News Archives

February 23, 2016March 18, 2016 by Bob King

NASA Releases Strange ‘Music’ Heard By 1969 Astronauts

Lunar module pilot Eugene Cernan en route to the Moon during the Apollo 10 mission in the spring of 1969. Credit: NASA

Calling it music is a stretch, but that’s exactly how the Apollo 10 astronauts described the creepy sounds they heard while swinging around the farside of the moon in May 1969. During the hour they spent alone cut off from communications with Earth, all three commented about a persistent “whistling” sound that lunar module pilot (LMP) likened to “outer-space-type-music”. Once the craft returned to the nearside, the mysterious sounds disappeared.

Apollo 10 Farside-of-the-Moon Music.

Hands down it was aliens! I wish. Several online stories fan the coals of innuendo and mystery with talk of hidden files and NASA cover-ups narrated to disturbing music. NASA agrees that the files were listed as ‘confidential’ in 1969 at the height of the Space Race, but the Apollo 10 mission transcripts and audio have been publicly available at the National Archives since 1973. Remember, there was no Internet back then. The audio files were only digitized and uploaded for easy access in 2012. Outside of the secretive ’60s, the files have been around a long time.

Part of the Apollo 10 transcript of the conversation among the three Apollo 10 astronauts while they orbited the farside of the Moon. Credit: NASA — Part of the Apollo 10 transcript of the conversation among the three Apollo 10 astronauts while they orbited the farside of the Moon. Click the image for a pdf copy of the full mission transcript. Credit: NASA

The story originally broke Sunday night in a show on the cable channel Discovery as part of the “NASA’s Unexplained Files” series; you’ll find their youtube video below. As I listen to the sound file, I hear two different tones. One is a loud, low buzz, the other a whooshing sound. My first thought was interference of some sort for the buzzing sound, but the whoosh reminded me of a whistler, a low frequency radio wave generated by lightning produced when energy from lightning travels out into Earth’s magnetic field from one hemisphere to another. Using an appropriate receiver, we can hear whistlers as descending, whistle-like tones lasting up to several seconds.

Earthrise as photographed by the Apollo 10 crew in May 1969. Credit: NASA

Lightning’s hardly likely on the Moon, and whistlers require a magnetic field, which the Moon also lacks. The cause turns out to be, well, man-made. Cernan’s take was that two separate VHF radios, one in the lunar module and the other in command module, were interfering with one another to produce the noise. This was later confirmed by Apollo 11 astronaut Mike Collins who flew around the lunar farside alone when Buzz Aldrin and Neil Armstrong walked on the Moon’s surface.

The Apollo 10 command/service module nicknamed "Charlie Brown" orbiting the Moon as seen from the lunar module. Credit: NASA — The Apollo 10 command service module nicknamed “Charlie Brown” orbiting the Moon as seen from the lunar module. Apollo 10 was a full dress rehearsal for the Apollo 11 mission to place a man on the Moon. Click the image to visit the Apollo 10 photo archive. Credit: NASA

In his book Carrying the Fire, Collins writes: “There is a strange noise in my headset now, an eerie woo-woo sound.” He said it might have scared him had NASA’s radio technicians not forewarned him. The “music” played when the two craft were near one another with their radios turned on. Unlike Apollo 10, which never descended to the Moon’s surface but remained near the command module, the Apollo 11 lunar module touched down on the Moon on July 20, 1969. Once it did, Collins writes that the ‘woo-woo’ music stopped.

The astronauts never talked publicly or even with the agency about hearing weird sounds in space for good reason. Higher-ups at NASA might think them unfit for future missions for entertaining weird ideas, so they kept their thoughts private. This was the era of the “right stuff” and no astronaut wanted to jeopardize a chance to fly to the Moon let alone their career.

Outer Space Music Part 1 of NASA’s Unexplained Files — to be taken with a boulder of salt

In the end, this “music of the the spheres” makes for a fascinating tidbit of outer space history. There’s no question the astronauts were spooked, especially considering how eerie it must have felt to be out of touch with Earth on the far side of the Moon. But once the sounds stopped, they soldiered on — part of the grand human effort to touch another world.

“I don’t remember that incident exciting me enough to take it seriously,” Gene Cernan told NASA on Monday. “It was probably just radio interference. Had we thought it was something other than that we would have briefed everyone after the flight. We never gave it another thought.”

