Showing posts with label Astronomy. Show all posts
Showing posts with label Astronomy. Show all posts

Thursday, February 28, 2013

APOTD: Ghost Nebula



Caption: NOAO

This image was obtained with the wide-field view of the Mosaic Camera on the Mayall 4-meter telescope at Kitt Peak National Observatory. vdB 141 is a reflection nebula located in the constellation Cepheus. Sometimes referred to as the ghost nebula, its awkward name is its catalog number in Sidney van den Bergh's catalog of reflection nebulae, published in 1966. Several stars are embedded in the nebula. Their light gives it a ghoulish brown color. North is down and East is to the right. Imaged August 28, 2009.

Image: T.A. Rector/University of Alaska Anchorage, H. Schweiker/WIYN and NOAO/AURA/NSF [high-resolution] Read NOAO Conditions of Use before downloading

Tuesday, January 29, 2013

APOTD: Molecular Cloud in Monoceros

Image: T.A. Rector (University of Alaska Anchorage) and N.S. van der Bliek (NOAO/AURA/NSF) [high-resolution] Read NOAO Conditions of Use before downloading

Caption: NOAO

This image was obtained with the wide-field view of the Mosaic II camera on the Blanco 4-meter telescope at Cerro Tololo Interamerican Observatory on January 11th, 2012. It shows a portion of the giant Monceros R2 molecular cloud. It is a location of massive star formation, particularly in the location of the bright red nebula just below the center of the image. The image was generated with observations in the Sulphur [SII] (blue) and Hydrogen-Alpha (red) filters. In this image, north is to the right, and east is up.

Wednesday, January 23, 2013

APOTD: Soap Bubble Nebula

Image: T. A. Rector/University of Alaska Anchorage, H. Schweiker/WIYN 
and NOAO/AURA/NSF [high-resolution]

Caption: NOAO

nformally known as the "Soap Bubble Nebula", this planetary nebula (officially known as PN G75.5+1.7) was discovered by amateur astronomer Dave Jurasevich on July 6th, 2008. It was noted and reported by Keith Quattrocchi and Mel Helm on July 17th, 2008. This image was obtained with the Kitt Peak Mayall 4-meter telescope on June 19th, 2009 in the H-alpha (orange) and [OIII] (blue) narrowband filters. In this image, north is to the left and east is down.

PN G75.5+1.7 is located in the constellation of Cygnus, not far from the Crescent Nebula (NGC 6888). It is embedded in a diffuse nebula which, in conjunction with its faintness, is the reason it was not discovered until recently. The spherical symmetry of the shell is remarkable, making it very similar to Abell 39.
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Monday, January 21, 2013

APOTD: Saturn's Glowing Aurora

Image: NASA/JPL/University of Arizona/University of Leicester[high-resolution]

Caption: Cassini Solstice team

This false-color composite image, constructed from data obtained by NASA's Cassini spacecraft, shows the glow of auroras streaking out about 1,000 km (600 miles) from the cloud tops of Saturn's south polar region. It is among the first images released from a study that identifies images showing auroral emissions out of the entire catalogue of images taken by Cassini's visual and infrared mapping spectrometer.

In this image constructed from data collected in the near-infrared wavelengths of light, the auroral emission is shown in green. The data represents emissions from hydrogen ions in of light between 3 and 4 microns in wavelength. In general, scientists designated blue to indicate sunlight reflected at a wavelength of 2 microns, green to indicate sunlight reflected at 3 microns and red to indicate thermal emission at 5 microns. Saturn's rings reflect sunlight at 2 microns, but not at 3 and 5 microns, so they appear deep blue. Saturn's high altitude haze reflects sunlight at both 2 and 3 microns, but not at 5 microns, and so it appears green to blue-green. The heat emission from the interior of Saturn is only seen at 5 microns wavelength in the spectrometer data, and thus appears red. The dark spots and banded features in the image are clouds and small storms that outline the deeper weather systems and circulation patterns of the planet. They are illuminated from underneath by Saturn's thermal emission, and thus appear in silhouette.

