Boeing 7. 77 - Wikipedia, la enciclopedia libre. El Boeing 7. 77 es un avi. Algunos de los rasgos m. El modelo 7. 77- 2. Las variantes de mayor alcance 7. ER y 7. 77- 2. 00. LR entraron en servicio en 2. Tanto las versiones de mayor alcance como la de carga incorporan motores General Electric GE9. El 7. 77- 2. 00. LR es el avi. Hasta junio de 2. Debido al aumento del coste del combustible, las aerol. Los competidores directos al 7. Airbus A3. 30- 3. Project Free tv, Watch Tv Shows on Project Free tv, Full episodes, Watch tv series online free, Projectfreetv online. Watch PAWG Perfection - Fat Ass PMV. Pornhub is the ultimate xxx porn and sex site. A3. 40, y el futuro A3. El siguiente desarrollo de Boeing, el 7. Dreamliner, tambi. En 1. 97. 8, Boeing desarroll. El 8 de diciembre de 1. Boeing comenz. El 7. X tuvo un fuselaje m. Para 1. 98. 8 Boeing se dio cuenta de que la . Por vez primera ocho de las principales l. Ya para marzo de 1. La nueva aeronave necesitaba la habilidad de volar tres rutas principales: Chicago a Hawaii, Chicago a Europa y sin escala desde el . El 1. 5 de octubre de 1. United Airlines se convirti. Divididos en 2. 40 equipos de dise. Todo fue creado con un sistema de dise. Todo esto hizo posible armar el 7. Fue tan exitoso que la totalidad de los prototipos contemplados fueron suspendidos. Entrada al servicio. En esta foto se le puede ver despegando. Boeing entreg. En junio de 1. Esos proveedores internacionales incluyen a Mitsubishi Heavy Industries y Kawasaki Heavy Industries (para los paneles de fuselaje), Fuji Heavy Industries, Ltd. Cashman, estrenando un programa de prueba de vuelo de 1. El 3. 0 de mayo, la Administraci. El desarrollo, las pruebas y la entrega del B7. El Avi. Los modernos motores con incidentes de fallo extremadamente bajos, (debido a la certificaci. La superficie alar se incrementaba desde los actuales 6. Entre los elementos del avi. La primera es el tama. El 7. 77- 2. 00 y sus derivados constituyen el tama. Para designar las variantes del 7. Por ejemplo, a un 7. ![]() ER se le designa como . Cualquier de estas designaciones se pueden ver en los manuales de los aeronaves o en los horarios de las l. El primero fue entregado a United Airlines el 1. Originalmente, fue conocido como el 7. IGW por su aumento de peso bruto. Es capaz de volar 9. Otros nuevos elementos incluyen las puntas de las alas m. El 7. 77- 2. 00. LR originalmente fue propuesto con la designaci. Con el avenimiento de motores de mayor potencia, el propuesto 7. X fue reemplazado por el programa 7. X, que luego evolucion. Fue registrado en el libro Guinness y excedi. Este aeronave no tiene una equivalente en la l. Otros nuevos elementos son: puntas de las alas reclinadas, un nuevo tren de aterrizaje, tanques de combustible nuevos (2. El programa 7. 77- 3. ER fue promovido por Air France, aunque por razones pol. ![]() El primer vuelo del 7. ER ocurri. La primera entrega a Air France ocurri. El equivalente directo de Airbus es el Airbus A3. El 7. 77- 3. 00. ER ha volado con un solo motor por seis horas, 2. Se requieren 1. 80 minutos de operaci. El alcance se aumenta si carga menos. Como ejemplo, el 7. F tiene la capacidad de hacer vuelos transpac. El propuesto A3. 50- 9. F ser. El MD- 1. 1F es otro avi. El 7. 47- 4. 00. ERF puede llevar m. En septiembre de 2. Boeing anunci. Desde julio de 2. Emirates es la compa. En el accidente hubo 4. Algunos pasajeros sufrieron heridas leves y la aeronave sufri. El fuselaje de la aeronave se incendi. Hasta casi ocho horas despu. A principios de agosto de 2. Isla de La Reuni. Consultado el 1. 8 de marzo de 2. Consultado el 1. 0 de abril de 2. Archivado desde el original el 2. Consultado el 1 de octubre de 2. Consultado el 1. 6 de abril de 2. The Atlanta Journal- Constitution. Archivado desde el original el 2. Consultado el 1. 6 de abril de 2. International Herald Tribune. Consultado el 1. 3 de abril de 2. Consultado el 1. 1 de abril de 2. Consultado el 1. 1 de abril de 2. A fresh and heartfelt new force in country music that feels like home and sounds like the truth. Cam’s country roots trace back to her grandparents ranch in. Lyrics to "Mayday" song by Cam: You are overbearing; I'm not in love But I don't wanna tell you We've been contemplating how to give. Holen Sie sich Informationen zu Busty Female Warrior Angel. Einige Fakten über Busty Female Warrior Angel. Busty Female Warrior Angel. Busty Female Warrior Angel.Consultado el 1. 