| И вот он готов - твой портрет... Смотри... |
Любовь к жизни - вот твое главное качество, которое дарит тебе и доброту, и чувство юмора, и любознательность, да много чего... Твое жизнелюбие - это прекрасно... И я старалась показать его на холсте... А получилось ли у меня - решать тебе. Было приятно с тобой пообщаться! (:![]() |
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Friday, May 07, 2010
Taigi taigi...
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Antony Micallef
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Thursday, May 06, 2010
Visions of Future Past

The Soyuz TMA-17 spacecraft is the subject of this long exposure, and is seen as it is rolled out by train to the launch pad at the Baikonur Cosmodrome, Kazakhstan, Friday, Dec. 18, 2009. The launch of the Soyuz spacecraft with Expedition 22 NASA Flight Engineer Timothy J. Creamer of the U.S., Soyuz Commander Oleg Kotov of Russia and Flight Engineer Soichi Noguchi of Japan, occurred on Monday, Dec. 21, 2009.
Image Credit: NASA/Bill Ingalls
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Laura Laine
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Beautiful spaces
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2010 Arthur C. Clarke Award
- “Yellow Blue Tibia” by Adam Roberts
- “Galileo’s Dream” by Kim Stanley Robinson
- “Far North” by Marcel Theroux
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Poem of the Week
To Helen by Edgar Allan Poe
Helen, thy beauty is to me
Like those Nicéan barks of yore,
That gently, o'er a perfumed sea,
The weary, way-worn wanderer bore
To his own native shore.
On desperate seas long wont to roam,
Thy hyacinth hair, thy classic face,
Thy Naiad airs have brought me home
To the glory that was Greece
And the grandeur that was Rome.
Lo! In yon brilliant window-niche
How statue-like I see thee stand,
The agate lamp within thy hand!
Ah, Psyche, from the regions which
Are Holy-Land!
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Stellar Nursery in the Rosette Nebula

This image from the European Space Agency's Herschel Space Observatory shows the cloud associated with the Rosette Nebula, a stellar nursery about 5,000 light-years from Earth in the Monoceros, or Unicorn, constellation. Herschel collects the infrared light given out by dust. The bright smudges are dusty cocoons containing massive embryonic stars, which will grow up to 10 times the mass of our sun. The small spots near the center of the image are lower mass stellar embryos. The Rosette Nebula itself, and its massive cluster of stars, is located to the right of the picture.
This image is a three-color composite showing infrared wavelengths of 70 microns (blue), 160 microns (green), and 250 microns (red). It was made with observations from Herschel's Photoconductor Array Camera and Spectrometer and the Spectral and Photometric Imaging Receiver instruments.
Herschel is an ESA cornerstone mission, with science instruments provided by consortia of European institutes and with participation by NASA.
A media day celebrating the release of the first results from ESA’s Herschel infrared space telescope will take place on May 6, 2010, at Space Expo, at the European Space Research and Technology Centre (ESTEC), Noordwijk, The Netherlands. Doors open at 11:30 CEST. The media day is organized in connection with the Herschel First Results Symposium taking place this week at ESTEC and the theme is Revealing the Hidden Side of Star Formation. For more information on the day's activities, see the press release.
For more information on this image, visit ESA's Herschel Program site.
Image Credit: ESA/PACS & SPIRE Consortium/HOBYS Key Programme Consortia
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Double Black Holes

