From horizon to horizon, in every direction, blue-grey skies descend into a flat, grey, monochromatic landscape that is only disrupted by strong winds and cloud cover.
SOUTH POLE JOURNAL
Refael Klein blogs about his year
working and living at the South Pole. Read his earlier posts here.
The sun circles at nearly the same height each day, its zenith angle dropping at such an imperceptibly slow rate that one often thinks — perhaps hopes — it has called a hiatus to its setting.
The sun rises and sets only once a year at the South Pole, rising in September and disappearing below the horizon in March, which means we experience up to 24 hours of sunlight in the summer and 24 hours of darkness in the winter.
It will get dark slowly here and, even after the sun disappears in about a week, will remain light for nearly a month afterwards. Not until April will dusk begrudgingly give way to night.
Life at Amundson-Scott Station is much like life on-board a ship. The crew — known as the winter-overs — share in collateral duties, cleaning spaces, swabbing decks, and hosting morale and recreation programs. Many of the entrances and exits into the station are dogged (use of a mechanical device called a “dog” to fasten something to something else) to keep out the weather and the wind on stormy days.
All of the skills and trades needed to keep the station operating without assistance from the outside world are present. If a generator fails, we have machinists, engine technicians and utility specialists who will get it back online. If a door needs to be re-leveled, a carpenter can fix it. If someone gets sick or injured, a full medical staff can provide care.
As on a ship, the days can be tedious and long. Rounds are conducted every morning —thermostats checked, glycol levels checked, engine temperatures and fuel usage checked. Many of the tradesmen follow the same routine each day, each week, each month, looking at the same things, performing the same preventive maintenance tasks that were carried out last year and the year before that.
Remaining focused on your job when everything is running smoothly takes mental discipline and, as they say on the bridge of many ocean-going vessels, “The work is 99 percent uneventful and 1 percent ‘Oh, <expletive>, we’re going to die’.”
At the South Pole, we are constantly training for the 1 percent scenario. What happens if there is a fire? What happens if someone gets lost in a whiteout or breaks their arm while working in the Machine Shop? How do we organize the response? How do we carry out the tasks that would otherwise be handled by professional search and rescue specialists, paramedics and firefighters?
Everyone who works on-station is a member of an emergency response team. The station has five teams, each specializing in a type of emergency or a general aspect of the response process. They include fire, medical, logistics and technical rescue teams and a group of first responders, to which I belong, whose role it is to secure the scene, and organize and lead the other groups as they attend to different emergency situations.
Each team meets weekly to train for an hour and, every month, there is a drill that the entire station participates in. Last month, we ran through a scenario in which someone had fallen off a ladder in the fuel arch, broken his leg, and lost consciousness. We carried the litter for a half-mile, climbing up numerous flights of steps, to get the patient to the sick bay. All in all, it took us about 50 minutes, not bad for a novice team carrying a limp 270-pound electrician.
This month’s scenario took place at our balloon inflation facility (BIF). I had just walked out to the Atmospheric Research Observatory (ARO), belly full from a lunch of grilled salmon and roasted vegetables, when the alarm went off and a computerized voice came over the PA announcing, “A fire has been detected”.
ARO sits close to a half-mile north of the BIF, so it was a challenge for me to get out there quickly. I radioed in my location and ETA to the on-scene commander, our group lead, and headed out the door, walking as fast as I could through soft snow while wearing heavy insulated boots.
The sun sat only a few degrees above the horizon. At that elevation and direction, it shined directly into my face. My goggles fogged up quickly from the exertion and cold, and soon I couldn’t see anything but a blurry, bright mass of snow and sky. I removed my goggles and instantly felt the full intensity of the sun against my face. As one shouldn’t do, I stared straight into it, unblinking, until my eyes began to water. I closed them tightly and turned away into the wind.
My eyelashes froze together, prompting the sun’s orange-and-yellow imprint to slowly fade from vision. I turned back towards the sun, tempted to look into it again, perhaps to create a more permanent memory, something to carry me through the winter, but I didn’t, and continued walk towards the emergency, eyes to the ground, indifferent to the cold.
More South Pole Diaries
South Polies Tackle Last-minute Preps to Survive Brutal Winter
South Pole Summer Camp Helps Combat Winter Blues
Stranded Until Spring: Last Flight Leaves South Pole Before Winter Hits
In Giant Parkas, Rank Is Less Apparent
A new study from researchers at the SETI Institute (Search for Extraterrestrial Intelligence) and the Southwest Research Institute (SwRI) has found that most of Saturn’s 62 moons and perhaps even its celebrated rings may only be a hundred million years old. That’s more recent than when dinosaurs were roaming Earth.