4 de septiembre de 2. Archivado desde el original el 8 de julio de 2. Consultado el 2. 5 de mayo de 2. Consultado el 2. 5 de mayo de 2. Consultado el 4 de junio de 2. Consultado el 2. 6 de julio de 2. ![]() Consultado el 1. 0 de marzo de 2. Consultado el 2. 0 de marzo de 2. Air Transport Intelligence via Flightglobal. Consultado el 1. 3 de febrero de 2. Consultado el 9 de octubre de 2. Consultado el 1. 2 de noviembre de 2. Consultado el 2. 5 de agosto de 2. Consultado el 2. 0 de marzo de 2. Consultado el 1. 2 de noviembre de 2. Consultado el 1. 2 de noviembre de 2. Consultado el 1. 9 de marzo de 2. Consultado el 2. 0 de noviembre de 2. Consultado el 1 de julio de 2. Consultado el 1 de julio de 2. Aviation International News. Consultado el 1 de julio de 2. Retrieved: August 2. Aviation Week & Space Technology. Consultado el 1 de julio de 2. Consultado el 2. 5 de noviembre de 2. Consultado el 1. 9 de septiembre de 2. Boeing, September 1. Consultado el 3. 1 de octubre de 2. Puget Sound Business Journal (Seattle,Washington: American City Business Journals). Archivado desde el original el 1. Consultado el 1. 3 de noviembre de 2. These are on top of an existing order for 3. Boeing 7. 77. X jets from Lufthansa, providing a total launch order of 2. Consultado el 1. 7 de noviembre de 2. Aviation Week (Penton). Consultado el 1. 7 de noviembre de 2. Lufthansa Group (Deutsche Lufthansa AG). Consultado el 1. 7 de noviembre de 2. Boeing 7. 77- 9. Xs and 2. Airbus A3. 50- 9. Lufthansa Group's wide- body fleet.» . Archivado desde el original el 2. Consultado el 2. 7 de diciembre de 2. Consultado el 1. 4 de abril de 2. Consultado el 1. 4 de abril de 2. Consultado el 1. 4 de abril de 2. Archivado desde el original el 2. Consultado el 1. 4 de abril de 2. Civil Aviation Authority of New Zealand. Consultado el 1 de diciembre de 2. Archivado desde el original el 2. Consultado el 2 de abril de 2. Archivado desde el original el 2. Consultado el 2. 0 de abril de 2. Consultado el 2. 0 de abril de 2. Consultado el 2. 8 de abril de 2. Consultado el 2. 9 de abril de 2. Air. Transport. Biz. Consultado el 2. 3 de mayo de 2. Consultado el 2. 3 de mayo de 2. Archivado desde el original el 8 de diciembre de 2. Consultado el 2. 3 de mayo de 2. Consultado el 6 de junio de 2. Consultado el 6 de junio de 2. Consultado el 6 de junio de 2. Consultado el 6 de junio de 2. Consultado el 6 de junio de 2. Consultado el 2. 3 de mayo de 2. Consultado el 2. 3 de mayo de 2. Consultado el 2. 3 de mayo de 2. Consultado el 2. 3 de mayo de 2. Consultado el 1. 6 de abril de 2. Consultado el 2. 0 de julio de 2. Consultado el 1. 0 de enero de 2. Aviation Safety Network. Consultado el 1. 7 de julio de 2. Aviation Safety Network. Consultado el 5 de abril de 2. Aviation Safety Network. Consultado el 5 de abril de 2. Aviation Safety Network. Consultado el 2. 1 de noviembre de 2. National Transportation Safety Board. Consultado el 2 de enero de 2. Mayday, Discovery Channel. Regulatory News Service. Consultado el 2. 1 de noviembre de 2. Consultado el 9 de febrero de 2. Consultado el 2. 0 de marzo de 2. Consultado el 1. 1 de diciembre de 2. Aviation Safety Network. Consultado el 2 de enero de 2. Jet Airliner Crash Data Evaluation Centre. Consultado el 2 de enero de 2. Archivado desde el original el 2. Consultado el 9 de octubre de 2. Archivado desde el original el 2. Consultado el 2. 3 de mayo de 2. Boeing 7. 77, Jetliner for a New Century(en ingl. Paul, Minnesota: Motorbooks International. Cusick, Stephen; Rodrigues, Clarence C. Commercial Aviation Safety(en ingl. Nueva York: Mc. Graw- Hill Professional. Encyclopedia Of Aircraft(en ingl. Civil Aircraft Today: The World's Most Successful Commercial Aircraft(en ingl. Londres: Amber Books Ltd. Frawley, Gerard (2. The International Directory of Civil Aircraft 2. Londres: Aerospace Publications. Glenday, Craig (2. Guinness World Records(en ingl. Londres/Nueva Tork: Hi. T Entertainment. Norris, Guy; Wagner, Mark (1. Paul, Minnesota: Motorbooks International. Norris, Guy; Wagner, Mark (1. Modern Boeing Jetliners(en ingl. Minneapolis, Minnesota: Zenith Imprint. Norris, Guy; Wagner, Mark (2. Boeing 7. 77: The Technological Marvel(en ingl. Minneapolis, Minnesota: Zenith Imprint. Popular Science Magazine(en ingl. Inside Boeing: Building the 7. Minneapolis, Minnesota: Zeniyh Press.