Messages from the Ringed Planet

Want to hear some real outer space music? Click the Saturn video and listen to the eerie sound of electrons streaming along Saturn’s magnetic field to create the aurora.

February 23, 2016March 18, 2016 by Evan Gough

NASA Thinks There’s a Way to Get to Mars in 3 Days

Interstellar travel will require near-light-speed to be feasible. Image: NASA

We’ve achieved amazing things by using chemical rockets to place satellites in orbit, land people on the Moon, and place rovers on the surface of Mars. We’ve even used ion drives to reach destinations further afield in our Solar System. But reaching other stars, or reducing our travel time to Mars or other planets, will require another method of travel. One that can approach relativistic speeds.

Your aim has to be really really good. Credit: UCSB Experimental Cosmology Group

We can execute missions to Mars, but it takes several months for a vehicle to reach the Red Planet. Even then, those missions have to be launched during the most optimal launch windows, which only occur every 2 years. But the minds at NASA never stop thinking about this problem, and now Dr. Philip Lubin, Physics Professor at the University of California, Santa Barbara, may have come up with something: photonic propulsion, which he thinks could reduce the travel time from Earth to Mars to just 3 days, for a 100 kg craft.

The system is called DEEP IN, or Directed Propulsion for Interstellar Exploration. The general idea is that we have achieved relativistic speeds in the laboratory, but haven’t taken that technology—which is electromagnetic in nature, rather than chemical—and used it outside of the laboratory. In short, we can propel individual particles to near light speed inside particle accelerators, but haven’t expanded that technology to the macro level.

Directed Energy Propulsion differs from rocket technology in a fundamental way: the propulsion system stays at home, and the craft doesn’t carry any fuel or propellant. Instead, the craft would carry a system of reflectors, which would be struck with an aimed stream of photons, propelling the craft forward. And the whole system is modular and scalable.

If that’s not tantalizing enough, the system can also be used to deflect hazardous space debris, and to detect other technological civilizations. As talked about in this paper, detecting these types of systems in use by other civilizations may be our best hope for discovering those civilizations.

There’s a roadmap for using this system, and it starts small. At first, DEEP IN would be used to launch small cube satellites. The feedback from this phase would then inform the next step, which would be to test a unit for defending the ISS from space debris. From then, the systems would meet goals of increasing complexity, from launching satellites to LEO (Low-Earth Orbit) and GEO (Geostationary Orbit), all the way up to asteroid deflection and planetary defense. After that, relativistic drives capable of interstellar travel is the goal.

There are lots of questions still to be answered of course, like what happens when a vehicle at near light-speed hits a tiny meteorite. But those questions will be asked and answered as the system is developed and its capabilities grow.

Obviously, DEEP IN has the potential to bring other stars into reach. This system could deliver probes to some of the more promising exo-planets, and give humanity its first detailed look at other solar systems. If DEEP IN can be successfully scaled up, as Lubin says, then it will be a transformational technology.

Here’s a longer video of Dr. Lubin explaining DEEP IN in greater depth and detail: http://livestream.com/viewnow/niac2015seattle

Here’s the website for the University of California Santa Barbara Experimental Cosmology Group: http://www.deepspace.ucsb.edu/

February 22, 2016April 26, 2016 by Bob King

Does Antarctica Have A Hidden Layer Of Meteorites Below Its Surface?

Dr. Barbara Cohen is seen with a large meteorite from the Antarctic's Miller Range. Credit: Antarctic Search for Meteorites

ANSMET 2012-2013 team collecting a meteorite sample (Image: Antarctic Search for Meteorites Program / Katherine Joy) — Two members of the Antarctic Search for Meteorites 2012-2013 team use tongs to collect a meteorite near the Transantarctic Mountains. Credit: Katherine Joy, University of Manchester / Antarctic Search for Meteorites Program

In the category of why-didn’t-I think-of-that ideas, Dr. Geoffrey Evatt and colleagues from the University of Manchester struck upon a brilliant hypothesis: that a layer of iron meteories might lurk just below the surface of the Antarctic ice. He’s the lead author of a recent paper on the topic published in the open-access journal, Nature Communications.

