Alien Life on Titan? Hang on Just a Minute…

This artist concept shows a mirror-smooth lake on the surface of the smoggy moon Titan. Image credit: NASA/JPL

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Two papers released last week detailing oddities found on Titan have blown the top off the ‘jumping to conclusions’ meter, and following media reports of NASA finding alien life on Saturn’s hazy moon, scientists are now trying to put a little reality back into the news. “Everyone: Calm down!” said Cassini imaging team leader Carolyn Porco on Twitter over the weekend. “It is by NO means certain that microbes are eating hydrogen on Titan. Non-bio explanations are still possible.” Porco also put out a statement on Monday saying such reports were “the unfortunate result of a knee-jerk rush to sensationalize an exciting but rather complex, nuanced and emotionally-charged issue.”

Astrobiologist Chris McKay told Universe Today that life on Titan is “certainly the most exciting, but it’s not the simplest explanation for all the data we’re seeing.”

McKay suggests everyone needs to take the Occam’s Razor approach, where the simplest theory that fits the facts of a problem is the one that should be selected.

The two papers suggest that hydrogen and acetylene are being depleted at the surface of Titan. The first paper by Darrell Strobel shows hydrogen molecules flowing down through Titan’s atmosphere and disappearing at the surface. This is a disparity between the hydrogen densities that flow down to the surface at a rate of about 10,000 trillion trillion hydrogen molecules per second, but none showing up at the surface.

“It’s as if you have a hose and you’re squirting hydrogen onto the ground, but it’s disappearing,” Strobel said. “I didn’t expect this result, because molecular hydrogen is extremely chemically inert in the atmosphere, very light and buoyant. It should ‘float’ to the top of the atmosphere and escape.”

The other paper (link not yet available) led by Roger Clark, a Cassini team scientist, maps hydrocarbons on Titan’s surface and finds a surprising lack of acetylene. Models of Titan’s upper atmosphere suggest a high level of acetylene in Titan’s lakes, as high as 1 percent by volume. But this study, using the Visual and Infrared Mapping Spectrometer (VIMS) aboard Cassini, found very little acetylene on Titan’s surface.

Of course, one explanation for both discoveries is that something on Titan is consuming the hydrogen and acetylene.

Even though both findings are important, McKay feels the crux of any possible life on Titan hinges on verifying Strobel’s discovery about the lack of hydrogen.

“To me, the whole thing hovers on this determination of whether there is this flux of hydrogen is real,” McKay said via phone. “The acetylene has been missing and the ethane has been missing, but that certainly doesn’t generate a lot of excitement, because how much is supposed to be there depends on how much is being made. There are a lot of uncertainties.”

McKay stressed both results are still preliminary and the hydrogen loss in particular is the result of a computer calculation, and not a direct measurement. “It is the result of a computer simulation designed to fit measurements of the hydrogen concentration in the lower and upper atmosphere in a self-consistent way,” he said in a statement he put out over the weekend. “It is not presently clear from Strobel’s results how dependent his conclusion of a hydrogen flux into the surface is on the way the computer simulation is constructed or on how accurately it simulates the Titan chemistry.”

However, the findings are interesting for astrobiology, and would require the actual existence of methane-based life, a theory McKay himself proposed five years ago, which he described today as an “odd idea.”

In 2005, McKay and Heather Smith (McKay and Smith, 2005) suggested that methane-based life (rather than water-based) called methanogens on Titan could consume hydrogen, acetylene, and ethane. The key conclusion of that paper was “The results of the recent Huygens probe could indicate the presence of such life by anomalous depletions of acetylene and ethane as well as hydrogen at the surface.”

Even though the two new papers seem to show evidence for all three of these on Titan, McKay said this is a still a long way from “evidence of life”. However, it is extremely interesting.

But what does McKay really think?

“Unfortunately, if I was betting, the most likely explanation is that Darrel’s (Strobel) results are wrong and that further analysis will show there is another explanation for the data he is trying to fit, besides the strong flux of hydrogen into the surface. I would be very happy if we did confirm all that data, but we do have to take it in steps.”

McKay provided four possibilities for the recently reported findings, listed in order of their likely reality:

1. The determination that there is a strong flux of hydrogen into the surface is mistaken. “It will be interesting to see if other researchers, in trying to duplicate Strobel’s results, reach the same conclusion,” McKay said.

