Detection of water vapour in the spectrum of TW Hydrae's protoplanetary disc. Credits: ESA/NASA/JPL-Caltech/M. Hogerheijde (Leiden Observatory)
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There’s enough water in a planet-forming disk around a distant star to fill several thousand Earth oceans, according to new observations with the Herschel space observatory. Astronomers have found evidence of water vapor originating from ice on dust grains in the disc around a young star, TW Hydrae. The star is between 5-10 million years old, so is in its final stages of formation.
“The detection of water sticking to dust grains throughout the disc would be similar to events in our own Solar System’s evolution, where over millions of years, similar dust grains then coalesced to form comets,” said Michiel Hogerheijde of Leiden University in the Netherlands, who led the study. “These comets we believe became a contributing source of water for the planets.”
But scientists say this latest research from Herschel breaks new ground in understanding water’s role in planet-forming discs and gives scientists a new testing ground for looking at how water came to our own planet.
“With Herschel we can follow the trail of water through all the steps of star and planet formation,” said Göran Pilbratt, Herschel Project Scientist at ESA.
Scientists think the water vapor signature is produced when the ice coated dust grains are warmed by interstellar UV radiation.
Artist concept of a settlement on the Moon. Credit: NASA/Pat Rawlings
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It’s long been a dream to have a human settlement on the Moon, but in this age of budget cuts and indecisive plans for NASA’s future, a Moon base may seem too costly and beyond our reach. However, noted lunar scientist Dr. Paul Spudis from the Lunar and Planetary Institute and a colleague, Tony Lavoie from the Marshall Space Flight Center, have come up with a plan for building a lunar settlement that is not only affordable but sustainable. It creates a Moon base along with a type of ‘transcontinental railroad’ in space which opens up cislunar space – the area between Earth and the Moon – for development.
“The ultimate goal in space is to be able to go anywhere, anytime with as much capability as we need,” Spudis told Universe Today. “This plan uses a robotic and human presence on the Moon to use the local resources to create a new spacefaring system. The key for doing this is to adopt a flexible approach that is incremental and cumulative.”
In a nutshell what Spudis proposes is to send robots to the Moon which are tele-operated from Earth to start extracting water from the polar deposits to create propellant. The propellant would be used to fuel a reusable space transportation system between the Earth and the Moon.
“The reason this is possible is because the Moon is close – it’s only three light-seconds round trip for radio signal get from Earth to the Moon back,” Spudis said, “which means you can control machines remotely with operators on the Earth actually doing the activities that an astronaut might do on the Moon.”
A lunar mining facility harvests oxygen from the resource-rich volcanic soil of the eastern Mare Serenitatis.Credit: NASA/Pat Rawlings.
The advantage here is that a large part of the needed infrastructure, such as the mining operation, the processing plants, the development of storage for the water and propellant, is created before people even arrive.
“So what we try to do is to develop an architecture that enables us to, first, do this in small, incremental steps, with each step building upon the next, and the net effect is cumulative over time,”Spudis said. “And finally we are able to bring people to the Moon when we’re ready to actually have them live there. We place an outpost — a habitat — that will be fully operational before the first humans arrive.”
The significant amount of water than has been found on the Moon at the poles makes this plan work.
“We estimate there are many tens of billions of tons of water at both poles,” Spudis said. “What we don’t know in detail is exactly how much water is distributed what physical state it is in, and that’s one of the reasons why the first step in our plan is to send robotic prospectors up there to map the deposits and see how they vary.”
Water is an important resource for humans in space: it supports life for drinking and cooking, it can be broken down into oxygen for breathing, and by combing the oxygen and hydrogen in a fuel cell, electricity can be generated. Water is also a very good shielding material that could protect people from cosmic radiation, so the habitat could be “jacketed” with water.
But the most important use of water is being able to create a powerful chemical rocket propellant by using the oxygen and hydrogen and freezing them into a liquid.
