Comet Siding Spring Was Bleeding Hydrogen As It Sped By Mars

Comet Siding Spring shines in ultraviolet in this image obtained by the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft. Credit: Laboratory for Atmospheric and Space Physics/University of Colorado; NASA

As Comet Siding Spring passed close by Mars on Sunday (Oct. 19), NASA’s newest Mars spacecraft took a time-out from its commissioning to grab some ultraviolet pictures of its coma. What you see above is hydrogen, a whole lot of it, leaving the comet in this picture taken from 5.3 million miles (8.5 million kilometers).

The hydrogen is a product of the water ice on the comet that the Sun is slowly melting and breaking apart into hydrogen and oxygen molecules. Because hydrogen scatters ultraviolet light from the Sun, it shows up rather clearly in this picture taken by the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft.

Check out more recent pictures of Siding Spring below.

Is this an image of Comet Siding Spring? It's the only fuzzy object in the field photographed on Sol 3817 (October 19) by the Opportunity Rover. Click for original raw image.
Is this an image of Comet Siding Spring? It’s the only fuzzy object in the field photographed on Sol 3817 (October 19) by the Opportunity Rover. Click for original raw image.
Comet Siding Spring near Mars in a composite image by the Hubble Space Telescope, capturing their positions between Oct. 18 8:06 a.m. EDT (12:06 p.m. UTC) and Oct. 19 11:17 p.m. EDT (Oct. 20, 3:17 a.m. UTC). Credit: NASA, ESA, PSI, JHU/APL, STScI/AURA
Comet Siding Spring near Mars in a composite image by the Hubble Space Telescope, capturing their positions between Oct. 18 8:06 a.m. EDT (12:06 p.m. UTC) and Oct. 19 11:17 p.m. EDT (Oct. 20, 3:17 a.m. UTC). Credit: NASA, ESA, PSI, JHU/APL, STScI/AURA
Another photo, just in, taken of the comet and Mars today (Oct. 19) by Rolando Ligustri. Beautiful!
Another photo, just in, taken of the comet and Mars today (Oct. 19) by Rolando Ligustri. Beautiful!
Comet 2013 A1 Siding Spring on October 17, 2014, with two days to go until its Martian encounter. Very dense Milkyway starfield in the background with many darker obscured regions. Credit and copyright: Damian Peach.
Comet 2013 A1 Siding Spring on October 17, 2014, with two days to go until its Martian encounter. Very dense Milkyway starfield in the background with many darker obscured regions. Credit and copyright: Damian Peach.

Stinky! Rosetta’s Comet Smells Like Rotten Eggs And Ammonia

A view of Comet 67P/Churyumov-Gerasimenko on Sept. 26, 2014 from the orbiting Rosetta spacecraft. Credit: ESA/Rosetta/NAVCAM

While you can’t smell in space — there is no medium to carry the molecules, the same reason you can’t hear things — you can certainly detect what molecules are emanating from comets and other solar system bodies. A new analysis of Comet 67P/Churyumov-Gerasimenko by the orbiting Rosetta spacecraft thus found a rather pungent chemistry combination.

The spacecraft detected hydrogen sulphide (the smell of rotten eggs), ammonia and formaldehyde with traces of hydrogen cyanide and methanol. But compared to the amounts of water and carbon monixide 67P has, these molecule concentrations are quite miniscule.

“This all makes a scientifically enormously interesting mixture in order to study the origin of our solar system material, the formation of our Earth and the origin of life,” stated the University of Bern’s Kathrin Altwegg, from the center of space and habitability.

“And after all: it seems like comet Churyumov was indeed attracted by comet Gerasimenko to form Churyumov-Gerasimenko, even though its perfume may not be Chanel No 5, but comets clearly have their own preferences.”

More seriously, astronomers do say that at three astronomical units (Earth-Sun distances) from the Sun, the comet is emitting more molecules than expected. The next step will be to compare Rosetta’s data with ground-based data of other comets to see if this is common.

Source: University of Bern

Videos: From Space, Lightning Looks Like Creepy White Blobs

Lightning over Equatorial Africa
Lightning over Equatorial Africa

Standing on the ground, we’re used to seeing the bolts and flashes of lightning during epic thunderstorms. But how would it look like from space? These three Vine videos from orbiting NASA astronaut Reid Wiseman provide a glimpse.

