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guide to orion 3-d flythrough
guide to orion 3-d flythrough

... The central area of the nebula is called the Trapezium cluster. It is dominated by four young, massive stars in a kite-like arrangement. The brightest of these stars, which has a luminosity 100,000 times that of the Sun, provides the energy that creates the nebula as we see it. It produces a flood o ...
SPECIAL REPORT
SPECIAL REPORT

... planned Giant Segmented Mirror Telescope will work with space-based instruments like NASA’s Spitzer, Kepler, and the future SIM PlanetQuest and James Webb telescopes. These studies will provide the observational tests needed to determine whether theoreticians’ amusements have a place in the real uni ...
36x48 vertical poster template
36x48 vertical poster template

... The Hubble Space Telescope was transitioned to gyro mode on August 28, 2005 in order to conserve the lifetime of the gyroscopes. Testing has shown that observations taken in 2 gyro mode are essentially indistinguishable from 3 gyro mode. HST was originally designed to use three rate-sensing gyros to ...
Chapter 9
Chapter 9

... What type of galaxy is shown below? ...
Chapter 9
Chapter 9

... What type of galaxy is shown below? ...
Stars Of Orion Essay Research Paper 01
Stars Of Orion Essay Research Paper 01

Exploring the Outer Solar System Jane Luu When I was
Exploring the Outer Solar System Jane Luu When I was

... away from their homeland started as early as the year 800, while the rest of Europe was still in the Medieval Ages. They established commerce between Scandinavia and the rest of Europe, they settled Iceland and Greenland, crossing the ocean in modest open boats called “knarr.” We have all heard of L ...
strolympics - Chandra X
strolympics - Chandra X

... Olympics, where the difference between gold and silver can be a fraction of a second. However, everyday technologies like GPS require even more precision. Time and our ability to measure it accurately is also key for many frontiers of science, including astrophysics. The Chandra X-ray Observatory ha ...
Unit 8 Chapter 30
Unit 8 Chapter 30

... The Milky Way galaxy is a spiral galaxy in which the sun is one of hundreds of billions of stars. Each star orbits around the center of the Milky Way galaxy. It takes the sun about 225 million years to complete one orbit around the galaxy. ...
the lives of stars
the lives of stars

... star, has been a main sequence star for about 5 billion years. It will continue to shine without changing for about 5 billion more years. Really large stars burn through their supply of hydrogen very quickly, so they ‘live fast and die young’! These very large stars may only be on the main sequence ...
Timeline, Topics, and Resources for iMovie Projects
Timeline, Topics, and Resources for iMovie Projects

... work when it was available. This was not until 1543, the year Copernicus died. As Copernicus' new picture of the universe became more widely known, misgivings arose. The universe had after all been created for mankind, so why wasn't mankind at the center? An intellectual revolutionary called Giorda ...
Issue 104
Issue 104

... Article of the Month—Seeing Straight by John Gifford Aligning the elements of a telescope system, how and why. From where we stand the sky appears to make one full turn around the Earth every day. The fact that what we see is really the Earth turning beneath the sky makes no difference to how it loo ...
Search for Life in the Universe
Search for Life in the Universe

... – Extrasolar planets around main sequence stars discovered in 1995 – Planets around neutron stars discovered previously – Spectroscopy (>100 cases): detect Doppler shift of stellar motion around center of mass – Astrometry (1 case): detect angular motion ...
An approach to ground based space surveillance
An approach to ground based space surveillance

... extend the life of orbiting satellites by fuel replenishment, repair, inspection, orbital maintenance or satellite repurposing, and possibly reduce the rate of space debris generation. OOS performed in geostationary orbit poses a unique challenge for the optical space surveillance community. Both sa ...
Radio and Optical observations of magnetospheres of outer planets
Radio and Optical observations of magnetospheres of outer planets

... Charged particles with relativistic energy are trapped in the dipole magnetic field. In Jupiter, due to the strong magnetic field and large amount of trapped electrons, strong synchrotron radiation is emitted: Jupiter's synchrotron radiation (JSR) ...
SASS_Talk_4_16_08
SASS_Talk_4_16_08

