The Two Shall Become One (Galaxy, that is)

This image of a pair of colliding galaxies called NGC 6240 shows them in a rare, short-lived phase of their evolution just before they merge into a single, larger galaxy. Image credit: NASA/JPL-Caltech/STScI-ESA

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An imminent collision of biblical proportions has been captured by the Hubble and Spitzer Space Telescopes. The image here offers a rare view of a collision about to happen between the cores of two merging galaxies, each powered by a black hole with millions of times the mass of the sun. Already this union is considered to be one galaxy: NGC 6240, located 400-million light years away in the constellation Ophiuchus. Millions of years ago, each core was the dense center of its own galaxy before the two galaxies collided and ripped each other apart. Now, these cores are approaching each other at tremendous speeds and preparing for the final cataclysmic collision. They will crash into each other in a just a few million years.

“One of the most exciting things about the image is that this object is unique,” said Stephanie Bush of the Harvard-Smithsonian Center for Astrophysics, Cambridge, Mass., lead author of a new paper describing the observation in an upcoming issue of the Astrophysical Journal. “Merging is a quick process, especially when you get to the train wreck that is happening. There just aren’t many galactic mergers at this stage in the nearby universe.”

Download and extra-large version of this image here.

It combines visible light from NASA’s Hubble Space Telescope and infrared light from Spitzer. It catches the two galaxies during a rare, short-lived phase of their evolution, when both cores of the interacting galaxies are still visible but closing in on each other fast.

NGC 6240 is already putting out huge amounts of infrared light, an indication that a burst of star formation is underway. The extra infrared radiation is common in interacting galaxies; as the two galaxies interact, dust and gas swept up by the collision form a burst of new stars that give off infrared light. Such galaxies are called luminous infrared galaxies. Spitzer’s infrared array camera can image the extra heat from newly formed stars, even though their visible light is obscured by thick dust clouds around them.

The blob-like shape of the galaxy is due to the sustained violence of the collision. Streams of millions of stars are being ripped off the galaxy, forming wispy “tidal tails” that lead off NGC 6240 in several directions. But things are about to get even more violent as the main event approaches and the two galactic cores meld into one.

In the center of NGC 6240, the two black holes in the cores will whip up a frenzy of radiation as they careen towards one another head-on, likely transforming the galaxy into a monster known as an ultra-luminous infrared galaxy, thousands of times as bright in infrared as our Milky Way.

Another fascinating aspect of this rare object is that no two galactic mergers are the same. “Not only are there few objects at this stage, but each object is unique because it came from different progenitor galaxies,” said Bush. “These observations give us another layer of information about this galaxy, and galactic mergers in general.”

Infrared light taken by Spitzer’s infrared array camera at 3.6 and 8.8 microns (red) shows cold dust and radiation from star formation; visible light from Hubble (green and blue) shows hot gas and stars.

Source: JPL

Indian Balloon Experiment Nets Three New Bacteria

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Indian scientists flying a giant balloon experiment have announced the discovery of three new species of bacteria from the stratosphere.

In all, 12 bacterial and six fungal colonies were detected, nine of which, based on gene sequencing, showed greater than 98 percent similarity with reported known species on earth. Three bacterial colonies, however, represented totally new species. All three boast significantly higher UV resistance compared to their nearest phylogenetic neighbors on Earth.

The experiment was conducted using a balloon that measures 26.7 million cubic feet  (756,059 cubic meters) carrying 1,000 pounds (459 kg) of scientific payload soaked in liquid Neon. It was flown from the National Balloon Facility in Hyderabad, operated by the Tata Institute of Fundamental Research (TIFR). 

An onboard cryosampler contained sixteen evacuated and sterilized stainless steel probes. Throughout the flight, the probes remained immersed in liquid Neon to create a cryopump effect. The cylinders, after collecting air samples from different heights ranging from 20 km to 41 km (12 to 25 miles) above the Earth’s surface, were parachuted down and retrieved. The samples were analyzed by scientists at the Center for Cellular and Molecular Biology in Hyderabad as well as the National Center for Cell Science in Pune for independent confirmation.

One of the new species has been named as Janibacter hoylei, after the astrophysicist Fred Hoyle, the second as Bacillus isronensis recognizing the contribution of ISRO in the balloon experiments which led to its discovery, and the third as Bacillus aryabhata after India’s celebrated ancient astronomer Aryabhata (also the name of ISRO’s first satellite).

