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Stars
Stars

Document
Document

... • Nebula: New stars form in a cloud of gas and dust. The gas and dust are pulled together by gravity in a ball and gets very dense. Temperature increases, and nuclear fusion begins and the ball of gas and dust starts to glow. • Stars don’t live forever. Stars expand as it grows old. After the hydrog ...
No Slide Title
No Slide Title

galaxies and stars - Valhalla High School
galaxies and stars - Valhalla High School

... faster it is moving. • It takes 2 million years for light from the Andromeda galaxy to reach earth. • Astronomers have classified most galaxies into three main categories: spiral, elliptical and irregular. ...
Startalk
Startalk

...  A big glowing ball of gas!  Contains mainly H and He  They have a core that is dense and super hot!  Nuclear fusion is the source of their energy! ...
Name and Address of your Star.
Name and Address of your Star.

ppt
ppt

... • From there we can calculate how much further away the star must be than the Sun to make it the brightness we see from Earth • Delta Cephei shows has a period of about 5 days • This is a reasonably bright star in the constellation of Cepheus • Cepheids are in other galaxies also, and used similarly ...
Document
Document

... b. Stars found in the lower right part of the main sequence? ...
The life cycle of a star
The life cycle of a star

The Northern sky - Visit Isle of Man
The Northern sky - Visit Isle of Man

... seven brightest stars of the Ursa Major constellation. In the days before we had compasses to navigate, people consulted the night sky and used the stars to work out which way pointed north was. Find the Plough and use the two stars at the end, (Merak & Dubhe) at edge of the plough’s bowl (these are ...
Orion
Orion

... Why does Mintaka appear so dim given that it is very luminous? Which stars are main sequence stars? Rigel is a true supergiant, blazing white-hot star of intense brilliance and dazzling beauty. Its surface temperature is about 12,000 K and its energy output exceeds that of our Sun by a factor of ma ...
Level 4 Constellations North Star, South Star
Level 4 Constellations North Star, South Star

... Next to the Big Dipper, Orion is the most well-known constellation of all. Its shape and group of bright stars dominate the winter sky. It contains more bright stars clustered together than any other single group. To the ancients, the figure represented the giant Orion, placed in the heavens, in a h ...
Science 8 Name: Unit 2 Astronomy Date: Period: LAB
Science 8 Name: Unit 2 Astronomy Date: Period: LAB

... 1. Using the data in the table, plot the location of each star and label it with its name. 2. Complete the data table based on the location of the star on the HR Diagram. 3. Color the columns of the HR Diagram. 4. Answer the questions. Background: The Hertzsprung-Russell Diagram is actually an elabo ...
Astronomy Exam review
Astronomy Exam review

... 39. The seasons on Earth are a direct consequence of the _______ 40. Planets are most easily distinguised from stars in the night time sky with your eye, because they 41.The _____ planets are characterized by deep atmospheres, many satellites, and a solar-like elemental abundance. 42.The _____ plane ...
Stellar Magnitude, Distance, and Motion
Stellar Magnitude, Distance, and Motion

...  Actual star brightness  The apparent magnitude that a star would have if it were (in our imagination) placed at a distance of 10 parsecs (which is 32.6 light years) from the Earth  Used to describe luminosity - The amount of energy a star gives off each second The 20 Brightest Stars in the Sky C ...
Cepheus (constellation)
Cepheus (constellation)

At the Heart of the Matter: The Blue White Dwarf in M 57. Paul Temple
At the Heart of the Matter: The Blue White Dwarf in M 57. Paul Temple

... comparison, the earth itself has an average density of only 5.4 x 103 kg/m3. That means a white dwarf is 200,000 times as dense! ...
SES4U Life Cycle of a Star
SES4U Life Cycle of a Star

Document
Document

... 1. The distance that light travels in space in 1 year is called a _______________. 2. An object that is so massive that light cannot escape its gravity is called a ___________ ___________. 3. A large, reddish star that is late in its life cycle is called a _______ ________. 4. A small, hot, dim star ...
21-2 - Laconia School District
21-2 - Laconia School District

ASTR2050 Spring 2005 • In this class we will cover: Brief review
ASTR2050 Spring 2005 • In this class we will cover: Brief review

... Greek letter (in order of brightness) then constellation e.g. α-Orionis is brightest star in Orion (aka Betelgeuse) δ-Cephei is fourth brightest star in Cepheus Variable stars Listed in order of discovery, starting with “R”, then “S” and on through “Z”, then “RR..RZ...SS...SZ...ZZ”, and then “AA...A ...
AST 207 Homework 5 Due 14 October 2011
AST 207 Homework 5 Due 14 October 2011

... 2. Life on Deneb. Here you will find out what it means to live near a giant like Deneb. Recall that the luminosity of a star, where T is its temperature and R is its radius. Star ...
stars
stars

... • Are a group of stars that are connected together to make a picture (like connect the dots) • They were used but early explorers to navigate the sea at night • All together there are 88 constellations in the night sky. ...
How Is a Star`s Color Related to Its Temperature?
How Is a Star`s Color Related to Its Temperature?

... On a clear night you have surely noticed that some stars are brighter than others. But stars also have different colors. Rigel is blue, and Betelgeuse is red. Capella and our sun are yellow. In this activity you will make your own Hertzsprung-Russell diagram. You will see how star brightness, color, ...
Life Cycle of a Star
Life Cycle of a Star

... Remnants can be seen for several weeks ...
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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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