Evan Gough, Author at Universe Today

May 11, 2016May 15, 2016 by Evan Gough

New Composite Image Of Saturn’s Polar Vortex Mesmerizes

This image of Saturn's southern polar vortex reveals previously unseen detail of the giant storm. Image: NASA/JPL/Space Science Institute

Atmospheric features on our Solar System’s gas giants dwarf anything similar on Earth. Earth’s atmosphere spawns hurricanes as larger as 1500 km in diameter. But on Saturn, a feature called the southern polar vortex has an eye that is 8,000 km across, or two thirds the diameter of the entire Earth.

A new high-resolution of Saturn’s southern polar vortex captured by the Cassini probe is ten times more detailed than any previous picture, and reveals details that were previously unseen. The image, which is a composite of two images taken by Cassini in July 2008, was captured when the spacecraft was 392,000 km from Saturn, and 56º below the plane of Saturn’s rings. Despite the distance and position, the image still has a resolution of 2 km per pixel.

Previous images of the vortex revealed clouds of immense proportions ringing the edge of the vortex, but showed the vortex itself to be clear. This is similar to a hurricane on Earth, where the eye itself is clear, but is ringed by wall-clouds of towering heights. This new image shows cloud formations within the vortex itself. The vortex is punctuated with wispy white cloud formations, and a smaller vortex at 10:00 within the larger formation.

The clouds inside the vortex are more than just pretty curiosities, of course. They are deep convective structures welling up from deep within Saturn’s atmosphere, and they form their own distinctive ring. This is all the more interesting because the eye of the vortex itself is generally clear, and is considered by scientists to be an area of downwelling.

The convection on display in Saturn’s southern polar vortex is an important clue to understanding how Saturn transfers energy through its atmosphere. On Earth, hurricanes are caused by warm water, and they move across the surface of the ocean as the warm water does.

Saturn, of course, has no liquid ocean, and the vortex is powered by warm atmospheric gases from deeper in Saturn. As they rise and cool they condense into clouds. The vortex also remains stationary, rather than following a warm mass of water. It’s locked into position over Saturn’s south pole.

Cassini’s narrow angle camera captured this new image, using a combination of two spectral filters. One was sensitive to wavelengths of polarized visible light centered at 617 nanometers, and the other to infrared light centered at 750 nanometers.

These two previously released infrared images of Saturn show the entire south polar region with the hurricane-like vortex in the center. The top image shows the polar region in false color, with red, green, and blue depicting the appearance of the pole in three different near-infrared colors (NASA/JPL/University of Arizona)

Cassini is a joint mission of NASA, the ESA, and the Italian Space Agency. It was launched in 1997, and has had its mission extended to September 2017. Cassini will end its mission in what the team operating Cassini is calling a Grand Finale. This will be a series of deep dives between Saturn and its rings, and will end with the spacecraft plunging into Saturn’s atmosphere.

To see a gallery of Cassini images, go here.

At Universe Today, we’ve written about Saturn’s polar vortices before. Have a look:

Violent Polar Cyclones on Saturn Imaged in Unprecedented Detail by Cassini

Hexagonal Structure at Saturn’s North Pole

May 10, 2016May 15, 2016 by Evan Gough

Winged Telescope Detects Martian Atomic Oxygen

SOFIA in flight, with its telescope exposed. Image: NASA/Jim Ross

Finding atomic oxygen in the Martian atmosphere is very difficult to do, which explains why it’s been 40 years since it was last detected. In the 1970’s, NASA’s Viking and Mariner missions detected Martian atmospheric oxygen, and now, the Stratospheric Observatory for Infrared Astronomy (SOFIA) has detected atomic oxygen in the upper portion of the Martian atmosphere called the mesosphere.

SOFIA is a specially modified Boeing 747 aircraft which carries a 100 inch telescope. It flies at altitudes between 37,000 to 45,000 feet, which puts it above most of the moisture in Earth’s atmosphere. This moisture would otherwise block the infrared radiation that SOFIA “sees.”

“Atomic oxygen in the Martian atmosphere is notoriously difficult to measure,” said Pamela Marcum, SOFIA project scientist. “To observe the far-infrared wavelengths needed to detect atomic oxygen, researchers must be above the majority of Earth’s atmosphere and use highly sensitive instruments, in this case a spectrometer. SOFIA provides both capabilities.”

A close-up of SOFIA's telescope and primary mirror. Image: NASA/Tom Tschida — A close-up of SOFIA’s telescope and primary mirror. Image: NASA/Tom Tschida

A special detector on board SOFIA, the German Receiver for Astronomy at Terahertz Frequencies (GREAT) allowed researchers to distinguish Martian atmospheric oxygen from Earthly oxygen. SOFIA-GREAT only detected half the amount of oxygen that scientists expected to find, which is probably due to changes and variations in the atmosphere. These results were published in a 2015 paper in Astronomy and Astrophysics.

