News from Space: “Life” Molecules Detected in Space!

SagitariusB2The secret to the creation to life in our universe appears to be seeding – the proper elements in the right mix in the right places to form the right kind of molecules. Only then can these molecules evolve chemically into more and more complex structures, thus following a general pathway toward biology. The pathway for life as we know it starts with carbon, but one which is specific organized and structured.

Recently, a team of astronomers  at the ALMA Observatory reported the discovery of this very element while probing distant galaxies. What they found was not just interstellar carbon, but a form of carbon with a branched structure. The discovery was made in the gaseous-star forming region known as Sagittarius B2 – a giant molecular cloud of gas and dust that is located about 390 light years from the center of the Milky Way.

radio-wave-dishesSimple carbon chains aren’t particularly unusual in the cosmos, but complex carbon is a different matter. It is what the researchers, based at Cornell University and the Max Planck Institute, describe as finding a molecular needle in a cosmic haystack. The actual molecule in question is isopropyl cyanide, and it was discerned thanks to the miracle known as radio astronomy.

Within clouds of interstellar dust and gas, elements find themselves shielded from the harsh radiation of open space and are, thus, free to form into more complex arrangements. These molecules don’t just sit there, but instead move around within their cloud-homes and bump into each other. The result of this activity are radio signals which can be detected light-years away – in this case, by radio telescopes here on Earth.

MaxPlanckIns_radiowavepulseEvery molecule has a different radio signal, so it’s possible to pick apart the contents of interstellar junk by examining a cloud’s frequency spectra. NASA, via the Ames Research Center, even maintains a radio-emission frequency database to aid in the tracking of polycyclic aromatic hydrocarbons, a form of molecule thought to contain much of the universe’s carbon stockpiles.

The branching carbon structure of isopropyle cyanide is of particular interest because it’s thought that this arrangement is a step on the way to the production of amino acids, the building blocks of proteins, and hence organic life. The discovery gives weight to the increasingly popular notion that life, or at least many of the key steps leading toward life, actually occurs off-planet.

alien-worldLife on Earth may have been well on its way while the planet was still just space dust waiting to come together into our rock-home. What’s more, the molecules discovered by the ALMA team probably aren’t alone.  As the authors, led by astronomer Arnaud Belloche, wrote:

[Isopropyle cyanide’s] detection therefore bodes well for the presence in the [interstellar medium] (ISM) of amino acids, for which such side-chain structure is a key characteristic… This detection suggests that branched carbon-chain molecules may be generally abundant in the [interstellar medium].

The discovery follows a general progression in recent years adding more and more life-ingredients to our picture of the ISM. A 2011 study revealed that complex organic matter should be created in large volumes from stars, while a 2012 report study found that conditions within the ISM are uniquely suited to the creation of increasingly complex molecules, “step[s] along the path toward amino acids and nucleotides, the raw materials of proteins and DNA, respectively.”

sugar-in-space-molecules_58724_990x742Also in 2012, astronomers working for ALMA found basic sugar molecules hanging out in the gas cloud around IRAS 16293-2422 – a young star located some 400 light-years from Earth. The particular form, glycoaldehyde, is thought to be a key component of the reaction behind the creation of DNA. Indeed, more and more, the universe is looking less and less like a harsh environment in which life must struggle to emerge, to a life factory.

Source: motherboard.vice.com

News From Space: Asteroid Misses Earth (Again!)

2000EM26_1Yesterday, an asteroid estimated to be the size of three football fields passed Earth by. Traveling at 43,000 kilometers per hour and passing at a distance of 8.8 lunar distances of Earth, the asteroid showed up just one year after a similar asteroid exploded over Russia and injured 1,200 people. The only problem was, the good people of Earth missed the show!

Slooh, an online “community observatory” that streams images from ground-based telescopes online during celestial events, was supposed to broadcast the approach of the asteroid as it raced past the planet, starting at 9 p.m. ET (2 a.m. MT).  Unfortunately, Slooh’s flagship observatory on Mount Teide in Spain’s Canary Islands was iced over and unable to catch the asteroid – named 2000 EM26 – as it passed us by.

