Spectacular View of the Alps From Space! Expedition 42 Flight Engineer Samantha Cristoforetti of the European Space Agency (ESA) took this photograph of the Alps from the International Space Station. She wrote, "I'm biased, but aren't the Alps from space spectacular? What a foggy day on the Po plane, though! #Italy" Credit: NASA/ESA/Samantha Cristoforetti
Spectacular View of the Alps From Space! Expedition 42 Flight Engineer Samantha Cristoforetti of the European Space Agency (ESA) took this photograph of the Alps from the International Space Station. She wrote, “I’m biased, but aren’t the Alps from space spectacular? What a foggy day on the Po plane, though! #Italy” Credit: NASA/ESA/Samantha Cristoforetti
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The current six person crew includes astronauts and cosmonauts from three nations – America, Russia, and Italy – and the four men and two women are celebrating New Year’s 2015 aboard the massive orbiting lab complex.
Happy New Year! Celebrating from space with @AstroTerry. Credit: NASA/Terry Virts
They comprise Expedition 42 Commander Barry “Butch” Wilmore and Terry Virts from NASA, Samantha Cristoforetti from the European Space Agency (ESA), and cosmonauts Aleksandr Samokutyayev, Yelena Serova, and Anton Shkaplerov from Russia.
Beauty everywhere! Flying from the Mediterranean to the Caspian Sea, this appeared through the clouds.#HelloEarth. Credit: NASA/ESA/Samantha Cristoforetti
The ISS has been continuously occupied by humans for 15 years. And they are joined by Robonaut 2 who recently got legs.
This area saw some serious action about 350 million years ago! Gweni-Fada meteorite crater in #Chad. Credit: NASA/ESA/Samantha Cristoforetti
Terry Virts and Samantha Cristoforetti have been especially prolific in picture taking and posting to social media for us all to enjoy the view while speeding merrily along at 17,500 mph from an altitude of about 250 miles (400 kilometers) above Earth.
Here’s a special New Year video greeting from Wilmore and Virts:
Video Caption: Happy New Year from the International Space Station from NASA astronauts Barry “Butch” Wilmore and Terry Virts. Credit: NASA
“Happy New Year from the International Space Station!” said Wilmore.
“We figure that we will be over midnight somewhere on the Earth on New Year’s for 16 times throughout this day. So we plan to celebrate New Year’s 16 times with our comrades and our people down on Earth.”
No sunsets until Jan 4th- we are in a “high beta” orbit now, so this is as dark as it gets. Credit: NASA/Terry Virts
“We wish everybody a happy, healthy, and prosperous 2015 as we get the awesome privilege of celebrating New Year’s here on the space station with our six station crewmates,” added Virts!
“We’ll enjoy our 16 New Year’s celebrations here.”
Part of the #Aral sea peaking through the clouds as we flew into #Kazakhstan! #HelloEarth. Credit: NASA/ESA/Samantha Cristoforetti
They plan to celebrate the dawn of 2015 with fruit juice toasts, NASA reports.
The year 2015 starts officially for the station crew at midnight by the Universal Time Clock (UTC), also known as Greenwich Mean Time (GMT), in London, or at 7 p.m. EST Dec. 31.
If I couldn’t be in space right now I’d want to be here- #Hawaii. Credit: NASA/Terry Virts
New Year’s Day 2015 is a day off for the crew.
And I’m certain they’ll be gazing out the windows capturing more views of “Our Beautiful Earth!”
42 è la risposta! // 42 is the answer! #Expedition42 Guide to the galaxy. Credit: @NASA_Astronauts #AstroButch
And don’t forget to catch up on the Christmas holiday imagery and festivities from the station crews in my recent stories – here and here.
#NewYork NewYork! Can almost see the Statue of Liberty. Which is, by the way, #UNESCO#WorldHeritage! Credit: NASA/ESA/Samantha Cristoforetti
Be sure to remember that you can always try and catch of glimpse of the ISS flying overhead by checking NASA’s Spot the Station website with a complete list of locations.
