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etlife_douglas_ewart_short

... Exoplanets are ‘drowned out’ by their parent star. That makes them very hard to see directly with ...
Scientific Results Summary
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... brought discoveries of interest to subjects ranging from Solar System bodies to stellar composition and distant dark matter. Subaru continues to lead the path of discovery for large 8m-class earth-based telescopes. One of the most globally exciting events, especially in the world of astronomy, was N ...
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... telescopes have directly measured the mass of an ultra-cool brown dwarf star and its companion dwarf star for the first time. Barely the size of the planet Jupiter, the dwarf star weighs in at just 8.5 percent of the mass of our Sun. This is the first ever mass measurement of a dwarf star belonging ...
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... extreme cases, billion solar masses. Our own galaxy, the Milky Way is no exception. ...
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Study Guide 4 Part A Outline
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... o Most of the mass of the Milky Way is dark matter. The existence of the dark matter is inferred from the effect that its gravity has on stars in the outer part of the Galaxy. Those stars are orbiting faster than they would be expected to be moving if there were no dark matter. Nobody knows what the ...
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... 1610, which opened up new worlds to humanity. In addition to revealing that the planets were in fact worlds of their own, his observations revealed:  The Milky Way (MW) consisted of countless stars, millions more than previously known.  Stars could be double or multiple, slowly orbiting each other ...
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... use almost the same method anytime we measure the masses of astronomical objects. What quantities would an astronomer have to measure to determine the mass of a cluster of galaxies? (Your method should include all of the mass, not just the mass of the luminous matter.) We measure masses by seeing ho ...
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... That means it would take 490 years traveling at 186,000 miles per second—the speed of light—to get there. It circles its home star, Kepler-186, in just 130 days. (11) That star is an M-dwarf, smaller, dimmer and cooler than our sun. So even though Kepler-186f sits closer to its sun than Mercury doe ...
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Introduction Notes - Sunflower Astronomy

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Space Interferometry Mission



The Space Interferometry Mission, or SIM, also known as SIM Lite (formerly known as SIM PlanetQuest), was a planned space telescope developed by the U.S. National Aeronautics and Space Administration (NASA), in conjunction with contractor Northrop Grumman. One of the main goals of the mission was the hunt for Earth-sized planets orbiting in the habitable zones of nearby stars other than the Sun. SIM was postponed several times and finally cancelled in 2010.In addition to hunting for extrasolar planets, SIM would have helped astronomers construct a map of the Milky Way galaxy. Other important tasks would have included collecting data to help pinpoint stellar masses for specific types of stars, assisting in the determination of the spatial distribution of dark matter in the Milky Way and in the Local Group of galaxies and using the gravitational microlensing effect to measure the mass of stars.The spacecraft would have used optical interferometry to accomplish these and other scientific goals. This technique collects light with multiple mirrors (in SIM's case, two) which is combined to make an interference pattern which can be very precisely measured.The initial contracts for SIM Lite were awarded in 1998, totaling US$200 million. Work on the SIM project required scientists and engineers to move through eight specific new technology milestones, and by November 2006, all eight had been completed.SIM Lite was originally scheduled for a 2005 launch, aboard an Evolved Expendable Launch Vehicle (EELV). As a result of continued budget cuts, the launch date has been pushed back at least five times. NASA has set a preliminary launch date for 2015 and U.S. federal budget documents confirm that a launch date is expected ""no earlier"" than 2015. The budget cuts to SIM Lite are expected to continue through FY 2010. As of February 2007, many of the engineers working on the SIM program had moved on to other areas and projects, and NASA directed the project to allocate its resources toward engineering risk reduction. However, the preliminary budget for NASA for 2008 included zero dollars for SIM.In December 2007, the Congress restored funding for fiscal year 2008 as part of an omnibus appropriations bill which the President later signed. At the same time the Congress directed NASA to move the mission forward to the development phase. In 2009 the project continued its risk reduction work while waiting for the findings and recommendations of the Astronomy and Astrophysics Decadal Survey, Astro2010, performed by the National Academy of Sciences, which would determine the project's future.On 13 August 2010, the Astro2010 Decadal Report was released and did not recommend that NASA continue the development of the SIM Lite Astrometric Observatory. This prompted NASA Astronomy and Physics Director, Jon Morse, to issue a letter on 24 September 2010 to the SIM Lite project manager, informing him that NASA was discontinuing its sponsorship of the SIM Lite mission and directing the project to discontinue Phase B activities immediately or as soon as practical. Accordingly, all SIM Lite activities were closed down by the end of calendar year 2010.
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