One of the study authors, Matija Cuk, principal investigator at the SETI Institute, said he and his team created computer simulations to check into the history of some of the ringed planet’s icy inner moons. Those computer models indicated that they were created ‘sometime during the most recent two percent of the planet’s history.’
Saturn’s rings have been known since Galileo first observed them back in the early 1600’s but scientists still argue about their age. Many assume that the rings are as old as the planet itself, between 4.5 – 4.6 billion years old. But, new research suggests that they, along with Saturn’s moons, were created more recently.
A moon’s orbit can be affected its gravitational interaction – tidal effects – with not only the host planet but with other moons.
To find out when Saturn’s moons were created, the researchers consulted data gathered by NASA’s Cassini mission.
By assuming that the moon’s geysers are driven by the energy created by these tidal effects and that the amount of its geothermal activity has always pretty much remained the same, the researchers figured that Saturn’s tides must be pretty strong.
Analyzing this information the team found that it would take Saturn’s tides nearly 100 million years for Enceladus to move from where it was formed to its current location, as it was predicted by the group’s simulations.
This would mean that except for Titan and Iapetus, which are further away, its major inner moons such as Tethys, Rhea, and Dione formed sometime during Earth’s Cretaceous Period, some 66 to 145 million years ago, which is known as the last portion of the “Age of Dinosaurs”.
The researchers add that they think Saturn once had a previous assortment of moons similar to its current inner moons. But they were destroyed when their orbits were disturbed by some event that caused them to smash each other to bits.
“From this rubble, the present set of moons and rings formed,” said Cuk in a press release.”
The researcher’s findings have been published in the Astrophysical Journal.
Earth’s Auroras – Borealis in the northern polar region and Australis in the south – are among the most beautiful and haunting light displays in nature.
Now, for the first time, scientists have been able to study Jupiter’s auroras, in x-ray wavelengths thanks to NASA’s Chandra X-Ray Observatory.
Auroras both on Earth and on Jupiter are triggered by high charged energy particles blasting their way through the solar system on the solar wind.
But scientists have found that Jupiter’s aurora, generated by a giant interplanetary coronal mass ejection in October 2011, happened to be eight times brighter and have hundreds times the energy than Earth’s.
The study of Jupiter’s aurora comes just months before NASA’s Juno spacecraft is set to arrive at the planet.
During its scheduled 37 orbits of the giant planet, the Juno mission will study Jupiter’s make-up, gravity field, magnetic field (or magnetosphere) and its relationship with the solar wind.
Music has the power to transcend barriers of language and culture and the ability to stir deep human emotion.
A group of Finnish researchers has found that it’s not only music itself but also where you listen to it that can influence its emotional impact.
Previous scientific research suggests that emotional reaction to music can be gauged by physical responses, such as changes in the electrical properties of the skin.
With this in mind the researchers played a selection of a Beethoven symphony as it would be heard in different concert halls to a group of test subjects.
The scientists from Aalto University attached sensors, to the subject’s fingers, which measured these electrical changes, as they listened to the music under the varied acoustic conditions.
The researchers found that music played in the acoustical environment of shoebox-type or rectangular concert halls produced the strongest emotional reaction in the listeners than other hall designs.
The study was published in the Journal of the Acoustical Society of America.
Artist Animation of Star Explosion (NASA/JPL/Australian National University)
Back in 2011, NASA’s Kepler Space Telescope captured two red supergiant stars as they exploded into supernovae.
Astrophysicists studying the Kepler data, were able to not only watch both stars as they exploded, but for the first time, spot the tremendous shockwave produced deep inside the smaller of the two as its core collapsed.
Called KSN 2011a, the smaller supernova is only 700 million light years away from us, and is nearly 300 times the size of our sun.
The other, called KSN 2011d, is located 1.2 billion light years away, and had 500 times the solar mass.
The supernova shockwave is described as resembling a nuclear explosion on a massive scale.
The astrophysicists say that their observations of the supernovae will help scientists better understand how the earliest moments of a star’s explosive death is affected by its makeup and size.
We have published several stories about the health dangers of sitting too much and its link to the onset of some chronic diseases and early death.
Now a new study published in the American Journal of Preventative Medicine finds sitting for more than three hours a day is to blame for 3.8% of all worldwide deaths.