ISS streaks over Princeton, NJ – time lapse image. Credit: Ken Kremer
Meanwhile the crew continues science operations and preparations for next week’s arrival of the next unmanned space station resupply ship on the SpaceX CRS-5 mission.
CRS-5 is slated to blast off atop a SpaceX Falcon 9 rocket on Jan. 6 from Cape Canaveral Air Force Station in Florida.
SpaceX Falcon 9 rocket is set to soar to the ISS after completing a successful static fire test on Dec. 19 ahead of the planned CRS-5 mission for NASA in early January 2015. Credit: Ken Kremer – kenkremer.com
Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.
ISS astronauts Barry “Butch” Wilmore, NASA, Samantha Cristoforetti, ESA, and Terry Virts, NASA, send Christmas 2014 greetings from the space station to the people of Earth. Credit: NASA/ESAISS Expedition 42. Credit: NASA/ESA/Roscosmos
We see the Moon differently depending upon the wavelength in which we view it. Top row from left:
“By the Light of the Silvery Moon” goes the song. But the color and appearance of the Moon depends upon the particular set of eyes we use to see it. Human vision is restricted to a narrow slice of the electromagnetic spectrum called visible light.
With colors ranging from sumptuous violet to blazing red and everything in between, the diversity of the visible spectrum provides enough hues for any crayon color a child might imagine. But as expansive as the visual world’s palette is, it’s not nearly enough to please astronomers’ retinal appetites.
Visible light is a sliver of light’s full range of “colors” which span from kilometers-long, low-energy radio waves (left) to short wavelength, energetic gamma rays. It’s all light, with each color determined by wavelength. Familiar objects along the bottom reference light wave sizes. Visible light waves are about one-millionth of a meter wide. Credit: NASA
Since the discovery of infrared light by William Herschel in 1800 we’ve been unshuttering one electromagnetic window after another. We build telescopes, great parabolic dishes and other specialized instruments to extend the range of human sight. Not even the atmosphere gets in our way. It allows only visible light, a small amount of infrared and ultraviolet and selective slices of the radio spectrum to pass through to the ground. X-rays, gamma rays and much else is absorbed and completely invisible.
Earth’s atmosphere blocks a good portion of light’s diversity from reaching the ground, the reason we launch rockets and orbiting telescopes into space. Large professional telescopes are often built on mountain tops above much of the denser, lower atmosphere. This expands the viewing “window” into the infrared. Credit: NASA
To peer into these rarified realms, we’ve lofting air balloons and then rockets and telescopes into orbit or simply dreamed up the appropriate instrument to detect them. Karl Jansky’s homebuilt radio telescope cupped the first radio waves from the Milky Way in the early 1930s; by the 1940s sounding rockets shot to the edge of space detected the high-frequency sizzle of X-rays. Each color of light, even the invisible “colors”, show us a new face on a familiar astronomical object or reveal things otherwise invisible to our eyes.
So what new things can we learn about the Moon with our contemporary color vision?
Radio Moon
Radio: Made using NRAO’s 140-ft telescope in Green Bank, West Virginia. Blues and greens represent colder areas of the moon and reds are warmer regions. The left half of Moon was facing the Sun at the time of the observation. The sunlit Moon appear brighter than the shadowed portion because it radiates more heat (infrared light) and radio waves.
Submillimeter Moon
Submillimeter: Taken using the SCUBA camera on the James Clerk Maxwell Telescope in Hawaii. Submillimeter radiation lies between far infrared and microwaves. The Moon appears brighter on one side because it’s being heated by Sun in that direction. The glow comes from submillimeter light radiated by the Moon itself. No matter the phase in visual light, both the submillimeter and radio images always appear full because the Moon radiates at least some light at these wavelengths whether the Sun strikes it or not.
