This Rover Could Hunt For Lunar Water And Oxygen In 2018

The RESOLVE rover during a 2012 demonstration at the Kennedy Space Center near Orlando, Fla. Credit: NASA/Dmitri Gerondidakis

In 2018, NASA plans to go prospecting at the moon’s south pole with a rover — possibly, a version of the Canadian one in the picture above. The idea is to look for water and similar substances on the lunar surface, with an eye to learn more about living off the land, so to speak.

Launching anything into space is expensive, so if it’s possible to harvest raw materials off a moon or planetary surface, this could make things a bit cheaper. Specifically, NASA is interested in oxygen, water, silicon and light metals such as aluminum and titanium in the moon’s soil or regolith. (This process is called in situ resource utilization capability.)

“The mission, currently planned to launch in early 2018, will demonstrate extraction of oxygen from lunar regolith to validate in situ resource utilization capability,” said NASA spokesperson Trent Perrotto in an e-mail to Universe Today.

“An essential element of this mission is the ability to travel significant distances on the surface to better understand water distribution in the lunar regolith.”

Building a lunar base might be easier if astronauts could harvest local materials for the construction, and life support in general. Credit: NASA/Pat Rawlings
Building a lunar base might be easier if astronauts could harvest local materials for the construction, and life support in general. Credit: NASA/Pat Rawlings

So that’s the background. Where does the rover stand in this? It would carry a payload called RESOLVE (the acronym stands for Regolith & Environment Science, and Oxygen & Lunar Volatile Extraction.) And the rover has already been through some field tests to see how well it performs in environments (fairly) similar to the moon.

In 2009, for example, the Canadian Space Agency did a summer field study with NASA, Perrotto said. “The Canadian rover carried the RESOLVE payload during field tests. The tests helped NASA better understand the requirements of a volatiles-sensing payload, and helped CSA understand tele-operation and rough terrain exploration,” he wrote.

At the time, NASA was working to get the payload ready for flight status in 2011, but the mission design has changed since then. The current design (called Resource Prospector Mission) would have RESOLVE, a Canadian Space Agency rover and drill, and a lander. NASA is now looking for somebody to work on the lander.

The RESOLVE payload and Canadian rover during field testing at the Kennedy Space Center near Orlando, Fla. in 2012. Credit: NASA/Dmitri Gerondidakis
The RESOLVE payload and Canadian rover during field testing at the Kennedy Space Center near Orlando, Fla. in 2012. Credit: NASA/Dmitri Gerondidakis

“A request for information was released in July to identify industry interest in a partnership to develop the lander; and an announcement of opportunity is anticipated to be released in early December,” Perrotto wrote.

This mission design is not a guarantee yet. For one thing, NASA is looking at rover alternatives and possibly getting a drill from a United States source instead. It also would depend on funding and agency priorities in the next few years. That said, however, the mission concept is proceeding right now.

In September, Perrotto added, the CSA and NASA did “initial RESOLVE thermal and vacuum testing in September, including a test in [a] regolith-filled vacuum chamber at the NASA Glenn Research Center (GRC) at lunar temperatures and pressures.” RPM passed a mission concept review on Sept. 17 and is in the midst of a preliminary design review that would conclude in fall 2014.

NASA’s Advanced Exploration Systems office has started to look at alternative options to understand “technical constraints by the mission and to assess affordability,” Perrotto added. Meanwhile, the payload team is assessing and looking to reduce risks, while the CSA and NASA are working to “refine technologies for ISRU.”

Representatives from the Canadian team also discussed the rover concept at the Canadian Space Society annual conference in Ottawa, Canada earlier this month. More information on RESOLVE is available on the CSA website; last year, the agency unveiled several rovers it developed for moon and Mars exploration.

A Self-Healing Satellite? Students Seek Your Funds To Launch Prototype

GPS Satellite
According to a new proposal, GPS satellites may be the key to finding dark matter. Credit: NASA

Imagine if your spacecraft was punctured and it could do the repair itself, without the need of you going outside on a dangerous spacewalk. Well, a Canadian team has a prototype idea that could lead to self-healing structures in space. The concept is all set, and they’re asking for financial help to launch it on crowdsourcing platform Kickstarter.