2000EM26_2014_logoShortly thereafter, Slooh’s robotic telescope tried to snap pictures attempted to snap pictures of the asteroid but failed to capture an image at the predicted position. And now, the asteroid has gone missing in the deep sea of space, giving rise to the nickname “Moby Dick”. This means that either the asteroid’s predicted path was in error, or the object was much fainter than expected.

Paul Cox, Slooh’s technical and research director, said that the asteroid should be somewhere in the visible star field. And rather than accept failure at retracing its path, he and the other folks at Slooh are calling upon amateur astronomers to conduct a photographic search for it in the next few nights. Finding it is not just a matter of honor, but of determining how much the space rock has shifted over time.

2000EM26_2Since the asteroid was last observed 14 years ago for only 9 days, it isn’t too surprising that uncertainties in its position could add up over time, shifting its position and path to a different part of the sky by now. As Cox pointed out:

Discovering these Near Earth Objects isn’t enough. As we’ve seen with 2000 EM26, all the effort that went into its discovery is worthless unless follow­up observations are made to accurately determine their orbits for the future.  And that’s exactly what Slooh members are doing, using the robotic telescopes at our world­-class observatory site to accurately measure the precise positions of these asteroids and comets.

Naturally, there were some who worried that this elusive rock might threaten Earth, given its proximity to our own orbit and the fact that it’s path may have changed. But there is no reason to fear, as these changes are not likely to bring it into our path and it won’t be returning anytime soon. And before it does, we ought to have eyes on it again and be able to accurately chart its course.

2000EM26And above all, similar sized asteroids, including ones passing even closer to Earth, zip by every month. 2000 EM26 received a lot of coverage yesterday in part because it arrived close to the anniversary of the Chelyabinsk meteorite fall over Russia. And though it remains hidden for now, eyes are on the sky to find the asteroid again and refine its orbit.

Hopefully the beast won’t get away next time!

 

Sources: cbc.ca, universetoday.com

News From Space: The Weird Atmospheres of Titan and Io

alien-worldStudying the known universe is always interesting, mainly because you never know what you’re going to find. And just when you think you’ve got something figured out – like a moon in orbit around one of the Solar Systems more distant planet’s – you learn that it can still find ways to surprise you. And interestingly enough, a few surprises have occurred back to back in recent weeks which are making scientists rethink their assumptions about these moons.

The first came from Io, Jupiter’s innermost moon and the most volcanically active body in the Solar System. All told, the surface has over 400 volcanic regions, roughly 100 mountains – some of which are taller than Mount Everest – and extensive lava flows and floodplains of liquid rock that pass between them. All of this has lead to the formation of Io’s atmosphere, which is basically a thin layer of toxic fumes.

Io_mapGiven its distance from Earth, it has been difficult to get a good reading on what the atmosphere is made up of. However, scientists believe that it is primarily composed of sulfur dioxide (SO2), with smaller concentrations of sulfur monoxide (SO), sodium chloride (NaCl), and atomic sulfur and oxygen. Various models predict other molecules as well, but which have not been observed yet.

However, recently a team of astronomers from institutions across the US, France, and Sweden, set out to better constrain Io’s atmosphere. Back in September they detected the second-most abundant isotope of sulfur (34-S) and tentatively detected potassium chloride (KCl). Expected, but undetected, were molecules like potassium chloride (KCl), silicone monoxide (SiO), disulfur monoxide (S2O), and other isotopes of sulfur.

Io_surfaceBut more impressive was the team’s tentative of potassium chloride (KCl), which is believed to be part of the plasma torus that Io projects around Jupiter. For some time now, astronomers and scientists have been postulating that Io’s volcanic eruptions produce this ring of plasma, which includes molecular potassium. By detecting this, the international team effectively found the “missing link” between Io and this feature of Saturn.

Another find was the team’s detection of the sulfur 34-S, an isotope which had previously never been observed.  Sulfur 32-S had been detected before, but the ratio between the 34-S and 32-S was twice that of what scientists believed was possible in the Solar System. A fraction this high has only been reported once before in a distant quasar – which was in fact an early galaxy consisting of an intensely luminous core powered by a huge black hole.