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When SB 2. 77 went into effect, many parents with young children who were behind the vaccination schedule or did not start vaccinating yet, were forced to catch up or they could longer go to a public school. ![]() As a result, many children received a high amount of vaccines in a very short period of time. When it comes to toxins in vaccinations, the more vaccines are given at one time, the bigger the risk that a child will experience a severe adverse reaction. When we hear of a child left disabled or even dead after receiving vaccinations, it is often after receiving multiple vaccines at a time. One example occurred when five- month- old Matthew Gage Downing- Powers went to the doctor in October 2. His parents were told that he needed to catch up on his vaccinations, so he received 8 in one visit: DTa. P (3 in 1), Polio, Hib, Hep B, Pneumococcal PCV and the oral Rotavirus vaccine. He passed less than two daysafter the visit.“I don’t want Matthew to die in vain because of vaccine manufacturers not doing a better job making safer vaccines, before pushing them onto unsuspecting parents and their innocent babies they view as profitable beings,” his mom writes.
If you were still somehow hoping that the Doctor Who spinoff series Torchwood could return to TV, six years after it last aired, then we’ve got some news for you.Matthew’s case is no longer rare, with similar tragedies occurring in many families. Many children survive, but end up being disabled for life. For example, Ryan Mojabi’s family received monetary compensation ($9. Autism Spectrum Disorder following receiving scheduled vaccinations. According to his parents, “as a cumulative result of his receipt of each and every vaccination between March 2. February 2. 2, 2. Ryan has suffered . Unfortunately, parents are being left in the dark, and if recent history is any indication, they may be putting their children at risk as well. If California is serious about protecting the health of its children more than profits of the pharmaceutical industry, they should prove it by addressing these concerns before it’s too late. Ten things you don't know about black holes. Well, they’re black, and they’re like bottomless holes. What would you call them?- Me, when a friend asked me why they’re named what they are. Ah, black holes. The ultimate shiver- inducer of the cosmos, out- jawing sharks, out- ooking spiders, out- scaring. But we’re fascinated by ’em, have no doubt — even if we don’t understand a whole lot about them. But then, that’s why I’m here. Allow me to be your tour guide to infinity. Or the inverse of it, I suppose. Since it’s Halloween this seems appropriate! Mwuhahahaha. So below I present ten facts about black holes — the third in my series of Ten Things You Don’t Know (the first was on the Milky Way; the second about the Earth). Regular readers will know a few of these since I’ve talked about them before, but I’m hoping you don’t know all of these. And if you do, then feel free to leave a comment preening about your superior intellect. Mind you, this list is nowhere near complete: I could have picked probably 5. But I like these. ![]() It’s not their mass, it’s their size that makes them so strong. OK, first, a really quick primer on black holes. Bear with me! The most common way for a black hole to form is in the core of a massive star. ![]() The core runs out of fuel, and collapses. This sets off a shockwave, blowing up outer layers of the star, causing a supernova. So the star’s heart collapses while the rest of it explodes outwards (this is the Cliff’s notes version; for more details on the process — which is way cool, so you should read it — check out my description of it). As the core collapses, its gravity increases. At some point, if the core is massive enough (about 3 times the