Here’s how the Concordia University material would work:

– It’s constructed out of carbon fiber (to reinforce it) and an epoxy resin (for its matrix).

– After the structure is damaged, it would “transport … a healing agent” to that area using microcapsules that are inside various spots on the resin.

– The structure then chemically repairs itself (more technical details here.)

“This self-healing material is of high interest within the aerospace community such as the Canadian Space Agency and the European Space Agency. If viable, it would be capable of increasing the lifetime of space structures,” the team stated on the fundraising page.

“Prolonging the life of a spacecraft will decrease the required maintenance over its lifetime, which is impossible in many cases. For example, the ammonia leak that happened on the International Space Station (ISS) in May was probably caused by a micrometeoroid and orbital debris (MMOD) impact. If a self-healing shield is implemented in the ISS, the advantage would be to reduce the amount of manual repairs needed on the exterior of the craft and generally improve its lifespan in orbit. This would allow for an overall cost reduction for the spacecraft.”

The engineering team (which calls itself Space Concordia) won the first Canadian Satellite Design Challenge and plans to launch the satellite from that challenge, ConSat-1, as part of a European Space Agency program. (The team did not disclose a launch date on Kickstarter, but said the project is “currently in the final stages of completion.”) This self-healing satellite would be called ConSat-2.

You can read more details about the campaign on their Kickstarter; the campaign concludes Saturday (Nov. 30). The material was developed by Concordia researcher Suong Van Hoa with help from MPB Technologies and the Canadian Space Agency, among others.

Anybody Want A Peanut? New Model Shows Tasty Orbital Shapes In Milky Way’s Bulge

Artist's impression of the Milky Way, looking at it edge on. This makes the bulge at the center look like a peanut, astronomers say. Credit: ESO/NASA/JPL-Caltech/M. Kornmesser/R. Hurt.

Remember that 3-D map of the Milky Way that postulated that the center of the galaxy is shaped like a box or peanut? A new math model of the bulge shows that stars in the center of that bulge move in figure-eight orbits (which can also be interpreted as a peanut-shell shape.) Before, previous studies suggested these orbits looked more like bananas.

“The difference is important; astronomers develop theories of star motions to not only understand how the stars in our galaxy are moving today but also how our galaxy formed and evolves,” the Royal Astronomical Society stated.

In the middle of the galaxy, there are a lot of gravitational forces at play due to the sheer number of stars, as well as particles of dust and dark matter, congregating in the area. This makes it harder to model orbits than in more simple situations, such as our own solar system.

This is how a new model envisions it working:

Milky Way. Image credit: NASA
Milky Way. Image credit: NASA

“As the stars go round in their orbits, they also move above or below the plane of the bar. When stars cross the plane they get a little push, like a child on a swing,” the RAS said.

“At the resonance point, which is a point a certain distance from the center of the bar, the timing of the pushes on the stars is such that this effect is strong enough to make the stars at this point move up higher above the plane. (It is like when a child on the swing has been pushed a little every time and eventually is swinging higher.) These stars are pushed out from the edge of the bulge.”

The researchers suppose that the stars would have two “vertical oscillations” in each orbit, but in between the orbits are shaped somewhat like a peanut shell. This “could give rise to the observed shape of the bulge, which is also like a peanut-shell,” RAS stated.

The research (led by Alice Quillen, an astronomy researcher at the University of Rochester) is available in the Monthly Notices of the Royal Astronomical Society, as well as (in preprint version) on Arxiv.

Source: Royal Astronomical Society

Kepler May Go Planet-Hunting Again! Infographic Shows How That Would Work

Infographic showing how the Kepler space telescope could continue searching for planets despite two busted reaction wheels. Credit: NASA Ames/W Stenzel

The planet-seeking Kepler space telescope had to stop its primary mission this summer after the failure of a second of its four reaction wheels, the devices that keep it pointing at a spot in the constellation Cygnus. NASA, however, has a backup plan. It’s considering stabilizing the spacecraft using the sun! You can see the details in this infographic.