The composite image was made from 65 individual observations by Cassini's visual and infrared mapping spectrometer on 1 November 2008. The observations were each six minutes long.

Monday, January 14, 2013

APOTD: Tectonics on Enceladus


On Oct. 5, 2008, just after coming within 25 kilometers (15.6 miles) of the surface of Enceladus, NASA's Cassini captured this stunning mosaic as the spacecraft sped away from this geologically active moon of Saturn.

Craters and cratered terrains are rare in this view of the southern region of the moon's Saturn-facing hemisphere. Instead, the surface is replete with fractures, folds, and ridges—all hallmarks of remarkable tectonic activity for a relatively small world. In this enhanced-color view, regions that appear blue-green are thought to be coated with larger grains than those that appear white or gray. Portions of the tiger stripe fractures, or sulci, are visible along the terminator at lower right, surrounded by a circumpolar belt of mountains. The icy moon's famed jets emanate from at least eight distinct source regions, which lie on or near the tiger stripes. However, in this view, the most prominent feature is Labtayt Sulci, the approximately one-kilometer (0.6 miles) deep northward-trending chasm located just above the center of the mosaic.

Near the top, the conspicuous ridges are Ebony and Cufa Dorsae. This false-color mosaic was created from 28 images obtained at seven footprints, or pointing positions, by Cassini's narrow-angle camera. At each footprint, four images using filters sensitive to ultraviolet, visible and infrared light (spanning wavelengths from 338 to 930 nanometers) were combined to create the individual frames. The mosaic is an orthographic projection centered at 64.49 degrees south latitude, 283.87 west longitude, and it has an image scale of 196 kilometers (122.5 miles) per pixel. The original images ranged in resolution from 180 meters (594 feet) to 288 meters (950 feet) per pixel and were acquired at distances ranging from 30,000 to 48,000 kilometers (18,750 to 30,000 miles) as the spacecraft receded from Enceladus. The view was acquired at a Sun-Enceladus-spacecraft, or phase, angle of 73 degrees.

Image: NASA/JPL/Space Science Institute [high-resolution]
Caption: NASA

Sunday, December 30, 2012

APOTD: A Star Making Waves




VIA: NASA/JPL:

"The giant star Zeta Ophiuchi is having a "shocking" effect on the surrounding dust clouds in this infrared image from NASA's Spitzer Space Telescope. Stellar winds flowing out from this fast-moving star are making ripples in the dust as it approaches, creating a bow shock seen as glowing gossamer threads, which, for this star, are only seen in infrared light.

Zeta Ophiuchi is a young, large and hot star located around 370 light-years away. It dwarfs our own sun in many ways -- it is about six times hotter, eight times wider, 20 times more massive, and about 80,000 times as bright. Even at its great distance, it would be one of the brightest stars in the sky were it not largely obscured by foreground dust clouds.

This massive star is travelling at a snappy pace of about 54,000 mph (24 kilometers per second), fast enough to break the sound barrier in the surrounding interstellar material. Because of this motion, it creates a spectacular bow shock ahead of its direction of travel (to the left). The structure is analogous to the ripples that precede the bow of a ship as it moves through the water, or the sonic boom of an airplane hitting supersonic speeds.

The fine filaments of dust surrounding the star glow primarily at shorter infrared wavelengths, rendered here in green. The area of the shock pops out dramatically at longer infrared wavelengths, creating the red highlights.

A bright bow shock like this would normally be seen in visible light as well, but because it is hidden behind a curtain of dust, only the longer infrared wavelengths of light seen by Spitzer can reach us.
Bow shocks are commonly seen when two different regions of gas and dust slam into one another. Zeta Ophiuchi, like other massive stars, generates a strong wind of hot gas particles flowing out from its surface. This expanding wind collides with the tenuous clouds of interstellar gas and dust about half a light-year away from the star, which is almost 800 times the distance from the sun to Pluto. The speed of the winds added to the star's supersonic motion result in the spectacular collision seen here.