The study authors also found that moderate or even vigorous physical exercise might not be able to offset the negative effects of sitting for too long.
They suggest that reducing daily sitting time to less than three hours a day would add an average of .2 years to a person’s life expectancy.
The researchers say the link between sitting and death was highest in Western Pacific nations, followed by European, Eastern Mediterranean, American, and then Southeast Asian countries.
Lately, more office workers are using work stations that allow them to alternate between sitting and standing throughout the day.
The last plane left two weeks ago and everyone is settling into their wintertime roles.
SOUTH POLE JOURNAL
Refael Klein blogs about his year
working and living at the South Pole. Read his earlier posts here.
Station population sits at 50 and most departments are only a fraction of the size they once were. Although the summer crew left us in good shape, there is still a lot of work to get done before the sun sets.
Outbuildings are being winterized — windows boarded up, electricity cut off. Food stores are hauled from the berms to storage facilities inside, all of the food we need for 50 people for 8 months. And our emergency systems are being tested and retested; we need to know our spare generators will work, no matter what.
It’s getting colder. Temperatures are regularly dropping into the minus 60s Fahrenheit (minus 51 Celsius). In a week, maybe two, it will be too cold to operate our heavy equipment. No fork trucks, no snow plows, no tractors. Snow drifts will begin to form anew and anything that needs to get dragged from one point to another will need to be pulled by snowmobile or by hand.
Needless to say, everyone is taking advantage of the current conditions, getting as much done before winter truly takes hold. It’s going to be a sprint to the finish, but when your only option is to “make it,” you “make it”.
At the Atmospheric Research Observatory (ARO), we are buttoning up the last of our more physically intensive, outside tasks. We raised our 2-meter meteorological instruments by a foot, so that they will still be at the same height, above the snow, in eight months, as they were when I first arrived. And we ran two new intake lines up our 30-meter tower for our gas chromatograph. Each activity took the better half of a day and resulted in cold hands, frost-nip and a few expletives, as work in these conditions often does.
Our gas chromatograph is perhaps the single most complex piece of equipment we utilize at ARO. It is the workhorse of our Halocarbon research group, taking continuous measurements of various ozone-depleting substances and their replacement compounds. Since these chemicals only exist at very trace levels in the atmosphere, the instrument is designed to measure accurately at the part per trillion scale.
In other words, if you were to fill 400 Olympic size swimming pools with sugar cubes and then throw in one that was painted red, we would find it. It’s what our gas chromatograph does, continuously every day of the year: find, identify and count highly-elusive compounds.
When all is said and done, why does this matter? If something only exists at part per trillion levels, does it really affect our planet? The answer is yes, and when it comes to ozone-depleting substances and their replacement compounds, it does so to a surprisingly high degree.
Chlorofluorocarbons, CFCs for short, make up the bulk of ozone-depleting substances. They were invented in the 1920s, as replacements for the refrigerants ammonia, sulfur dioxide and methyl chloride — all of which were highly toxic and dangerous to human health. At the time, CFCs were seen as a big step forward. They were relatively inert, could withstand a seemingly endless number of refrigeration cycles and, if there happened to be a leak in your refrigerator, you wouldn’t die while pouring yourself a glass of milk.
What wasn’t known in the 1920s was the effect that trace amounts of CFCs would have on the ozone layer.
When there is a leak in your refrigerator, freezer or air-conditioner, refrigerant escapes and, if that refrigerant is a CFC, it will remain intact, unreactive, all the way to the stratosphere. Once in the stratosphere, with the help of UV radiation, CFCs are broken apart and release chlorine atoms, which proceed to bounce from ozone molecule to ozone molecule, tearing each one apart. It can do this for decades, which means that, even at a part per trillion levels, CFCs can do a lot of damage.
In fact, CFCs turned out to be so effective in destroying the ozone layer that, in the late 1980s, 27 nations, including the United States, drew up a treaty banning their use. To this day, the Montreal Protocol is considered by many to be the single most successful piece of international environmental legislation ever enacted. It stopped the use and production of CFCs, and replaced them with compounds that had shorter atmospheric lifespans and less ozone-destroying potential.
The gas chromatograph used by NOAA’s Global Monitoring Division (GMD) is helping us better understand the dynamics of ozone recovery and predict what will happen in the future. The main focus of the instrument is to measure the presence of banned compounds, under the Montreal Protocol, and their replacements. As one would predict, CFCs are becoming less abundant and their replacement compounds are becoming more so, meaning the treaty is doing what it was designed to do: protect the ozone layer.
