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Posts tagged: a still more glorious dawn

carl sagan: “you are always home.”

carl sagan: “you are always home.”

Every fall into love involves [to adapt Oscar Wilde] the triumph of hope over self-knowledge. We fall in love hoping that we will not find in the other what we know is in ourselves – all the cowardice, weakness, laziness, dishonesty, compromise and brute stupidity. We throw a cordon of love around the chosen one, and decide that everything that lies within it will somehow be free of our faults and hence lovable. We locate inside another a perfection that eludes us within ourselves, and through union with the beloved, hope somehow to maintain [against evidence of all self-knowledge] a precarious faith in the species.
Planck mission steps closer to the cosmic blueprint

This all-sky image shows the distribution of carbon monoxide (CO), a molecule used by astronomers to trace molecular clouds across the sky, as seen by Planck. The inserts provide a zoomed-in view onto three individual regions on the sky where Planck has detected concentrations of CO: Cepheus, Taurus and Pegasus, respectively. Credits: ESA/Planck Collaboration
Planck’s primary goal is to observe the Cosmic Microwave Background (CMB), the relic radiation from the Big Bang, and to measure its encoded information about the constituents of the Universe and the origin of cosmic structure.
But it can only be reached once all sources of foreground emission, such as the galactic haze and the carbon monoxide signals, have been identified and removed.

Planck mission steps closer to the cosmic blueprint

This all-sky image shows the distribution of carbon monoxide (CO), a molecule used by astronomers to trace molecular clouds across the sky, as seen by Planck. The inserts provide a zoomed-in view onto three individual regions on the sky where Planck has detected concentrations of CO: Cepheus, Taurus and Pegasus, respectively. Credits: ESA/Planck Collaboration

Planck’s primary goal is to observe the Cosmic Microwave Background (CMB), the relic radiation from the Big Bang, and to measure its encoded information about the constituents of the Universe and the origin of cosmic structure.

But it can only be reached once all sources of foreground emission, such as the galactic haze and the carbon monoxide signals, have been identified and removed.

strag2001:

This is a high resolution image of the sand dunes in the Noachis Terra Region of Mars, taken with NASA’s HiRISE. (source)

strag2001:

This is a high resolution image of the sand dunes in the Noachis Terra Region of Mars, taken with NASA’s HiRISE. (source)

There are two ways to live: you can live as if nothing is a miracle; you can live as if everything is a miracle.

Albert Einstein

(via jellydonut52)

kateoplis:

mills:

Kateoplis posted a “Moon model by Johann FJ Schmidt at Chicago’s Field Museum, 1898.” One can scarcely imagine a more beautiful representation of knowledge, that strange abstraction which exerts so much control over the irreducible physical cosmos; as David Deutsch noted in his first TED talk:

Now how do we know about an environment that’s so far away, and so different, and so alien, from anything we’re used to? Well, the Earth —our environment, in the form of us— is creating knowledge. Well, what does that mean? Well, look out even further than we’ve just been —I mean from here, with a telescope— and you’ll see things that look like stars. They’re called “quasars.” “Quasars” originally meant quasi-stellar object. Which means things that look a bit like stars. But they’re not stars. And we know what they are. Billions of years ago, and billions of light years away, the material at the center of a galaxy collapsed towards a super-massive black hole. And then intense magnetic fields directed some of the energy of that gravitational collapse. And some of the matter, back out in the form of tremendous jets which illuminated lobes with the brilliance of —I think it’s a trillion suns.
Now, the physics of the human brain could hardly be more unlike the physics of such a jet. We couldn’t survive for an instant in it. Language breaks down when trying to describe what it would be like in one of those jets. It would be a bit like experiencing a supernova explosion, but at point-blank range and for millions of years at a time. And yet, that jet happened in precisely such a way that billions of years later, on the other side of the universe, some bit of chemical scum could accurately describe, and model, and predict, and explain, —above all— what was happening there, in reality. The one physical system, the brain, contains an accurate working model of the other, the quasar. Not just a superficial image of it, though it contains that as well, but an explanatory model, embodying the same mathematical relationships and the same causal structure.
Now that is knowledge. And if that weren’t amazing enough, the faithfulness with which the one structure resembles the other is increasing with time. That is the growth of knowledge. So, the laws of physics have this special property. That physical objects, as unlike each other as they could possibly be, can nevertheless embody the same mathematical and causal structure and to do it more and more so over time.