A likely stony meteorite found during the ANSMET 2014-15 expedition in Antarctica. Credit: JSC Curation / NASA — A possible stony meteorite found during the ANSMET 2014-15 expedition in Antarctica. Credit: Antarctic Search for Meteorites Program

Remote Antarctica makes one of the best meteorite collecting regions on the planet. Space rocks have been accumulating there for millennia preserved in the continent’s cold, desert-like climate. While you might think it’s a long and expensive way to go to hunt for meteorites, it’s still a lot cheaper than a sample return mission to the asteroid belt. Meteorites fall and become embedded in ice sheets within the continent’s interior. As that ice flows outward toward the Antarctic coastlines, it pushes up against the Transantarctic Mountains, where powerful, dry winds ablate away the ice and expose their otherworldly cargo.

Meteorite recovery sites in the Transantarctic Mountains. Credit: NASA

Layer after layer, century after century, the ice gets stripped away, leaving rich “meteorite stranding zones” where hundreds of space rocks can be found within an area the size of a soccer field. Since most meteorites arrive on Earth coated in a black or brown fusion crust from their searing fall through the atmosphere, they contrast well against the white glare of snow and ice. Scientists liken it to a conveyor belt that’s been operating for the past couple million years.

Scientists form snowmobile posses and buzz around the ice fields picking them up like candy eggs on Easter morning. OK, it’s not that easy. There’s much planning and prep followed by days and nights of camping in bitter cold with high winds tearing at your tent. Expeditions take place from October through early January when the Sun never sets.

The U.S. under ANSMET (Antarctic Search for Meteorites, a Case Western Reserve University project funded by NASA), China, Japan and other nations run programs to hunt and collect the precious from the earliest days of the Solar System before they find their way to the ocean or are turned to dust by the very winds that revealed them in the first place. Since systematic collecting began in 1976, some 34,927 meteorites have been recovered from Antarctica as of December 2015.

A team of scientists document the find of a small meteorite found among rocks on the Antarctic ice during the ANSMET 2014-15 hunt. Credit: JSC Curation / NASA — A team of scientists document the find of a small meteorite found among rocks on the Antarctic ice during the ANSMET 2014-15 expedition. Credit: Antarctic Search for Meteorites Program / Vinciane Debaille

Meteorites come in three basic types: those made primarily of rock; stony-irons comprised of a mixture of iron and rock; and iron-rich. Since collection programs have been underway, Antarctic researchers have uncovered lots of stony meteorites, but meteorites either partly or wholly made of metal are scarce compared to what’s found in other collecting sites around the world, notably the deserts of Africa and Oman. What gives?

A fragment of the Sikhote-Alin iron meteorite that fell over eastern Russia (then the Soviet Union) on Feb. 12, 1947. Some of the dimpling are pockets on the meteorite's surface called regmeglypts. Credit: Bob King — This fragment of the massive Sikhote-Alin meteorite that fell over eastern Russia (then the Soviet Union) on Feb. 12, 1947 is a typical iron-nickel meteorite. Another specimen of this meteorite was used in the experiment to determine how quickly it burrowed into the ice when heated. Credit: Bob King

Dr. Evatt and colleagues had a hunch and performed a simple experiment to arrive at their hypothesis. They froze two meteorites of similar size and shape — a specimen of the Russian Sikhote-Alin iron and NWA 869, an ordinary (stony) chondrite — inside blocks of ice and heated them using a solar-simulator lamp. As expected, both meteorites melted their way down through the ice in time, but the iron meteorite sank further and faster. I bet you can guess why. Iron or metal conducts heat more efficiently than rock. Grab a metal camera tripod leg or telescope tube on a bitter cold night and you’ll know exactly what I mean. Metal conducts the heat away from your hand far better and faster than say, a piece of wood or plastic.

Antarctic researchers carefully pack meteorites into collection boxes. Looks cold! Credit: JSC Curation / NASA — Antarctic researchers carefully pack meteorites found along the Transantarctic Range into collection boxes. Looks cold! Credit: Antarctic Search for Meteorites Program / Vinciane Debaille

The researchers performed many trials with the same results and created a mathematical model showing that Sun-driven burrowing during the six months of Antarctic summer accounted nicely for the lack of iron meteorites seen in the stranding zones. Co-author Dr. Katherine Joy estimates that the fugitive meteorites are trapped between about 20-40 inches (50-100 cm) beneath the ice.

