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Brighter than the average star?
Brighter than the average star?

... Many popular astronomy books start by explaining how small and unimportant our Solar System is. The famous ‘Hitchhiker’s Guide to the Galaxy’ begins by describing our own star with the words “Far out in the uncharted backwaters of the unfashionable end of the Western Spiral arm of the galaxy lies a ...
File - Mr. Fifield`s Corner
File - Mr. Fifield`s Corner

... Orbit is a regular, repeating path that one object in space takes as it revolves around another one. All orbits are elliptical, which means they are an ellipse, similar to an oval. These orbits result from gravitational forces ...
M13 – The Great Hercules Cluster
M13 – The Great Hercules Cluster

... asterism but so far have not been able to identify it. If anyone out there can describe it better and tell me how to find it I would be grateful. Lastly, check out the nearby 11th magnitude spiral galaxy NGC 6207. It lies just 30’ to the northeast of M13 and can be seen along with M13 in the same wi ...
Physics@Brock - Brock University
Physics@Brock - Brock University

Lecture 3 - Night Sky and Motion of the Earth around the Sun
Lecture 3 - Night Sky and Motion of the Earth around the Sun

... What causes the seasons? 1. The orbit of the Earth is an ellipse, not a circle, and the Earth is closer to the Sun in summer than in winter. 2. The rotation of the Earth is tilted relative to its orbit. ...
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Teacher Subject Title Concept Context Tek/SE Verb
Teacher Subject Title Concept Context Tek/SE Verb

... science notebook: What do you see when you look up at the sky? Does the sky look the same during the day as it does at night? Other than the Moon, what do we see in the night sky? What do you know about stars? Misconceptions: students may think that all of the stars in a constellation are near each ...
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MULTIPLE CHOICE QUESTIONS (50 pts
MULTIPLE CHOICE QUESTIONS (50 pts

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Space Systems - RPS Cloud Server
Space Systems - RPS Cloud Server

... appear to move across the night sky because of Earth’s rotation. They will construct and support an argument regarding why we see differences in the brightness of the sun compared to other stars. Finally, students will use evidence, data, and/or models to describe the gravitational force exerted by ...
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Astronomy 102, Spring 2003 Solutions to Review Problems
Astronomy 102, Spring 2003 Solutions to Review Problems

... from the angular separation of the two stars, you need to know the distance to the system. Properties not requiring knowledge of the distance: temperature, color, spectral type, and chemical compostion. All of these can be measured from the spectrum of the star. For each of them, you will be compari ...
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... center of the solar system. And he put all of the planets in the correct order up to Saturn. Even though he had the sun as the center of the solar system he still believed that the planets traveled in perfect circles and so he still had to use small epicycles to explain the planets motion. He used t ...
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RASC Bulletin June 1996 - Royal Astronomical Society of Canada
RASC Bulletin June 1996 - Royal Astronomical Society of Canada

... always a bad speller! The more important in­ sight was that one can do amazing things with ...
Physics@Brock - Brock University
Physics@Brock - Brock University

... 11. Suppose that you are not very familiar with the stars and constellations, but you notice that the circumpolar stars which you observe move counterclockwise. Then you must be located in the (a) northern hemisphere. (b) southern hemisphere. (c) [No definite statement can be made.] 12. How can one ...
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... The spyglass-turned-telescope had limitations, some of which Galileo was able to design around. To reduce distortions such as elongations and blurriness caused by the curvature of the "objective" lens—the convex lens at the far end of the telescope—Galileo ground a lens larger than he needed, for ex ...
The Fate of Massive Stars
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... increased opacity due to presence of various Ions (including Fe) in stellar atmosphere Diagonal upper-luminosity cutoff that is temperature dependent Hotter --> Higher Luminosity cutoff Greater mass-loss/stellar winds for cooler stars at lower luminosities Stellar winds important contribution to ISM ...
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Tour of the Universe

... ● 6 of the planets have moons orbiting them. Them bigger ones have more moons than the  smaller ones.  ● Earth's moon was formed 4.5 billion years ago from material ejected when a collision  occurred between a Mars­size object and the Earth.  Asteroids  ● Rocky objects orbiting the Sun­ with million ...
The Sun and the Solar System
The Sun and the Solar System

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... The moon can come between us and the sun. The planets (in order of speed) – Mercury, only seen near sunrise and sunset – Venus, also a morning or evening star – Mars, Jupiter and Saturn travel the enitre zodiac ...
ASTRONOMY AND ASTROPHYSICS
ASTRONOMY AND ASTROPHYSICS

... atmosphere using molecular lines as diagnostics, properties of the 5-minutes oscillations in the photosphere now known as the p-mode oscillations, mapping of the weak longitudinal magnetic fields with a Babcock type magnetograph constructed at Kodaikanal. A study of the spectroscopic profiles in the ...
te acher`s guide te acher`s guide
te acher`s guide te acher`s guide

... question using computer graphics and space footage. What are the signs of the zodiac? The signs of the zodiac are twelve different groups of stars that are named after animals or mythical creatures.They are constellations — patterns of stars in the night sky — that appear to create outlines of pictu ...
81 - Armenian Astronomical Society
81 - Armenian Astronomical Society

... The IAU fully supports the involvement of the general public in the naming of astronomical objects, whether directly or through an independent organised vote, in the naming of planetary satellites, newly discovered exoplanets, and their host stars. This follows a well-established tradition for namin ...
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International Ultraviolet Explorer



The International Ultraviolet Explorer (IUE) was an astronomical observatory satellite primarily designed to take ultraviolet spectra. The satellite was a collaborative project between NASA, the UK Science Research Council and the European Space Agency (ESA). The mission was first proposed in early 1964, by a group of scientists in the United Kingdom, and was launched on January 26, 1978 aboard a NASA Delta rocket. The mission lifetime was initially set for 3 years, but in the end it lasted almost 18 years, with the satellite being shut down in 1996. The switch-off occurred for financial reasons, while the telescope was still functioning at near original efficiency.It was the first space observatory to be operated in real time by astronomers who visited the groundstations in the United States and Europe. Astronomers made over 104,000 observations using the IUE, of objects ranging from solar system bodies to distant quasars. Among the significant scientific results from IUE data were the first large scale studies of stellar winds, accurate measurements of the way interstellar dust absorbs light, and measurements of the supernova SN1987A which showed that it defied stellar evolution theories as they then stood. When the mission ended, it was considered the most successful astronomical satellite ever.
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