Showing posts with label Jules Verne. Show all posts
Showing posts with label Jules Verne. Show all posts

Thursday, May 30, 2013

Truncated Rille in Jules Verne

A lunar rille comes to an abrupt termination at a crater rim (34.342°S, 145.430°E). LROC Narrow Angle Camera (NAC) frame M1122636898R, LRO orbit 17626, May 8, 2013; illumination from east-northeast, an approximate 1 km wide field of view at 0.74 meters resolution [NASA/GSFC/Arizona State University].
James Ashley
LROC News System

We invite you to take a close look at this sinuous rille in Jules Verne crater on the lunar farside.

Why do we see it approach this portion of an ancient, mare-flooded crater rim and suddenly terminate?

Any flowing river of molten rock (the process responsible for most sinuous rilles) would skirt the base of such a positive-relief structure once encountered ... unless the crater rim formed after the rille. But if the crater is flooded by mare basalts (see context image below) the crater must have formed before the rille, which established itself during mare emplacement.

M192002047LR-NSJ-58b-40p-3910x5393
Simple contextual seven kilometers wide field of view shows a wide distribution of debris aprons bordering nearly every contact zone in the vicinity of this ghost crater on the floor of Jules Verne. View a much larger rendition HERE. LROC NAC mosaic M192002047LR, orbit 13328, May 18, 2012; 66.47° angle of incidence, resolution 0.72 meters per pixel from 70.65 km [NASA/GSFC/Arizona State University].
LROC Wide Angle Camera (WAC) mosaic covering a 100 km wide field of view, including the western interior of Jules Verne [NASA/GSFC/Arizona State University].
A clue may be present within the rille itself. Note the sloping wall of debris entering the rille at the point where it encounters the crater wall near the center of the Featured Image. This is accumulated debris, which has been shed from the crater rim. If you look closely at the full NAC frame, HERE, you can also see a subtle break in slope around the perimeter of the crater wall that betrays the presence of a debris apron or pediment.

This eroded material may have buried other portions of rille that might indeed have skirted the original rim, giving the visible portion an appearance of protruding out of the rim at a sharp angle. Can you find any additional clues that would help solve the puzzle?

Other examples of rilles are highlighted in the LROC Featured Image posts "Meanders in Posidonius," "The Old and the Young in Tsiolkovskiy," and "Rimae Prinz Region - Constellation Region of Interest."

Thursday, November 1, 2012

Scours and Ejecta near Jules Verne Y

A topographic depression is mantled by impact debris (31.4°S; 145.0°E). An 800 meter-wide field of view from LROC Narrow Angle Camera (NAC) frame M130700036R, illumination is from the east, angle of incidence 73.63° at 55 centimeters resolution (in the original), from 53.74 kilometers [NASA/GSFC/Arizona State University].
James Ashley
LROC News System

The extreme energy of ground-hugging debris surges emanating from impact events often results in a distinctive V-shaped surface expression where the deposits are relatively fresh. Here we see such striations oriented with their apices pointing toward a fresh, unnamed impact crater just northwest of Jules Verne Y in the farside Highlands. The Featured Image highlights an area where this effect, which results from low-angle secondary impacts of ejected debris, seems to have been accentuated by local topography.

A wider view of NAC frame M130700036R. Image field of view is approximately 5 km in width [NASA/GSFC/Arizona State University].
A wider field of view from the same NAC frame gives increased context to the area highlighted in the LROC Featured Image.

Enlarging this LROC Wide Angle Camera (WAC) mosaic will permit inspection of scours radiating from the fresh impact just northwest of Jules Verne Y. Image with is approximately 950 km [NASA/GSFC/Arizona State University].
Even in the 100 m/pixel WAC mosaic, scours from interacting ejecta and terrain are clearly visible. To the northeast of the fresh crater can be seen additional scours that are oriented in a southwesterly to northeasterly direction, away from the impact site. Click HERE for the full NAC frame. Other examples of recent deposits can be found in the LROC Featured Images, In the Wake of Giordano Bruno, Ejecta Starburst, and Action Shot.

Additional perspective from a simulated perspective 170 km over this under-appreciated area of the Moon's farside highlands. ILIADS application, NASA Lunar Mapping and Modeling Project (LMMP), LROC WAC mosaic over LRO LOLA laser altimetry-based digital terrain model [NASA/GSFC/Arizona State University].

