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sábado, 9 de fevereiro de 2013

3933 Portugal é nome de asteróide

O asteróide 3933 Portugal (1986 EN4) foi descoberto em 12 de Março de 1986 pelo astrónomo dinamarquês Richard Martin West, no Observatório La Silla (ESO), no Chile.

É um pequeno corpo celeste, irregular e de cor escura, planetóide (troiano), proveniente da cintura principal externa de asteróides, tem cerca de 10 km de diâmetro, orbita o sol entre Marte e Júpiter, a 485 milhões de km do Sol (cerca de três vezes mais afastado do que a Terra), com uma órbita quase circular de 5,9 anos (2.137 dias) em torno da nossa estrela. Apresenta uma órbita caracterizada por um semi-eixo maior de 3,2479002 UA e com uma exentricidade de 0,0967363, inclinada de 1,70434° relativamente à elíptica.

Foi chamado Portugal em 1990 para comemorar a adesão de Portugal à organização astronómica do Observatório Europeu do Sul (ESO).

Segundo o Jet Propulsion Laboratory, do Instituto de Tecnologia da Califórnia, da NASA, este asteróide foi avistado pela primeira vez em 1953 e pela última vez a 7 de Janeiro de 2013. Os astrónomos amadores Alberto Fernando, José Ribeiro, e Filipe Alves conseguiram captar imagens de 3933 Portugal em 2004, e em 2009 foi a vez de João Gregório também conseguir fazer fotos ao asteróide.

Mais informações em http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=3933


quinta-feira, 1 de novembro de 2012

Quantum leap

Que fique registado para o futuro: Assim que ouvi falar de informática quântica, soube instintivamente que era a resposta para a viagem intergalática à escala humana.

Se eu estiver errado, paciência. Mas se estiver certo, estamos apenas a algumas décadas de viajarmos mais rapidamente que a luz.

A teoria quântica da acção-fantasma das partículas elementares é o nos conduzirá às viagens inter-galáxias (graças à energia quântica) como inter-dimensões (graças ao imbricamento quântico)..

terça-feira, 16 de outubro de 2012

Um planeta iluminado por 4 sóis


Uma equipa internacional de astrónomos amadores (Planet Hunters) e profissionais (Universidade de Yale) anunciou hoje a descoberta de um planeta num sistema binário duplo (ou quaternário).

Quem desse planeta pudesse observar os céus, veria quatro sóis. Apesar de popularizado em muitas obras de ficção científica, é a primeira vez que um sistema estelar deste tipo é observado.

O planeta, baptizado PH1 (Planet Hunters 1), é seis vezes maior do que a Terra e fica situado a mais de cinco mil anos-luz da Terra. O PH1 orbita em torno de dois sóis, em volta dos quais também evoluem duas estrelas. Até hoje, os astrónomos descobriram apenas 6 planetas que orbitam em sistemas binários e nunca em sistemas binários duplos.

Este sistema estelar binário duplo foi descoberto por dois astrónomos amadores dos EUA, Kian Jek e Robert Gagliano, através do programa Planet Hunters. Este programa reagrupa num site os astrónomos amadores, incentivando-os a descobrirem e identificarem exoplanetas (planetas fora do nosso sistema solar), utilizando os dados recolhidos pelo telescópio espacial Kepler.

Astrónomos profissionais norte-americanos e britânicos efectuaram depois observações e medidas com os telescópios Keck situados no monte Mauna Kea, no Havai. "Os planetas binários representam o que há de mais extremo na formação planetária", diz Meg Schwamb, um investigador da Universidade de Yale, no Estado do Connecticut, principal autor da pesquisa, apresentada hoje na conferência anual da Divisão de Planetologia da Sociedade Americana de Astronomia, reunida em Reno, no Nevada (EUA). "A descoberta de tais sistemas satelitários força-nos a repensar como estes planetas se podem formar e evoluir em tais ambientes", frisou.

Lusa/AFP/Yale

Um mergulho no vazio dos 39 mil metros



O pára-quedista austríaco Felix Baumgartner tornou-se no domingo, 14 de Outubro de 2012, o primeiro homem a saltar em queda livre dos 39 mil metros de altitude, ultrapassando a barreira do som. Durante o salto, o austríaco, de 43 anos, atingiu a velocidade máxima de 1341,9 km/h, ultrapassando 1,24 vezes a barreira do som. Com este salto supersónico , bateu também o recorde do salto mais alto de sempre, pulverizando o recorde estabelecido em 1960 por Joseph Kittinger, que tinha saltado dos 31 mil metros. Kittinger foi, 52 anos depois e hoje com 83 anos, o contacto rádio na Terra durante o salto de Felix. O austríaco saltou de uma cápsula levada por um balão à estratosfera, numa subida que levou 2h30min. Depois, abriu a escotilha e saltou. Um mergulho no vazio que demorou cerca de 10 minutos, dos quais 4m20s em queda livre, sobre Roswell e o deserto do Novo México, nos EUA. O austríaco abriu finalmente o seu pára-quedas a 1.500 metros do solo. Ileso e já em terra firme, Felix afirmou querer “inspirar a próxima geração” com este feito. Mais de oito milhões de pessoas viram o salto pelo Youtube, onde a proeza foi transmitida em directo na página da Red Bull, que patrocinou o projecto.    

