CONTRA EL PINGALISMO CASTRISTA/ "Se que no existe el consuelo que no existe la anhelada tierrra de mis suenos ni la desgarrada vision de nuestros heroes. Pero te seguimos buscando, patria,..." - Reinaldo Arenas

Mostrando entradas con la etiqueta Astronomia. Mostrar todas las entradas
Mostrando entradas con la etiqueta Astronomia. Mostrar todas las entradas

jueves, julio 10, 2014

Supernova Reveals Origins of Universe's Dust

supernova SN 2010
The supernova SN 2010jl (large white spot near top) produced dust much larger than usually found in the Milky Way. X-ray: NASA/CXC/RCA CA/P.Chandra et al); Optical: NASA/STScI
Cosmic dust is crucial to the birth of stars and rocky planets, and provides the elemental ingredients for life. But its origin is obscure. Many astrophysicists think that dust is forged during the explosive supernova deaths of massive, short-lived stars, yet some observations of supernovas near our galaxy indicate that they produce too little material to account for the copious amounts of dust present in the young Universe.
In Nature today, astronomers lift the veil on the mystery, documenting the formation of dust in a supernova from just a few weeks after the explosion to almost 2.5 years after it. The study reveals the formation of oversized dust grains that were able to withstand the shocks of the exploding star. It also shows that dust production was slow at first, but later sped up.
Most previous studies looked at each supernova for short periods of time, so “they did not tell us the full story of how much dust supernovas produce”, says co-author Christa Gall, an astrophysicist at Aarhus University in Denmark. She and her colleagues monitored the supernova SN 2010jl, first spotted in a nearby galaxy in 2010.
Light and heat
Using a spectrograph on the Very Large Telescope on Cerro Paranal in Chile, the team measured the amount of visible light absorbed by the dust particles and the infrared radiation that the particles themselves emitted.  
The team's data are particularly compelling because they provide this simultaneous coverage at a range of wavelengths from weeks to years after the explosion, says astronomer Rubina Kotak of Queen’s University Belfast, UK. This provides information about both the size and the composition of the grains.
Such coverage “is difficult to obtain for all but the nearest and brightest supernova events”, she says.
The team concluded that the dust present between 40 and 240 days after the explosion must have been made of material expelled before the star went supernova, because the only other possibility would be the debris hurled into interstellar space by the supernova itself. And this is too hot to condense into dust particles so soon after the explosion, Gall notes. As the expanding shock wave from the supernova swept by in this period after the explosion, it compressed the previously ejected material into a cold, dense shell — the perfect environment for dust to coalesce and grow.
Resistant to shockwaves
To their surprise, the astronomers found that the dust particles were enormous by Milky Way standards, measuring 1 to 4.2 micrometers across — at least four times the typical width of dust particles found between star systems in our home Galaxy. It is harder to form large dust particles, notes Gall, but their size makes them resistant to destruction by shocks associated with the supernova slamming into interstellar material, and probably accounts for their longevity. Large interstellar dust grains have previously been found in our Solar System.
During early observations, the amount of dust around SN 2010jl was relatively small, equivalent to less than one-ten-thousandth the mass of the Sun. But between 500 and 868 days after the explosion, dust formation accelerated and the dust mass increased more than 10-fold.
The revved-up rate marks a transition to a second phase in supernova dust production, says Gall. Once carbon-rich material and other debris generated during the supernova has cooled sufficiently, it begins to coalesce into dust, speeding up production. At day 868, the last time Gall’s team observed the supernova, the amount of dust had increased to 0.04 of the Sun’s mass, or 830 Earth masses.
If the increased dust production continues, in 20 years SN 2010jl will have produced the equivalent of half the Sun’s mass in dust particles, similar to the amount observed in the widely observed supernova SN 1987A. If numerous supernovae early in the Universe produced dust at a similar rate, it could indeed account for the dust observed in the young cosmos, says Gall.

