gazette inspiration collector / on space

Our Story

the video above is inspired from the video below. both worth watching

video 1:

A tapestry of footage tracing the cosmic and biological origins of our species, set to original music. mp3: melodysheep.bandcamp.com/track/our-story

Video sources:

image

  • Through The Wormhole with Morgan Freeman
  • Into the Universe with Stephen Hawking
  • Do We Really Need the Moon? BBC
  • How Planet Earth Was Made
  • David Attenborough’s First Life
  • Dinosaurs Alive
  • Journey to the Edge of the Universe
  • Last Day of the Dinosaurs
  • Walking With Cavemen
  • Human Planet
  • Mankind: The Story of All of Us
  • Hubble Ultra Deep Field
  • Wonders of the Universe
  • Quest for Fire
  • Baraka
  • The Tree of Life

video 2:

“My final project I made for my video productions class “Cutaway Productions” at my high school. I don’t own the rights to the song or the pictures and I am not trying to claim them, I just did this video for fun and i spent many a hour on it.” drivinman687

Song: Mind Heist (yes it is from Inception)
by: Zack Hemsey

Pictures: from all over the internet

some of the space pictures, are made by the digital artist “antifanfan

Grounded

by Kevin Margo

image

“One astronaut’s journey through space and life ends on a hostile exosolar planet. Grounded is a metaphorical account of the experience, inviting unique interpretation and reflection by the viewer. Themes of aging, inheritance, paternal approval, cyclic trajectories, and behaviors passed on through generations are explored against an ethereal backdrop.  About this Tip Jar - Did Grounded inspire you? My dad’s life inspired me and his death inspired Grounded. 100% proceeds of this Tip Jar (note vimeo’s 15% service fee) goes to the American Cancer Society in memory of Paul Vincent Margo. Or donate yourself to www.cancer.org

Kevin’s website / Grounded website / Credits

The Scale of the Universe 2
What does the universe look like on small scales? On large scales? Humanity is discovering that the universe is a very different place on every proportion that has been explored. For example, so far as we know, every tiny proton is exactly the same, but every huge galaxy is different. On more familiar scales, a small glass table top to a human is a vast plane of strange smoothness to a dust mite — possibly speckled with cell boulders. Not all scale lengths are well explored — what happens to the smallest mist droplets you sneeze, for example, is a topic of active research — and possibly useful to know to help stop the spread of disease. The below interactive flash animation, a modern version of the classic video Powers of Ten, is a new window to many of the known scales of our universe. By moving the scroll bar across the bottom, you can explore a diversity of sizes, while clicking on different items will bring up descriptive information. (text source)
experience it on the official website on it’s actual size
You need a more recent version of Adobe Flash Player. 
Flash Animation Credit & Copyright : Cary & Michael Huang
14 year old Cary said he invites people to correct any errors they find. This is the second version.
______Powers of Ten is a 1968 American documentary film written and directed by Charles and Ray Eames. The film depicts the relative scale of the Universe in factors of ten (see also logarithmic scale and order of magnitude)duration 9 mins

The Scale of the Universe 2

What does the universe look like on small scales? On large scales? Humanity is discovering that the universe is a very different place on every proportion that has been explored. For example, so far as we know, every tiny proton is exactly the same, but every huge galaxy is different. On more familiar scales, a small glass table top to a human is a vast plane of strange smoothness to a dust mite — possibly speckled with cell boulders. Not all scale lengths are well explored — what happens to the smallest mist droplets you sneeze, for example, is a topic of active research — and possibly useful to know to help stop the spread of disease. The below interactive flash animation, a modern version of the classic video Powers of Ten, is a new window to many of the known scales of our universe. By moving the scroll bar across the bottom, you can explore a diversity of sizes, while clicking on different items will bring up descriptive information. (text source)

experience it on the official website on it’s actual size

You need a more recent version of Adobe Flash Player.

Flash Animation Credit & Copyright : Cary & Michael Huang

14 year old Cary said he invites people to correct any errors they find. This is the second version.

______
Powers of Ten is a 1968 American documentary film written and directed by Charles and Ray Eames. The film depicts the relative scale of the Universe in factors of ten (see also logarithmic scale and order of magnitude)
duration 9 mins

The Average Color of the Universe 
Credit: Karl Glazebrook & Ivan Baldry (JHU)
Explanation: What color is the universe? More precisely, if the entire sky were smeared out, what color would the final mix be? This whimsical question came up when trying to determine what stars are commonplace in nearby galaxies. The answer, depicted above, is a conditionally perceived shade of beige. To determine this, astronomers computationally averaged the light emitted by one of the largest sample of galaxies yet analyzed: the 200,000 galaxies of the 2dF survey. The resulting cosmic spectrum has some emission in all parts of the electromagnetic spectrum, but a single perceived composite color. 
via NASA