sábado, 25 de agosto de 2012

Morreu Neil Armstrong, o primeiro homem a pisar a Lua


O astronauta norte-americano Neil Armstrong, o primeiro homem que caminhou na Lua, morreu hoje aos 82 anos, anunciou a cadeia de televisão americana NBC News.

Neil Armstrong tinha sido operado ao coração a 7 de Agosto. 

O astronauta Neil Armstrong e o seu companheiro da Apollo 11, Buzz Aldrin, foram os primeiros homens a caminhar na superfície lunar, a 20 de Julho de 1969. 

Armstrong nasceu em 1930 e foi astronauta, piloto de testes e aviador naval. Antes de se tornar astronauta, estava na Marinha dos Estados Unidos e serviu na Guerra da Coreia. Após a guerra, serviu como piloto de testes na Estação de Voo do Comitê Consultivo Nacional para a Aeronáutica (NACA) de alta velocidade.

Armstrong interessou-se pela NASA cinco ou seis meses depois da abertura das inscrições para a formação de um novo grupo de astronautas, em 1962, e foi escolhido para o chamado Grupo dos Nove, denominação decorrente do modo como eram conhecidos os primeiros astronautas norte-americanos seleccionados em 1960 para o Projeto Mercury, o Grupo dos Sete, tornando-se o primeiro astronauta norte-americano civil.

Toda a saga de Armstrong, Aldrin, Michael Collins e do voo pioneiro está contada na história da missão Apollo 11. A sua frase épica, "Este é um pequeno passo para o homem, um salto gigantesco para a Humanidade" ao pisar pela primeira vez a superfície lunar, é uma das mais conhecidas na História, mas só veio à cabeça de Neil poucos momentos antes de descer da nave, já pousado na Lua, pelo menos é o que reza a lenda.

Além de algumas experiências científicas que ali fizeram, Armstring e o piloto do Módulo Lunar, "Buzz" Aldrin, plantaram no Mar da Tranqüilidade uma bandeira dos Estados Unidos e colocaram uma placa junto ao Módulo Lunar Eagle, assinada pelos astronautas e pelo presidente americano Richard Nixon: "Aqui os homens do planeta Terra puseram pela primeira vez os pés na Lua, em 20 de Julho de 1969. Viemos em paz em nome de toda a Humanidade".

Após a cirurgia ao coração no início de Agosto, para desobstrução das artérias, encontrava-se a recuperar no Hospital de Cincinnati, cidade onde morava com a esposa. Mas Armstrong não resistiu às intervenções e acabou por falecer em Columbus, no estado de Ohio.

(Lusa/Wikipedia)

domingo, 22 de abril de 2012

WARP DRIVE EXPLAINED BY MEXICAN PHYSICIAN MIGUEL ALCUBIERRE AS MATHEMATHICALLY POSSIBLE

Alcubierre drive


Concept of the Alcubierre drive, showing the opposing regions of expanding and contracting spacetime that propel the central region
 
The Alcubierre drive (or Alcubierre metric / Metric tensor) is a speculative idea based on a valid solution of the Einstein field equations as proposed by Miguel Alcubierre by which a spacecraft might be accelerated to speeds greater than the speed of light in order to achieve the objective of interstellar flight.

History

In 1994 Alcubierre proposed a way of changing the geometry of space by creating a wave which would cause the fabric of space ahead of a spacecraft to contract and the space behind it to expand The ship would then ride this wave inside a region of flat space known as a warp bubble, and would not move within this bubble, but instead be carried along as the region itself moves as a consequence of the actions of the drive. If this is so, conventional relativistic effects such as time dilation would not apply in the way they would in the case of a ship moving at a very great velocity through flat spacetime, relative to other objects. This method of propulsion would not involve objects in motion at speeds faster than light with respect to the contents of the warp-bubble; that is, a light beam within the warp-bubble would still always move faster than the ship. Thus the mathematical formulation of the Alcubierre metric does not contradict the conventional claim that the laws of relativity do not allow a slower-than-light object to accelerate to faster-than-light speeds. The Alcubierre drive, however, remains a hypothetical concept with seemingly insuperable problems: The amount of energy required is unobtainably large, there is no method to create a warp bubble in a region that does not already contain one, and there is no method to move from the warp-bubble once having arrived at a supposed destination.

