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Andromeda Galaxy www.AssignmentPoint.com The Andromeda
Andromeda Galaxy www.AssignmentPoint.com The Andromeda

... Local Group, which also contains the Milky Way, the Triangulum Galaxy, and about 44 other smaller galaxies. ...
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...  Is there life outside the Solar system?  What fraction of stars harbor planets and what fraction are habitable? ...
Populations of Galaxies and their Formation at z < 7
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... What could these galaxies be, and are they most of the galaxy population at high redshift? No. ...
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... Stellar Lifetime Quiz Consider the information given below about the lifetime of three main sequence stars A, B, and C. Star A will be a main sequence star for 2 million years Star B will be a main sequence star for 70 million years Star C will be a main sequence star for 45,000 million years Which ...
Observational Data
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... by assuming intrinsic ratio of Hβ/Hα constant) as metallicity indicator. If these z~2 starbursts are progenitors of z~1 EROs and local ellipticals, their metallicity should be high, at least near-solar or more. Metallicity is a good indicator of stellar mass. ...
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... • Thirty years ago images were created by crude temperature readings and simple recording devices • In 1980’s the military dedicated the first large sum of money towards infrared advancement (high background infrared) • Recently scientists have changed the technology to focus on lower background hea ...
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... late to resolve “The” comet (at this time, I no longer own the big reflector – had to sell it to buy college supplies for my eldest son many years ago). But the Astroscan did not resolve Mars as I thought it should have. Even with Edmund Scientifics’ bulky Barlow lens, and some very good viewing con ...
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... dependence of the erosion line on mass, combined with the mass distribution observed in Fig. 2, confirms that FX is the main variable, with few massive planets surviving exposure to high radiation as discussed below. The distribution of density with mass displayed in Fig. 3 is also consistent with t ...
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... that the planet must be quite close to receive the same flux as the Earth receives from the Sun. Figure 1b shows the planet orbital distance at which it receives a flux S0 = 1360 W m−2 (the Solar constant) as a dashed line; for white dwarfs the habitable zone is ≈ 102 times closer than on the main s ...
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... • How are stars classified into spectral types? • Stars are classified according to their spectra, with different  spectral types generally corresponding to different  temperatures. In order from hottest to coolest, the major  spectral types are O, B, A, F, G, K, and M. These are subdivided into num ...
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... A galaxy is an assembly of between a billion (109) and a hundred billion (1011) stars. There is often a large amount of dust and gas intermingled, all held together by gravity. The Sun and Earth are in the Milky Way Galaxy. Galaxies have many different characteristics, but the easiest way to classif ...
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... Based on averaged proper motions from PPM and Hipparcos catalogs. UVW are positive in the directions of the Galactic center, Galactic rotation, and the north Galactic pole. Errors in UVW are all smaller than 2.0 km s!1 in all components except for HIP 88399, 88726, and 92024, where poor radial veloc ...
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... clusters. Globular clusters are made up of low metallicity, dense aggregates of 50,000–100,000 stars, gravitationally bound with orbits that are randomly distributed, which leads to their spherical shape. The stars are redder, older ≈ 10 Gyr1 and we do not see any signs of SF taking place there. The ...
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... IZw18 and below (Kudritzki 2002): the number of such stars needed to explain Q(HeII)obs implies a cluster mass ~ 10 - 20 x Mstar of the NW knot of IZw18 These models cannot produce the highest values of HeII4686/Hβ 300 M stellar sources are not detected in IZw18 to date Szecsi, Langer, Yoon+2015: m ...
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the magellanic clouds newsletter - Keele University Astrophysics

... dwarf galaxy (Sgr). Such effects are larger than previous estimates based on the torque of the LMC alone. As a result, Sgr deposits debris in regions of the sky that are not aligned with the present-day Sgr orbital plane. In addition, we find that properly accounting for the movement of the Milky Wa ...
Galaxy Powerpoint Notes
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... Inside of galaxies Ever wondered what was inside a galaxy? Well look no farther, because you’re in one! Unfortunately, galaxies are massive, and we can’t see as much as we wish, and that is why with the assistance of telescopes, astronomers have been able to identify certain things in space. Our gal ...
First Light Sources at the End of the Dark Ages: Direct
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... range of ~6 x 10-19 erg/s/cm2 for 25-30-meter class telescopes. When strong Lyman ! emitters are found, both the Lyman ! and the HeII lines can be observed with R>3000 spectroscopy using a GSMT. Observations can focus on the region in which HeII is expected (e.g., at 1.44 µm or H-band, for the z~7.7 ...
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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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