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miércoles, junio 25, 2014

Mysterious signal detected in galaxy 240 million light years away from earth

ITN 
Astronomers have detected a mysterious signal 240 million light years away from Earth. The unidentified signal is a 'spike of intensity at a very specific wavelength of x-ray light', but scientists don't yet know what the origin is. Picked up in the Perseus Cluster, one of the biggest objects in the universe, the discovery is said to be the best evidence of dark matter yet. Astronomers believe dark matter constitutes 85 per cent of the matter in the universe, but doesn't emit or absorb light like normal matter such as protons or electrons, which are known to make up the familiar elements seen in planets, stars, and galaxies. Researchers suggest intensity coming from the Perseus Cluster could be a signature from the decay of a 'sterile neutrino' - which are a hypothetical type of neutrino thought to interact with normal matter via gravity. But while holding exciting potential, the results must be confirmed with additional data to rule out ... (More

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viernes, junio 06, 2014

Huge asteroid named 'Beast' to fly by Earth on Sunday

Visit NBCNews.com for breaking news, world news, and news about the economy

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jueves, abril 03, 2014

Already Being Built Spacecraft To Capture Asteroids and Missions To Moon and Mars

Mary Greeley


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domingo, marzo 23, 2014

A Celebration of Carl Sagan

LibraryOfCongress
Librarian of Congress James H. Billington was joined by Emmy Award-winner Seth MacFarlane and Ann Druyan, the longtime collaborator and widow of astrobiologist Carl Sagan, to celebrate the official opening of the Seth MacFarlane Collection of the Carl Sagan and Ann Druyan Archive to the public at the Library of Congress. 


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jueves, marzo 20, 2014

Scientists Say Destructive Solar Blasts Narrowly Missed Earth in 2012

Mary Greeley

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lunes, marzo 17, 2014

'Smoking Gun' Reveals How the Inflationary Big Bang Happened

Read on NBC News >>
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martes, enero 28, 2014

Moon Has UFO Sighting Same Time China's Jade Rabbit Rover Malfunctions

Mary Greeley

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Este gráfico te dice a qué velocidad te estás moviendo debido a la rotación de la Tierra

microsiervos

Vizual Statistix / Seth Kadish.
Dependiendo de en qué parte del planeta se encuentre uno el movimiento circular debido a la rotación de la Tierra sobre su eje es mayor o menor. En el ecuador esta velocidad es de unos 1600 km/h y en cambio cerca de en los polos la velocidad del movimiento circular se reduce y llega a ser cero, ninguno. Aquí en España estamos girando a unos 1300 km/h según este gráfico de Vizual Statistix.
Lo anterior sin contar la velocidad con la que la Tierra se mueve alrededor del Sol ni la velocidad con la que el Sol se desplaza por el espacio.
# Enlace Permanente
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viernes, enero 17, 2014

Stunning photos of the Earth from the Moon: China's lunar probe Chang'e-3 takes pictures of globe

ITN


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jueves, enero 09, 2014

The Sights And Sounds Of The Solar System

TIME

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NASA space telescope spots new asteroid


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sábado, diciembre 14, 2013

China successfully soft lands probe on the moon


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martes, diciembre 03, 2013

Seis mundos, seis horizontes, seis superficies

Distant Horizons - Different Surfaces es una composición hecha por Mike Malaska en la que se ven las superficies de cinco mundos que hemos visitado, además del nuestro.
De izquierda a derecha son el asteroide Itokawa, visitado por la sonda Hayabusa, la Luna, en una imagen de la misión Apolo 17, la última en la que dos seres humanos pisaron su superficie, Venus, en una imagen de la sonda Venera 14, Marte por Spirit, Titán visto por la Huygens, y la Tierra, aunque lo que salga es el mar, ya que cubre el 71 por ciento de su superficie.
Los créditos de la imagen son:
Itokawa: ISAS / JAXA / Gordan Ugarkovic
Luna: NASA
Venus: IKI / Don Mitchell / Ted Stryk / Mike Malaska
Marte: NASA / JPL / Cornell / Mike Malaska
Titán: ESA / NASA / JPL / University of Arizona
Tierra: Mike Malaska
(Vía @Tokaidin y @LuisMendoTomas; localicé el origen vía Zemiorka).