Mid-infrared Moon
Mid-infrared: This image of the Full Moon was taken by the Spirit-III instrument on the Midcourse Space Experiment (MSX) at totality during a 1996 lunar eclipse. Once again, we see the Moon emitting light with the brightest areas the warmest and coolest regions darkest. Many craters look like bright dots speckling the lunar disk, but the most prominent is brilliant Tycho near the bottom. Research shows that young, rock-rich surfaces, such as recent impact craters, should heat up and glow more brightly in infrared than older, dust-covered regions and craters. Tycho is one of the Moon’s youngest craters with an age of just 109 million years.
Near-infrared Moon
Near-infrared: This color-coded picture was snapped just beyond the visible deep red by NASA’s Galileo spacecraft during its 1992 Earth-Moon flyby en route to Jupiter. It shows absorptions due to different minerals in the Moon’s crust. Blue areas indicate areas richer in iron-bearing silicate materials that contain the minerals pyroxene and olivine. Yellow indicates less absorption due to different mineral mixes.
Visible light Moon
Visible light: Unlike the other wavelengths we’ve explored so far, we see the Moon not by the light it radiates but by the light it reflects from the Sun.
The iron-rich composition of the lavas that formed the lunar “seas” give them a darker color compared to the ancient lunar highlands, which are composed mostly of a lighter volcanic rock called anorthosite.
UV Moon
Ultraviolet: Similar to the view in visible light but with a lower resolution. The brightest areas probably correspond to regions where the most recent resurfacing due to impacts has occurred. Once again, the bright rayed crater Tycho stands out in this regard. The photo was made with the Ultraviolet Imaging Telescope flown aboard the Space Shuttle Endeavour in March 1995.
X-ray Moon
X-ray: The Moon, being a relatively peaceful and inactive celestial body, emits very little x-ray light, a form of radiation normally associated with highly energetic and explosive phenomena like black holes. This image was made by the orbiting ROSAT Observatory on June 29, 1990 and shows a bright hemisphere lit by oxygen, magnesium, aluminum and silicon atoms fluorescing in x-rays emitted by the Sun. The speckled sky records the “noise” of distant background X-ray sources, while the dark half of the Moon has a hint of illumination from Earth’s outermost atmosphere or geocorona that envelops the ROSAT observatory.
Gamma ray Moon
Gamma rays: Perhaps the most amazing image of all. If you could see the sky in gamma rays the Moon would be far brighter than the Sun as this dazzling image attempts to show. It was taken by the Energetic Gamma Ray Experiment Telescope (EGRET). High-energy particles (mostly protons) from deep space called cosmic rays constantly bombard the Moon’s surface, stimulating the atoms in its crust to emit gamma rays. These create a unique high-energy form of “moonglow”.
Astronomy in the 21st century is like having a complete piano keyboard on which to play compared to barely an octave a century ago. The Moon is more fascinating than ever for it.
Night sky view from New Zealand. Credit and copyright: Manoj Kesavan.
Photographer Manoj Kesavan has been working on this timelapse since mid-2013 and the results are stunning and spellbinding. ‘Leave Home’ was shot from many locations in Palmerston North, New Zealand in 2013 then continued in 2014 from Taupo and Auckland. Early in the timelapse you’ll see daytime views of the New Zealand landscape but midway, the night views kick in. Hang on while watching some of the spinning Milky Way shots, and the wave scenes might leave you hypnotized! All in all, this is a gorgeous look at the land, sea and skies of New Zealand.
The images were shot with Canon 20D, Canon 7D & 60D with various Canon & Sigma Lenses and batch processed with Lightroom 5. Motion control was achieved by Dynamic Perception stage one dolly & Emotimo TB3 Black.
Artist's impression of an asteroid breaking up. Credit: NASA/JPL-Caltech
The early Solar System was a shooting gallery. Smaller-body collisions happened far more frequently than we see it today, pockmarking the Moon and Mercury. On a larger scale, simulation show the Earth came close to blowing apart when a Mars-sized object crashed into us long ago.
So we’d be forgiven for thinking that it’s asteroid collisions that cause these tiny bodies to break up, given their numbers and the history of our neighborhood. But it turns out, a new study says, that the larger asteroids likely have another way of coming apart.