Our own sun has significantly weaker solar winds and is passing much more slowly through our galactic neighborhood so it may not have a bow shock at all. NASA's twin Voyager spacecraft are headed away from the solar system and are currently about three times farther out than Pluto. They will likely pass beyond the influence of the sun into interstellar space in the next few years, though this is a much gentler transition than that seen around Zeta Ophiuchi.

For this Spitzer image, infrared light at wavelengths of 3.6 and 4.5 microns is rendered in blue, 8.0 microns in green, and 24 microns in red.

JPL manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at Caltech. Data are archived at the Infrared Science Archive housed at the Infrared Processing and Analysis Center at Caltech."

For more information about Spitzer, visit http://spitzer.caltech.edu and http://www.nasa.gov/spitzer.

And Now, Neil deGrasse Tyson Dances To Michael Jackson


There WILL be gifs. Oh, yes- There WILL be gifs.

Seriously though, I'm making gifs.

-CAINE-

Tuesday, November 20, 2012

Astronomers Believed to Have Found First Rogue planet




Posted by YouTube user: VideoFromSpace

In case you're completely unfamiliar:

Rouge (nomadic/orphan/ETC) planets are, well, exactly what they sound like- planetary bodies which are not gravitationally bound to a parent star or system; instead revolving around galaxies themselves. These objects are believed to occur as a result of their having either been ejected from a parent system, or developing as a type of sub brown dwarf (objects that never quite attained enough mass to achieve fusion and become a star) that was never actually bound to any other object in the first place. Last week, a team of astrophysicists from the University of Montreal, reported the discovery of what they believe to be the first direct observation of such a planet.

The object in question; Planet "CFBDSIR2149" - which isn't even the entire designation for the object BTW- was found amongst a group of  relatively young stars (around 50-120 million years old) which make up a formation called the AB Doradus Moving group. The apparent planet's "close" proximity to our own, around 75 light years from Earth, and the fact that there isn't a nearby parent star obstructing our view with it's own intense glow, means researchers have actually been able to do a detailed analysis of the object's atmosphere.

Actual image of newly found rogue planet CFBDSIR2149.
Image Credit: CFHT/P. Delorme
Using infrared imaging collected from the Canada-France-Hawaii Telescope (CFHT) and the European Southern Observatory's Very Large Telescope (VLT.), researchers have determined  CFBDSIR2149 to be a gas giant with a mass 4 to 7 times that of Jupiter, and an average temperature of around 450 degrees Celsius (850 degrees Fahrenheit).

This isn't actually the first potential rogue planet ever to have been discovered. And there is always a chance that further observation could contradict these initial findings, given that this is the closest and least obstructed candidate yet known. But it seems likely at this stage that CFBDSIR2149, will end up as our first confirmed observation of an unbound planetary mass. 

Oh, and in case you were wondering. Yes, people have already started asking the "Nibiru" question. Is Ancient Astronauts still a thing? And are they currently filming? If so, $20 says they're the first to work this angle into their...um, "theories".

-CAINE-

SOURCE: UdeMNouvelles, SLATE/BadAstronomy

Thursday, November 8, 2012

In Other Neil deGrasse Tyson News...


Neil shows up in Action Comics #14, to help superman find Krypton. Which, it turns out,

“is found 27.1 light-years from Earth, in the southern constellation Corvus (The Crow), orbiting  the red dwarf star LHS 2520, which is cooler and smaller than our sun.”

Just in case you’re not sure, comic books aren’t real, so neither is planet Krypton. Though its a safe bet that it will be someday, in name anyway, should we ever actually find a planet orbiting LHS 2520, which is a real life star, located 2.7 years from Earth, ETC, Etc.

-CAINE-

VIA:Scientific American

Wednesday, May 23, 2012

APOTD: Late Afternoon SHadows at Endeavour Crater on Mars

Image credit: NASA/JPL-Caltech/Cornell/Arizona State Univ.

NASA’s Mars Rover Opportunity catches its own late-afternoon shadow in this dramatically lit view eastward across Endeavour Crater on Mars.