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miércoles, octubre 16, 2013

Huge Russian meteorite breaks after it's pulled out of lake

 
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sábado, octubre 12, 2013

Meet the asteroid that might hit Earth in 2880

Radar image of 1950 DA acquired by the Arecibo Observatory on March 4, 2001. (NASA/JPL/S. Ostro)
By Jason Majors/
There are over 10,000 near-Earth objects (NEOs) that have been identified so far — asteroids and comets of varying sizes that approach the Earth’s orbital distance to within about 28 million miles. Of the 10,000 discoveries, roughly 10 percent are larger than six-tenths of a mile in size — large enough to have disastrous global consequences should one impact the Earth.
This is one of them.
First discovered in February 1950, 1950 DA is a 1.1-kilometer-wide asteroid that was observed for 17 days and then disappeared from view. Then it was spotted again on Dec. 31, 2000 — literally on the eve of the 21st century. Coupled with radar observations made a few weeks later in March 2001 it was found that, along with a rather high rotation rate (2.1 hours), asteroid 1950 DA has a trajectory that will bring it very close to Earth on March 16, 2880. How close? Close enough that, within a specific 20-minute window, a collision can not be entirely ruled out.
Top 10 Ways to Stop an Asteroid
The image above was made from radar observations by the Arecibo Observatory in Puerto Rico in March 2001, when 1950 DA passed within 4.8 million miles of Earth. Is this the mug shot of a future continent-killer?
Radar analysis and research of 1950 DA performed by NASA’s Jet Propulsion Laboratory scientists J.D. Giorgini, S. J. Ostro, Don Yeomans and several others from JPL and other institutions revealed that the impact probability from 1950 DA in March 2880 is, at most, 1 in 300 based on what is known about the asteroid so far.
1 in 300 may sound like a slim chance, but actually this represents a risk 50% greater than that of the average hazard due to all other asteroids from now to then.
However, that’s a maximum value. The study also noted the collision probability for 1950 DA as being in the range from 0 to 0.33%. That upper limit could increase or decrease as more is learned about the asteroid. (The next opportunity for studying 1950 DA via radar is in 2032.)
There are many factors that influence the path of an asteroid through space. Its spin rate, reflectivity (albedo), composition, mass, terrain variations… gravitational interactions with other bodies, some of which may not even have been discovered yet… all of these can affect the movement of an asteroid and, more specifically, its exact position at a future point in time. While many of these things still aren’t precisely known for 1950 DA, one in particular could end up being the saving grace for our descendants: the Yarkovsky effect.
PHOTOS: Russian Meteor Strike Aftermath
A small but important force acting upon asteroids, the Yarkovsky effect is a “nudge” created by thermal emission. As an asteroid gathers heat energy from the sun, it releases some of that energy back into space. Thanks to Newtonian mechanics the sheer act of doing so creates a physical push back on the asteroid itself, altering its course ever so slightly. Over a long span of time, this slight alteration could result in the relocation of 1950 DA away from the spot in space where Earth will be on March 16, 2880… at least enough so that a miss is certain.
In fact, recent research by JPL scientists D. Farnocchia and S.R. Chesley have taken into consideration the Yarkovsky effect on 1950 DA based on known values from previous observations, as well as new research suggesting that the asteroid has a retrograde rotation. While their latest assessment does put the risk of an impact in 2880 within the lower end of the probability spectrum (4×10^-4, or -0.58 on the Palermo Scale) it is still far from zero, and in fact remains higher than any other known potential impacts.
PHOTOS: NASA’s Asteroid Capture Mission
So what would happen if the half-mile-wide 1950 DA were to hit Earth? While that depends on a lot of things, such as its composition, speed, angle of impact, where it impacts, etc., needless to say it would cause a lot of damage across a large area. I’m talking an energy release upwards of half a million megatons, which, were it to strike say, New York City, everything within at least a 100-mile radius would be flattened by the force of the impact alone — that’s halfway to Boston and Washington, DC. And that’s not even taking into consideration the air blast, atmospheric dust cloud, secondary impacts from debris, or damage from any resulting tsunami (if the impact were in the ocean)… the destruction would easily extend out many more hundreds of miles, and the repercussions — physical, financial, economic, and emotional — would extend around the globe.
But again, precisely where 1950 DA will be in another 866 1/2 years (and whether or not it will occupy the same point in space as our planet) relies on many factors that aren’t well known — even though its orbit is pretty well understood. More in-depth observations will need to be made, and that is why asteroids like this must be carefully — and continually — watched.
Luckily, 35 generations offers plenty of time to improve our knowledge. According to JPL’s Near-Earth Object program, “If it is eventually decided 1950 DA needs to be diverted, the hundreds of years of warning could allow a method as simple as dusting the surface of the asteroid with chalk or charcoal, or perhaps white glass beads, or sending a solar sail spacecraft that ends by collapsing its reflective sail around the asteroid. These things would change the asteroids reflectivity and allow sunlight to do the work of pushing the asteroid out of the way.”
ANALYSIS: Meet Asteroid 2013 MZ5, 10,000th Near-Earth Object
Still, whether because of ongoing research, faith in future generations of scientists, or just sheer probability, JPL remains confident that 1950 DA should cause little concern. “The most likely result will be that St. Patrick’s Day parades in 2880 will be a little more festive than usual as 1950 DA recedes into the distance, having passed Earth by.”
Let’s just hope the luck of the Irish is with our planet big time that year…

