Stardust-Next Press Kit February 2011
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TV Channel Lineup 607-589-6235
True TV Channel Lineup 607-589-6235 : www.htva.net Spencer East System – Barton, Candor, Halsey Valley, Smithboro, Spencer, Tioga, Weltonville, Willseyville, Lockwood v: 04302020 s Lifeline Tier Basic Tier (ctd.) Digital Tier (ctd) Digital Tier (ctd) High Def (ctd) Premium 3 WBGH NBC 3 Bing. 47 Lifetime 115 IFC 209 WSKG3 PBS Create 506 TBS HD 2 HBO 4 Local Ads 48 Animal Planet 116 TCM 210 WSKG4 PBS World 514 HLN HD 5 Cinemax 6 WICZ FOX 40 Bing. 49 Food Network 117 FX Movies 212 WENY3 CW 2 Elm. 515 CNN HD 98 HBO 2 7 WSKG PBS 46 Bing. 50 Comedy Central 118 Outdoor Channel 216 ESPNU 516 MSNBC HD 400 HBO SD 8 WENY2 CBS Elm. 51 HLN 119 The Golf Channel 223 Paramount 517 FOX News HD 401 HBO 2 SD 9 WIVT ABC 34 Bing. 52 CNN 120 FXX 261 VH1 521 Nick HD 402 HBO Signature 11 WBXI CW 11 Bing. 53 MSNBC 121 ESPN News 523 BIG10 Network HD 403 HBO Family 12 WBNG CBS 12 Bing. 54 FOX News 122 SEC Network 182High DefinitionWSPX Ion 56 HD 524 NFL Network HD* 404 HBO HD 13 WENY ABC 36 Elm. 55 CNBC 124 NFL Network 525 TNT HD 405 HBO 2 HD 14 WBPN MY 8 Bing. 56 Travel Channel 125 NBC Sports 182 WSPX ION 56 HD 527 Discovery HD 410 Cinemax SD 15 Weather Channel 57 VH1 126 RFD 185 WBXI CW 11 HD 528 CMT HD 411 MoMAX 17 Channel Guide 58 MTV 128 BBC World News 200 WBNG CBS 12HD 529 BBC America HD* 412 Cinemax HD 22 WSPX ION 56 Syr. -
FCC-06-11A1.Pdf
Federal Communications Commission FCC 06-11 Before the FEDERAL COMMUNICATIONS COMMISSION WASHINGTON, D.C. 20554 In the Matter of ) ) Annual Assessment of the Status of Competition ) MB Docket No. 05-255 in the Market for the Delivery of Video ) Programming ) TWELFTH ANNUAL REPORT Adopted: February 10, 2006 Released: March 3, 2006 Comment Date: April 3, 2006 Reply Comment Date: April 18, 2006 By the Commission: Chairman Martin, Commissioners Copps, Adelstein, and Tate issuing separate statements. TABLE OF CONTENTS Heading Paragraph # I. INTRODUCTION.................................................................................................................................. 1 A. Scope of this Report......................................................................................................................... 2 B. Summary.......................................................................................................................................... 4 1. The Current State of Competition: 2005 ................................................................................... 4 2. General Findings ....................................................................................................................... 6 3. Specific Findings....................................................................................................................... 8 II. COMPETITORS IN THE MARKET FOR THE DELIVERY OF VIDEO PROGRAMMING ......... 27 A. Cable Television Service .............................................................................................................. -
Rosetta Craft Makes Historic Comet Rendezvous European Space Agency's Comet-Chasing Mission Arrives After 10-Year Journey
NATURE | NEWS Rosetta craft makes historic comet rendezvous European Space Agency's comet-chasing mission arrives after 10-year journey. Elizabeth Gibney 06 August 2014 ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA Comet 67P/Churyumov–Gerasimenko, as seen by Rosetta from a distance of 285 kilometres. No one can deny that it was an epic trip. The European Space Agency's comet-chasing Rosetta spacecraft has arrived at its quarry, after launching more than a decade ago and travelling 6.4 billion kilometres through the Solar System. That makes it the first spacecraft to rendezvous with a comet, and takes the mission a step closer to its next, more ambitious goal of making the first ever soft landing on a comet. Speaking from mission control in Darmstadt, Germany, Matt Taylor, Rosetta project scientist for the European Space Agency (ESA), called the space mission “the sexiest there’s ever been”. Rosetta is now within 100 kilometres of its target, comet 67P/Churyumov–Gerasimenko (or 67P for short), which in July was discovered to be shaped like a rubber duck. After a six-minute thruster burn, at 11:29 a.m. local time on 6 August, ESA scientists confirmed that Rosetta had moved into the same orbit around the Sun as the comet. Rosetta is now moving at a walking pace relative to the motion of 67P — though both are hurtling through space at 15 kilometres per second. Unlike NASA’s Deep Impact and Stardust craft, and ESA’s Giotto mission, which flew by their target comets at high speed, Rosetta will now stay with the comet, taking a ring-side seat as 67P approaches the Sun, and eventually swings around it in August 2015. -
