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September 2016 News letter - Crawley Astronomical Society
September 2016 News letter - Crawley Astronomical Society

... the equivalent of the old Barn door mounts but very much more refined. With prices of course to match the level of refinement. I decided that the Sky Watcher Astro adventurer would be my best choice. It was stated to have a load capacity of around 7lbs and had a built in polar alignment scope. Align ...
Magnetic field and convection in Betelgeuse
Magnetic field and convection in Betelgeuse

New Suns in the Cosmos?
New Suns in the Cosmos?

... upsurge along the past 15 years, with the discovery of many extra-solar planetary systems, demonstrating that the Sun is not unique as a planet host star. In this context, the main question now is the extent to which the properties of the Sun and its planetary system can be considered as representat ...
Earth in Space - Learning Outcomes
Earth in Space - Learning Outcomes

... is also a lot of information on the major contributors over the centuries to our knowledge of gravitation. A brief historical note on these people follows. Claudius Ptolemy (A.D. 120) assumed the Earth was immovable and tried to explain the strange motion of various stars and planets on that basis. ...
ISP 205: Visions of the Universe
ISP 205: Visions of the Universe

... • Early universe contained only the elements hydrogen and helium. • All other elements were made in stars and recycled into new generations of stars within galaxies. • We are “star stuff” ...
What Comets Are Made
What Comets Are Made

... studied both chunks using NASA’s Infrared Telescope Facility and the Keck II telescope, both on Hawaii’s Mauna Kea. The researchers found that B and C have nearly identical compositions, with the same proportions of substances such as water and carbon dioxide. Those results suggest that comets have ...
asteroids
asteroids

... In fact: can tell the (P,T) at which they  condensed Recall: Except for INERT GASES and some  VOLATILES, chondrites have solar  compositions. ...
Shielding vs. Deshielding
Shielding vs. Deshielding

...  Chemical bonds are anisotropic in space: they ...
The deep OB star population in Carina from the VST Photometric Hα
The deep OB star population in Carina from the VST Photometric Hα

Chapter16.2
Chapter16.2

... temperature rises above 107 K. • Thermal pressure cannot stop contraction because the star is constantly losing thermal energy from its surface through radiation. • Is there another form of pressure that can stop ...
Chandra Observation of Pulsar Wind Nebula
Chandra Observation of Pulsar Wind Nebula

... 12CO ...
Communication with Extraterrestrial Intelligence (CETI)
Communication with Extraterrestrial Intelligence (CETI)

... greater and easier to observe if the star mass is small. What we haven’t found thus far is a planet like the Earth orbiting its star at just the right distance so that its surface temperature might be conducive to permitting liquid water. This just-so region around any star is called the habitable z ...
NuSeti-2015 - Department of Physics and Astronomy
NuSeti-2015 - Department of Physics and Astronomy

... star contracts due to gravity. And the process repeats. ...
PowerPoint file - Departament d`Astronomia i Meteorologia
PowerPoint file - Departament d`Astronomia i Meteorologia

... CO(2-1) emission extends from -8 up to 38 km (the systemic velocity is 11.2 km s-1). The integrated emission for the low-velocities, from 8 to 14 km s-1 reveals two filamentary structures associated with the fan-shape structure found in H2. From the low-velocity map, it is also clear the association ...
Stellar Evolution
Stellar Evolution

... Could there have been an intervening dust cloud? (Then where is it?) Could its companion have been a red giant? (It became a white dwarf very quickly, then!) Astronomy 1-2 ...
AR2013 - Vatican Observatory
AR2013 - Vatican Observatory

... data (just to name a few) with future observational projects with telescopes (such as VATT). Asteroseismology: The Kepler and CoRot missions have provided a wealth of data on pulsating stars (such as sdB stars); using VATT, Brown and Boyle could perform a follow-up survey using the GUFI camera to co ...
All Solid State Laser Source for Tunable Blue and Ultraviolet Radiation.
All Solid State Laser Source for Tunable Blue and Ultraviolet Radiation.

... By observing the frequency spectrum with an optical Fabry–Pérot spectrum analyzer we found that reliable tunable single mode operation could not be achieved because of uncontrolled optical feedback from the beam shaping optics. To get control over the optical elements we have removed the MOPA from ...
Ben R. Oppenheimer1,2 and Sasha Hinkley1,2
Ben R. Oppenheimer1,2 and Sasha Hinkley1,2

ppt
ppt

... Each has associated dark frames May have multiple exposures to co-add DAYCAL are approx. 1 per observation date NIGHTCAL are usually once per science target, but can be common between targets if grating config not changed ...
6.1 Polarization Light is a transverse wave: the electric and magnetic
6.1 Polarization Light is a transverse wave: the electric and magnetic

... Choose three wavelengths that collectively span most of the visible spectrum and record the intensity at the three selected wavelengths. Then rotate the TA by 10( and repeat the measurements. Continue in 10( increments until the intensity is almost zero. Make a table of your data (in MAPLE). Subtrac ...
30-1 - Fremont Peak Observatory Association
30-1 - Fremont Peak Observatory Association

... course of 24 hours Polaris makes a 1° (1 degree) circle around the NCP. It is somewhat difficult to believe, but at the present time, Polaris is more than one Moon width from the NCP. In addition, Polaris is getting closer to the NCP. Polaris will be closest in the year 2102 AD, and at that time it ...
Doppler`s Effect, Gravity and Cosmology
Doppler`s Effect, Gravity and Cosmology

CO emissions from optically selected galaxies at z ∼0.1–0.2: Tight
CO emissions from optically selected galaxies at z ∼0.1–0.2: Tight

... z < 1 has progressed, but there is only a very small number of studies on molecular gas of normal galaxies at this redshift range1 (Geach et al. 2011; Matsui et al. 2012; Bauermeister et al. 2013). The next most abundant molecule after H2 , carbon monoxide (CO), has been widely utilized to measure m ...
2. The Anatomy of Stellar Life and Death
2. The Anatomy of Stellar Life and Death

... Observations by Henrik Beuther (University of Heidelberg) and Peter Schilke (University of Cologne) of a star-forming region IRAS 19410–2336 revealed that the process of massive stars formation appeared to mirror that of lower mass star formation with a very similar scaling of the mass of protostars ...
High Energy Neutrino Astronomy
High Energy Neutrino Astronomy

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Astronomical spectroscopy



Astronomical spectroscopy is the study of astronomy using the techniques of spectroscopy to measure the spectrum of electromagnetic radiation, including visible light, which radiates from stars and other hot celestial objects. Spectroscopy can be used to derive many properties of distant stars and galaxies, such as their chemical composition, temperature, density, mass, distance, luminosity, and relative motion using Doppler shift measurements.
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