2. There is a physical process that is transporting H2 from the upper atmosphere into the lower atmosphere. One possibility is adsorption onto the solid organic atmospheric haze particles which eventually fall to the ground. However this would be a flux of H2, and not a net loss of H2.

3. If the loss of hydrogen at the surface is correct, the non-biological explanation requires that there be some sort of surface catalyst, presently unknown, that can mediate the hydrogenation reaction at 95 K, the temperature of the Titan surface. “That would be quite interesting and a startling find although not as startling as the presence of life,” McKay said.

4. The depletion of hydrogen, acetylene, and ethane, is due to a new type of liquid-methane based life form as predicted (Benner et al. 2004, McKay and Smith 2005, and Schulze-Makuch and Grinspoon 2005 (Astrobiology, vol. 5, no. 4., p. 560-567.).

McKay said if further analysis shows that a strong flux of hydrogen into the surface really is happening, “then my first two explanations are no longer options and we are then left with two really quite remarkable alternatives, either there is some mysterious metalysis going on, which at 95 k is really hard to imagine, and would have enormous implications for things like chemical engineering. And the second alternative is that there is life, which is even more amazing.”

“So to make process on this,” McKay continued, “we have to confirm Darrel’s result that there is hydrogen being fluxed onto the surface of Titan, that is really way unexpected, and unfortunately, it constitutes extraordinary claims that need extraordinary evidence. Darrel’s paper is just a first step in that.”

What does McKay think about the rash of media reports claiming life on Titan?

“Well, I think it reflects our human fascination and desire to find life out there,” he said. “We want it to be true. When we’re given a set of facts, if they are consistent with biology we jump to that explanation first. The most biologically interesting explanation is the first one we look to. We ought to give that a name — something like ‘Carl Sagan’s Razor’ as opposed to ‘Occam’s Razor,’ which would say that ‘The most exciting explanation is assumed to be true until it is proven false.'”

You can read all of McKay’s written response on the CICLOPS website, which Porco said will be “the first installment in a new feature on the CICLOPS website, called ‘Making Sense of the News’, where from time to time, scientists, both involved in Cassini and not, will be invited to comment on new developments that bear on the exploration of the solar system and the study of planetary systems, including our own.”

Dramatic Moonset — Amazing Sight on Cerro Paranal

Moonset on Cerro Paranal. Credit: ESO

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Need a new desktop image? Usually the Very Large Telescope on Cerro Paranal in Chile provides us with stunning views of the cosmos. This image, however, is a gorgeous view of the observatory itself. As the Moon was setting after a long night of observing, ESO staff member Gordon Gillet welcomed the new day by capturing this stunning image from 14 km away. This image is not a montage or computer-generated (such as the infamous ‘Moon and Sun over the North Pole‘ urban legend)

The ESO website explains:

The Moon appears large because it is seen close to the horizon and our perception is deceived by the proximity of references on the ground. In order to get this spectacular close view, a 500-mm lens was necessary. The very long focal length reduces the depth of field making the objects in focus appear as if they were at the same distance. This effect, combined with the extraordinary quality of this picture, gives the impression that the Moon lies on the VLT platform, just behind the telescopes, even though it is in fact about 30,000 times further away.

Interestingly, Gillet took the image from the road leading to the nearby Cerro Armazones, the peak recently chosen by the ESO Council as the preferred location for the planned 42-meter European Extremely Large Telescope (E-ELT), which should be open for business by 2018.

Source: ESO

Astronomy Without A Telescope – Exoplanet Weather Report

Trying to determine the behaviour of the atmosphere of a hot Jupiter – a gas giant so close to its star that it is either tidally locked or caught in a slow orbital resonance – is tricky, given that we have no precedents here in our solar system. But it is possible to explore in detail what exoplanet atmospheres might be like, based on solar system examples.

For example, there’s Venus – which, although not tidally locked, has such a slow rotation (once every 243 Earth days) that its dynamics virtually match those of a tidally locked planet.

Interestingly, Venus’ upper atmosphere super-rotates, meaning it circulates in the same direction as the planet’s rotation but much faster – in Venus’ case, at sixty times the speed of the planet’s rotation. It’s likely that these winds are driven by the large temperature gradient that exists between the day and night sides of the planet.

Conversely Earth, with its rapid rotation, has much less potential difference between its day and night side temperatures – so that its weather systems are more strongly influenced by the actual rotation of the planet and also by the temperature gradient between equator and pole. The nett result is lots of circular weather systems with their direction determined by the Coriolis effect – counter-clockwise in the northern hemisphere and clockwise in the southern.