The Average Color of the Universe

Credit: Karl Glazebrook & Ivan Baldry (JHU)

Explanation: What color is the universe? More precisely, if the entire sky were smeared out, what color would the final mix be? This whimsical question came up when trying to determine what stars are commonplace in nearby galaxies. The answer, depicted above, is a conditionally perceived shade of beige. To determine this, astronomers computationally averaged the light emitted by one of the largest sample of galaxies yet analyzed: the 200,000 galaxies of the 2dF survey. The resulting cosmic spectrum has some emission in all parts of the electromagnetic spectrum, but a single perceived composite color. 

via NASA

In the shadows of Saturn’s rings
Titan appears to be strung like a bead on Saturn’s rings, which cast shadows onto the southern hemisphere of the gas giant in this beautiful image from Cassini.
Faint but exquisite detail in the gas giant’s upper atmosphere paints a tranquil scene. A thin band of bright white ammonia ice clouds is etched into the planet’s disc towards the top of the image while clouds dotted below are faded scars of a huge storm that raged across the planet through much of 2011.
Shadows cast by Saturn’s iconic rings appear painted onto the planet’s southern hemisphere in two thick bands broken by thin, lighter stripes, reflecting the intricacies of the individual rings. As Saturn’s seasons progress towards northern hemisphere summer, the rings will appear to grow wider and wider.
Meanwhile Titan, Saturn’s largest moon, appears to hang on the planet’s rings like a bead on a necklace. The effect is a result of the line-of-sight viewing position; Titan orbits Saturn at an average distance of 1,221,870 km.
reblogged from unknownskywalker

In the shadows of Saturn’s rings

Titan appears to be strung like a bead on Saturn’s rings, which cast shadows onto the southern hemisphere of the gas giant in this beautiful image from Cassini.

Faint but exquisite detail in the gas giant’s upper atmosphere paints a tranquil scene. A thin band of bright white ammonia ice clouds is etched into the planet’s disc towards the top of the image while clouds dotted below are faded scars of a huge storm that raged across the planet through much of 2011.

Shadows cast by Saturn’s iconic rings appear painted onto the planet’s southern hemisphere in two thick bands broken by thin, lighter stripes, reflecting the intricacies of the individual rings. As Saturn’s seasons progress towards northern hemisphere summer, the rings will appear to grow wider and wider.

Meanwhile Titan, Saturn’s largest moon, appears to hang on the planet’s rings like a bead on a necklace. The effect is a result of the line-of-sight viewing position; Titan orbits Saturn at an average distance of 1,221,870 km.

reblogged from unknownskywalker

Transit of Venus

On June 5th, 2012, Venus will pass across the face of the sun, producing a silhouette that no one alive today will likely see again.

Transits of Venus are very rare, coming in pairs separated by more than a hundred years. This June’s transit, the bookend of a 2004-2012 pair, won’t be repeated until the year 2117. Fortunately, the event is widely visible. Observers on seven continents, even a sliver of Antarctica, will be in position to see it

The nearly 7-hour transit begins at 3:09 pm Pacific Daylight Time (22:09 UT) on June 5th. The timing favors observers in the mid-Pacific where the sun is high overhead during the crossing.  In the USA, the transit will at its best around sunset. That’s good, too. Creative photographers will have a field day imaging the swollen red sun “punctured” by the circular disk of Venus.

Observing tip: Do not stare at the sun. Venus covers too little of the solar disk to block the blinding glare.  Instead, use some type of projection technique or a solar filter. A #14 welder’s glass is a good choice…more

check the links below for more info
link 1

link 2

The Transit of Venus / myth

LIVE link from NASA on 5th of June

Celestial Lights

a video by Ole C. Salomonsen

image

“auroras are caused by solar activity. This is shortly visualized in the video. Our suns activity varies in 11 year cycles, and we are closing solar maximum (solar max) for our current solar cycle somewhere between 2012-2013, and solar activity has clearly been picking up. The beginning of 2011 was lots of clouds but weather improved late 2011 and out 2012. This video contains recordings from some of the most spectacular auroral displays I have ever witnessed, and I have seen a few.

For this video I did shoot approx 150.000 exposures from sept.2011 - april.2012 using Canon DSLR’s and various wide angle lenses. Approx 6.000 frames in this video. To achieve pannings I used the fantastic Stage Zero + MX2 controller time-lapse gear from Dynamic Perception.