It is not solely humanity which is capable of this; all life, to some degree, embodies knowledge as a function of selection processes which reward, so to speak, successful adaptive responses to environments. But humans have a vastly greater degree of precision and accuracy in their knowledge than any other creature, in part because our knowledge is so often explicit, rather being than coded into inexplicit, lossy genomic systems; in part because our knowledge is representational in many ways, rather than merely responsive to stimuli; in part because of our capacity for abstraction and generalization; and largely because ours is aided, in innumerable ways, by tools we have constructed to help acquire knowledge.
These tools now themselves contain models precisely as our minds do; inside this room is a model of the moon, just as inside your mind are the models for countless phenomena you will never witness, never touch or feel, and yet whose shape and behavior you can predict with stunning accuracy. We know a great deal through statistical computation, but all such computation is contingent on explanatory models which “embody the same mathematical and causal structure” as this or that element of the natural world.
Man is above all else the maker of models. Real knowledge is not merely predictive but virtualizes; one needn’t go to the moon; one merely keeps a model of it at hand.

FOLLOW MILLS.

OKAY.

kateoplis:

mills:

Kateoplis posted a “Moon model by Johann FJ Schmidt at Chicago’s Field Museum, 1898.” One can scarcely imagine a more beautiful representation of knowledge, that strange abstraction which exerts so much control over the irreducible physical cosmos; as David Deutsch noted in his first TED talk:

Now how do we know about an environment that’s so far away, and so different, and so alien, from anything we’re used to? Well, the Earth —our environment, in the form of us— is creating knowledge. Well, what does that mean? Well, look out even further than we’ve just been —I mean from here, with a telescope— and you’ll see things that look like stars. They’re called “quasars.” “Quasars” originally meant quasi-stellar object. Which means things that look a bit like stars. But they’re not stars. And we know what they are. Billions of years ago, and billions of light years away, the material at the center of a galaxy collapsed towards a super-massive black hole. And then intense magnetic fields directed some of the energy of that gravitational collapse. And some of the matter, back out in the form of tremendous jets which illuminated lobes with the brilliance of —I think it’s a trillion suns.

Now, the physics of the human brain could hardly be more unlike the physics of such a jet. We couldn’t survive for an instant in it. Language breaks down when trying to describe what it would be like in one of those jets. It would be a bit like experiencing a supernova explosion, but at point-blank range and for millions of years at a time. And yet, that jet happened in precisely such a way that billions of years later, on the other side of the universe, some bit of chemical scum could accurately describe, and model, and predict, and explain, —above all— what was happening there, in reality. The one physical system, the brain, contains an accurate working model of the other, the quasar. Not just a superficial image of it, though it contains that as well, but an explanatory model, embodying the same mathematical relationships and the same causal structure.

Now that is knowledge. And if that weren’t amazing enough, the faithfulness with which the one structure resembles the other is increasing with time. That is the growth of knowledge. So, the laws of physics have this special property. That physical objects, as unlike each other as they could possibly be, can nevertheless embody the same mathematical and causal structure and to do it more and more so over time.

It is not solely humanity which is capable of this; all life, to some degree, embodies knowledge as a function of selection processes which reward, so to speak, successful adaptive responses to environments. But humans have a vastly greater degree of precision and accuracy in their knowledge than any other creature, in part because our knowledge is so often explicit, rather being than coded into inexplicit, lossy genomic systems; in part because our knowledge is representational in many ways, rather than merely responsive to stimuli; in part because of our capacity for abstraction and generalization; and largely because ours is aided, in innumerable ways, by tools we have constructed to help acquire knowledge.

