Ares I-X Manager Addresses Booster Damage, Stage Tumbling and Thrust Oscillation

Divers recover the Ares I-X booster. Credit: NASA, via Spaceflightnow.com

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The damage seen on the Ares I-X booster occurred as a result of parachute failure, which caused the rocket to impact the water harder than expected. Ares I-X manager Bob Ess briefed reporters today on the preliminary data from Wednesday’s test flight of NASA new rocket, and said the parachute failure was not a significant event. “The damage we see is analogous to when there has been parachute failure on the space shuttle boosters, but actually the parachute guys were ecstatic overall and are not worried about it,” Ess said. “This is all part of doing a test flight, so team is still very elated. The fact that the parachute team has something interesting to go work makes them excited. The damage was all collateral because of the parachute.” He also touched on the “tumbling” of the second stage, and their findings on thrust oscillation for the vehicle.

Ess said all three chutes initially deployed as planned: pilot chute, then drogue chutes, then the three main chutes come out and partially deploy to a 50% open condition to avoid shock to the material. But at that point one of the mains failed and basically became a streamer. Ess said it appeared the lines went slack, which would be indicative of a problem with the riser lines and not the parachute material. Then a second chute may have gotten damaged from the bad “streamer” parachute and the second chute didn’t open all the way. So instead of coming down on three parachutes, it only had one and a half. “So that caused the booster to hit the water at a higher speed than expected, with more horizontal velocity, so booster slapped down pretty hard which caused damage on the booster.”

Additionally the booster was 15% heavier than the booster that will be used for Ares 1. “This was an overtest, so it does not detract from the success of the flight,” Ess said.

Image from NASA TV showing the Ares I-X stage separtion.
Image from NASA TV showing the Ares I-X stage separtion.

The tumbling seen as the two stages separated was actually not unexpected and Ess said he misspoke at the press briefing on the day of the test flight as the separation being “interesting” (and his team immediately let him hear about it!). “We’ve actually done thousands of animations showing this type of behavior on the upper stage, and the models predicted this is what we would see. It was the manager who didn’t say it right,” Ess joked.

The upper stage on the test flight was a “dummy” and was loaded with 30,000 pounds of ballast near the bottom to simulate a full load of liquid oxygen rocket propellant and another 30,000 pounds higher up to simulate liquid hydrogen fuel.

The center of gravity was in an unusual spot, making it inherently unstable, so it behaved exactly as a heavy, unstable projectile would. “Once you separate, there’s nothing to control it,” Ess said. “In reality, the Ares I will have the J-2X engine on it, and everything will be fine.”

The much ballyhooed thrust oscillations the vehicle might encounter were basically non-existent on Wednesday’s test flight. “We had two sensors to measure this and so far the oscillations look very small, similar to what the shuttle might encounter,” Ess said. “We didn’t see anything unusual or remotely like anything to indicate that thrust oscillation was a factor.”

Ares I-X.  Credit: NASA/Scott Andrews
Ares I-X. Credit: NASA/Scott Andrews

At Wednesday’s briefing, Ess said the vehicle has three pairs of thrusters to keep things under control if thrust oscillation would become a problem. Their simulations said they might encounter 20-25 firings of the automatic thrusters during flight, but in actuality, there were only three.

“We’re just not seeing any significant numbers for thrust oscillation,” Ess said. “It’s the impact on the vehicle that you worry about, and so far we haven’t seen it but we’ll look closer at the data in the next few weeks.”
The damaged booster contains the flight data recorder, and Ess thought they should get access to it on Saturday and begin looking at the data from over 700 sensors on board the vehicle.

Since test flights are done to bring up major problems, Ess was asked if he wished there were more issues to tackle. “It was a great flight, and the parachute problem is a minor thing, and we have a few more year to go look at it,” he said. “When something is a little different, you get excited, as an engineer. But we were ecstatic and no one is sad we didn’t have any more problems. We still have to look at the sensors, so there’s a lot in front of us. But there’s nothing pride from the team that it went as well as it did.”