Who wouldn’t be happy to find this treasure? Dr. Barbara Cohen is seen with a large meteorite from the Antarctic’s Miller Range. Credit: Antarctic Search for Meteorites Program

You can imagine how hard it would be to dig meteorites out of Antarctic ice. It’s work enough to mount an expedition to pick up just what’s on the surface.

With the gauntlet now thrown down, who will take up the challenge? The researchers suggests metal detectors and radar to help locate the hidden irons. Every rock delivered to Earth from outer space represents a tiny piece of a great puzzle astronomers, chemists and geologist have been assembling since 1794 when German physicist Ernst Chladni published a small book asserting that rocks from space really do fall from the sky.

Like the puzzle we leave unfinished on the tabletop, we have a picture, still incomplete, of a Solar System fashioned from the tiniest of dust motes in the crucible of gravity and time.

February 19, 2016April 26, 2016 by Bob King

Hubble Directly Measures Rotation of Cloudy ‘Super-Jupiter’

Illustration of the hot extrasolar planet 2M1207b orbiting a brown dwarf. Credits: NASA, ESA, and G. Bacon/STScI

Astronomers using the Hubble Space Telescope have measured the rotation rate of an extreme exoplanet 2M1207b by observing the varied brightness in its atmosphere. This is the first measurement of the rotation of a massive exoplanet using direct imaging.

This is a composite image of the brown dwarf object 2M1207 (centre) and the fainter object seen near it, at an angular distance of 778 milliarcsec. Designated "Giant Planet Candidate Companion" by the discoverers, it may represent the first image of an exoplanet. Further observations, in particular of its motion in the sky relative to 2M1207 are needed to ascertain its true nature. The photo is based on three near-infrared exposures (in the H, K and L' wavebands) with the NACO adaptive-optics facility at the 8.2-m VLT Yepun telescope at the ESO Paranal Observatory. — This is a composite image of the brown dwarf object 2M1207 (blue-white) and the planet 2M1207b, seen in red, located 170 light years from Earth in the constellation Centaurus. The photo is based on three near-infrared exposures with the taken with the 8.2-m VLT Yepun telescope at the ESO Paranal Observatory. Credit: ESO

Little by little we’re coming to know at least some of the 2,085 exoplanets discovered to date more intimately despite their great distances and proximity to the blinding light of their host stars. 2M1207b is about four times more massive than Jupiter and dubbed a “super-Jupiter”. Super-Jupiters fill the gap between Jupiter-mass planets and brown dwarf stars. They can be up to 80 times more massive than Jupiter yet remain nearly the same size as that planet because gravity compresses the material into an ever denser, more compact sphere.

2M1207b lies 170 light years from Earth and orbits a brown dwarf at a distance of 5 billion miles. By contrast, Jupiter is approximately 500 million miles from the sun. You’ll often hear brown dwarfs described as “failed stars” because they’re not massive enough for hydrogen fusion to fire up in their cores the way it does in our sun and all the rest of the main sequence stars.

Researchers used Hubble’s exquisite resolution to precisely measure the planet’s brightness changes as it spins and nailed the rotation rate at 10 hours, virtually identical to Jupiter’s. While it’s fascinating to know a planet’s spin, there’s more to this extraordinary exoplanet. Hubble data confirmed the rotation but also showed the presence of patchy, “colorless” (white presumably) cloud layers. While perhaps ordinary in appearance, the composition of the clouds is anything but.

exoplanet 2M1207 b with the Solar System planet Jupiter. Although four times more massive than the Jovian planet, gravity compresses its matter to keep it relatively small. Credit: Wikipedia / Aldaron — Exoplanet 2M1207 b with the Solar System planet Jupiter for comparison. Although four times more massive than the Jovian planet, gravity compresses its matter to keep it relatively small. Credit: Wikipedia / Aldaron

The planet appears bright in infrared light because it’s young (about 10 million years old) and still contracting, releasing gravitational potential energy that heats it from the inside out. All that extra heat makes 2M1207b’s atmosphere hot enough to form “rain” clouds made of vaporized rock. The rock cools down to form tiny particles with sizes similar to those in cigarette smoke. Deeper into the atmosphere, iron droplets are forming and falling like rain, eventually evaporating as they enter the lower levels of the atmosphere.