“The Moon offers us this water not only to support human life there, but also to make rocket propellant to allow us to refuel our spacecraft both on the Moon and space above the Moon.”
In a series of 17 incremental missions, a human base would be built, made operational and occupied. It starts with setting up communication and navigation satellites around the Moon to enable precision operation for the robotic systems.
Next would sending rover to the Moon, perhaps a variant of the MER rovers that are currently exploring Mars, to prospect the best places for water at the lunar poles. The poles also provide areas of permanent sunlight to generate electrical power.
Next, larger equipment would be sent to experiment with digging up the ice deposits, melting the ice and storing the products. (See our previous article about using bulldozers on the Moon).
“Now, all those are simple conceptually, but we’ve never done them in practice,” said Spudis, “so we don’t know how difficult it is. But by sending the small robotic missions to the Moon and practicing this via remote control from Earth, we can evaluate how difficult it is — where the chokepoints are — and what are the most efficient ways to get to these deposits and to extract usable a product from them.”
The next step is to increase the magnitude of the effort by landing bigger robotic machines that can actually start making product on industrial scales so that a depot of supplies can be stockpiled on the Moon for when the first human humans to return to the Moon.
Cislunar space. Graphic courtesy Paul Spudis.
In the meantime, a constant transportation system between Earth and Moon would be created, with another system that goes between the Moon and lunar orbit, which opens up all kinds of possibilities.
“The analogy I like to make is this is very similar to the Transcontinental Railroad,” Spudis said. “We didn’t just build the Transcontinental Railroad to from the East Coast directly to the West Coast; we also built it to access all the points in between, which consequently were developed economically as well.”
By having a system where the vehicles are refueled from the resources extracted on the Moon, a system is created that routinely accesses the Moon and allows for returning to Earth, but all the other points in between can be accessed as well.
“We create a transportation system that accesses all those points between Earth and Moon. The significance of that is, much of our satellite assets reside there,” said Spudis, “ for example communication satellites and weather monitoring satellites reside in geosynchronous orbit, (about 36,000 km above the Earth’s equator) and right now we cannot reach that from low Earth orbit. If we have system that can routinely go back and forth to the Moon, we could also go to these high orbits where a lot of commercial and national security assets are.”
Spudis added that a fuel depot could go in various locations, including the L1 LaGrange point which would enable space flight beyond the Moon.
How long will this take?
“We estimate that we can create an entire turn-key lunar outpost on the Moon within about 15 to 16 years, with humans arriving about 10 years after the initial robotic missions go,” Spudis said. “The mining operation would produce about 150 tons of water per year and roughly 100 tons of propellant.
And do any new technologies or hardware have to be built?
“Not really,” said Spudis. “Effectively this plan is possible to achieve right now with existing technology. We don’t have any ‘unobtainium’ or any special magical machine that has to be built. It is all very simple outgrowths of existing equipment, and many cases you can use the heritage equipment from previous missions.”
And what about the cost?
Spudis estimates that the entire system could be established for an aggregate cost of less than $88 billion, which would be about $5 billion a year, with peak funding of $6.65 billion starting in Year 11. This total cost includes development of a Shuttle-derived 70 mT launch vehicle, two versions of a Crew Exploration Vehicles (LEO and translunar), a reusable lander, cislunar propellant depots and all robotic surface assets, as well as all of the operational costs of mission support for this architecture.
“The best part is that because we have broken our architecture into small chunks, each mission is largely self-contained and once it gets to the Moon it interacts and works with the pieces that are already there,” Spudis said.
And the budget would be flexible.
“We can do this project at whatever speed the resources permit,” Spudis said. “So if you have a very constrained budget with very low levels of expenditure, you can go you just go much more slowly. If you have more resources available you can increase the speed and increase the rate of asset emplacement on the Moon and do more in a shorter period of time. This architecture gets us back to the Moon and creates real capability. But the free variable is schedule, not money.”
Artist concept of a Moon base. Credit: NASA/Pat Rawlings.