“For asteroids about 100 meters [328 feet] in diameter collisions are not the primarily cause of break ups – rapid rotation is,” the Smithsonian Astrophysical Observatory stated.
“Moreover, because the rate of collisions depends on the numbers and sizes of objects but rotation does not, their results are in strong disagreement with previous models of collisionally-produced small asteroids.”
Most near-Earth asteroids fall into three classes named after the first asteroid discovered in that class. Apollo and Aten asteroids cross Earth’s orbit; Amors orbit just beyond Earth but cross Mars’ orbit. Credit: Wikipedia
It turns out that rotation has a strong effect on such a small body. First, the asteroid is emitting stuff that can produce a spin — water evaporating, or its surface expanding as heat from the Sun strikes it. Also, the Sun’s pressure on the asteroid creates a rotation. Between these different effects, at the right (or wrong) moment it can cause a catastrophic breakup.
As a simulation (coupled with observations from the Pan-STARRS telescope), the research is not done with complete certainty. But the model shows 90% confidence that asteroids in the so-called “main belt” (between Mars and Jupiter”) experience disruptions in this way, at least once per year.
The research was published in the journal Icarus and is also available in preprint version on Arxiv. It was led by Larry Denneau at the University of Hawaii.
A new Avengers movie. A reboot of the Star Wars franchise. The final installment of the Hunger Games. The Martian makes it to the big screen. Yup, even if the zombie apocalypse occurs in 2015, it’ll still be a great year. But trading science fiction for fact, we’re also on track for a spectacular year in space science and exploration as well.
Humanity will get its first good look at Ceres and Pluto, giving us science writers some new pics to use instead of the same half dozen blurry dots and artist’s conceptions. SpaceX will also attempt a daring landing on a sea platform, and long duration missions aboard the International Space Station will get underway. And key technology headed to space and on Earth may lead the way to opening up the window of gravitational wave astronomy on the universe. Here’s 10 sure-fire bets to watch for in the coming year from Universe Today:
LISA Pathfinder deployed at L1. Credit: ESA/Artist’s concept.
10. LISA Pathfinder
A precursor to a full-fledged gravitational wave detector in space, LISA Pathfinder will be launching atop a Vega rocket from Kourou, French Guiana in July 2015. LISA stands for the Laser Interferometer Space Antenna, and the Pathfinder mission will journey to the L1 Lagrange point between the Earth and the Sun to test key technologies. LISA Pathfinder will pave the way for the full fledged LISA space platform, a series of three free flying spacecraft proposed for launch in the 2030s.
Looking down one of the arms of LIGO Hanford. Credit: Photo by author.
9. AdLIGO Goes Online
And speaking of gravitational waves, we may finally get the first direct detection of the same in 2015, when Advanced LIGO is set to go online. Comprised of two L-shaped detectors, one based in Livingston Louisiana, and another in Hanford Washington, AdLIGO will feature ten times the sensitivity of the original LIGO observatory. In fact, as was the case of the hunt for the Higgs-Boson by CERN, a non-detection of gravitational waves by AdLIGO would be a much stranger result!
A replica of the Hubble Space Telescope on display at the Kennedy Space Center. Credit: Photo by author.
8. Hubble Turns 25
Launched on April 24th, 1990 aboard the Space Shuttle Discovery, the Hubble Space Telescope celebrates 25 years in space in 2015. The final servicing mission in 2009 gave Hubble a reprieve from the space junk scrap heap, and the orbiting telescope is still going strong. Hubble has no less than pushed the limits in modern astronomy to become a modern icon of the space age.
MESSENGER wraps up its mission in 2015. Credit: NASA/MESSENGER/JPL/APL.
7. The End of MESSENGER
NASA’s Mercury exploring spacecraft wraps up its mission next year. Launched in 2004, MESSENGER arrived in orbit around Mercury after a series of flybys on March 18th, 2011. MESSENGER has mapped the innermost world in detail, and studied the space environment and geology of Mercury. In late March 2015, MESSENGER will achieve one final first, when it impacts the surface of Mercury at the end of its extended mission.