Source: NASA press briefing

Bacteria Could Survive in Martian Soil

Certain strains of bacteria, including Bacilus Pumilus, may be able to survive on the Martian surface. Image credit: NASA

Multiple missions have been sent to Mars with the hopes of testing the surface of the planet for life – or the conditions that could create life – on the Red Planet. The question of whether life in the form of bacteria (or something even more exotic!) exists on Mars is hotly debated, and still requires a resolute yes or no. Experiments done right here on Earth that simulate the conditions on Mars and their effects on terrestrial bacteria show that it is entirely possible for certain strains of bacteria to weather the harsh environment of Mars.

A team led by Giuseppe Galletta of the Department of Astronomy at the University of Padova simulated the conditions present on Mars, and then introduced several strains of bacteria into the simulator to record their survival rate. The simulator – named LISA (Laboratorio Italiano Simulazione Ambienti) – reproduced surface conditions on Mars, with temperatures ranging from +23 to -80 degrees Celsius (73 to -112 Fahrenheit), a 95% CO2 atmosphere at low pressures of 6 to 9 millibars, and very strong ultraviolet radiation. The results – some of the strains of bacteria were shown to survive up to 28 hours under these conditions, an amazing feat given that there is nowhere on the surface of the Earth where the temperatures get this low or the ultraviolet radiation is as strong as on Mars.

Two of the strains of bacteria tested – Bacillus pumilus and Bacillus Nealsonii – are both commonly used in laboratory tests of extreme environmental factors and their effects on bacteria because of their ability to produce endospores when stressed. Endospores are internal structures of the bacteria that encapsulate the DNA and part of the cytoplasm in a thick wall, to prevent the DNA from being damaged.

Galletta’s team found that the vegetative cells of the bacteria died after only a few minutes, due to the low water content and high UV radiation. The endospores, however, were able to survive between 4 and 28 hours, even when exposed directly to the UV light. The researchers simulated the dusty surface of Mars by blowing volcanic ash or dust of red iron oxide on the samples. When covered with the dust, the samples showed an even higher percentage of survival, meaning that it’s possible for a hardy bacterial strain to survive underneath the surface of the soil for very long periods of time. The deeper underneath the soil an organism is, the more hospitable the conditions become; water content increases, and the UV radiation is absorbed from the soil above.

Given these findings, and all of the rich data that came in last year from the Phoenix lander – especially the discovery of perchlorates –  continuing the search for life on Mars still seems a plausible endeavor.

Though this surely isn’t a confirmation of life on Mars, it shows that even life that isn’t adapted to the conditions of the planet could potentially hold out against the extreme nature of the environment there, and bodes well for the possibility of Martian bacterial life forms. The LISA simulations also indicate the importance of avoiding cross-contamination of bacteria from Earth to Mars on any scientific missions that travel to the planet. In other words, when we finally are able to definitively test for life on our neighboring planet, we don’t want to find out that our Earth bacteria have killed off all the native lifeforms!

Sources: Arxiv papers here and here.

Northern Spring Approaches on Mars: Will Phoenix Phone Home?

Phoenix landing site in Dec. 2008 and August 2009. Credit: NASA/JPL/ U of Arizona; annotations by Phil Stooke

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I was just thinking of the Phoenix lander earlier this week, wondering if our little buddy was surviving the Martian winter when, boom: via Twitter came this:

@MarsPhoenix “Spring has sprung in the north hemi(sphere) of Mars! Team is waiting for longer daylight hours, around mid-Jan., to ‘listen’ for our lander.”

