Goals & Objectives - Sierra College Astronomy Home Page
... Read all the homework questions before the first lecture of the week. Attend lectures with PowerPoint lecture notes from the Student Handbook and CPS devices (“clickers”) Work in groups. Do not wait to the last minute to prepare for exams. ...
... Read all the homework questions before the first lecture of the week. Attend lectures with PowerPoint lecture notes from the Student Handbook and CPS devices (“clickers”) Work in groups. Do not wait to the last minute to prepare for exams. ...
The Solar System
... • By this definition, Pluto is no longer a planet since it has not cleared its neighbourhood of other bodies. – Pluto, and other small spherical solar system bodies in orbit around the Sun are now known as dwarf planets. Spherical bodies in the solar system are in hydrostatic equilibrium. The inward ...
... • By this definition, Pluto is no longer a planet since it has not cleared its neighbourhood of other bodies. – Pluto, and other small spherical solar system bodies in orbit around the Sun are now known as dwarf planets. Spherical bodies in the solar system are in hydrostatic equilibrium. The inward ...
A new Cosmos – a novel Physics
... after adaption in Arabian science, was then used in some variations for centuries in the Arabian culture and Europe for calculating astronomical events, until it was finally replaced by Copernican astronomy. Although Ptolemaic astronomy within a geocentric cosmos allowed a respectably good calculati ...
... after adaption in Arabian science, was then used in some variations for centuries in the Arabian culture and Europe for calculating astronomical events, until it was finally replaced by Copernican astronomy. Although Ptolemaic astronomy within a geocentric cosmos allowed a respectably good calculati ...
Classifying Stars (pages 753–754) Key Concept: Characteristics
... Classifying Stars (pages 753–754) Key Concept: Characteristics used to classify stars include color, temperature, size, composition, and brightness. ...
... Classifying Stars (pages 753–754) Key Concept: Characteristics used to classify stars include color, temperature, size, composition, and brightness. ...
Final Revision Sheet Grade (1) Quarter (3) Multiple Choice
... 30-____11. 30-What is the sun? A. a large ball of rock B. the star closest to Earth C. a sphere that does not give off its own light ____ 12. ____ 13. 31-What can a magnifier do? A. make the sky darker B. make things look bigger C. move things to a new place ____ 14. 32-What is a large ball of rock ...
... 30-____11. 30-What is the sun? A. a large ball of rock B. the star closest to Earth C. a sphere that does not give off its own light ____ 12. ____ 13. 31-What can a magnifier do? A. make the sky darker B. make things look bigger C. move things to a new place ____ 14. 32-What is a large ball of rock ...
The Life Cycle of the Stars
... The star-filled sky is in many ways like a large crowd of people. Within that group you may find babies, children, teenagers, adults and even senior citizens. Like humans, stars pass through different stages in their lives. They are born, they mature and, eventually, they die. However, unlike humans ...
... The star-filled sky is in many ways like a large crowd of people. Within that group you may find babies, children, teenagers, adults and even senior citizens. Like humans, stars pass through different stages in their lives. They are born, they mature and, eventually, they die. However, unlike humans ...
Starry Night¨ Times - October 2008
... Orion Nebula. Although it is 1500 lightyears away, M42 is a great target to view in small telescopes. This is due not only to its brightness, but also to its wonderful cloud structure, which in telescopes takes on a clearly three-dimensional shape. Observers new and old come back to M42 time and tim ...
... Orion Nebula. Although it is 1500 lightyears away, M42 is a great target to view in small telescopes. This is due not only to its brightness, but also to its wonderful cloud structure, which in telescopes takes on a clearly three-dimensional shape. Observers new and old come back to M42 time and tim ...
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 ...
... 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 ...
FREE Sample Here
... One of the things that many of us who teach general education science courses believe we do is to help students learn to critically observe pictures and learn to read graphs and charts. Yet, few of us test this skill. Several of the exam questions in the test bank make use of pictures, tables, and g ...
... One of the things that many of us who teach general education science courses believe we do is to help students learn to critically observe pictures and learn to read graphs and charts. Yet, few of us test this skill. Several of the exam questions in the test bank make use of pictures, tables, and g ...
Stars & Constellations
... Constellations What are constellations? Can you name any? Constellations are groups of stars which may resemble ...
... Constellations What are constellations? Can you name any? Constellations are groups of stars which may resemble ...
Exam Study Guide
... 98. According to the Chart of Stellar Evolution (see Reference Item 7), planetary nebula can form from main sequence stars of mass … UNIT 8 — Galaxies and Cosmology — Bits of Chapters 15-18 100. What makes Cephied Variables very useful for measuring distances? 101. Contrast the motion of the disk st ...
... 98. According to the Chart of Stellar Evolution (see Reference Item 7), planetary nebula can form from main sequence stars of mass … UNIT 8 — Galaxies and Cosmology — Bits of Chapters 15-18 100. What makes Cephied Variables very useful for measuring distances? 101. Contrast the motion of the disk st ...
Constellations
... • The sun blocks star light during the day. • The earth blocks stars too far to the south. • The horizon is the line of the ground for an observer. • A star finder provides a cover that act as the horizon. – You use a different cover depending on your latitude • The planisphere’s wheel turns to set ...
... • The sun blocks star light during the day. • The earth blocks stars too far to the south. • The horizon is the line of the ground for an observer. • A star finder provides a cover that act as the horizon. – You use a different cover depending on your latitude • The planisphere’s wheel turns to set ...
Astronomy Webquest _2 STARS
... Today You Will Learn About the Life Cycle of a Star—Called Stellar Evolution. ...