Akatsuki on Earth prior to departure. Credit: JAXA.
6. Akatsuki at Venus
This Japanese spacecraft missed orbital insertion a few years back, but gets a second chance at life in 2015. Launched in 2010 atop an H-IIA rocket from the Tanegashima Space Center in Japan, Akatsuki failed to enter orbit around Venus at the end of 2010, and instead headed out for a heliocentric path around the Sun. Some quick thinking by JAXA engineers led to a plan to attempt to place Akatsuki in Venusian orbit in November 2015. This would be a first for the Japanese space agency, as attempts by JAXA at placing a spacecraft in orbit around another planet – including the Mars Nozomi probe – have thus far failed.
The target for the Falcon-9 first stage later next week. Credit: SpaceX.
5. SpaceX to Attempt to Land on a Sea Platform
It’ll definitely rock if they pull it off next week: on January 6th, a SpaceX Falcon 9 rocket will lift off from Cape Canaveral with its Dragon spacecraft headed to the International Space Station on mission CRS-5. Sure, these resupply missions are becoming routine, but after liftoff, SpaceX is attempting something new and daring: landing the Falcon-9 first stage Buck Rodgers style, “fins first” on a floating barge. This is the next step in ultimately proving the feasibility of having the rocket fly back to the launch site for eventual reuse. If nothing else, expect some stunning video of the attempt soon!
An artist’s concept of an asteroid retrieval mission. Credit: NASA.
4. NASA to Decide on an Asteroid Mission
Some major decisions as to the fate and the future of manned space exploration are due next year, as NASA is expected to decide on the course of action for its Asteroid Redirect Mission. The current timeline calls for the test of the SLS rocket in 2018, and the launch of a spacecraft to recover an asteroid and place it in orbit around the Moon in 2019. If all goes according to plan – a plan which could always shift with the political winds and future changes in administrations – we could see astronauts exploring a captured asteroid by the early 2020s.
Astronaut Scott Kelly (left), and cosmonaut Mikhail Korniyenko. Credit: NASA/Roscomos.
3. Long Duration ISS Missions
Beginning in 2015, astronauts and cosmonauts will begin year-long stays aboard the ISS to study the effects of long duration space missions. In March of 2015, cosmonaut Mikhail Korniyenko and U.S. astronaut Scott Kelly will launch as part of Expedition 43 headed to the ISS. The Russians have conducted stays in space longer than a year aboard the Mir space station, but Kelly’s stay aboard the ISS will set a duration record for NASA astronauts. Perhaps, a simulated “Mars mission” aboard the ISS could be possible in the coming years?
An artist’s concept of Dawn approaching 1 Ceres. Credit: NASA/JPL.
2. Dawn at Ceres
Fresh off of exploring Vesta, NASA’s Dawn spacecraft will become the first mission to enter orbit around a second object, the asteroid 1 Ceres next year in April 2015. The largest asteroid and the first object of its kind discovered on the first day of the 19th century, Ceres looks to be a fascinating world in its own right. Does it possess water ice? Active geology? Moons of its own? If Dawn’s performance at Vesta was any indication, we’re in for another exhilarating round of space exploration!
And artist’s conception of New Horizons at Pluto. Credit: NASA/JPL/Thierry Lombry.
1. New Horizons at Pluto
An easy No. 1,we finally get our first good look at Pluto in July, as NASA’s New Horizons spacecraft flies less than 14,000 kilometres from the surface of the distant world. Launched in 2006, New Horizons will “thread the needle” between Pluto and Charon in a flurry of activity as it passes by. New Horizons will then turn back as it passes into the shadows of Pluto and Charon and actually view the two worlds as they occult the distant Sun. And from there, New Horizons will head out to explore Kuiper Belt Objects of opportunity.
And these are just the top stories that are slated to be big news in space in 2015. Remember, another Chelyabinsk meteor or the next big comet could drop by at any time… space news can be unpredictable, and its doubtless that 2015 will have lots more surprises in store.