Then, via another Tweet from @doug_ellison, (Doug Ellision) I found out the folks at Unmannedspaceflight.com have been thinking about the Phoenix lander, too. Phil Stooke from the UMSF crew had searched for Phoenix in the latest images released by the HiRISE camera on board the Mars Reconnaissance Orbiter, taken in August 2009 and found of glimmer of hope the lander was still visible among the CO2 frost and “snow.” See the comparison above of the landing site from Dec. 2008 to August 2009. Then Emily Lakadawalla of the Planetary Society Blog took things one step further and made a little “movie” of HiRISE images of Phoenix during the different seasons on Mars (check out her extensive post here.) Hope springs eternal for many of us as to whether we’ll ever hear from Phoenix again, and time will only tell. But its nice to know there were lots of us with Phoenix on the brain this week; kind of a shared experience! (except everyone else did all the work….) See below for more closeups of Phoenix’s winter surroundings from UMSF.

Phoenix landing site, August, 2009. Credit: NASA/JPL/U of Arizona.  Annotations by Phil Stooke
Phoenix landing site, August, 2009. Credit: NASA/JPL/U of Arizona. Annotations by Phil Stooke

Phil wrote on UMSF that it took him several tries to match up the landing site from the two different HiRISE images. “When the two sides of this comparison are blinked a thousand features match up, not just a dozen. This is a lesson to people searching for Mars Polar lander – it’s easy to be fooled! … The parachute and backshell are invisible, the heatshield almost so, but the lander’s clear.”

And below is one of just the lander from July 2009. Unfortunately, HiRISE has been unable to take any recent images of Phoenix or any other location on Mars because of MRO being in an extended safe mode. It went into safe mode over 9 weeks ago, and mission engineers have yet to determine the cause. They are playing it safe and want to get to the root cause, since this has happened four times over the course of the mission. Latest word reported in the Arizona Star is that if the system reboots itself enough times, the memory of the main computer could be reset, and basically wiped. That would be bad. “Engineers are now working to create a safeguard against that worst-case scenario as well as finding the cause of the mysterious voltage signals,” the Star said.

Phoenix close up from July 2009. Annotated by Phil Stooke.
Phoenix close up from July 2009. Annotated by Phil Stooke.

See all the Mars Phoenix lander images from HiRISE here.

Thanks again Phil at UMSF and Emily at the Planetary Society

Ares I-X Booster Damaged

Buckling on the first stage booster for Ares I-X. Credit: NASA via Spaceflightnow.com

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The booster rocket used in the Ares I-X test flight was found to be badly dented when divers located it in the Atlantic Ocean. The damage could have occurred as the booster hit the water. UPDATE (7:30 pm CDT): Bill Harwood from CBS news is reporting that according to NASA officials, one of the three 150-foot-wide parachutes designed to gently lower NASA’s Ares I-X first stage booster to the Atlantic Ocean deflated after deployment, resulting in a harder splashdown than expected. All three main chutes deployed, but while two inflated fully, the third collapsed. “A source said the deflated parachute contacted one of the others as it whipped about in the wind, causing a partial deflation. That could not be immediately confirmed, although a splashdown in that condition might explain the buckling seen in the lower segment of the rocket’s case,” Harwood wrote. (end of update).

Spaceflightnow.com reported that engineers have said shuttle boosters can be damaged depending on the impact angle and how rough the ocean is. But it’s not yet known whether such a “slap down” or some other issue might have caused the damage noted in the Ares I-X booster.

Divers recover the Ares I-X booster. Credit: NASA, via Spaceflightnow.com
Divers recover the Ares I-X booster. Credit: NASA, via Spaceflightnow.com

Parachute deploy was one of the major test objectives for the flight. The 327-foot-tall I-X rocket was equipped with a four-segment shuttle booster, a fifth segment loaded with avionics gear, a dummy upper stage and Orion crew module mockup.

The booster is being towed back to Kennedy Space Center, and should arrive late Thursday, where engineers will be able to look more closely at the damage.