“So at higher altitudes it rains glass, and at lower altitudes it rains iron,” said Yifan Zhou of the University of Arizona, lead author on the research paper in a recent Astrophysical Journal. “The atmospheric temperatures are between about 2,200 to 2,600 degrees Fahrenheit.” Every day’s a scorcher on 2M1207b.

Both Jupiter and Saturn also emit more heat than they receive from the sun because they too are still contracting despite being 450 times older. The bigger you are, the slower you chill.

Illustration of the extrasolar planet 2M1207b (foreground) orbiting a brown dwarf. Credits: NASA, ESA, and G. Bacon/STScI — Illustration of the extrasolar planet 2M1207b (foreground) orbiting a brown dwarf. Both shine brightly in infrared light. Credits: NASA, ESA, and G. Bacon/STScI

All the planets in our Solar System possess only a fraction of the mass of the Sun. Even mighty Jove is a thousand times less massive. But Mr. Super-Jupiter’s a heavyweight compared to its brown dwarf host, being just 5-7 times less massive. While Jupiter and the rest of the planets formed by the accretion of dust and rocks within a clumpy disk of material surrounding the early Sun, it’s thought 2M1207b and its companion may have formed throughout the gravitational collapse of a pair of separate disks.

This super-Jupiter will an ideal target for the James Webb Space Telescope, a space observatory optimized for the infrared scheduled to launch in 2018. With its much larger mirror — 21-feet (6.5-meters) — Webb will help astronomers better determine the exoplanet’s atmospheric composition and created more detailed maps from brightness changes.

Teasing out the details of 2M1207b’s atmosphere and rotation introduces us to a most alien world the likes of which never evolved in our own Solar System. I feel like I’m aboard the Starship Enterprise visiting far-flung worlds. Only this is better. It’s real.

February 19, 2016March 18, 2016 by Evan Gough

We Have Underestimated Our Sun’s Destructive Reach

Artists concept of a shredded asteroid getting too close to a star. (NASA/JPL-Caltech)

The Sun has enormous destructive power. Any objects that collide with the Sun, such as comets and asteroids, are immediately destroyed.

But now we’re finding that the Sun has the ability to reach out and touch asteroids at a far greater distance than previously thought. The proof of this came when a team at the University of Hawaii Institute of Astronomy was looking at Near-Earth Objects (NEOs) catalogued by the Catalina Sky Survey, and trying to understand what asteroids might be missing from that survey.

An asteroid is classified as an NEO when, at its closest point to the Sun, it is less than 1.3 times the distance from the Earth to the Sun. We need to know where these objects are, how many of them there are, and how big they are. They’re a potential threat to spacecraft, and to Earth itself.

The 60 inch Mt. Lemmon telescope is one of three telescopes used in the Catalina Sky Survey. Image: Catalina Sky Survey, University of Arizona.

The Catalina Sky Survey (CSS) detected over 9,000 NEOs in eight years. But asteroids are notoriously difficult to detect. They are tiny points of light, and they’re moving. The team knew that there was no way the CSS could have detected all NEOs, so Dr. Robert Jedicke, a team member from the University of Hawaii Institute of Astronomy, developed software that would tell them what CSS had missed in its survey of NEOs.

This took an enormous amount of work—and computing power—and when it was completed, they noticed a discrepancy: according to their work, there should be over ten times as many objects within ten solar diameters of the Sun as they found. The team had a puzzle on their hands.

The team spent a year verifying their work before concluding that the problem did not lay in their analysis, but in our understanding of how the Solar System works. University of Helsinki scientist Mikael Granvik, lead author of the Nature article that reported these results, hypothesized that their model of the NEO population would better suit their results if asteroids were destroyed at a much greater distance from the sun than previously thought.

They tested this idea, and found that it agreed with their model and with the observed population of NEOs, once asteroids that spent too much time within 10 solar diameters of the Sun were eliminated. “The discovery that asteroids must be breaking up when they approach too close to the Sun was surprising and that’s why we spent so much time verifying our calculations,” commented Dr. Jedicke.

There are other discrepancies in our Solar System between what is observed and what is predicted when it comes to the distribution of small objects. Meteors are small pieces of dust that come from asteroids, and when they enter our atmosphere they burn up and make star-gazing all the more eventful. Meteors exist in streams that come from their parent objects. The problems is, most of the time the streams can’t be matched with their parent object. This study shows that the parent objects must have been destroyed when they got too close to the Sun, leaving behind a stream of meteors, but no apparent source.

