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Section 19.2
Section 19.2

Lecture 24 - Empyrean Quest Publishers
Lecture 24 - Empyrean Quest Publishers

... Hipparchus rated stars he could see from 1 to 6. A '1' is 2.52 x brighter than a '2', etc. ...
The Stars and the Solar System
The Stars and the Solar System

Chapter 5 Notes
Chapter 5 Notes

... A. __________ gravity holds together a large collection of stars, gas, and dust 1. Earth galaxy is Milky Way which is part of a galaxy cluster named the ______ _____. 2. _______ _______ - spiral arms wind out from inner section; some have barred spirals with stars and gas in a central bar 3. _______ ...
The Stars and the Solar System
The Stars and the Solar System

Where do you find yourself now??
Where do you find yourself now??

Stars
Stars

... •The ratio and sum provide each mass individually. ...
The Universe
The Universe

The Electromagnetic Spectrum: Astronomy 1
The Electromagnetic Spectrum: Astronomy 1

Document
Document

Stellar Classification and Evolution What is a star? A cloud of gas
Stellar Classification and Evolution What is a star? A cloud of gas

...  The Death of Low-Mass Giants and Supergiants  In _________ mass stars (0.4 – 8.0 x solar mass) strong solar winds and energy bursts from helium fusion _____________ much of their mass  The ejected material expands and cools, becoming a planetary ________________ (which actually has nothing to do ...
The Universe
The Universe

What is a star?
What is a star?

The Night Sky May 2016 - Bridgend Astronomical Society
The Night Sky May 2016 - Bridgend Astronomical Society

Two Summers in the UCSC Science Internship Program
Two Summers in the UCSC Science Internship Program

... stars are unusual: Stars are known to form in clusters, so it is rare to find a young, recently formed star in isolation. This anomalous behavior makes field stars an exciting and hotly debated subject. One theory proposes that field stars do, in fact, form by themselves; another claims that field s ...
TYPES OF STARS
TYPES OF STARS

... When astronomers look through their telescopes, they see billions of stars. How do they make sense of all these stars? The 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 (cal ...
dtu7ech11 - Fort Thomas Independent Schools
dtu7ech11 - Fort Thomas Independent Schools

Astronomy 100  Name(s):
Astronomy 100 Name(s):

... Once The Sky is open, go to Data → Location and confirm the location is Seattle, Washington (if not, you can choose this from the predefined list). Next go to Data → Time and set the time for 9 p.m. tonight. If you have time, you may wish to play with some of the following controls: on the second li ...
Transcript_Forbidden Planets
Transcript_Forbidden Planets

Stellar Evolution - Harnett County High Schools Wiki
Stellar Evolution - Harnett County High Schools Wiki

mam.evolution
mam.evolution

... We already know that hotter stars are brighter. ...
Small Wonders: Ursa Minor
Small Wonders: Ursa Minor

... from the showing true north. Not only that, but the relationship between North and the North Star is constantly changing. Because of a phenomenon known as precession, (basically a wobble of earth along it's axis - much like a top) the northern pole carves out a 47 degree diameter circle on the nigh ...
Orion- The Swordsman of the Sky - A Winter Constellation from the
Orion- The Swordsman of the Sky - A Winter Constellation from the

HR Diagram and Life of a star
HR Diagram and Life of a star

... The hot core remains with all of the gas around it. We call this a Planetary Nebula Eventually the gas surrounding the core blows off and we are left with a hot core called a White Dwarf This will cool off after 20 billion years leaving a cold core called a Black dwarf ...
ppt
ppt

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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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