Additionally, NASA is saying there was more damage to the launchpad following the Ares I-X launch than what is customarily seen after a shuttle launch. Leaks of toxic propellant at launch pad 39B forced NASA to evacuate the pad. Two separate leaks occurred at the 95-foot-level where the pad’s fixed service structure and gantry-like rotating service structure meet.

Meanwhile, on the shuttle side of the program, after a Flight Readiness Review, mission managers for the STS-129 mission have cleared space shuttle Atlantis to launch on Nov. 16 at 2:28 p.m. EST. The target date depends on the planned Nov. 14 launch of an Atlas V rocket from nearby Cape Canaveral Air Force Station. The Atlas has reserved the Eastern Range on Nov. 14 and 15. If the Atlas launch is delayed to Nov. 15, the shuttle’s liftoff will move to no earlier than 2:02 p.m. on Nov. 17.

The STS-129 mission will focus on storing spare hardware on the exterior of the space station. The flight will include three spacewalks and install two platforms on the station’s truss, or backbone. The platforms will hold spare parts to sustain station operations after the shuttle fleet is retired.

Also, the mission will bring up communications equipment for the SpaceX Dragon capsule and future commercial cargo missions to the ISS.

Sources: Spaceflightnow.com, NASA

What’s Next for the Ares Rocket?

Launch day. Photo credit: NASA/Sandra Joseph and Kevin O'Connell

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After Wednesday’s picture perfect launch of the Ares I-X test rocket — which revealed no real showstoppers or issues as of yet for the vehicle — the obvious next question is: now what? Much of what comes next for the Ares program, and Constellation in general, hinges on any decisions the Obama administration and Congress make in regards to NASA’s budget and the options put forth by the Augustine Commission. But if the Ares program is given the green light, here’s an overview of the next steps, future test flights and milestones. First on the list? We won’t hear the word “triboelectrification” ever again.

No more trouble with triboelectrification.

At Wednesday’s press briefing following the launch, program managers said they didn’t realize what a big issue the triboelectrification rule would be. Flying through high-level clouds can generate “P-static” (P for precipitation), which can create a corona of static around the rocket that interferes with radio signals sent by or to the rocket. This would create problems when the rocket tries to transmit data down to the ground or if the Range Safety Officer at Cape Canaveral Air Force Station needed to send a signal to terminate (blow up) the rocket in the event of a problem.

“We can coat the vehicle with something to dissipate the charge, or you certify the vehicle to show it is not sensitive to that effect,” said Bob Ess, Ares I-X mission manager. “We’ve done analysis that our vehicle isn’t sensitive, but we didn’t go and get it certified with the Range. This was a bigger implication to us than we expected.”

Constellation program manager Jeff Hanley said had there been a lengthy delay of the test flight, for whatever reason, they likely would have had the time and opportunity to do the certification. But from now on, Hanley said, all rockets will be certified before launch to avoid the “trouble with triboelectrification.”

In-flight anomaly.

Image from NASA TV showing the Ares I-X stage separtion.
Image from NASA TV showing the Ares I-X stage separtion.

The only initial anomaly during the test flight was some unusual dynamics on the dummy second stage after separation. It went into a flat tumble, and appeared as if it might hit the first stage as it turned. The reason for the tumble wasn’t initially known, and will be of interest to the team as they analyze data from over 700 sensors. “We know all the motors fired, but it might be the aerodynamics,” said Ess, “perhaps a higher aerodynamic pressure than what we expected. It was interesting, and interesting is good. It wasn’t dramatically different from what we expected, though”.

As far as the future, Hanley said the flight test program is constantly under review as far as what budget and schedule allows but here’s the current plan:

Spring 2010: Launch Abort System Test.

Launch abort system. Credit: NASA
Launch abort system. Credit: NASA

The Ares’ Orion crew capsule includes a launch abort system, which is scheduled to undergo the first of three tests early next year. The abort system involves three separate motors to move the capsule away from the rocket and/or launchpad. It will have directional control to separate and jettison the entire launch abort system so the capsule can parachute back to Earth.