This image from the Chandra X-ray Observatory shows the central region of the starburst galaxy M82 and contains two bright X-ray sources of special interest. New studies with Chandra and ESA's XMM-Newton show that these two sources may be intermediate-mass black holes, with masses in between those of the stellar-mass and supermassive variety. These "survivor" black holes avoided falling into the center of the galaxy and could be examples of the seeds required for the growth of supermassive black holes in galaxies, including the one in the Milky Way.
This is the first case where good evidence for more than one mid-sized black hole exists in a single galaxy. The evidence comes from how their X-ray emission varies over time and analysis of their X-ray brightness and spectra, i.e., the distribution of X-rays with energy. These results are interesting because they may help address the mystery of how supermassive black holes in the centers of galaxies form. M82 is located about 12 million light years from Earth and is the nearest place to us where the conditions are similar to those in the early Universe, with lots of stars forming.
Multiple observations of M82 have been made with Chandra beginning soon after launch. The Chandra data shown here were not used in the new research because the X-ray sources are so bright that some distortion is introduced into the X-ray spectra. To combat this, the pointing of Chandra is changed so that images of the sources are deliberately blurred, producing fewer counts in each pixel.
Image credit: NASA/CXC/Tsinghua Univ./H. Feng et al.
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Wednesday, May 05, 2010
Poem of the Week
Eros Turannos by Edwin Arlington Robinson
She fears him, and will always ask
What fated her to choose him;
She meets in his engaging mask
All reasons to refuse him;
But what she meets and what she fears
Are less than are the downward years,
Drawn slowly to the foamless weirs
Of age, were she to lose him.
Between a blurred sagacity
That once had power to sound him,
And Love, that will not let him be
The Judas that she found him,
Her pride assuages her almost,
As if it were alone the cost –
He sees that he will not be lost
And waits and looks around him.
A sense of ocean and old trees
Envelops and allures him;
Tradition, touching all he sees,
Beguiles and reassures him;
And all her doubts of what he says
Are dimmed with what she knows of days –
Till even prejudice delays
And fades, and she secures him.
The failing leaf inaugurates
The reign of her confusion:
The pounding wave reverberates
The dirge of her illusion;
And home, where passion lived and died,
Becomes a place where she can hide,
While all the town and harbour side
Vibrate with her seclusion.
We tell you, tapping on our brows,
The story as it should be –
As if the story of a house
Were told, or ever could be;
We'll have no kindly veil between
Her visions and those we have seen –
As if we guessed what hers had been,
Or what they are, or would be.
Meanwhile we do no harm; for they
That with a god have striven,
Not hearing much of what we say,
Take what the god has given;
Though like waves breaking it may be
Or like a changed familiar tree,
Or like a stairway to the sea
Where down the blind are driven.
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Ehe...
| Ну что же, все ясно. Вы не кто иной, как Константин Устинович Черненко |
| Константин Устинович Черненко (11 сентября 1911 — 10 марта 1985) — Генеральный секретарь ЦК КПСС с 13 февраля 1984, Председатель Президиума Верховного Совета СССР с 11 апреля 1984 (депутат — с 1966-го). Член КПСС с 1931 года, ЦК КПСС — с 1971 года (кандидат с 1966-го), член Политбюро ЦК КПСС с 1978 года (кандидат с 1977-го). Чиновник до мозга костей, безраздельно преданный Леониду Ильичу, инерцией его покровительства на склоне лет оказался вознесенным на самую вершину власти, что не прибавило ни авторитета стране, ни уважения ему самому. |
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Building Planets
This artist's animation illustrates a massive asteroid belt in orbit around a star the same age and size as our Sun. Asteroids are chunks of rock from "failed" planets, which never managed to coalesce into full-sized planets. Asteroid belts can be thought of as construction sites that accompany the building of rocky planets.
Announced on April 28, 2010, scientists using NASA’s Infrared Telescope Facility have detected water-ice and carbon-based organic compounds on the surface of an asteroid. The cold hard facts of the discovery of the frosty mixture on one of the asteroid belt's largest occupants, suggests that some asteroids, along with their celestial brethren, comets, were the water carriers for a primordial Earth.
Image credit: NASA/JPL-Caltech
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Ring of Fire

This new image from the Solar Dynamics Observatory’s Atmospheric Imaging Assembly (AIA) shows in great detail a solar prominence taken from a March 30, 2010 eruption. The twisting motion of the material is the most noticeable feature.
Launched on Feb. 11, 2010, SDO is the most advanced spacecraft ever designed to study the sun. During its five-year mission, it will examine the sun's magnetic field and also provide a better understanding of the role the sun plays in Earth's atmospheric chemistry and climate. Since launch, engineers have been conducting testing and verification of the spacecraft’s components. Now fully operational, SDO will provide images with clarity 10 times better than high-definition television and will return more comprehensive science data faster than any other solar observing spacecraft.
Image Credit: NASA/SDO/AIA
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