The plan is still preliminary as it needs testing, and it also needs budgetary approval while NASA is fighting to keep other programs going at the funding levels the agency wants. But if it works, this is what NASA is proposing:

  • Keep the spacecraft oriented almost parallel to its orbit around the sun.
  • Gaze at a particular part of the sky for 83 days.
  • When the sun is close to coming into the telescope, move the spacecraft and do another 83-day observation period.
  • This would mean the spacecraft will have 4.5 “unique viewing periods” a year, NASA says.

“With the failure of a second reaction wheel, the spacecraft can no longer precisely point at the mission’s original field of view. The culprit is none other than our own sun,” NASA stated in a recent press release.

Artist's conception of the Kepler Space Telescope. Credit: NASA/JPL-Caltech
Artist’s conception of the Kepler Space Telescope. Credit: NASA/JPL-Caltech

“The very body that provides Kepler with its energy needs also pushes the spacecraft around by the pressure exerted when the photons of sunlight strike the spacecraft. Without a third wheel to help counteract the solar pressure, the spacecraft’s ultra-precise pointing capability cannot be controlled in all directions.”

But this could be a way to counteract it. Mission managers put Kepler through a 30-minute test in October where the telescope looked at a spot in the constellation Sagittarius, which “produced an image quality within five percent of the primary mission image quality,” NASA stated. More testing is underway.

NASA should have more details at the end of this year as to whether to proceed to a 2014 Senior Review, which is held every two years to review current missions and decide which ones are still worth funding.

Source: NASA

Astronauts To Chase Down Turkey Meal For Thanksgiving

NASA astronaut Rick Mastracchio inspects a spacesuit during repairs in the Quest airlock aboard the International Space Station. Taken during Expedition 38 in November 2013. Credit: NASA

Judging from the way those food packets are floating around, looks like the folks on the International Space Station will have to catch their turkey! NASA astronauts Rick Mastracchio and Mike Hopkins, two of the six people working on Expedition 38, recently shared their plans for U.S. Thanksgiving on Thursday.

“Though we miss our families, it’s great to be in space. As astronauts, this is what we train for and this is where we want to be. Opportunities to fly in space are rare, so we have to take advantage of them whenever they occur,” Hopkins said in the message.

The best part of this missive? Watching the astronauts casually toss the microphone back and forth in between their statements. That’s the fun of recording in microgravity.

Thanksgiving will be a full workday on station as the astronauts continue to work on their experiments. A recent status report indicated that Mastracchio (the crew medical officer) was examining Hopkins’ eyes as part of ongoing work looking at how microgravity affects ocular health. Flight controllers also moved one of the solar arrays for Mastracchio to take pictures and monitor how the mast is doing “for future inspections”, NASA stated.

Home Computers Discover Gamma-Ray Pulsars

Gamma-ray pulsars in the Milky Way's plane, found by volunteers using Einstein@Home. The sky map is from Fermi's Large Area Telescope. The brighter the color you see, the more intense the radiation in that spot. The small flags show the nationality of the volunteers whose computers spotted the pulsars. Credit: Knispel/Pletsch/AEI/NASA/DOE/Fermi LAT Collaboration

Imagine that you’re innocently running your computer in pursuit of helping data crunch a huge science project. Then, out of the thousands of machines running the project, yours happens to stumble across a discovery. That’s what happened to several volunteers with Einstein@Home, which seeks pulsars in data from the Fermi Gamma-Ray Space Telescope, among other projects.

“At first I was a bit dumbfounded and thought someone was playing a hoax on me. But after I did some research,” everything checked out. That someone as insignificant as myself could make a difference was amazing,” stated Kentucky resident Thomas M. Jackson, who contributed to the project.