The researchers have pointed out in a press release that precautionary measures and controls operating in the experiment inspire confidence that the new species were picked up in the stratosphere.

“While the present study does not conclusively establish the extra-terrestrial origin of microorganisms, it does provide positive encouragement to continue the work in our quest to explore the origin of life,” they added.

This was the second such experiment conducted by ISRO, with the first one in 2001. Even though the first experiment had yielded positive results, the researchers decided to repeat the experiment while exercising extra care to ensure that it was totally free from any terrestrial contamination.

Source: Indian Space Research Organisation

Additional links: Center for Cellular and Molecular BiologyNational Center for Cell Science, Tata Institute of Fundamental Research

ESO Image Reveals Galaxy Duo in Explosive Dance

The ‘peculiar galaxy’ Arp 261 has been imaged in unprecedented detail, revealing two galaxies in a slow motion — but highly chaotic and disruptive — close encounter. 

Arp 261 lies about 70 million light-years distant in the constellation of Libra, the Scales. The new close-up was captured by the ESO’s Very Large Telescope, at the Paranal Observatory in Chile.

Although individual stars are very unlikely to collide in such an interaction, the huge clouds of gas and dust certainly do crash into each other at high speed, leading to the formation of bright new clusters of very hot stars that are clearly seen in the picture. The paths of the existing stars in the galaxies are also dramatically disrupted, creating the faint swirls extending to the upper left and lower right of the image. Both interacting galaxies were probably dwarfs not unlike the Magellanic Clouds orbiting our own galaxy.

Arp 261 is listed in Halton Arp’s catalogue of Peculiar Galaxies that appeared in the 1960s, with the goal of chronicling objects in the sky that appear strange and may tell rewarding science stories. 

The images used to create the new picture of Arp 261 were not actually taken to study the interacting galaxies at all, but to investigate the properties of the inconspicuous object just to the right of the brightest part of Arp 261 and close to the center of the image. This is an unusual exploding star, called SN 1995N, that is thought to be the result of the final collapse of a massive star at the end of its life, a so-called core collapse supernova. SN 1995N is unusual because it has faded very slowly — and still shows clearly more than seven years after the explosion took place.

SN 1995N is also one of the few supernovae to have been observed to emit X-rays. It is thought that these unusual characteristics are a result of the exploding star being in a dense region of space so that the material blasted out from the supernova plows into it and creates X-rays.

Apart from the interacting galaxy and its supernova, the image also contains several other objects at wildly different distances from us. Starting very close to home, two small asteroids, in our Solar System between the orbits of Mars and Jupiter, happened to cross the images as they were being taken and show up as the red-green-blue trails at the left and top of the picture. The trails arise as the objects are moving during the exposures and also between the exposures through different colored filters. The asteroid at the top is number 14670 and the one to the left number 9735. They are probably less than 5 km (3 miles) across. The reflected sunlight from these small bodies takes about 15 minutes to reach Earth.

The next closest object is probably the apparently bright star at the bottom. It may look bright, but it is still about one hundred times too faint to be seen with the unaided eye. It is most likely a star rather like the Sun and about 500 light-years from us — 20 million times further away than the asteroids. Arp 261 itself, and the supernova, are about 140,000 times farther away than this star, but still in what astronomers would regard as our cosmic neighborhood. Much more distant still, perhaps some fifty to one hundred times further away than Arp 261, lies the cluster of galaxies visible on the right of the picture.

Videos of the unusual system are available here and here.

Source: ESO

Carnival of Space #94

This week the Carnival of Space moves to Out of the Cradle, with Ken the Lunar Librarian as your host. This week we’ve got Dark Skies, info on space access and a look at the evolution of spacesuits.

Click here to read the Carnival of Space #94

And if you’re interested in looking back, here’s an archive to all the past carnivals of space. If you’ve got a space-related blog, you should really join the carnival. Just email an entry to [email protected], and the next host will link to it. It will help get awareness out there about your writing, help you meet others in the space community – and community is what blogging is all about. And if you really want to help out, let Fraser know if you can be a host, and he’ll schedule you into the calendar.

Finally, if you run a space-related blog, please post a link to the Carnival of Space. Help us get the word out.