Atomic oxygen has a strong effect on Mars’ atmosphere because it affects how other gases escape the atmosphere. It’s extreme volatility means it bonds with nearby molecules very easily; oxygen will combine with almost all chemical elements, except for the noble gases.

SOFIA is the largest airborne observatory in the world, and is a joint project between NASA and the German Aerospace Center. SOFIA has a 20 year mission timeline. Researchers will continue using SOFIA to study the Martian atmosphere, in order to better understand the variations in oxygen content.

SOFIA is not the only mission with eyes on Mars’ atmosphere. NASA’s Mars Atmosphere and Volatile EvolutioN (MAVEN) was launched in 2013 to explore the upper atmosphere of Mars, and how it’s affected by the solar wind. It’s thought that Mars’ atmosphere was much thicker in the past, and has been stripped away over time. Atomic oxygen played a role in Mars’ escaping atmosphere in the past, and no doubt will play a role in the future. SOFIA and other missions like MAVEN will hopefully shed some light on Mars’ past and future atmospheres.

May 9, 2016May 15, 2016 by Evan Gough

SpaceX Maiden Falcon Heavy Launch May Carry Satellite In November

An artist's illustration of the Falcon Heavy rocket. The Falcon Heavy has 3 engine cores, each one containing 9 Merlin engines. Image: SpaceX

Move over Arianespace and United Launch Alliance. SpaceX’s Falcon Heavy rocket is set for its maiden launch this November. The long-awaited Falcon Heavy should be able to outperform both the Ariane 5 and the ULA Delta-4 Heavy, at least in some respects.

The payload for the maiden voyage is uncertain so far. According to Gwynne Shotwell, SpaceX’s President and CEO, a number of companies have expressed interest in being on the first flight. Shotwell has also said that it might make more sense for SpaceX to completely own their first flight, without the pressure to keep a client happy. But a satellite payload for the first launch hasn’t been ruled out.

Delivering a payload into orbit is what the Falcon Heavy, and its competitors the Ariane5 and the ULA Delta-4 Heavy, are all about. Since one of the main competitive points of the Falcon Heavy is its ability to put larger payloads into geo-stationary orbits, accomplishing that feat on its first flight would be a great coming out party for the Falcon Heavy.

This artist's illustration of the Falcon Heavy shows the rocket in flight prior to releasing its two side boosters. Image: SpaceX — This artist’s illustration of the Falcon Heavy shows the rocket in flight prior to releasing its two side boosters. Image: SpaceX

SpaceX has promised that it will make its first Falcon Heavy launch useful. They say that they will use the flight either to demonstrate to its commercial customers the rocket’s capability to deliver a payload to GTO, or to demonstrate to national security interests its ability to meet their needs.

National security satellites require different capabilities from launch vehicles than do commercial communication satellites. Since these spacecraft are top secret, and are used to spy on communications, they need to be placed directly into their GTO, avoiding the lower-altitude transfer orbit of commercial satellites.

The payload for the first launch of the Falcon Heavy is not the only thing in question. There’s some question whether the November launch date can be achieved, since the Falcon Heavy has faced some delays in the past.

The inaugural flight for the big brother to the Falcon 9 was originally set for 2013, but several delays have kept bumping the date. One of the main reasons for this was the state of the Falcon 9. SpaceX was focussed on Falcon 9’s landing capabilities, and put increased manpower into that project, at the expense of the Falcon Heavy. But now that SpaceX has successfully landed the Falcon 9, the company seems poised to meet the November launch date for the Heavy.

One of the main attractions to the Falcon Heavy is its ability to deliver larger payloads to geostationary orbit (GEO). This is the orbit occupied by communications and weather satellites. These types of satellites, and the companies that build and operate them, are an important customer base for SpaceX. SpaceX claims that the Falcon Heavy will be able to place payloads of 22,200 kg (48,940 lbs) to GEO. This trumps the Delta-4 Heavy (14,200 kg/31,350 lbs) and the Ariane5 (max. 10,500 kg/23,100 lbs.)

There’s a catch to these numbers, though. The Falcon Heavy will be able to deliver larger payloads to GEO, but it’ll do it at the expense of reusability. In order to recover the two side-boosters and central core stage for reuse, some fuel has to be held in reserve. Carrying that fuel and using it for recovery, rather than burning it to boost larger payloads, will reduce the payload for GEO to about 8,000 kg (17,637 lbs.) That’s significantly less than the Ariane 5, and the upcoming Ariane 6, which will both compete for customers with the Falcon Heavy.

The Falcon Heavy is essentially four Falcon 9 rockets configured together to create a larger rocket. Three Falcon 9 first stage boosters are combined to generate three times as much thrust at lift-off as a single Falcon 9. Since each Falcon 9 is actually made of 9 separate engines, the Falcon Heavy will actually have 27 separate engines powering its first stage. The second stage is another single Falcon 9 second-stage rocket, consisting of a single Merlin engine, which can be fired multiple times to place payloads in orbit.