There was another surprise in store for the team. Darker asteroids are destroyed at a greater distance from the Sun than lighter ones are. This explains an earlier discovery, which showed that brighter NEOs travel closer to the Sun than darker ones do. If darker asteroids are destroyed at a greater distance from the Sun than their lighter counterparts, then the two must have differing compositions and internal structure.

“Perhaps the most intriguing outcome of this study is that it is now possible to test models of asteroid interiors simply by keeping track of their orbits and sizes. This is truly remarkable and was completely unexpected when we first started constructing the new NEO model,” says Granvik.

February 18, 2016March 18, 2016 by Evan Gough

Did a Gamma Ray Burst Accompany LIGO’s Gravity Wave Detection?

An artist's impression of a Gamma Ray Burst. Credit: Stanford.edu

Last week’s announcement that Gravitational Waves (GW) have been detected for the first time—as a result of the merger of two black holes—is huge news. But now a Gamma Ray Burst (GRB) originating from the same place, and that arrived at Earth 0.4 seconds after the GW, is making news. Isolated black holes aren’t supposed to create GRB’s; they need to be near a large amount of matter to do that.

NASA’s Fermi telescope detected the GRB, coming from the same point as the GW, a mere 0.4 seconds after the waves arrived. Though we can’t be absolutely certain that the two phenomena are from the same black hole merger, the Fermi team calculates the odds of that being a coincidence at only 0.0022%. That’s a pretty solid correlation.

So what’s going on here? To back up a little, let’s look at what we thought was happening when LIGO detected gravitational waves.

Our understanding was that the two black holes orbited each other for a long time. As they did so, their massive gravity would have cleared the area around them of matter. By they time they finished circling each other and merged, they would have been isolated in space. But now that a GRB has been detected, we need some way to account for it. We need more matter to be present.

According to Abraham Loeb, of Harvard University, the missing piece of this puzzle is a massive star—itself the result of a binary star system combining into one—a few hundred times larger than the Sun, that spawned two black holes. A star this size would form a black hole when it exhausted its fuel and collapsed. But why would there be two black holes?

Again, according to Loeb, if the star was rotating at a high enough rate—just below its break up frequency—the star could actually form two collapsing cores in a dumbbell configuration, and hence two black holes. But now these two black holes would not be isolated in space, they would actually be inside a massive star. Or what was left of one. The remnants of the massive star is the missing matter.

When the black holes joined together, an outflow would be generated, which would produce the GRB. Or else the GRB came “from a jet originating out of the accretion disk of residual debris around the BH remnant,” according to Loeb’s paper. So why the 0.4 s delay? This is the time it took the GRB to cross the star, relative to the gravitational waves.

It sounds like a nice tidy explanation. But, as Loeb notes, there are some problems with it. The main question is, why was the GRB so weak, or dim? Loeb’s paper says that “observed GRB may be just one spike in a longer and weaker transient below the GBM detection threshold.”

But was the GRB really weak? Or was it even real? The European Space Agency has their own gamma ray detecting spacecraft, called Integral. Integral was not able to confirm the GRB signal, and according to this paper, the gamma ray signal was not real after all.

As they say in show business, “Stay tuned.”

February 17, 2016March 18, 2016 by Evan Gough

First Super-Earth Atmosphere Detected

A new paper says that a Super-Earth may have formed in our Solar System and been swallowed by the Sun. Image Credit: ESA/Hubble, M. Kornmesser

55 Cancri-e was once touted as one of the most exotic exo-planets ever discovered. Mass and radius modelling led some astronomers to speculate that its interior could be rich in carbon. And that much carbon crushed together under extreme pressure = diamonds. That’s how it got its nickname “Diamond Planet.”

But 55 Cancri-e—now named “Janssen” (Thank you International Astronomical Union!)—is even more exotic with the recent discovery of an atmosphere. A February 7th research paper in the Astrophysical Journal, by a team of European astronomers, reports that Janssen has an atmosphere rich in hydrogen. This makes Janssen the first exo-planet, that we know of, to have an atmosphere.

