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10 June 2009

The End of Kayuga



Japan's Lunar Probe Kayuga (Selene) is set to execute the final part of it's mission:

Crashing into the surface of the Moon. Kayuga's orbit is decaying and set to intersect the lunar surface. The crash should take place at a speed of about 6000 km/hr on today 10 June around 1830 UMT (2:30 PM EST). If the Moon is visible at that time (East Asia & Australia), keep your eyes pointed towards the southeastern limb of the Moon. If the 2600 kg probe's crash and resultant explosion are going to be visible, that's where it will be.



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09 June 2009

Lawmakers Slash NASA Budget Request


Especially worrying since everyone else is stepping up in the manned spaceflight department - China even has a Mars probe in the pipeline for later this year.

From Space.com:

Move called a ‘time-out’ as White House awaits review of post-shuttle plans.

WASHINGTON - In a move that reflects the uncertainty surrounding NASA's current strategy for replacing the space shuttle and returning astronauts to the moon by 2020, House appropriators slashed by 16 percent the space agency's $4 billion request for manned space exploration in 2010.




The proposed legislation, marked up June 4 by the House Appropriations commerce, justice, science subcommittee, trims $483 million overall from U.S. President Barack Obama's $18.7 billion budget request for NASA next year. The $670 million cut to the 2010 manned exploration request would leave $3.21 billion, which is less than is available for the effort this year.

Rep. Alan Mollohan (D-W.Va.), the subcommittee's chairman, described the move as a "time-out" in the budget process as the White House awaits the findings of a 10-member panel tasked by the White House to reassess NASA's post-shuttle exploration plans. That panel, led by former Lockheed Martin chief Norm Augustine, is expected to report back with its findings in August.



In his opening statement at the markup hearing, Mollohan said the cut should not be viewed as a diminution of the subcommittee's support for NASA's human spaceflight activities. "Rather, it's a deferral taken without prejudice; it is a pause, a time-out, to allow the president to establish his vision for human space exploration and to commit to realistic future funding levels to realize this vision."

Mollohan told Space News June 4 he is "open to responding to an amended budget request" based on Augustine's review. Mollohan also said he expects the Obama administration to deliver to Congress a "realistic and sustainable" cost assessment of NASA's human spaceflight program in time to amend the 2010 request.

"We invite this report and the administration's response to it, whatever it is," Mollohan said. "We want very much for the funding to be an honest and realistic cost assessment."

Concerns raised
NASA's current human spaceflight plan calls for retiring the space shuttle in 2010 and replacing it with a crew capsule dubbed Orion that would be launched atop a shuttle-derived rocket, the Ares-1, starting in 2015. At the president's request, Augustine's panel is taking a second look at this plan, along with NASA's strategy for returning astronauts to the Moon by 2020, given the likely available budgets over the next several years.

During the hearing, key Republicans expressed concern that the bill would hold NASA's funding next year to 2009 levels. In a June 4 statement Rep. Robert Aderholt (R-Ala.), said he was joining colleagues "in expressing my strong support for increasing this funding as we continue the Fiscal Year 2010 bill process."

Aderholt specifically named fellow Republican Reps. Jerry Lewis of California, the ranking member of the Appropriations Committee; Frank Wolf of Virginia, the ranking member of the commerce, justice, science subcommittee; and John Culberson of Texas.

Other recommendations contained in the bill include a $77million reduction in NASA's proposed space operations budget, which includes the space shuttle and international space station; a $6 million reduction in science; and a $332 million shift in funds from the Cross Agency Support account to a new budget line-item included in the subcommittee's mark. Dubbed Construction and Environmental Compliance, the new account would be funded at $441 million. Congressional aides said the new line item and accompanying funds are aimed at consolidating NASA's various construction efforts into a single pot of money.

Following the markup, the subcommittee posted on its Web site an exhaustive list of earmarks sought by its members. According to the document, money tapped for NASA earmarks totaled close to $15 million.

While increasing NASA's topline funding figure over 2009, Obama's 2010 funding request included an out-year budget profile for the space agency that is some $3 billion lower than was anticipated at this time last year.