Working on the gas chromatograph has its challenges. It requires the most maintenance out of any project I work on — changing gas cylinders, tightening valves, adjusting air flows, building and replacing small fittings. Sometimes our data shows a .5 part per trillion difference from what we expect to see. Where did the error come from? Was it me, the instrument, or the environment? It can be hard to figure out and, on occasion, working on such minute issues feels like chasing ghosts.
Studying the computer that runs the system, I watch data tick by; peaks form, they grow and shrink. Each one represents the presence of a certain compound and its abundance. Cycle after cycle, hour after hour, more data is displayed, compiled, and sent back to our labs for analysis.
I watch global trends unfold, the ebbs and flows of culture and industry as seen through the chemicals we produce. Everything measured at the smallest scale, the highest accuracy, and absolutely representative of our planet.
They chose to explore in the ultraviolet range since there are so many hot and extremely massive stars in the cluster that mostly radiate energy within that part of the electromagnetic radiation spectrum.
The group used a combination images gathered by the Hubble Space Telescope’s Wide Field Camera 3 (WFC3) and the Space Telescope Imaging Spectrograph (STIS) to detect dozens of stars with at least 50 times the mass of the sun and about nine others with more than 100 times the solar mass.
The nine most massive of these stars were found to be not only incredibly enormous, but together they produce an extremely bright light that is 30 million times more luminous than our own Sun.
While the group was able to spot a number of supermassive stars, a previously detected star in the cluster called R136a1 is the most massive star known to exist in the Universe. It has a solar mass of about 265 times that of the Sun and is thought that to have had a solar mass of about 320.
The astronomer’s findings were outlined in a paper published by the Monthly Notices of the Royal Astronomical Society,
“The ability to distinguish ultraviolet light from such an exceptionally crowded region into its component parts, resolving the signatures of individual stars, was only made possible with the instruments aboard Hubble,” explains the paper’s lead author Paul Crowther of the United Kingdom’s University of Sheffield in a press release.
Another of the paper’s authors, Saida Caballero-Nieves, also from the University of Sheffield, said that while some scientists have previously suggested that these monster stars were created by the merger of smaller binary system stars, this doesn’t really explain the supermassive stars in the R136 cluster.
Instead, he says that it appears the road that led to the huge size of these stars may have begun with its formation process.
The astronomers plan to continue analyzing the Hubble data they’ve gathered to learn more about the giant star’s origination.
They’ll also analyze new information from the Space Telescope’s Imaging Spectrograph to look for nearby binary star systems, where orbiting black hole binaries may lurk.
The twin black holes would eventually merge and produce the gravitational waves such as those predicted by Einstein in his Theory of General Relativity and were only recently detected by the LIGO Scientific Collaboration.
The dwarf planet Ceres is the largest body in the asteroid belt, which is a large collection of small to very large space rocks between the orbits of Mars and Jupiter.
Among the features of the dwarf planet that’s fascinated a lot of people are several bright spots on its surface.
Some scientists think that this might suggest Ceres is more active than any neighbors in the asteroid belt.
The most noticeable spots are located within Ceres’ Occator crater.
Scientists think that the bright spots may be collections of brine that contain magnesium sulfate hexahydrate.
Now, astronomers using the HARPS spectrograph at the European Southern Observatory’s La Silla Observatory in Chile have found that these bright spots go through some surprising changes.
While the spots have been known to change as Ceres rotates, the scientists also found that they also vary and brighten during the day.
The scientists say that their observations suggest that the bright spots may be made up of volatile substance and that solar radiation make cause it to evaporate.
NASA’s DAWN spacecraft has been circling and studying Ceres and its mysterious bright spots since arriving there a year ago.
About 21-percent of world electricity generation is estimated to be from non-fossil fuels such as the wind or sun.
But scientists hope to boost that number by looking at new ways to create it – one of which involves spoiled fruit.
A team of researchers found that damaged or spoiled tomatoes can be turned into a unique and powerful source of renewable energy when fed to biological and microbial electrochemical cells.
And the good news is, there seems to be a nearly endless supply of damaged and rotten tomatoes. Florida alone generates 396,000 tons of tomato waste every year.
The scientists admit that right now the power produced by their tomato fueled energy cells is quite small.
But they’re quite optimistic that with continued research they’ll be able to greatly increase the electrical output of their energy cells.