The team used the Wide Field Camera 3 (WDF3) on the Hubble Space Telescope, and a new scanning technique, to gain an understanding of Janssen’s atmosphere. Along with hydrogen, the team also found helium, and potentially, hydrogen cyanide.

Given Janssen’s surface temperature of 2000 K (1727 C), and its proximity to its host star, the existence of an atmosphere is surprising. The team suspects that the hydrogen-rich atmosphere is left over from the planet’s formation 8 billion years ago, and is a remnant of the nebula that the planet and star formed from.

“Our observations of 55 Cancri e’s atmosphere suggest that the planet has managed to cling on to a significant amount of hydrogen and helium from the nebula from which it formed,” said Angelos Tsiaras, a PhD student at UCL, who helped develop the new scanning technique. “This is a very exciting result because it’s the first time that we have been able to find the spectral fingerprints that show the gases present in the atmosphere of a super-Earth.”

Super-Earths are the most common type of planet in our galaxy, though none exist in our solar system. They are called super-Earths because they have more mass than Earth, but are smaller than the gas giants. A greater understanding of super-Earths should mean a greater understanding of the most common type of planet around.

“This result gives a first insight into the atmosphere of a super-Earth. We now have clues as to what the planet is currently like, how it might have formed and evolved, and this has important implications for 55 Cancri e and other super-Earths,” said Professor Giovanna Tinetti of UCL.

The existence of hydrogen cyanide in Janssen’s atmosphere is also significant. Its presence indicates a carbon-rich atmosphere. This supports the idea that Janssen is a diamond planet, though that conclusion is still far from certain. “If the presence of hydrogen cyanide and other molecules is confirmed in a few years time by the next generation of infrared telescopes, it would support the theory that this planet is indeed carbon rich and a very exotic place,” said Professor Jonathan Tennyson, UCL.

The team has used their new technique on 2 other super-Earths, but no atmosphere was found.

55-Cancri e is about 40 light years from Earth. Its host star is slightly smaller, cooler, and a little dimmer than our Sun, and its year is shorter than an Earth day.

February 16, 2016March 18, 2016 by Evan Gough

Russia’s New Ballistic Missiles to be Tested on Asteroids

Asteroids represent a real danger to Earth. But is targeting them with missiles, maybe nuclear, a good idea? Image: NASA/JPL/CalTech

In a shocking announcement, Russian scientists say they want to test improved ballistic missiles on the asteroid Apophis, which is expected to come dangerously close to Earth in 2036. If this doesn’t send chills down your spine, you haven’t read enough science fiction.

In a February 11th article in the Russian state-owned news agency TASS, Sabit Saitgarayev, the lead researcher at the Makeyev Rocket Design Bureau, says Russian scientists are developing a program to upgrade Inter-Continental Ballistic Missiles (ICBMs) to destroy near-Earth meteors from 20-50 metres in size. Apophis’ approach in 2036 would be a test for this program.

ICBM’s are the kind of long range nukes that the USSR and the USA had pointed at each other for decades during the Cold War. They still have some pointed at each other, and they can be launched quickly. This program would take that technology and improve it for anti-asteroid use.

Typical rockets of the type that take payloads into space are not good candidates for intercepting asteroids. They require too much lead time to meet the threat of an incoming asteroid that might be detected only days before impact. They can take several days to fuel. But ICBM’s are different. They can stand at the ready for long periods of time, and be launched at a moment’s notice. But to be suitable for use as asteroid killers, they have to be upgraded.

Design work on the asteroid-killing ICBM’s has already begun, admitted Saitgarayev, but he did not say whether the money has been committed or whether the authorization has been given to go ahead with the project. But like a lot of things that are said and done by Russia, it’s difficult to know exactly where the truth lies.

There’s no question that being prepared to prevent an asteroid strike on Earth is of the utmost importance. No matter where on Earth one was to strike, the effects could be global. But one thing’s certain: the development and testing of missiles designed to be used in space is unsettling.

It’s also unsettling in light of the January 16th TASS article stating that “The international scientific community has asked Russian scientists to develop an asteroid deflection system on the basis of nuclear explosions in space.” Taken together, the two announcements point towards a program of weaponizing space, something the international community has agreed should be avoided. In fact, there is a ban on nuclear explosions in space.