The three main boosters for the Falcon Heavy will all be built this summer, with construction of one already underway. Once complete, they will be transported from their construction facility in California to the testing facility in Texas. After that, they will be transported to Cape Canaveral.

Once at Cape Canaveral, the launch preparations will have all of the 27 engines in the first stage fired together in a hold-down firing, which will give SpaceX its first look at how all three main boosters operate together.

Eventually, if everything goes well, the Falcon Heavy will launch from Pad 39A at Cape Canaveral. Pad 39A is the site of the last Shuttle launches, and is now leased from NASA by SpaceX.

The Falcon Heavy will be the most powerful rocket around, once it’s operational. The versatility to deliver huge payloads to orbit, or to keep its costs down by recovering boosters, will make its first flight a huge achievement, whether or not it does deliver a satellite into orbit on its first launch.

May 6, 2016May 15, 2016 by Evan Gough

SpaceX Taps Superhero Designer For Its Spacesuits

Designer Jose Fernandez has been hired by SpaceX to design spacesuits. Fernandez has designed many superhero costumes, including the Bat Armor, pictured here in a collectible from Hot Toys. Image: Sideshow Collectibles

Everything about SpaceX seems exciting right now. In April, SpaceX successfully landed their reusable rocket, the Falcon 9, on a droneship at sea. Also in April, SpaceX announced that they intend to send a Dragon capsule to Mars by 2018. Now, Elon Musk’s private space company has hired Jose Fernandez, superhero movie costume designer, to design spacesuits for his astronauts.

Fernandez, with his company Ironhead Studio, has quite a resume when it comes to costume design. He’s designed superhero costumes for movies like Batman vs Superman: Dawn of Justice and Captain America: Civil War. He’s also designed costumes for X-Men movies, for Wonder Woman, Tron, and for The Penguin in Batman Returns.

Spacesuits have been slaves to function for a long time. The extreme environments in space have constrained their design to utilitarian forms, out of necessity. But now that Elon Musk has hired Fernandez, things could change. Considerably.

Jose Fernanzed heads Ironhead Studios, where he and his team create stunning super-hero costumes. Image: Jose Fernandez/Ironhead Studios

Whatever designs Fernandez comes up with, they will still have to have functionality as their primary concern. There’s no escaping that. But having someone with excellent visual design skills will certainly spice things up.

SpaceX had four other companies working on bids for this design work, but in the end it was Fernandez that won. This is no surprise given Fernandez’ long track record of making great costumes for superheroes. Over a twenty year span, he has also created costumes for Wolverine, Spiderman, The Fantastic Four, and Thor. That is an enviable collection of designs.

It will be super interesting to see what Fernandez comes up with, and how design will meld with engineering requirements to create a safe, effective spacesuit. After all, the people wearing them won’t be actors, and they will require the absolute best performance possible.

Purists may scoff at having someone from Hollywood involved in spacesuit design. After all, this is serious business. The surface of Mars is not a movie set, it’s a dangerous, alien world. But there’s no telling what Fernandez will come up with. If his success in movie costumes is any indication, he might convert any nay-sayers into supporters.

The ESA and NASA are also working on new spacesuit designs. The video below is a good discussion of spacesuit design. Compare the blocky, clunky look of the first spacesuits to what astronauts now use.

May 4, 2016May 15, 2016 by Evan Gough

Is A New Particle About To Be Announced?

New data from two experiments at the LHC has shown that, contrary to previous indications, they have not discovered a new subatomic particle. Credit: CERN/LHC

Particle physicists are an inquisitive bunch. Their goal is a working, complete model of the particles and forces that make up the Universe, and they pursue that goal with a vigour matched by few other professions.

The Standard Model of Physics is the result of their efforts, and for 25 years or so, it has guided our thinking and understanding of particle physics. The best tool we have for studying physics further is the Large Hadron Collider (LHC), near Geneva, Switzerland. And some recent, intriguing results from the LHC points to the existence of a newly discovered particle.

The Large Hadron Collider is the most powerful particle accelerator in the world. Image: CERN

The LHC has four separate detectors. Two of them are “general purpose” detectors, called ATLAS and CMS. Last year, separate experiments in both the ATLAS and CMS detectors produced what is best called a “bump” in their data. Initially, the two teams conducting the experiments were puzzled by the data. But when they compared them, they found that the bumps in their data were the same in both experiments, and they hinted at what could be a new type of particle, never before detected.

The two experiments involved smashing protons into each other at near-relativistic speeds. The collisions produced more high-energy photons than theory predicts. Not a lot more, but physics is a detailed endeavour, so even a slight increase in the amount of photons produced is a big deal. In physics, everything happens for a reason.

To be more specific, ATLAS and CMS recorded increased activity at an energy level around 750 giga electron-volts (GeV). What that means, for all you non-particle physicists, is that the new particle decays into two photons at the point of the proton-proton collision. If the new particle exists, that is.