The rover used the panoramic camera (Pancam) between about 4:30 and 5:00 p.m. local Mars time to record images taken through different filters and combined into this mosaic view.

Most of the component images were recorded during the 2,888th Martian day, or sol, of Opportunity’s work on Mars (March 9, 2012). At that time, Opportunity was spending low-solar-energy weeks of the Martian winter at the Greeley Haven outcrop on the Cape York segment of Endeavour’s western rim. In order to give the mosaic a rectangular aspect, some small parts of the edges of the mosaic and sky were filled in with parts of an image acquired earlier as part of a 360-degree panorama from the same location.

Opportunity has been studying the western rim of Endeavour Crater since arriving there in August 2011. This crater spans 14 miles (22 kilometers) in diameter, or about the same area as the city of Seattle. This is more than 20 times wider than Victoria Crater, the largest impact crater that Opportunity had previously examined. The interior basin of Endeavour is in the upper half of this view.

The mosaic combines about a dozen images taken through Pancam filters centered on wavelengths of 753 nanometers (near infrared), 535 nanometers (green) and 432 nanometers (violet). The view is presented in false color to make some differences between materials easier to see, such as the dark sandy ripples and dunes on the crater’s distant floor.

VIA: NASA.gov

Friday, April 6, 2012

Does New Data Challenge Giant Impact Theory?

Image Credit: Joe Tucciarone

Sometimes referred to as "the big splat" or "the big splash" hypothesis, the giant impact hypothesis is currently the most widely accepted explanation for the formation of Earth's only moon. According to this theory, sometime in our planet's distant past -as in, around 4.6 billion years ago- Earth was struck by a Mars-sized object dubbed Theia. This impact resulted in the ejection of a portion of material from the Earth's surface, which, along with Theia's remains, eventually coalesced to form the moon we see today. While there are, of course, several popular alternate explanations for the formation of our moon, none of them are as well supported by either physical observations or experimental results as the Giant impact theory; hence it's place of prominence on the issue.

One of the methods of testing the giant impact theory is to compare the isotope structure of basic elements found within rocks both on the moon and here on Earth. Because the the number of neutrons contained within each elemental isotope's nucleus can change, finding, say, an oxygen isotope with same atomic structure to be present in both samples, is a strong indicator that the samples in question originated from the same place. Which is exactly what previous analysis of lunar materials have shown.

But if 40% of the moon is made of the remains of the hypothetical object known as Theia, as is proposed by the giant impact theory. Then one would expect to eventually find some variance in the isotope structure of elements found in materials on the moon vs those on Earth, as those originating from Theia would presumably have been slightly different. But so far, that isn't the case. In fact, a recent analysis conducted by geochemists led by Junjun Zhang at the University of Chicago in Illinois, together with a colleague at the University of Bern in Switzerland, found, not only oxygen isotopes, but that also titanium isotopes taken from lunar materials, were identical to those found on Earth, which is a significant result. Because, while oxygen isotopes on each body could have been homogenized as a result of the formation process (meaning, oxygen isotopes originating from Theia cold basically have been "burnt off" and replaced) the high boiling point of titanium makes the same explanation an unlikely one for the presence of identical titanium isotopes.

So if the Giant impact hypothesis is correct, Thia really was a thing, and it's remains now account for 40% of the material on the moon, then why haven't we found any pieces of it yet?

The answer, of course, could be as simple as scientists having over estimated the size of Theia, that we merely haven't managed to collect a sample of it's remains yet, or some other variable or detail that we have yet to discover. But while it's an absolute certainty that the details of the Giant impact theory will change over time as new discoveries are made, and I think instances like this are both interesting and important examples of how the scientific process works. I think it's unlikely that this single data set will lead to the dethroning of the theory, and I'm personally not even convinced that it's a significant contradiction of previous findings, as the giant impact theory still accounts for more observed physical effects both on the Earth as well as the moon, than any of the alternate lunar formation theories around today.