Close-up view of a raindrop falling on a granular surface, which produces effects similar to an asteroid collision (but on a much smaller scale). Credit: Xiang Cheng, University of Minnesota et al./APS Physics/YouTube (screenshot)
It’s hard to study what an asteroid impact does real-time as you’d need to be looking at the right spot at the right time. So simulations are often the way to go. Here’s a fun idea captured on video — throwing drops of water on to granular particles, similar to what you would find on a beach. The results, the researchers say, look surprisingly similar to “crater morphology”.
A quick caution — the similarity isn’t completely perfect. Raindrops are much smaller, and hit the ground at quite a lower speed than you would see an asteroid slam into Earth’s surface. But as the authors explain in a recent abstract, there is enough for them to do high-speed photography and make extrapolations.
Although the mechanism of granular impact cratering by solid spheres is well explored, our knowledge on granular impact cratering by liquid drops is still very limited. Here, by combining high-speed photography with high-precision laser profilometry, we investigate liquid-drop impact dynamics on granular surface and monitor the morphology of resulting impact craters. Surprisingly, we find that despite the enormous energy and length difference, granular impact cratering by liquid drops follows the same energy scaling and reproduces the same crater morphology as that of asteroid impact craters.
There are of course other ways of understanding how craters are formed. A common one is to look at them in “airless” bodies such as the Moon, Vesta or Ceres — and that latter world will be under extensive study in the next year. NASA’s Dawn spacecraft is en route to the dwarf planet right now and will arrive there in 2015 to provide the first high-resolution views of its surface.
Amateurs can even collaborate with professionals in this regard by participating in Cosmoquest, an organization that hosts Moon Mappers, Planet Mappers: Mercury and Asteroid Mappers: Vesta — all examples of bodies in a vacuum with craters on them.
Undated image of a U-2 aircraft on an "operational mission." Credit: Central Intelligence Agency
A single aircraft in the 1950s and 1960s accounted for half of all UFO sightings collected by the Air Force at the time, according to a newly highlighted CIA report. The agency made a coy reference to the report on its Twitter account Monday (Dec. 29): “Reports of unusual activity in the skies in the ’50s? It was us,” the tweet read.
The aircraft was known as the U-2, and was deemed an essential piece of security hardware in an era that had very few satellites. Recall it wasn’t until 1957 that the first satellite was launched — Sputnik, a Soviet one — and it wasn’t until 1958 that the first American one (Explorer 1) followed.
According to the Air Force, the U-2 was a top-secret project completed by Lockheed Skunk Works and Kelly Johnson, and which flew in August 1955. It was used for flying over the Soviet Union (a former republic that now includes Russia and several surrounding countries) starting in the late 1950s. In 1962, the aircraft played a pivotal role in the Cuban Missile Crisis after a U-2 pilot captured photographs of nuclear missiles in that country.
A photograph of a launch pad at the Tyaratam Missile Testing Range in the Soviet Union taken by a U-2 flight. It is now a part of the Baikonur Cosmodrome in Kazakhstan. Credit: Central Intelligence Agency
High-altitude testing of the U-2 soon led to an unexpected side effect — a tremendous increase in reports of unidentified flying objects (UFOs) … Such reports were most prevalent in the early evening hours from pilots of airliners from east to west. When the Sun dropped below the horizon of an airliner flying at 20,000 feet, the plane was in darkness. But, if a U-2 was airborne in the vicinity of the airliner at the same time, its horizon from an altitude of 60,000 feet was considerably more distant, and being so high in the sky, its silver wings would catch and reflect the rays of the Sun.
According to the CIA, the pilots talked about their sightings with the local air traffic controllers and even wrote into the Air Force. This led to the famous Project Blue Book investigation that dealt with UFO sightings. “This enabled the investigators to eliminate the majority of the UFO reports, although they could not reveal to the letter writers the true cause of the UFO sightings,” the CIA report adds.
For more information about Project Blue Book, you can consult this CIA webpage or this mini-library of information at the National Archives. A version of the U-2 still flew as of at least 2005, which you can read more about at this Air Force website.
