What will happen when the fragments hit Jupiter? ... All the fragments will enter Jupiter's atmosphere at an angle of 42 degrees from the vertical and impact near a latitude of 44 degrees south, but on the back side of the planet as seen from Earth (about 10 degrees in longitude behind the edge of Jupiter, as seen from Earth). ... Any body moving through an atmosphere is slowed by atmospheric drag, by having to push the molecules of that atmosphere out of the way. ...

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• ASP: More About Deep Space Objects and Cosmic Terms
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... Space Flight . ... With warp drive we could perhaps see NGC3572 up close. (image credit: ESO/G. Beccari) . ... In science fiction, most famously the Star Trek franchise, €аa propulsion system called warp drive enables starships to travel faster than light across the Milky Way. How is this meant to work?€а According to fiction, a warp drive bends space around the starship, enclosing it in a bubble of curved space. ... Reply . ... Do you think NASA is actually building a faster than light starship? ...

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... Ciel Espace, le magazine qui vous guide toujours plus loin . ... Ciel Espace, nouvelle formule, c'est . des actualitГїs . des reportages . ... Accueil La Lune Г 100 km, en 3D depuis la capsule Apollo . ... Le troisiГЕme homme des missions Apollo, celui qui ne marchait pas sur la Lune, restait en orbite, Г observer la surface lunaire. ... Lors de la mission Apollo 16, la rГїgion d'alunissage du module Orion Гїtait Г la mГ?me latitude que le grand cratГЕre ThГїophile (100 km de diamГЕtre). ...

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• LRO photographie un †йtrange chenal lunaire | Ciel et Espace

Astronomical Data Analysis Software and Systems VII ASP Conference Series, Vol. ... An Optimal Data Loss Compression Technique for Remote Surface Multiwavelength Mapping Sergei V. Vasilyev Solar­Environmental Research Center, P.O. Box 30, Kharkiv, 310052, Ukraine Abstract. This paper discusses the application of principal component analysis (PCA) to compress multispectral images taking advantage of spectral correlations between the bands. ... 506 Vasilyev Figure 1. ... 1985; Vasilyev 1996). ...

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• HST NICMOS Observations of Circumstellar Matter Around CYG X-3
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General Forum Message . ... The END Of The DARK ENERGY . ... THE DECREASING UNIVERSE AND THE END OF THE DARK ENERGY . ... The dark energy is a УAd-HocФ hypothesis postulated with the only purpose of explaining the apparent fast separation of distant galaxies. ... Light through space . ... End of the Dark Energy . ... www.astronomy.net . About Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• CCD And What's Needed????? - an Astronomy Net CCD Equipment and Techniques
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. Wind Baffle Altitude Drive Chain: March 26, 2002 . Shown lying free at maximum sideways curvature: . chain length max (tension) - 140 5/8" . chain length min (compression) = 139 1/2" . Close up shows typical gaps in side bars of adjoining links

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• Mechanical Properties of Ribbed Plastic Sleeves

from __future__ import division from visual import * import math spacing = 1.0E-10 k = 8.0E-4 # Tension compression constant kt = 3.0E-5 # Torsion constant u = 1.660E-27 ioncharge = 1.0 *1.602E-19 rad = 3.0E-11 scale = 2.0* spacing scene = display(range=(scale,scale,scale),width=1200,height=800, background=color.black) theta = 30.*math.pi/180.0 oxy1 = sphere() oxy1.pos = vector ( spacing *math.cos(theta), ...

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• http://www.mso.anu.edu.au/pfrancis/simulations/h2o.py
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Feb 28 2016 Vulpecula - The Fox CR 399 12x50 Open Cluster III3m B,L,NO COMPRESSION,R=G Nov 14 2006 1.9" IC 4954 11mmT6 FAINT,SMALL,R=F Nebula R Nov 16 2012 18" NGC 6793 11mmT6 H81-8 Open Cluster III 2 p CL,P,LC Aug 18 2010 12" PF,PS,R=F, STARS 10-12 NGC 6800 11mmT6 H21-8 PF,CS,R=P,STARS 8+? ... Aug 18 2010 12" NGC 6802 11mmT6 H14-6 PF,CS,R=F Open Cluster 14.0 I 1 m CL,L,VC,E0,ST14.. ... 12 Jun 20 2007 1.9" Jul 23 2006 8" NGC 6830 11mmT6 H9-7 B,PS,R=F Open Cluster 10.0 II 2 p CL,L,PRI,PC,*11.. ...

