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PLANETS
PLANETS

... square root of semi-major axis • No strong selection bias in favour / against detecting planets with different eccentricities Of the first 100 stars found to harbor planets, more than 30 stars host a Jupiter-sized world in an orbit smaller than Mercury's, whizzing around its star in a matter of days ...
Cosmology with GMRT
Cosmology with GMRT

... distribution in dwarfs should reflect that predicted by numerical simulations  Details of ‘baryon physics’, e.g.  the mass to light ratio of the stellar population,  feedback from baryonic cooling and collapse on the structure of the Dark Matter Halo ...
– 1 – 1. Historical Notes for Ay 123 1.1.
– 1 – 1. Historical Notes for Ay 123 1.1.

... Either on the ground or in space, a parallax project must observe a star repeatedly over a year (probably over several years) to measure a parallax. The project must have a list of stars to be observed BEFORE the project can begin (an input catalog). There must be a scheduling algorithm (minimize te ...
The cosmic distance ladder
The cosmic distance ladder

... distances in terms of the AU. Mercury: 0.307-0.466 AU Venus: 0.718-0.728 AU Earth: 0.98-1.1 AU Mars: 1.36-1.66 AU Jupiter: 4.95-5.46 AU Saturn: 9.05-10.12 AU Uranus: 18.4-20.1 AU Neptune: 29.8-30.4 AU ...
Document
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... Describing the Wavefronts The aberrated wavefront is compared to an ideal spherical wavefront called a the reference wavefront. The optical path difference (OPD) is measured between the spherical reference surface (SRS) and aberated wavefront (AWF) The OPD function can be described by a polynomical ...
The Fundamental Plane, Stellar Popula6ons
The Fundamental Plane, Stellar Popula6ons

... What
is
the
relaBon
between
stellar
mass
and
dynamical
mass,
 and
how
does
this
vary
with
parent
halo
mass
&
environment?
   How
do
the
observed
trends
in
stellar
populaBons
vary
with
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(NN/local
density/cluster
radius/cluster
richness)?
   What
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of
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FP
and
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Universe 8e Lecture Chapter 24 Galaxies
Universe 8e Lecture Chapter 24 Galaxies

... Hot intergalactic gases in rich clusters account for a small part of the unobserved mass. These gases are detected by their X-ray emission. The remaining unobserved mass is probably in the form of dark-matter halos that surround the galaxies in these clusters. Gravitational lensing of remote galaxie ...
The cosmic distance ladder
The cosmic distance ladder

... distances in terms of the AU. Mercury: 0.307-0.466 AU Venus: 0.718-0.728 AU Earth: 0.98-1.1 AU Mars: 1.36-1.66 AU Jupiter: 4.95-5.46 AU Saturn: 9.05-10.12 AU Uranus: 18.4-20.1 AU Neptune: 29.8-30.4 AU ...
15-3 Notes: Galaxies
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... two-thirds of the way between the center of the galaxy and the galaxy’s edge. Because most elliptical galaxies are round or oval, they can be thought of as “cosmic snowballs.” Some elliptical galaxies are slightly flattened. Elliptical galaxies are among the largest in the galaxies in the universe. ...
The Milky Way
The Milky Way

... • Out to solar distance (about 8 kpc) the mass is about 1 x 1011 M (mostly stars) • Out to ~15 kpc, (the visible radius) a good estimate for the mass is nearly 4 x 1011 M ...
Lecture Notes – Galaxies
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... 2 = G M/R to determine the mass (M) inside a star at orbital radius (R), given a rotation velocity Vrot (Vrot ). (M as ∼ 1011 M for our Galaxy.) Plotting V against R gives the rotation curve of the Galaxy. Our own galaxy, in common with other spiral galaxies, is observed to have a flat rotation cur ...
Upcoming Events
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... The year 2015 marked big progress on NASA's James Webb Space Telescope and there are still a number of large milestones before the next generation telescope is launched in 2018. Recently, all of the 18 segments of the Webb telescope primary mirror segments were installed on the observatory's backpla ...
Basic Properties of Stars
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... Adults ...
Multiple Choice, continued Stars, Galaxies, and the Universe
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... Today, we know that Copernicus was right: the stars are very far from Earth. In fact, stars are so distant that a new unit of length—the light-year—was created to measure their distance. A light-year is a unit of length equal to the distance that light travels through space in 1 year. Because the sp ...
Hubble`s Use of Cepheids (PDF version)
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... astronomer, had earlier noticed the variability of these stars on photographs and had described that to Shapley, when he was still working at Mount Wilson. (Shapley later moved to Harvard.) Shapley had dismissed this as impossible – he ‘knew’ that the spiral nebulae were small, nearby objects. It wa ...
Stars and Their Characteristics
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... Black hole: The final life stage of an extremely massive star, with a gravitational field so intense that not even light can escape. Black holes are areas in space where there is a huge amount of mass in a very small space. The gravity of this mass is so great that everything in the area is pulled ...
Gugus Bintang [Compatibility Mode]
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... 2. Identify stellar types (such as blue giant stars and red giant stars), determine luminosity from the type, measure brightness, and then calculate distance. If the giant star is in a cluster, then we can determine the distance to the cluster by using several giant stars in the cluster to get its d ...
Chapter 31 - The Galaxy & Universe
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... Other Galaxies – 30.2 Objectives • Describe how astronomers classify galaxies • Identify how galaxies are organized into clusters and superclusters • Describe the expansion of the universe ...
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... irregulars with low mass; most are satellites of MW, M31 or M33 • The gravitational interaction between these systems is complex but the local group is apparently bound. • Major advantages – close and bright- all nearby enough that individual stars can be well measured as well as HI, H2, IR, x-ray s ...
Galaxies and Cosmology
Galaxies and Cosmology

... (Copernicus, Shapley) should make us skeptical of this idea How else can we explain these facts? If the entire universe is expanding then every galaxy sees all others receding, and if that expansion is uniform, then the rate of motion apart is proportional to distance (Hubble’s Law) Note: because gr ...
Introduction
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... have the same “gravitational charge”. The structure and evolution of stars is governed by a delicate balance between gravity, radiation, and nuclear processes. The structure of a galaxy, on the other hand, is basically determined by gravity – other forces only enter indirectly. The three key ingredi ...
Word Document - Montana State University Extended
Word Document - Montana State University Extended

... Scientists generally agree that the Earth formed about 4.5 billion years ago yet complex life has existed on the Earth for about the last 500 million years. It is still unclear exactly what chain of events lead up to the emergence of complex life on this planet. One of the factors that scientists be ...
Astronomy 115: Finding New Worlds
Astronomy 115: Finding New Worlds

... other stars? How do solar systems form? and How can we study these distant worlds to look for life? Until a little over a decade ago planets were known to exist around exactly one star, our sun. Since then hundreds of planets have been identified around other stars opening up an entirely new field d ...
Frontiers of Astrophysics - Space Telescope Science Institute
Frontiers of Astrophysics - Space Telescope Science Institute

... structures seen in simulations. Galaxies form along filaments. Clusters of galaxies form at the intersection of filaments. ...
Supermassive black holes
Supermassive black holes

... Edwin Hubble used observations of _______ to determine the distance to the ...
< 1 ... 42 43 44 45 46 47 48 49 50 ... 113 >

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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