Mars Archives

November 5, 2011April 13, 2022 by Ken Kremer

Phobos-Grunt and Yinghuo-1 Encapsulated for Voyage to Mars and Phobos

Phobos-Grunt spacecraft being encapsulated inside the nose cone for November 9 launch to Mars and its tiny moon Phobos. Credit: Roscosmos

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Phobo-Grunt, Russia’s first interplanetary mission in nearly two decades, has now been encapsulated inside the payload fairing and sealed to the payload adapter for mating to the upper stage of the Zenit booster rocket that will propel the probe to Mars orbit and carry out history’s first ever landing on the petite Martian moon Phobos and eventually return pristine samples to Earth for high powered scientific analysis.

“Phobos-Grunt will launch on November 9, 2011 at 00:16 a.m. Moscow time [Nov. 8 3:16 p.m. EST],” said Alexey Kuznetsov, Head of the Roscosmos Press Office in an exclusive interview with Universe Today. Roscosmos is the Russian Federal Space Agency, equivalent to NASA and ESA.

“The launch window extends until November 25.”

“At this moment we are preparing the “Zenit-2SB” launch vehicle, the cruise propulsion system and the “Phobos Grunt” automatic interplanetary station at the Baikonur Cosmodrome,” Kuznetzov told me. Phobos-Grunt translates as Phobos-Soil.

Phobos-Grunt spacecraft attached to payload adapter prior to encapsulation. Note folded solar panels, gold colored sample transfer tube leading to return capsule, landing legs, antennae and propulsion tanks. Credit: Roscosmos

China’s first ever mission to Mars, the Yinghuo-1 micro-satellite, is also encased inside the nose cone and is tucked in a truss segment between the lander and interplanetary propulsion stage.

Yinghuo-1 follows closely on the heels of China’s stunning success in demonstrating the nation’s first ever docking in space between two Chinese spacecraft earlier this week on November 3.

Sealing up Phobos-Grunt. Credit: Roscosmos

Technicians completed the two vehicles enclosure inside the protective fairing at Building 31 at the Baikonur Cosmodrome and have now transported the spaceships to Building 41 where the payload is now being stacked to the upgraded “Fregat-SB” upper stage atop the Zenit-2SB rocket.

Martian moon Phobos imaged by Mars Express Orbiter from ESA. Credits: ESA/DLR/FU Berlin (G. Neukum)

The payload fairing protects the Phobos-Grunt and Yinghuo-1 spacecraft during the first few minutes of flight from the intense frictional heating and buildup of aerodynamic pressures. After the rocket soars through the discernable atmosphere the fairing splits in half and is jettisoned and falls back to Earth.

The nose cone sports a beautiful mission logo painted on the side of the fairing along with the logos of various Russian and International partner agencies and science institutes.

Phobos-Grunt payload fairing. Credit: Roscosmos

Propellants have already been loaded aboard the cruise stage, Phobos-Grunt lander and Earth return vehicle.

“The Phobos Grunt automatic interplanetary station was built, prepared and tested at NPO Lavochkin [near Moscow]. They were also responsible for inspection of the devices, instruments and systems integration,” Kuzntezov explained.

“Significant improvements and modifications and been made to both the “Fregat-SB” upper stage and the “Zenit-2SB” rocket,” said Kuznetzov.

View inside nose cone and preparing to encapsulate Phobos-Grunt. Click to enlarge. Credit: Roscosmos

Phobos-Grunt will blastoff from Launch Pad 45 at Baikonur,

Following an 11 month journey, the spaceship will enter Mars orbit in October 2012, spend several months investigating Phobos and then land around February 2013.

The goal is to snatch up to 200 grams of soil and rock from Phobos and fly them back to Earth in a small capsule set to plummet through the atmosphere in August 2014.

ESA, the European Space Agency, is assisting Russia determine a safe landing site by targeting their Mars Express Orbiter to collect high resolution images of Phobos. Look at 2 D and 3 D images and an animation here.

The regolith samples will help teach volumes about the origin and evolution of Phobos, Mars and the Solar System. Scientists would be delighted if miniscule bits of Martian soil were mixed in with Phobos soil.