OSIRIS-Rex, Returning the Asteroid Sample
OSIRIS-REx, Returning the Asteroid Sample Thomas Ajluni Timothy Linn William Willcockson ASRC Federal Space & Defense Lockheed Martin Space Systems Lockheed Martin Space Systems 7000 Muirkirk Meadows Drive Company, P.O. Box 179 Company, P.O. Box 179 Suite 100, Beltsville, MD 20705 Denver, CO 80201 Denver, CO 80201 301.286.1831 303-977-0659 303-977-5094 [email protected] [email protected] [email protected] David Everett Ronald Mink Joshua Wood NASA Goddard Space Flight NASA Goddard Space Flight Lockheed Martin Space Systems Center, 8800 Greenbelt Road Center, 8800 Greenbelt Road Company, P.O. Box 179 Greenbelt, MD 20771 Greenbelt, MD 20771 Denver, CO 80201 301.286.1596 301.286.3524 303-977-3199 [email protected] [email protected] [email protected] Abstract—This paper addresses the technical aspects of the sample return system for the upcoming Origins, Spectral x attitude control Interpretation, Resource Identification, and Security-Regolith x propulsion Explorer (OSIRIS-REx) asteroid sample return mission. The x power overall mission design and current implementation are presented as an overview to establish a context for the x thermal control technical description of the reentry and landing segment of the x telecommunications mission. x command and data handling x structural support to ensure successful rendezvous The prime objective of the OSIRIS-REx mission is to sample a with Bennu primitive, carbonaceous asteroid and to return that sample to Earth in pristine condition for detailed laboratory analysis. x characterization of Bennu’s properties Targeting the near-Earth asteroid Bennu, the mission launches x delivery of the sampler to the surface, and return of in September 2016 with an Earth reentry date of September the spacecraft to the vicinity of the Earth 24, 2023. -
Channel Guide
Channel Guide Station Channel Station Channel Station Channel Analog Test 2 A&E HD 32.1 CNBC HD 50.1 CBS KLKN-HD 8.1 USA Network HD 32.2 MSNBC HD 50.2 ABC KAQY-HD 8.2 BET HD 33.1 Fox News Channel HD 51.1 CW KNOE-HD 8.3 Tru-TV HD 33.2 Fox Business Network HD 51.2 Justice 8.5 FX HD 34.1 Bloomberg Television HD 52.1 Quest 8.6 FXX HD 34.2 Link TV 52.2 NBC KTVE-HD 10.1 MTV Live HD 35.1 CSPAN 53.1 FOX KARD-HD 10.2 MTV HD 35.2 CSPAN2 53.2 Laff 10.3 MTV2 36.1 TBN 54.1 Escape 10.4 VH1 HD 36.2 Inspiration Network 54.2 MeTV KMLU 11.1 Fuse HD 37.1 BYU TV 55.1 Heroes & Icons 11.2 FM 37.2 TV Land 55.2 Movies 11.3 AXS TV HD 38.1 Animal Planet HD 56.1 Start TV 11.4 CMT HD 38.2 E! Entertainment HD 56.2 PBS KLTM-HD / LBP 13.1 Pursuit TV HD 39.1 Comedy Central HD 57.1 PBS Kids / LBP2 13.2 Weather Channel HD 39.2 Cartoon Network HD 57.2 Bounce TV 14.2 Lifetime HD 41.1 Disney Channel HD 58.1 Grit 14.3 We TV HD 41.2 Disney XD 58.2 Cozi TV 14.4 OWN HD 42.1 Nickelodeon HD 59.1 ESPN HD 25.1 Oxygen 42.2 NickToons 59.2 ESPN2 HD 25.2 Bravo HD 43.1 TeenNick 60.1 ESPNews HD 26.1 HGTV HD 43.2 ION HD 60.2 ESPNU HD 26.2 Food Network HD 44.1 Freeform HD 61.1 FOX Sports 1 HD 27.1 Cooking Channel HD 44.2 GetTV 61.2 NBC Sports Network HD 27.2 Syfy Channel HD 45.1 Hallmark Channel HD 62.1 NFL Network HD 28.1 BBC America HD 45.2 HM Movies&Mysteries HD 62.2 NBA TV HD 28.2 Travel Channel HD 46.1 In Country Network 63.1 MLB Network HD 29.1 TLC HD 46.2 ReelzChannel HD 63.2 NHL Network HD 29.2 National Geographic HD 47.1 Paramount Network HD 64.1 Golf Channel HD 30.1 Discovery Channel HD 47.2 POP HD 64.2 Motor Trend HD 30.2 History Channel HD 48.1 IFC HD 65.1 TNT HD 31.1 NASA TV 48.2 AMC HD 65.2 TBS HD 31.2 HLN HD 49.1 Analog Test 116 CNN HD 49.2 Connecting Your TV & Apogee Support Whenever you hook up a new or existing TV, you will need to run a scan to receive all your channels. -