Europe’s Climate Satellite Fails to Leave Pad

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Europe’s Gravity field and steady-state Ocean Circulation Explorer (GOCE) seems to be stuck on the pad.

The climate change satellite was expected to launch out of Russia at 14:21 GMT (10:21 EDT) today, from the Plesetsk Cosmodrome in northern Russia. The weather was fine and mission managers were optimistic with seconds to liftoff — and then, everything froze. With seven seconds left on the countdown clock, an unexpected hold went into place and ESA broadcasters simply stopped talking.

Update, 12:30 p.m. EDT: The ESA has announced that launch failed when the doors of the launch service tower did not open. The tower was held in position and did not move back as required for a launch. An investigation is under way, and the agency intends to try again tomorrow at the same time (15:21 CET; 14:21 GMT; 10:21 a.m. EDT).

GOCE is the first of a new family of ESA satellites, called Earth Explorers, designed to study our planet and its environment in order to improve our knowledge and understanding of Earth-system processes and their evolution, to characterize the challenges of global climate change.

The satellite is supposed to launch into a Sun-synchronous, near-circular polar orbit by a Russian Rockot vehicle – a converted SS-19 ballistic missile. Its specific mission is to map Earth’s gravity field with unprecedented accuracy, providing insight into ocean circulation, sea-level change, climate change, volcanism and earthquakes.

GOCE has been undergoing preparations for launch since it was taken out of storage around three weeks ago. Launch campaign activities included a series of mechanical and electrical tests, mating to the Upper Stage and finally encapsulation in the launcher fairing. A video of the anticipated fairing separation was produced pre-launch, and is available here.

Today’s go-ahead followed a successful countdown rehearsal conducted by ESA’s Mission Control Team, the Russian Mission Control Centre and the international tracking station network on Friday.

“We’ve been in this room for many hours and many days in the past. We want to do the real thing now,” said Paolo Laberinti, head of verification and testing, just moments before the seemingly foiled launch.

This isn’t the first time GOCE has encountered problems. The craft had to stand down from launch in September 2008 when problems were discovered with the guidance and navigation subsystems on the Russian Breeze KM rocket. GOCE had to be de-mated from the rocket and brought back into the clean room.

Stay tuned for updates to this post as the ESA releases details about the failure.

Source: ESA

Liftoff! Discovery Finally Leaves Earth for ISS

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NASA’s space shuttle discovery launched successfully from Cape Canaveral Air Force Base at 7:43 p.m. (EDT) on Sunday, under flawless skies and without a single significant complication, despite past issues that had postponed the launch no less than five times.

Less than a minute after leaving the launch pad, Discovery was traveling 365 miles (578 kilometers) per hour. Less than two minutes after that, the craft was speeding away at 1,100 miles (17,000 kilometers) per hour and climbing, toward the International Space Station.

All three main engines performed perfectly throughout Discovery’s flight. Eight minutes after launch,  the twin solid rocket boosters burned out and fell away as the craft was traveling 17,500 miles (28,000 kilometers) an hour. 

Now that it’s orbiting Earth, it will take Discovery about two days to catch up to the International Space Station. 

Early Sunday afternoon, Launch Director Mike Leinbach sent a “red team” to launch pad 39A to manually correct a valve issue that caused a drop in helium pressure. But following that minor adjustment, NASA encountered no issues to delay the launch. 

In fact, the weather improved as the day went on. Original weather predictions had been 80 percent favorable for launch, but by 6 p.m. that prediction had been upgraded to 100 percent. 

Discovery’s payload includes technology to boost the station’s power capacity in line with doubling the size of the ISS crew from three to six in May.

The set of solar arrays that the STS-119 crew will be bringing up includes two solar array wings, each of which has two 115-foot-long arrays, for a total wing span of 240 feet, including the equipment that connects the two halves and allows them to twist as they track the sun. Altogether, the four sets of arrays can generate 84 to 120 kilowatts of electricity – enough to provide power for more than 40 average homes. Since the three existing arrays can handle the majority of the station’s day-to-day operational and life support needs, the newest solar array will double the amount of power available for scientific research. 

The Discovery crew has been bouncing between NASA’s Kennedy Space Center, in Florida, and the Johnson Space Center in Houston since late January; the first launch attempt was scheduled for early February. But four times, managers rescheduled the launch based on their concern following a hydrogen control valve malfunction on the shuttle Endeavour last fall. They wanted to rule out any similar glitches on Discovery.