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Mark Kelly gives an astronaut’s view of ‘Gravity’ - TWP


Last weekend, my wife, Gabby, and I went to see the movie “Gravity” at our neighborhood theater in Tucson. I’m a retired astronaut who has been to space four times, so I’m usually a bit skeptical of films that take place in space. For me, watching movies about space is like a congresswoman watching “House of Cards.” It’s entertaining, but it’s obviously not the real thing.
Director Alfonso Cuarón does come remarkably close with “Gravity.” I’ve spent a total of 55 days in space so I know what to look for, and Cuarón really was able to capture what it looks like inside and outside of a spacecraft. It’s extremely difficult to film a movie that is almost entirely without gravity. In “Apollo 13,” Ron Howard achieved the effect of zero-gravity flight by filming in NASA’s zero-gravity airplane, the “Vomit Comet.”
Keep reading on The Washington Post >>
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viernes, septiembre 06, 2013

NASA Heads Back to the Moon



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lunes, junio 03, 2013

Never-before-seen alien planet just 300 light years from Earth


A newly discovered gaseous planet has been directly photographed orbiting a star about 300 light-years from Earth. Imaging alien planets is difficult, and this world may be the least massive planet directly observed outside of the solar system, scientists say.
A sharp new photo released by the European Southern Observatory (ESO) Monday, June 3, depicts the suspected gas giant (called HD 95086 b) circling its young star (named HD 95086) in infrared light. The star has been removed from the image to allow the planet — shown as a bright blue dot at the bottom left of the picture — to shine through.
HD 95086 b was sighted by ESO's Very Large Telescope in Chile. Based on the planet's brightness, scientists estimate that it is only about four or five times more massive than Jupiter. [See Amazing Photos of the Very Large Telescope]
Most exoplanets are discovered via indirect means, such as detecting a dip in a star's light when a planet passes in front of it, blocking part of its face, or finding a slight wobble in a star's movement caused by the gravitational tug of planets orbiting it.
"Direct imaging of planets is an extremely challenging technique that requires the most advanced instruments, whether ground-based or in space," Julien Rameau, an astronomer at the Institute of Astrophysics and Planetology in France and lead author of the study announcing the discovery, said in a statement. "Only a few planets have been directly observed so far, making every single discovery an important milestone on the road to understanding giant planets and how they form."
Another photo from ESO shows the star and its planet in context with other stars in the southern constellation of Carina, the keel.
The planet orbits its star at about twice the distance from the sun to Neptune and about 56 times the distance between Earth and the sun. The blue circle in the photo represents the distance between the sun and Neptune.
HD 95086 is relatively young star at only 10 million to 17 million years old, making the formation of the exoplanet and the dusty disc surrounding the star potentially intriguing to researchers.
"[The planet's] current location raises questions about its formation process," Anne-Marie Lagrange, one of Rameau's team members, said in a statement. "It either grew by assembling the rocks that form the solid core and then slowly accumulated gas from the environment to form the heavy atmosphere, or started forming from a gaseous clump that arose from gravitational instabilities in the disc. Interactions between the planet and the disc itself or with other planets may have also moved the planet from where it was born."
The research will be published in an upcoming issue of Astrophysical Journal Letters.

