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α Cen A + iodine cell spectrum - Department of Physics and Astronomy
α Cen A + iodine cell spectrum - Department of Physics and Astronomy

... by Guedes et al. for α CenB. All simulations yield 1 to 4 Earth-mass planets of which 42% lie inside the star’s habitable zone (dashed lines). The planetary configuration of the solar system is shown for reference. Starting conditions: N lunar-mass bodies in a disk with 1/a surface density. ...
The Milky Way By
The Milky Way By

... the Local Fluff inside the Local Bubble, and in the Gould Belt, at a distance of 7.62±0.32 kpc (~25,000±1,000 ly) from the Galactic Center. Padurariu Cristian & Danciu Serban ...
Fact Sheet - NASA Spitzer Space Telescope
Fact Sheet - NASA Spitzer Space Telescope

... With the help of NASA's sponsorship, industrial fabricators and university researchers worked together to reduce the electronic noise and increase the sensitivity and performance of infrared detectors. The great leap in light sensitivity has been matched by a dramatic increase in the size of detecto ...
The cosmic distance ladder
The cosmic distance ladder

... have implied that the stars were an absurdly large distance away. ...
Extrasolar Planets - University of Maryland Astronomy
Extrasolar Planets - University of Maryland Astronomy

... earlier. High-mass, short-period planets are much easier to detect than low-mass or longperiod planets. None of the terrestrial planets (Mercury through Mars) could be seen, for example. It is therefore not surprising that we have this bias. As the time of observation has lengthened, so has the maxi ...
News Release - האוניברסיטה העברית
News Release - האוניברסיטה העברית

... The question that emerged was how these galaxies were able to form stars so quickly and in large quantities at such an early stage without massive galactic mergers. In the article published in Nature, Prof. Dekel and his Hebrew University and French associates, pose their new theoretical model, whic ...
PDF - BYU Studies
PDF - BYU Studies

... energy stores and (2) to infer the life story (evolution) of a star. These in turn required (a) an understanding of the nature of energy and its relation to work and heat, (b) a fair estimate of the total power output of the sun and stars, and (c) knowledge of the chemical composition of the stars. ...
Starbursts – from 30 Doradus to Lyman
Starbursts – from 30 Doradus to Lyman

... to last more than a few years. A robotic repair mission is currently under design, but many are sceptical that this will be realized rapidly enough to avert disaster for our community. ...
The Reflector: January 2010 - Peterborough Astronomical Association
The Reflector: January 2010 - Peterborough Astronomical Association

... star birthing area in Sagittarius to two double stars in Cygnus, a million stars in a ball in Hercules, and finally to the final stages of star life in M57 and M27, all in one night. It’s quite a story and you’ll meet a red giant star—Antares—along the way. Planet buffs will also be able to take in ...
ph507lecnote06
ph507lecnote06

... telescope in survey mode (2) Practical: • stellar activity - young or otherwise active stars are not stable at the m/s level and cannot be monitored with this technique • remaining systematic errors in the observations Currently, the best observations achieve:  ~ 3 m/s ...in a single measurement. T ...
Exploring the Universe and Our Origins - from Hubble to JWST!
Exploring the Universe and Our Origins - from Hubble to JWST!

... Animation from the HST SWEEPS Project Sagittarius Window Eclipsing Exo-Planet Survey! ...
GEARS Workshop Monday - Georgia Southern University
GEARS Workshop Monday - Georgia Southern University

... • Engage: What are some questions you have about stars right now? • Brainstorm a list on your whiteboards. ...
The Life Cycle of Spiral Arm Galaxies
The Life Cycle of Spiral Arm Galaxies

... As  a  star  goes  supernova,  it  releases  a  great  amount  of  energy  (light)  and  also  ejects  a   massive  amount  of  matter  (galactic  cosmic  rays),  which  are  charged  particles  such  as   protons  and  pieces  of   ...
Planetary system
Planetary system

... Terrestrial planets: include mercury, venus, earth, and mars which are made up of mostly refractory materials. Giant planets: include Jupiter, Saturn, Uranus, and Neptune which are made up of volatile materials. ...
Lecture 13
Lecture 13

... • All stars become larger and redder after exhausting their core hydrogen fuel: giants and supergiants. • Most stars end up small and white after all fusion has ceased: white dwarfs. • The white dwarf stage is the final stage for most stars. ...
Target Stars for Earth-like Planet Searches with the Terrestrial
Target Stars for Earth-like Planet Searches with the Terrestrial

... (2) Using catalogued colors and magnitudes it is possible to calculate the basic parameters for an Earth-like planet near each of the stars, including the diameter of the Habitable Zone (HZ). For these purposes, the HZ is defined as the distance from the star at which an Earth-like planet would have ...
ppt
ppt

... How can we test theories of star evolution? • Binaries help, because one can get mass so that theories can be tested • But stars change so slowly, it is impossible to test theories by watching just one star move through phases • Fortunately, there are 1011 stars in our Galaxy, all with a range of ma ...
Kepler-452b is not a new Earth A twin of the Sun
Kepler-452b is not a new Earth A twin of the Sun

... by the Alice spectrograph, which demonstrate how Pluto’s upper atmosphere is overall much more extended into space than previously thought: 1,600 km instead of 270 km. This new measurement is the result of a Sun-Pluto-spacecraft alignment, carefully planned in order to backlit its atmosphere to inve ...
Stars and Planets - The University of Texas at Dallas
Stars and Planets - The University of Texas at Dallas

... Scale Models of Planetary Systems Using the same 1 to 10 billion scale factor we used for the Scale Model Solar System and our everyday objects to represent stars and planets, we can model the extrasolar planetary systems found around other stars. ...
W > 1 - The Open University
W > 1 - The Open University

... Further west than Uranus and beginning to emerge into the predawn skies Neptune is still not an easy object to observe. ...
Astrobiology: The Search for Extraterrestrial Life
Astrobiology: The Search for Extraterrestrial Life

... that life should be present on other planets with similar characteristic to Earth-like organisms. Currently, there are several different projects aimed at detecting Earth-like exoplanets, including NASAs Terrestrial Planet Finder (TPF: recently canceled) and Kepler, launched in 2009. The goal of the ...
1 Marsbugs: The Electronic Astrobiology Newsletter, Volume 12
1 Marsbugs: The Electronic Astrobiology Newsletter, Volume 12

... In the new CU-Boulder scenario, it is a hydrogen and CO2-dominated atmosphere that leads to the production of organic molecules, not the methane and ammonia atmosphere used in Miller's experiment, Toon said. Tian and other team members said the research effort will continue. The duration of the hydr ...
Document
Document

... Low mass stars are stars like our Sun. Low mass stars are stars with mass < 8 times the mass of our Sun. High mass stars are stars with mass > 8 times the mass of our Sun. Most stars are 0.2 to 20 times MSun (over 30 MSun very rare) Upper limit 150 MSun Lower limit 0.08 MSun Below the lower limit, n ...
European Extremely Large Telescope (E-ELT) - DESY
European Extremely Large Telescope (E-ELT) - DESY

... formation history, and decoding this information offers detailed insights into the galaxy's past. However, studying stellar populations requires the capability of resolving and measuring individual stars and so up until now such studies have been limited to our own Galaxy and its nearest neighbours. ...
Chapter 31 Galaxies & the Universe
Chapter 31 Galaxies & the Universe

... holes that cannot be seen. ...
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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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