Things were looking good for the fifth attempt on Wednesday — when skies would have been clear across much of the east coast — but a leak during refueling led to another cancellation.

Fueling of Discovery’s tank — with nearly 500,000 gallons of chilled liquid oxygen and hydrogen propellants  — went off Sunday morning without a hitch. 

Discovery’s flight is STS-119, but NASA has actually flown 131 missions with shuttles. Under the Obama administration, the shuttle program is expected to retire next year.

Discovery Launch: Sixth Attempt a Charm?

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With just over four hours to go before launch, NASA is 80 percent optimistic that tonight’s Discovery launch will be a go — with the weather holding the only foreseeable wild card. Launch time is 7:43 p.m. local time (EDT) from the Cape Canaveral Air Force Station. 

Unfortunately for east coast skywatchers, a storm system that’s been dumping rain all weekend will obstruct a view of the launch that would otherwise be a beauty, as the shuttle will cruise northeast over the ocean nearly parallel to the shore. Without the clouds, the launch would have been visible as far west as the Appalachian Mountains, and as far north as the southern tip of Nova Scotia. 

But Florida’s weather is looking promising, partly cloudy (and 80 degrees at the time of this post) with an 80 percent chance of cooperating with the launch.

7:20 p.m. (EDT) update: With less than a half hour to go, daylight is fading under clear skies in Florida. Earlier, the weather forecast improved from 80 percent to 100 percent favorable for launch. NASA is reporting no problems.

The Discovery crew members are set to fly a new truss segment to the International Space Station and install the final set of power-generating solar arrays, boosting the station’s power capacity and paving the way for doubling the size of the ISS crew from three to six.

The Discovery crew has been bouncing between NASA’s Kennedy Space Center, in Florida, and the Johnson Space Center in Houston since late January; the first launch attempt was scheduled for early February. But four times, managers rescheduled the launch based on their concern following a hydrogen control valve malfunction on the shuttle Endeavour last fall. They wanted to rule out any similar glitches on Discovery.

Things were looking good for the fifth attempt on Wednesday — when skies would have been clear across much of the east coast — but a leak during refueling sent up another red flag. 

Understandably, this morning’s fueling was a bit tense. But for three hours beginning at 10:20 EDT, nearly 500,000 gallons of chilled liquid oxygen and hydrogen propellants flowed into Discovery’s external tank without incident. 

Two irregularities have been reported so far this afternoon: a bat was found clinging to Discovery’s external tank, and Launch Director Mike Leinbach sent a “red team” to launch pad 39A to manually correct a valve issue that caused a drop in helium pressure. 

Neither issue is expected to interfere with launch.

Stay tuned for updates, either to this post or a new one.

LEAD IMAGE CAPTION: NASA’s Discovery shuttle pictured under a full moon on Wednesday, when its fifth launch attempt was scrapped. Tonight marks the sixth. NASA/Bill Ingalls

Source: NASA

Journey Inside M104

Sombrero Parallel by Jukka Metsavainio

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Almost every amateur astronomer is familiar with the Sombrero Galaxy (also known as M104 or NGC 4594) – an unbarred spiral galaxy in the constellation Virgo. We’ve seen it in both small and large telescopes, picked up its ghostly signature in binoculars and dreamed over its structure in photographs. Now, for the first time ever, Jukka Metsavainio is giving us the opportunity to visualize what it might be like to approach this amazing galaxy from space and see it in dimension. Step inside and let’s learn.

Like all our our “stereo” image produced for UT by Jukka Metsavainio, two versions are presented here. The one above is parallel vision – where you relax your eyes and when you are a certain distance from the monitor screen the two images will merge into one to produce a 3D version. The second – which appears below – is crossed vision. This is for those who have better success crossing their eyes to form a third, central image where the dimensional effect occurs. Jukka’s visualizations of what M104 would look like if we were able to see it in dimension comes from studying the object, photographing it, knowing the field star distances and the different wavelengths of light. Are you ready to “cross” the boundary? Then let’s rock…

Sombrero Cross by Jukka Metsavainio
Sombrero Cross by Jukka Metsavainio

Discovered by Pierre Mechain in 1781 and added by Charles Messier’s own hand to his personal notes on May 11, 1781, Messier Object 104 wasn’t officially added to the official catalog of Messier objects until 1921 by Camille Flammarion. Although Messier had already ended his studies, he hadn’t quite ended his fascination with the sky and when Pierre discovered this amazing galaxy, he confirmed his observation by adding his description of a “very faint nebula” to the records. On May 9, 1784 – almost three years later to the date – Sir William Herschel independently recovered the galaxy and whose notes state: “Extended [elongated]. Very bright toward the middle. 5 or 6′ long.”

