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Orion constellation

Orion Constellation This is a mosaic picture of 18 (6x3) frames. Additional four frames are added around the Barnard Loop region to increase S/N. Vignetting of the telescope is corrected by flat fielding, using proprietary software written in IDL. Distortion correction and initial colour match is done in Registar, with final colour correction and mosaic processed using Photoshop. (Reproduced by permission of Wei-Hao Wang, Institute for Astronomy at University of Hawaii)... [Pg.341]

Jupiter, the book included the observations of the milky-way, stars in Orion constellation, the bright Pleiades and beehive cluster. [Pg.61]

Figure 2 Ground-based line surveys of a star-forming region in the Orion constellation in three atmospheric windows centred at 240, 330 and 700 GHz. Note the richness of the spectrum. Some of the more prominent lines are labelled by the molecule responsible. Courtesy of TG Philips. Figure 2 Ground-based line surveys of a star-forming region in the Orion constellation in three atmospheric windows centred at 240, 330 and 700 GHz. Note the richness of the spectrum. Some of the more prominent lines are labelled by the molecule responsible. Courtesy of TG Philips.
Now that we have a simple model for the continuum spectrum of the stars based around the Planck curve, the temperature and the luminosity, we can make some observations and classifications of the stars. There are some constellations that dominate the night sky in both the northern and southern hemispheres and even a casual look should inspire wonder. Star hopping in the night sky should lead to the simplest observation not all stars have the same colour. A high-quality photograph of the constellation of Orion (see page 2 of the colour plate section) shows stars... [Pg.21]

Fig. 6.1. Stellar nursery in the constellation of Orion. Molecular clouds A and B were detected by their radio emissions. They appear to have given birth to several generations of stars (la, It and Ic). Fig. 6.1. Stellar nursery in the constellation of Orion. Molecular clouds A and B were detected by their radio emissions. They appear to have given birth to several generations of stars (la, It and Ic).
An object which is about 300 light years in diameter and which closely resembles the terminal stage of a supernova explosion is visible today in the constellation Orion (the Orion Halo). A number of very bright young stars are located within the Orion Halo, and their ages are estimated to be less than 5-10 million years obviously their formation was triggered by the shock wave of the supernova explosion. [Pg.95]

Bob likes his large bedroom in the museum ship. He looks out the windows at the stars. The more recognizable constellations are unmistakable. Orion s square shoulders and feet. The beautiful zigzagging Cassiopeia. The enigmatic Pleiades. They all remind him of life back on Earth where he studied the con-... [Pg.39]

Miss Muxdroozol takes a deep breath. I can think of other things that would change if your dominant civilizations first appeared in what you call the Southern Hemisphere. The names of the constellations would be different.5 For example, viewed from Australia, Orion the Hunter is standing on his head—hardly a heroic pose The direction clockwise would be opposite from how you now define it. Your human clocks rotate as does the shadow in a sundial in the Northern Hemisphere. In the Southern Hemisphere, the sundial s shadow is counterclockwise. ... [Pg.50]

Figure 5.4 Betelgeuse, the second brightest star in the constellation Orion. Betelgeuse, a red supergiant, is one of the largest stars known and has a diameter around 500 times the diameter of the Sun. Figure 5.4 Betelgeuse, the second brightest star in the constellation Orion. Betelgeuse, a red supergiant, is one of the largest stars known and has a diameter around 500 times the diameter of the Sun.
Figure 5.5 The constellations of Orion and Canis Major. Note the location of Sirius, the Orion Nebula, and Betelgeuse, which are discussed throughout this book. [From Hubert Reeves, Atoms of Silence (Cambridge, Massachusetts MIT Press, 1984), 127, fig. 41, after Vesalius.]... Figure 5.5 The constellations of Orion and Canis Major. Note the location of Sirius, the Orion Nebula, and Betelgeuse, which are discussed throughout this book. [From Hubert Reeves, Atoms of Silence (Cambridge, Massachusetts MIT Press, 1984), 127, fig. 41, after Vesalius.]...
Job 38 31-32 Can you bind the beautiful Pleiades Can you loose the cords of Orion Can you bring forth the constellations in their seasons or lead out the Bear with its cubs Do you know the laws of the heavens ... [Pg.213]