Rendering showing the location and size of water vapor plumes coming from Europa's south pole. Credit: NASA/ESA/L. Roth/SWRI/University of Cologne
It was about this time last year that Europa really began to excite us again. Following a sci-fi movie about the Jupiter moon, astronomers using the Hubble Space Telescope announced they had found possible water vapor near the icy moon — maybe from geysers erupting from its icy surface. (That is, if the finding was not due to signal noise, which researchers acknowledged at the time.)
As NASA ramped up (distant) plans to get close to Europa again, scientists began plumbing data from the Cassini spacecraft to see if its glance at the moon circa 2001 revealed anything. Turns out that the spacecraft didn’t see any sign of a plume. Which leads to the greater question, what is happening?
Now scientists are scurrying for a second look. Hubble is in the midst of a six-month search of the moon (from afar) to see if any more of the plumes are showing up. Now the theory is that the plumes, if they do exist, would be intermittent — at least, that’s according to the team looking at data from Cassini’s ultraviolet imaging spectograph (UVIS).
Europa (bottom left) in orbit around its planet, Jupiter, as spotted from the Cassini spacecraft in 2000. Credit: NASA/JPL/University of Arizona
“It is certainly still possible that plume activity occurs, but that it is infrequent or the plumes are smaller than we see at Enceladus,” stated co-author Amanda Hendrix, a Cassini UVIS team member with the Planetary Science Institute in Pasadena. “If eruptive activity was occurring at the time of Cassini’s flyby, it was at a level too low to be detectable by UVIS.”
This finding was part of a greater set of observations showing that it’s not really Europa that is contributing plasma (superheated gas) to space — it’s the ultra-volcanic moon Io. And Europa itself is sending out 40 times less oxygen than previously believed to the area surrounding the moon.
“A downward revision in the amount of oxygen Europa pumps into the environment around Jupiter would make it less likely that the moon is regularly venting plumes of water vapor high into orbit, especially at the time the data was acquired,” NASA stated. This would stand in contrast to, say, Saturn’s Enceladus — which Cassini has seen sending plumes high above the moon’s surface.
The findings were presented at the American Geophysical Union meeting earlier this month and also published in the Astrophysical Journal. The research was led by Don Shemansky, a Cassini UVIS team member with Space Environment Technologies.
Image of a gecko foot, whose ability to stick on to surfaces inspired NASA's Jet Propulsion Laboratory to develop a possible space debris snagging system. Credit: Wikimedia Commons
We’ve written extensively about the orbital debris problem here on Universe Today. In a nutshell, just about every time we launch something from Earth there are bits and pieces that are left behind. Screws. Paint flecks. Sometimes bigger pieces from rocket stages, or at worst, dysfunctional satellites.
Added to the list of lasers, magnets, robot hands and other ideas to get space junk out of orbit is a new one from NASA — gecko grippers. Yes, lizard hands. The idea is by using techniques from these animal appendages, we might be able to efficiently snag dead satellites or other debris at low cost.
Space debris is all whizzing above us and puts us at risk for devastating crashes that can create a sort of prison of debris for any spacecraft hoping to fly above the atmosphere. We’ve already had to move the shuttle and International Space Station due to threats, and the fear is as more satellites reach space, the problem will get worse.
Here’s what NASA has to say about the idea, which is led by Aaron Parness, a robotics researcher at the Jet Propulsion Laboratory:
The gripping system … was inspired by geckos, lizards that cling to walls with ease. Geckos’ feet have branching arrays of tiny hairs, the smallest of which are hundreds of times thinner than a human hair. This system of hairs can conform to a rough surface without a lot of force. Although researchers cannot make a perfect replica of the gecko foot, they have put “hair” structures on the adhesive pads of the grippers.
The grippers were put through their paces in a simulated microgravity test in August (recently highlighted on NASA’s website). On a plane that flew parabolas with brief “weightless” periods, the grippers managed to grab on to a 20-pound cube and a 250-pound researcher-plus-spacecraft-material-panels combination.