As you can see in these videos he uploaded to his Twitter account a few days ago, flashes and pools of light appear in this lightning storm over Kansas that he spotted from the International Space Station. Check out more below the jump. Continue reading “Videos: From Space, Lightning Looks Like Creepy White Blobs”

Rosetta’s Comet Springs Spectacular Leaks As It Gets Closer To The Sun

This Rosetta image of Comet 67P/Churyumov-Gerasimenko shows spectacular jets erupting from the small body on Sept. 10, 2014. Credit: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

Jet! The comet that the Rosetta spacecraft is visiting is shedding more dust as machine and Solar System body get closer to the Sun.

While activity was first seen at the “neck” of the rubber-duckie shaped comet a few weeks ago, now scientists are seeing jets spring from across the comet.

This is just one signal of cometary activity picking up as 67P gets closer to the Sun. For the moment, it appears the prime landing site is still safe enough for Philae to land on Nov. 19, officials said, while noting there is a jet about a kilometer away that the lander can study when it gets there.

Jets spring from the "neck" area of Comet 67P/Churyumov-Gerasimenko. The smaller lobe is on the left, and the larger on the right. These images were taken about 7.2 kilometers (4.5 miles) from the surface. Credit: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA
Jets spring from the “neck” area of Comet 67P/Churyumov-Gerasimenko. The smaller lobe is on the left, and the larger on the right. These images were taken about 7.2 kilometers (4.5 miles) from the surface. Credit: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

“At this point, we believe that a large fraction of the illuminated comet’s surface is displaying some level of activity,” stated Jean-Baptiste Vincent a scientist from the Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) that took the pictures. He is with the Max Planck Institute for Solar System Research in Germany.

The comet is about 470 million kilometers (292 miles) from the Sun and will make its closest approach in 2015. Rosetta is the first mission to orbit a comet as it gets close to the Sun, and Philae (if successful) will make the first “soft” landing on a cometary surface.

Source: European Space Agency

The Physics Behind “Interstellar’s” Visual Effects Was So Good, it Led to a Scientific Discovery

Kip Thorne’s concept for a black hole in 'Interstellar.' Image Credit: Paramount Pictures

While he was working on the film Interstellar, executive producer Kip Thorne was tasked with creating the black hole that would be central to the plot. As a theoretical physicist, he also wanted to create something that was truly realistic and as close to the real thing as movie-goers would ever see.

On the other hand, Christopher Nolan – the film’s director – wanted to create something that would be a visually-mesmerizing experience. As you can see from the image above, they certainly succeeded as far as the aesthetics were concerned. But even more impressive was how the creation of this fictitious black hole led to an actual scientific discovery.

Continue reading “The Physics Behind “Interstellar’s” Visual Effects Was So Good, it Led to a Scientific Discovery”

Assembly Complete for NASA’s Maiden Orion Spacecraft Launching in December 2014

Technicians complete final assembly of NASA’s first Orion spacecraft with installation of the close out panels on the Launch Abort System that smooth airflow. Credit: Photo credit: Kim Shiflett

Technicians at the Kennedy Space Center have completed the final major assembly work on NASA’s maiden Orion crew module slated to launch on its first unmanned orbital test flight this December, dubbed Exploration Flight Test-1 (EFT-1)

After first attaching the Launch Abort System (LAS) to the top of the capsule, engineers carefully installed a fairing composed of a set of four ogive panels over the crew module and the abort systems lower structural framework joining them together.

“The ogive panels smooth the airflow over the conical spacecraft to limit sound and vibration, which will make for a much smoother ride for the astronauts who will ride inside Orion in the future,” according to a NASA description.

Upon finishing the panel assembly work inside the Launch Abort System Facility (LASF) at NASA’s Kennedy Space Center, the teams cleared the last major hurdle before the Orion stack is rolled out to launch pad 37 in mid-November and hoisted to the top of the Delta IV Heavy rocket.

Technicians complete final assembly of NASA’s first Orion spacecraft with installation of the  last ogive close out panels on the Launch Abort System that smooth airflow. Credit: Photo credit: Kim Shiflett
Technicians complete final assembly of NASA’s first Orion spacecraft with installation of the last ogive close out panels on the Launch Abort System that smooth airflow. Photo credit: Kim Shiflett

The Orion stack is comprised of the LAS, crew module (CM) and service module (SM).