Wednesday, October 1, 2008

ATV Re-Entry Video

The European Space Agency's ATV "Jules Verne"
Ends its spectacularly successful six month mission
over the eastern South Pacific Ocean
As seen from NASA DC-8

Monday, September 29, 2008

Spectacular planned Re-Entry of first ESA ATV Jules Verne caught on tape.

ESA's ATV Jule Verne re-entry as seen from DC-8, over southern Pacific

The end of the first European Space Agency's planned series of "ATV's" (for Automated Transfer Vehicle) concludes a spectacularly successful mission many years in the making. ESA's "Jules Verne" re-entered Earth's atmosphere and what remained after that fiery encounter fell into the "graveyard" of spacecraft in the southeastern Pacific Ocean.

The versatility of the ESA's design was proven again and again, on this historic flight, and ESA continues its strong hints that the ATV design may become the work horse for Near Earth Orbital operations by the agency, and even be morphed to become a Human Transfer Vehicle (HTV) long before similar plans, by the Japanese Space Agency or Space-X in the Uniteds States, come to fruition.

Background HERE.

Monday, June 23, 2008

Jules Verne boosts ISS to 345 Kilometers

Toulouse - Prototype Automated Transfer Vehicle Jules Verne continues to impress ESA designers and ground controllers.

During a seven minute burn, Friday, the ESA's ATV performed a flawless second boost manuver since docking on the Russian Zvezda module in March, raising the ISS complex 7 kilometers to 345 kilometers.

The 300 metric ton International Space Station loses ~300 feet in altitude from atmospheric drag each day, and must recieve a regular boost to maintain orbital velocity, either from a visiting Space Shuttle, Progress or the nominally functional boosters, with limited fuel, on Zvezda. Now the increasingly real-world proven capabilities of ESA has been demonstrated once again in a banner year marked by repeated successful launches of its Arianne V heavy-lift from Kourou.

"We should have at least one more reboost in July and two in August," said Hervé Côme, ESA's ATV Mission Director at the ATV Control Centre.

The Jules Verne is scheduled to retire from ISS in September, departing with 6.5 metric tonnes of debris and be destroyed on re-entry over the South Pacific. But the better than hoped for performance of the prototype has encouraged boldness in the ESA to transform the ATV into a manned spacecraft, in direct competition with NASA-contractor SpaceX and the Commercial Orbital Transfer System under development in the United States.

Read more HERE.

Friday, May 30, 2008

ESA's ambitions for ATV

In the days when NASA's last three Apollo missions were scrapped, if you don't count Apollo-Soyuz as "Apollo 18," the agency had ambitions for a more glorious future. They were keen to maintain their booster capacity, and grasped at various straws.

Long-term plans offered by Congress and the Nixon administration for a "cheaper" Space Shuttle, built around a Space Telescope were cause for much grumbling. Among the concepts floated in hope of selling Congress on maintaining the Saturn booster plant and personnel was an idea very much like the European Space Agency's multi-purpose Automated Transfer Vehicle.

The first of its kind docked with the International Space Station right after the departure of Atlantis in early April. The Jules Verne will still be there when Discovery arrives once again next week.

Launched using the Arianne V heavy booster, ESA has a multitude of multi-purpose concepts in mind for the deceptively simple looking design, including a manned Crew Exploration Vehicle. Nancy Atkinson in Universe Today writes about the ESA's unveiling of what a manned-ATV's interior might look like HERE.

ESA's "evolution scenarios" are somewhat detailed HERE.

Monday, March 31, 2008

Jules Verne ATV tests ISS approach


On course for Wednesday docking, Jules Verne tests tight maneuvering near ISS

NASA The Jules Verne Automated Transfer Vehicle is approaching the International Space Station today for its “Demo Day 2″ practice maneuvers. It will have moved to within 12 meters of the Zvezda Service Module in a rehearsal for docking on Thursday.

Jules Verne reached closest point to the station around 16:38 UT today, at which time it was commanded by the crew to retreat to a point 20 meters away. From there it executed an automated “escape” command, to depart the station for its three-day phasing prior to final approach and docking around 14:41 Thursday, April 3.