The test will take place at the White Sands Missile with a “boiler plate capsule,” a mock-up the Orion capsule outfitted with several instruments to measure how the abort motors work. “This is a key part of any human launch system as far as safety is concerned,” Hanley said.

Summer 2010: First Stage Motor Testing

ATK has just started casting the second Ares I first stage motor that will be test fired summer 2010. “We have more first stage recovery parachute testing as well, schedule for April,” Trina Patterson from ATK told Universe Today. She is the Senior Manager Media Relations for ATK Space Systems.

2010: Mobile launcher completed.

The new Ares mobile launcher, as it looked under contruction in Sept. 2009. Credit: NASA
The new Ares mobile launcher, as it looked under contruction in Sept. 2009. Credit: NASA

The new mobile launcher, currently under construction, will be the base for the Ares rocket to launch the Orion crew exploration vehicle and the cargo vehicle. “Two tiers are up, and the third tier is ready to go up later this week,” Hanley said. The base will be lighter than space shuttle mobile launcher platforms so the crawler-transporter can pick up the added load of the 345-foot tower and taller rocket. When the structural portion of the new launcher is complete, umbilical lines, access arms, communications equipment and command/control equipment will be installed.

Late 2010: Design review for the Orion capsule.

“At the end of next year, there is a critical design review for the Orion capsule,” said Hanley. “Progress is underway to build components. The first copy of Orion is being welded together at the Michoud Assembly Facility (in New Orleans). We will go through bunch of testing through the next couple of years, getting everything designed. It had a successful PDR (preliminary design review) in August and has the CDR (critical design review) next year. The Orion factory is actually here KSC, it is coming together, and as soon as all the parts come, they can put it together.”

Hanley said the program is paced by the current budget on when they can order parts for both Orion and Ares. “We’re under a continuing resolution, and that puts pressure on a program that want to be ramping up to its peak at this time,” he said. “More money sooner is would be good – that gets the parts purchased and into the supply chain. It takes about 3 years to actually get the parts you need. To build parts, you have to get the design done and know what you want to buy and then get your parts to assemble the rocket.”

A J-2 engine undergoes static firing. Image Credit: NASA
A J-2 engine undergoes static firing. Image Credit: NASA

Early 2011: J2X engine initial test.

The Ares I second, or upper, stage is propelled by a J-2X main engine fueled with liquid oxygen and liquid hydrogen.

The J-2X is an evolved variation of two historic predecessors: the powerful J-2 engine that propelled the Apollo-era Saturn IB and Saturn V rockets, and the J-2S, a simplified version of the J-2 developed and tested in the early 1970s but never flown.

March 2014: Arex 1Y test flight.

Artist concept of Ares I. Image Credit: NASA
Artist concept of Ares I. Image Credit: NASA

This will be a suborbital flight of the five-segment first stage reusable solid-rocket first with a flight-production upper stage, but containing a dummy J-2X engine. It will also conduct a high altitude test of the launch abort system. Hanley said they have studied putting an actual J-2X engine on that flight to prove that it will start at that altitude, but that is still under review.

“We’d all like to fly sooner; I would have liked to see Orion in completed in 2012 or 13, but the funding didn’t materialize for that, so we adjusted,” Hanley said. “That’s what we have to to do budget cycle to budget cycle. And that’s what we have to continue to do. But we’re making progress on the system, and the flight test schedule, we look for the opportunity to do more flight testing, but that is predicated on the budget.”

Where In The Universe #77

Here’s this week’s image for the WITU Challenge, a spooky Halloween version, to test your visual knowledge of the cosmos. You know what to do: take a look at this image and see if you can determine where in the universe this image is from; give yourself extra points if you can name the spacecraft responsible for the image. An added “bonus round” this week: name the circular feature in the image, too. We’ll provide the image today, but won’t reveal the answer until tomorrow. This gives you a chance to mull over the image and provide your answer/guess in the comment section. Please, no links or extensive explanations of what you think this is — give everyone the chance to guess.