-CAINE-

VIA: ScienceNOW

Friday, January 20, 2012

Herschel's Revisit of The Pillars of Creation


Alright, let's take a break from the SOPA/Internet censorship debacle, for something that isn't depressing and awful. The ESA's Herschel space observatory's revisit of the Eagle Nebula, or "Pillars of Creation" as it has been dubbed.

The rest of the text in this entry comes from the HSO website.

In 1995, NASA's Hubble Space Telescope took an iconic image of the Eagle nebula, dubbed the "Pillars of Creation," highlighting its finger-like pillars where new stars are thought to be forming. Now, the Herschel Space Observatory has a new, expansive view of the region captured in longer-wavelength infrared light.

The Herschel mission is led by the European Space Agency, with important NASA contributions.

The Eagle nebula is 6,500 light-years away in the constellation of Serpens. It contains a young, hot star cluster, NGC6611, visible with modest backyard telescopes, which is sculpting and illuminating the surrounding gas and dust. The result is a huge, hollowed-out cavity and pillars, each several light-years long.

The new Herschel image shows the pillars and the wide field of gas and dust around them. Captured in far-infrared wavelengths, the image allows astronomers to see inside the pillars and structures in the region. Herschel's image also makes it possible to search for young stars over a much wider region, and come to a much fuller understanding of the creative and destructive forces inside the Eagle nebula.

VIA: Herschel Space Observatory

Friday, January 6, 2012

The Growing Evidence for Mars' Watery Past

From questioning the probability of life of distant worlds, we turn to evidence of life, past or present, on worlds within our own solar system. Beginning with a look at the mounting evidence suggesting that Mars may, at the very least, have once been home to one of the key elements to the development of life as we understand it, Water.

In 1877, Italian astronomer Giovanni Schiaparelli, was the first to suggest that water may have once flowed on the Martian surface, after observing what he described as canals or "Canali", crisscrossing the planet's surface. Years later, in 1895, astronomer Percival Lowell, concluded that Schiaparelli's canals, must have been the work of a once great Martian civilization. Though we all now know that no such civilization ever existed on the red planet, and that even the canals themselves don't actually exist. Today, the consensus amongst planetary scientists still seems to be that Mars was once a wet world, much more similar to our own than it is today.

Observations made in recent years during various missions to Mars, have revealed, amongst other things, the presence of Jarosite -a mineral formed in the presence of highly acidic water- as well as gypsum, and other water-based minerals on the Martian surface. In 2008, the Pheonix lander confirmed the presence of water ice just beneath the soil in the planet's southern hemisphere. And in August of last year, images from the HRISE camera on board the Mars Reconnaissance orbiter, seemed to suggest that small amounts of salt water might still be seeping out from just beneath the planets soil.



A series of dark trails were observed radiating down from the edges of steep slopes of Mars' Newton Basin crater in the planet's southern hemisphere. Evidence suggested those lines may have been created by small amounts of salt water -lying frozen on or just beneath the soil- melting in the heat of the sun, and then trickling down the basin slopes. However, no one actually saw the water itself and instruments on board the MRO also failed to detect the presence of water in the Martian atmosphere. So the actual cause of those mysterious dark lines, remains inconclusive.


But the most recent, and what is being described as the most unambiguous evidence yet seen for the presence of liquid water in Mars' past, came in December of last year with the announcement that the Opportunity rover had discovered a small vein of Gypsum (seen in the false-color image to the left) just above the bedrock around the rim of Mars' Endeavor crater. Unlike previous detections of the mineral in the loose sands of various dunes, this newly found deposit -which is only 16 - 20 inches long, and about the width of a human thumb- was found in a fixed state, right where it was originally formed. A fact which Opportunity's principal investigator Steve Squyres, referred to as a; "slam-dunk story that water flowed through underground fractures in the rock,".

Normally, this would be the part where I warn you not to get to excited about the implications of such findings. And like any other new scientific discovery, this one will require multiple confirmations before it truly becomes an accepted fact. But it does, to my completely uneducated eye, seem as though the Phoenix rover's latest find is in fact another major step towards the absolute confirmation of Mars' watery past. Which would obviously have profound implications where the potential for life on the red planet -past or present- is concerned. But then again, I know as much about geology, as I do the ancient Mongolian art of fish-juggling. Which is to say nothing, since I just made that whole fish-juggling thing up. So I guess we'll just have to wait and see.

