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Ch.1, Sec.3 - Mapping the Stars
Ch.1, Sec.3 - Mapping the Stars

... planets and we use the lightyear to measure their distance from us - one light-year represents the distance light travels in 365 days (6 trillion miles @ 186,000 miles per second) ...
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... These questions are not the same as questions on the exam. It is important to understand the topics covered in class in the slides as well as the lecture tutorials. The exam is not based on rote learning. ...
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Stars Galaxies Sun

... from an observer.  Blue Shift: shorter wavelengths, stars moving towards Earth  Red Shift: longer wavelengths, stars moving away from Earth ...
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... proposed research is the provision of a data set and pipeline that can be searched, by members of PALFA and the astronomical community, for transient phenomena according to whatever templates they chose. The raw dataset is currently 240TB, accumulated from 210,000 on-sky "beams"; a reduction by a fa ...
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Milky Way galaxy - Uplift North Hills Prep
Milky Way galaxy - Uplift North Hills Prep

... Before October 6, 1923, astronomers thought the Andromeda Nebula and similar objects were bright pockets of matter inside the Milky Way. On that day astronomer Edwin Hubble noticed, looking at the photograps, a particular type of star inside the Andromeda Nebula. Hubble realized that the star (Ceph ...
The Temperatures of Stars
The Temperatures of Stars

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Distances to Stars: Parsecs and Light Years
Distances to Stars: Parsecs and Light Years

... E le altre stelle”… Dante, end Of Paradiso ...
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... • The Andromeda Galaxy is 2.2 million light years away from Earth. • This Means that the light we see from Andromeda Galaxy left there 2.2 million years ago. • It is therefore very possible that some of the stars in Andromeda have exploded as a supernova or gone out long ago. The message of these st ...
History of Astronomy
History of Astronomy

... • All of Galileo's observations were pointing towards a heliocentric view of the universe • Galileo published his observations and conclusions in multiple works, including some published in Italian to appeal to a wider audience • Galileo was threatened with torture, forced to deny his beliefs in the ...
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SES4U Life Cycle of a Star

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Jun 2015 - Astronomical Society of Northern New England
Jun 2015 - Astronomical Society of Northern New England

... atmosphere's airflow all in one swoop. It's also the best way, so long as you're up at high enough altitudes, to view an entire 50 percent of Earth all at once. And if you place your observatory at just the right location, you can observe the same hemisphere of Earth continuously, tracking the chang ...
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... revisited a part of sky that had been imaged in 1995. This star forming region in the Eagle Nebula was dubbed the “Pillars of Creation”. Here is the image that was released this year showing just how much Hubble’s abilities had improved after its 2009 serving mission. In addition, Hubble’s new camer ...
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... multiple-star system. Scientists suspected that the process was casused by a gravitational instability, but new observations from the Atacama Large Millimeter/submillimeter Array (ALMA) and the Karl G. Jansky Very Large Array (VLA) showed the process in action. John Tobin, from the University of Okl ...
Spring 2014 Astronomy Exam Study Guide (Co-Taught)
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...  Core becomes either a neutron star or a black hole Supernovae  Creation of heavy elements in the supernova explosion  Role of supernovae in dispersing interstellar space with heavy elements General Review Questions: 39. Describe the full life cycle of our sun, including all major stages of its l ...
It is evident from our observations of impact craters on planets and
It is evident from our observations of impact craters on planets and

... telescopes and instruments that accurately measure and analyze starlight. In particular, stellar spectra provide useful information. From the spectrum a star’s composition and temperature can be determined. (See the lecture handouts for descriptions of how stellar properties are determined.) Astrono ...
stars - Chatt
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... that can last for weeks and reach 40,000 km high. • Solar Flare: Like a solar prominence, but the gases travel into the corona, and last only a few minutes. ...
PHS 111 Test 3 Review Chapters 26-28
PHS 111 Test 3 Review Chapters 26-28

... According to relativity theory, it is possible to reverse time and grow younger when you: are near a black hole. are near a very large gravitational field. travel at nearly the speed of light. you can never grow younger. Dark Matter is matter that: cannot be seen, felt, or measured. cannot be seen o ...
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PHS 111 Test 3 Review Chapters 26-28
PHS 111 Test 3 Review Chapters 26-28

January 2015 - Hermanus Astronomy
January 2015 - Hermanus Astronomy

... atmosphere. "It's almost like theses electrons are running into a glass wall in space," said Baker, "somewhat like the shields created by force fields on Star Trek that were used to repel alien weapons, we are seeing an invisible shield blocking these electrons. It's an extremely puzzling phenomenon ...
I pledge that I have neither given nor received any unauthorized aid
I pledge that I have neither given nor received any unauthorized aid

... C) in an elliptical orbit, with the Sun on the minor axis of the ellipse. D) in an elliptical orbit, with the Sun at the center of the ellipse. ...
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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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