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Something Big Out There - binaryresearchinstitute.com
Something Big Out There - binaryresearchinstitute.com

... km in diameter found to be orbiting our sun in a pattern quite similar to Sedna, one of the largest dwarfs, discovered in 2002. Mike Brown, an astrophysicist at Caltech, famed for killing Pluto by his discovery of so many of these minor planets, was the first to note that Sedna cannot exist in its c ...
Astronomy Galaxies & The Universe
Astronomy Galaxies & The Universe

... uses data from lots of stars, so there are lots of dots. The position of each dot on the diagram corresponds to the star's luminosity and its temperature  The vertical position represents the star's luminosity (absolute magnitude).  The horizontal position represents the star's surface temperature ...
23.1 Telescopes - Ms. Billings Website
23.1 Telescopes - Ms. Billings Website

... Some very hot stars emit light primarily at ultraviolet (UV) wavelengths, while some very cool stars emit mostly in the infrared. There are extremely hot objects that emit X-rays and even gamma rays. Light from some of the faintest, most distant objects is in the form of radio waves. In fact, a lot ...
Word doc - UC
Word doc - UC

... quantified the fraction of planets that might have been missed by their census, either because the planes of their orbits were tilted so the planets could not transit the host star as seen from Earth, or those that the TERRA software itself could have missed. Shedding (the right amount of) light The ...
Lecture 13
Lecture 13

... Stellar Temperatures, from spectra Can match full stellar spectrum to a 'best fit' blackbody. ­ eg: Sun's spectrum (red)  Inverse wavelength (cm­1) Sometimes, this fitting is complicated by the many spectral lines present. ­ so a 'best' match is   a bit of an art... ­ stars are not perfect  blackbo ...
Earth in the Universe
Earth in the Universe

... much different paths of evolution. • Exist as a main sequence for a much shorter time, about 100 million years. • These stars still turn into super giants. • They then undergo a supernova and quickly collapse forming a center that is so dense only neutrons can exist (neutron star) • Even larger star ...
Another Earth in the Universe
Another Earth in the Universe

... large stars and therefore are the best candidates for planetary systems in which life could be present. In fact, for biological evolution and for biochemical reactions to take place, very long periods of time are required, longer than the average age of the large stars. Furthermore, M dwarfs are ver ...
Astronomy
Astronomy

... Something that is achieved when the inward force of gravity is balanced by the outward pressure from fusion and radiation inside a star ...
Gaia Fact Sheet
Gaia Fact Sheet

... The payload consists of three instruments sharing the same telescope, optical bench and focal plane: • The astrometric instrument will measure the angular position of stars • The photometric instrument will provide continuous star spectra in the band 330 nm to 1000 nm • The spectrometric instrume ...
Mar - Wadhurst Astronomical Society
Mar - Wadhurst Astronomical Society

... come from Mars and was thought to have contained a microscopic bacteriological type structure but this was later discounted. Yet missions to Mars have discovered evidence in rocks that water may once have been present, so life may have been present a long time ago. Jan talked about other possible pl ...
File
File

... own axis 365.26 times per each orbit around the sun, which gives us 365 days in each year. In turn, the moon orbits the earth, affecting the ocean tides, and slowing the Earth’s rotation with its gravity. The Earth and its solar system are part of a bigger area of space called the Milky Way galaxy. ...
The activities of the Astronomical Institute of the Slovak Academy of
The activities of the Astronomical Institute of the Slovak Academy of

... The activities of the Astronomical Institute of the Slovak Academy of Sciences (AISAS), Tatranská Lomnica (http://www.astro.sk), related to COSPAR, were devoted to the research in solar and stellar physics using different satellite observations, mainly in the UV, XUV and X-ray spectral regions. Main ...
Chapter 01
Chapter 01

... between objects—which are big, which are small, and which are contained inside others. In other words, this chapter will give us perspective for all of our exploration to follow. It is easy to learn a few facts, but it is the relationships between facts that are interesting. The relationships illust ...
The Milky Way - Department of Physics
The Milky Way - Department of Physics

... between objects—which are big, which are small, and which are contained inside others. In other words, this chapter will give us perspective for all of our exploration to follow. It is easy to learn a few facts, but it is the relationships between facts that are interesting. The relationships illust ...
Lifetimes of stars
Lifetimes of stars

... Stellar Lifetimes • The Sun (and all stars) will eventually run out of fuel (hydrogen in regions where it is hot enough for fusion). • If all the hydrogen in the Sun could fuse to helium, the Sun’s lifetime would be 100 billion years. • But, by the time about 10% of the Sun’s H has been converted in ...
UNIT 4 - Rowan County Schools
UNIT 4 - Rowan County Schools

... The Crab Nebula (M1) • The crab nebula is a supernova remnant (SNR) • A SNR is the expanding shell of gas that is ejected into space after a massive star reaches the end of it’s life and explodes. • The Crab nebula exploded in 1054 AD. It was observed by the Chinese and Arabs and was known to the C ...
Lifecycle of Stars - Mrs. Plante Science
Lifecycle of Stars - Mrs. Plante Science

... forming larger and larger balls of gas and dust molecules. • When the mass becomes large enough, gravitational contraction results in high pressure and temperature, and a protostar is formed. ...
The measure of Cosmological distances
The measure of Cosmological distances

... Found new planet (Uranus)Discover Infra-Red lightFirst map of the sky: Idea: All the stars are the same. Therefore, bright stars are closer. ...
Two Small Pieces of Glass: The Amazing Telescope
Two Small Pieces of Glass: The Amazing Telescope

... Objects can be seen if light is available to illuminate them or if they give off their own light. (By end of grade 2). Some materials allow light to pass through them, others allow only some light through and others block all the light and create a dark shadow on any surface beyond them, where the l ...
Scale of the Cosmos ppt.
Scale of the Cosmos ppt.

... distance (even at a speed of 186,000 mi/s)  It takes 8 minutes for the sunlight to reach earth.  So…. The light we see from a star that is 1500 ly away, left that star 1500 years ...
Have a Safe and Happy Holiday
Have a Safe and Happy Holiday

... ...
Blaise Pascal Tine - Clarkson University
Blaise Pascal Tine - Clarkson University

... The automation of the telescope is done by adding stepper motor to the rotational axis of the motors. There are 2 rotational axes:  The RA axis (East/West movement). (See Fig 2)  The DEC axis (North/South movement). (See Fig 1) The telescope possesses a RA drive corrector motor that is used to adj ...
Unit I – The Size, Shape and Motion of the Earth
Unit I – The Size, Shape and Motion of the Earth

... stars in its vicinity, not just this one!) at a speed of ~30 km/sec; and six months later we are moving the opposite direction! Of course it is because we are orbiting the Sun. ...
Historical Astronomers - Clayton State University
Historical Astronomers - Clayton State University

... 4. He also found imperfections on the supposedly perfect body of the Sun. He discovered sunspots, and found that the Sun rotated, like an ordinary, material object. 5. He resolved the Milky Way into a multitude of stars, showing that stars were more distant than had been imagined, and that some of t ...
here - British Astronomical Association
here - British Astronomical Association

... due to an exchange of material from one star to the other, often via an “accretion disc”. • One of the most interesting areas of observing ...
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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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