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Extra-Solar Planets
Extra-Solar Planets

... In 1977, NASA did this. They built two Voyager spacecrafts, which flew by Jupiter, Saturn, Uranus, and Neptune. In the 1990’s, these satellites passed the orbit of Pluto, and both will eventually reach nearby stars (in ~ 25,000 years). ...
Standard Set 2 - Atascadero High School
Standard Set 2 - Atascadero High School

... stars in the galaxy. If viewed under a low-powered telescope from a planet in another galaxy, the Milky Way would look like a fuzzy patch of light. If viewed with more powerful telescopes from that far planet, the Milky Way would look like a typical spiral galaxy. One would need to travel at the spe ...
New Stars, New Planets?
New Stars, New Planets?

... beautiful Eagle Nebula is shown in figure 1. The Hubble Space Telescope will surely find many other equally fascinating regions in future years, because after all, at this time we know very little about the detailed structure of space. The complexity of space appears to be designed to get our attent ...
Integrative Studies 410 Our Place in the Universe
Integrative Studies 410 Our Place in the Universe

... The Mass of the Galaxy • Can be determined using Kepler’s 3rd Law – Solar System: the orbital velocities of planets determined by mass of Sun – Galaxy: orbital velocities of stars are determined by total mass of the galaxy contained within that star’s orbit ...
Guide to Deep Space Poster PDF
Guide to Deep Space Poster PDF

... slightly shorter wavelength, moving through the colours to blue and violet the wavelengths get smaller and smaller. Light waves from moving sources are stretched or compressed by the motion. If an object is coming towards you its light is blueshifted meaning the light waves are squeezed together app ...
Goal: To understand life in our universe.
Goal: To understand life in our universe.

... • Lets suppose we sent a craft to the alpha Centauri system at a speed of 0.1 c. • It would take 43 years to get there… • The large distances make interplanetary travel unlikely for a long time – and even then very impractical. ...
Topic 3 Earth in the Universe
Topic 3 Earth in the Universe

... • Coriolis Effect – the tendency of objects moving over the earth (air, water, planes, projectiles) to be deflected (curve away) from a straight line path. The French scientist, Gaspard Coriolis, first explained the deflection of objects moving over the surface due to Earth’s rotation • The deflecti ...
our solar system - Harvard-Smithsonian Center for Astrophysics
our solar system - Harvard-Smithsonian Center for Astrophysics

... Explore the universe by shrinking cosmic scale in 4 steps, zooming out from the realm of the Earth and Moon to the realm of the galaxies. At each step, hold up the image that represents that cosmic object scaled down to 2 inches (about 5 cm) in diameter. Ask a friend to predict the scaled sizes and ...
Slide 1
Slide 1

... A galaxy is a collection of billions of stars, plus gas and dust, held together by gravity. There are billions of galaxies in the universe. ...
PPT - University of Delaware
PPT - University of Delaware

... massive star(s) in our Milky Way Galaxy 10 M_sun Bipolar Nebula enshrouds star(s) from 1840’s “Giant Eruption” Very close so lots of data Data predicts system is actually a binary system with one star ~90 M_sun and the other ~30 M_sun Think it is in last stages of life before big star undergoes a su ...
Theoretical Modeling of Massive Stars Mr. Russell University of Delaware
Theoretical Modeling of Massive Stars Mr. Russell University of Delaware

... massive star(s) in our Milky Way Galaxy 10 M_sun Bipolar Nebula enshrouds star(s) from 1840’s “Giant Eruption” Very close so lots of data Data predicts system is actually a binary system with one star ~90 M_sun and the other ~30 M_sun Think it is in last stages of life before big star undergoes a su ...
Galaxies - schoolphysics
Galaxies - schoolphysics

... rotating very slowly – one complete rotation taking about 240 million years! As the galaxy spins the Sun moves with it at about 235 km/s. Figure 1 ...
Day_39
Day_39

... Most of the extrasolar planets discovered to date are quite massive and have orbits that are very different from planets in our solar system ...
Document
Document

... for the Big Bang is the observed 3 K cosmic background radiation, which is believed to be the remnant of the primordial reball through which the universe made its appearance. In about a million years after the Big Bang, the temperature of this reball decreased from unbelievably high values of more ...
Supplemental Resources - Morehead Planetarium and Science
Supplemental Resources - Morehead Planetarium and Science

... 4d. Explain what we see when we look at the Milky Way. The Milky Way Galaxy is our home in the universe. At night, all the stars we see are part of the Milky Way. On a clear night we can see the band of the Milky Way, the fuzzy light that runs across the sky. This band is made up of gas, dust, and m ...
Stars_Galaxies_Introduction - Etiwanda E
Stars_Galaxies_Introduction - Etiwanda E

... – How is energy produced by the sun? – How are sunspots, prominences, and solar flares related? – Why is our sun considered to be an average star? – How does our sun differ from stars in binary systems? ...
3A8d
3A8d

... of occasional instances of galaxies merging at the present time. In each case explain why the same observations are not as readily understood in the traditional formation/evolution model, which proposed that the formation of galaxies was largely completed in single rapid collapse events more than 10 ...
Temporal and Special Variance of chemical species in the
Temporal and Special Variance of chemical species in the

... which can be addressed by the science question: " What are the proportions and compositions of the major components (e.g., crust, mantle, core, atmosphere/exosphere) of the inner planets? ...
`A ship flying in space:` Earth seen through the eyes of an astronaut
`A ship flying in space:` Earth seen through the eyes of an astronaut

... Planets about the same distance from their parent stars as Earth take roughly a year to complete an orbit. Scientists want to see at least three transits to be able to rule out other explanations for fluctuations in a star’s light, such as small companion stars. Results also are verified by ground a ...
Word doc - UC-HiPACC - University of California, Santa Cruz
Word doc - UC-HiPACC - University of California, Santa Cruz

... of data due to stellar surface activity and/or instrumental errors. Tuomi also developed methods for analyzing the long-term pattern of a star’s barycentric motion to calculate number of possible planets, ...
Where is the Solar System in the Universe?
Where is the Solar System in the Universe?

... – Comets – Space rocks ...
Kepler
Kepler

... The fact that there are two stars instead of one makes it difficult to determine the size of the planet and its distance from its star and therefore whether it is in the habitable zone. ...
Galaxies - Where Science Meets Life
Galaxies - Where Science Meets Life

...  Very little gas or dust.  No recent star formation within galaxy. ...
AN INTRODUCTION TO ASTRONOMY Dr. Uri Griv Department of Physics, Ben-Gurion University
AN INTRODUCTION TO ASTRONOMY Dr. Uri Griv Department of Physics, Ben-Gurion University

... Explanation: Yes it does look like Saturn, but Saturn is only one of four giant ringed planets in our Solar System. And while Saturn has the brightest rings, this system of rings and moons actually belongs to planet Uranus, imaged here in near-infrared light by the Antu telescope at the ESO Paranal ...
ppt
ppt

... was embedded in enormous shell of stars… Emmanuel Kant (1755) suggested instead that the MW is a giant disk of stars. Kant also hypothesized that space was full of other, similar disks of stars (island universes). ...
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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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