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The Solar Neighborhood
The Solar Neighborhood

... Hotter stars are brighter in blue light than in yellow light, have low values of B-V color, and are found on the left side of the diagram. Cooler stars are brighter in yellow light than in blue light, have larger values of B-V color, and are found on the right side of the diagram. ...
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E8B6_CRT_CR_MSTIPS_Final
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... 1. A star map that show stars to at least the 7th magnitude will make the effort much easier. The Cambridge Star Atlas is adequate but Sky Atlas 2000 is even better. 2. At first glance, these galaxies reside in an apparently vacant stretch of the sky from Vindemiatrix (Epsilon Virginis) to Denebola ...
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... The most notable star in Cetus is Mira ("the Wonderful"), designated Omicron Ceti, the first variable star to be discovered and the prototype of its class. Over a period of 332 days it reaches a maximum apparent magnitude of 3 - visible to the naked eye - and dips to a minimum magnitude of 10, invis ...
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... When there is turbulence in the atmosphere refraction is not uniform or steady, changes from moment to moment, changing the direction of light slightly all the time. Stars are so far away that, their angular diameters are extremely small, typically 1/100th of an arc second or less. So even a tiny ch ...
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... when the Moon is in the sky or black and blue when it is not. The areas where the Moon is shown black indicate that the sky is completely dark. See Page 7 for charts showing the positions of planets. MERCURY rises and sets after the Sun so it is in the sky during the day, close to the Sun and not vi ...
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... American Henry Russell, determined a pattern in the life of stars. They arranged stars on a chart according to their color and brightness. The most amazing thing is that they did not even know one other, and did their experiments completely independent of each other. Therefore, this chart is called ...
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... On the morning of the 7th the Moon rises at around 07:00, and with Mercury and Venus present a photo opportunity in the south-east. Saturn, Mars and Jupiter can be found at this time too, hugging the line of the ecliptic traced towards the west. Take an opportunity to observe them during the first t ...
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... The original H-R diagram plotted the star’s luminosity versus its spectral type. It only included stars within 100 pc of the Sun as that was the limit for determining distances using the heliocentric parallax method, the only known method at the time. ...
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... the size of the Sun’s, there is a lot more of it to shine light into space, so it still ends up brighter than the Sun. It’s a old star too, being much further through its lifecycle than the Sun, having exhausted its supply of hydrogen it is now generating energy by fusing atoms of helium into carbon ...
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... portions. As with M8, OIII and Deep Sky filters work well here. Messier 17 is my favorite emission nebula in Sagittarius. Commonly known variously as the Omega, Swan, or Horseshoe Nebula, resides about 4,900 light years away. M17 is a relatively large object at 40’, with a combined magnitude of 6, a ...
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... B. Find Polaris again. Then find the constellation Cassiopeia to the east. Click roughly midway and slightly below a line connecting Cassiopeia and Pegasus within the constellation boundary of Andromeda and hit the space bar to center. Slowly zoom in until you see a galaxy in the field of view. Clic ...
The magnitude scale, parallax, the parsec, and Cepheid distances
The magnitude scale, parallax, the parsec, and Cepheid distances

... •  But  not  convenient  when  comparing  sources  of  very   different  brightness   –  e.g.  if  f  ranges  from  101  to  1030  units   ...
Hertzsprung-Russell Diagrams and Distance to Stars
Hertzsprung-Russell Diagrams and Distance to Stars

... Discovering whether this was true presented some obvious challenges. Since the distances to the stars were unknown, one could not determine the intrinsic brightness of a star, but only its apparent brightness. As we’ve already said, a bright star that’s very far away would appear much fainter than ...
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Crux



Crux /ˈkrʌks/, located in the deep southern sky, is the smallest yet one of the most distinctive of the 88 modern constellations. Its name is Latin for cross, and it is dominated by a cross-shaped asterism that is commonly known as the Southern Cross. Although visible to the Ancient Greeks, it was seen as part of the constellation Centaurus, and not defined or accurately mapped till the 16th century.Known as Acrux, blue-white Alpha Crucis is the constellation's brightest star and the bottom star of the cross. Nearly as bright are Beta and Gamma, while Delta and Epsilon make up the asterism. Many of the constellation's brighter stars are members of the Scorpius–Centaurus Association, a loose group of hot blue-white stars that appear to share a common origin and motion across the Milky Way. Two star systems have been found to have planets. The constellation also contains four Cepheid variables visible to the naked eye under optimum conditions. Crux also contains the Jewel Box, a bright open cluster, and the Coalsack Nebula, the most prominent dark nebula in the sky.
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