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Binary Orbits
Binary Orbits

... • Different kinds of binary systems – both normal stars – one may be a neutron star – test theories of stellar evolution • Mass transfer possible if stars are in close proximity – accretion- affects evolution of the stars • Accretion may dramatically change evolution of the star e.g. formation of bi ...
Answers - Physics@Brock
Answers - Physics@Brock

... 12. The universe is believed to have an age of about (a) 14 thousand years. (b) 14 million years. (c) * 14 billion years. (d) 14 trillion years. 13. The planets change their positions relative to the stars because (a) of the rotation of the Earth. (b) of the Sun’s motion along the ecliptic. (c) of t ...
Astronomical spectroscopy
Astronomical spectroscopy

... which the beam passes through the surface. When following the optical path of the beam through an optical system, E is constant, in particular, it cannot be reduced For a telescope, E is the product of the primary mirror surface and the two-dimensional field (in sterad) transmitted by the optical sy ...
Types of Stars http://space.about.com/od/stars/tp/What-Are
Types of Stars http://space.about.com/od/stars/tp/What-Are

... star is a system of two stars that are gravitationally bound to each other. They orbit around a common point, called the center of mass. It is estimated that about half of all the stars in our galaxy are part of a binary system. Visual binaries can be seen as two separate stars through a telescope. ...
The World-Wide Telescope, an Archetype for Online
The World-Wide Telescope, an Archetype for Online

... that give exact answers, these algorithms will likely be heuristic and give approximate answers [Connolly, Szapudi]. Astronomy as an Archetype for Online Science Astronomy exemplifies these phenomena. For thousands of years astronomy was primary empirical with few theoretical models. Theoretical ast ...
February 2013 - astronomy for beginners
February 2013 - astronomy for beginners

... brightest stars are called Pollux (β) and Castor (α) and are known as the Gemini Twins. The twins originated in a Greek myth which told that they had one mother but two fathers. Castor was the mortal son of King Tyndareus but Pollux was the immortal son of the God Zeus who had disguised himself as C ...
MSci Astrophysics 210PHY412 - Queen's University Belfast
MSci Astrophysics 210PHY412 - Queen's University Belfast

... paucity of very bright stars on the AGB. The latter (Prialnik P. 161) comes from the number of AGB stars expected compared to observed is >10. Hence a process prevents them completing their movement up the AGB, while losing mass at the Reimer’s rate. This is a superwind which removes the envelope ma ...
File
File

... proportional to distance ...
L10 - QUB Astrophysics Research Centre
L10 - QUB Astrophysics Research Centre

... paucity of very bright stars on the AGB. The latter (Prialnik P. 161) comes from the number of AGB stars expected compared to observed is >10. Hence a process prevents them completing their movement up the AGB, while losing mass at the Reimer’s rate. This is a superwind which removes the envelope ma ...
Light and Spectroscopy Concept Inventory
Light and Spectroscopy Concept Inventory

... All three objects have the same temperature. The relative temperatures of these objects cannot be determined from this information. ...
Astro 210 Lecture 4 Sept. 4, 2013 Announcements: • PS 1 available
Astro 210 Lecture 4 Sept. 4, 2013 Announcements: • PS 1 available

... ⊲ apologies for technical difficulties! ⊲ blackbody radiation Q: what’s a blackbody? what objects emit BB radiation? Q: what sets surface flux from a BB? Q: how is BB color related to temperature? ...
ArAS News - Armenian Astronomical Society
ArAS News - Armenian Astronomical Society

... "The Physics of the ISM: 6 years of ISM-SPP 1573: What have we learned?" conference took place in the University of Cologne, Germany, from 12-17 February, 2017. It was organized by the DFG priority program 1573 for the interstellar medium (ISM-SPP) jointly with the I. Physics Institute of the Univer ...
The Ursa Major Moving Cluster, Collinder 285
The Ursa Major Moving Cluster, Collinder 285

... Most of the stars making up the Big Dipper show a common proper motion, as R.A. Proctor has found as early as 1869 (see e.g. Burnham). When W. Huggins, in 1872, determined their radial velocities from their spectra, it became apparent that they move approximately in the same spatial direction, and t ...
Comets - Cloudfront.net
Comets - Cloudfront.net

... years and predicted its reappearance in 1758 It has been recorded as early as 240 BCE, and as recently as 1986 when a probe imaged its nucleus ...
AV_Paper1_TheAgeOfTheUniverse
AV_Paper1_TheAgeOfTheUniverse

... measurement read: kilometers/second/megaparsec, meaning for every megaparsec (3 million light years) you go out the universe is expanding 550km/sec faster. This parameter approximated the age of the universe to be around 1.8 billion years which conflicted with geological claims of the day that had E ...
The World`s Easiest Equatorial Mount Instruction Manual
The World`s Easiest Equatorial Mount Instruction Manual

Grzegorz F
Grzegorz F

... small, and the light did not have the nature of the wave and did not result in the phenomenon of diffraction at the edges of the diaphragm. - Real, because the image cast on the screen is made up by the actual light rays coming from the observed object. - Inverted, because the ray of the upper part ...
11 Stellar Remnants - Journigan-wiki
11 Stellar Remnants - Journigan-wiki

... The actual matter is passed through a mass transfer stream. Where this stream passes from the meeting Roche Lobes is called the LaGrange Point. The LaGrange Point is a point of gravitational neutrality where the influence of each star counteracts the gravitational force of its companion. To pass the ...
Stars 3
Stars 3

... energetic electrons as they spiral through the Crab’s magnetic field -- is powered by the Crab Pulsar. The picture on the right shows a Hubble Space Telescope image of the inner parts of the Crab. The pulsar itself is visible as the left of the pair of stars near the center of the frame. Surrounding ...
Astronomy Assignment #1
Astronomy Assignment #1

... Sketch the apparent motion of the stars, following the example in class, looking in the four cardinal directions (N, E, S & W) for the following four locations: The North Pole (90 N), Syracuse, NY (43 N), The Equator (0 N), Punta Arenas, Chile (53 S). Include all relevant timescales (time for st ...
Astronomy 100  Name(s):
Astronomy 100 Name(s):

... lab is designed to help you understand how the software works and what its capabilities are. Obtain a laptop computer from the cart (remember to leave the AC adapter in the cart), turn on the computer and, once the Windows desktop is displayed, click on “the Sky” icon along the bottom row or else th ...
Introduction to Astronomy
Introduction to Astronomy

... – Bringing mass closer to the axis of rotation makes the rotation speed increase – Same principle during formation of solar system from slowly rotating IS cloud – If Sun shrank down to 10 km: ...
PHYS_3380_100714_bw - The University of Texas at Dallas
PHYS_3380_100714_bw - The University of Texas at Dallas

... Special detectors/receivers record light invisible to the human eye - gamma rays, x-rays, ultraviolet, infrared, radio waves. - each type of light can provide information not available from other types. Digital images are reconstructed using false-color coding so that we can see this light. ...
Apparent Magnitude
Apparent Magnitude

... of mass. For each star, the other is its companion star. A large percentage of stars are part of systems with at least two stars. Binary star systems are very important in astrophysics, because observing their mutual orbits allows their mass to be determined. The masses of many single stars can then ...
Part 3
Part 3

... Yunnan Astronomical Observatory April, 2010 Beijing ...
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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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