During its first approach Saturday, the ATV fired its engines several times to bring it approximately two miles from the station. Once in position, the Jules Verne conducted thruster firings and other systems tests before it pulled back into a phasing orbit.

Thursday, March 20, 2008

ESA ATV Jules Verne Reaches Parking Orbit

Toulouse - Jules Verne ATV has today reached a parking position 2000 km ahead of the International Space Station. Europe’s ISS re-supply spacecraft will wait at this holding point for the completion of the STS-123 Space Shuttle mission before proceeding with the first of two rendezvous demonstration days.

Two boosts late last night took the Automated Transfer Vehicle (ATV) to its parking orbit at the same orbital altitude as the International Space Station (ISS). In the course of this manoeuvre ATV passed just 30 km underneath the Space Station.

Three smaller boosts in the course of the morning were used to adjust the spacecraft’s orbit, with Jules Verne ATV finally arriving at the parking position shortly before 12:00 UT today.

ATV’s second propulsion chain was used to execute today’s manoeuvres and, according to Alberto Novelli, ESA’s Mission Director at the ATV Control Centre in Toulouse, France, it performed perfectly. “In doing the boosts we have tested all the pressure regulators and that worked perfectly fine. So as of today we have the proof that the propulsion system as a whole, including all the redundancies, is working fine,” said Novelli.

According to the mission schedule, ESA has also submitted an official report to the ISS partners. The report gathers together all data on the performance of Jules Verne ATV during the phasing stage of the mission since the launch from Kourou, French Guiana, ten days ago.

“We will discuss the data in a meeting with the partners on 25 March. In principle that will give us the go-ahead to continue with the first rendezvous demonstration day,” explained Novelli. “As of today, this report is green and a ‘go’ from our side on all the criteria.”

Jules Verne ATV will remain in the parking orbit until 27 March. The spacecraft will then be taken to a position ready to perform the two rendezvous demonstration days set for 29 and 31 March.

Jules Verne ATV is scheduled to dock with the International Space Station on 3 April.

Friday, March 14, 2008

A Week in Space: Success Built on Failure

The Fountains of Enceladus

"Institutional memory is no luxury at NASA."
Joel Raupe
LUNAR PIONEER

The week in space saw demonstrations of astounding success, with stubbed toes and skinned knees here and there. Around Saturn, in low-Earth-orbit and here on the surface humans are building success on the shoulders of monumental failure.

Twentieth Century astronomer Harlow Shapley may have been wrong to disagree with Edmund Hubble’s theory that the Milky Way is yet another Galaxy, in a universe filled with similar “islands” in "the Great Debate" with Heber D. Curtis in 1920, but Shapley was prophetic in believing the quest for the stars would be a rugged one.

Planning for Failure:

At Langley Research Center NASA showed off an engineering mock up of an Orion engineering mock-up built to test launch failure escape systems. It evoked memories of similar Apollo mock-ups rolled out in 1961, even as Project Mercury was barely underway, and also memories also of Apollo 1 and the launch test Oxygen fire incinerating it's crew, Gus Grissom, Ed White and Roger Chaffee in 1967.

"Institutional Memory isn't a luxury with NASA. Failure to remember is far too expensive.

Last month Thomas D. Jones remembered his friends aboard Columbia five years ago when he wrote in Popular Science that “Orion will launch with a powerful escape motor that can rocket its crew away from a disintegrating booster. A conical crew cabin structure will protect the heat shield beneath it from a debris strike like the one that doomed Columbia.”

Institutional Memory isn't a luxury with NASA. Failure to remember is far too expensive, as is contingency planning that would give a soccer mom a brain cramp. The costly fire on the pad killing the crew of Apollo 1, and the Apollo 204 Investigation Board, led by future Apollo 8 commander Frank Borman, and the discovering of 20,000 design flaws in the Apollo/Saturn vehicles, saved future success for Apollo and nine visits by 27 people to lunar realm.

Of course, the pad fire would not have been prevented by a capsule escape system, a contingency never used in American manned spaceflight, but it does show contingency planning works. It works where failure is anticipated. Critical faults that did end up failing in the future appear always to be ones not planned for in contingency policy, but deadly failure always brought harsh light to systemic and mechanical flaws in need of being contingency planning priorities.