The maiden blastoff of the state-of-the-art Orion spacecraft on the EFT-1 mission is slated for December 4, 2014, from Space Launch Complex 37 (SLC-37) at Cape Canaveral Air Force Station in Florida atop the triple barreled United Launch Alliance (ULA) Delta IV Heavy booster.

Orion is NASA’s next generation human rated vehicle that will eventually carry America’s astronauts beyond Earth on voyages venturing farther into deep space than ever before – beyond the Moon to Asteroids, Mars, and other destinations in our Solar System.

NASA’s completed Orion EFT 1 crew module loaded on wheeled transporter during move to the Payload Hazardous Servicing Facility (PHFS) on Sept. 11, 2014 at the Kennedy Space Center, FL.  Credit: Ken Kremer - kenkremer.com
NASA’s completed Orion EFT 1 crew module loaded on wheeled transporter during move to the Payload Hazardous Servicing Facility (PHSF) on Sept. 11, 2014, at the Kennedy Space Center, FL. Credit: Ken Kremer – kenkremer.com

The two-orbit, four and a half hour EFT-1 flight around Earth will lift the Orion spacecraft and its attached second stage to an orbital altitude of 3,600 miles, about 15 times higher than the International Space Station (ISS) – and farther than any human spacecraft has journeyed in 40 years. It will test the avionics and electronic systems inside the Orion spacecraft.

Then the spacecraft will travel back through the atmosphere at speeds approaching 20,000 mph and temperatures near 4,000 degrees Fahrenheit to test the heat shield, before splashing down for a parachute assisted landing in the Pacific Ocean.

Launch Abort System (LAS) for Orion EFT-1 on view horizontally inside the Launch Abort System Facility at the Kennedy Space Center, Florida, prior to installation atop the crew module. Credit: Ken Kremer/kenkremer.com
Launch Abort System (LAS) for Orion EFT-1 on view horizontally inside the Launch Abort System Facility at the Kennedy Space Center, Florida, prior to installation atop the crew module. Credit: Ken Kremer/kenkremer.com

The LAS plays a critically important role to ensure crew safety.

In case of an emergency situation, the LAS is designed to ignite within milliseconds to rapidly propel the astronauts inside the crew module away from the rocket and save the astronauts’ lives. The quartet of LAS abort motors would generate some 500,000 pounds of thrust to pull the capsule away from the rocket.

And don’t forget that you can fly your name on Orion and also print out an elegant looking “boarding pass.”

Details below and in my article – here.

NASA announced that the public can submit their names for inclusion on a dime-sized microchip that will travel on Orion and succeeding spacecraft voyaging to destinations beyond low-Earth orbit, including Mars.

The deadline to submit your name is soon: Oct 31, 2014.

Click on this weblink posted online by NASA today: http://go.usa.gov/vcpz

NASA invites you to send your name to Mars via the first Orion test flight in December 2014.  Deadline for submissions is Oct 31, 2014. Join over 170,000 others! See link below. Credit: NASA
NASA invites you to send your name to Mars via the first Orion test flight in December 2014. Deadline for submissions is Oct 31, 2014. Join over 170,000 others! See link below. Credit: NASA

“NASA is pushing the boundaries of exploration and working hard to send people to Mars in the future,” said Mark Geyer, Orion Program manager, in a NASA statement.

“When we set foot on the Red Planet, we’ll be exploring for all of humanity. Flying these names will enable people to be part of our journey.”

NASA’s Orion Program manager Mark Geyer discusses Orion EFT-1 mission.  Credit: Ken Kremer - kenkremer.com
NASA’s Orion Program manager Mark Geyer discusses Orion EFT-1 mission, while holding a model of the Launch Abort System. Credit: Ken Kremer – kenkremer.com

Stay tuned here for Ken’s continuing Orion and Earth and planetary science and human spaceflight news.

