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AbbreviationVelVelorumPronunciation,genitiveSymbolismthe9 h−50°QuadrantSQ2500 sq. 5/stars50Stars with7Stars brighter than 3.00 m5Stars within 10.00 pc (32.62 ly)3Brightest star(1.75 )0BorderingconstellationsVisible at latitudes between +° and −°.Best visible at 21:00 (9 p.m.) during the month of March.Vela is a in the southern sky. Its name is for the of a ship, and it was originally part of a larger constellation, the ship, which was later divided into three parts, the others being. With an apparent magnitude of 1.8, its brightest star is the hot blue multiple star, one component of which is the brightest star in the sky. And, together with and, form the known as the. 1.95-magnitude Delta is actually a triple or quintuple star system. Contents.History was one of the 48 classical constellations listed by the 2nd-century astronomer, and represented the ship, used by and the on their quest for the in.
German cartographer depicted the constellation on his of 1603, and gave the stars from Alpha to Omega. However, his chart was inaccurate as the constellation was not fully visible from the Northern Hemisphere.Argo was more accurately charted and subdivided in 1752 by the French astronomer, forming Carina (the ), Vela (the sails), and Puppis (the ). Despite the division, Lacaille kept Argo's. Therefore, Carina has the Alpha, Beta and Epsilon originally assigned to Argo Navis, while Vela's brightest stars are Gamma and Delta, Puppis has Zeta as its brightest star, and so on. Characteristics Vela is bordered by and to the north, to the northwest, to the south and southwest, and to the east. Covering 500 square degrees, it ranks 32nd of the 88 in size.
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The three-letter abbreviation for the constellation, as adopted by the in 1922, is 'Vel'.The official constellation boundaries, as set by in 1930, are defined by a polygon of 14 segments. In the, the coordinates of these borders lie between 08 h 13.3 m and 11 h 05.5 m, while the coordinates are between −37.16° and −57.17°. Features Stars. See also:The brightest star in the constellation, is a complex multiple star system. The brighter component, known as Gamma 2 Velorum or Suhail, shines as a blue-white star of apparent magnitude 1.83. It is a spectroscopic binary made up of two very hot blue stars orbiting each other every 78.5 days and separated by somewhere between 0.8 and 1.6 Astronomical Units (AU).
The brighter component is a hot blue main-sequence star of spectral type O7.5 and is around 280,000 times as luminous, is around 30 times as massive and is 17 times the diameter of our Sun with a surface temperature of 35,000 K. The second component is an extremely rare example of hot star known as a, and is the brightest example in the sky.
It has a surface temperature of 57,000 and is around 170,000 times as luminous as our sun, though it radiates most of its energy in the ultraviolet spectrum. Gamma 1 is a blue-white star of spectral type B2III and apparent magnitude 4.3. The two pairs are separated by 41 arcseconds, easily separable in binoculars. Parallax measurements give a distance of 1,116 light-years, meaning that they are at least 12,000 AU apart. Further afield are 7.3-magnitude Gamma Velorum C and 9.4-magnitude Gamma Velorum D, lying 62 and 93 arcseconds south-southeast from Gamma 2. Dusty ring around double star.The next brightest star is or Alsephina, also a multiple star system and one of the brightest eclipsing binaries in the sky.
Together with or Markeb, or Aspidiske and or Avior, it forms the diamond-shaped known as the —so called because it is sometimes mistaken for the, causing errors in. Appearing as a white star of magnitude 1.95, Delta is actually a triple or possibly quintuple star system located around 80 light-years from the. Delta A has a magnitude of 1.99 and is an composed of two A-type white stars (Delta Aa and Ab) which orbit each other every 45.2 days and lie 0.5 AU from each other, with a resulting drop in magnitude of 0.4 when the dimmer one passes.in front of the brighter. Delta B is a 5.1 magnitude yellow G-class star of similar dimensions to our sun which ranges between 26 and 72 AU away from the brighter pair, taking 142 years to complete a revolution. Further out still, at a distance of 1700 AU, are two red dwarfs of magnitudes 11 and 13.
If they are part of the multiple system, they take 28000 years to complete an orbit. Also called Markeb, Kappa appears as a blue-white star of spectral type B2IV-V and magnitude 2.47 but is in fact a spectroscopic binary. The two orbit around each other with a period of 116.65 days, but the size, mass and nature of the companion are as yet unclear.The orange-hued, or Suhail, is the third-brightest star in the constellation. A supergiant of spectral type K4Ib-II, it varies between magnitudes 2.14 and 2.3, and lies 545 light-years distant.