A new particle would be a huge discovery. The Standard Model has describe all the particles present in nature pretty well. It even predicted the existence of one type of particle, the Higgs Boson, long before the LHC actually verified its existence. The discovery of a new type of particle would be very exciting news indeed, and could break the Standard Model.

Since this data from the experiments at the LHC was released last year, the physics world has been buzzing. Over 100 papers have been written to try to explain what the results might mean. But some caution is required.

The first thing scientists do when faced with results like this is to try to quantify the likelihood that it could be chance. If only one experiment had this bump in its data, then the likelihood that it was just a chance occurrence is pretty high. There are many reasons why an experiment can have a result like this, which is why repeatability is such a big deal in science. But when two independent, separate, experiments have the same result, people’s ears perk up.

A few months have passed since the experiments were run, and in that time, the experimenters have tried to determine exactly what the likelihood is of these result occurring by chance. After working with the data, a funny thing has happened. The significance of the extra photons detected by CMS has risen, while the significance of the extra photons detected by ATLAS has fallen. This has definitely left physicists scratching their heads.

Also in that time, about four main explanations for the experimental results have percolated to the surface. One states that the new particle, if it exists, is made up of smaller particles, similar to how a proton is made up of quarks. These smaller particles could be held together by an unknown force. Some theoretical physicists think this is the best fit with the data.

Another possibility is that the new particle is a heavier version of the Higgs Boson. About 12 times heavier. Or it could be that the Higgs Boson itself is made up of smaller particles, and that’s what the experiment detected.

The Standard Model of Elementary Particles. Image: By MissMJ - Own work by uploader, PBS NOVA [1], Fermilab, Office of Science, United States Department of Energy, Particle Data Group, CC BY 3.0 — The Standard Model of Elementary Particles. Image: By MissMJ – Own work by uploader, PBS NOVA [1], Fermilab, Office of Science, United States Department of Energy, Particle Data Group, CC BY 3.0

Or, it could be the much-hypothesized graviton, the theoretical particle that carries the gravitational force. The four fundamental forces in the Universe are electromagnetism, the strong nuclear force, the weak nuclear force, and gravity. So far, we have discovered the particles that transmit all of those forces, except for gravity. If their was a new particle detected, and if it proved to be the graviton, that would be enormous, earth-shattering news. At least for those who are passionate about understanding nature.

That’s a lot of “ifs” though.

There are a lot of holes in our knowledge of the Universe, and physicists are eager to fill those gaps. The discovery of a new particle might very well answer some basic questions about dark matter, dark energy, or even gravity itself. But there’s a lot more experimentation to be done before the existence of a new particle can be announced.

May 3, 2016May 15, 2016 by Evan Gough

Boiling Water Is Carving Martian Slopes

These dark streaks, called recurring slope lineae, are on a sloped wall on a crater on Mars. A new study says they may have been formed by boiling water. Image: NASA/JPL-Caltech/Univ. of Arizona — These dark streaks, called recurring slope lineae (RSL), are on the sloped wall of a crater on Mars. A new study says they may have been formed by boiling water. Credit: NASA/JPL-Caltech/Univ. of Arizona

Finding water on Mars is a primary focus of human efforts to understand the Red Planet. The presence of liquid water on Mars supports the theory that life existed there. Now it looks as though some puzzling features on the surface of Mars could have been caused by boiling water.

Recurring slope lineae (RSL) are dark streaks found on slopes on the surface of Mars. It was thought that these streaks could have been caused by seasonal melting. Other proposed causes were dust avalanches or the venting of carbon dioxide gas. Since the same features are also found on the Moon, they could also be caused by tiny meteorites that cause avalanches. But now a study from researchers at the Open University of England shows that boiling water could have created the patterns.

We don’t have to go looking for thermal vents to find the source of this boiling water. The atmospheric pressure on Mars is so low that any liquid water would boil, without the need for a heat source. At about 1/100th the atmospheric pressure of Earth, Martian water will boil easily.

You don’t have to travel to Mars, or build an atmospheric pressure simulator, to observe the fact that water boils more readily under lower atmospheric pressure. You can see it happen here on Earth. As hikers and mountaineers know from experience, water boils more quickly the higher you go in the mountains. The greater your altitude, the less atmosphere there is pushing down on you, which lowers the boiling point of water. On Mars, that effect is extreme.

The team of researchers, led by M. Masse, performed their experiments in a chamber that can recreate the atmospheric pressure on Mars. Inside the chamber, they built a slope of loose, fine-grained material, and placed a block of ice on it. At first, the team kept the pressure inside the chamber identical to Earth’s atmospheric pressure, and the melting ice had little effect on the slope of loose material.

The 'Martian Chamber' used to re-create the atmospheric pressure on Mars. Image: M. Masse — The ‘Martian Chamber’ used to re-create the atmospheric pressure on Mars. Image: M. Masse

But when they reduced the atmosphere inside the chamber to that of Mars, the water boiled quickly, creating a much more pronounced effect. This vigorous boiling action caused sand grains to fly into the air, creating heaps. As these heaps collapsed, avalanches were triggered. The end result was the same kind of flow patterns observed on Mars.