... Today You Will Learn About the Life Cycle of a Star—Called Stellar Evolution. ...
The Celestial Sphere
... the NCP, so it will seem to stand still, while the rest of the stars rotate around it. It is therefore also known as the Pole Star or the North Star. Some stars will rise and set in the course of the day, while some will rise and set. Stars that never set are called circumpolar. ...
... the NCP, so it will seem to stand still, while the rest of the stars rotate around it. It is therefore also known as the Pole Star or the North Star. Some stars will rise and set in the course of the day, while some will rise and set. Stars that never set are called circumpolar. ...
2012 New York State Science Olympiad Astronomy
... Egregious and/or repeated violations of this rule will be dealt with strictly. 12. Do not be discouraged if you do not finish in the allotted time, as this test is designed to be very difficult, in order to differentiate between the top teams. 13. Please remove this front page before leaving the roo ...
... Egregious and/or repeated violations of this rule will be dealt with strictly. 12. Do not be discouraged if you do not finish in the allotted time, as this test is designed to be very difficult, in order to differentiate between the top teams. 13. Please remove this front page before leaving the roo ...
Astronomy Webquest Part 1: Life of Stars: Go to http://www.odec.ca
... 8. After a supernova, a ___________________________ remains unless the star was dense enough. If the star was extremely dense, a ____________________ forms. Part 2: Analyzing Stars with the H-R Diagram: Go to http://sunshine.chpc.utah.edu/labs/star_life/hr_app.html and answer these questions. 1. If ...
... 8. After a supernova, a ___________________________ remains unless the star was dense enough. If the star was extremely dense, a ____________________ forms. Part 2: Analyzing Stars with the H-R Diagram: Go to http://sunshine.chpc.utah.edu/labs/star_life/hr_app.html and answer these questions. 1. If ...
chapter 2 - Test Bank 1
... People from different cultures all see the same stars, but the asterisms and constellations are different. Technically, we would now all see the same constellations, because these have official definitions and borders; however, this designation might not be well accepted by people of various culture ...
... People from different cultures all see the same stars, but the asterisms and constellations are different. Technically, we would now all see the same constellations, because these have official definitions and borders; however, this designation might not be well accepted by people of various culture ...
A short history of astronomy and telescopes
... “seeing things far away as if they were nearby” • 1609 Galileo built a 1 diameter refracting telescope with 3x magnification and made observations of celestial objects ...
... “seeing things far away as if they were nearby” • 1609 Galileo built a 1 diameter refracting telescope with 3x magnification and made observations of celestial objects ...
Chapter 27 Stars and Galaxies
... Absolute Magnitude Brightness from 32.6 ly Ex: If the sun was 32.6 ly away, it would be a fifth magnitude star. Its absolute magnitude = +5 Most stars are between a -5 and +15 ...
... Absolute Magnitude Brightness from 32.6 ly Ex: If the sun was 32.6 ly away, it would be a fifth magnitude star. Its absolute magnitude = +5 Most stars are between a -5 and +15 ...
Stars and Galaxies
... 9. The constellations also appear to change positions in the sky because the Earth ____________________ around the sun. 10. For example, ________________ is visible in the winter sky, but not in the summer. 11. The _____________________________ of a star is a measure of the amount of light a star ac ...
... 9. The constellations also appear to change positions in the sky because the Earth ____________________ around the sun. 10. For example, ________________ is visible in the winter sky, but not in the summer. 11. The _____________________________ of a star is a measure of the amount of light a star ac ...
Stargazing in ancient Egypt
... the attention of any inquisitive person. Phenomena that typically go unnoticed today would have been obvious to anyone who looked. As in all primitive cultures, the sky was ...
... the attention of any inquisitive person. Phenomena that typically go unnoticed today would have been obvious to anyone who looked. As in all primitive cultures, the sky was ...
ASTR 105 Intro Astronomy: The Solar System
... The Celestial Sphere Stars at different distances all appear to lie on the celestial sphere. ...
... The Celestial Sphere Stars at different distances all appear to lie on the celestial sphere. ...
Chinese astronomy
Astronomy in China has a very long history, with historians indicating that the Chinese were the most persistent and accurate observers of celestial phenomena anywhere in the world before the Arabs. Star names later categorized in the twenty-eight mansions have been found on oracle bones unearthed at Anyang, dating back to the middle Shang Dynasty (Chinese Bronze Age), and the mansion (xiù:宿) system's nucleus seems to have taken shape by the time of the ruler Wu Ding (1339-1281 BC).Detailed records of astronomical observations began during the Warring States period (fourth century BC) and flourished from the Han period onward. Chinese astronomy was equatorial, centered as it was on close observation of circumpolar stars, and was based on different principles from those prevailing in traditional Western astronomy, where heliacal risings and settings of zodiac constellations formed the basic ecliptic framework.Some elements of Indian astronomy reached China with the expansion of Buddhism after the Eastern Han Dynasty (25–220 AD), but the most detailed incorporation of Indian astronomical thought occurred during the Tang Dynasty (618-907), when numerous Indian astronomers took up residence in the Chinese capital, and Chinese scholars, such as the great Tantric Buddhist monk and mathematician Yi Xing, mastered its system. Islamic astronomers collaborated closely with their Chinese colleagues during the Yuan Dynasty, and, after a period of relative decline during the Ming Dynasty, astronomy was revitalized under the stimulus of Western cosmology and technology after the Jesuits established their missions. The telescope was introduced in the seventeenth century. In 1669, the Peking observatory was completely redesigned and refitted under the direction of Ferdinand Verbiest. Today, China continues to be active in astronomy, with many observatories and its own space program.