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2011 - Astronomy WA
2011 - Astronomy WA

... Cross (constellation of Crux) and Pointers (alpha and beta Centauri). The natural star colour is a highlight of this image, having been preserved over the long exposure. The Coal Sack is clearly visible beside the Southern Cross. Some red nebulosity is also visible throughout the Milky Way. A single ...
The Stars - Department of Physics and Astronomy
The Stars - Department of Physics and Astronomy

... Great Idea: The Sun and other stars use nuclear fusion reactions to convert mass into energy. Eventually, when a star’s nuclear fuel is depleted, the star must ...


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30.2 PowerPoint Stellar Evolution
30.2 PowerPoint Stellar Evolution

... blue super-giant with its ring and bipolar outflow marks the end of the life cycle. ...
the printable Hartness House Workshop Schedule in pdf
the printable Hartness House Workshop Schedule in pdf

... collodion (nitrated cotton dissolved in ether and alcohol) and chemicals on sheets of glass. Wet plate collodion photography was much cheaper than daguerreotypes; the negative/positive process permitted unlimited reproductions. The process was published but not patented. 1851- First daguerreotype of ...
February 2005 - Otterbein University
February 2005 - Otterbein University

... – Galaxies (used to be called nebulae also) ...
“Crossroads of Astronomy.” Talk about Five Remarkable
“Crossroads of Astronomy.” Talk about Five Remarkable

... variable and their periods." Henrietta also realized that "since the variables are probably nearly the same distance from the earth, their periods are apparently associated with their actual emission of light, as determined by their mass, density, and surface brightness." The Cepheids were in the Sm ...
Observing Nebulosities: The Cygnus Superbubble Chris
Observing Nebulosities: The Cygnus Superbubble Chris

... The Cygnus star-forming complex is one of the largest isolated features of interstellar gas and dust recognized in the Milky Way. In the sky, it is associated with the Northern Cross asterism, the bright supergiant star Deneb and the picturesque North America and Pelican emission nebulae (Fig. 1). O ...
Wide-Field Optical Spectrometer (WFOS)
Wide-Field Optical Spectrometer (WFOS)

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Dec 2016 - Astronomical Society of Northern New England
Dec 2016 - Astronomical Society of Northern New England

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Chapter 20
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... Still, many astronomers think that since it is not difficult to form complex molecules, primitive life may well have arisen not only on the Earth but also in other locations. The appearance of very simple organisms in Earth rocks that are 3.5 billion years old, and indirect evidence for life as far ...
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Science 3rd prep. 1st term unit 3 lesson 2 The Solar System Millions

... under the Earth’s surface. - the sunlight is gathered , then separated into a solar spectrum by the spectrometer (( device that shows the different light waves of the sun.)) - Astronomers got most of their information about the sun from the study of its spectra. - a picture of sun is formed in a mon ...
Larger, high-res file, best for printing
Larger, high-res file, best for printing

... shadow of another. That’s not what this event was. Technically, the May event was really a transit, the Moon being too small to completely cover the Sun (which would have been an occultation), and it thus passed across the face of another body, which is the definition of a transit. And as a transit, ...
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... they have after a few million years. When this happens, the outer shell of the star begins to expand. It grows to about triple the size that it currently is. The Blue Supergiant now becomes a Supergiant. Supergiants are orange/yellow and are mostly helium. This is the last stage before it blows up. ...
Charge-Coupled Device (CCD) Detectors
Charge-Coupled Device (CCD) Detectors

... • Recall that the focal ratio of a telescope f/ = [ focal length]/ [diameter] (of primary) • Plate scale P = 206,265 µ / f [arcsec/pixel] where µ : pixel size [in microns] f : focal length of the primary [in mm] e.g., Lulin 1 m, f = 8000 mm ...
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Estimating the Costs of Extremely Large Telescopes

... provided 'point design' for GSMT -- key element of TMT planning supports site testing (northern chile; Baja, CA; Hawaii); serves both theGMT and TMT communities interfaces with ESO to advance technologies of mutual interest has contributed key technical and management leadership within TMT post TMT ...
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Version presented at conference - DCC

... and numerical models predict nova-like transients from double neutron star and black hole/neutron star mergers [2]. GRB afterglows and supernovas are both well-studied phenomenon associated with gravitational radiation [3,4]. While GW and EM signals are expected to travel at the same speed, a common ...
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Weighing a Black Hole
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... region near Sagittarius A, an area in the sky located in the constellation Sagittarius from which there is a lot of radio emission, and which is believed to correspond to the approximate location of the galactic center. This was not easy to do! In order to track the motions of these stars, they obse ...
Ellipses
Ellipses

... celestial body, the more mass it can exert on smaller objects around it. One massive body, acting alone would create a circular orbit. If there’s more than one massive celestial body, the orbiting object will have have an eccentric or elliptical orbit. This has many consequences, not on how we obser ...
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Spitzer Space Telescope



The Spitzer Space Telescope (SST), formerly the Space Infrared Telescope Facility (SIRTF), is an infrared space observatory launched in 2003. It is the fourth and final of the NASA Great Observatories program.The planned mission period was to be 2.5 years with a pre-launch expectation that the mission could extend to five or slightly more years until the onboard liquid helium supply was exhausted. This occurred on 15 May 2009. Without liquid helium to cool the telescope to the very low temperatures needed to operate, most of the instruments are no longer usable. However, the two shortest-wavelength modules of the IRAC camera are still operable with the same sensitivity as before the cryogen was exhausted, and will continue to be used in the Spitzer Warm Mission. All Spitzer data, from both the primary and warm phases, are archived at the Infrared Science Archive (IRSA).In keeping with NASA tradition, the telescope was renamed after its successful demonstration of operation, on 18 December 2003. Unlike most telescopes that are named after famous deceased astronomers by a board of scientists, the new name for SIRTF was obtained from a contest open to the general public.The contest led to the telescope being named in honor of astronomer Lyman Spitzer, who had promoted the concept of space telescopes in the 1940s. Spitzer wrote a 1946 report for RAND Corporation describing the advantages of an extraterrestrial observatory and how it could be realized with available or upcoming technology. He has been cited for his pioneering contributions to rocketry and astronomy, as well as ""his vision and leadership in articulating the advantages and benefits to be realized from the Space Telescope Program.""The US$800 million Spitzer was launched from Cape Canaveral Air Force Station, on a Delta II 7920H ELV rocket, Monday, 25 August 2003 at 13:35:39 UTC-5 (EDT).It follows a heliocentric instead of geocentric orbit, trailing and drifting away from Earth's orbit at approximately 0.1 astronomical unit per year (a so-called ""earth-trailing"" orbit). The primary mirror is 85 centimeters (33 in) in diameter, f/12, made of beryllium and is cooled to 5.5 K (−449.77 °F). The satellite contains three instruments that allow it to perform astronomical imaging and photometry from 3 to 180 micrometers, spectroscopy from 5 to 40 micrometers, and spectrophotometry from 5 to 100 micrometers.
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