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viernes, mayo 31, 2013

Asteroid 1998 QE2 has a moon, radar shows

cosmiclog
When astronomers analyzed radar readings to create their first maps of 1998 QE2, the big asteroid that's due to sail past Earth on Friday, they were surprised to find that it has a moon twice as big as an ocean liner.
1998 QE2 itself is way bigger: The latest readings from NASA's Deep Space Network antenna in Goldstone, Calif., are consistent with earlier estimates that the asteroid is about 1.7 miles (2.7 kilometers wide). But the moon is hefty as well. Astronomers estimate its diameter at 2,000 feet (600 meters). That's big enough to wipe out an area of the size of Virginia if it were to strike land.
Fortunately, neither space rock will come any closer than 3.6 million miles (5.8 million kilometers), or about 15 times the distance between Earth and the moon, during a flyby that reaches its climax at 4:59 p.m. ET Friday.
Even though Earth is in no danger, the close encounter is stirring up interest because it gives astronomers a rare opportunity to see an asteroid up close. Such observations could help NASA plan for efforts as the Osiris-Rex mission, which will bring back a sample from the asteroid Bennu in 2023; and an even more ambitious mission to corral an asteroid by the mid-2020s.
Goldstone's first radar observations of 1998 QE2 were made on Wednesday evening, producing images with a resolution of about 250 feet (75 meters) per pixel. The pictures show that QE2 has a rotation period of less than four hours, and is marked by several dark surface features that are suggestive of large craters. In an image advisory, NASA's Jet Propulsion Laboratory says that the image resolution will get better as more radar readings become available, from Goldstone as well as the Arecibo Observatory in Puerto Rico.

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"Hablame"

"EN TIEMPOS DIFÍCILES" - Heberto Padilla

A aquel hombre le pidieron su tiempo

para que lo juntara al tiempo de la Historia.

Le pidieron las manos,

porque para una época difícil

nada hay mejor que un par de buenas manos.

Le pidieron los ojos

que alguna vez tuvieron lágrimas

para que contemplara el lado claro

(especialmente el lado claro de la vida)

porque para el horror basta un ojo de asombro.

Le pidieron sus labios

resecos y cuarteados para afirmar,

para erigir, con cada afirmación, un sueño

(el-alto-sueño);

le pidieron las piernas

duras y nudosas

(sus viejas piernas andariegas),

porque en tiempos difíciles

¿algo hay mejor que un par de piernas

para la construcción o la trinchera?

Le pidieron el bosque que lo nutrió de niño,

con su árbol obediente.

Le pidieron el pecho, el corazón, los hombros.

Le dijeron

que eso era estrictamente necesario.

Le explicaron después

que toda esta donación resultaria inútil.

sin entregar la lengua,

porque en tiempos difíciles

nada es tan útil para atajar el odio o la mentira.

Y finalmente le rogaron

que, por favor, echase a andar,

porque en tiempos difíciles

esta es, sin duda, la prueba decisiva.

