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AST4930 Star and Planet Formation
AST4930 Star and Planet Formation

... Spectroscopic analysis can identify if an early type star is in main-sequence or already leaving the main sequence. In the first case, it follows a given temperature-luminosity relation, which can be exploited to determine their distance (but reddening must be corrected for). ...
81 KB - CSIRO Publishing
81 KB - CSIRO Publishing

... Milky Way ‘dwarf spheroidal galaxies’ and ‘dwarf elliptical galaxies’ are not galaxies.  Hosts a Satellite Stellar System Evidence that a galaxy dominates its environment could come from the presence of smaller satellite stellar systems, such as dwarf galaxies (for large galaxies) or globular clust ...
Characteristics of Stars
Characteristics of Stars

... distance from Earth and how bright the star actually is. The brightness of a star can be described in two different ways: apparent brightness and absolute brightness. A star’s apparent brightness is its brightness as seen from Earth. Astronomers can measure apparent brightness fairly easily using el ...
EASTERN ARIZONA COLLEGE Lab - Introduction to Astronomy
EASTERN ARIZONA COLLEGE Lab - Introduction to Astronomy

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Collaborations with East Asian VLBI stations

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... 1.  The  distance  of  Earth  to  the  sun  (one  AU)  is  very  small   compared  to  interstellar  distances,  so  parallax  angles  are   smaller  than  one  arcsecond,  which  is  1/3600  of  a  degree. 2.  An  alternative  distance  measurement  for  stars  used  by   most  astronomers  is  the ...
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Investigate Planets, Stars, Galaxies, and the Universe

... the city, state, country, and continent. Continue with Earth, the Solar System, the Milky Way Galaxy, the Virgo Supercluster, and the observable universe (the school’s “long address”). This will give students a sense of their place in space. Next, have them watch a video called “The Known Universe” ...
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... Our Milky Way galaxy displays the same characteristics that we associate with ecosystems if we view it on appropriately large scales of distance and time. This can most clearly be seen if we take an imaginary trip outside our Galaxy, to view it from afar. Seen face-on the Galaxy appears as a spiral, ...
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... (an example of spherical aberration) The Hubble primary mirror was polished to an incorrect shape meaning it is slightly too flat on the edges and light was not all focused to the same point. Hubble was then given eyeglasses in the form of COSTAR (Corrective Optics Space Telescope Axial Replacement) ...
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Planet Formation

... Planets form from the accretion disk present around a young star. Rocky planets like the terrestrial planets of the solar system form mainly from the dust inside this disk while gas giants are mainly build out of gas, with a solid core. The formation occurs in various steps. The first step is for th ...
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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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