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The Antares Emission Nebula and Mass Loss of α Sco A
The Antares Emission Nebula and Mass Loss of α Sco A

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... Copyright © 2010 Pearson Education, Inc. ...
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... region and looks for a match. All this may take a few seconds. When it's done, it will spit out the results of its match. For the Hale-Bopp image, CHARON finds 9 Guide Star Catalog stars in the image that match within a tolerance of 1 arcsecond. It spits out some details of the match, such as resid ...
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... the middle and shows a nice disk at higher powers. It was spotted at 100X but the central star was never seen, just a brightening in the middle. At 330X on a great night I saw the east side as consistently brighter than the west side. I called the color grey in the 13", using my old 17.5" Dobsonian ...
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... 1.Let's say we find a star that is located on the following points or circles in the sky. Then, on the same night we move to a location on Earth that is some significant distance from our first location. There will now be a different star at or on: a. the celestial north pole b. the zenith c. the ce ...
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... stars, we expect to find two classes of objects: young stars and chromospherically active binaries. Sometimes, a star suspected of being young can be instead a spectroscopic binary (Soderblom et al. 1998), not yet investigated by radial velocity surveys. The chromospheric activity surveys by the Mou ...
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Ursa Minor



Ursa Minor (Latin: ""Smaller She-Bear"", contrasting with Ursa Major), also known as the Little Bear, is a constellation in the northern sky. Like the Great Bear, the tail of the Little Bear may also be seen as the handle of a ladle, hence the name Little Dipper. It was one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Ursa Minor has traditionally been important for navigation, particularly by mariners, due to Polaris being the North Star.Polaris, the brightest star in the constellation, is a yellow-white supergiant and the brightest Cepheid variable star in the night sky, ranging from apparent magnitude 1.97 to 2.00. Beta Ursae Minoris, also known as Kochab, is an aging star that has swollen and cooled to become an orange giant with an apparent magnitude of 2.08, only slightly fainter than Polaris. Kochab and magnitude 3 Gamma Ursae Minoris have been called the ""guardians of the pole star"". Planets have been detected orbiting four of the stars, including Kochab. The constellation also contains an isolated neutron star—Calvera—and H1504+65, the hottest white dwarf yet discovered with a surface temperature of 200,000 K.
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