These observations were made using the Atacama Pathfinder Experiment (APEX) antenna – a radio telescope located in northern Chile. This dish is a prototype antenna for the Atacama Large Millimeter Array (ALMA). And while Io is certainly an extreme example, it will likely help terrestrial scientists characterize volcanism in general – providing a better understanding of it here on Earth as well as outside the Solar System.

TitanThe second big discovery was announced just yesterday, and comes from NASA’s Cassini space probe. In its latest find investigating Saturn’s largest moon, Cassini made the first off-world detection of the molecule known as propelyne. This simple organic compound is a byproduct of oil refining and fossil fuel extraction, and is one of the most important starting molecules in the production of plastics.

The molecules were detected while Cassini used its infrared spectrometer to stare into the hydrocarbon haze that is Titan’s atmosphere. The discovery wasn’t too surprising, as Titan is full of many different types of hydrocarbons including methane and propane. But spotting propylene has thus far eluded scientists. What’s more, this is the first time that the molecule has been spotted anywhere outside of Earth.

titan_cassiniThese finding highlight the alien chemistry of Saturn’s giant moon. Titan has moisture and an atmosphere, much like our own, except that its rains are made of hydrocarbons and its seas composed of ethane. Scientists have long wanted to explore this world with a boat-like rover, but given the current budget environment, that’s a distant prospect. Still, sales of propylene on Earth are estimated at $90 billion annually.

While no one is going to be mounting a collection mission to Titan anytime soon, it does offer some possibilities for future missions. These include colonization, where atmospheric propylene could be used to compose settlements made of plastic. And when it comes to terraforming, knowing the exact chemical makeup of the atmosphere will go a long way towards finding a way to make it breathable and warm.

And in the meantime, be sure to enjoy this video about Cassini’s latest discovery. With the government shutdown in effect, NASA’s resources remain offline. So we should consider ourselves lucky that the news broke before today and hope like hell they get things up and running again soon!


Sources: universetoday.com, wired.com

I Saw Sunspots Today!

solar1Today, I achieved a personal first and got to see an astronomical phenomena that few people will. While attending an open house event at my local Aviation Museum, I managed to meet up with a man who had set up a stargazing station and was showcasing some serious equipment. After waiting my turn, I got to peer through his special telescope with a sun filter. And what I saw, as the title would suggest, was something truly amazing – sunspots!

As some may know, sunspots have remained something of a mystery to astronomers and philosophers until the Scientific Revolution of the 16th century. It was at this time that Galileo observed them using his own telescope, which he did by projecting the image onto sheets of paper and recording the imperfections in the light.

sunspots1The discovery was important in helping to disprove the prevailing theory that the Earth was at the center of the universe – aka. the Geocentric theory. Up until this time, European philosophers were living under the impression that the Sun, like all celestial bodies that were believed to orbit the Earth, was a perfect sphere. By showing it to be riddled with imperfections, Galileo placed an additional nail in the philosophical basis of this idea.

This in turn helped pave the way for the acceptance of Copernicus’ theory of a Heliocentric universe. As with his observations that Jupiter had its own set of moons, that the Moon itself did not have a polished crystalline surface, and that Copernicus’ theory resolved numerous logical inconsistencies in the other model, Galileo helped to establish the field of truly scientific astronomy.

sunspot_activityToday, I learned that observing sunspots continues to be a difficult thing, since direct observation with a telescope is impossible without sun filter. Not only that, but many people mistake high-magnification for high-power, which in turn leads to images that are not of the best quality. And observing them can by difficult since they go through cycles.

As the kind host of the solar observation explained, and this NASA graph shows, sunspot activity goes through a cycle that repeats every eleven years. As we are currently at the edge of a peek in the cycle, its prime time to get a look at sunspots in the sky. The last time anyone could get a good look was in 2001, and the next opportunity won’t come until 2023.

So I feel pretty privileged, both as a geeky, space-enthusiast and a regular person. If you know someone who has access to a telescope with a solar filter, or just happen to live near an observatory that conducts tours, get out there and spot those surface imperfections. I’m not exaggerating when I say its a rare treat!