And of course we do have gas giants, even if they aren’t hot. Being so far from the Sun, dayside-nightside and equator-pole temperature gradients have little influence on our gas giants’ atmospheric circulation. The most significant issues are each planet’s rotation speed and each planet’s size.

Jupiter and Saturn’s larger radius exceeds their Rhines scale forcing the bulk flow of their atmospheres to break up into distinct bands with turbulent eddies between them. However, the smaller radius of Uranus and Neptune allows the bulk of the atmosphere to circulate as an unbroken whole, only breaking into two smaller bands at each pole.

The 'Rhines Scale' applied to solar system gas giants predicts that atmospheric circulation on large radius planets (Jupiter and Saturn) fragments into distinct bands, but doesn't on smaller radius planets (Uranus and Neptune). Credit: Showman et al 2010.

Partly because it’s cooler, but mostly because it’s smaller, Neptune’s atmosphere has much less turbulent flow than Jupiter – which goes some way to explaining why it has the fastest stratospheric wind speeds in the solar system.

All these factors are useful in trying to determine how the atmosphere of a hot Jupiter might behave. Being so close to their star, it’s likely these planets will be partly or fully tidally locked – so the main driver for atmospheric circulation will be, like Venus, the dayside-nightside temperature gradient . So a super-rotating stratosphere, circulating many times faster than the inner parts of the planet, is plausible.

From there, modelling suggests that the combination of fast wind speed and slow rotation means the Rhines scale will become bigger than a Jupiter-sized planetary radius , so there will be less turbulent flow and the upper atmosphere might circulate as one, without breaking up into the multiple bands we see on Jupiter.

Anyway, that’s my take on an interesting 50 page arXiv article with lots of (to me) bewildering formulae, but also lots of comprehensible narrative and diagrams. The article consolidates current thinking and lays a sound foundation for making sense of future observational data – both hallmarks of a nicely crafted ‘lit review’.

Spirialing ‘UFO’ Over Australia Was Likely Falcon 9 Rocket

Image of spiraling object over Australia, taken by Lance Godwin, from the 9MSN news station website.


Logical explanations take all the fun out of UFO’s. After the Falcon 9 rocket launched successfully, later, over on the other side of the world, people in Australia saw a spiraling object in their early morning skies, about 6 am local time. Geoffrey Wyatt, from the Sydney Observatory, said it appeared to have been the Falcon 9 rocket, which launched about an hour earlier.

Another image below.

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The image is from the 9MSN website in Australia, where you can see more images.

If you recall, there was another spiraling rocket that created a visual sensation over Norway in December of 2009.

Hat tip to The Original Rocket Dungeon. Added later: Oh, and I see the Bad Astronomer has fully explained the whole thing!

Falcon 9 Launch Gallery; ‘Fantastic Day,’ P–G Singularity and More

A Prandtl–Glauert singularity, or shock cone forms around the Falcon 9 rocket during launch. Credit: Alan Walters (awaltersphoto.com) for Universe Today.

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Universe Today photographer Alan Walters was on hand for Friday’s spectacular and picture-perfect launch of SpaceX’s Falcon 9 rocket. Enjoy a gallery of images, including this great shot of a Prandtl–Glauert singularity, or shock cone that formed around the rocket, which sometimes occurs when a sudden drop in air pressure occurs when rockets or aircraft are traveling at transonic speeds.

“This has really been a fantastic day,” said an exuberant Elon Musk, CEO of SpaceX, speaking with reporters after the flight. “It’s been one of the best days of my life. It’s certainly been one of the greatest days for the people of SpaceX.”

Falcon 9 launch on June 4, 2010. Credit: Alan Walters (awaltersphoto.com) for Universe Today.

Falcon 9 launch on June 4, 2010. Credit: Alan Walters (awaltersphoto.com) for Universe Today.
Falcon 9 launch on June 4, 2010. Credit: Alan Walters (awaltersphoto.com) for Universe Today.
Falcon 9 launch on June 4, 2010. Credit: Alan Walters (awaltersphoto.com) for Universe Today.
Falcon 9 launch on June 4, 2010. Credit: Alan Walters (awaltersphoto.com) for Universe Today.
Falcon 9 pre-launch on June 4, 2010. Credit: Alan Walters (awaltersphoto.com) for Universe Today.

