• Study Resource
  • Explore Categories
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
Earth Science, 10th edition Chapter 23: Beyond Our Solar System I
Earth Science, 10th edition Chapter 23: Beyond Our Solar System I

... 1. Measuring a star's distance can be very difficult 2. Stellar parallax a. Used for measuring distance to a star b. Apparent shift in a star's position due to the orbital motion of Earth c. Measured as an angle d. Near stars have the largest parallax e. Largest parallax is less than one second of a ...
or view
or view

... diameter (65% of the size of our own Moon). Up to now, its existence has baffled astronomers. Recent observations of these outer regions, however, have shown that there are other similar-sized objects, known collectively as transneptunian objects, in this area of the Solar System. It is possible tha ...
Classifying the Solar System
Classifying the Solar System

... 1. Classify each of the eight planets using these criteria:  Its orbit in relation to Earth  Inferior (between Earth & Sun)  Superior (farther away from the Sun than the Earth).  The make-up of its surface  Rocky (Terrestrial)  Gas (Jovian)  Its size or diameter  Giant (larger than Earth)  ...
The Milky Way Galaxy
The Milky Way Galaxy

... shape. The mass spiral galaxy. distribution within the Galaxy closely • Consists of a barresembles the Sbc shaped core region Hubble . surrounded by a disk of gas, dust and stars. ...
TCI_Paper2_ConditionsForLife
TCI_Paper2_ConditionsForLife

... a given solar system, it has been postulated that there may exist so-called ‘tidally heated habitable zones’ around very large planets. According to researchers at NASA, “tidal dissipation in the satellite of a giant planet may provide sufficient heating to maintain an environment favorable to life” ...
Exoplanets - An ESO/OPTICON/IAU summer school on modern
Exoplanets - An ESO/OPTICON/IAU summer school on modern

... Stars: over 80 Jupiter-masses (hydrogen-fusion and later stages if mass is large enough) Brown dwarfs: between 13-80 Jupiter-masses (only deuterium-fusion) Planetary bodies: below 13 Jupiter-masses (no natural fusion) These mass limits depend slightly on the chemical composition. But: (i) no definit ...
Cosmic Distance Ladder
Cosmic Distance Ladder

... Parallax and distance • Only direct measure of distance astronomers have for objects beyond solar system is parallax – Parallax: apparent motion of nearby stars against background of very distant stars as Earth orbits the Sun – Requires images of the same star at two different times of year separat ...
Kepler - STScI
Kepler - STScI

... • The processes that affect H2-dominated atmosphere gain/escape should be investigated in much more detail • The Kepler-11 system is a natural laboratory to study atmospheric mass loss •Planet types keep emerging that we have no analog for in the solar ...
structure of the universe practice quiz
structure of the universe practice quiz

... • Galaxies with billions upon billions of stars are called ...
Kepler
Kepler

... The scientific objective of the Kepler Mission is to explore the structure and diversity of planetary systems. This is achieved by surveying a large sample of stars to: • Determine the percentage of terrestrial and larger planets there are in or near the habitable zone of a wide variety of stars; • ...
the star
the star

... structure, and little gas or dust. Reddish in color. Very few new stars being born. Elliptical galaxies come in all sizes from just a little larger than globular clusters to 10 times the mass of the Milky Way. The most common kind of galaxy nowadays are the dwarf ellipticals. Gas used up long ago ma ...
globular cluster - Harding University
globular cluster - Harding University

... Determine our Place in the Milky Way Shapley made use of RR Lyra variable stars found in many globular clusters to determine the distances to these clusters.  RR Lyra variables, like the Cepheid variables also have a period – luminosity relationship.  By measuring the distances to, and the relativ ...
Figure 1
Figure 1

...  NGC5253 is a very nearby dwarf Irregular, hosting a central burst of star formation  LEGUS observations at F275W and F336W are joined by ACS/WFC and HRC and WFC3/IR images from different programs  Availability of both Ha (0.6563 mm) and Pb (1.282 mm) emission lines enables accurate foreground du ...
No. 53 - Institute for Astronomy
No. 53 - Institute for Astronomy

... that kept it pointing at a fixed spot in space. Kepler, ...
Exoplanet
Exoplanet

... What we really want is the total number of them, because that tells us how far we might have to search. The Drake equation assigns a symbol for each one of these key factors, representing its probability of occurrence, and multiplies all of them together. It is not something that is actually solved, ...
Chapter 8, Lesson 5, pdf
Chapter 8, Lesson 5, pdf

... • Gravity has caused matter to collect into clumps forming stars and galaxies. • The galaxies continue to move outward. • Evidence for the big bang theory comes from background radiation, radiation that is left over from the beginning moments of the universe and is coming from all directions in spac ...
The Turbulent Birth of Stars and Planets - Max-Planck
The Turbulent Birth of Stars and Planets - Max-Planck

... the intended successor to the Hubble Space Telescope. With its 6.5-meter-mirror, it is set to peer much deeper into space than its predecessor, receiving infrared light from planetary systems-inthe-making, as well as the most distant galaxies. However, due to financial reasons, the project was recen ...
The extragalactic universe and distance measurements
The extragalactic universe and distance measurements

... Milky Way as “detached nebula”, with Sun near center. – Thought that the nebulae could be similar systems – Turns out that his conclusions were heavily effected by dust in the Milky Way – Milky Way is much bigger and better ordered than he ...
Document
Document

... X-ray View of the Galactic Center Galactic center ...
Return both exam and scantron sheet when you
Return both exam and scantron sheet when you

... 12. Planetary nebula is (a) a supernova remnant. (b) a nebula in which planets form around a star. (c) a glowing shell of material ejected by a dying medium-mass star. (d) [None of the above.] 13. Which of these white dwarfs has larger radius? (a) Half a solar mass white dwarf. (b) One solar mass wh ...
Measuring Stellar Distances
Measuring Stellar Distances

... http://homework.uoregon.edu/pub/tycho.html - When you first open the simulator you can see a very small movement of the star but the movement of that star is still confined to one detector element. Actual movement can not be detected until the star moves from one detector element (e.g. a pixel) to t ...
The Life Cycle of Stars Webquest
The Life Cycle of Stars Webquest

... 2. Investigate the process of nuclear fusion explained by Einstein's famous equation E = mc2 and learn how mass in the form of hydrogen atoms is converted to helium and causes a release of energy that makes stars shine. 3. Understand the forces involved in stars that maintain this nuclear reaction a ...
Astronomy Unit 4 Galaxies
Astronomy Unit 4 Galaxies

... 19. To measure the mass of our galaxy, the _____________________ of stars at the _________________________ regions is measured. 20. The speed of stars in the outer parts of the Milky Way are moving ____________ than they should be implying that there is _______________ mass than can be seen in the ...
Objects In Space -- research questions
Objects In Space -- research questions

... 5. Can we see them from Earth? If so, what do they look like? ...
Detection and spectroscopy of exo-planets like Earth J.R.P. Angel
Detection and spectroscopy of exo-planets like Earth J.R.P. Angel

... all transferred to the other output. In this case all the radiation from a neighboring planet at angular separation X12s will appear in full strength while the star is nulled at the same output. This is the principle of the nulling interferometer proposed by Bracewell for planet detection nearly 20 ...
< 1 ... 80 81 82 83 84 85 86 87 88 ... 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.
  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report