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Phys 100 – Astronomy (Dr. Ilias Fernini) Review Questions for
Phys 100 – Astronomy (Dr. Ilias Fernini) Review Questions for

... 13. In science fiction movies, it is common to use a space craft to travel across the Milky Way Galaxy or to assert that we have been visited by alien space craft from the other side of the Milky Way Galaxy. If one has a space craft that can travel at the speed of light, to an observer on the earth, ...
Prime Focus - Tri-City Astronomy Club
Prime Focus - Tri-City Astronomy Club

... orbiting about 370 million miles from its parent star, slightly less than the distance between Jupiter and the sun. The host star, however, is about 70 percent as massive as our sun. "These chance alignments are rare, occurring only about once every 1 million years for a given planet, so it was thou ...
6-Where to Survey - The Challenger Learning Center
6-Where to Survey - The Challenger Learning Center

... If the star is huge, much larger than our sun, a supernova explosion results from the stars death, spreading left over star material back into space and possibly leaving a black hole. If a black hole is not produced by a supermassive star’s death, a pulsar may result where the star use to reside. T ...
Preparing astronomical observations and observing with OHP facilities
Preparing astronomical observations and observing with OHP facilities

... general knowledge of what is going to be observed and of the instruments used. A guideline is given to prepare an observing program and to follow it as efficiently as possible. Finally, some examples are given of observations to be made by ERCA participants at OHP observatory. ...
Chapter 2
Chapter 2

... observations, they were the first to use a careful and systematic manner to explain the workings of the heavens • Limited to naked-eye observations, their idea of using logic and mathematics as tools for investigating nature is still with us today • Their investigative methodology is in many ways as ...
Astronomy Notes: Deep Space
Astronomy Notes: Deep Space

Optical Discussion Summary
Optical Discussion Summary

... Teaching and postgraduate training is an essential role for these universityoperated ‘small’ telescope facilities. However, they also have a vital role as test-beds for instrument development and innovation, new technology, and thereby maintaining Australia’s expertise and training in instrumentatio ...
Picture 1 present an negative image of sky taken by ccd camera
Picture 1 present an negative image of sky taken by ccd camera

... Picture 3 presents a sky chart which includes the region shown in the CCD images. The stars in the images are far away and should ideally be seen as point sources. However, diffraction on the telescope aperture and the effects of atmospheric turbulence (known as 'seeing') blur the light from the sta ...
Earth in Space and Time: SC.5.E.5.1
Earth in Space and Time: SC.5.E.5.1

... 5) Latoya is studying the stars and she learns that Barnard's star is the third closest star to Earth, although it cannot be seen without a telescope. She also knows that the brightest star in the night sky, Sirius, is much farther away but can be seen by the naked eye. ...
File
File

... final detonation. Everything that they wished to preserve, all the fruit of their genius, they brought here to this distant world in the days before the end, hoping that some other race would find it and that they would not be utterly forgotten. Would we have done as well, or would we have been too ...
Chapter 24 Section 2 pwrpnt
Chapter 24 Section 2 pwrpnt

... This 2.4 meter space telescope has 10 billion times more light gathering power than the human eye. Hubble has given us many spectacular images and provided us with data about black holes, births of stars, planets orbiting other stars and the age of the universe. ...
FLIGHT International, 7 March 1963 347 satellite camera are stored
FLIGHT International, 7 March 1963 347 satellite camera are stored

... on a quartz clock and, from this time and the position of the stars on the plate, the precise direction of the camera axis can be obtained. With this camera, it is possible to measure satellite positions to an accuracy of lsec of arc (equivalent to about 1ft in 40 miles). To obtain this precision, t ...
Progress in the Australian Virtual Observatory
Progress in the Australian Virtual Observatory

... Data reduction pipelines for: – Molonglo Observatory Synthesis Telescope – AT Compact Array archive – Gemini, for Australian-used instruments Portal for theoretical astrophysics jobs: – configuration and execution ...
Telescopes
Telescopes

... mirror (primary mirror) to collect the light and reflect it to a focus. Because the mirror reflected light back into the tube, he had to use a small, flat mirror (secondary mirror) in the focal path of the primary mirror to deflect the image out through the side of the tube, to the eyepiece; otherwi ...
U7 Review WS KEY
U7 Review WS KEY

... b. cosmic background radiation d. abundance of light elements (H, He and Li)  The first elements that were formed in the universe were? a. hydrogen and lithium c. hydrogen and helium b. lithium and helium d. lithium and beryllium 10. I can describe tools and models used by scientists to predict the ...
Beyond our Sol. System
Beyond our Sol. System

... wavelengths of light that they give off. Mrs. Degl ...
Full Press Release - The Open University
Full Press Release - The Open University

... stars in the dense gas itself, and emits infrared light. The formation of a new generation of stars is now taking place within this compressed gas in these outer shell structures. The AKARI data reveals for the first time, the detailed distribution of this swept out gas and dust over the entire nebu ...
Meade® 8" and 10" LX200GPS Schmidt
Meade® 8" and 10" LX200GPS Schmidt

... Positioning System (GPS), a satellite system that enables extremely precise communication to the telescope of the observer’s latitude and longitude, as well as local time. Integrated true-level and North electronic sensors in combination with a 16-channel GPS receiver located in the “…Viewing a 2nd- ...
Light and Telescopes - Otterbein University
Light and Telescopes - Otterbein University

... • Meditations on first Philosophy (1641) [6 Meditations: Of the Things that we may doubt; Of the Nature of the Human Mind; Of God: that He exists; Of Truth and Error; Of the Essence of Material Things; Of the Existence of Material Things; Of the Real Distinction between the Mind and the Body of Man] ...
Lectures 10 & 11 powerpoint (stellar formation) [movie below]
Lectures 10 & 11 powerpoint (stellar formation) [movie below]

... • Hot intercloud medium: Hot (T ~ a few 1000 K), ionized hydrogen (HII); low density (n ~ 0.1 atom/cm3); gas can remain ionized because of very low density. ...
The Sky
The Sky

... Formal Labs about every other week. Weeks without Lab we will assign small Observing projects. • Record ALL observations in an Observing Notebook. • 2 one-hour in-class exams. • One final. ...
PHYS 175 Fall 2014 Final Recitation Ch. 16 The Sun
PHYS 175 Fall 2014 Final Recitation Ch. 16 The Sun

... Photons released in the core (where fusion takes place) collide almost instantaneously with other core constituents. This energy gradually flows outward, until the density of the sun decreases sufficiently to allow for radiative diffusion of the energy. Again, the photons still undergo many collisio ...
Telescopes – How They work – Basics
Telescopes – How They work – Basics

... Telescopes – How They work – Basics Lets start with a lens – the heart of a telescope A lens can focus light: ...
Stars
Stars

... star, but you see the Doppler shift (lecture 2B) due to its orbital motion. – Double-line – see lines from both stars – Single-line – see only one set of lines ...
Time From the Perspective of a Particle Physicist
Time From the Perspective of a Particle Physicist

... are remnants from the first few minutes after the Big Bang • To explore back to earlier times we use our understanding of physics • The earlier you go in time the hotter was the Universe. Particle accelerators can ...
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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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