Numerous other studies have found evidence of liquid water on Mars, and features like the RSL appear to have been caused by water. But though this study seems to add to that growing evidence, it also puts the brakes on the idea that liquid water is present on Mars.

For these RSL to occur on Earth requires a certain amount of water. But because of the ‘boiling water effect’ of the lower pressure atmosphere on Mars, much less water is required to create them. Not only that, but the fact that water boils away so quickly means that any liquid water is short-lived, and would not provide an adequate environment for micro-organisms.

Experimental results from the new study show the effect that the atmospheres of Earth and Mars have on flowing water. Image: M. Masse

Also, the effect that Mars’ lower gravity has on the formation of RSLs is not well understood, and may be another part of the equation. The researchers’ ‘Martian Chamber’ was not built to mimic Mars’ gravity.

These are interesting preliminary results, flawed only by the lack of simulated Martian gravity. For these results to be conclusive, the same process would have to be observed on Mars itself. And that’s not happening anytime soon.

April 29, 2016May 15, 2016 by Evan Gough

Fermi Links Neutrino Blast To Known Extragalactic Blazar

This image shows the galaxy PKS B1424-418, and the blazar that lives there. The dotted circle is the area in which Fermi detected the neutrino Big Bird. Image: NASA/DOE/LAT Collaboration.

A unique observatory buried deep in the clear ice of the South Pole region, an orbiting observatory that monitors gamma rays, a powerful outburst from a black hole 10 billion light years away, and a super-energetic neutrino named Big Bird. These are the cast of characters that populate a paper published in Nature Physics, on Monday April 18th.

The observatory that resides deep in the cold dark of the Antarctic ice has one job: to detect neutrinos. Neutrinos are strange, standoffish particles, sometimes called ‘ghost particles’ because they’re so difficult to detect. They’re like the noble gases of the particle world. Though neutrinos vastly outnumber all other atoms in our Universe, they rarely interact with other particles, and they have no electrical charge. This allows them to pass through normal matter almost unimpeded. To even detect them, you need a dark, undisturbed place, isolated from cosmic rays and background radiation.

This explains why they built an observatory in solid ice. This observatory, called the IceCube Neutrino Observatory, is the ideal place to detect neutrinos. On the rare occasion when a neutrino does interact with the ice surrounding the observatory, a charged particle is created. This particle can be either an electron, muon, or tau. If these charged particles are of sufficiently high energy, then the strings of detectors that make up IceCube can detect it. Once this data is analyzed, the source of the neutrinos can be known.

The next actor in this scenario is NASA’s Fermi Gamma-Ray Space Telescope. Fermi was launched in 2008, with a specific job in mind. Its job is to look at some of the exceptional phenomena in our Universe that generate extraordinarily large amounts of energy, like super-massive black holes, exploding stars, jets of hot gas moving at relativistic speeds, and merging neutron stars. These things generate enormous amounts of gamma-ray energy, the part of the electromagnetic spectrum that Fermi looks at exclusively.

Next comes PKS B1424-418, a distant galaxy with a black hole at its center. About 10 billion years ago, this black hole produced a powerful outburst of energy, called a blazar because it’s pointed at Earth. The light from this outburst started arriving at Earth in 2012. For a year, the blazar in PKS B1424-418 shone 15-30 times brighter in the gamma spectrum than it did before the burst.

Detecting neutrinos is a rare occurrence. So far, IceCube has detected about a hundred of them. For some reason, the most energetic of these neutrinos are named after characters on the popular children’s show called Sesame Street. In December 2012, IceCube detected an exceptionally energetic neutrino, and named it Big Bird. Big Bird had an energy level greater than 2 quadrillion electron volts. That’s an enormous amount of energy shoved into a particle that is thought to have less than one millionth the mass of an electron.

The IceCube Neutrino Observatory is a series of strings of detectors, drilled deep into the Antarctic ice. Image: Nasa-verve - IceCube Science Team - Francis Halzen, Department of Physics, University of Wisconsin, CC BY 3.0, https://commons.wikimedia.org/w/index.php?curid=26350372 — The IceCube Neutrino Observatory is a series of strings of detectors, drilled deep into the Antarctic ice. Image: Nasa-verve – IceCube Science Team – Francis Halzen, Department of Physics, University of Wisconsin, CC BY 3.0, https://commons.wikimedia.org/w/index.php?curid=26350372

Big Bird was clearly a big deal, and scientists wanted to know its source. IceCube was able to narrow the source down, but not pinpoint it. Its source was determined to be a 32 degree wide patch of the southern sky. Though helpful, that patch is still the size of 64 full Moons. Still, it was intriguing, because in that patch of sky was PKS B1424-418, the source of the blazar energy detected by Fermi. However, there are also other blazars in that section of the sky.

