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ASTR2100 - Saint Mary's University | Astronomy & Physics
ASTR2100 - Saint Mary's University | Astronomy & Physics

... inertial reference frame for the precessional corrections, the resulting compilation of positions and motions tied to the inertial reference frame is known as a Fundamental Catalogue, e.g. the FK4 and FK5. (vi) Proper motion data for stars in Position Catalogues but not in a Fundamental Catalogue ar ...
Stellar Evolution: the Death of Stars
Stellar Evolution: the Death of Stars

... – Type 1a supernova: explosion of white dwarf in a closed binary system; mass accumulation exceeds the critical mass and ignites the carbon fusion at the core – Type 1b supernova: core collapse of massive star with hydrogen shell lost before – Type 1c supernova: core collapse of massive star with bo ...
btg_2016_astromony
btg_2016_astromony

... The Kulin People, who come from the region around the city of Melbourne, and the Wotjalbaluk People of western Victoria have a creator being named Bunjil the eagle. Bunjil is represented in the sky by the star Altair (Alpha Aquilae) in the constellation Aquila. There are no prizes for guessing that ...
X-rays - Astronomy at Swarthmore College
X-rays - Astronomy at Swarthmore College

... d. The holy grail of science: a measurement that can discriminate between two contradictory theories 2. What we have observed/measured with the new generation of high-resolution x-ray telescopes 3. Our empirical model and fits to the data 4. An answer…and more questions ...
Sep 2012 - Bays Mountain Park
Sep 2012 - Bays Mountain Park

... from Mars’ atmosphere to slow the spacecraft down), MGS ultimately achieved an orbit that ranged from 68 to 280 miles each orbit, circling the planet in 2 hours. It was also placed so that each photographic pass occurred at 2 p.m. local time, resulting in every surface image having the same lighting ...
young science communicator`s competition
young science communicator`s competition

... [This is a highly dramatised version of the Great Debate, held in 1920. Many details have been neglected for brevity and clarity. Directions for the voice actors are shown with square brackets. If possible, sound effects of a crowd cheering and shouting (as directed) should be included. The voice of ...
Stars
Stars

... A blue giant is very bright. Like a light house, they shine across a great distance. Even though blue giant stars are rare, they make up many of the stars we see at night. Blue giant stars die in a spectacular way. They grow larger just like the Sun sized stars, but then instead of shrinking and for ...
the magellanic clouds newsletter - Keele University Astrophysics
the magellanic clouds newsletter - Keele University Astrophysics

... Motivated by recent studies suggesting that the Large Magellanic Cloud (LMC) could be significantly more massive than previously thought, we explore whether the approximation of an inertial Galactocentric reference frame is still valid in the presence of such a massive LMC. We find that previous est ...
DIY Astronomy – Electronic Telescope Focuser
DIY Astronomy – Electronic Telescope Focuser

... Could this possibly be: ...
Astrophysics E1. This question is about stars.
Astrophysics E1. This question is about stars.

... Option E — Astrophysics E1. This question is about the relative population density of stars and galaxies. The number of stars around the Sun, within a distance of 17 ly, is 75. The number of galaxies in the local group, within a distance of 4.0 x 106 ly from the Sun, is 26. (a) Calculate the average ...
The Night Sky
The Night Sky

... Will Comet ISON be the Comet of the Century? There has been much discussion about Comet ISON since its discovery in September 2012 from photos taken with the International Scientific Optical Network (ISON) telescope in Russia. When discovered, this comet was quite bright for its distance from the su ...
Air Cherenkov Methods in Cosmic Rays: A Review
Air Cherenkov Methods in Cosmic Rays: A Review

educator guide - In Saturn`s Rings
educator guide - In Saturn`s Rings

... Using simple numeric processing, this activity gives you a basic understanding of how a digital camera works and how the images from IN SATURN’S RINGS come to life. A digital camera uses a lens to project an image onto a lightsensitive surface in a dark chamber. Its electronic sensor then records th ...
http://www
http://www

... examining their UV spectrum. Actually the spectra of other electromagnetic waves apart from UV are also analyzed, but it is performed by analysing the UV spectra that enables us most effectively to tell the relative composition of different elements in the atmosphere of a particular star. This is h ...
Document
Document

... 6. What do star clusters tell us about the formation of stars? 7. Where in the Galaxy does star formation take place? 8. How can the death of one star trigger the birth of many other stars? ...
Hifz schooling scienc summer vacation task 5th
Hifz schooling scienc summer vacation task 5th

... Q.1 Fill in the blanks. 1. Stars are the burning ball of ____________________. 2. The sun is_____________________ times bigger than the earth. 3. The distance between the sun and earth is ________________________. 4. One would have to run around the earth ______________ times to cover the distance. ...
the printable Observing Olympics Object Info Sheet in pdf
the printable Observing Olympics Object Info Sheet in pdf

Section 1 Notes on Stars
Section 1 Notes on Stars

... 6. What do star clusters tell us about the formation of stars? 7. Where in the Galaxy does star formation take place? 8. How can the death of one star trigger the birth of many other stars? ...
FREE Sample Here - We can offer most test bank and
FREE Sample Here - We can offer most test bank and

... How do astronomers refer to stars and compare their brightness? Astronomers now divide the sky into 88 constellations. Although the constellations originated in Greek and Middle Eastern mythology, the names are Latin. Even the modern constellations, added to fill in the spaces between the ancient fi ...
Our Universe SPA-4101
Our Universe SPA-4101

Evolution of low
Evolution of low

... Evolution of 4Mo Stars • For stars less than 6Mo these last slides describe the evolution pretty well. There are some differences in the details that depend on the initial main-sequence mass. • For stars that start with 4Mo, it gets hot enough in the cores to (1) avoid the helium flash and (2) to ...
FREE Sample Here
FREE Sample Here

... How do astronomers refer to stars and compare their brightness? Astronomers now divide the sky into 88 constellations. Although the constellations originated in Greek and Middle Eastern mythology, the names are Latin. Even the modern constellations, added to fill in the spaces between the ancient fi ...
Document
Document

... 6. What do star clusters tell us about the formation of stars? 7. Where in the Galaxy does star formation take place? 8. How can the death of one star trigger the birth of many other stars? ...
FREE Sample Here
FREE Sample Here

... How do astronomers refer to stars and compare their brightness? Astronomers now divide the sky into 88 constellations. Although the constellations originated in Greek and Middle Eastern mythology, the names are Latin. Even the modern constellations, added to fill in the spaces between the ancient fi ...
Document
Document

...  H-R diagrams are useful because they help astronomers categorize stars into groups:  Main sequence stars, like the Sun, are in a very stable part of their life cycle.  White dwarfs are hot and dim and cannot be seen without a telescope.  Red giants are cool and bright and some can be seen witho ...
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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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