Ken Kremer

The United Launch Alliance Delta-IV Heavy rocket tasked with launching NASA’s Orion EFT-1 mission being hoisted vertical atop Space Launch Complex-37B at Cape Canaveral Air Force Station in Florida on the morning of Oct. 1, 2014. Photo Credit: Alan Walters / AmericaSpace
The United Launch Alliance Delta-IV Heavy rocket tasked with launching NASA’s Orion EFT-1 mission being hoisted vertical atop Space Launch Complex-37B at Cape Canaveral Air Force Station in Florida on the morning of Oct. 1, 2014. Photo Credit: Alan Walters / AmericaSpace

…………….

Learn more about Orion, Space Taxis, and NASA Human and Robotic Spaceflight at Ken’s upcoming presentations:

Oct 26/27: “Antares/Cygnus ISS Rocket Launch from Virginia”; Rodeway Inn, Chincoteague, VA

This 3-D Martian Picture Feels Like You’re Standing Beside The Opportunity Rover

A 3-D image of "Wdowiak Ridge" on Mars, based on images from the left and right side of the Opportunity rover's Pancam. Credit: NASA/JPL-Caltech/Cornell Univ./Arizona State Univ.

Grab your 3-D glasses (you do have a pair handy, right?) and take a look at this latest vista from Mars. This is a view taken by the Opportunity rover that looks at a location nicknamed “Wdowiak Ridge”, on the rim of Endeavour Crater.

This mosaic was obtained Sept. 17 as Opportunity continued its journey to “Marathon Valley”, a spot that could hold clays (which would indicate a water-rich environment in the past.) The rover is more than a decade into its mission and has been sending back images amid battling Flash memory problems lately.

Check out more recent pictures below, including a probable one of Comet Siding Spring passing by Mars (which Bob King wrote about in detail earlier this week.)

“Wdowiak Ridge sticks out like a sore thumb.  We want to understand why this ridge is located off the primary rim of Endeavour Crater and how it fits into the geologic story of this region,” stated Jim Rice, the Opportunity science-team of the Planetary Science Institute in Arizona.

More specifically, the team is interested in why this ridge is so prominent and sharp — they are calling it one of the most distinctive features Opportunity has ever seen. How it resisted erosion in an area so worn down is one thing scientists are hoping to learn about.

A Martian mosaic showing "Wdowiak Ridge", which the Opportunity rover imaged Sept. 17, 2014. The rover's tracks are visible at right. Credit: NASA/JPL-Caltech/Cornell Univ./Arizona State Univ.
A Martian mosaic showing “Wdowiak Ridge”, which the Opportunity rover imaged Sept. 17, 2014. The rover’s tracks are visible at right. Credit: NASA/JPL-Caltech/Cornell Univ./Arizona State Univ.

The last Opportunity rover update talks about activities through Sept. 30, but NASA has released raw images available since then. Check out a selection below.

Is this an image of Comet Siding Spring? It's the only fuzzy object in the field photographed on Sol 3817 (October 19) by the Opportunity Rover. Click for original raw image.
Is this an image of Comet Siding Spring? It’s the only fuzzy object in the field photographed on Sol 3817 (October 19) by the Opportunity Rover. Click for original raw image.
The Opportunity rover at work on Mars on Sol 3,817 in October 2014. Credit: NASA/JPL-Caltech
The Opportunity rover at work on Mars on Sol 3,817 in October 2014. Credit: NASA/JPL-Caltech
An image of Martian terrain with the Opportunity's rover solar panel just visible at the bottom of the panel. Picture taken Sol 3,817 in October 2014. Credit: NASA/JPL-Caltech
An image of Martian terrain with the Opportunity’s rover solar panel just visible at the bottom of the panel. Picture taken Sol 3,817 in October 2014. Credit: NASA/JPL-Caltech
A dramatic, shadowy picture showing part of the Opportunity rover on Mars lit by the Sun (at top). Picture taken Sol 3,812 in October 2014. Credit: NASA/JPL-Caltech
A dramatic, shadowy picture showing part of the Opportunity rover on Mars lit by the Sun (at top). Picture taken Sol 3,812 in October 2014. Credit: NASA/JPL-Caltech
The Opportunity rover's tracks dominate this image taken on Mars on Sol 3,807 in October 2014. Credit: NASA/JPL-Caltech
The Opportunity rover’s tracks dominate this image taken on Mars on Sol 3,807 in October 2014. Credit: NASA/JPL-Caltech

Stunning View of Solar System’s Largest Volcano and Valles Marineris Revealed by India’s Mars Orbiter Mission

Olympus Mons, Tharsis Bulge trio of volcanoes and Valles Marineris from ISRO's Mars Orbiter Mission. Note the clouds and south polar ice cap. Credit: ISRO

India’s Mars Orbiter Mission (MOM) has delivered another sweet treat – a stunning view of our Solar System’s largest volcano and the largest canyon.