The scientists looking for Big Bird’s source needed more data. They got it from TANAMI, an observing program that used the combined power of several networked terrestrial telescopes to create a virtual telescope 9,650 km(6,000 miles) across. TANAMI is a long-term program monitoring 100 active galaxies that are located in the southern sky. Since TANAMI is watching other active galaxies, and the energetic jets coming from them, it was able to exclude them as the source for Big Bird.

The team behind this new paper, including lead author Matthias Kadler of the University of Wuerzberg in Germany, think they’ve found the source for Big Bird. They say, with only a 5 percent chance of being wrong, that PKS B1424-418 is indeed Big Bird’s source. As they say in their paper, “The outburst of PKS B1424–418 provides an energy output high enough to explain the observed petaelectronvolt event (Big Bird), suggestive of a direct physical association.”

So what does this mean? It means that we can pinpoint the source of a neutrino. And that’s good for science. Neutrinos are notoriously difficult to detect, and they’re not that well understood. The new detection method, involving the Fermi Telescope in conjunction with the TANAMI array, will not only be able to locate the source of super-energetic neutrinos, but now the detection of a neutrino by IceCube will generate a real-time alert when the source of the neutrino can be narrowed down to an area about the size of the full Moon.

This promises to open a whole new window on neutrinos, the plentiful yet elusive ‘ghost particles’ that populate the Universe.

April 29, 2016 by Evan Gough

The New Vostochny Cosmodrome Brings Launches Back To Russian Soil

The successful launch of a Soyuz 2.1a rocket from the Vostochny Cosmodrome on April 27th was the first launch from Russia's new spaceport. Image: Roscosmos

Russia’s new Vostochny Cosmodrome launched its first rocket on Wednesday, April 27th, carrying three new satellites into orbit. After an initial 24-hour launch delay due to a computer-initiated abort, a Soyuz-2.1a lifted off from its pad at 10:01 am EDT. Every successful space launch is important in its own way, but this one even more so because of the importance of this new cosmodrome to Russia.

The breakup of the Soviet Union in 1991 threw that country into chaos. The formal dissolution of the USSR on December 26th, 1991, created a lot of financial and political turmoil. The Soviet space program was a victim of that chaos, and with the USSR’s main cosmodrome now located on foreign territory, at Baikonur, Kazakhstan, things were uncertain.

Roscosmos, the Russian space agency, has been renting the Baikonur cosmodrome for $115 million annually. But this dependence on a foreign launch site has been a thorn in the side of Russia for decades. Russia is a fiercely independent and proud nation, so it surprised no one when construction of a new spaceport was announced. In 2010, Vladimir Putin emphasized the importance of the new facility, saying “The creation of a new space center … is one of modern Russia’s biggest and most ambitious projects.”

The new facility, called the Vostochny Cosmodrome, will eventually be home to multiple launch pads, though only one is functional for now. It’s located at 51 degrees north, whereas the Baikonur site is located at 46 degrees North. Though further north, it will still be able to launch almost the same payloads as Baikonur.

Russia has other spaceports on its own territory. The Svobodny Cosmodrome is also located in Russia’s far east, and at the same 51 degrees north as Vostochny. But Svobodny was originally an ICBM launch site, and couldn’t handle the launching of crewed missions. All crewed missions had to be launched from Baikonur. Russia has another cosmodrome, the Plesetsk Cosmodrome, where satellites can be launched into geostationary orbit.

The site for the new Vostochny Cosmodrome (Vostochny means ‘eastern’ in Russian) was chosen for a few reasons. The site is serviced by both highway and rail, and is remote enough that launch paths won’t interfere with any built up areas. It’s also located several hundred kilometres from the Pacific Ocean, to avoid complications that proximity to an ocean can cause, yet close enough that spent stages can be jettisoned and will fall harmlessly into the ocean.

The Vostochny Cosmodrome is located in Russia's far east. Image: Wikimedia Commons, CC by SA 3.0 — The Vostochny Cosmodrome is located in Russia’s far east. Image: Wikimedia Commons, CC by SA 3.0

Vostochny is about the same size as the Kennedy Space Centre in Cape Canaveral. Vostochny covers 551.5 square kilometers, while the Kennedy facility covers 583 square kilometers. The new cosmodrome will eventually house over 400 separate facilities, including engineering and transport infrastructure.

The Vostochny Cosmodrome project has suffered some setbacks. Parts of the assembly complex for the Soyuz 2 rocket were built too small, which delayed the planned initial launch set for December 2015. There’ve been accusations of corruption, and even a worker’s strike in the Spring of 2015 over unpaid wages.

These and other problems led Valdimir Putin to release a statement saying he was taking personal control of the project. Since then, Putin has kept a close eye on the Vostochny project. In response to the recent 24 hour launch delay of the cosmodrome’s inaugural launch, Putin criticized Roscosmos for the delay, and for all of the glitches and failures in the Russian space program recently.