These tools now themselves contain models precisely as our minds do; inside this room is a model of the moon, just as inside your mind are the models for countless phenomena you will never witness, never touch or feel, and yet whose shape and behavior you can predict with stunning accuracy. We know a great deal through statistical computation, but all such computation is contingent on explanatory models which “embody the same mathematical and causal structure” as this or that element of the natural world.

Man is above all else the maker of models. Real knowledge is not merely predictive but virtualizes; one needn’t go to the moon; one merely keeps a model of it at hand.

FOLLOW MILLS.

OKAY.

gallen:

Herschel Finds Oceans of Water in Disk of Nearby Star

PASADENA, Calif. — Using data from the Herschel Space Observatory, astronomers have detected for the first time cold water vapor enveloping a dusty disk around a young star. The findings suggest that this disk, which is poised to develop into a solar system, contains great quantities of water, suggesting that water-covered planets like Earth may be common in the universe. Herschel is a European Space Agency mission with important NASA contributions.Scientists previously found warm water vapor in planet-forming disks close to a central star. Evidence for vast quantities of water extending out into the cooler, far reaches of disks where comets take shape had not been seen until now. The more water available in disks for icy comets to form, the greater the chances that large amounts eventually will reach new planets through impacts.

gallen:

Herschel Finds Oceans of Water in Disk of Nearby Star

PASADENA, Calif. — Using data from the Herschel Space Observatory, astronomers have detected for the first time cold water vapor enveloping a dusty disk around a young star. The findings suggest that this disk, which is poised to develop into a solar system, contains great quantities of water, suggesting that water-covered planets like Earth may be common in the universe. Herschel is a European Space Agency mission with important NASA contributions.

Scientists previously found warm water vapor in planet-forming disks close to a central star. Evidence for vast quantities of water extending out into the cooler, far reaches of disks where comets take shape had not been seen until now. The more water available in disks for icy comets to form, the greater the chances that large amounts eventually will reach new planets through impacts.

dvdp:

“A wide field meteor camera at NASA’s Marshall Space Flight Center recorded this spectacular meteor breaking up in Earth’s atmosphere on Sept. 30, 2011, 8:37 p.m. EDT. Also visible is a star-like object moving slowly toward the upper middle of the field of view — the upper stage of the Zenit booster that launched the Russian Cosmos 2219 intelligence satellite back in 1992. Orbiting 500 miles above Earth, this empty rocket body can get bright enough to be seen with the unaided eye.”

dudes are always harshing all ‘where is my flying car //this future is disappoint// meanwhile i am watching a gif of a meteor impact that nasa made with a satellite //on my telephone//.

dvdp:

“A wide field meteor camera at NASA’s Marshall Space Flight Center recorded this spectacular meteor breaking up in Earth’s atmosphere on Sept. 30, 2011, 8:37 p.m. EDT. Also visible is a star-like object moving slowly toward the upper middle of the field of view — the upper stage of the Zenit booster that launched the Russian Cosmos 2219 intelligence satellite back in 1992. Orbiting 500 miles above Earth, this empty rocket body can get bright enough to be seen with the unaided eye.”

dudes are always harshing all ‘where is my flying car //this future is disappoint// meanwhile i am watching a gif of a meteor impact that nasa made with a satellite //on my telephone//.

wilwheaton:

A time-lapse taken from the front of the International Space Station as it orbits our planet at night. This movie begins over the Pacific Ocean and continues over North and South America before entering daylight near Antarctica.

What does it feel like to fly over planet Earth? (by yesterday2221)

# a still more glorious dawn

this-is-ryan:

nasa :: astronomy picture of the day

The robotic Cassini spacecraft … drifted in [the] giant planet’s shadow for about 12 hours in 2006 and looked back toward the eclipsed Sun. Cassini saw a view unlike any other. First, the night side of Saturn is seen to be partly lit by light reflected from its own majestic ring system. Next, the rings themselves appear dark when silhouetted against Saturn, but quite bright when viewed away from Saturn, slightly scattering sunlight, in this exaggerated color image. Saturn’s rings light up so much that new rings were discovered, although they are hard to see in the image. Seen in spectacular detail, however, is Saturn’s E ring, the ring created by the newly discovered ice-fountains of the moon Enceladus and the outermost ring visible above. Far in the distance, at the left, just above the bright main rings, is the almost ignorable pale blue dot of Earth.