Black holes aren’t usually visible since material surrounding them, even light, is devoured by their intense gravity.
But occasionally a black hole can draw in material, such as a star, so rapidly that it spits some of it out, producing a powerfully bright light in the process.
Last June, astronomers noticed that a black hole called V404 Cygni, some 7,800 light years from Earth, became very bright for about a two week period.
As they observed this phenomena, they noticed the black hole also produced very bright flashes of red light that lasted only fractions of a second.
The astronomers say that each of these flashes produced light so intense it had the equivalent power of about 1,000 suns.
Poshak Gandhi, lead author of a study detailing the astronomer’s discovery, says that the red flashes seem to have been produced when the black hole was at the peak of its feeding frenzy.
The first of two ExoMars missions took off for the Red Planet from the Baikonur Cosmodrome on Monday, March 14th.
ExoMars is joint project between the European Space Agency and the Russian Federal Space Agency, Roscosmos.
The purpose of ExoMars is to find out if life ever existed on Mars.
The two spacecraft now being sent to Mars are the Trace Gas Orbiter and its attached Schiaparelli EDM lander.
Once they arrive at the Red Planet sometime in October the lander will be sent from the orbiter to the surface.
The orbiter will circle Mars and will sniff out the sources of methane and other gases in the Martian atmosphere.
The lander will monitor various weather conditions on Mars and gather information that will be used in the second ExoMars probe, which will be launched in 2018.
Methane has been seen as a possible sign of life since the gas is produced here on Earth by living organisms.
Construction on the Amundson-Scott elevated station began in 1998 and was completed in 2008.
SOUTH POLE JOURNAL
Refael Klein blogs about his year
working and living at the South Pole. Read his earlier posts here.
During the height of construction, the summer population at the South Pole ballooned to over 250 people. To accommodate the overflow in personnel, plastic, blue half-moon-shaped berthing units were installed south of the station. And heated plywood workshops were built for storage and shop space.
In addition, two unpainted, unfinished lounges were constructed, as well as a small gym with free weights and treadmills. This small village of about a dozen out-buildings was known as Summer Camp.
The cold dry Antarctic climate has been kind to Summer Camp and, seven years later, the buildings look as new as the day they were built. A few have been buried by drifting snow, but those that are still above ground continue to be used for storage and construction workshops.
When it’s too cold or windy to go skiing, I often find myself at the eastern-most side of Summer Camp, in a squat rectangular building with three poly-carbonate windows.
From the outside, the building, the old gym — a mishmash of mis-cut pieces of wood — looks like it was built by a group of elementary school boys to use as a club-house. The first time you see it, you half expect to see a sign that says, “NO GROWN UPS OR GIRLS ALLOWED”.
In a way, the old Summer Camp gym is a bit of a boy’s fort. It’s dimly lit, dirty and filled with broken exercise equipment and a spartan collection of free weights. That being said, any shortcomings of the building are made up by the fact that it is heated, has a good sound system, and is home to the southernmost climbing wall in the world.
As an avid rock climber, I was beside myself with excitement when I discovered the existence of a small climbing facility on station. Apparently, the wall didn’t always exist and wasn’t part of the gym’s original design.
As the story goes, two Italian scientists who were serious alpinists came to the South Pole a few years ago. Unwilling to let their wrists, hands and fingers atrophy, they spent their free time outside the lab stockpiling discarded building supplies and secretively building a small climbing wall at the summer camp gym. When they were done, they broke the news to station management — who, remarkably, were not upset — and convinced them to order two dozen pairs of climbing shoes and a few hundred plastic hand and foot holds.
WATCH VIDEO: Refael Klein blows off steam on the South Pole’s Summer Camp climbing wall
Today, thanks to altruism of the Italians, I, and many others on station, have a fun way to exercise and blow off steam after work. On a typical day, I spend an hour at the gym traversing the wall and setting new “problems”, short sequences of climbing movements, which I mark with colored tape.
The wall isn’t big and it takes a number of laps around its perimeter, or up its central overhang, before I get tired. As I climb, I like to have music playing and I keep the volume turned up loud enough to drown out the sound of the wind and heavy equipment clearing snow drifts.
Sometimes I become so focused on a challenging movement that I forget where I am. It could be Colorado, California or Corsica. It’s not until a foot slips, or I miss a hand hold and fall, that I remember I’m living at the bottom of the world and that I am thousands of miles away from any fantasy.