Just days ago, MOM captured a new global image of the Red Planet dominated by Olympus Mons and Valles Marineris – which is the largest known volcano and the largest known canyon in the Solar System, respectively.

Situated right in between lies a vast volcanic plateau holding a trio of huge volcanoes comprising the Tharsis Bulge: Arsia Mons, Pavonis Mons, and Ascraeus Mons. All four volcanoes are shield volcanoes.

To give an idea of its enormity, Olympus Mons stands about three times taller than Mount Everest and is about the size of Arizona.

Olympus Mons from Mars orbit compared to the state of Arizona. Credit: NASA
Olympus Mons from Mars orbit compared to the state of Arizona. Credit: NASA

Olympus Mons is located in Mars’ western hemisphere and measures 624 kilometers (374 miles) in diameter, 25 km (16 mi) high, and is rimmed by a 6 km (4 mi) high scarp.

Valles Marineris is often called the “Grand Canyon of Mars.” It spans about as wide as the entire United States.

The Indian Space Research Organization (ISRO), India’s space agency which designed and developed the orbiter released the image on Oct. 17, barely two days ahead of the planet’s and spacecrafts’ extremely close encounter with comet Siding Spring.

By the way, a relieved ISRO tweeted MOM’s survival of her close shave with the once-in-a-lifetime cometary passage with gusto, soon after the swingby:

“Phew! Experience of a lifetime. Watched the #MarsComet #SidingSpring whizzing past the planet. I’m in my orbit, safe and sound.”

The new global image was taken by the tri-color camera as MOM swooped around the Red Planet in a highly elliptical orbit whose nearest point to Mars (periapsis) is at 421.7 km and farthest point (apoapsis) at 76,993.6 km, according to ISRO.

To date ISRO has released four global images of the Red Planet, including a 3-D view, reported here.

Olympus Mons, the Tharsis Bulge, and Valles Marineris are near the equator.

Valles Marineris stretches over 4,000 km (2,500 mi) across the Red Planet, is as much as 600 km wide, and measures as much as 7 kilometers (4 mi) deep.

Here’s a comparison view of the region taken by NASA’s Viking 1 orbiter in the 1970s.

Global Mosaic of Mars Centered on Valles Marineris
Global Mosaic of Mars Centered on Valles Marineris from NASA’s Viking 1 orbiter. Credit: NASA

MOM is India’s first deep space voyager to explore beyond the confines of her home planet’s influence and successfully arrived at the Red Planet only one month ago after the “history creating” orbital insertion maneuver on Sept. 23/24 following a ten month journey.

The $73 million MOM mission is expected to last at least six months.

MOM’s success follows closely on the heels of NASA’s MAVEN orbiter which also successfully achieved orbit barely two days earlier on Sept. 21 and could last 10 years or more.

With MOM’s arrival, India became the newest member of an elite club of only four entities that have launched probes that successfully investigated Mars – following the Soviet Union, the United States, and the European Space Agency (ESA).

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer

ISRO's Mars Orbiter Mission captures spectacular portrait of the Red Planet and swirling dust storms with the on-board Mars Color Camera from an altitude of 74500 km on Sept. 28, 2014.  Credit: ISRO
ISRO’s Mars Orbiter Mission captures spectacular portrait of the Red Planet and swirling dust storms with the on-board Mars Color Camera from an altitude of 74,500 km on Sept. 28, 2014. Credit: ISRO

Mr. Fusion? Compact Fusion Reactor Will be Available in 5 Years Says Lockheed-Martin

Could the future of fusion driven rockets for interplantary or even interstellar travel be near at hand? Engineers at the Lockheed-Martin Skunk Works believe they will have a compact fusion reactor prototype operational in five years and in use within 10 years. (Illustration Credit:© David A. Hardy/www.astroart.org, Project Daedalus)

The Farnsworth Fusor; Pons and Fleishmann. It seems the trail to fusion energy has long gone cold — stone cold, that is, and not cold as in cold fusion. Despite the promise of fusion providing a sustainable and safe energy source, fusion reactors are not a dime a dozen and they won’t be replacing coal fired power plants any time soon. Or will they? Lockheed-Martin Skunk Works announced a prototype compact fusion reactor that could be ready within five years. This revelation has raised eyebrows and sparked moments of enthusiasm.