We don’t want to be alarmist. There are only a handful of countries in the world that have the capacity to develop some protective system against asteroids, and Russia is definitely one of them. And if Earth were threatened by an asteroid, the weaponization of space would be the least of our concerns.

The fact that Russia wants to develop a missile system with nuclear warheads, and employ it in space, is not entirely unreasonable. But it should make us stop and think. What will happen if something goes wrong?

It’s easy to imagine a scenario where an atomic explosion went off in low-Earth orbit. What would the consequences be? And what are the consequences to having one country develop this capability, rather than an international group? How can this whole endeavour be managed responsibly?

What do you think?

February 14, 2016March 18, 2016 by Matt Williams

Chinese Fusion Test Reportedly Reaches New Milestone

Researchers at the Experimental Advanced Superconducting Tokamak facility in China have achieved a new milestone in fusion power. Credit: ipp.cas.cn

Fusion power has long been considered to be the holy grail of alternative energy. Clean, abundant power, created through a self-sustaining process where atomic nuclei are fused at extremely high temperatures. Achieving this has been the goal of atomic researchers and physicists for over half a century, but progress has been slow. While the science behind fusion power is solid, the process has not exactly been practical.

In short, fusion can only be considered a viable form of power if the amount of energy used to initiate the reaction is less than the energy produced. Luckily, in recent years, a number of positive steps have been taken towards this goal. The latest comes from China, where researchers at the Experimental Advanced Superconducting Tokamak (EAST) recently report that they have achieved a fusion milestone.

Continue reading “Chinese Fusion Test Reportedly Reaches New Milestone”

February 12, 2016March 18, 2016 by Evan Gough

Retro Travel Posters Show Us The Future

Visitors to Jupiter view the Jovian auroras from balloons. Image: NASA/JPL.

One of the greatest things about being a space enthusiast is all of the discoveries that come out on an almost daily basis. One of the saddest things about being a space enthusiast is all of the discoveries and destinations that are so close, just beyond the horizon of our lifespan.

Will we colonize other planets? Sure, but most of us living will be gone by then. Will we spend time in glorious, gleaming space habitats? Obviously, but we’ll just be epitaphs by then. Sentient, alien species that gift us faster-than-light travel and other wonders? Maybe, but not before my bucket list has its final item checked off.

Citizen space travel? Hmmmm, tantalizingly within reach.

But now, new retro style posters from NASA, designed by the team at Invisible Creature, are making us feel nostalgic about things that haven’t even happened yet, and are helping us leave behind gloomy thoughts of being born at the wrong time.

The Grand Tour celebrates a time when our probes toured the planets, using gravity assist to propel them on their missions.

“Grandpa, do you remember the Grand Tour, when spacecraft used gravity assist to visit other worlds?”

“I sure do. Gravity assist. Those were the days. Swooping so close to Jupiter, you could feel the radiation killing your hair follicles. Only to be sling-shotted on to the next planet.”

“But why didn’t you just use a quantum drive to bend space time and appear at your destination?”

“Quantum drives! Those things ain’t natural. And neither is bending space-time. Give me a good old-fashioned chemical rocket any time.”

“Oh Grandpa.”

Visit the Historic Sites of Mars recalls a time when space pioneers colonized and terraformed Mars.

“Grandpa, what was Mars like in the Early Days?”

“You mean before it was terraformed? Very tough times.”

“Because conditions were so difficult? And food was hard to grow?”

“No. Because of the protesters.”

“Protesters? On Mars?”

“Yup. Every time we found a good spot for a Bacterial Production Facility (BPF), it seemed like there was an expired old rover in the way. The protesters didn’t think we should move ’em. Part of our heritage.”

“So what did you do Grandpa?”

“We created a network of computers that everybody would stare at all day. After that, nobody noticed what we did anymore.”

“Oh Grandpa.”

Visit Beautiful Southern Enceladus. Image: NASA/JPL

Visit Beautiful Southern Enceladus invites vacationers to visit Saturn’s sixth largest moon to view the ice geysers there.

“Grandpa, did you ever visit Enceladus?”

“I sure did. A beautiful, haunting place.”

“Was it scary? With all of the ice geysers erupting unpredictably?”

“On no. I always knew when one was going to erupt.”

“What? How did you know?”

“My arthritis would flare up.”

“Oh Grandpa.”

Category: News