mass of the Sun), the gravity gets so strong that right at the surface of the collapsing core the escape velocity increases to the speed of light. That means that nothing can escape the gravity of this object, not even light. And since nothing can escape, well, read the quotation at the top of the page. The region around the black hole itself where the escape velocity equals the speed of light is called the event horizon. Any event that happens inside it is forever invisible. OK, so now you know what one is, and how they form. Now, I could explain why they have such strong gravity, but you know what? I’d rather let this guy do it. I hear he’s good. So there you go. Sure, the mass is important, but sometimes it’s the little things that count. They’re not infinitely small. So OK, they’re small, but how small are they? I was writing about black holes in my previous job, and we got in a fun discussion over just what we meant by black hole: did we mean the object itself that collapses down to a mathematical point, or the event horizon surrounding it? I said the event horizon, but my boss said it was the object. I decided she had a point (HAHAHAHAHA! Man, I kill me), and made sure that when I wrote about the event horizon versus the black hole itself I was making myself clear. Like I said above, to the collapsing core, its clock keeps ticking, so it sees itself collapsing all the way down to a point, even if the event horizon has some finite size. What happens to the core? The actual mass that collapsed? Out here, we’ll never know for sure. We can’t see in, and it sure enough isn’t gonna send any info out. But our math in these situations is pretty good, and we can at least apply them to the collapsing core, even when it’s smaller than the event horizon. It will continue to collapse, and the gravity increases. That really bugged me, as you can imagine. Because it’s wrong. At some point, the collapsing core will be smaller than an atom, smaller than a nucleus, smaller than an electron. A Planck Length is a kind of quantum size limit: if an object gets smaller than this, we literally cannot know much about it with any certainty. The actual physics is complicated, but pretty much when the collapsing core hits this size, even if we could somehow pierce the event horizon, we couldn’t measure its real size. If the Universe itself prevents you from measuring it, you might as well say the term has no meaning. And how small is a Planck Length? Teeny tiny: about 1. That’s one one- hundred quintillionth the size of a proton. So if someone says a black hole has zero size, you can be all geeky and technical and say, not really, but meh. Close enough. 3) They’re spheres. And they’re definitely not funnel shaped. The gravity you feel from an object depends on two things: the object’s mass, and your distance from that object. This means that anyone at a given distance from a massive object — say, a million kilometers — would feel the same force of gravity from it. That distance defines a sphere around an object: anyone on that sphere’s surface would feel the same gravity from the object at the center. The size of an event horizon of a black hole depends on the gravity, so really the event horizon is a sphere surrounding the black hole. From the outside, if you could figure out how to see the event horizon in the first place, it would look like a pitch black sphere. Some people think of black holes as being circles, or worse, funnel- shaped. The funnel thing is a misconception from people trying to explain gravity as a bending in space, and they simplify things by collapsing 3. D space into 2. D; they say the space is like a bed sheet, and objects with mass bend space the same way that a massive object (a bowling ball, say) will warp a bed sheet. But space is not 2. D, it’s 3. D (even 4. D if you include time) and so this explanation can confuse people about the actual shape of a black hole event horizon. I’ve had kids ask me what happens if you approach a black hole from underneath! They sometimes don’t get that black holes are spheres, and there is no underneath. I blame the funnel story. Sadly, it’s the best analogy I’ve seen, so we’re stuck with it. Use it with