A Trilogy of Tremendous Volcanoes

Mt. Cleveland in Alaska. NASA Earth Observatory image by Jesse Allen & Robert Simmon, using data from the NASA/GSFC/METI/ERSDAC/JAROS, and U.S./Japan ASTER Science Team.

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You like volcanoes? We’ve got volcanoes! Three recent images from space show some tremendous volcanoes on Earth. This very unusual image shows a small volcanic plume rising above remote Mount Cleveland on June 1, 2010. The snow-covered upper slopes of the Aleutian alaska volcano were also marked by dark debris flow deposits (descending to the east) and ash fall to the south of the summit. This false-color image was acquired by the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) aboard NASA’s Terra satellite. Snow is white, clouds are pink, vegetation is red, and water is almost black. The Alaska Volcano Observatory reported an ash emission above Mount Cleveland no higher than 16,000 feet (4,900 meters) on May 30th. Mount Cleveland is frequently restless, and the current activity is not unusual, but Ash from Cleveland could threaten flights between Asia and North America. Satellites are the best way to monitor the volcano, which is about 900 miles (1,500 kilometers) from Anchorage.

Next: @Astro_Soichi strikes again:

Mt. Fuji in Japan, as seen from the ISS. Credit: NASA/JAXA/Soichi Noguchi

Before he left the International Space Station to return back to Earth, Soichi Noguchi, who shared his experiences in space like no other astronaut via his Twitter feed and pictures, took this image of Mt. Fuji in his home country of Japan.

Iceland, without ash and smoke from the Eyjafjallajokull volcano. Credit: ESA

Ok, this one isn’t specifically of a volcano, but it is one of the first satellite images of Iceland to show smoke- and ash-free skies above Iceland.

This image is from ESA’s Envisat satellite and the Medium Resolution Imaging Spectrometer on May 24, 2010.

The Eyjafjallajokull volcano, which had a series of eruptions in April and May, is visible in the dark area on the southern coast. The Vatnajokull glacier (visible in white northeast of Eyjafjallajokull) is the largest in Iceland and in Europe. The white circular patch in the center of the country is Hofsjokull, the country’s third largest glacier and its largest active volcano. The elongated white area west of Hofsjokull is Langjokull, Iceland’s second largest glacier.

Sources: Goddard Spaceflight Center, @Astro_Soichi, ESA

Weekend SkyWatcher’s Forecast: June 4-6, 2010

Greetings, fellow SkyWatchers! Sorry to be so late, but satellite internet connections and electrical storms don’t mix! Even though there’s not a snowball’s chance in the desert of observing here tonight, don’t let that stop you from enjoying some of the finest galaxies you’ll ever trip the light fantastic with! Find yourself a dark sky site and enjoy three of my favorites of the season… and share your observations! This time I’ll join you in your backyard….

June 4, 2010 – Did you ever wonder who was the first to organize an astronomy group? No less a personage than Baron Franz Xaver Freiherr von Zach. Born on this date in 1754, von Zach was the director of an observatory near Gotha, and in 1798 he organized the first congress of astronomers, with Joseph LaLande as the honored guest. He later formed another group of two dozen astronomers to help locate the ‘‘missing planet’’ between the orbits of Mars and Jupiter. I wonder what they discovered?

Tonight we’ll head toward Leo for another galaxy worth a visit. . . and even binoculars can spot it! You’ll need to identify slightly fainter Lambda to the southwest of Epsilon and head south about one finger-width for NGC 2903 (RA 09 32 09 Dec +21 30 02). William Herschel discovered this awesome oblique spiral galaxy in 1784. At slightly brighter than magnitude 9, it’s in easy range of most binoculars. It is odd that Messier missed this one, considering both its brightness and the fact that three of the comets he discovered passed by it! Perhaps it was cloudy when Messier was looking, but we can thank Herschel for cataloging NGC 2903 as H I.56.


Although small optics will only perceive this 25-million-light-year-distant beauty as a misty oval with a slightly brighter core region, larger aperture will light this baby up. Soft suggestions of its spiral arms and concentration will begin to appear. One such knot is star cloud NGC 2905—a detail in a distant galaxy so prominent that it received its own New General Catalog designation. NGC 2903 is roughly the size of our own Milky Way and includes a central bar, yet the nucleus of our distant cousin has ‘‘hot spots’’ that were studied by the HST and extensively by the Arecibo telescope. Although our own galactic halo is filled with ancient globular clusters, this galaxy sports brand new ones! Be sure to mark your notes with your observations, because many different organizations consider this to be on their ‘‘Best of’’ lists.