-CAINE-

Source: NASA/JPL
Image credits: NASA/JPL/Caltech/Cornel/ASU

Wednesday, January 4, 2012

Planetquest: A Historic Timeline of the Search for Exoplanets


Posted by Youtube user: Best0fScience

If you'd like to learn more about the history of the search for exoplanets, check out this video from Planetquest, which gives a detailed account of exactly that. Chances are, the search for worlds outside our own solar system has been going on for longer than you think.

-CAINE-

You can checkout more videos from Planetquest HERE.

Tuesday, January 3, 2012

Exoplanets Everywhere: Kepler's ongoing Search for Other Worlds

Artists depiction of Kepler 11, a system with 6 known planets.

Launched in 2009, the Kepler spacecraft was designed to search a portion of the milky way for sings of other worlds. More specifically, Kepler specializes in searching for earth sized planets which, because of their relatively small size, are much more difficult to detect than the giants that have typically been identified in the past. Since it's launch, Kepler has managed to identify a total of 2, 326 potential planets orbiting around other stars in the in the tiny swatch of the Milky Way it's been tasked with searching.

When an object of a significant enough size passes in front of any star within Kepler's field of view (that's about 150,000, in case you were wondering), it causes a dip in the magnitude of light being emitted by the star. Revealing, not only the presence of any extrasolar planets around said star, but also the distance at which those planets orbit their parent star. This method of detection is commonly referred to as the transit method, and like any other method of detecting such planets, requires multiple observations for confirmation.

In the latest wave of confirmed observations, NASA announced that Kepler had identified the two smallest planets ever confirmed around another star; Kepler20-e (Diameter:11,100 km (6900 miles) and Kepler 20f (Diameter:13,200 km (8200 miles). Found in orbit around the star Kepler 20, located 950 light years from Earth in the Lyra constellation, these newly discovered Earth-sized planets join 3 other known planets in the system (Kepler 20, a,b, and c), all of which are closer in size to Neptune or Uranus. Though Kepler 20 e and f may in fact be the closet size match to Earth yet discovered, the proximity around which they orbit their parent star -which is extremely similar in size and intensity to our own sun- means they'd have average surface temperatures in the range of 800 -1400 degrees F. Making them both far from Earth-like, where their potential for habitation is concerned. That title may actually belong to another newly discovered planet that was also revealed just this month: Kepler 22b.


Found Orbiting the class G star Kepler 22, which is located around 600 light years from Earth in the Cygnus constellation. Planet Kepler 22b, was found to have a 290 day orbital cycle, which places the planet within what we have defined as the habitable zone of its parent star; which is lower in mass, and cooler than our own sun. But there's a catch. While the planet's diameter is estimated to be around 2.4 times that of Earth's, the actual mass of the planet is impossible to determine based on Kepler's observations alone. So it's impossible to say weather or not Kepler 22b is a rocky planet like Earth, or gaseous ball like Jupiter and Saturn. But if it is a world like our own, and assuming that it also has the proper atmosphere Kepler 22b would have an estimated average surface temperature of around 72 degrees F. Which would make it not only the most Earth-like world yet discovered, but also the most likely home for life as we know it outside of our own solar system. The prospect is obviously tantalizing.

To date, scientists have confirmed the existence of over 500 exoplanets * using Kepler, The Hubble Space Telescope, and various other observational techniques. As time goes on, even more discoveries will be made, and long term observations will slowly scratch all of the potential candidates off Kepler's list; possibly resulting in the confirmed discovery of several thousand more worlds orbiting stars light years away from our own. And while it will likely be some time before we ever definitively confirm that conditions on one those planets is conducive to life. The apparent abundance of stars with planetary systems would seem to suggest that it's only a matter of time before we do. And even if we can't say for certain that there's life on any of those planets, to think that we live in a time when discovering worlds in other star systems has become common place, is astonishing, to say the least.