Advancing technology is making it possible for scientists to investigate the early universe.
About 200 million years after the Big Bang, it is thought that clumps of condensed primordial cold gas clouds provided material for the first stars to be born. As stars were created they formed small galaxies.
An international team of researchers are now saying that they’ve discovered about 80 galaxies that may have existed in the young universe about 12.6 billion years ago, which is around 1.2 billion years after the Big Bang.
The research team comes from Japan’s Ehime University, Nagoya University, and Tohoku University and the Space Telescope Science Institute (STScI) at Johns Hopkins University and the California Institute of Technology, in the U.S.
The team developed a list of galaxies to look for from data gathered by the Subaru Suprime Focus Camera (Suprime-Cam) instrument.
With that information they were able to locate these 80 early galaxies and were able to conduct a detailed analysis on imaging data gathered by the Hubble Space Telescope’s (HST) Advanced Camera for Surveys (ACS).
The ACS is the Hubble’s prime imaging instrument.
The researchers were able to determine that around 1.2 billion years after the Big Bang these small galaxies were continuously merging together and growing into larger galaxies like our own Milky Way, which contains about 200 billion stars.
The researchers outlined their findings in a paper that was published in the Astrophysical Journal.
The new galaxy created by this merger of the Milky Way with Andromeda galaxies has been nicknamed Milkomeda.
According to the Harvard-Smithsonian Center for Astrophysics (CfA), the Milky Way is zooming towards the Andromeda galaxy, at a rate of about 120 kilometers per second.
Both the Milky Way and Andromeda galaxies are part a group of galaxies known as “The Local Group“.
This grouping of galaxies also includes about forty other, much smaller galaxies and all are bound together by gravity.
The LISA – which stands for Laser Interferometer Space Antenna – Pathfinder’s job is to test and establish crucial technologies and techniques that would make it possible for future mission such as ESA’s proposed Evolved Laser Interferometer Space Antenna (eLISA), a space observatory that would detect and study gravitational waves in outer space.
Last month the LIGO Scientific Collaboration set the scientific community abuzz with news of the first discovery of these fluctuations in the fabric of spacetime, which was predicted by Albert Einstein a little over a century ago in his theory of General Relativity.
The proposed eLISA, which has been tentatively scheduled for launch some time in 2034, will be so sensitive that it would be able to detect gravitational waves with longer wavelengths than those that can be detected on the ground. This would provide scientists with tool capable of investigating some of the most massive and powerful objects in the Universe.
To lay the groundwork needed for developing the needed technologies to produce such an observatory, the LISA Pathfinder spacecraft will attempt to create a “near perfect free fall”.
The LISA Pathfinder crew has released two identical gold-platinum cubes, or test masses, that are suspended in its own vacuum enclosure inside the spacecraft.
Each cube weighs 2 kg and measures 46 mm; the enclosures are separated by a distance of 38 cm.
ESA scientists are working to create conditions with the spacecraft to ensure that only the force of a gravitational wave could cause them to wiggle around.
To do this, the spacecraft continually measures the cube’s positions and uses micro-thrusters to manipulate the spacecraft around them with to avoid it ever touching them.
Over next half-year, ESA scientists will conduct a number of experiments and ‘poking’ the cubes to study their motion and then experiment with different technologies that will help maintain their near perfect free-fall.
The experiments will include one where scientists boost the temperature inside each cube’s enclosure to heat any remaining gas molecules and determine it has any effect on the cube’s motion.
ESA is also planning to apply increasingly stronger magnetic and electric forces to the two test masses to determine just how much force would be needed to disturb them from their perfect freefall.
The LISA Pathfinder cannot detect gravitational waves itself since the distance between the two cubes is too small to measure the slight vibration in the fabric of spacetime.
To measure gravitational waves in space the distance between test masses would have to be much greater.
The proposed eLISA mission would be made up of one “Mother” and two “Daughter” spacecraft that will orbit the Sun – similar to Earth’s orbit – in a triangular configuration.
The “Mother” and two “Daughter” spacecraft would be separated by a distance of a million kilometers and will be connected to each other by laser beams, which form the arms of a highly precise Michelson-like laser interferometer.
Any incoming gravitational waves would be detected by this interferometer by monitoring for any changes in the distance between its lengthy arms.
The eLISA mission, formerly known as LISA, was originally proposed as a joint project between ESA and NASA. But due to funding limitations, NASA had to withdraw from the partnership on April 8, 2011. The project was later revised as Europe only mission.