BURNHAM S CELESTIAL HANDBOOK, Robert Burnham, Jr. Thorough guide to the stars beyond our solar system. Exhaustive treatment. Alphabetical by constellation Andromeda to Geius in Vol. 1 Chamaeleon to Orion in Vol. 2 and Pavo to Vulpecula in Vol. 3. Hundreds of illustrations. Index in Vol. 3. 2,000pp. 6X x 9X. 23567-X, 23568-8,23673-0 Pa.. Thiee-vol. set 38.85... [Pg.122]

This is the well-known Horsehead nebula in the constellation Orion. It is made mostly of dust, plus some cold hydrogen gas, and it stands out in silhouette against a more distant mass of hot, luminous hydrogen. It is similar to the great black rift and the indistinct dark clouds which obscure great sections of the veil of stars in the Milky Way. [Pg.221]

P13.30 The question of whether to use CN or CH within the interstellar cloud of constellation Ophiuchus for the determination of the temperature of the cosmic background radiation depends upon which one has a rotational spectrum that best spans blackbody radiation of 2.726 K. Given flo(CH) = 14.90 cm-1, the rotational constant that is needed for the comparative analysis may be calculated from the 226.9 GHz spectral line of the Orion Nebula. Assuming that the line is for the l2Cl4N isotopic species and J + 1 <— 7=1, which gives a reasonable estimate of the CN bond length (117.4 pm), the CN rotational constant is calculated as follows. [Pg.264]

Plate 2 illustrates the dramatic difference between the visible and infrared image of the sky looking towards Orion. The infrared radiation that dominates the IR image of the constellation (colored red in the figure) comes from the blackbody radiation of the interstellar dust particles comprising what is known as... [Pg.85]

JUGGLER Occ. WIRTH 1927 relates this first arcanum of the Tarot pack to the Hebraic ALEPK, and thus to the constellation Orion and zodiacal Taurus, He accords the card the sigii and the point drawn as the centre of the pupil in the Eye of God, Q thus completing a cycle in the 22 arcana with the of the last in the series, the... [Pg.149]

Bezaleel also bears a remarkable similarity to Azazel (Azdzil in Arabic) or Shemyaza, the leader of the fallen Watchers in the Judaic-Christian apocryphal Book of Enoch. Just as Prometheus presented man with fire, Azazel released to humankind the secrets of metallurgy, the manufacture of weapons and jewelry, and the use of antimony in art and medicine. He also taught women the art of cosmetics, to be promiscuous and to enjoy sex. For these transgressions, God condemned Azazel to remain forever bound in the desert of Dudael. As Shemyaza, he hangs upside down between heaven and earth in the constellation of Orion. The only known statute of this leader of the Watchers is in the choir of Rosslyn Chapel, in Scotland. [Pg.155]

FIGURE P.1 Left Orion Nebula Constellation, right The Crab Nebula neutron star, as they were registered by Hubble Space Telescope (Cahfomia) [Hubble Site (2014). http // hubblesite.org/newscenter/archive/ieleases/2005/37/]. [Pg.526]


See other pages where Orion constellation is mentioned: [Pg.461]    [Pg.12]    [Pg.86]    [Pg.432]    [Pg.944]    [Pg.461]    [Pg.12]    [Pg.86]    [Pg.432]    [Pg.944]    [Pg.28]    [Pg.29]    [Pg.114]    [Pg.215]    [Pg.150]    [Pg.57]    [Pg.465]    [Pg.78]    [Pg.87]    [Pg.134]    [Pg.199]    [Pg.249]    [Pg.40]    [Pg.5]    [Pg.321]    [Pg.350]    [Pg.14]    [Pg.46]    [Pg.37]    [Pg.80]    [Pg.264]    [Pg.526]    [Pg.170]   
See also in sourсe #XX -- [ Pg.12 ]




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Constellations

Orion

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