By 1828, John Herschel was seeing things much differently: “There is a faint diffused oval light all about it, and I am almost positive that there is a dark interval or stratum separating the nucleus and general mass of the nebula from the light above (s of) it. Surely no illusion.” Then Emil Dreyer in 1877: “Remarkable, very bright, very large, extremely extended toward position angle 92 deg, very suddenly much brighter toward the middle where there is a nucleus.” And the results of Curtis from the same year “A remarkable, slightly curved, clear-cut dark lane runs along the entire length to the south of the nucleus; probably the finest known example of this phenomenon. There are very slight traces of spiral whorls.” But it was 1912 and Vesto M. Slipher at Lowell Observatory who was about to make the most amazing discovery of all…

During 1910, Slipher (and later Carl Wirtz) was the first to use a spectroscope to observe the radial velocities of galaxies. What Vesto noticed was that M104 appeared to be cruising away from Earth at 700 miles per second. Such an tremendous speed was an important clue that the Sombrero was really another galaxy, and that the universe was expanding in all directions – but they didn’t know that at the time. At home (within our Milky Way galaxy) noted redshifts almost always correspond to the line of sight velocities associated with the objects being observed. These observations of redshifts and blueshifts have allowed science to measure velocities by a method first designed in 1868 by British astronomer William Huggins. Redshift is also an important tool to measure the velocity of gas of interstellar clouds, the rotation of galaxies, and the actions of accretion around neutron stars and black holes.

What we know now is there’s a supermassive black hole at the center of the Sombrero… one of the most massive black holes measured in any nearby galaxies. According the the findings by a research group led by John Kormendy and using spectroscopy data from both the CFHT and the Hubble Space Telescope, the group showed that the speed of rotation of the stars within the center of the galaxy could not be maintained unless a mass 1 billion times the mass of the Sun was present at the core. No wonder the eye is drawn there! The nucleus is also a strong source of synchrotron emission – produced when high velocity electrons oscillate as they pass through regions with strong magnetic fields. Although we can’t see radio waves, the low ionization nuclear emission region (LINER) at M104’s heart may be the energy source that weakly ionizes the gas in the Sombrero Galaxy.

And what of the dark dust ring? It’s cold atomic hydrogen gas. According to infrared spectroscopic studies, it’s the primary site for star formation and not the amazing nucleus. “The brightest infrared sources in the galaxy are the nucleus and the dust ring. The spectral energy distribution of the AGN demonstrates that, while the environment around the AGN is a prominent source of mid-infrared emission, it is a relatively weak source of far-infrared emission, as had been inferred for AGNs in previous research.” Says George Bendo, “The weak nuclear 160 um emission and the negligible polycyclic aromatic hydrocarbon emission from the nucleus also implies that the nucleus is a site of only weak star formation activity and the nucleus contains relatively little cool interstellar gas needed to fuel such activity. We propose that this galaxy may be representative of a subset of low-ionization nuclear emission region galaxies that are in a quiescent AGN phase because of the lack of gas needed to fuel circumnuclear star formation and Seyfert-like AGN activity.”

Take the time to check out this beautiful galaxy yourself. You’ll find it eleven degrees west of Spica….

Earth Cyclones, Venus Vortices Have Much in Common

Scientists have spotted an S-shaped feature in the center of the vortices on Venus that looks familiar — because they’ve seen it in tropical cyclones on Earth.

Researchers from the United States and Europe spotted the feature using NASA’s Pioneer Venus Orbiter and The European Space Agency’s Venus Express. Their new discovery confirms that massive, swirling wind patterns have much in common where they have been found — on Venus, Saturn and Earth.

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At cloud top level, Venus’ entire atmosphere circles the planet in just about four Earth days, much faster than the solid planet does. Despite this “superrotation,” some dynamical and morphological similarities exist between the vortex organization in the atmospheres of Venus’s northern and southern hemispheres and tropical cyclones and hurricanes on Earth.