Pulsars, a type of neutron star, are the leftovers of stars that exploded as supernovae. They rotate rapidly, with such precision in their rotation periods that they have sometimes been likened to celestial clocks. Although the discovery is exciting to the eight volunteers because they are the first to find these gamma-ray pulsars as part of a volunteer computing project, the pulsars also have some interesting scientific features.

Artist's illustration of a neutron star, a tiny remnant that remains after its predecessor star explodes. Here, the 12-mile (20-kilometer) sphere is compared with the size of Hannover, Germany. Credit: NASA's Goddard Space Flight Center
Artist’s illustration of a neutron star, a tiny remnant that remains after its predecessor star explodes. Here, the 12-mile (20-kilometer) sphere is compared with the size of Hannover, Germany. Credit: NASA’s Goddard Space Flight Center

The four pulsars were discovered in the plane of the Milky Way in an area that radio telescopes had looked at previously, but weren’t able to find themselves. This means that the pulsars are likely only visible in gamma rays, at least from the vantage point of Earth; the objects emit their radiation in a narrow direction with radio, but a wider stripe with gamma rays. (After the discoveries, astronomers used the Max Planck Institute for Radio Astronomy’s 100-meter Effelsberg radio telescope and the Australian Parkes Observatory to peer at those spots in the sky, and still saw no radio signals.)

Two of the pulsars also “hiccup” or exhibit a pulsar glitch, when the rotation sped up and then fell back to the usual rotation period a few weeks later. Astronomers are still learning more about these glitches, but they do know that most of them happen in young pulsars. All four pulsars are likely between 30,000 and 60,000 years old.

Artist's conception of a gamma-ray pulsar. Gamma rays are shown in purple, and radio radiation in green. Credit: NASA/Fermi/Cruz de Wilde
Artist’s conception of a gamma-ray pulsar. Gamma rays are shown in purple, and radio radiation in green. Credit: NASA/Fermi/Cruz de Wilde

“The first-time discovery of gamma-ray pulsars by Einstein@Home is a milestone – not only for us but also for our project volunteers. It shows that everyone with a computer can contribute to cutting-edge science and make astronomical discoveries,” stated co-author Bruce Allen, principal investigator of Einstein@Home. “I’m hoping that our enthusiasm will inspire more people to help us with making further discoveries.”

Einstein@Home is run jointly by the Center for Gravitation and Cosmology at the University of Wisconsin–Milwaukee and the Albert Einstein Institute in Hannover, Germany. It is funded by the National Science Foundation and the Max Planck Society. As for the volunteers, their names were mentioned in the scientific literature and they also received certificates of discovery for their work.

Source: Max Planck Institute for Gravitational Physics

How Could We Recycle Satellites For Newer Missions?

Artist's conception of ESA's OTS-2 telecom satellite, which was retired from geostationary orbit in 1991 after nearly 13 years of service. Credit: ESA

Space junk is an ongoing concern for NASA, the European Space Agency and many others. After satellites live out their useful lives in orbit, more and more the agencies are trying to either move them far away from Earth, or to have the satellites burn up in the atmosphere. That’s basically to preserve orbital slots around the planet for others, and to reduce the risk of collisions.

But here’s an alternate approach — why not leave a few satellites handy for other missions to pick up? ESA recently opened a tender exploring this idea, and put a few thoughts out in a press release. Maybe leftover solid rocket fuel could be re-used. Metal alloys could be ground down for potential 3-D printing materials. Life support systems could use biodegradable materials. Since it costs so much to haul stuff into orbit, maybe it might be worthwhile to leave some available for future missions, ESA reasons.

Image plot of space junk. Image credit: NASA
Image plot of space junk. Image credit: NASA

“ESA’s new invitation for ‘Sustainable Materials Concepts’ is seeking companies to study various concepts of this approach, including considering the kinds of materials that could be reused as biological or technical nutrients – serving as resources for new other processes,” ESA stated.

“Also under consideration: what sustainable materials might replace current space-grade materials such as titanium and aluminium alloys or carbon-fibre epoxy resins? And how might the use of materials as biological or technical nutrients work in practice?”