But, ever the politician, Putin also tempered his remarks, saying “Despite all its failings, Russia remains the world leader in the number of space launches.” “But the fact that we’re encountering a large number of failures is bad. There must be a timely and professional reaction,” he added.

Russian President Vladimir Putin has taken a personal interest in the Vostochny Cosmodrome. In October 2015 he visited the site. Image: Roscosmos/Kremlin CC BY 4.0

As for Vostochny itself, it will allow Russia to conduct much more of its space launches on its own soil. By 2020, Vostochny will conduct 45% of Russia’s space launches. Baikonur will still be used, but much more sparingly. It currently is responsible for 65% of Russian launches, but that will drop to 11%. The Plesetsk Cosmodrome will account for the other 44%.

As for the inaugural launch, it went flawlessly after its initial 24 hour technical delay. The three satellites it carried into orbit will fulfill several different functions. Together, they will study the Earth’s upper atmosphere, observe gamma-ray bursts, and test new electronics modules for use in space. They will also carry high-resolution cameras for remote sensing and scientific work, test communication systems with ground stations, and will develop control algorithms for use with nano-satellites.

April 28, 2016May 5, 2016 by Evan Gough

James Webb Space Telescope Takes The Gloves Off

Behold, the mighty primary mirror of the James Webb Space Telescope, in all its gleaming glory! Image: NASA/Chris Gunn — The primary mirror of the James Webb Space Telescope, in all its gleaming glory! Image: NASA/Chris Gunn

The James Webb Space Telescope (JWST) isn’t even operational yet, and already its gleaming golden mirror has reached iconic status. It’s segmented mirror is reminiscent of an insect eye, and once that eye is unfolded at its eventual stationary location at L2, the JWST will give humanity its best view of the Universe yet. Now, NASA has unveiled the JWST’s mirrors in a clean room at the Goddard Space Flight Centre, giving us a great look at what the telescope will look like when it’s operational.

Even if you didn’t know anything about the JWST, its capabilities, or its torturous path to finally being built, you would still look at it and be impressed. It’s obviously a highly technological, highly engineered, one of a kind object. In fact, you could be forgiven for mistaking it for a piece of modern art. (I’ve seen less appealing modern art, have you?)

The fact that the JWST will outperform its predecessor, the Hubble, is a well-known fact. After all, the Hubble is pretty long in the tooth now. But how exactly it will outperform the Hubble, and what the JWST’s mission objectives are, is less well-known. It’s worth it to take a look at the objectives of the JWST, again, and re-visit the enthusiasm that has surrounded this mission since its inception.

The James Webb Space Telescope in the clean room at the Goddard Space Flight Center. Image: NASA/Chris Gunn

NASA groups JWST’s science objectives into four areas:

infrared vision that acts like a time-machine, giving us a look at the first stars and galaxies to form in the Universe, over 13 billion years ago.
a comparative study of the stately spiral and elliptical galaxies of our age with the faintest, earliest galaxies to form in the Universe.
a probing gaze through clouds of dust, to watch stars and planets being born.
a look at extrasolar planets, and their atmospheres, keeping an eye out for biomarkers.

That is an impressive list, even in an age where people take technological and scientific progress for granted. But alongside these noble objectives, there will no doubt be some surprises. Guessing what those surprises might be is a bit of a fool’s errand, but this is the internet, so let’s dare to be foolish.

We have an idea that abiogenesis on Earth happened fairly quickly, but we have nothing to compare it to. Will we learn enough about exoplanets and their atmospheres to shed some light on conditions needed for life to happen? It’s a stretch, but who knows?

We have an understanding of the expansion of the Universe, and it’s backed up by pretty solid evidence. Will we learn something surprising about this? Or something that sheds some light on Dark Matter and Dark Energy, and their role in the early Universe?

Or will there be surprising findings in the area of planetary and stellar formation? The capability to look deeply into dust clouds should certainly reveal things previously unseen, but only guessed at.

Of course, not everything needs to be surprising to be exciting. Evidence that supports and fine tunes current theories is also intriguing. And the James Webb should deliver a boatload of evidence.

There’s no question that the JWST will outdo the Hubble in the science department. But for a generation or two of people, the Hubble will always have a special place. It drew many of us in, with its breathtaking pictures of nebulae and other objects, its famous Deep Field study, and, of course, its science. It was probably the first telescope to gain celebrity status.

The James Webb will probably never gain the social status that the Hubble gained. It’s kind of like the Beatles, there can only be one ‘first of its kind.’ But the JWST will be much more powerful, and will reveal to us a lot that has been hidden.

The JWST will be a grand technological accomplishment, if all goes well and it makes it to L2 and is fully functional. Its ability to look deeply into dust clouds, and to look back in time, to the early days of the Universe, make it a potent scientific tool.