Returning to the Moon is important, Spudis believes, because not only can we use the resources there, but it teaches us how to be a spacefaring civilization.
“By going to the Moon we can learn how to extract what we need in space from what we find in space,” he said. “Fundamentally that is a skill that any spacefaring civilization has to master. If you can learn to do that, you’ve got a skill that will allow you to go to Mars and beyond.”
This latest video rendering from from Analytical Graphics, Inc. (AGI) shows ROSAT’s current orbit, the satellite’s ground track, and the estimated model of the break-up and debris scattering. Deutsches Zentrum für Luft- und Raumfahrt (DLR), the German Space Agency has now refined the re-entry to sometime between October 22 and 23, 2011, plus or minus one day. DLR says this slot of uncertainty will be reduced as the date of re-entry approaches. However, even one day before re-entry, the estimate will only be accurate to within plus/minus five hours.
The orbit extends from 53 degrees northern and southern latitude, and all areas in that region could be affected by its re-entry. The bulk of the debris will impact near the ground track of the satellite, but larger parts of the satellite, including its 32 inch, 400 kg mirror, could fall to Earth in a 80-kilometer-wide path along the track.
Update: A report from the ROSAT_Renetry Twitter feed posted at 18:00 UT on October 20 said they expect re-entry in 64 hours. “ROSAT orbit 88.58 minutes 196.8 x 201.7 km, Position 26.6S,164.0W alt=203.2km Lit ~Re-entry 64 hours”
We’ll provide more updates as they become available. You can check the DLR ROSAT webpage for more updates.
Soyuz VS01, the first Soyuz flight from Europe’s Spaceport in French Guiana. Credit: ESA
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The first launch of a Russian Soyuz rocket from Europe’s new South American Spaceport in French Guiana has been postponed at least 24 hours due to technical problems. “Following an anomaly detected during fueling of the Soyuz launcher’s third stage, the final countdown has been interrupted,” ESA said in a statement. “Soyuz and its two Galileo IOV satellites, along with the launch facility, have been placed in a safe mode. A new launch date will be announced later today.”
UPDATE: ESA has announced a new launch time for Friday, October 21 at 10:30:26 GMT (6:30 EDT).
The problem was caused by a leak inside a valve. The Galileo system is being launched as a new GPS system, which will provide more than double the coverage and more accurate locations than the current US-provided Global Positioning System.
The launch was originally scheduled for last year, bad weather delayed the construction of the Soyuz launch facility.
A new NOVA show airs tonight (October 19) in the US on public television, called “Finding Life Beyond Earth.” It includes interviews with many big names in planetary science and like any NOVA show, should be excellent. PBS has a great website that goes along with the show, and for those of you that don’t live in the US or get a public television station, PBS usually posts the videos of NOVA shows online later. Above is a trailer for the show. Check your local listings for when it will air; if you miss it first time around, local stations will sometimes re-air the show during the middle of the night!
Remember the amazing night-time timelapse video that James Drake stitched together from space station photos? Well, he’s gone back through the astronaut photographs and create six more videos. They’re shorter… but they’re AMAZING. Daytime, night time, auroras, it’s all there. Check them out.
Glowing ripples in the electromagnetic field of planet Earth.
Six main rocket engines from the Endeavour and Atlantis shuttles. Credit: NASA/Dimitri Gerondidakis
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That’s a lot of power under one roof! For the first time in… well, ever… all fifteen Space Shuttle Main Engines (SSMEs) are together inside NASA’s Engine Shop at Kennedy Space Center. They will be prepped for shipment to Stennis Space Center in Mississippi where they’ll become part of the propulsion used on NASA’s next generation heavy-lift rocket: the Space Launch System.
The engines, built by Pratt & Whitney Rocketdyne, are each 14 feet (4.2 meters) long & 7.5 feet (2.3 meters) in diameter at the end of its nozzle, and weighs approximately 7,000 lbs (3175 kg).
