f yeah, Carl Sagan
virtualsky:

From the Cells to the Stars 
This work, titled, “From the Cells to the Stars,” was painted by artist Michele Banks to in honor of her friend Cathy, who passed in August after a five-year battle with cancer. Not wanting to create another “cancer painting,” Banks drew her inspiration for the piece from Carl Sagan’s memorable quote that humans are all made of “star stuff.” As she explained on her blog:

I was reading about astronomer Carl Sagan, who often expressed the idea that humans are made of “star stuff”. That is, that all the basic elements of life on earth derive from “space debris” from the gigantic explosions of massive, ancient stars. This concept is at once so simple and so mind-boggling that it’s a struggle to absorb, much less to express artistically. I started looking around for ideas of how to visually portray the basic elements such as hydrogen, helium and nitrogen. Um. This is difficult, because you can’t see them. If you do a Google image search on Carbon, it comes up with a lot of gray-black cars. But when I thought about how the elements were released, I found supernovas. Not only are supernovas beautiful and awe-inspiring, they bear a strong resemblance to dividing cells, especially explosively dividing cancer cells.
Here’s the other thing. Carl Sagan also had [myelodysplastic syndrome]. He underwent three bone marrow transplants before he died in 1996. So this painting, besides celebrating the cosmic connection that all living creatures share, goes out to Cathy and Carl. From the infinitely tiny cells deep in the marrow of their bones, to the billions of stars in the sky.

Image courtesy Michele Banks

virtualsky:

From the Cells to the Stars

This work, titled, “From the Cells to the Stars,” was painted by artist Michele Banks to in honor of her friend Cathy, who passed in August after a five-year battle with cancer. Not wanting to create another “cancer painting,” Banks drew her inspiration for the piece from Carl Sagan’s memorable quote that humans are all made of “star stuff.” As she explained on her blog:

I was reading about astronomer Carl Sagan, who often expressed the idea that humans are made of “star stuff”. That is, that all the basic elements of life on earth derive from “space debris” from the gigantic explosions of massive, ancient stars. This concept is at once so simple and so mind-boggling that it’s a struggle to absorb, much less to express artistically. I started looking around for ideas of how to visually portray the basic elements such as hydrogen, helium and nitrogen. Um. This is difficult, because you can’t see them. If you do a Google image search on Carbon, it comes up with a lot of gray-black cars. But when I thought about how the elements were released, I found supernovas. Not only are supernovas beautiful and awe-inspiring, they bear a strong resemblance to dividing cells, especially explosively dividing cancer cells.

Here’s the other thing. Carl Sagan also had [myelodysplastic syndrome]. He underwent three bone marrow transplants before he died in 1996. So this painting, besides celebrating the cosmic connection that all living creatures share, goes out to Cathy and Carl. From the infinitely tiny cells deep in the marrow of their bones, to the billions of stars in the sky.

Image courtesy Michele Banks

brainmashh:

In the words of Sagan: “we’re made of star stuff”

Space blows my mind. The featured video literally gave me a funny feeling in my tummy. I really love this shit, like really really do. 

We embarked on our journey to the stars with a question first framed in the childhood of our species and in each generation asked anew with undiminished wonder: What are the stars? Exploration is in our nature. We began as wanderers, and we are wanderers still. We have lingered long enough on the shores of the cosmic ocean. We are ready at last to set sail for the stars.
Carl Sagan, Cosmos, Page 193 (via strangeandbittercrop)
Did exploding stars help life on Earth to thrive?