Deep Impact As a World Observatory Event Held in Brussels, Belgium, 7–10 August 2006
Other Astronomical News Report on the Workshop on Deep Impact as a World Observatory Event held in Brussels, Belgium, 7–10 August 2006 Hans Ulrich Käufl1 One of the spectacular deconvolved images from the Christiaan Sterken2 Deep Impact Spacecraft High Resolution Imager shown in the conference (courtesy Mike A’Hearn and the Deep Impact Team). This is a colour composite of an infrared, a green and a violet filter forced to av- 1 ESO erage grey. Note the blueish areas on the surface 2 Vrije Universiteit Brussel, Belgium close to the crater-like structure. Those were entirely unexpected. It is highly interesting to find out if those structures can be correlated with the jets which were meticulously monitored from ground-based ob- In the context of NASA’s Deep Impact servers worldwide. This aspect in the picture – en- space mission, Comet 9P/Tempel1 tirely unrelated to the impact plume – illustrates very well how comet research, apart from the impact has been at the focus of an unprece- experiment, will profit from the synergy of spacecraft dented worldwide long-term multi- data and the unprecedented worldwide coordinated wavelength observation campaign. The observing campaign. comet has been studied through its perihelion passage by various spacecraft including the Deep Impact mission it- self, HST, Spitzer, Rosetta, XMM and all To make full use of the global data set, a To inspire new ideas, it was very helpful major ground-based observatories in workshop bringing together observers and interesting to have Roberta Olson basically all wavelength bands used in across the electromagnetic spectrum and from the New York Historical Society, astronomy, i.e. -
Chondrule-Like Material in Wild 2: a New Insight from Impact Experiments of Chondrule Fragments on Stardust Analogue Al Foil
52nd Lunar and Planetary Science Conference 2021 (LPI Contrib. No. 2548) 1925.pdf CHONDRULE-LIKE MATERIAL IN WILD 2: A NEW INSIGHT FROM IMPACT EXPERIMENTS OF CHONDRULE FRAGMENTS ON STARDUST ANALOGUE AL FOIL. M. Van Ginneken1 and P. J. Wozniakiewicz1, 1Centre for Astrophysics and Planetary Science, School of Physical Sciences, University of Kent, United Kingdom ([email protected]; [email protected]) Introduction: NASA’s Stardust mission was the shape of craters depends mainly on the physical first mission to bring back to Earth material from a properties of the impactor [19]. Solid grains or dense celestial body, i.e. the Jupiter Family Comet (JFC) consolidated aggregates similar to chondrule fragments 81P/Wild 2 (hereafter Wild 2) [1]. Cometary dust was will result in bowl-shaped craters, the depth of which captured via impact into a collector that was deployed depending on the density of the material, whereas loose during a fly-by through the coma of Wild 2 at a relative aggregates of submicron particles result in complex speed of 6 km s-1. The collector consisted of silica features. Simulation of Stardust impacts using silicate aerogel secured into a metal frame by aluminum 1100 grains have shown that about 50% of silicate dominated foil (hereafter Al foil). A major result of the mission was impactors are retained as residue, which can be analysed the discovery that, contrary to expectations, Wild 2 was and provide precious chemical information [20]. not predominantly composed of presolar grains and low Studies of residues in a small (ø < 10 µm) or large temperature outer solar nebula material, but rather high (ø > 10 µm) craters on Stardust foil have shown that temperature (>>1000 °C) material typical of primitive these can give information on the bulk chemistry of the meteorites [1 - 3]. -
Size of Particles Ejected from an Artificial Impact Crater on Asteroid