Paul Shawcross, chief of the science and space branch in the White House Office of Management and Budget, said the administration's commitment to NASA was evident in the 2009 stimulus package — which included $1 billion for NASA programs — as well as in its 2010 budget request.

"But after 2010, it's flat to 2013," Shawcross said June 2 during a symposium hosted by the George Washington University here. He attributed the flat funding profile to the recession and anticipated recovery measures. He said the Obama administration is facing a $1.26 trillion deficit in 2010, a figure the president hopes to reduce to about $500 billion by 2014. Consequently, funding for NASA and other discretionary spending will be squeezed in the out-years.

"That fiscal environment is reflected in NASA's topline request," Shawcross said.

Meanwhile, W. Michael Hawes, associate NASA administrator for program analysis and evaluation — who is charged with leading the agency team that will provide technical and analytic support to the Augustine panel — said the blue-ribbon commission's work is under way.

"We're starting to get questions from the panel, and we'll be doing a series of fact-finding telecons, site visits, public meetings," he told the symposium audience. Hawes said one area on which the panel will focus is the role international cooperation plays in U.S. manned spaceflight. He said the panel would hear from four international space station partners as part of the review process.

Damon Wells, senior policy analyst in the White House Office of Science and Technology Policy, said pursuing international relationships is a key aspect of space policy. "The panel has been explicitly asked to look at international cooperation," Wells told the audience. "It is part of the dialogue."



Hawes told Space News June 2 that the panel would not have time to produce an interim report, though the committee expects to brief the White House on its findings mid-August. The committee's final report is expected at the end of that month. The Augustine panel's first public meeting is slated for June 17.

Other speakers at the symposium questioned whether the Augustine panel has been granted sufficient time to do its work.

Marcia Smith, president of the Space and Technology Policy Group, a consultancy here, said the Augustine panel would provide little more than a snapshot in time given its deadline.

"Not everyone agrees on the mandated timing," she said. "Congress, in particular, wants it not to be constrained."

Jeffery Bingham, a member of the Senate Commerce, Science and Transportation Committee's Republican staff and senior adviser on space and aeronautics, agreed.

"I am worried about the time they have, and the resources they have," he told the audience. "It's going to be dicey."

Bingham expressed concern that Augustine was told to limit the options his panel is to present to the administration.

"We think it prejudges the outcome," he said. "We want to see that it is wide open and that all options are on the table."

Richard Obermann, staff director for the House Science and Technology space and aeronautics subcommittee, said lawmakers are encouraged by the additional funds for NASA programs in the 2009 stimulus package and the 2010 budget request. But Obermann expressed "uncertainty with the new administration's intentions," particularly in the out-years, where NASA's topline funding is flat.

Oberman said increases in other parts of NASA's budget, including aeronautics and Earth science, came at the expense of out-year funding for space exploration. Obermann said he sees NASA's current funding projections for 2010-2014 as a placeholder, and that he expects the Augustine panel's review to influence funding for the space agency's exploration programs in the out-year timeframe. Obermann said he was encouraged by the choice of Augustine to lead the human spaceflight review, noting testimony Augustine gave before the House Science and Technology Committee in 2004, shortly after former President George W. Bush announced plans to replace the space shuttle and return astronauts to the Moon.

At that time Augustine said manned space exploration offered many benefits, but that "it would be a grave mistake to try to pursue a space program on the cheap. To do so is in my opinion an invitation to disaster. There is a tendency in any can-do organization to believe that it can operate with almost any budget that is made available. The fact is that trying to do so is a mistake — particularly when safety is a major consideration."



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10 April 2009

The Search for the Moon's Mother





NASA launches the twin STEREO probes in search of remnants of the collision that produced the Moon.


Some scientists believe that the Moon was created when the Earth was hit by a Mars sized object. Theia was conceieved by Edward Belbruno and Richard Gott if Princeton. The Theia Hypothesis is a subset of the Great Impact Theory of lunar formation. Belbruno and Gott believe that the impactor that hit the Earth 4.5 billion years ago came from one the Earth-Sun Langrangian points. Langrangian points are the five places where the gravitational pull of two bodies cancels each other out.



