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Life Cycles of Stars
Life Cycles of Stars

... • Remaining core of a supergiant that was more than 40 times the size of our Sun • The core of the supergiant, after a supernova, is so dense that its gravitational pull sucks in space, time, light and matter • Thought to be at the centre of all galaxies ...
Stellar Evolution and the HR Diagram Study Guide
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... Any hot, bright sphere of gas like the sun is called a star ...
Some space objects are visible to the human eye.
Some space objects are visible to the human eye.

... By contrast, the Moon moves across the star background a distance equal to its width every hour as it orbits Earth. The Moon is our closest neighbor. The planets are farther away, but you can see their gradual movements among the constellations over a period of weeks or months. ...
TIME SERIES CENTER-IIC
TIME SERIES CENTER-IIC

... Dark matter (Baryonic). Pan-STARRS will discover more lensing events in a single year than the combination of all monitoring programs which have been active to date. This is because it covers a larger area of the sky and goes deeper. Pan-STARRS data taken over an interval of several years can theref ...
All I Want for Christmas Are Astronomy Toys!
All I Want for Christmas Are Astronomy Toys!

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December - Naples Free-Net
December - Naples Free-Net

... mass of Earth despite being more than one quarter of the Earth's diameter, Io seems like an unlikely candidate for volcanoes, as 4.5 billion years is more than enough time for it to have cooled and become stable. Yet Io is anything but stable, as an abundance of volcanic eruptions were predicted bef ...
CHERENKOV TELESCOPE ARRAY Dainis Dravins OPTIMIZING THE FOR INTENSITY INTERFEROMETRY
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Lecture 5 - Orbits, Sizes, Precession
Lecture 5 - Orbits, Sizes, Precession

... arcsec (p = 0.1″) This means that Vega appears to move from +0.1″ to 0.1″ with respect to distant stars over a year’s observation D(pc) = 1/p(″) = 1/0.1 = 10 pc ...
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... Aldebaran, the brightest star in the constellation of Taurus, which will also be visible this fall? How much brighter or fainter is it? (a) Fomalhaut is 0.36 magnitudes brighter than Aldebaran (b) Fomalhaut is 1.45 magnitudes fainter than Aldebaran (c) Fomalhaut is 2.07 magnitudes brighter than Alde ...
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Lecture 24, PPT version

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Space - Logan Petlak

... • e. Compare the efficacy of various historical and contemporary models of planetary motion, including geocentric and heliocentric models, for explaining observed astronomical phenomena. • f. Describe and explain the role of experimentation, collecting evidence, finding relationships, proposing expl ...
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... Long Essay Questions (choose 1 of each pair of essay questions below): 1A) Define and describe the science of astrobiology. Provide its goals and its methods. 1B) Describe why scientists believe that life could exist on other worlds in our solar system, while also believing that we are unlikely to f ...
ASTRONOMY After Unit 2 you should be able to
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... of the spectrum  Light from distant galaxies is redshifted so they are moving away ...
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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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