Alcubierre metric

The Alcubierre metric defines the warp drive spacetime. This is a Lorentzian manifold which, if interpreted in the context of general relativity, allows a warp bubble to appear in previously flat spacetime and move off at effectively superluminal speed. Inhabitants of the bubble feel no inertial effects. The object(s) within the bubble are not moving (locally) faster than light, instead, the space around them shifts so that the object(s) arrives at its destination faster than light would in normal space.
Alcubierre chose a specific form for the function f, but other choices give a simpler spacetime exhibiting the desired "warp drive" effects more clearly and simply.

Mathematics of the Alcubierre drive

Using the ADM formalism of general relativity, the spacetime is described by a foliation of space-like hypersurfaces of constant coordinate time t. The general form of the metric described within the context of this formalism is:
ds^2 = -\left(\alpha^2- \beta_i \beta^i\right)\,dt^2+2 \beta_i \,dx^i\, dt+ \gamma_{ij}\,dx^i\,dx^j
where
\alpha is the lapse function that gives the interval of proper time between nearby hypersurfaces,
\beta^i is the shift vector that relates the spatial coordinate systems on different hypersurfaces
\gamma_{ij} is a positive definite metric on each of the hypersurfaces.

The particular form that Alcubierre studied is defined by:
\alpha=1\,
\beta^x=-v_s(t)f\left(r_s(t)\right),
\beta^y = \beta^z =0 \,\!
\gamma_{ij}=\delta_{ij} \,\!

where

v_s(t)=\frac{dx_s(t)}{dt},

r_s(t)=\sqrt{(x-x_s(t))^2+y^2+z^2}

and

f(r_s)=\frac{\tanh(\sigma (r_s + R))-\tanh(\sigma (r_s - R))}{2 \tanh(\sigma R)}

with R > 0 and \sigma > 0 arbitrary parameters. Alcubierre's specific form of the metric can thus be written;

ds^2 =  \left(v_s(t)^2 f(r_s(t))^2 -1\right)\,dt^2 - 2v_s(t)f(r_s(t))\,dx\,dt +dx^2 + dy^2 + dz^2

With this particular form of the metric, it can be shown that the energy density measured by observers whose 4-velocity is normal to the hypersurfaces is given by

-\frac{c^4}{8 \pi G} \frac{v_s^2 (y^2+z^2)}{4 g^2 r_s ^2} \left(\frac{df}{dr_s}\right)^2


where  g\! is the determinant of the metric tensor.
Thus, as the energy density is negative, one needs exotic matter to travel faster than the speed of light. The existence of exotic matter is not theoretically ruled out; however, generating enough exotic matter and sustaining it to perform feats such as faster-than-light travel (and also to keep open the 'throat' of a wormhole) is thought to be impractical. Low has argued that within the context of general relativity, it is impossible to construct a warp drive in the absence of exotic matter.It is generally believed that a consistent theory of quantum gravity will resolve such issues once and for all.

Physics of the Alcubierre drive

For those familiar with the effects of special relativity, such as Lorentz contraction and time dilation, the Alcubierre metric has some apparently peculiar aspects. In particular, Alcubierre has shown that even when the ship is accelerating, it travels on a free-fall geodesic. In other words, a ship using the warp to accelerate and decelerate is always in free fall, and the crew would experience no accelerational g-forces. Enormous tidal forces would be present near the edges of the flat-space volume because of the large space curvature there, but by suitable specification of the metric, these would be made very small within the volume occupied by the ship.
The original warp drive metric, and simple variants of it, happen to have the ADM form which is often used in discussing the initial-value formulation of general relativity. This may explain the widespread misconception that this spacetime is a solution of the field equation of general relativity. Metrics in ADM form are adapted to a certain family of inertial observers, but these observers are not really physically distinguished from other such families. Alcubierre interpreted his "warp bubble" in terms of a contraction of "space" ahead of the bubble and an expansion behind. But this interpretation might be misleading, since the contraction and expansion actually refers to the relative motion of nearby members of the family of ADM observers.
In general relativity, one often first specifies a plausible distribution of matter and energy, and then finds the geometry of the spacetime associated with it; but it is also possible to run the Einstein field equations in the other direction, first specifying a metric and then finding the energy-momentum tensor associated with it, and this is what Alcubierre did in building his metric. This practice means that the solution can violate various energy conditions and require exotic matter. The need for exotic matter leads to questions about whether it is actually possible to find a way to distribute the matter in an initial spacetime which lacks a "warp bubble" in such a way that the bubble will be created at a later time. Yet another problem is that, according to Serguei Krasnikov, it would be impossible to generate the bubble without being able to force the exotic matter to move at locally FTL speeds, which would require the existence of tachyons. Some methods have been suggested which would avoid the problem of tachyonic motion, but would probably generate a naked singularity at the front of the bubble.