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EMI test using VXD3 R20 assembly Nick Sinev, University of Oregon Outline The problem Why we want beam test? ... What do we need for test ? Conclusion January 7, 2005 Nick Sinev, MDI workshop, SLAC 2 The problem As you already know from M.Breidenbach talk, we had observed Electromagnetic Interference (EMI) effects in VXD3 operation. ... January 7, 2005 Nick Sinev, MDI workshop, SLAC 3 Why beam ? ... January 7, 2005 Nick Sinev, MDI workshop, SLAC 12 ...

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• http://zebu.uoregon.edu/~uochep/talks/talks00/brau_D3.pdf

VISTA Data Flow System: Status Jim Emerson*a, Mike Irwinb, Nigel Hamblyc b a Astronomy Unit, Queen Mary Universit y o f London, Mile End Road, London E1 4NS, UK Inst itute of Astronomy, Universit y of Cambridge, Madingley Road, Cambridge CB3 0HA, UK, c Inst itute for Astronomy, School of Phys ics, Universit y of Edinburgh, Edinburgh EH9 3HJ, UK ABSTRACT Data from two IR survey cameras UKIRT's WFCAM and ESO's VISTA can arrive at rates approaching 1.4 TB/night for of order 10 years. ...

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• http://www.vista.ac.uk/Files/docs/vdfs/spie-5493-30_VDFS-Overview.pdf

... Stanley G. Love (Ph.D.)б  . NASA Astronaut . ... Postdoctoral Fellowship, California Institute of Technology (1995);б  NOVA Award, Jet Propulsion Laboratory (1998);б  Lyndon B. Johnson Space Center Group Achievement Award (Expedition 6 Spacewalk Team , 2003);б  NASA Space Flight Awareness Team Award (ISS Testbed for Analog Research Team (2013); Orbital Space Plane Team (2004);б  United States Antarctica Service Medal (2006);б  Orion Phase 2 Source Evaluation Team (2007);б  ...

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SPI Imaging : 16° fully coded FOV Angular resolution : 2.6° Energy range : 20 keV- 8 MeV Energy resolution : 0.2 % Time resolution : 100 microsec Shield : active BGO shield Camera :19 HPGe detectors. ... Energy range : [60,1836] keV. 4 MeV-van de Graaf accelerator, calibration up to 8062 keV. ... IMAGING PERFORMANCES 2.7 MeV Response matrix generation by Monte-Carlo simulation Instrument Response: Overview · A detailed mass model was created "by hand" based on technical drawings. ...

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TOPSIDE AUTOMATED SOUNDER TOPAS/W . ... Table 6 TOPAS/W Subassembly Power Details . ... The TOPside Automated Sounder for the Ukrainian WARNING mission (TOPAS/W) will probe plasma densities from the altitude of the spacecraft at 600 km down to the peak of the F2-layer using only 30 W peak transmitter power. ... Upon power-up of the TOPAS/W, the TOPAS/W will load a bootstrap program from on-board EPROM, then load the operating software and the measurement and schedule tables from on-board EEPROM. ...

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• Olga P. Verkhoglyadova
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Retrofitting a 13" Dobsonian By Dave Aucoin . ... I had retrofitted the scope, not the older box and tube, but the newer tube design, to break apart to fit in my then Chevy Chevette. ... Then my girlfriend mentioned that I should build up the pads with blocks so that the mirror box would slide properly over the Teflon and not catch on the ZHRB. ... Now the lower block, attached to the mirror box has 2 angles that have to be used for the tube to reach the upper clamp block without too much bending. ...

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Class 1 Introduction, Background History of Modern Astronomy The Night Sky, Eclipses and the Seasons Kepler's Laws Newtonian Gravity General Relativity Matter and Light Telescopes Class 2 Solar System Characteristics Formation Exosolar Planets Class 3 Stars The Sun Stellar Evolution of Low and High Mass Stars Deaths of Stars Class 4 Galaxies Galaxy Classification Formation of Galaxies Galactic Evolution Large-Scale Structure of the Universe Big Bang Cosmology Why is Pluto no longer a planet? ...