Vulpecula: Difference between revisions

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=HGS Session References== HGS Sessions - Clearing [[]] - 3/24/2015 <ref> HGS Session</ref>==References==<references/>Found in HGS Manual on Page 108 Found in HGS Manual on Page 115 [[Category: Ascension]][[Category: HGS Manual]]
=HGS Session References==  
 
HGS Sessions - Clearing [[]] - 3/24/2015 <ref> HGS Session</ref>
 
==References==
 
 
<references/>
 
 
Found in HGS Manual on Page 108 Found in HGS Manual on Page 115  
 
 
 
[[Category: Ascension]][[Category: HGS Manual]]

Revision as of 00:48, 25 March 2015

Vulpecula is a faint constellation in the northern sky. Its name is Latin for "little fox", although it is commonly known simply as the fox. It was identified in the seventeenth century, and is located in the middle of the Summer Triangle(an asterism consisting of the bright stars Deneb, Vega and Altair).Vulpecula is also home to HD 189733 b, one of the closest extrasolar planet currently being studied by the Spitzer Space Telescope. On 12 July 2007 the Financial Times(London) reported that the chemical signature of water vapour was detected in the atmosphere of this planet.



Deep-sky objects

Two well-known deep-sky objects can be found in Vulpecula. The Dumbbell Nebula (Messier 27), is a large, bright planetary nebula which was discovered by the French astronomer Charles Messier in 1764 as the very first object of its kind. It can be seen with good binoculars in a dark sky location, appearing as a dimly glowing disk approximately 6 arcminutes in diameter. A telescope reveals its double-lobed shape, similar to that of an hourglass. Brocchi's Cluster (Collinder 399) is an asterism formerly thought to be an open cluster. It is also called "the Coathanger" because of its distinctive star pattern when viewed with binoculars or a low power telescope.


NGC 7052 is an edge-on spiral galaxy in Vulpecula at a distance of 214 million light-years from Earth. It has a central dusty disk with a diameter of 3700 light-years; there is a supermassive black hole with a mass of 300 million solar masses in its nucleus. Astronomers surmise that the disk is the remnant of a smaller galaxy that merged with NGC 7052. Jets can be seen emanating from the galaxy, and it has very strong radio emissions. This means that it is also classified as a radio galaxy.

The eastern part of Vulpecula is occupied by the Hercules–Corona Borealis Great Wall. It is a galaxy filament, with the length of 3,000 megaparsecs, making it the largest structure in the universe.


HGS Session References=

HGS Sessions - Clearing [[]] - 3/24/2015 [1]

References

  1. HGS Session


Found in HGS Manual on Page 108 Found in HGS Manual on Page 115