But, let’s considers this story and where it all fits in both the history and future.

For every Skunk Works project that has made the runway such as the Stealth Fighter or SR-71 Blackbird, there are untold others that never see the light of day. This adds to the surprise and mystery of Lockheed-Martin’s willingness to release images and a detailed narrative describing a compact fusion reactor project. The impact that such a device would have on humanity can be imagined … and at the same time one imagines how much is unimaginable.

Lockheed-Martin engineers in the Skunkworks prepare a vessel, one component of an apparatus that they announced will lead to nuclear fusion in a truck-sized reactor within 5 years. An international effort is underway in Europe to create the worlds first practical tokamak fusion reactor, a much larger and costlier design that has never achieved the long sought "breakeven" point. (Photo Credit: Lockheed-Martin)
Lockheed-Martin engineers in the Skunkworks prepare a vessel, one component of an apparatus that they announced will lead to nuclear fusion in a truck-sized reactor within 5 years. An international effort is underway in Europe to create the world’s first practical tokamak fusion reactor, a much larger and costlier design that has never achieved the long sought “breakeven” point. (Photo Credit: Lockheed-Martin)

The program manager of the Skunk Works’ compact fusion reactor experiment is Tom Maguire. Maguire and his team places emphasis on the turn-around time for modifying and testing the compact fusion device. With the confidence they are expressing in their design and the ability to quickly build, test and modify, they are claiming only five years will be needed to reach a prototype.

What exactly the prototype represents was left unexplained, however. Maguire continues by saying that in 10 years, the device will be seen in military applications and in 20 years it will be delivered to the world as a replacement for the dirty energy sources that are in use today. Military apps at 10 years means that the device will be too expensive initially for civilian operations but such military use would improve performance and lower costs which could lead to the 20 year milestone moment if all goes as planned.

Their system uses magnetic confinement, the same basic principle behind the tokamak toroidal plasma confinement system that has received the greatest attention and government funding for over 50 years.

The ITER Tokamak Fusion Reactor is expected to begin operational testing in 2020 and begin producing deuterium-tritium fusion reactions in 2027. (Credits: ITER, Illus. T.Reyes)
The ITER Tokamak Fusion Reactor is expected to begin operational testing in 2020 and begin producing deuterium-tritium fusion reactions in 2027. (Credits: ITER, Illus. T.Reyes)

The International Thermonuclear Experimental Reactor (ITER) is currently under construction in Europe under the assumption that it will be the first net energy producing fusion generator ever. It is funded by the European Union, India, Japan, People’s Republic of China, Russia, South Korea and the United States. But there are cost over-runs and its price has gone from $5 billion to $50 billion.

ITER is scheduled to begin initial testing in 2019 about the time Lockheed-Martin’s compact fusion reactor prototype is expected. If Lockheed-Martin succeeds in their quest, they will effectively have skunked ITER and laid to waste a $50 billion international effort at likely 1/1000th the cost.

There are a few reasons Lockheed-Martin has gone out on a limb. Consider the potential. One ton of Uranium used in Fission reactors has as much energy as 1,500 tons of coal. But fission reactors produce radioactive waste and are a finite resource without breeder reactors, themselves a nuclear proliferation risk. Fusion produces 3 to 4 times more energy per reaction than fission. Additionally, the fuel — isotopes of hydrogen — is available from sea water — which is nearly limitless — and the byproducts are far less radioactive than with fission. Fusion generators once developed could provide our energy needs for millions of years.

More pragmatically, corporations promote their R&D. They are in a constant state of competition. They present a profile that ranges from the practical to the cutting edge to instill confidence in their Washington coffers. Furthermore, their competitors have high profile individuals and projects. A fusion project demonstrates that Lockheed-Martin is doing more than creating better mouse-traps.