News From Space: Center of the Universe Closing!

center_universeYeah, that title might be a bit misleading. Technically, the news comes from Earth, but has everything to do with our study of the heavens. And this story comes to you from my own neck of the woods where – just a few kilometers from my house – the Dominion Astrophysical Observatory is about to shut down due to budget cuts.

Typically, it goes by the name of Center of the Universe, a national historic site and a hub for astronomy education in Victoria. And at the end of the summer, in what I can only say its a tragedy, it will be closed to the public for good. The National Research Council (NRC) put the official closing date at the end of August, right after the last of the student summer camps ends.

center_universe2In addition, the facility houses historical artifacts like the original 1.8 metre mirror from the Plaskett Telescope and runs historical tours, multimedia shows, and youth programs. Unfortunately, this all costs about $32,000 to operate and $245,000 in employee wages, and brings in only about $47,000 per year in revenue. This gives the NRC a deficit of about $230,000 a year for this facility alone.

Naturally, Charles Drouin, spokesman for the NRC in Ottawa, said that the decision did not come easy, but was necessary. He confirmed that the active astronomy facility and national historic site will have no public outreach come late August or early September, and locals and visitors will no longer be able to tour the Plastkett Telescope, in operation since May 6, 1918.

center_universe3On the bright side, the historical artifacts and displays in the Centre of the Universe building will remain in place after the facility is closed. The NRC will also be working with local community groups to find volunteers to use the space, so it will remain in operation, though in a limited capacity. This much is good news, since the loss of the site in its entirety would be an immeasurable loss for this community.

Interestingly enough, Drouin also claimed that the decision to close the facility was unrelated to the federal governments announcement in May to reorganize the NRC as an “industry-focused research and technology organization.” In short, the budget-driven decision is not being blamed on funding cuts or the desire to privatize. I wonder…

center_universe1Personally, I am sad and ashamed to hear this news. The wife and I have been saying for ages that we need to go to this place and take a tour. Granted, that is not the easiest thing in the world to arrange, what with all the booked tours and the way the place seems to have an odd schedule. But you’d think we could have arranged something by now. It’s a national observatory, and right in my backyard for God sakes! To think we might have missed our chance is just plain sad…

However, there is still time, and I strongly recommend that anybody in the Saanich, Victoria, or Vancouver and Island region get their butts out and do what they can to see the place in operation before it shuts down. No telling what kind of hours and limited services it will be offering once its got only volunteers manning it. We need to take a gander at this star-gazing facility now before we lose the opportunity!

And be sure to check out their website too!

Source: vicnews.com, nrc-cnrc.gc.ca

New Super-Earth Discovered

It has been an exciting year for the discovery exoplanets! First, there was the news from Gliese 581 g, then the discovery of an Earth-like planet in Alpha Centauri. And now, scientists working in the European Southern Observatory’s HARPS apparatus have announced the discovery of the latest Super-Earth, which they believe to be the greatest candidate for extra-terrestrial life yet.

The planet is located in the HD 40307 system, an orange dwarf star that is just 42 light years from Earth. Although scientists are still not entirely sure that it’s a rocky planet, there are a number of strong indications that point towards and hospital terrestrial environment. For starters, as the sixth and farthest planet in the system, it lies within the sun’s habitable zone.

Second, the planet has a very reasonable 320 day annual cycle, which means that it receives a similar amount of solar energy compared to Earth – about 62% of what we get year round. This is positive news since most Super-Earths are situated too close to their parent stars to boast life. And last, but not least, the planet is unique amongst its near-Earth exoplanet kin in that it is not tidally locked, meaning it has a night and day cycle. Though this is not absolutely crucial to life, it is a bonus seeing as how it means one side of the planet is  not constantly exposed to radiation while the other is constantly in a state of cold, life denying darkness.

Mikko Tuomi of the University of Hertfordshire in the UK, and Guillem Anglada-Escude from Germany’s University of Goettingen are chiefly responsible for this discovery. In the coming weeks, months and years, their team will be doing their best to ascertain the planet’s composition, which they hope to be rocky in nature. If this should prove to be the case, it will move to the top of likely candidates for exoplanet colonization, pushing such planets as Gliese 581 g, the most Earth-like exoplanet discovered to date, out of the top spot.

Source: Discovery News