Most people are familiar with Jupiter's Trojan points and the asteroids that reside there. Earth and the Moon also share Lagrangian points. NASA's STEREO probes are going to the two most stable Lagrangian points belonging the Earth-Sun system, L4 and L5. Part of STEREO's mission is to look for planetoids leftover form the formation of Theia. STEREO is primarily a solar observatory mission, similar to the NASA/ESA stalwart SOHO. SOHO has been in orbit around the Sun-Earth L1 Langrangian point since 1996. The STEREO will be passing through the Sun-Earth L4 and L5 points, which are 60 degrees ahead and behind of Earth in its orbit, and they will continue on their paths past both sides of the Sun.



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25 February 2009

Skylon contact on DRADIS



On the single stage to orbit (SSTO) development front, British scientist Alan Bond, formerly of the HOTOL concept and now classified RB545 air-breathing rocket engine that was to be mated to the HOTOL, has gotten go-ahead funding from the European Space Agency (ESA) and the government of the United Kingdom to the tune of a million euros.



Bond's company - Reaction Engines LTD - designed the Skylon SSTO as the spiritual successor to the British HOTOL, which was to be Great Britain's answer to the Space Shuttle. The cancellation of HOTOL was due to design issues stemming from the placement of the the RB545 engines.



With its massive engines placed at the rear of the craft, HOTOL's center of gravity was further back than normal airplane designs and it introduced some stability issues. A redesign of the spacecraft reduced the cargo capability of the HOTOL and affected the economics of the launch system. Skylon is the answer to the design issues of the HOTOL.



Placing the new SABRE engines outboard on wings moves the the center of gravity back to the middle of the spacecraft, giving ideal stability and cargo room, as the engines are no longer taking up space in the the main body of the spacecraft. Skylon is big - 82 m long, 6.3 m in diameter and a 25 m wingspan. Its dry weight is estimated at 41,000 kg and can carry 12,000 kg of payload. The heart of the system are the SABRE engines.



On Skylon, the oxidizer used is liquid oxygen (LOX). LOX is very heavy and for a standard hydrogen oxygen reaction, you need two oxygen atoms at 8 times the weight each of hydrogen for every hydrogen atom burned. For comparison, the Space Shuttle carries 106,000 kg of hydrogen at liftoff and 630,000 kg of LOX. 85% percent of the Space Shuttle's fuel weight is oxidizer. The good people at Reaction Engines LTD decided that carrying their own LOX was crazy when Skylon would be flying through it on its way up. The SABRE engine harvests oxidizer from the atmosphere during flight.

The SABRE engine is essentially a closed cycle rocket engine with an additional precooled turbo-compressor to provide a high pressure air supply to the combustion chamber. This allows operation from zero forward speed on the runway and up to Mach 5.5 in air breathing mode during ascent. As the air density falls with altitude the engine eventually switches to a pure rocket propelling Skylon to orbital velocity (around Mach 25).



From Wikipedia:

style="font-weight: bold;">The Precooleran>

As the air enters the engine at supersonic/hypersonic speeds, it becomes very hot due to compression effects. The high temperatures are traditionally dealt with in jet engines by using heavy copper or nickel based materials, and by throttling back the engine at the higher airspeeds to avoid melting. However, for an lass="blsp-spelling-error" id="SPELLING_ERROR_20">SSTO craft, such heavy materials are unusable, and maximum thrust is necessary for orbital insertion at the earliest time to minimise gravity losses. Instead, using a gaseous helium coolant loop, SABRE dramatically cools the air from 1000 °C down to -140 °C in a heat exchanger while avoiding liquefaction of the air or blockage from freezing water vapour.

Previous versions of precoolers such as HOTOL put the hydrogen fuel directly through the precooler, but inserting a helium cooling loop between the air and the cold fuel avoids problems with hydrogen embrittlement in the air precooler.

Avoiding liquification improves the efficiency of the engine since less liquid hydrogen is boiled off; even simply cooling the air needs more liquid hydrogen than can be burnt in the engine core, the excess is dumped overboard (through a ramjet.)

However, the dramatic cooling of the air raised a potential problem: it is necessary to prevent blocking the precooler from frozen water vapour and other fractions. A suitable precooler, which rejects condensed water before it freezes has now been experimentally demonstrated.