UPDATE: The answer is now posted below.

This is a picture of auroras over Earth, specifically Canada with the large Manicouagan impact crater in the foreground. Clouds and Earth’s surface are illuminated by moonlight. The image was taken from the International Space Station by Mr. Wizard himself, astronaut Don Pettit. Read more about Pettit and his photography and wizardry at Science@NASA

Check back next week for another WITU challenge!

Telescopes Open Up the Jewel Box

A Snapshot of the Jewel Box cluster with the ESO VLT

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Nothing in my jewelry box compares to the Kappa Crucis Cluster, also known as NGC 4755 or simply the “Jewel Box.” This object is just bright enough to be seen with the unaided eye, but a combination of images taken by three exceptional telescopes, the Very Large Telescope, the 2.2-meter telescope at the La Silla observatory and the Hubble Space Telescope, has allowed the stunning Jewel Box star cluster to be seen in a whole new light. Above is the image from ESO’ Very Large Telescope, which zooms in for a close look at the cluster itself. This new image is one of the best ever taken of this cluster from the ground, taken with an exposure time of just 5 seconds.

A Hubble gem: the Jewel Box.  Credit: NASA/ESO
A Hubble gem: the Jewel Box. Credit: NASA/ESO

The Hubble Space Telescope can capture light of shorter wavelengths than ground-based telescopes can, and this new HST image of the core of the cluster represents the first comprehensive far ultraviolet to near-infrared image of an open galactic cluster. It was created from images taken through seven filters, allowing viewers to see details never seen before. It was taken near the end of the long life of the Wide Field Planetary Camera 2, Hubble’s workhorse camera up until the recent Servicing Mission, when it was removed and brought back to Earth, and replaced with an new and improved version. Several very bright, pale blue supergiant stars, a solitary ruby-red supergiant and a variety of other brilliantly colored stars are visible in the Hubble image, as well as many much fainter ones. The intriguing colors of many of the stars result from their differing intensities at different ultraviolet wavelengths.

Wide Field Image  of the Jewel Box.  Credit:  ESO
Wide Field Image of the Jewel Box. Credit: ESO

A new image taken with the Wide Field Imager (WFI) on the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile shows the cluster and its rich surroundings in all their multicolored glory. The large field of view of the WFI shows a vast number of stars. Many are located behind the dusty clouds of the Milky Way and therefore appear red.

Composite image of the Jewel Box. Credit: ESO
Composite image of the Jewel Box. Credit: ESO

Star clusters are among the most fascinating objects in the sky. Open clusters such as NGC 4755 typically contain anything from a few to thousands of stars that are loosely bound together by gravity. Because the stars all formed together from the same cloud of gas and dust their ages and chemical makeup are similar, which makes them ideal laboratories for studying how stars evolve.

Source: ESO

Ares I-X Launch Image Gallery

A bowshock forms around the Arex I-X rocket. Credit: NASA

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There are some great images of Wednesday’s Ares I-X launch. Most notable is this one of the Prandtl–Glauert singularity bow shock that formed around the 327-foot-tall rocket as it went supersonic at about 39 seconds into the flight. Liftoff of the 6-minute flight test from Launch Pad 39B at NASA’s Kennedy Space Center in Florida was at 11:30 a.m. EDT Oct. 28. This was the first launch from Kennedy’s pads of a vehicle other than the space shuttle since the Apollo Program’s Saturn rockets were retired. See more great images below.

Launch day.  Photo credit: NASA/Sandra Joseph and Kevin O'Connell
Launch day. Photo credit: NASA/Sandra Joseph and Kevin O'Connell

With more than 12 times the thrust produced by a Boeing 747 jet aircraft and 23 times the power output of the Hoover Dam, the Ares I-X test rocket produces 2.96 million pounds of thrust at liftoff. Interestingly, the Ares I-X booster was put together with parts from shuttle boosters that flew on 30 different shuttle missions ranging from STS-29 in 1989 to STS-106 in 2000. Ares I-X weighed 1.8 million pounds, almost twice that of a full 747 airliner.