What do you think satellites could be used for? Leave your thoughts in the comments.

NASA Plans To Deepen Asteroid Searches With Planetary Resources

An artist's conception of two tidally locked objects orbiting the Sun from afar. The system: 2010 WG9 may likely look like this. Credit: zmescience

Planetary Resources Inc. — that company that is developing a crowdsourced space telescope to search for asteroids — is planning to work on “crowdsourced software solutions” to make it easier to find asteroids and other near-Earth objects, using NASA-funded data.

NASA announced that Planetary Resources will receive a non-reimbursable Space Act Agreement to help NASA characterize near-Earth objects. It’s the first initiative announced under NASA’s Asteroid Grand Challenge, which the agency announced this summer as a vehicle to find threats to Earth.

A contest is planned in 2014 that will also include participation from the Zooniverse’s forthcoming Asteroid Zoo platform (which includes participation from Planetary Resources). Zooniverse is known for providing ordinary people the chance to participate in astronomical searches, including galaxies and asteroid features.

NASA’s role will be to “develop and manage” the contest, while Planetary Resources is expected to “facilitate the use of NASA-funded sky survey data and help support the algorithm competition and review results,” the agency stated.

NASA is trying mightily to move forward with its plans to capture an explore an asteroid in the next few years, but there’s no guarantee that the agency will receive the funds it wants for it in the fiscal 2014 budget. Politicians have expressed concern that the mission is not interesting the public; besides which, the agency is already battling for funds for its commercial crew and planetary science programs, among others.

Source: NASA

‘Will We Soon Find Ourselves Back In The Stone Age?’ Why Swarm Is Watching Our Magnetic Field

Artist's conception of the Swarm satellites during launch. Credit: ESA–P. Carril, 2013

A satellite triplet was born last week. The European Space Agency’s Swarm constellation flew into space on Friday (Nov. 22) on a quest to understand more about the Earth’s magnetic field.

Around the same time, ESA put out a few videos explaining why the magnetic field is important. This one explains that the magnetic field has weakened over the past few years, while the north pole has shifted direction. “In fact, a whole pole reversal is possible,” the narrator says. “It happened last 780,000 years ago at the very beginning of human history. But cavemen didn’t have mobile phone networks, GPS networks or power supplies.”

If a reversal did happen, it could affect those systems, the video adds, asking “Will we soon find ourselves back in the stone age?”

In the short term, however, the focus is on Swarm’s science. The satellites successfully unfurled their booms on Saturday (Nov. 23) and are now starting three months of commissioning before their planned four-year mission.

Once they get going, the satellites will make observations from two altitudes — a pair at about 285 miles (460 kilometers) in altitude and the final of the trio at a higher altitude of 330 miles (530 kilometers). They will monitor any changes in the Earth’s magnetic field, looking at spots ranging from the core of our planet to areas of the upper atmosphere.

Check out this ESA web page for more information about the mission.

Speedy Science: Here’s Four Years Of Herschel Telescope Work In A Short Video

ESA's Herschel telescope used liquid helium to keep cool while it observed heat from the early Universe. Credit: ESA

In just one minute, you can watch the Herschel space telescope painting the sky blue, green and yellow! The colors in this new video represent four years of observations from the European Space Agency telescope, which was active between 2009 and 2013.

“In total, Herschel observed almost a tenth of the entire sky for over 23,500 hours, providing new views into the previously hidden universe, pointing to unseen star birth and galaxy formation, and tracing water through the universe from molecular clouds to newborn stars and to their planet-forming discs and belts of comets,” ESA stated on a video explanation.

As ESA explains, Herschel had two cameras and imaging spectrometers on board, called PACS (Photoconductor Array Camera and Spectrometer, in blue) and SPIRE (Spectral and Photometric Imaging Receiver, in green). When they worked together, their observations are shown in yellow.

Herschel was officially shut down on June 17 — check out the video of those commands here — but the scientific information the telescope produced is still being plumbed by astronomers.

Source: ESA