The Compressor

The cooled air is then passed into a reasonably conventional turbo-compressor, similar in design to those used on a jet engine, but in this case powered by a gas turbine running on the helium loop, rather than off combustion gases as in a conventional jet engine. Thus, the turbo-compressor is powered by waste heat collected by the helium loop.

The Engines

After being launched and brought to speed by a short burst of the rockets, the jets are started, fed by air bled from the shock cone. At this point the precooler/turbo-compressor is not being used. As the craft ascends and the outside air pressure drops, more and more air is passed into the compressor as the effectiveness of the ram compression alone drops. In this fashion the jets are able to operate to a much higher altitude than would normally be possible.

At Mach 5.5 the jets become inefficient and are powered down, and stored liquid oxygen/liquid hydrogen is used for the rest of the ascent in the separate rocket engines; the turbopumps are powered by the helium loop from the heat produced by cooling the engine.

The Helium Loop

The 'hot' helium from the air precooler, and cooling the combustion chambers is recycled by cooling it in a heat exchanger with the liquid hydrogen fuel.

The loop forms a self starting Brayton cycle engine, and is used to both cool critical parts of the engine, but also to power turbines and numerous miscellaneous parts of the engine.

The heat passes from the air into the helium. This heat energy is not entirely wasted, it is in fact used to power the various parts of the engine, and the remainder is used to vaporise hydrogen, which is burnt in ramjets.

Performance

The designed thrust/weight ratio of SABRE ends up several times higher—up to 14, compared to about 5 for conventional jet engines, and just 2 for scramjets. This high performance is a combination of the cooled air being denser and hence requiring less compression, but more importantly, of the low air temperatures permitting lighter alloy to be used in much of the engine. Overall performance is much better than the RB545 engine or scramjets.

The engine gives good fuel efficiency peaking at about 2800 seconds within the atmosphere. Typical all-rocket systems are around 450 at best, and even "typical" nuclear thermal rockets only about 900 seconds.

The combination of high fuel efficiency and low mass engines means that a single stage to orbit approach for Skylon can be employed, with air breathing to mach 5.5+ at 26 km altitude, and with the vehicle reaching orbit with more payload mass per take-off mass than just about any non-nuclear launch vehicle ever proposed.

Like the RB545, the precooler idea adds mass and complexity to the system, normally the antithesis of rocket design. The precooler is also the most aggressive and difficult part of the whole SABRE design. The mass of this heat exchanger is an order of magnitude better than has been achieved previously; however, experimental work has proved that this can be achieved. The experimental heat exchanger has achieved heat exchange of almost 1 GW/m³, believed to be a world record. Small sections of a real precooler now exist.

The losses from carrying around a number of engines that will be turned off for some portion of the flight would appear to be heavy, yet the gains in overall efficiency more than make up for this. These losses are greatly offset by the different flight plan. Conventional launch vehicles such as the Space Shuttle usually start a launch by spending around a minute climbing almost vertically at relatively low speeds; this is inefficient, but optimal for pure-rocket vehicles. In contrast, the SABRE engine permits a much slower, shallower climb, air breathing and using wings to support the vehicle, giving far lower fuel usage before lighting the rockets to do the orbital insertion.



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18 February 2009

Home on Lagrange

--Home on Lagrange (The L5 Song)
© 1978 by William S. Higgins and Barry D. Gehm


CHORUS: Home, home on LaGrange,
Where the space debris always collects,
We possess, so it seems, two of Man's greatest dreams:
Solar power and zero-gee sex.

Oh, give me a locus where the gravitons focus
Where the three-body problem is solved,
Where the microwaves play down at three degrees K,
And the cold virus never evolved. (chorus)
We eat algea pie, our vacuum is high,
Our ball bearings are perfectly round.
Our horizon is curved, our warheads are MIRVed,
And a kilogram weighs half a pound. (chorus)
If we run out of space for our burgeoning race
No more Lebensraum left for the Mensch
When we're ready to start, we can take Mars apart,
If we just find a big enough wrench. (chorus)
I'm sick of this place, it's just McDonald's in space,
And living up here is a bore.
Tell the shiggies, "Don't cry," they can kiss me goodbye
'Cause I'm moving next week to L4! (chorus)





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03 February 2009

Carnival of Space #88 is live


Carnival of Space #88 is live.