Los Aldeanos: "El Socialismo en Tiempos del Colera: Toda Una Nación"

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La columna de Cubanalisis

NEOCASTRISMO [Hacer click en la imagen]

NEOCASTRISMO [Hacer click en la imagen]
¨Saturno jugando con sus hijos¨/ Pedro Pablo Oliva

Seguidores

Carta desde la carcel de Fidel Castro Ruz

“…después de todo, para mí la cárcel es un buen descanso, que sólo tiene de malo el que es obligatorio. Leo mucho y estudio mucho. Parece increíble, las horas pasan como si fuesen minutos y yo, que soy de temperamento intranquilo, me paso el día leyendo, apenas sin moverme para nada. La correspondencia llega normalmente…”

“…Como soy cocinero, de vez en cuando me entretengo preparando algún pisto. Hace poco me mandó mi hermana desde Oriente un pequeño jamón y preparé un bisté con jalea de guayaba. También preparo spaghettis de vez en cuando, de distintas formas, inventadas todas por mí; o bien tortilla de queso. ¡Ah! ¡Qué bien me quedan! por supuesto, que el repertorio no se queda ahí. Cuelo también café que me queda muy sabroso”.
“…En cuanto a fumar, en estos días pasados he estado rico: una caja de tabacos H. Upman del doctor Miró Cardona, dos cajas muy buenas de mi hermano Ramón….”.
“Me voy a cenar: spaghettis con calamares, bombones italianos de postre, café acabadito de colar y después un H. Upman #4. ¿No me envidias?”.
“…Me cuidan, me cuidan un poquito entre todos. No le hacen caso a uno, siempre estoy peleando para que no me manden nada. Cuando cojo el sol por la mañana en shorts y siento el aire de mar, me parece que estoy en una playa… ¡Me van a hacer creer que estoy de vacaciones! ¿Qué diría Carlos Marx de semejantes revolucionarios?”.
¨La patria es dicha de todos, y dolor de todos, y cielo para todos, y no feudo ni capellaní­a de nadie¨ - Marti

"No temas ni a la prision, ni a la pobreza, ni a la muerte. Teme al miedo"
-
Giacomo Leopardi

¨Por eso es muy importante, Vicky, hijo mío, que recuerdes siempre para qué sirve la cabeza: para atravesar paredes¨Halvar de Flake [El vikingo]

"Como no me he preocupado de nacer, no me preocupo de morir" - Lorca

"Al final, no os preguntarán qué habéis sabido, sino qué habéis hecho" - Jean de Gerson

"Si queremos que todo siga como está, es necesario que todo cambie" - Giuseppe Tomasi di Lampedusa

"Todo hombre paga su grandeza con muchas pequeñeces, su victoria con muchas derrotas, su riqueza con múltiples quiebras" - Giovanni Papini


"Life is what happens while you are busy making other plans" - John Lennon

"Habla bajo, lleva siempre un gran palo y llegarás lejos" - Proverbio Africano

"No hay medicina para el miedo" - Proverbio escoces

"El supremo arte de la guerra es doblegar al enemigo sin luchar"
- Sun Tzu

"You do not really understand something unless you can explain it to your grandmother" - Albert Einstein

"It is inaccurate to say I hate everything. I am strongly in favor of common sense, common honesty, and common decency. This makes me forever ineligible for public office" - H. L. Menken

"I swore never to be silent whenever and wherever human beings endure suffering and humiliation. We must always take sides. Neutrality helps the oppressor, never the victim. Silence encourages the tormentor, never the tormented" - Elie Wiesel

"Stay hungry, stay foolish" -
Steve Jobs

"If you put the federal government in charge of the Sahara Desert , in five years ther'ed be a shortage of sand" - Milton Friedman

"The tragedy of modern man is not that he knows less and less about the meaning of his own life, but that it bothers him less and less" - Vaclav Havel

"No se puede controlar el resultado, pero si lo que uno haga para alcanzarlo" -
Vitor Belfort [MMA Fighter]

Liborio

Liborio
A la puerta de la gloria está San Pedro sentado y ve llegar a su lado a un hombre de cierta historia. No consigue hacer memoria y le pregunta con celo: ¿Quién eras allá en el suelo? Era Liborio mi nombre. Has sufrido mucho, hombre, entra, te has ganado el cielo.