Capsule escape systems were never used during the Mercury, Gemini and Apollo missions, but early NASA officials were informed by the spectacular booster explosions on the pad and just after lift-off of unmanned vehicles before and after, just as they're reminded today by more recent failure. Thomas D. Jones' article in POPSCI shows a return to expendable boosters and “capsules” won't mean that Constellation will be uninformed by the space shuttle and the lessons of both Challenger and Columbia, perhaps in finally giving design and mission critics a voice equal to those of accountants and vendors, and their friends in Congress.

Working the Problem:

In low-Earth-orbit, STS-123 and Endeavour docked with the International Space Station and joined Expedition 16 a few minutes later than planned, and by the end of our work week the first of five planned spacewalks during the shuttle's stay ended with attachment of the Japanese Kibo module and new dexterity added to the space station’s robotic Canadarm2 and crane with Dextre properly installed, at least where it should be.

Initial Power Couplings for the improvement didn't power-up, however, but costly failure was diverted in time when Primary Couplings were installed on the second spacewalk of STS-123, Saturday.

It's been a working weekend for NASA-Houston, and mostly according to plan for the ten people falling around Earth five miles a second, and 200 miles overhead.

On the first spacewalk, EVA record holder and ISS Expedition 16 commander Dr. Peggy Whitson reported her first look inside Kibo from the station showed "nothing unexpected." She was also happy to confirm no "floaters" inside the new station segment, now the first manned space vehicle built by Japan.

Expedition 16 flight engineer Dr. Garrett Reisman and STS-123 mission specialist Dr. Rick Linnehan completed the first spacewalk of the shuttle mission at 0919 UT, out in the void for seven hours and one minute.

Hiccups.

Far beyond the Moon, and just past conjunction, the soft yellowish star overhead before sidereal midnight testifies to the distance Cassini first had to travel even to begin its mission at Saturn.

It has been darting up and around and over and under the gaseous giant, using orbital mechanics of astounding complexities and Saturn and its many moon's gravity wells as third and fourth dimensional side pockets to fly out and away and quickly drawn back in again in precise maneuvering over and over again in an orbit around Saturn unlike any in nature.

Wednesday evening, in a much anticipated event Cassini was busy collecting data as it sliced just under the brightest moon in the solar system, over fresh snow on the south pole of Enceladus.

Slewing cameras as it moved by at 9 miles a second (14.4 kps); and only 32.3 miles above its surface, Cassini performed another unprecedented maneuver in a mission composed of unprecedented maneuvers to discover more about still another outer solar system discovery.

Almost everyone who read a newspaper on Earth knew the purpose. Ice geysers, shooting towers of wispy strands the fan directly away at distances far greater than Enceladus' width had been discovered where a heat signature was spotted in the Infrared spectrum earlier in the mission. Cassini, steered by controllers at JPL a billion miles away in Pasadena, was forced to zip directly through what apparently were the highest water fountains known to exist in our star system.

Enceladus has joined its Saturnian sister Titan, and Jupiter’s Io and Europa, as a member of the human "Hit Parade" of most intriguing moons.” It's large enough for its mass to have crushed itself into a sphere, but has a snow-blinding diameter roughly equal to the length of Interstate 95 in North Carolina.

As monumental a success as the maneuver turned out to be in adding another achievement to Pasadena’s long list of unsurpassed magic, as JPL waited for the data to download as it arrived in packets from 90 light minutes away as it was being scooped up by the Deep Space Network, and as Cassini continued a mad dash toward Titan, it became clear after a time that a “software hiccup” had spoiled a most important part of the show.

Planetary scientists won’t be disappointed with the pictures. They may even yet begin to answer the question of what forces are at play making Enceladus so “dynamic” and new in its south while so obviously ancient and quiet in its north. Those same scientists continue to puzzle over the awesome complexities of Saturn’s rings, and Enceladus with her high fountains of water ice somehow plays a role in that mystery.

Leading into the flyby Cassini shot side glances of those rings nearly edge on and caught now alomost routine shots of more than a few of the Ring’s Shepherd Moons, dancing to a melody we still can’t quite hear. Enceladus may be chief among them, particulary concerning its part in the cycling of Saturn's E-Ring.

But the very experiment onboard Cassini needing to be inside those tremendous Fountains of Enceladus became useless at the very moment it was most needed, though shuffling of software that had been rehearsed and rehearsed, and rehearsed again in the days beforehand. It was an anomaly suitable to a short story by Arthur C. Clarke.