Photo from a test firing of an SSME at the Stennis Space Center in 1981. Credit: NASA.
Each engine is capable of generating a force of nearly 400,000 pounds (lbf) of thrust at liftoff, and consumes 350 gallons (1,340 liters) of fuel per second. They are engineered to burn liquid hydrogen and liquid oxygen, creating exhaust composed primarily of water vapor.
The engines will be incorporated into the Space Launch System (SLS), which is designed to carry the Orion Multi-Purpose Crew Vehicle – also currently in development – as well as serve as backup for commercial and international transportation to the ISS. By utilizing current technology and adapting it for future needs, NASA will be able to make the next leap in human spaceflight and space exploration – while getting the most “bang” out of the taxpayers’ bucks.
“NASA has been making steady progress toward realizing the president’s goal of deep space exploration, while doing so in a more affordable way. We have been driving down the costs on the Space Launch System and Orion contracts by adopting new ways of doing business and project hundreds of millions of dollars of savings each year.”
– NASA Deputy Administrator Lori Garver
Nine of the 15 SSMEs await shipment inside NASA's Engine Shop. Each weighs approximately 7,000 lbs. Credit: NASA.
While it’s sad to see these amazing machines removed from the shuttles, it’s good to know that they still have plenty of life left in them and will soon once again be able to take people into orbit and beyond!
Compare the view of the ROSAT satellite, as seen from Earth on September 23 and October 16, 2011. Credit: Theirry Legault. Used by permission.
I was waiting for this, and I know our readers have been looking forward to seeing astrophotographer Thierry Legault’s images of the ROSAT satellite as it heads towards its uncontrolled re-entry through Earth’s atmosphere to its ultimate demise. Legault took a series of images on October 16, 2011 from France and combined them into a video. The speed of the sequences is accelerated 3 times with regard to real time (30 frames per second vs 10 fps). The distance to observer is 275 km, with the altitude of the satellite at 235 km. Angular speed at culmination: 1.66°/s.
“It looks very steady, no sign of tumbling or flares like UARS,” Legault told Universe Today via Skype.
You can compare it to earlier images taken by Legault on September 23, 2011, below.
Legault said he drove 100s of kilometers in order to capture ROSAT, and had to deal with clouds and fog before successfully imaging the satellite.
The latest prediction put out by the German Space Agency (DLR) has the ROSAT satellite re-entering sometime between October 21 and 24. This is a slightly narrower time window than the last prediction, which lasted until October 25. We’ll keep you posted on when and where the pieces of the satellite might fall. Legault told Universe Today that he is hoping ROSAT will provide some nice fireworks right over his location in France!
The video below, taken by Legault on September 23, 2011 at 04:36 UT shows ROSAT at an altitude of 284 km, with distance to observer at 458 km. Angular speed at culmination: 0.94°/s.
This image from VISTA is a tiny part of the VISTA Variables in the Via Lactea (VVV) survey that is systematically studying the central parts of the Milky Way in infrared light. On the right lies the globular star cluster UKS 1 and on the left lies a much less conspicuous new discovery, VVV CL001 — a previously unknown globular, one of just 160 known globular clusters in the Milky Way at the time of writing. The new globular appears as a faint grouping of stars about 25% of the width of the image from the left edge, and about 60% of the way from bottom to top. Credit: ESO/D. Minniti/VVV Team
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Where there once was 158, there is now more… Globular clusters, that is. Thanks to ESO’s VISTA survey telescope at the Paranal Observatory in Chile, the Via Lactea (VVV) survey has cut through the gas and dust of the Milky Way to reveal the first star cluster that is far beyond our center. But keep your eyes on the prize, because as dazzling as the cluster called UKS 1 is on the right is, the one named VVV CL001 on the left isn’t as easy to spot.