The video is a merge of two parts; the first part contains some more wild and aggressive auroras, as well as a few milky way sequences, hence either auroras are moving fast because they are, or they are fast due to motion of the milky way / stars. Still, some of the strait up shots are very close to real-time speed, although auroras mostly are slower, she can also be FAST! The second part has some more slow and majestic auroras, where I have focused more on composition and foreground. The music should give you a clear indication of where you are…” more

Red Dwarf Star
Distant rocky planet ‘could be future human home’ 
While Gliese 581d shows potential, it would take around 300,000 years to get there with current space traveling technology.
PARIS — A rocky world orbiting a nearby star has been confirmed as the first planet outside our solar system to meet key requirements for sustaining life, scientists said on Monday.
 
Modelling of planet Gliese 581d shows it has the potential to be warm and wet enough to nurture Earth-like life, they said.
 
It orbits a red dwarf star called Gliese 581, located around 20 light years from Earth, which makes it one of our closest neighbours.
 
Gliese 581d orbits on the outer fringes of the star’s “Goldilocks zone”, where it is not so hot that water boils away, nor so cold that water is perpetually frozen. Instead, the temperature is just right for water to exist in liquid form.
 
“With a dense carbon dioxide atmosphere — a likely scenario on such a large planet — the climate of Gliese 581d is not only stable against collapse but warm enough to have oceans, clouds and rainfall,” France’s National Centre for Scientific Research said in a press release.
 
More than 500 planets orbiting other stars have been recorded since 1995, detected mostly by a tiny wobble in stellar light.
Exoplanets are named after their star and listed alphabetically, in order of discovery.
 
Until now, the big interest in Gliese 581’s roster of planets focussed on Gliese 581g.
 
It leapt into the headlines last year as “Zarmina’s World,” after its observers announced it had roughly the same mass as Earth’s and was also close to the Goldilocks zone.
 
But that discovery has since been discounted by many. Indeed, some experts suspect that the Gliese 581g may not even exist but was simply a hiccup in starlight.
 
Its big brother, Gliese 581d, has a mass at least seven times that of Earth and is about twice our planet’s size, according to the new study, which appears in a British publication, The Astrophysical Journal Letters.
 
The planet, spotted in 2007, had initially been dismissed as a candidate in the hunt for life.
 
It receives less than a third of the solar radiation Earth gets, and may be “tidally locked”, meaning that one side of it always faces the sun, which would give it permanent dayside and nightside.
 
But the new model, devised by CNRS climate scientists Robin Wordsworth, Francois Forget and colleagues, showed surprising potential.
 
Its atmosphere would store heat well, thanks to its dense CO2, a greenhouse gas. And the red light from the star would also penetrate the atmosphere and warm the surface.
 
“In all cases, the temperatures allow for the presence of liquid water on the surface,” say the researchers.
 
For budding travellers, though, Gliese 581d would “still be a pretty strange place to visit,” the CNRS said.
 
“The denser air and thick clouds would keep the surface in a perpetual murky red twilight, and its large mass means that surface gravity would be around double that on Earth.”
 
Getting to the planet would still require a sci-fi breakthrough in travel for earthlings.
 
A spaceship travelling close to light speed would take more than 20 years to get there, while our present rocket technology would take 300,000 years.

Red Dwarf Star

Distant rocky planet ‘could be future human home’

While Gliese 581d shows potential, it would take around 300,000 years to get there with current space traveling technology.

PARIS — A rocky world orbiting a nearby star has been confirmed as the first planet outside our solar system to meet key requirements for sustaining life, scientists said on Monday.
 
Modelling of planet Gliese 581d shows it has the potential to be warm and wet enough to nurture Earth-like life, they said.
 
It orbits a red dwarf star called Gliese 581, located around 20 light years from Earth, which makes it one of our closest neighbours.
 
Gliese 581d orbits on the outer fringes of the star’s “Goldilocks zone”, where it is not so hot that water boils away, nor so cold that water is perpetually frozen. Instead, the temperature is just right for water to exist in liquid form.
 
“With a dense carbon dioxide atmosphere — a likely scenario on such a large planet — the climate of Gliese 581d is not only stable against collapse but warm enough to have oceans, clouds and rainfall,” France’s National Centre for Scientific Research said in a press release.
 
More than 500 planets orbiting other stars have been recorded since 1995, detected mostly by a tiny wobble in stellar light.
Exoplanets are named after their star and listed alphabetically, in order of discovery.
 
Until now, the big interest in Gliese 581’s roster of planets focussed on Gliese 581g.
 
It leapt into the headlines last year as “Zarmina’s World,” after its observers announced it had roughly the same mass as Earth’s and was also close to the Goldilocks zone.
 
But that discovery has since been discounted by many. Indeed, some experts suspect that the Gliese 581g may not even exist but was simply a hiccup in starlight.
 