Para Raul Castro

Cuba ocupa el penultimo lugar en el mundo en libertad economica solo superada por Corea del Norte.

Cuba ocupa el lugar 147 entre 153 paises evaluados en "Democracia, Mercado y Transparencia 2007"

Cuando vinieron

Cuando vinieron a buscar a los comunistas, Callé: yo no soy comunista.
Cuando vinieron a buscar a los sindicalistas, Callé: yo no soy sindicalista.
Cuando vinieron a buscar a los judíos, Callé: yo no soy judío. Cuando vinieron a buscar a los católicos, Callé: yo no soy “tan católico”.
Cuando vinieron a buscarme a mí, Callé: no había quien me escuchara.

Reverendo Martin Niemöller

Martha Colmenares

Martha Colmenares
Un sitio donde los hechos y sus huellas nos conmueven o cautivan

CUBA LLORA Y EL MUNDO Y NOSOTROS NO ESCUCHAMOS

Donde esta el Mundo, donde los Democratas, donde los Liberales? El pueblo de Cuba llora y nadie escucha.
Donde estan los Green, los Socialdemocratas, los Ricos y los Pobres, los Con Voz y Sin Voz? Cuba llora y nadie escucha.
Donde estan el Jet Set, los Reyes y Principes, Patricios y Plebeyos? Cuba desesperada clama por solidaridad.
Donde Bob Dylan, donde Martin Luther King, donde Hollywood y sus estrellas? Donde la Middle Class democrata y conservadora, o acaso tambien liberal a ratos? Y Gandhi? Y el Dios de Todos?
Donde los Santos y Virgenes; los Dioses de Cristianos, Protestantes, Musulmanes, Budistas, Testigos de Jehova y Adventistas del Septimo Dia. Donde estan Ochun y todas las deidades del Panteon Yoruba que no acuden a nuestro llanto? Donde Juan Pablo II que no exige mas que Cuba se abra al Mundo y que el Mundo se abra a Cuba?
Que hacen ahora mismo Alberto de Monaco y el Principe Felipe que no los escuchamos? Donde Madonna, donde Angelina Jolie y sus adoptados around de world; o nos hara falta un Brando erguido en un Oscar por Cuba? Donde Sean Penn?
Donde esta la Aristocracia Obrera y los Obreros menos Aristocraticos, donde los Working Class que no estan junto a un pueblo que lanquidece, sufre y llora por la ignominia?
Que hacen ahora mismo Zapatero y Rajoy que no los escuchamos, y Harper y Dion, e Hillary y Obama; donde McCain que no los escuchamos? Y los muertos? Y los que estan muriendo? Y los que van a morir? Y los que se lanzan desesperados al mar?
Donde estan el minero cantabrico o el pescador de percebes gijonese? Los Canarios donde estan? A los africanos no los oimos, y a los australianos con su acento de hombres duros tampoco. Y aquellos chinos milenarios de Canton que fundaron raices eternas en la Isla? Y que de la Queen Elizabeth y los Lords y Gentlemen? Que hace ahora mismo el combativo Principe Harry que no lo escuchamos?
Donde los Rockefellers? Donde los Duponts? Donde Kate Moss? Donde el Presidente de la ONU? Y Solana donde esta? Y los Generales y Doctores? Y los Lam y los Fabelo, y los Sivio y los Fito Paez?
Y que de Canseco y Miñoso? Y de los veteranos de Bahia de Cochinos y de los balseros y de los recien llegados? Y Carlos Otero y Susana Perez? Y el Bola, y Pancho Cespedes? Y YO y TU?
Y todos nosotros que estamos aqui y alla rumiando frustaciones y resquemores, envidias y sinsabores; autoelogios y nostalgias, en tanto Louis Michel comulga con Perez Roque mientras Biscet y una NACION lanquidecen?
Donde Maceo, donde Marti; donde aquel Villena con su carga para matar bribones?
Cuba llora y clama y el Mundo NO ESCUCHA!!!

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