care. Black holes spin! It’s kind of an odd thought, but black holes can spin. Stars rotate, and when the core collapses the rotation speeds way, way up (the usual analogy is that of an ice skater who brings in his arms, increasing his rotation rate). As the core of the star gets smaller it rotates more rapidly. If it doesn’t quite have enough mass to become a black hole, the matter gets squeezed together to form a neutron star, a ball of neutrons a few kilometers across. We have detected hundreds of these objects, and they tend to spin very rapidly, sometimes hundreds of times a second! The same is true for a black hole. Even as the matter shrinks down smaller than the event horizon and is lost to the outside Universe forever, the matter is still spinning. It’s not entirely clear what this means if you’re trying to calculate what happens to the matter once it’s inside the event horizon. Does centrifugal force keep it from collapsing all the way down to the Planck length? The math is fiendish, but do- able, and implies that matter falling in will hit matter inside the event horizon trying to fall further but unable to due to rotation, This causes a massive pile up and some pretty spectacular fireworks. Bummer. 5) Near a black hole, things get weird. The spin of the black hole throws a monkey in the wrench of the event horizon. Black holes distort the fabric of space itself, and if they spin that distortion itself gets distorted. Space can get wrapped around a black hole — kind of like the fabric of a sheet getting caught up in a rotating drill bit. This creates a region of space outside the event horizon called the ergosphere. It’s an oblate spheroid, a flattened ball shape, and if you’re outside the event horizon but inside the ergosphere, you’ll find you can’t sit still. Space is being dragged past you, and carries you along with it. You can easily move in the direction of the rotation of the black hole, but if you try to hover, you can’t. In fact, inside the ergosphere space is moving faster than light! Matter cannot move that fast, but it turns out, according to Einstein, space itself can. So if you want to hover over a black hole, you’d have to move faster than light in the direction opposite the spin. You can’t do that, so you have to move with the spin, fly away, or fall in. Those are your choices. I suggest flying away. And by fun, I mean gruesome, horrifying, and really really ookie. Sure, if you get too close, plop! But even if you keep your distance you’re still in trouble. The farther you are from an object, the weaker its gravity. So if you have a long object near a massive one, the long object will feel a stronger gravitational force on the near end versus a weaker force on the far end! This change in gravity over distance is called the tidal force (which is a bit of a misnomer, it’s not really a force, it’s a differential force, and yes, it’s related to why we have ocean tides on Earth from the Moon). The thing is, black holes can be small — a BH with a mass of about three times the Sun has an event horizon just a few kilometers across — and that means you can get close to them. And that in turn means that the tidal force you feel from one can get distressingly big. Let’s say you fall feet first into a stellar- mass BH. It turns out that as you approach, the difference in gravity between your head and your feet can get huge. The force can be so strong that your feet get yanked away from your head with hundreds of millions of times the force of Earth’s gravity. You’d be stretched into a long, thin strand and then shredded. Astronomers call this spaghettification. Ewwww. So getting near a black hole is dangerous even if you don’t fall in. Evidently, there really is a tide in the affairs of men. Black holes aren’t always dark. The thing is, black holes can kill from a long way off. Matter falling into a black hole would rarely if ever just fall straight in and disappear. If it has a little bit of sideways motion it’ll go around the black hole. As more matter falls in, all this junk can pile up around the hole. Muse - Dig Down. Check out the official video. The Museum Of Ice Cream
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