To date, no nuclear fusion reactor has achieved breakeven. This is when the fusion device outputs as much energy as is input to operate it. Magnetic confinement such as the various tokamak designs, Lawrence Livermore’s laser-based inertial confinement method, and even the simple Philo Farnsworth Fusor can all claim to be generating energy from fusion reactions. They are just all spending more energy than their devices output.

An example of a homemade Fusor. Originally invented in the 1960s by the inventor of the television, Philo Farnsworth. (Credit: Wikipedia, W.Jack)
An example of a homemade Fusor. Originally invented in the 1960s by the inventor of the television, Philo Farnsworth. (Credit: Wikipedia, W.Jack)

The fusor, invented in the 1960s by Farnsworth and Hirsh, is a electrostatic plasma confinement system. It uses electric fields to confine and accelerate ions through a central point at which some ions will collide with sufficient energy to fuse. Although the voltage needed is readily achieved by amateurs – about 4000 volts – not uncommon in household devices, no fusor has reached breakeven and theoretically never will. The challenge to reaching breakeven involves not just energy/temperature but also plasma densities. Replicating conditions that exist in the core of stars in a controllable way is not easy. Nevertheless, there is a robust community of “fusioneers” around the world and linked by the internet.

Mr Fusion, the compact fusion reactor that drove the 21st Century version of the DeLorian in Back to the Future. The movie trilogy grossed $1 billion at the box office. Mr Fusion could apparently function off of any water bearing material. (Credit: Universal Pictures)
Mr Fusion, the compact fusion reactor that drove the 21st Century version of the DeLorean in Back to the Future. The movie trilogy grossed $1 billion at the box office. Mr Fusion could apparently function off of any water bearing material. (Credit: Universal Pictures)

It remains to be seen who, what and when a viable fusion reactor will be demonstrated. With Lockheed-Martin’s latest announcement, once again, fusion energy is “just around the corner.” But many skeptics remain who will quickly state that commercial fusion energy remains 50 years in the future. So long as Maguire’s team meets milestones with expected performance improvements, their work will go on. The potential of fusion energy remains too great to dismiss categorically.

Source: Lockheed-Martin Products Page, Compact Fusion

Could ‘Heavy Metal’ Frost Lurk Beneath Venus’ Hothouse Clouds?

A radar view of Venus taken by the Magellan spacecraft, with some gaps filled in by the Pioneer Venus orbiter. Credit: NASA/JPL

Talk about using old data for a new purpose! Researchers re-examining information from the completed NASA Magellan mission found signs of what could be “heavy metal” frost on the hell-like surface. What the researchers saw in radio-wave reflectance is the highlands appear brighter, with dark spots in the tallest locations.

What substance exactly is causing the patches on the surface is unknown, and it is extremely hard to make predictions given the difficulty of simulating Venus’ 900-degree Fahrenheit (500-degree Celsius) surface temperature, which is also 90 times Earth’s air pressure at sea level.

“Like on Earth, the temperature changes with elevation,” stated Elise Harrington, an Earth sciences undergraduate at British Columbia’s Simon Fraser University who led the research. “Among the possibilities on Venus are a temperature dependent chemical-weathering process or heavy metal compound precipitating from the air – a heavy metal frost.”

Venus' volcano Sapas Mons, which was imaged by the Magellan mission in 1991. Credit: NASA
Venus’ volcano Sapas Mons, which was imaged by the Magellan mission in 1991. Credit: NASA

Scrutiny of a previously examined area on Venus, the Odva Regio highlands, saw a low radar reflection at 2,400 meters (7,900 feet), which progressively gets brighter until dark spots begin appearing and reflections drop at 4,700 meters (15,400 meters).

While previous research spotted a few of these patches, Harrington and supervisor Allan Treiman (Lunar and Planetary Institute) saw hundreds. There’s no radar-imaging spacecraft in orbit around Venus right now, but the authors hope that the finding will generate more interest in this planet. (Of note, the European Space Agency’s Venus Express is finishing up a mission there now, which included several daring atmosphere-skimming maneuvers earlier this year.)

The research was presented at the Geological Society of America meeting in Vancouver, British Columbia.

Source: Geological Society of America