Need more? Then keep on looking, because VVV CL001 isn’t alone. The next victory for VISTA is VVV CL002, which is shown in the image below. What makes it special? It’s quite possible that VVV CL002 is the closest of its type to the center of our galaxy. While you might think discoveries of this type are commonplace, they are actually out of the ordinary. The last was documented in 2010 and it’s only through systematically studying the central parts of the Milky Way in infrared light that new ones turn up. To add even more excitement to the discovery, there is a possibility that VVV CL001 is gravitationally bound to UKS 1, making it a binary pair! However, without further study, this remains unverified.
This image from VISTA is a tiny part of the VISTA Variables in the Via Lactea (VVV) survey that is systematically studying the central parts of the Milky Way in infrared light. In the centre lies the faint newly found globular star cluster, VVV CL002. This previously unknown globular, which appears as an inconspicuous concentration of faint stars near the centre of the picture, lies close to the centre of the Milky Way. Credit: ESO/D. Minniti/VVV Team
Thanks to the hard work of the VVV team led by Dante Minniti (Pontificia Universidad Catolica de Chile) and Philip Lucas (Centre for Astrophysics Research, University of Hertfordshire, UK) we’re able to feast our eyes on even more. About 15,000 light years away on the other side of the Milky Way, they’ve turned up VVV CL003 – an open cluster. Due the intristic faintness of these new objects, it’s a wonder we can see them at all… In any light!
1st Russian Soyuz poised for blastoff from Europe’s Spaceport in South America. Soyuz VS01, the first Soyuz flight from Europe’s Spaceport in French Guiana is scheduled to liftoff on 20 October 2011. Credit: ESA - S. Corvaja
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A Russian Soyuz-2 rocket sits poised for its first ever blast off in less than 24 hours from a brand new launch pad built in the jungles of French Guiana, South America by the European Space Agency (ESA) .
The payload for the debut liftoff of the Soyuz ST-B booster consists of the first pair of operational Galilieo satellites, critical to Europe’s hopes for building an independent GPS navigation system in orbit.
Soyuz VS01, the first Soyuz flight from Europe’s Spaceport in French Guiana, will lift off on 20 October 2011. The rocket will carry the first two satellites of Europe’s Galileo navigation system into orbit. Credit:ESA - S. Corvaja
The Soyuz VS01 mission is set to soar on Thursday, Oct. 20 at 6:34 a.m. EDT (1034 GMT ) from Europe’s new South American pad, specially built for the Soyuz rocket. The three stage rocket was rolled out 600 meters horizontally to the launch pad and vertically raised to its launch position.
Soyuz VS01 on launch pad. Soyuz VS01vehicle was rolled out horizontally on its erector from the preparation building to the launch zone and then raised into the vertical position. The ‘Upper Composite’, comprising the Fregat upper stage, payload and fairing, was also transferred and added onto the vehicle from above, completing the very first Soyuz on its launch pad at Europe’s Spaceport. Soyuz VS01 will lift off on 20 October 2011. The rocket will carry the first two satellites of Europe’s Galileo navigation system into orbit. Credit: ESA - S. Corvaja
The two Galileo satellites were mated to the Fregat-MT upper stage, enclosed inside their payload fairing and then hoisted atop the Soyuz rocket. They should seperate from the upper stage about 3.5 hous after launch.
Because French Guiana is so close to the equator, the Soyuz gains a significant boost in performance from 1.7 tons to 3 tons due to the Earth’s greater spin.
This marks the first time in history that the renowned Soyuz workhorse will blast off from outside of Kazakhstan or Russia and also the start of orbital construction of Europe’s constellation of 30 Gallileo satellites.
28 more of the navigation satellites, built by the EADS consortium based in Germany, will be lofted starting in 2012 aboard the medium class Soyuz rockets.
French Guiana is already home to Europe’s venerable Ariane rocket family and will soon expand further to include the new Vega rocket for smaller class satellites.
ESA will begin live streaming coverage starting about an hour before the planned launch time of 6:34 a.m. EDT (1034 GMT)
Soyuz VS01 poised for launch on Oct. 20, 2011. Credit: ESA - S. Corvaja