... I will try to motivate you with two scenarios 1) You accidentally black out at a party and wake up in a field somewhere*. You want to know where you are**, what time it is***, and figure out which way east is 2) You hear there is a comet that just became very bright in the sky and you want to know w ...
slides - Indico
slides - Indico

... The Sloan Digital Sky Survey • The most ambitious astronomy project ever undertaken – Obtain accurately calibrated imaging of 10,000 square degrees of (northern) sky, in five filters (ugriz) – Obtain medium-resolution spectroscopy for • 1,000,000 galaxies ...
The Milky Way - 清華大學物理系歡迎頁 Welcome to
The Milky Way - 清華大學物理系歡迎頁 Welcome to

... Stars form from the interstellar medium and reach stability fusing hydrogen in their cores. This chapter is about the long, stable middle age of stars on the main sequence and their old age as they swell to become giant stars. Here you will answer three ...
Lecture 1 - Simon P Driver
Lecture 1 - Simon P Driver

... –  Calculate  how  many  days  your  birthday  is  awer  21st  March  =  N     –  Add  12h+24hxN/365.25    =  Q    Because  the  sky  completes  one  rota/on  during  the  course   of  one  year.   –  Calculate  how  many  hours   ...
S LAR SYSTEM - Fleet Science Center
S LAR SYSTEM - Fleet Science Center

... some objects fall slower than expected. For instance, a feather or a piece of paper has little mass and a large surface area, so air resistance has a bigger influence on these objects. The Moon has no atmosphere, so gravity is the only force that acts on dropped objects. All of your objects would fa ...
4. Massive Stars and HII Regions
4. Massive Stars and HII Regions

... if rare in numbers, have a profound impact on their environment. They are the fundamental producers of heavy elements, generate huge amounts of high energy radiation, trigger star formation. Their lifetime on the main sequence is rather short: ...
Galileo
Galileo

... 1. Calculate the time for one of the moons to go around Jupiter? 2. How far away each moon is from Jupiter? (the diameter of its orbit?) Is there a relationship (equation?) between the diameter and the orbiting time More questions…???? …. interpretations/extensions from the “measurements” ...
Refuges for Life in a - University of Arizona
Refuges for Life in a - University of Arizona

StarFlight - Center for the Presentation of Science
StarFlight - Center for the Presentation of Science

... We designed a front-end evaluation to determine popular knowledge of two astronomical subjects: (1) the Solar System, and (2) common constellations. The form of the evaluation was an open-ended discussion where we asked people to draw the Solar System and any constellations they could remember, and ...
Science and the Universe
Science and the Universe

... • Stars in a number of places form clusters, each containing up to hundreds of thousands of stars and taking up a volume of space hundreds of light years across • Stars have a long, but not infinite, life (billions of years) – They die or collapse in spectacular ways 11 Jan 2005 ...
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International Ultraviolet Explorer



The International Ultraviolet Explorer (IUE) was an astronomical observatory satellite primarily designed to take ultraviolet spectra. The satellite was a collaborative project between NASA, the UK Science Research Council and the European Space Agency (ESA). The mission was first proposed in early 1964, by a group of scientists in the United Kingdom, and was launched on January 26, 1978 aboard a NASA Delta rocket. The mission lifetime was initially set for 3 years, but in the end it lasted almost 18 years, with the satellite being shut down in 1996. The switch-off occurred for financial reasons, while the telescope was still functioning at near original efficiency.It was the first space observatory to be operated in real time by astronomers who visited the groundstations in the United States and Europe. Astronomers made over 104,000 observations using the IUE, of objects ranging from solar system bodies to distant quasars. Among the significant scientific results from IUE data were the first large scale studies of stellar winds, accurate measurements of the way interstellar dust absorbs light, and measurements of the supernova SN1987A which showed that it defied stellar evolution theories as they then stood. When the mission ended, it was considered the most successful astronomical satellite ever.
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