-CAINE-

Source: NASA1, NASA2
Image credit: Kepler 11- NASA/Tim Pyle, Kepler 20e, 20 f, and 22b- NASA/Ames/JPL-Caltech

*The exact number of confirmed exoplanets was actually kind of hard to nail down, The Extrasolar Planets Encyclopedia claims 716. But the most common figure I found was in the 500-600 range.

Sunday, September 18, 2011

Kepler Finds it's First Circumbinary Planet (Insert Obligatory Star Wars Refernce Here)

Image Credit: NASA

NASA's Kepler mission has announced the first direct detection of a circumbinary planet – a planet orbiting two stars- in a binary star system designated Kepler-16, located 200 light-years from Earth. While potential planets have previously been detected in other binary systems, Kepler-16b, as this newest exoplanet is now known, is the first confirmed planet to have been observed orbiting both it's parent stars.

A binary star system, as the name suggests, is a system with two stars orbiting around a common center of mass. Because from our vantage point on Earth, each of the two stars regularly passes in front of the other during their orbit, Kepler-16 is classified as an eclipsing binary.

Observations of Kepler-16 showed a drop in light from the system, not only when the stars eclipsed one another, as expected, but also a when neither star was eclipsing the other, indicating the presence of a much smaller 3rd object orbiting around them. By measuring the gravitational tug applied to the stars by this third objects, scientists were able to estimate it's mass, and Kepler-16b, as the new planet is now known, is believed to be a cold, uninhabitable world, about the size of Saturn, comprised of gas and rock.

Though Kepler-16b may be a cold, gaseous world -incapable of harboring any Jedi resistance fighters -or even sand people. As Kepler's Principal investigator William Borucki points out, the confirmation of a planet orbiting in a binary system - which are much more common than the single star system in which we reside-

"confirms a new class of planetary systems that could harbor life,"
and "Given that most stars in our galaxy are part of a binary system, this means the opportunities for life are much broader than if planets form only around single stars. This milestone discovery confirms a theory that scientists have had for decades but could not prove until now."

Sorry kids, not gonna happen. Besides, Star Wars happened in a different galaxy, duh.

-CAINE-

Source: NASA.gov
VIA: GGB on tumblr

Thursday, August 18, 2011

NASA Finds Possible Proof of liquid Water on Mars


Earlier this month, NASA sent out a press release along with a series of images taken by the HRISE camera on board the Mars Reconnaissance orbiter showing a series of dark trails radiating down from the edges of steep slopes of Mars' Newton Basin crater, located on the planet's southern hemisphere. These trails first begin to appear and grow throughout the warmer months on the planet, and then recede as temperatures drop in the winter. Because the temperature in this particular area is too warm to allow for the creation of carbon dioxide frost, researchers concluded that the the most likely candidate behind the unusual markings were deposits of salt water, either on or just beneath the planet's surface, thawing and draining down the slopes with the changing of the seasons.

While it is generally accepted that Mars once had liquid water, possibly even an ocean flowing on it's surface, and the existence of water ice just beneath the planet's soil has been confirmed in various regions. These strange dark trails in the martian sand represent the best evidence to date that liquid water could in fact still exist on the red planet. Which would of course greatly increase the odds that Mars is also potentially host to at least microbial life.

However, while the images are compelling. The argument they make as proof of flowing water, is little more than circumstantial. As the water itself has yet to be directly observed or detected, and an attempt to confirm it's presence using the Compact Reconnaissance Imaging Spectrometer for Mars on board the MRO, was unsuccessful. Which could either mean that the water isn't there, it evaporates too quickly to detect, or that there simply isn't enough of it present in the atmosphere for it to be detected at all. Only time and further observation will tell for sure.

-CAINE-

Source:NASA

You can also view this post on: GGB on Tumblr

check out today's video for a look at the region of Mars in question. As narrated by Alfred McEwen, principal investigator for HiRISE and lead author of a report about the recurring flows published in Thursday's edition of the journal Science,


Posted by Youtube user: SpaceRip