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Testing
Testing

MS Word version
MS Word version

... At t = 6 hours? _____________________________________________________ At t = 12 hours? _____________________________________________________ Draw in each of these locations and connect the path between the stars. For what fraction of the day is star B visible? _____________________________ d) Draw ...
Nebulae - Innovative Teachers BG
Nebulae - Innovative Teachers BG

December - Rose City Astronomers
December - Rose City Astronomers

... scanty star grouping of DolidzeDžimšelejšvili 1 (Do-Dž 1). This triple star and open cluster combo is a remarkable stroke of cosmic serendipity in an area nearly devoid of other major deep-sky objects. The refractor at 44x shows the 12' diameter star cluster as six stars (9th to 11thmagnitude) embed ...
MS Word version
MS Word version

... At t = 6 hours? _____________________________________________________ At t = 12 hours? _____________________________________________________ Draw in each of these locations and connect the path between the stars. For what fraction of the day is star B visible? _____________________________ d) Draw ...
Chapter 15: The Deaths of Massive Stars
Chapter 15: The Deaths of Massive Stars

... 4. Population I stars contain heavier elements in their atmospheres. They are young stars. 5. The Sun is a Population I star. We know this from its spectrum but also from the fact that the Earth contains heavier elements, and the Earth formed from the same material that made the Sun. Advancing the M ...
Micro_lect20a
Micro_lect20a

... Sun, it is more massive and over 1000 times larger. If placed at the center of our Solar System, it would extend past the orbit of Jupiter. ...
Lesson Overviews and Content Standards
Lesson Overviews and Content Standards

... Key concepts include: • Stars are different ages. • Stars are born in giant clouds of gas and dust. • Many more low mass (cool) stars are born than high mass (hot) stars. Lifetimes of Stars: In this activity, students return to the concept of a scale model to make a scale model of time rather than d ...
Student Exploration Sheet: Growing Plants
Student Exploration Sheet: Growing Plants

The Milky Way Galaxy
The Milky Way Galaxy

Astronomy Part 1 Regents Questions
Astronomy Part 1 Regents Questions

... 11. How soon did protons and neutrons form after the beginning of the universe? A) 10 -43 second C) 10 -6 second ...
Prof. Kenney C lass 8 September 26, 2016
Prof. Kenney C lass 8 September 26, 2016

Astronomical Chronicle  for September, 2008
Astronomical Chronicle for September, 2008

THE HERTZSPRUNG-RUSSELL DIAGRAM
THE HERTZSPRUNG-RUSSELL DIAGRAM

SM_Taurus - Cloudy Nights
SM_Taurus - Cloudy Nights

... beginning of spring planting. Our constellation for the month is located on the edge of the winter Milky Way, and our targets include; three open clusters, one of the brightest supernova remnants in the night sky and a lesser known planetary nebula. By no means is this an exhaustive list of targets ...
Small Wonders: Taurus
Small Wonders: Taurus

... beginning of spring planting. Our constellation for the month is located on the edge of the winter Milky Way, and our targets include; three open clusters, one of the brightest supernova remnants in the night sky and a lesser known planetary nebula. By no means is this an exhaustive list of targets ...
- saspcsus
- saspcsus

... 4. Objects in the sky move in regular and predictable patterns. As a basis for understanding this concept: A. Students know the patterns of stars stay the same, although they appear to move across the sky nightly, and different stars can be seen in different seasons. B. Students know the way in whic ...
Fixed Stars - Mark Dodich
Fixed Stars - Mark Dodich

Practice Exam for 3 rd Astronomy Exam
Practice Exam for 3 rd Astronomy Exam

... peppered with dense cores that are the seed points for future stars. If the GMC is very cold, about 10 K, then it can collapse under the gravity of its own mass and the process of star formation begins. The GMC will collapse and fragment around the very many dense cores in its interior. An empirical ...
Proper Motion of a Star
Proper Motion of a Star

5 Understanding stars and star ClUsters
5 Understanding stars and star ClUsters

20 pm - Starmap
20 pm - Starmap

11 Celestial Objects and Events Every Stargazer Should See
11 Celestial Objects and Events Every Stargazer Should See

Test 3 Review
Test 3 Review

... • Bring at least 2 pencils, UNM student ID, and a calculator 2) During the Test: • Write out and bubble your last name, space, first name and Exam color in the name space of the scantron form. Write out and bubble your Banner ID in the ID space. • Draw simple sketches to help visualize problems • So ...
PHYS_3380_082615_bw - The University of Texas at Dallas
PHYS_3380_082615_bw - The University of Texas at Dallas

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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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