June 5, 2010 – Let’s take a look at John Couch Adams, a discoverer of Neptune who was born on this date in 1819. Said he: ‘‘. . .the beginning of this week of investigating, as soon as possible after taking my degree, the irregularities in the motion of Uranus. . .in order to find out whether they may be attributed to the action of an undiscovered planet beyond it.’’ But that’s not all Adams contributed! He was the first to associate the Leonid meteor shower with the orbital path of a comet, and he also observed the Moon.

Tonight we’ll take a look at our moving universe, and we begin by locating 5th magnitude 6 Comae Berenices about three finger-widths east of Beta Leonis. Remember this star! We are going on a galaxy hop to a Mechain discovery that is less than a degree west, and its designation is M98 (RA 12 13 48 Dec +14 53 58). At magnitude 10, this beautiful galaxy is a telescope-only challenge and a bit on the difficult side for small aperture. Long considered part of the Virgo Cluster , M98 is approaching us at a different rate than other cluster members, giving rise to speculation that it may simply be in the line of sight. Quite simply put, it has a blue shift instead of red! But considering that all these galaxies (and far fainter ones than we can see), are in close proximity leads some researchers to believe it is a true member by virtue of the extreme tidal forces that must exist in the area—pushing it toward us at this point in time, rather than away.


In a small telescope, M98 will appear like a slim-line with a slightly brighter nucleus, a characteristic of an edge-on galaxy. To large aperture, its galactic disk is hazy and contains patchiness in structure. These are regions of newly forming stars and vast regions of dust, yet the nucleus remains a prominent feature. M98 is a very large galaxy, so be sure to use a minimum of magnification and plenty of aversion to make out small details in this fine Messier object!

June 6, 2010 – Today we begin with the 1932 birth on this date of David Scott, the seventh person to walk on the Moon and the first to ride the Lunar Rover on the surface during the Apollo 15 mission. Sharing his birth date, but almost 500 years earlier, was the astronomer Regiomontanus (1436). Regiomontanus made observations of a comet, which were accurate enough to associate it with Comet Halley 210 years later, and his interest in the motion of the Moon led him to make the important observation that lunar distances could be used to determine longitude at sea!

No galactic tour through Coma Berenices would be complete without visiting one of the most incredible ‘‘things that Messier missed.’’ You’ll find NGC 4565 (RA 12 36 21 Dec +25 59 13) located less than 2 degrees east of 17 Comae. Residing at a distance of around 30 million light-years, this large 10th magnitude galaxy is probably one of the finest edge-on structures you will ever see. Perfectly suited for smaller scopes, this ultra-slender galaxy with the bright core has earned its nickname of the ‘‘Needle.’’ Although photographs sometimes show more than what can be observed visually, mid-to-large aperture can easily trace out NGC 4565’s full photographic diameter.


Although Lord Rosse in 1855 saw the nucleus of the Needle as stellar, most telescopes will resolve a bulging core region with a much sharper point in the center and a dark dust lane upon aversion. The core itself has been extensively studied for its cold gas and emission lines, pointing to the fact that it has a barred structure. This is much how the Milky Way would look if viewed from the same angle! It, too, shines with the light of 30 billion stars. Chances are NGC 4565 is an outlying member of the Virgo Cluster, but its sheer size points to the fact that it is probably closer than the others. If we were to place it at the accepted distance of 30 million years, its diameter would be larger than any galaxy yet known! Get acquainted with it tonight… Because big is beautiful, too!

Until next week? Keep reaching for the stars!

This week’s awesome images are (in order of appearance): NGC 2903, M98 and NGC 4565 are from Palomar Observatory, courtesy of Caltech. We thank you so much!

New Discovery Supports Possibility of Microbial Life on Mars

Lost Hammer Spring on Axel Heiberg Island, Nunavut Territory, Canada. Credit: Dept. Natural Resource Sciences, McGill University, Montreal.

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The discovery of methane-eating bacteria in a very unique region of Canada’s extreme north supports the theory that similar organisms could be on Mars. Researchers have found methane-eating bacteria in a cold, methane filled spring located on Axel Heiberg Island in Canada, and say the spring is similar to possible past or present springs on Mars, and that therefore they too could support life.