The space shuttle and Ares I-X.  Credit: NASA/Scott Andrews
The space shuttle and Ares I-X. Credit: NASA/Scott Andrews

KSC is a busy spaceport, with the Ares I-X launching and space shuttle Atlantis poised on Launch Pad 39A for liftoff, targeted for Nov. 16. The Ares 1-X is nearly 143 feet taller than the space shuttle stack.
Another view of the launch.  Credit: NASA/ Scott Andrews
Another view of the launch. Credit: NASA/ Scott Andrews


The data returned from more than 700 sensors throughout the rocket will be used to refine the design of future launch vehicles and bring NASA one step closer to reaching its exploration goals.

View from inside mission control.  Credit: (NASA/Bill Ingalls)
View from inside mission control. Credit: (NASA/Bill Ingalls)

NASA Ares I-X mission managers watch from mission control as the Ares I-X rocket launches.

Ares I-X.  Credit: NASA/Scott Andrews
Ares I-X. Credit: NASA/Scott Andrews

Here’s the full shot from the lead image showing the Prandtl–Glauert singularity, and here’s Wikipedia’s definition:

“The Prandtl–Glauert singularity or P.G. singularity is sometimes referred to as a vapor cone, shock collar, or shock egg.

The point at which a sudden drop in air pressure occurs is generally accepted as the cause of the visible condensation cloud that often surrounds an aircraft traveling at transonic speeds, though there remains some debate. It is an example of a mathematical singularity in aerodynamics.”

NASA's Ares I-X rocket is seen on Launch Pad 39B at NASA's Kennedy Space Center. Photo Credit: NASA/Bill Ingalls
NASA's Ares I-X rocket is seen on Launch Pad 39B at NASA's Kennedy Space Center. Photo Credit: NASA/Bill Ingalls

This is a gorgeous shot of the Ares I-X on the pad on an evening before launch.

For information on the Ares I-X vehicle and flight test, visit NASA’s website.

Supernova 2009js… Another One Bites The Dust!

SN 2009 JS in NGC 918 by Joe Brimacombe

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Far away in the constellation of Aries, in a 14th magnitude barred spiral galaxy designated as NGC 918… a star exploded with enough candlepower to briefly outshine its home. Discovered independently by Lick Observatory Supernova Search (LOSS) and Koichi Itagaki (Japan) on October 11, 2009, this Type II supernova might be hiding in the intergalactic dust, but it isn’t hiding from Joe Brimacombe.

So who is to blame for this poor intergalactic housekeeping condition, eh? Just exactly where did this film of dust come from that dims distant galaxies and cloaks supernova events? Try our own Milky Way. We’ve known since the first Palomar Sky Surveys that we’re looking through clouds and filaments of dust at high galactic latitudes. But it isn’t just our galaxy either… It’s our whole family! Chances are the entire local group is puffing out enough hydrogen to send up a smoke screen – possibly even with higher redshift extragalactic objects. And just who is the smoker of our group?

The Andromeda Galaxy – M31…

“Finally we come to the aspect which could most shake conventional beliefs about the Local Group and the nature of near space. Deep prints of a red sensitive Schmidt plate (Arp and Sulentic 1991) show unmistakable filamentary dust features reaching back along the minor axis direction toward M31.This filament is repeated in the blue photographs and 100 the hundred micron infra red scans. They have to be real. Although no one has cared to take a spectrum there is no hint of gaseous emission.” says Halton Arp.