JPL explained the "hiccup" this way:

"During Cassini's closest approach, two instruments were collecting data--the Cosmic Dust Analyzer and the Ion and Neutral Mass Spectrometer. An unexplained software hiccup with Cassini's Cosmic Dust Analyzer instrument prevented it from collecting any data during closest approach, although the instrument did get data before and after the approach. During the flyby, the instrument was switching between two versions of software programs. The new version was designed to increase the ability to count particle hits by several hundred hits per second. The other four fields and particles instruments on the spacecraft, in addition to the ion and neutral mass spectrometer, did capture all of their data, which will complement the overall composition studies and elucidate the unique plume environment of Enceladus."And the raw imagery doesn't disappoint, with promising new information promising to be teased out in the days ahead.

Amazing Cassini, unscathed, roboticly unembarrassed, now speeds on toward Titan, continuing a long and amazing tour.

Cassini returns to Enceladus next October.

Europe’s Progress:

And then there’s the Jules Verne, ESA's new unmanned ATV space truck, which was inserted safely into a parking orbit after being lifted high and fast aloft from equatorial Kourou while perched atop a powerful Ariane 5.

During initial orbital checkout, in a “holding pattern” and with time to kill as controllers waits for Endeavour to depart for its turn at the Harmony Node at ISS, ESA ground controllers worked feverishly to restore 7 of 28 reaction control thrusters and one of three of the ATV’s main engines, failing to respond to command.

They were successful in restoring the fire (though ESA was confident the cargo vessel would safely make it to ISS regardless) and they can stop sweating, for the moment, ahead they can look forward to new ATV’s first semi-automated docking depending the hardcore-proven Russian-supplied and Ukrainian-built Kurs docking system.

Conclusion:

Noteworthy in all this are simple facts illustrating little problems are always essential parts of the stories of big successes, and big success seems highly dependant upon now-working systems that were once spectacular failures.

That Kurs docking system, an unquestioned success today and essential to the ISS and Russia's Progress, was a buggy and unholy mess, playing a role in breath-stealing human and mechanical error such as more than one complete miss, near miss and at least one catastrophic accident in the days of the Soviet MIR space station program only eleven years ago.

And Jules Verne was successfully propelled to its present station-keeping orbit by the once- equally disastrous Ariane 5, which exploded nine miles up and rained debris on the French Guyana and Brazilian coast over an area of many miles twelve years ago.

Remembered clearly that day the cry of a Kourou facility launch director, when it happened, who reported with tears, “it is all over, it is all finished.”

Clearly, it was not.

And then the beginning of this present NewSpace Race, even throughout the world, might well be marked by the hellish disintegration of Columbia over Texas on February 1, 2003., though some would mark it with Ronald Reagan's determination to open the sky to entrepreneurship the previous decade. It was Columbia that refocused public attention, and without political will, Lincoln believed, nothing is possible.

Far from ending manned and unmanned space exploration, renewed Vision starts with documented mechanical and systemic failure. Failure may not be "an option," but it is a proven element essential to success.

Tuesday, March 11, 2008

Space truck orbits despite fault

Jonathan Amos

BBC
Europe's new ATV space truck is up and running following Sunday's launch, although one propulsion glitch means a back-up system is currently being used.

The freighter is sitting in a 260km high orbit and is due to deliver just under five tonnes of supplies to the space station on 3 April.

The anomaly has shut down seven of the 28 attitude control jets and one of the space truck's four main engines.

Engineers are now investigating with a view to getting them all back online.

Even if they cannot, the vehicle is more than capable of completing its approach and docking to the space station, say European Space Agency (Esa) officials.

The ATV cannot approach the orbiting platform until Endeavour has completed its mission.

Read More HERE.

Tuesday, March 4, 2008

Jules Verne ATV launch delayed 24 hours

Arianespace and the European Space Agency confirm today that the launch of Jules Verne, the first Automated Transfer Vehicle, is delayed 24 hours due to a technical concern about the ATV/Ariane 5 launcher separation system.

During the last validation step for the device which separates the 20-tonne European spacecraft from its launcher, a potential problem was identified with the fitting of the grounding straps located in the separation system. After removal of the Ariane 5 fairing, this item will be checked again, consistent as always with the conservative and precautionary approach taken by ESA to its missions.