The spring, called Lost Hammer supports microbial life. It is so salty that it doesn’t freeze despite the cold, and it has no consumable oxygen in it, said Dr. Lyle Whyte from McGill University in Montreal. There are, however, big bubbles of methane that come to the surface, which made the research team – which also included scientists from National Research Council of Canada, the University of Toronto and the SETI Institute –curious as to whether the gas was being produced geologically or biologically and whether anything could survive in this extreme hypersaline subzero environment.

“We were surprised that we did not find methanogenic bacteria that produce methane at Lost Hammer,” Whyte said, “but we did find other very unique anaerobic organisms – organisms that survive by essentially eating methane and probably breathing sulfate instead of oxygen.”

The discoveries of methane and frozen water on Mars, along with recently formed gullies are similar to what is occurring on Axel Heiberg Island. The methane on Mars is quite intriguing since the short-lived gas is obviously being replenished in some way.

But just the fact that methane is on Mars could mean the planet could support life.

“The point of the research is that it doesn’t matter where the methane is coming from,” Whyte explained. “If you have a situation where you have very cold salty water, it could potentially support a microbial community, even in that extreme harsh environment.”

The Lost Hammer spring region is very analogous to Mars. “There are places on Mars where the temperature reaches relatively warm -10 to 0 degrees and perhaps even above 0 degrees C,” Whyte said, “and on Axel Heiberg it gets down to -50, easy. The Lost Hammer spring is the most extreme subzero and salty environment we’ve found. This site also provides a model of how a methane seep could form in a frozen world like Mars, providing a potential mechanism for the recently discovered Martian methane plumes.”

Source: McGill University

SpaceX Falcon 9 Successfully Launches, Reaches Orbit

Screenshot from SpaceX's video feed of the launch of Falcon 9. Credit: SpaceX

It was history in the making that could have a huge bearing on the future of US spaceflight. The commercial space company SpaceX successfully launched their Falcon 9 rocket on Friday, with what seemed to be a picture-perfect lift-off and flight. The Falcon 9 rocket performed magnificently (at least from initial reports), hitting all the flight parameters precisely on time. The SpaceX team overcame delays for telemetry problems, a boat that unknowingly sailed into the restricted zone of the launch range, and one last-second launch abort on an earlier try. The team then successfully recycled the engines and sent the rocket off on a beautiful launch. Video from the rocket in flight was streamed online, showing the stage separation and engine cutoff, with a view of Earth in the background.

UPDATE: Spaceflightnow.com reports that SpaceX founder Elon Musk said the Falcon 9 rocket’s second stage and dummy Dragon capsule achieved a nearly perfect orbit during today’s dramatic blastoff, hitting a bullseye of the orbital target. The apogee, or high point, was about 1 percent higher than planned and the perigee, or low point, was 0.2 percent off the target.


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The Falcon 9 blasted off at 2:45 p.m. EDT (1845 GMT) from launch pad 40 at Cape Canaveral Air Force Station in Florida.

The nine Merlin engines, fueled by liquid oxygen and RP-1 kerosene rocket fuel, provided a million pounds of thrust, sending the rocket to orbit in just over 9 minutes.

SpaceX was shooting for the Falcon 9 to reach a circular orbit 250 kilometers, or 155 miles, high and an inclination of 34.5 degrees.

On the video, it is evident the rocket experienced a slight roll, which was not expected.

Having a rocket succeed on its maiden voyage is quite unusual (it took the Atlas rocket 13 tries for success), so the SpaceX team has to be extremely pleased with not only the rocket’s performance, but the team’s ability to overcome problems and press on with a successful launch.

Screenshot from Falcon 9 video feed, showing the glowing hot nozzle of the rocket. Credit: SpaceX

180-foot (55 meter)-high Falcon 9 carried a mock-up of SpaceX’s Dragon capsule. With this success, the next flight may be a flight to the International Space Station to practice docking techniques — it won’t actually dock, but practice approach. If that goes well, the next flight might actually dock and bring supplies to the ISS.

Congratulations to SpaceX!

Mars Gets Autotuned!

You’ve probably seen “A Glorious Dawn” –– the autotune wonder that allowed Carl Sagan to sing to us. The Symphony of Science music video series has been steadily adding new sciency music videos, and the new “The Case for Mars” is the sixth installment. It features Robert Zubrin, Carl Sagan, Brian Cox, and Penelope Boston. John Boswell, the head musician and producer behind the Symphony of Science says this new video is intended to pique curiosity about the planet Mars and to promote human exploration of it.

You can watch all six videos at Symphony of Science.