And if engineering can figure out a way to reverse the polarity in the warp core without it going crit, we should be able to fire a beam of tachyon anti-matter neutrinos and de-cloak a Romulan Warbird at a distance of 3 AUs. Not bad for something Congress threatened to cancel!

April 27, 2016May 5, 2016 by Evan Gough

New Highest Resolution Images Of Long-Lost Beagle 2 Lander

On the left are original photos from NASA's Mars Reconnaissance Orbiter. On the right are sharper photos of the same, created by stacking matching photos on top of one another. Image: NASA/JPL-Caltech/Univ. of Arizona/Yu Tao et al/University College London.

We like to focus on successful space missions and celebrate what those successes add to our knowledge. But, obviously, not all missions are completely successful. And since some missions are at such huge distances from Earth, their fate can remain a mystery.

This was true of the Beagle 2 Lander, until recently.

The Beagle 2 was a UK contribution to the ESA’s Mars Express mission, launched in 2003. Mars Express consisted of two components; the Mars Express Orbiter and the Beagle 2 Lander. The mission arrived at Mars in December 2003, when the Beagle 2 separated from the orbiter and landed on the Martian surface.

Beagle 2’s destination was Isidis Planitia, a vast sedimentary basin. Beagle 2 was supposed to operate for 180 days, with a possible extension up to one Martian year. But the ESA was unable to contact the lander after several attempts, and in February 2004, the ESA declared the mission lost.

The Beagle 2, named after the ship that Darwin took on his famous voyage, had some solid science goals in mind. It was going to study the geology, mineralogy, and the geochemistry of the landing site, and also the physical properties of the atmosphere and Mars’ surface. It was also going to study the Martian meteorology and climate, and search for biosignatures. But all that was lost.

There was lots of conjecture, but the Beagle 2’s fate was a mystery.

Now, thanks to a new method of ‘stacking and matching’ photos of the Martian surface, which results in higher resolution images than previously possible, the likely fate of the Beagle 2 is known. It appears that the spacecraft landed softly as planned, but that solar panels failed to deploy properly. This not only starved the lander of electrical power, but blocked the craft’s antenna from functioning. This is why no signal was ever received from Beagle 2.

This is a zoomed in image of the Beagle 2 on Mars, with a to-scale sketch of the Beagle 2 super-imposed beside it. Credit: NASA/JPL-Caltech/Univ. of Arizona/Yu Tao et al/University College London/University of Leicester

It took quite a bit of sleuthing to find the Beagle 2. The MRO has used its High Resolution Imaging Science Experiment (HiRise) camera to search for other craft on the surface of Mars, but the Beagle 2 was harder to find. It never sent even a brief signal after touchdown, which would have made it much easier to locate.

Adding to the difficulty is the huge landing area the Beagle 2 had. Beagle 2’s landing site at the time of its launch was an ellipse 170 km by 100 km in the Isidis Planitia. That’s an enormous area in which to locate a spacecraft that’s less than a few meters across once deployed, with a camera that has an image scale of about 0.2m, (10 inches).

The MRO has been using its HiRise to look for Beagle 2 since it was lost. As it went about the business of its science objectives, it captured occasional images of the Beagle 2’s landing site. Eventually, the lander was identified by Michael Croon, a former member of the ESA’s Mars Express Orbiter team. In HiRise images from February 2013 and June 2014, Croon found visual evidence of the lander and its entry and descent components.

The puzzling thing was that the image seemed to shift around in different photos. This could be because the lander deployed its solar panels like flower petals arranged around the center. The panels will reflect light differently in different lighting conditions, which could make the lander appear to change location in subsequent photos. If Beagle 2 is sitting on an uneven surface, that could add to the illusion.

The HiRise images are consistent with the idea that the panels failed to deploy, and that also makes sense if the panels blocked the antenna from operating. It’s also possible that the sun glinting off the panels only makes it appear that not all of them opened.

A replica of the Beagle 2 lander at the London Science Museum. Image: By user:geni - Photo by user:geni, GFDL, https://commons.wikimedia.org/w/index.php?curid=5258554 — A replica of the Beagle 2 lander at the London Science Museum. Image: By user:geni – Photo by user:geni, GFDL, https://commons.wikimedia.org/w/index.php?curid=5258554

But what’s bad news for Beagle 2 is good news for the human endeavour to study Mars. The new technique of combining images of the surface of Mars yields photos with 5 times the resolution that MRO can provide. This will make selecting landing sites for future missions much easier, and will also contribute to the science objectives of the MRO itself.

These two images show the power of the new high-resolution imaging technique. The top shows two original images, on the left a rock field, and on the right, an area containing tracks left by the Spirit rover. Image: Credit: NASA/JPL-Caltech/Univ. of Arizona/Yu Tao et al/University College London

The Mars Express Orbiter is still in operation above Mars, and has been for over 12 years. Among its achievements are the detection of water ice in Mars’ South Polar cap and the discovery of methane in the atmosphere of Mars. The orbiter also performed the closest-ever flyby of Mars’ moon Phobos.