“The ejection path across the whole Local Group sky from M31 to 3C120 must have carried material either dusty or capable of forming dust from the ejecting M 31. But that means dust and obscuration within the Local group of galaxies – a point which has never before been seriously advanced. But how can one escape the mult-iwavelength evidence? The most provocative object in the M31 minor axis line is NGC 918. The nebulous dust is most concentrated at the position of the galaxy but a region has been cleared on either side of the minor axis of the galaxy. Higher resolution images would give invaluable information on the process whereby ejections come out along the minor axis of galaxies. In addition the nebulosity is of such long extent across the sky and so coincident with the alignment along the M31 minor axis that it must be in the Local Group. Therefore interaction with the dust filament would represent direct evidence for a distance much smaller than NGC 918’s conventional redshift distance.”

“The filamentary features surrounding NGC 918 are well shown in this image. The outer features appear to be dust illuminated by the galaxy. Immediately around the galaxy the dust appears to cleared away. By either outflow of matter or radiation pressure from the galaxy.” explains Arp, “If the galaxy is not interacting with the nebulosity but just shining through a serendipitous hole we still have the remarkable inference that material has been ejected along the minor axis of M31 into the middle of the Local Group of galaxies. The question then arises as to how many other nearby galaxy groups contain intergalactic material and what this would do to our view of purportedly more distant galaxies.”

If dust is to blame for a clouded view here, is it possible that NGC 918 could be just as guilty of ignoring the Swiffer? Darn right it could. According to research done by E. E. Martinez-Garcia (et al), NGC 918 has its share of spiral density waves that present azimuthal color gradients that even an infrared passband won’t fully penetrate. “We believe that this effect may be due to the position of the dust lanes and stars with respect to the observer.” says Garcia, “More research needs to be done to understand the origin of this effect.”

In the meantime, we’ll thank Joe Brimacombe of Northern Galactic for being on watch and capturing this distant supernova within 24 hours of its discovery. Cuz’ another one bites the dust!

LRO Takes Closer Look at Apollo 17 Landing Site

The Apollo 17 Lunar Module Challenger descent stage comes into focus from the new lower 50-km mapping orbit, image width is 102 meters [NASA/GSFC/Arizona State University].

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The Lunar Reconnaissance Orbiter maneuvered into its 50-km mapping orbit on September 15, which enables it to take a closer look at the Moon than any previous orbiter. This also allows for comparing previous images taken by LRO when it was at its higher orbit. Here’s the Apollo 17 landing site: just look at what is all visible, especially in the image below! These images have more than two times better resolution than the previously acquired images.

Region of Taurus-Littrow valley around the Apollo 17 landing site. NASA/GSFC/Arizona State University.
Region of Taurus-Littrow valley around the Apollo 17 landing site. NASA/GSFC/Arizona State University.

At the time of this recent pass, the Sun was high in the sky (28° incidence angle) helping to bring out subtle differences in surface brightness. The descent stage of the lunar module Challenger is now clearly visible, at 50-cm per pixel (angular resolution) the descent stage deck is eight pixels across (four meters), and the legs are also now distinguishable. The descent stage served as the launch pad for the ascent stage as it blasted off for a rendezvous with the command module America on December 14, 1972.

Also visible is the ALSEP, the Apollo Lunar Surface Experiments, which for Apollo 17 included 1) Lunar Seismic Profiling Experiment (geophones), 2) Lunar Atmospheric Composition Experiment (LACE) to measure the composition of the Moon’s extremely tenuous surface bound exosphere, 3) Lunar Ejecta and Meteorites (LEAM) experiment, 4) central station, 5) Heat Flow Experiment, 6) all powered by a Radioisotope Thermoelectric Generator (RTG). Below is how it looked from the surface, taken by the Apollo astronauts.

View of the ALSEP looking south-southeast.  Credit: NASA
View of the ALSEP looking south-southeast. Credit: NASA

Compare these most recent images to one taken previously.

Apollo 17 LRO. Credit: NASA
Apollo 17 LRO. Credit: NASA

See more images from LRO’s previous looks at the Apollo landing sites

See more at the LROC site.