In order to maintain safe margins for the countdown, ESA and Arianespace decided to postpone the launch by one day. The Jules Verne launch is rescheduled for 00:59 Kourou time, 03:59 UTC, Sunday March 9, 2008.

ESA's Jules Verne ATV will re-supply the International Space Station, delivering experiments, equipment and spare parts, as well as food, air and water for the permanent onboard crew.

Monday, February 25, 2008

Joint ESA And Russian Team In Moscow Ready To Support Jules Verne

ESA
When the Jules Verne Automated Transfer Vehicle (ATV) is launched in early March it will use several key spacecraft hardware items such as the docking and refuelling systems, and the Kurs radar, procured in Russia. European and Russian engineers have worked together to adapt them from their previous use on the Russian spacecraft Progress and Soyuz to the much larger 20-tonne ATV vessel.

Several weeks after launch from Europe's Spaceport in Kourou, French Guiana, Jules Verne will reach the International Space Station (ISS) orbiting about 400 km above our heads, and rendezvous and dock with the Russian segment of the ISS. Jules Verne and the Russian Service Module will then form an integrated European/Russian complex that will have to function as one vehicle for up to 6 months.

The ATV and the Russian Service Module will not only support together critical functions such as refuelling in orbit and re-boosting the ISS, but they will also share numerous interfacing systems like power, data handling, thermal and life support systems.

Obviously this requires close links between European and Russian engineering communities, throughout the entire Jules Verne mission. To meet this need, in 2004 ESA set up a small Engineering Support Team (EST-MO) co-located at Moscow Control Centre.

The main function of this group, varying from 8 to 15 people, is to monitor the behaviour of Jules Verne in relation to its Russian components or Russian interfaces, and to interact with the local ISS Russian engineering representatives on any matters requiring direct technical exchanges.

This support group also has to work in close coordination with the main ATV Engineering Support Team based at the ATV Control Centre in Toulouse (ATV-CC).

Experts to monitor Jules Verne's flight
At the ATV-CC, next to the Flight Control Team in charge of the ATV operations, sits the main Engineering Support Team which includes experts from ESA and prime contractor EADS-Astrium, constantly monitoring the data and daily operations planning, and ready to support the flight controllers if anything unexpected happens with the ATV systems.

Since they know all the hardware and systems, they are able to propose quick corrective measures in case of an anomaly or failure.

The official language during ATV operations is English, including communications with Moscow and Houston, but the EST-MO group can also switch to Russian when both parties are Russian. EST-MO experts do not speak directly to flight controllers nor send commands to the ATV.

This complex setup, about to be put to the test for the first time with Jules Verne, has of course required a thorough training programme. Since July 2007, the EST-MO team members, from both ESA and RSC-Energia, have participated in a series of Joint Integrated Simulations (JIS), involving all three main Control Centres in Toulouse, Moscow and Houston.

The JIS programme has covered both nominal and off-nominal mission scenarios. "One example of what the future EST-MO role could be was when the 'trainer' suddenly ordered a failure scenario with the interruption of the docking system probe retraction, shortly after the ATV was captured by the ISS.

At the same time, an unexpected simulator behaviour added further complexity to this training session. This was eventually resolved because the ATV docking system experts were able to establish a direct technical exchange with their ISS counterparts sitting in the next room", said Massimo Cislaghi, ESA's EST-MO Leader.

Although the main EST-MO working location has been and will be the ESA Moscow Support Room (EMSR) located inside the Moscow premises, some of the EST-MO training has taken place directly at ATV-CC in Toulouse, in order to allow the team to get acquainted with that working environment and with their colleagues based there. During actual flight operations they will coordinate mainly through voice exchanges.

At the end of the EST-MO training programme all ESA and RSC-Energia Russian Systems specialists are ready to face the various situations practised in the training exercises.

"At the same time, their wide experience and know-how accumulated through dozens of Russian vehicle rendezvous, docking and attached operations, represent a guarantee of their ability to face unforeseen events that can never be excluded for such a challenging programme," added Cislaghi.

During the Jules Verne mission, the ATV will perform automated manoeuvres which are closely monitored by almost 60 controllers in Toulouse, Houston and Moscow. For the first time in history, three space centres will interact from different sides of the world.