Research by a Danish physicist suggests that the explosion of massive stars – supernovae – near the Solar System has strongly influenced the development of life. Prof. Henrik Svensmark of the Technical University of Denmark (DTU) sets out his novel work in a paper in the journal Monthly Notices of the Royal Astronomical Society.Prof. Svensmark looked back through 500 million years of geological and astronomical data and considered the proximity of the Sun to supernovae as it moves around our Galaxy, the Milky Way. In particular, when the Sun is passing through the spiral arms of the Milky Way, it encounters newly forming clusters of stars. These so-called open clusters, which disperse over time, have a range of ages and sizes and will have started with a small proportion of stars massive enough to explode as supernovae. From the data on open clusters, Prof. Svensmark was able to deduce how the rate at which supernovae exploded near the Solar System varied over time.Comparing this with the geological record, he found that the changing frequency of nearby supernovae seems to have strongly shaped the conditions for life on Earth. Whenever the Sun and its planets have visited regions of enhanced star formation in the Milky Way Galaxy, where exploding stars are most common, life has prospered. Prof. Svensmark remarks in the paper, “The biosphere seems to contain a reflection of the sky, in that the evolution of life mirrors the evolution of the Galaxy.”In the new work, the diversity of life over the last 500 million years seems remarkably well explained by tectonics affecting the sea-level together with variations in the supernova rate, and virtually nothing else. To obtain this result on the variety of life, or biodiversity, he followed the changing fortunes of the best-recorded fossils. These are from invertebrate animals in the sea, such as shrimps and octopuses, or the extinct trilobites and ammonites.They tended to be richest in their variety when continents were drifting apart and sea levels were high and less varied when the land masses gathered 250 million years ago into the supercontinent called Pangaea and the sea-level was lower. But this geophysical effect was not the whole story. When it is removed from the record of biodiversity, what remains corresponds closely to the changing rate of nearby stellar explosions, with the variety of life being greatest when supernovae are plentiful. A likely reason, according to Prof. Svensmark, is that the cold climate associated with high supernova rates brings a greater variety of habitats between polar and equatorial regions, while the associated stresses of life prevent the ecosystems becoming too set in their ways.He also notices that most geological periods seem to begin and end with either an upturn or a downturn in the supernova rate. The changes in typical species that define a period, in the transition from one to the next, could then be the result of a major change in the astrophysical environment.Life’s prosperity, or global bioproductivity, can be tracked by the amount of carbon dioxide in the air at various times in the past as set out in the geological record. When supernova rates were high, carbon dioxide was scarce, suggesting that flourishing microbial and plant life in the oceans consumed it greedily to grow. Support for this idea comes from the fact that microbes and plants dislike carbon dioxide molecules that contain a heavy form of carbon atom, carbon-13. As a result, the ocean water is left enriched by carbon-13. The geological evidence shows high carbon-13 when supernovae were commonest – again pointing to high productivity. As to why this should be, Prof. Svensmark notes that growth is limited by available nutrients, especially phosphorus and nitrogen, and that cold conditions favour the recycling of the nutrients by vigorously mixing the oceans.Although the new analysis suggests, perhaps surprisingly, that supernovae are on the whole good for life, high supernova rates can bring the cold and changeable climate of prolonged glacial episodes. And they can have nasty shocks in store. Geoscientists have long been puzzled by many relatively brief falls in sea-level by 25 metres or more that show up in seismic soundings as eroded beaches. Prof. Svensmark finds that they are what can be expected when chilling due to very close supernovae causes short-lived glacial episodes. With frozen water temporarily bottled up on land, the sea-level drops.The data also support the idea of a long-term link between cosmic rays and climate, with these climatic changes underlying the biological effects. And compared with the temperature variations seen on short timescales as a consequence of the Sun’s influence on the influx of cosmic rays, the heating and cooling of the Earth due to cosmic rays varying with the prevailing supernova rate have been far larger.The director of DTU Space, Prof. Eigil Friis-Christensen, comments: “When this enquiry into effects of cosmic rays from supernova remnants began 16 years ago, we never imagined that it would lead us so deep into time, or into so many aspects of the Earth’s history. The connection to evolution is a culmination of this work.”

Did exploding stars help life on Earth to thrive?

Research by a Danish physicist suggests that the explosion of massive stars – supernovae – near the Solar System has strongly influenced the development of life. Prof. Henrik Svensmark of the Technical University of Denmark (DTU) sets out his novel work in a paper in the journal Monthly Notices of the Royal Astronomical Society.

Prof. Svensmark looked back through 500 million years of geological and astronomical data and considered the proximity of the Sun to supernovae as it moves around our Galaxy, the Milky Way. In particular, when the Sun is passing through the spiral arms of the Milky Way, it encounters newly forming clusters of stars. These so-called open clusters, which disperse over time, have a range of ages and sizes and will have started with a small proportion of stars massive enough to explode as supernovae. From the data on open clusters, Prof. Svensmark was able to deduce how the rate at which supernovae exploded near the Solar System varied over time.

Comparing this with the geological record, he found that the changing frequency of nearby supernovae seems to have strongly shaped the conditions for life on Earth. Whenever the Sun and its planets have visited regions of enhanced star formation in the Milky Way Galaxy, where exploding stars are most common, life has prospered. Prof. Svensmark remarks in the paper, “The biosphere seems to contain a reflection of the sky, in that the evolution of life mirrors the evolution of the Galaxy.”

In the new work, the diversity of life over the last 500 million years seems remarkably well explained by tectonics affecting the sea-level together with variations in the supernova rate, and virtually nothing else. To obtain this result on the variety of life, or biodiversity, he followed the changing fortunes of the best-recorded fossils. These are from invertebrate animals in the sea, such as shrimps and octopuses, or the extinct trilobites and ammonites.

They tended to be richest in their variety when continents were drifting apart and sea levels were high and less varied when the land masses gathered 250 million years ago into the supercontinent called Pangaea and the sea-level was lower. But this geophysical effect was not the whole story. When it is removed from the record of biodiversity, what remains corresponds closely to the changing rate of nearby stellar explosions, with the variety of life being greatest when supernovae are plentiful. A likely reason, according to Prof. Svensmark, is that the cold climate associated with high supernova rates brings a greater variety of habitats between polar and equatorial regions, while the associated stresses of life prevent the ecosystems becoming too set in their ways.

He also notices that most geological periods seem to begin and end with either an upturn or a downturn in the supernova rate. The changes in typical species that define a period, in the transition from one to the next, could then be the result of a major change in the astrophysical environment.