this-is-ryan:

nasa :: astronomy picture of the day

The robotic Cassini spacecraft … drifted in [the] giant planet’s shadow for about 12 hours in 2006 and looked back toward the eclipsed Sun. Cassini saw a view unlike any other. First, the night side of Saturn is seen to be partly lit by light reflected from its own majestic ring system. Next, the rings themselves appear dark when silhouetted against Saturn, but quite bright when viewed away from Saturn, slightly scattering sunlight, in this exaggerated color image. Saturn’s rings light up so much that new rings were discovered, although they are hard to see in the image. Seen in spectacular detail, however, is Saturn’s E ring, the ring created by the newly discovered ice-fountains of the moon Enceladus and the outermost ring visible above. Far in the distance, at the left, just above the bright main rings, is the almost ignorable pale blue dot of Earth.

jesuisperdu:

eclipse, ansel adams

jesuisperdu:

eclipse, ansel adams

The central region of the Milky Way :: physorg:

A false-color composite image of the central 50 light-years of the Milky Way as seen for the first time in the entirely of the far infrared. Many of the previously-known structures in the region are labeled; the location of the black hole is labeled “SagA*,” and the inner donut as “CND.” Colder material is shown in red; warmer (but still relatively cold) in blue. Credit: NASA; ESA and M. Etxaluze
(PhysOrg.com) — The center of our Milky Way galaxy is about 27,000 light-years away in the direction of the constellation of Sagittarius. At the very center of the galaxy lies a black hole whose mass is about four million solar masses. Around it is a donut-shaped structure about eight light-years across that rings the inner volume of neutral gas and an estimated thousands of individual stars. Around that, stretching out to 700 light-years, is a dense molecular zone of activity, unique to the galaxy, with massive star forming clusters of luminous stars, giant molecular clouds, and many more, poorly understood regions as well.

[h/t ellis king]

The central region of the Milky Way :: physorg:

A false-color composite image of the central 50 light-years of the Milky Way as seen for the first time in the entirely of the far infrared. Many of the previously-known structures in the region are labeled; the location of the black hole is labeled “SagA*,” and the inner donut as “CND.” Colder material is shown in red; warmer (but still relatively cold) in blue. Credit: NASA; ESA and M. Etxaluze

(PhysOrg.com) — The center of our Milky Way galaxy is about 27,000 light-years away in the direction of the constellation of Sagittarius. At the very center of the galaxy lies a black hole whose mass is about four million solar masses. Around it is a donut-shaped structure about eight light-years across that rings the inner volume of neutral gas and an estimated thousands of individual stars. Around that, stretching out to 700 light-years, is a dense molecular zone of activity, unique to the galaxy, with massive star forming clusters of luminous stars, giant molecular clouds, and many more, poorly understood regions as well.

[h/t ellis king]

First of all, let’s clarify what the NASA budget is. Do you realize that the $850 billion dollar bailout, that sum of money is greater than the entire 50-year running budget of NASA?

And so when someone says, “We don’t have enough money for this space probe,” I’m asking, no, it’s not that you don’t have enough money, it’s that the distribution of money that you’re spending is warped in some way that you are removing the only thing that gives people something to dream about tomorrow.

You remember the 60s and 70s. You didn’t have to go more than a week before there’s an article in Life magazine, “The Home of Tomorrow,” “The City of Tomorrow,” “Transportation of Tomorrow”. All of that ended in the 1970s. After we stopped going to the Moon, it all ended. We stopped dreaming.

And so I worry that the decision that Congress makes doesn’t factor in the consequences of those decisions on tomorrow. Tomorrow’s gone. They’re playing for the quarterly report, they’re playing for the next election cycle, and that is mortgaging the actual future of this nation, and the rest of the world is going to pass us by.

Neil deGrasse Tyson (via david)

This is brilliant and sad. It’s the end of dreams time.

(via discoverynews)

(via guerillamamamedicine)