It has around 11,000 times the luminosity, 9 to 12 times the mass and 207 times the diameter or our sun.is a Cepheid variable located less than a degree to the northeast of Gamma. A yellow-white supergiant of spectral type F7Ib-II, it pulsates between magnitudes 5.5 and 5.89 over 4.2 days.
Also lying close to Gamma, is a Cepheid of spectral type F6-F9II ranging from magnitude 7.2 to 7.9 over 4.4 days. Is located 2.8 degrees north-northeast of Gamma, a Delta Scuti variable of spectral type A2p-F2pIV/V that ranges between magniudes 6.15 and 6.76 in around 2.7 hours.is an aged star that has been found to be surrounded by a dusty disk. An, it has a spectral type of F3e and ranges between magnitudes 9.01 and 9.27 over nearly 95 days.is a blue-white subgiant of spectral type B3III-IV located around 495 light-years from the Solar System. A slowly pulsating B star, it ranges between magnitudes 3.57 and 3.63 over 2.8 days. It is the brightest star in, and gives its name to, the Omicron Velorum Cluster, also known as, an located around 500 light-years away.Seven star systems have been found to have.
Is a Sun-like star of spectral type G0V with a planetary companion that takes only about 3.51 days to revolve at an of 0.0482. Is a star of apparent magnitude 12.3 located 815 light-years away, which has a hot Jupiter-like planet that orbits every 0.7 days. Deep-sky photograph of, also known as the Eight-Burst or Southern Ring Nebula. © NASA.The is a faint, believed to be the remains of a million-year-old supernova. Within it lie the smaller and younger.
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This is the of a explosion that is believed to have been visible from Earth around 10,000 years ago. The remnant contains the, the first to be identified optically.
Nearby is, also known as the Pencil Nebula.is a, a young star around 1,400 from the Sun that is ejecting material at tremendous speed (up to a million kilometres per hour) into its surrounds. This material glows as it hits surrounding gas.is an located in Vela. It has an overall magnitude of 7.8 and is 3,200 light-years from Earth. The stars of NGC 2670, a Trumpler class II 2 p and Shapley class-d cluster, are in a conformation suggesting a bow and arrow. Its class indicates that it is a poor, loose cluster, though detached from the star field. It is somewhat concentrated at its center, and its less than 50 stars range moderately in brightness.Located 2 degrees south of Gamma Velorum, is an open cluster containing around 50 stars of magnitudes 7 to 15.is a discovered by on May 28, 1826. Its stellar population is inhomogeneous, varying with distance from the core.
The of the stars shows an increase with greater distance, with the redder and cooler stars tending to be located closer to the core. As of 2010, is one of only two clusters (including ) that shows a definite inhomogeneous population.is a star-forming region in Vela, and one of the nearest sites of massive star formation. This star-forming region has given rise to a cluster of several hundred young stars that power an HII region. The star-forming region lies in Clump 6 in the Cloud C. References.
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DSM-5 Guidebook Ebook ContentThis guidebook serves as a companion to the Diagnostic and Statistical Manualof Mental Disorders, 5th Edition (DSM-5; American Psychiatric Association 2013).DSM has long been used as the psychiatric diagnostic system in the United States andelsewhere, and DSM-5 follows in the grand tradition of its predecessors. For manymental health practitioners, however, the method of psychiatric diagnostic classificationis daunting. Because DSM-5 is large, totaling 947 pages (not including the classificationlisting and preface), many users will find it intimidating. Many will think,“Where do I begin? How will I ever understand and use the criteria?” Also, users ofDSM-IV-TR (American Psychiatric Association 2000) will wonder how DSM-5 differs.These are some of the bread-and-butter issues we tackle in this guidebook.Our goal with this book is not to recapitulate DSM-5.
Wikispaces was founded in 2005 and has since been used by educators, companies and individuals across the globe.Unfortunately, the time has come where we have had to make the difficult business decision to end the Wikispaces service.We first announced the site closure in January 2018, through a site-wide banner that appeared to all logged-in users and needed to be clicked on to dismissDuring the closure period a range of banners were shown to users, including a countdown banner in the final month. Additionally, the home page of Wikispaces.com became a blog, detailing the reasons for the closure. Private Label Site Administrators were contacted separately regarding the closureWikispaces TierClosedown DateClassroom and Free Wikis end of service31st July 2018Plus and Super Wikis end of service30th September 2018Private Label Wikis end of service31st January 2019.
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