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Boy Scout Astronomy Merit Badge Workbook
Boy Scout Astronomy Merit Badge Workbook

3.1 Using Technology
3.1 Using Technology

... appears as blue, X-ray data from Chandra is coded red, and infrared data from the Spitzer Space Telescope appears green. The anomalous arms appear as purple and blue emission. ...
Life Cycle of a Star Vocabulary
Life Cycle of a Star Vocabulary

... nuclear fuel, some of its mass flows into its core. • Core becomes so heavy that it cannot withstand its own ...
Supercomputer simulation provides missing link between turbulence, hypernovae and gamma-ray bursts
Supercomputer simulation provides missing link between turbulence, hypernovae and gamma-ray bursts

... “The breakthrough here is that Philipp’s team starts from a relatively weak magnetic field and shows it building up to be a very strong and large-scale coherent magnetic field of the kind that is usually assumed to be there when people make models of gamma-ray bursts,” Quataert said. Brightest even ...
The Sun Worksheet
The Sun Worksheet

... 23. What is the name of the result of solar wind particles entering the Earth’s upper atmosphere and releasing energy to produce patterns of glowing light in the sky? ...
Measuring Distances - Stockton University
Measuring Distances - Stockton University

... galaxy approaching them and part of the galaxy running away. This causes the emission from the galaxy to show redshifted, blueshifted, and no-shifted emission. The motion will thus cause a narrow line, e.g., a line due to some element like hydrogen, to be smeared out and to appear broad to the exter ...
Astro 10B Study Questions for Each Chapter
Astro 10B Study Questions for Each Chapter

Astronomy
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... • research and describe the use of astronomy in ancient civilizations such as the Egyptians, Mayans, Aztecs, Europeans, and the native Americans.[4A] • research and describe the contributions of scientists to our changing understanding of astronomy, including Ptolemy, Copernicus, Tycho Brahe, Kepler ...
Using Photometric Data to Derive an HR Diagram
Using Photometric Data to Derive an HR Diagram

... That’s where STAR CLUSTERS come in! All the stars in a cluster are at the same distance from us (neglecting the depth of the cluster itself, which is tiny compared with its overall distance from us). All the stars in a cluster are the same absolute age, although at different stages of evolution, dep ...
Lecture - UMass Amherst
Lecture - UMass Amherst

... 1.  The Sun would hold 1.3 million Earths. i.e. the radius of the Sun is about 100 times that of the Earth. 2. There are ~100 billion "Suns" in a galaxy like our ...
Nonfiction Text Feature
Nonfiction Text Feature

... How Does the Text Feature Help You as a Reader? Special types in a nonfiction text, help to expand our vocabulary by using context clues or the glossary to define the word. According to the text, galaxies are huge swarms of stars in space. This is an important vocabulary word in the text because the ...
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Winter 2014
Winter 2014

... brightest, Betelgeuse, has a reddish cast. Betelgeuse is a red supergiant and glows orange-red because its surface is actually cooler than the surfaces of most other stars we see in the night sky. Having exhausted the hydrogen fuel in its core, someday Betelgeuse will explode in a brilliant supernov ...
Slide 1 - Typepad
Slide 1 - Typepad

... the three with an apparent magnitude +5.6. M36 - 60 stars with an angular width of 12 arcminutes.M38 100stars and is the dimmest of the three at magnitude+6.4. All three of these clusters, 4000 light-years away, can be seen with a small telescope. Courtesy - Dave Garner teaches astronomy at Conestog ...
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... 1-Multiple Choice: 1. Which tool measures wind direction? A. ...
Photons
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... value of S λ . For the sake of comparison, the bottom panel presents the spectra of Vega (A0V), the Sun (G2V), and a M5 giant, in arbitrary scales of Fλ . ...
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Why are Binary Stars so Important for the Theory

... modern model-simulation method by Wood. The two independent methods give consistent results and the radii of the two components are determined better than 1 %. The surface gravities are then also known very precisely (2 %). The temperature difference is small and weil defined. 80th of the components ...
Characteristics of Main Sequence Stars
Characteristics of Main Sequence Stars

... nuclear reactions in high mass stars are generally confined to a very small region, much smaller than the size of the convective core. • As the stellar mass increases, so does the size of the convective core (due again to the large increase in ² with temperature). Supermassive stars with M ∼ 100M¯ w ...
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... Earth determines which constellations remain below the horizon. (They depend on time of year because Earth’s orbit changes the apparent location of the Sun among the stars.) ...
HR4AGN Powerpoint Presentation-a
HR4AGN Powerpoint Presentation-a

... • So we want a color magnitude diagram for AGN so that by looking at the color of an AGN we can get its luminosity – But AGN have no fusion, why would we expect a color-magnitude relation? – The gas that accretes onto the black hole is still hot and so must follow the Blackbody Radiation law. ...
1 Do Massive Stars Trigger New Waves of Star Formation
1 Do Massive Stars Trigger New Waves of Star Formation

... I. Proposed Research Stars form in the universe. We know this because we can see thousands of stars in the night sky, and we also orbit the most famous star, our Sun. However, the mechanisms that lead to their formation are still very much unknown. Astronomers also now believe that stars were the fi ...
The Ever-Changing Sky
The Ever-Changing Sky

... Sun. B. The stars near the Sun are all too dim to be seen by either our eyes or the telescopes. C. The Sun is too bright compared with distant stars. If we block Sun light, then we can see the stars---this is true only in space. D. The sky during the day is much brighter than the stars.  Back to Pr ...
First firm spectral classification of an early-B PMS star
First firm spectral classification of an early-B PMS star

... massive nearby star-forming regions in the Galaxy (Hoffmeister et al. 2008; Broos et al. 2007; Povich et al. 2009). For the “normal” OB stars Hanson et al. (1997) found a good correspondence between the optical and K -band spectra, but the massive YSO optical spectra remained inconclusive. For four ...
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Corvus (constellation)



Corvus is a small constellation in the Southern Celestial Hemisphere. Its name comes from the Latin word ""raven"" or ""crow"". It includes only 11 stars with brighter than 4.02 magnitudes. One of the 48 constellations listed by the 2nd-century astronomer Ptolemy, it remains one of the 88 modern constellations. The four brightest stars, Gamma, Delta, Epsilon, and Beta Corvi from a distinctive quadrilateral in the night sky. The young star Eta Corvi has been found to have two debris disks.
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