NASA-funded researchers test “gecko grippers” on a simulated-microgravity flight to see how effective they could be for snagging satellites. Here, a researcher has strapped spacecraft-like panels to his body to perform the test. Credit: NASA/YouTube (screenshot)
The key limitation was researchers actually held on to their invention themselves, but eventually they hope to use a robotic leg or arm to achieve the same purpose. Meanwhile, on the ground, the grippers have been used on dozens of spacecraft surfaces in a vacuum and in temperatures simulating what you’d find in orbit.
There’s no guarantee that the system itself will make it to space, as it’s still in the early stages of testing. But in a statement, Parness said he thinks it’s possible that “our system might one day contribute to a solution.” NASA also said these could be used for small satellites to attach to the space station, but development would need to move quickly in that case. The station is only guaranteed to be in use until 2020, with possible extension to 2024.
The bright supernova (at tick marks) in the galaxy NGC 4666 photographed on December 24, 2014. Credit: Gregor Krannich
A 14th magnitude supernova discovered in the spiral galaxy NGC 4666 earlier this month has recently brightened to 11th magnitude, making it not only the second brightest supernova of the year, but an easy find in an 8-inch or larger telescope. I made a special trip into the cold this morning for a look and saw it with ease in my 10-inch (25-cm) scope at low power at magnitude 11.9.
Before the Moon taints the dawn sky, you may want to bundle up and have a look, too. The charts below will help you get there.
NGC 4666 is also known as the Superwind Galaxy. Home to vigorous star formation, a combination of supernova explosions and strong winds from massive stars in the starburst region drives a vast outflow of gas from the galaxy into space, called a “superwind”. Credit: ESO/J. Dietrich
With the temporary name ASASSN-14lp, this Type Ia supernova was snatched up by the catchy-titled “Assassin Project”, short for Automated Sky Survey for SuperNovae (ASAS-SN)on December 9th. Only 80 million light years from Earth, NGC 4666 is a relatively nearby spiral galaxy famous enough to earn a nickname.
Hot, X-ray emitting gas in NGC 4666 billows around the main galaxy as a superwind seen here as outflows on either side of the optical image. Photo taken with the XMM-Newton telescope. Credit: M. Ehle and ESO
Called the Superwind Galaxy, it’s home to waves of intense star formation thought to be caused by gravitational interactions between it and its neighboring galaxies, including NGC 4668, visible in the lower left corner of the photo above.
Supernovae also play a part in powering the wind which emerges from the galaxy’s central regions like pseudopods on an amoeba. X-ray and radio light show the outflows best. How fitting that a bright supernova should happen to appear at this time. Seeing one of the key players behind the superwind with our own eyes gives us a visceral feel for the nature of its home galaxy.
“Big picture” map showing the location of the galaxy NGC 4666 in Virgo not far from Porrima. The view faces south shortly before the start of dawn in early January. Source: Stellarium
Spectra taken of ASASSN-14lp show it to be a Type Ia object involving the explosive burning of a white dwarf star in a binary system. The Earth-size dwarf packs the gravitational might of a sun-size star and pulls hydrogen gas from the nearby companion down to its surface. Slowly, the dwarf gets heavier and more massive.
When it attains a mass 1.4 times that of the sun, it can no longer support itself. The star suddenly collapses, heats to incredible temperatures and burns up explosively in a runaway fusion reaction. Bang! A supernova.
Detailed map with stars to about magnitude 10. The galaxy is just a little more than a degree northeast of Porrima (Gamma Virginis). Source: Stellarium
Here are a couple maps to help you find the new object. Fortunately, it’s high in the sky just before the start of dawn in the “Y” of Virgo only a degree or so from the 3rd magnitude double star Porrima, also known as Gamma Virginis. Have at it and let us know if you spot the latest superwind-maker.
For more photos and magnitude updates, check out Dave Bishop’s page on the supernova. You can also print a chart with comparison magnitudes by clicking over to the AAVSOand typing in ASASSN-14lp in the “name” box.