Its big brother, Gliese 581d, has a mass at least seven times that of Earth and is about twice our planet’s size, according to the new study, which appears in a British publication, The Astrophysical Journal Letters.
 
The planet, spotted in 2007, had initially been dismissed as a candidate in the hunt for life.
 
It receives less than a third of the solar radiation Earth gets, and may be “tidally locked”, meaning that one side of it always faces the sun, which would give it permanent dayside and nightside.
 
But the new model, devised by CNRS climate scientists Robin Wordsworth, Francois Forget and colleagues, showed surprising potential.
 
Its atmosphere would store heat well, thanks to its dense CO2, a greenhouse gas. And the red light from the star would also penetrate the atmosphere and warm the surface.
 
“In all cases, the temperatures allow for the presence of liquid water on the surface,” say the researchers.
 
For budding travellers, though, Gliese 581d would “still be a pretty strange place to visit,” the CNRS said.
 
“The denser air and thick clouds would keep the surface in a perpetual murky red twilight, and its large mass means that surface gravity would be around double that on Earth.”
 
Getting to the planet would still require a sci-fi breakthrough in travel for earthlings.
 
A spaceship travelling close to light speed would take more than 20 years to get there, while our present rocket technology would take 300,000 years.
The Case of the Missing Dark Matter
A survey of the galactic region around our solar system by the European Southern Observatory (ESO) has turned up a surprising lack of dark matter, making its alleged existence even more of a mystery.
Dark matter is an invisible substance that is suspected to exist in large quantity around galaxies, lending mass but emitting no radiation. The only evidence for it comes from its gravitational effect on the material around it… up to now, dark matter itself has not been directly detected. Regardless, it has been estimated to make up 80% of all the mass in the Universe.
A team of astronomers at ESO’s La Silla Observatory in Chile has mapped the region around over 400 stars near the Sun, some of which were over 13,000 light-years distant. What they found was a quantity of material that coincided with what was observable: stars, gas, and dust… but no dark matter.
“The amount of mass that we derive matches very well with what we see — stars, dust and gas — in the region around the Sun,” said team leader Christian Moni Bidin of the Universidad de Concepción in Chile. “But this leaves no room for the extra material — dark matter — that we were expecting. Our calculations show that it should have shown up very clearly in our measurements. But it was just not there!”
Based on the team’s results, the dark matter halos thought to envelop galaxies would have to have “unusual” shapes — making their actual existence highly improbable.
Still, something is causing matter and radiation in the Universe to behave in a way that belies its visible mass. If it’s not dark matter, then what is it?
“Despite the new results, the Milky Way certainly rotates much faster than the visible matter alone can account for,” Bidin said. “So, if dark matter is not present where we expected it, a new solution for the missing mass problem must be found.
“Our results contradict the currently accepted models. The mystery of dark matter has just became even more mysterious.”

The Case of the Missing Dark Matter

A survey of the galactic region around our solar system by the European Southern Observatory (ESO) has turned up a surprising lack of dark matter, making its alleged existence even more of a mystery.

Dark matter is an invisible substance that is suspected to exist in large quantity around galaxies, lending mass but emitting no radiation. The only evidence for it comes from its gravitational effect on the material around it… up to now, dark matter itself has not been directly detected. Regardless, it has been estimated to make up 80% of all the mass in the Universe.

A team of astronomers at ESO’s La Silla Observatory in Chile has mapped the region around over 400 stars near the Sun, some of which were over 13,000 light-years distant. What they found was a quantity of material that coincided with what was observable: stars, gas, and dust… but no dark matter.

“The amount of mass that we derive matches very well with what we see — stars, dust and gas — in the region around the Sun,” said team leader Christian Moni Bidin of the Universidad de Concepción in Chile. “But this leaves no room for the extra material — dark matter — that we were expecting. Our calculations show that it should have shown up very clearly in our measurements. But it was just not there!”

Based on the team’s results, the dark matter halos thought to envelop galaxies would have to have “unusual” shapes — making their actual existence highly improbable.

Still, something is causing matter and radiation in the Universe to behave in a way that belies its visible mass. If it’s not dark matter, then what is it?

“Despite the new results, the Milky Way certainly rotates much faster than the visible matter alone can account for,” Bidin said. “So, if dark matter is not present where we expected it, a new solution for the missing mass problem must be found.

“Our results contradict the currently accepted models. The mystery of dark matter has just became even more mysterious.”

(via quantumaniac)

Reblogged from Quantumaniac

Umbra

by Malcolm Sutherland

image

An explorer adventures into an unknown world, yet it seems that he has been there before…

music by Alison Melville and Ben Grossman, and foley by Leon Lo. Sound design / mix by Malcolm Sutherland.

The animation is all hand-drawn; a mix of drawing / pastels on paper and digital animation.