelength of peak emission at

... Use the blackbody simulator to get a better feel for this inverse relation and review the material in Module 1 Lecture F. Also, as I said in class, if this inverse relation did not hold then cooler objects would be emitting short wavelength high energy photons which doesn’t make any physical sense b ...
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Finish up Sun and begin Stars of the Sun Test 1 Study

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Lecture 11

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The Sun and other Stars

... If two stars are the same temperature but differ in luminosity, then they must be different in size. Bright cool stars are called ___________________. Red giants are large stars. They are very bright because they are very big, but are also relatively cool. They appear red because of their low temper ...
Physics: Principle and Applications, 7e (Giancoli) Chapter 33
Physics: Principle and Applications, 7e (Giancoli) Chapter 33

... 8) Pulsars are rapidly spinning A) regular stars like our sun. B) red giant stars. C) neutron stars. D) white dwarfs. Answer: C Var: 1 9) Stars A and B are both black holes but have different masses. If the mass of star A is twice as much as the mass of star B, the average density of star A, compare ...
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Sun and Other Stars Notes

Sky Diary - Society for Popular Astronomy
Sky Diary - Society for Popular Astronomy

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lecture

Teaching astrophysics in VCE Physics
Teaching astrophysics in VCE Physics

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... - Estimated 1M years old - Most stars clouded from view by dust - Only 4-5 stars visible with small scope ...
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S T A R S

Visual Photometry - El Camino College
Visual Photometry - El Camino College

... human eye can detect stars brighter than about 6th magnitude when in a very dark site (far from city lights). Unfortunately, around El Camino, the eye can barely see 4th magnitude stars due to all of the light pollution from the surrounding LA city lights. However, with the additional light collecti ...
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Cassiopeia (constellation)



Cassiopeia is a constellation in the northern sky, named after the vain queen Cassiopeia in Greek mythology, who boasted about her unrivalled beauty. Cassiopeia was one of the 48 constellations listed by the 2nd-century Greek astronomer Ptolemy, and it remains one of the 88 modern constellations today. It is easily recognizable due to its distinctive 'M' shape when in upper culmination but in higher northern locations when near lower culminations in spring and summer it has a 'W' shape, formed by five bright stars. It is bordered by Andromeda to the south, Perseus to the southeast, and Cepheus to the north. It is opposite the Big Dipper.In northern locations above 34ºN latitude it is visible year-round and in the (sub)tropics it can be seen at its clearest from September to early November in its characteristic 'M' shape. Even in low southern latitudes below 25ºS is can be seen low in the North.
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