Difficulties

Significant problems with the metric of this form stem from the fact that all known warp drive spacetimes violate various energy conditions. It is true that certain experimentally verified quantum phenomena, such as the Casimir effect, when described in the context of the quantum field theories, lead to stress-energy tensors which also violate the energy conditions, such as negative mass-energy, and thus one can hope that Alcubierre-type warp drives can be physically realized by clever engineering taking advantage of such quantum effects. However, if certain quantum inequalities conjectured by Ford and Roman hold, then the energy requirements for some warp drives may be absurdly gigantic, e.g. the energy equivalent of -1067 grams might be required to transport a small spaceship across the Milky Way galaxy. This is orders of magnitude greater than the estimated mass of the universe. Counter-arguments to these apparent problems have also been offered.
Chris Van Den Broeck, in 1999, has tried to address the potential issues. By contracting the 3+1 dimensional surface area of the 'bubble' being transported by the drive, while at the same time expanding the 3 dimensional volume contained inside, Van Den Broeck was able to reduce the total energy needed to transport small atoms to less than 3 solar masses. Later, by slightly modifying the Van Den Broeck metric, Krasnikov reduced the necessary total amount of negative energy to a few milligrams.
Krasnikov proposed that, if tachyonic matter cannot be found or used, then a solution might be to arrange for masses along the path of the vessel to be set in motion in such a way that the required field was produced. But in this case, the Alcubierre Drive vessel is not able to go dashing around the galaxy at will. It is only able to travel routes which, like a railroad, have first been equipped with the necessary infrastructure. The pilot inside the bubble is causally disconnected with its walls and cannot carry out any action outside the bubble. Thus, because the pilot cannot place infrastructure ahead of the bubble while "in transit", the bubble cannot be used for the first trip to a distant star. In other words, to travel to Vega (which is 25 light-years from the Earth) one first has to arrange everything so that the bubble moving toward Vega with a superluminal velocity would appear and these arrangements will always take more than 25 years.
Coule has argued that schemes such as the one proposed by Alcubierre are infeasible as matter placed en route of the intended path of a craft has to be placed at superluminal speed. Thus, according to Coule, an Alcubierre Drive is required in order to build an Alcubierre Drive. Since none have been proven to exist already then the drive is impossible to construct, even if the metric is physically meaningful. Coule argues that an analogous objection will apply to any proposed method of constructing an Alcubierre Drive.
A paper by José Natário published in 2002 argued that it would be impossible for the ship to send signals to the front of the bubble, meaning that crew members could not control, steer or stop the ship.
A more recent paper by Carlos Barceló, Stefano Finazzi, and Stefano Liberati makes use of quantum theory to argue that the Alcubierre Drive at FTL velocities is impossible; mostly due to extremely high temperatures caused by Hawking radiation destroying anything inside the bubble at superluminal velocities and leading to instability of the bubble itself. These problems do not arise if the bubble velocity is kept subluminal, but it is still necessary to provide exotic matter for the drive to work.
More difficulties emerge in regards to the amount of exotic matter required for such a propulsion. According to Pfenning and Allen Everett of Tufts, a warp bubble traveling at 10 times light-speed must have a wall thickness of no more than 10−32 meters. This is only slightly longer than the Planck length, 10−35. A bubble macroscopically large enough to enclose a ship 200 meters across would require a total amount of exotic matter equal to 10 billion times the mass of the observable universe. Straining the exotic matter to an extremely thin band of 10−32 meters is considered impractical. Similar constraints apply to Krasnikov's superluminal subway. A modification of Alcubierre's model was recently constructed by Chris van den Broeck of the Catholic University of Louvain in Belgium. It requires much less exotic matter but places the ship in a curved space-time "bottle" whose neck is about 10−32 meters. So-called cosmic strings, hypothesized in some cosmological theories, involve very large energy densities in long, narrow lines. But[clarification needed] all known physically reasonable cosmic-string models have positive (positive space-time warping effects) energy densities. These results seem to make it rather unlikely that one could construct Alcubierre warp drives using exotic matter generated by quantum effects.

The Alcubierre drive and science fiction

Faster-than-light travel is often used in science fiction to denote a wide variety of imaginary propulsion methods, most of which have nothing to do with the Alcubierre drive or any other physical theory. Some science-fiction works, particularly of the 'hard' genre, have explicitly made use of the Alcubierre theory, such as Stephen Baxter's novel Ark.
The Alcubierre drive theory is proposed as a possible reason for events occurring in the graphic novel "Orbiter" by Warren Ellis and Colleen Doran.
The Ian Douglas "Star Carrier" series exclusively uses the Alcubierre drive as the main mode of interstellar travel.
Also, in M. John Harrison's novel Light, the character Ed Chianese, while trying to get a job with the Circus of Pathet Lao, claims that he "rode navigator on Alcubierre ships."


From Wikipedia, the free encyclopedia