A&A 647, A43 (2021) Astronomy https://doi.org/10.1051/0004-6361/202039777 & © K. Wada et al. 2021 Astrophysics Size of particles ejected from an artificial impact crater on asteroid 162173 Ryugu K. Wada1, K. Ishibashi1, H. Kimura1, M. Arakawa2, H. Sawada3, K. Ogawa2,4, K. Shirai2, R. Honda5, Y. Iijima3, T. Kadono6, N. Sakatani7, Y. Mimasu3, T. Toda3, Y. Shimaki3, S. Nakazawa3, H. Hayakawa3, T. Saiki3, Y. Takagi8, H. Imamura3, C. Okamoto2, M. Hayakawa3, N. Hirata9, and H. Yano3 1 Planetary Exploration Research Center, Chiba Institute of Technology, Narashino 275-0016, Japan e-mail: [email protected] 2 Department of Planetology, Kobe University, Kobe 657-8501, Japan 3 Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan 4 JAXA Space Exploration Center, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan 5 Department of Science and Technology, Kochi University, Kochi 780-8520, Japan 6 Department of Basic Sciences, University of Occupational and Environmental Health, Kitakyusyu 807-8555, Japan 7 Department of Physics, Rikkyo University, Tokyo 171-8501, Japan 8 Aichi Toho University, Nagoya 465-8515, Japan 9 School of Computer Science and Engineering, The University of Aizu, Aizu-Wakamatsu 965-8580, Japan Received 28 October 2020 / Accepted 26 January 2021 ABSTRACT A projectile accelerated by the Hayabusa2 Small Carry-on Impactor successfully produced an artificial impact crater with a final apparent diameter of 14:5 0:8 m on the surface of the near-Earth asteroid 162173 Ryugu on April 5, 2019. At the time of cratering, Deployable Camera 3 took± clear time-lapse images of the ejecta curtain, an assemblage of ejected particles forming a curtain-like structure emerging from the crater. -
+ New Horizons
Media Contacts NASA Headquarters Policy/Program Management Dwayne Brown New Horizons Nuclear Safety (202) 358-1726 [email protected] The Johns Hopkins University Mission Management Applied Physics Laboratory Spacecraft Operations Michael Buckley (240) 228-7536 or (443) 778-7536 [email protected] Southwest Research Institute Principal Investigator Institution Maria Martinez (210) 522-3305 [email protected] NASA Kennedy Space Center Launch Operations George Diller (321) 867-2468 [email protected] Lockheed Martin Space Systems Launch Vehicle Julie Andrews (321) 853-1567 [email protected] International Launch Services Launch Vehicle Fran Slimmer (571) 633-7462 [email protected] NEW HORIZONS Table of Contents Media Services Information ................................................................................................ 2 Quick Facts .............................................................................................................................. 3 Pluto at a Glance ...................................................................................................................... 5 Why Pluto and the Kuiper Belt? The Science of New Horizons ............................... 7 NASA’s New Frontiers Program ........................................................................................14 The Spacecraft ........................................................................................................................15 Science Payload ...............................................................................................................16 -
A Ballistics Analysis of the Deep Impact Ejecta Plume: Determining Comet Tempel 1’S Gravity, Mass, and Density
Icarus 190 (2007) 357–390 www.elsevier.com/locate/icarus A ballistics analysis of the Deep Impact ejecta plume: Determining Comet Tempel 1’s gravity, mass, and density James E. Richardson a,∗,H.JayMeloshb, Carey M. Lisse c, Brian Carcich d a Center for Radiophysics and Space Research, Cornell University, Ithaca, NY 14853, USA b Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721-0092, USA c Planetary Exploration Group, Space Department, Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA d Center for Radiophysics and Space Research, Cornell University, Ithaca, NY 14853, USA Received 31 March 2006; revised 8 August 2007 Available online 15 August 2007 Abstract − In July of 2005, the Deep Impact mission collided a 366 kg impactor with the nucleus of Comet 9P/Tempel 1, at a closing speed of 10.2 km s 1. In this work, we develop a first-order, three-dimensional, forward model of the ejecta plume behavior resulting from this cratering event, and then adjust the model parameters to match the flyby-spacecraft observations of the actual ejecta plume, image by image. This modeling exercise indicates Deep Impact to have been a reasonably “well-behaved” oblique impact, in which the impactor–spacecraft apparently struck a small, westward-facing slope of roughly 1/3–1/2 the size of the final crater produced (determined from initial ejecta plume geometry), and possessing an effective strength of not more than Y¯ = 1–10 kPa. The resulting ejecta plume followed well-established scaling relationships for cratering in a medium-to-high porosity target, consistent with a transient crater of not more than 85–140 m diameter, formed in not more than 250–550 s, for the case of Y¯ = 0 Pa (gravity-dominated cratering); and not less than 22–26 m diameter, formed in not less than 1–3 s, for the case of Y¯ = 10 kPa (strength-dominated cratering). -