Of interest is this link to a electric space drive simulator.

A little history for you here outlining a lunar lander mission proposed right after the 1st anniversary of the Apollo 1 fire.



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26 January 2009

Chandrayaan-1 Takes First X-Rays of the Moon


The C1XS X-ray camera, jointly developed by the UK's STFC Rutherford Appleton Laboratory and the Indian Space Research Organisation (ISRO), has successfully detected its first X-ray signature from the Moon.




Credit: RAL/Brunel


The C1XS camera is a Compact Imaging X-ray Spectrometer that uses x-rays to map the composition of the lunar surface and in doing so, will offer up clues as to the origin of the Moon. The C1XS X-ray spectrometer was constructed at the Rutherford Appleton Laboratory, UK, in collaboration with colleagues at ISRO, who designed and constructed the main Chandrayaan-1 lunar probe. The instrument is a technology development of the D-C1XS instrument which successfully conducted science operations at the Moon aboard ESA's SMART-1 mission between 2003 to 2006.

C1XS will provide high resolution coverage of the lunar surface in X-rays, and will provide an absolute measurement of the elemental abundances of the rock forming elements Mg, Al and Si under normal solar conditions and several other elements during solar flare events. This first measurement was three minutes of observation taken in the vicinity of the Apollo landing sites during a solar flare. The is measurement is also noteworthy because C1XS collected data from a source that was reportedly 20 times below its minimum effective detection threshold.

Geochemical data will allow for advances in several areas of lunar science, including a detailed study of the nature of the crust. In combination with information to be obtained by the other instruments on Chandrayaan-1 and the data already provided by the Smart-1, Clementine and Lunar Prospector missions, this information will provide a more detailed look at some of the fundamental questions that remain regarding the origin and evolution of the Moon.


Credit: ISRO

From: Space Daily



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23 January 2009


Carnival of Space #87 is live.



Of interest is this summary of the recent confirmation of the existence of methane on Mars and what it means to the search for extraterrestrial life.

Even more intriguing is the theory being put forward about the holographic properties of the universe. I don't completely understand it, but it reminds me of something I've seen in sci-fi: One spot in normal space corresponds to another spot in hyperspace, except the distances are shorter in hyperspace. It'll be interesting if this pans out.



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21 January 2009

Lunar rover


Though I missed it live on TV, I understand NASA's new lunar rover made an appearance during the parade. Take a look at those tweels. They were tested here.



NASA's Chariot rover was showing off its 360 degree steering ability for the President and VP. As seen here, the Chariot is in its Small Pressurized Rover configuration. The SPR allows the astronauts to explore the lunar surface without having to wear a full spacesuit.



Here is a link to a video of the Chariot in action.

The Chariot consists of the Mobility chassis and the removable SPR cabin unit. Chariot gives astronauts three options for riding. Without the SPR in suits in rotating turrets is probably the option the system got its name from - Chariot. The next option is to ride without suits inside the SPR - car mode. The final option is a combination of both - the SPR is mounted to the chassis, and astronauts ride in a turret - ideal for transporting large, unstable loads.

The suits are intergated into airlocks called suitports the allow quick ingress/egress with a minimum of air waste.



Chariot masses 1000 kg and has a top speed of 10 kph. It can carry a payload of 3000 kg, which matches the weight of the SPR. It's 4.5 m long, 1.3 m high and has a 4 m wheelbase. The SPR gives Chariot a potential range of 240 km, compared to 10 km for Apollo's rover. In addition, the suitport airlock is rated for 72 hours storm shelter protection from a solar particle event, or solar flare. The lock is lined with 2.5 cm of water ice, one of the best natural radiation shields known.

Download Small Pressurized Rover Fact Sheet (3.7 MB PDF)
http://www.nasa.gov/directorates/esmd/home/black_point.html




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13 January 2009

SpaceX's Falcon 9 on the Pad


SpaceX has completed integration of their Falcon 9 vehicle at Space Launch Complex 40 at Cape Canaveral and have raised it to a vertical position in preparation for a demonstration flight. See pictures below.














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