Organization of the Venus atmospheric circulation into two circumpolar vortices, one centered on each pole, was first deduced more than 30 years ago from Mariner 10 ultraviolet images. The S-shaped feature in the center of the vortices on Venus was first detected by the Pioneer Venus Orbiter near the northern pole and recently by Venus Express orbiter around the southern pole. It is also known to occur in Earth’s tropical cyclones.

Using an idealized nonlinear and nondivergent barotropic model, lead author Sanjay S. Limaye, of the University of Wisconsin-Madison, and his colleagues are proposing that these S-shaped features are the manifestations of barotropic instability. The feature can be simulated with a barotropic model and, like in the vortices on Venus and in tropical cyclones, it is found to be transient.

Another similarity between the observed features in the vortex circulations of Venus and in terrestrial hurricanes is the presence of transverse waves extending radially outward from the vortex centres. The lack of observations of such features in Earth’s polar vortices is suggestive that the dynamics of the Venus polar vortices may have more in common with hurricanes than their more direct terrestrial counterparts. 

Given the challenges in measuring the deep circulation of Venus’s atmosphere, the authors expect that the morphological similarities between vortices on Earth and Venus might help scientists better understand atmospheric superrotation on Venus and guide future observations.

IMAGE CAPTIONS: 1. The ‘eye of the hurricane’ on Venus, taken by the Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) on board Venus Express. The yellow dot represents the south pole. Credit: ESA 2. An infrared satellite image of Hurricane Howard [1998], showing an S-shaped pattern in the low (warm) clouds in the tropical cyclone’s eye. Credit: Sanjay S. Limaye. 

Source: Geophysical Research Letters

Google Earth Now ‘Live From Mars’

Mars in Google Earth. Credit: Google

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Google Earth announced a big update today of its Mars features, including a chance to see a continuous stream of new, high resolution satellite imagery just hours after NASA receives them. Called “Live from Mars,” this section features imagery from NASA’s THEMIS camera on board the Mars Odyssey spacecraft, and the HiRISE Camera from the Mars Reconnaissance Orbiter. You can become one of the very first people to lay eyes on images taken just days or even hours ago. You can also see live satellite orbital tracks, or check out where these cameras plan to image next.

But wait! There’s more! Users can also travel back in time to see the Red Planet through the eyes of the pioneers of Mars science in the ‘Historical Maps’ layer by exploring antique maps by astronomers Giovanni Schiaparelli, Percival Lowell, and others. But also, if you don’t know exactly where to start with your Mars exploration, there are guided tours of Mars narrated by Ira Flatow of Public Radio’s Science Friday and Bill Nye the Science Guy, allowing you to enjoy the PB&J (passion, beauty and joy) of the Red Planet through their eyes.

Mars in Google Earth.  Credit: Google
Mars in Google Earth. Credit: Google

So how do you enjoy these new features? Open Google Earth, and after selecting ‘Mars’ from the toolbar in Google Earth, users fly to a 3D view of the Red Planet, complete with informational layers, imagery, and terrain. The tools for navigation and exploration on Mars are identical to those on Earth – zoom in and out, change the camera view, or spin the entire planet with a click of the mouse.
Historical maps in Google Mars.  Credit: Google.
Historical maps in Google Mars. Credit: Google.

Just as in the original version of Mars in Google Earth, users can read geo-located articles from Hartmann’s “A Traveler’s Guide to Mars” about the solar system’s largest canyon, Valles Marineris, its tallest volcano, Olympus Mons, the infamous ‘Face on Mars’, and many other famous Martian locations. Users can also follow the paths of Mars rovers and view hi-resolution panoramic photos of the Mars surface.

Google’s Communication and Public Affairs officer Aaron Stein noted the “Live From Mars” imagery is the most current available from the THEMIS camera. ” Our live imagery is the most current available imagery from THEMIS,” he said. “It’s not unusual for NASA to save up and download one or two days of images at a time, so downloads do not always occur within hours of image acquisition. Despite this, Live from Mars is orders of magnitude more “live” than the typical NASA public data release process, which for Mars imagery typically takes many months.”

Enjoy — It’s fun, it’s free, and a great way to lose yourself for a few hours!

Source: Google Earth