Channel Lineup 3
International 469 ART (Arabic) MiVisión 818 Ecuavisa International 476 ITV Gold (South Asian) 780 FXX 821 Music Choice Pop Latino 477 TV Asia (South Asian) 781 FOX Deportes 822 Music Choice Mexicana 478 Zee TV (South Asian) 784 De Película Clasico 823 Music Choice Musica 479 Aapka COLORS 785 De Película Urbana 483 EROS NOW On Demand 786 Cine Mexicano 824 Music Choice Tropicales 485 itvn (Polish) 787 Cine Latino 825 Discovery Familia 486 TVN24 (Polish) 788 TR3s 826 Sorpresa 488 CCTV- 4 (Chinese) 789 Bandamax 827 Ultra Familia 489 CTI-Zhong Tian (Chinese) 790 Telehit 828 Disney XD en Español 497 MBC (Korean) 791 Ritmoson Latino 829 Boomerang en Español 498 TVK (Korean) 792 Latele Novela 830 Semillitas 504 TV JAPAN 793 FOX Life 831 Tele El Salvador 507 Rai Italia (Italian) 794 NBC Universo 832 TV Dominicana 515 TV5MONDE (French) 795 Discovery en Español 833 Pasiones 521 ANTENNA Satellite (Greek) 796 TV Chile MiVisión Plus 522 MEGA Cosmos (Greek) 797 TV Espanola Includes ALL MiVisión Lite 528 Channel One Russia 798 CNN en Español channels PLUS (Russian) 799 Nat Geo Mundo 805 ESPN Deportes 529 RTN (Russian) 800 History en Español 808 beIN SPORTS Español 530 RTVI (Russian) 801 Univision 820 Gran Cine 532 NTV America (Russian) 802 Telemundo 834 Viendo Movies 535 TFC (Filipino) 803 UniMas 536 GMA Pinoy TV (Filipino) 806 FOX Deportes 537 GMA Life TV (Filipino) 809 TBN Enlace 538 Myx TV (Pan Asian) 810 EWTN en Español 539 Filipino On Demand 813 CentroAmérica TV 540 RTPi (Portuguese) 815 WAPA America 541 TV Globo (Portuguese) 816 Telemicro Internacional 542 PFC (Portuguese) 817 Caracol TV = Available on RCN On Demand RCN On Demand With RCN On Demand get unlimited access to thousands of hours of popular content whenever you want - included FREE* with your Streaming TV subscription! We’ve added 5x the capacity to RCN On Demand, so you never have to miss a moment. -
EPOXI COMET ENCOUNTER FACT SHEET Nov
EPOXI COMET ENCOUNTER FACT SHEET Nov. 2, 2010 Quick Facts Flyby Spacecraft Dimensions: 3.3 meters (10.8 feet) long, 1.7 meters (5.6 feet) wide, and 2.3 meters (7.5 feet) high Weight: 601 kilograms (1,325 pounds) at launch, consisting of 517 kilograms (1,140 pounds) spacecraft and 84 kilograms (185 pounds) fuel. On 10/25/10 there was 4 kilograms (8.8 pounds) of fuel remaining. Power: 2.8-meter-by-2.8-meter (9-foot-by-9 foot) solar panel providing up to 750 watts, depending on distance from sun. Power storage via small, 16-amp- hourrechargeable nickel hydrogen battery Comet Hartley 2 Nucleus shape: Elongated Nucleus size (estimated): About 2.2 kilometers (1.4 miles) long Nucleus mass: Roughly 280 million metric tons Nucleus rotation period: About 18 hours Nucleus composition: Water ice, carbon dioxide ice, silicate dust Mission Launch: Jan. 12, 2005 Launch site: Cape Canaveral Air Force Station, Florida Launch vehicle: Delta II 7925 with Star 48 upper stage Impact with Tempel 1: 10:52 p.m. PDT July 3, 2005 (1:52 a.m. EDT July 4, 2005) Earth-comet distance at time of impact: 133.6 million kilometers (83 million miles) Total distance traveled by spacecraft from Earth to Tempel 1: 431 million kilometers (268 million miles) Flyby of Hartley 2: About 10 a.m. EDT or 7 a.m. PDT Nov. 4, 2010 Additional distance traveled by spacecraft to Hartley 2: About 4.6 billion kilometers (2.9 billion miles) Program Cost of Deep Impact: $267 million total (not including launch vehicle), consisting of $252 million spacecraft development and $15 million mission operations Cost of EPOXI extended mission: $42 million, for operations from 2007 to end of project at the end of fiscal year 2011.