Life’s prosperity, or global bioproductivity, can be tracked by the amount of carbon dioxide in the air at various times in the past as set out in the geological record. When supernova rates were high, carbon dioxide was scarce, suggesting that flourishing microbial and plant life in the oceans consumed it greedily to grow. Support for this idea comes from the fact that microbes and plants dislike carbon dioxide molecules that contain a heavy form of carbon atom, carbon-13. As a result, the ocean water is left enriched by carbon-13. The geological evidence shows high carbon-13 when supernovae were commonest – again pointing to high productivity. As to why this should be, Prof. Svensmark notes that growth is limited by available nutrients, especially phosphorus and nitrogen, and that cold conditions favour the recycling of the nutrients by vigorously mixing the oceans.

Although the new analysis suggests, perhaps surprisingly, that supernovae are on the whole good for life, high supernova rates can bring the cold and changeable climate of prolonged glacial episodes. And they can have nasty shocks in store. Geoscientists have long been puzzled by many relatively brief falls in sea-level by 25 metres or more that show up in seismic soundings as eroded beaches. Prof. Svensmark finds that they are what can be expected when chilling due to very close supernovae causes short-lived glacial episodes. With frozen water temporarily bottled up on land, the sea-level drops.

The data also support the idea of a long-term link between cosmic rays and climate, with these climatic changes underlying the biological effects. And compared with the temperature variations seen on short timescales as a consequence of the Sun’s influence on the influx of cosmic rays, the heating and cooling of the Earth due to cosmic rays varying with the prevailing supernova rate have been far larger.

The director of DTU Space, Prof. Eigil Friis-Christensen, comments: “When this enquiry into effects of cosmic rays from supernova remnants began 16 years ago, we never imagined that it would lead us so deep into time, or into so many aspects of the Earth’s history. The connection to evolution is a culmination of this work.”

weareallstarstuff:

NGC 281
nebulosaplanetaria:

Night Sky from Natural Bridges (by Codeve)

nebulosaplanetaria:

Night Sky from Natural Bridges (by Codeve)

expose-the-light:

Baby Stars

1. Beautiful newborns

In a universe of fantastic images, a newborn star is a mystical masterpiece. Cradled within the dusty arms of a nebula, a baby star seems to blink its way to a new life. The lifespan of a star is a series of sequences. A star may spend most of its life in a “main sequence phase” where nuclear fusion of hydrogen into helium is happening in its core. But before this happens, it lives as a protostar, or baby star.

2. Young stars in Serpens

Here the Spitzer Space Telescope reveals the Serpens South star cluster, in which 50 or so young stars exist. They are seen as the “green, yellow, and orange-tinted specks sitting atop the black dust lane.” A supernova or galaxy collision can cause a star to form when huge clouds of hydrogen and helium collapse under mutual gravity. As the cloud collapses, it heats up and starts to spin. Since protostars are covered in dust, they can be seen only through infrared telescopes like Hubble and Spitzer. As Universe Today writes, “After about 100,000 years or so, the protostar stops growing and the disk of material surrounding it is destroyed by radiation.” Then this star, now called a T Tauri or pre-main sequence star, is visible from Earth.

3. Bubbly little star

We are used to images of babies blowing bubbles, and it looks like the infants of the cosmos do the same. This image, taken by the Spitzer Space Telescope, shows the HH 46/47 baby star blowing bubbles into space via powerful jets of gas. Located about 1,140 light-years from Earth, HH 46/47 is the bright white star at the middle of the image. Two bubbles reach out in opposite directions and are formed when the jets collide with the dust and gas surrounding the star

4. Young stars emerge from Orion’s head

Orion just might be the stud of our Milky Way, a fitting compliment because since the constellation takes its name from a Greek story of a legendary hunter. Pictured here is another “hatching” of baby stars located in the head of Orion. The Spitzer Space Telescope captures this area known as Barnard 30, which sits on the right side of Orion’s head. It is around 1,300 light-years away from Earth.

cwnl:

IRAS: Looking to the Heavens
The pearly wisps surrounding the central star IRAS 10082-5647 in this Hubble image certainly draw the eye towards the heavens. The divine-looking cloud is a reflection nebula, made up of gas and dust glowing softly by the reflected light of nearby stars, in this case a young Herbig Ae/Be star.
The star, like others of this type, is still a relative youngster, only a few million years old. It has not yet reached the so-called main sequence phase, where it will spend around 80% of its life creating energy by burning hydrogen in its core.
Credit: ESA/Hubble & NASA

cwnl:

IRAS: Looking to the Heavens

The pearly wisps surrounding the central star IRAS 10082-5647 in this Hubble image certainly draw the eye towards the heavens. The divine-looking cloud is a reflection nebula, made up of gas and dust glowing softly by the reflected light of nearby stars, in this case a young Herbig Ae/Be star.

The star, like others of this type, is still a relative youngster, only a few million years old. It has not yet reached the so-called main sequence phase, where it will spend around 80% of its life creating energy by burning hydrogen in its core.

Credit: ESA/Hubble & NASA