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Stars Unit
Stars Unit

Document
Document

Star Maps and Constellations (pdf 3.7 Megs)
Star Maps and Constellations (pdf 3.7 Megs)

... Winter 2006 ...
20 Stars/Distances/Magnitudes
20 Stars/Distances/Magnitudes

"Stars" Power Point notes
"Stars" Power Point notes

Name: ____________ Period: ______ STAR BIOGRAPHY Name of
Name: ____________ Period: ______ STAR BIOGRAPHY Name of

... *May include diagram *Talk about the birth of your star, include its age if known, what life cycle it is in, and predict what will happen in the future with your star. (Include each Life Cycle Stage) ...
U7 Review WS KEY
U7 Review WS KEY

ď - Google Sites
ď - Google Sites

... 2. Stars with surface temperatures up to 3,500 °C are red. Shade a vertical band from 2,000 °C to 3,500 °C a light red. 3. Shade other color bands as follows: Stars up to 5,000 °C are orange-red, up to 6,000 °C yellowwhite, up to 7,500 °C blue-white, and up to 40,000 °C blue. 4. Label the main seque ...
CONSTELLATIONS OF THE SOUTHERN SKY VOLANS
CONSTELLATIONS OF THE SOUTHERN SKY VOLANS

... Created by Bayer in 1603, this constellation used to be called PiscisVolans, the Flying Fish, before it was shortened to Volans. Volans was one of the 12 new constellations introduced at the end of the 16th century by the Dutch navigators Pieter Dirkszoon Keyser and Frederick de Houtman. Volans repr ...
celestial equator
celestial equator

... equator. It is a projection of the Earth's equator out to the celestial sphere. The number of degrees that a celestial object is north or south of the celestial equator is called the declination (DEC) It is the analogue of latitude on the sky. The analogue of longitude is called right ascension (RA) ...
CHAPTER 32 1. What is happening inside a star that isn`t happening
CHAPTER 32 1. What is happening inside a star that isn`t happening

Apparent Magnitude - RanelaghALevelPhysics
Apparent Magnitude - RanelaghALevelPhysics

sun notes
sun notes

The Night Sky
The Night Sky

Lifetimes of stars
Lifetimes of stars

canopus e.g procyon
canopus e.g procyon

Lecture 19 The Milky Way Galaxy
Lecture 19 The Milky Way Galaxy

... of stars: published the ‘Grindstone model’ – the Sun at the center of An irregularly shaped disc of stars ...
Star Classification
Star Classification

... Most stars, including the sun, are "main sequence stars," fueled by nuclear fusion converting hydrogen into helium. For these stars, the hotter they are, the brighter. These stars are in the most stable part of their existence; this stage generally lasts for about 5 billion years. As stars begin to ...
Stars - winterk
Stars - winterk

... Fast-burning, hot (blue) stars only last for a million years… yikes! ...
Here - Thanet Astronomy Group
Here - Thanet Astronomy Group

Assessment 1 - Stars - Teacher Key
Assessment 1 - Stars - Teacher Key

... 4. Gravity pulls particles together. 2 5. Large cloud of gas and dust. 1 ...
Classification_of_Stars_By_Luminosity
Classification_of_Stars_By_Luminosity

... He called the brightest stars in the sky first magnitude and the dimmest visible to the naked eye sixth magnitude. Stars of intermediate brightness were given intermediate values. ...
Word
Word

... In recent years radio astronomers have tracked the angular position of the supermassive black hole (aka, Sgr A*) located at the center of our Milky Way galaxy with respect to a very distant, fixed background of quasars. That location seems to move because of the Sun’s orbital motion in our galaxy. I ...
ppt
ppt

Looking out at the Night Sky What questions do you have?
Looking out at the Night Sky What questions do you have?

< 1 ... 142 143 144 145 146 147 148 149 150 ... 200 >

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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