Phobos-Grunt , Earth’s next mission to Mars, is equipped with an advanced 50 kg payload array of some 20 science instruments.

NASA’s Curiosity Mars rover was also enclosed in her payload fairing a few days ago and is on course for liftoff on November 25.

The Phobos-Grunt spacecraft is scheduled to blastoff on November 9, 2011 from Baikonur Cosmodrome. It will reach Mars orbit in 2012 and eventually land on Phobos and return the first ever soil samples back to Earth in 2014. Credit Roscosmos

Read Ken’s continuing features about Phobos-Grunt here:
Phobos and Jupiter Conjunction in 3 D and Amazing Animation – Blastoff to Martian Moon near
Russia Fuels Phobos-Grunt and sets Mars Launch for November 9
Phobos-Grunt and Yinghou-1 Arrive at Baikonur Launch Site to tight Mars Deadline
Phobos-Grunt: The Mission Poster
Daring Russian Sample Return mission to Martian Moon Phobos aims for November Liftoff

Read Ken’s continuing features about Curiosity & Nov. 25 launch starting here:
Closing the Clamshell on a Martian Curiosity
Curiosity Buttoned Up for Martian Voyage in Search of Life’s Ingredients
Assembling Curiosity’s Rocket to Mars
Encapsulating Curiosity for Martian Flight Test
Dramatic New NASA Animation Depicts Next Mars Rover in Action

November 4, 2011January 14, 2016 by Nancy Atkinson

Hatch Opens as Simulated Mars Mission Ends

The first Mars crew has “returned” home. Thee Mars500 crew of six complete their simulated mission to Mars, with the hatch opening today, November 4, 2011. You can watch the replay the crew coming out of their 520 days of isolation inside a mock spaceship, which was actually in Russia. They crew has done countless hours of experiments, testing both the physiological and psychological effects of being “away from Earth” — isolated — for long periods of time.

November 4, 2011April 13, 2022 by Ken Kremer

NASA Robot seeks Goldmine of Science and Sun at Martian Hill along vast Crater

Opportunity - Panoramic view inside vast Endeavour Crater snapped ascending Cape York crater ridge on Sol 2754, October 23, 2011. Opportunity wheel tracks at right. Cape Tribulation and distant, far side Endeavour crater rim in background. Opportunity is now driving to the northern tip of Cape York in search of a winter haven to survive upcoming brutal Martian Antarctic winter temperatures. Credit: NASA/JPL/Cornell. See the entire panorama in 2 D and 3 D and route maps below.

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NASA’s intrepid robogirl Opportunity is now swiftly scouting out locations at a Martian hill along gigantic Endeavour crater that would simultaneously proffer a goldmine of sun and science as her power level drops significantly in these waning days of Martian autumn ahead of the absolutely brutal and potentially deadly 6 month long Antarctic winter that’s fast approaching. Opportunity has just discovered a geologic vein possibly formed as a result of flowing water eons ago.

But, search time for a sunny exposure at the Martian hill known as Cape York is running out says the Mars rover team in new interviews with Universe Today. Recall that lack of power and utterly frigid temperatures killed her twin sister Spirit last winter.

“Martian winter in the southern hemisphere starts on March 29, 2012 or Sol 2908. But, Solar power levels already begin dropping dramatically months before Martian winter starts,” said Alfonso Herrera to Universe Today, Herrera is a Mars rover mission manager at NASA’s Jet Propulsion Laboratory in Pasadena, Calif.

“Orbital imagery indicates that the northern-most tip of Cape York might have north facing slopes which Opportunity will need in order to generate enough solar power to sustain her comfortably throughout the winter,” Herrera explained to me.

The team is very excited about the science implications of the vein detection.

“The importance of veins is that often they occur from the deposition of material that was dissolved and transported by hot water in cracks deep underground,” said Bruce Banerdt to Universe Today. Banerdt is the Project Scientist for the Mars rover mission at JPL.

Traverse map showing the 7 Year Journey of Opportunity from Eagle Crater landing site Sol 1 (Jan. 24, 2004) to current location around Homestake on Sol 2763 (November 2011) at Cape York ridge at Endeavour Crater rim. Endeavour Crater is 14 miles or 22 kilometers in diameter. Opportunity has driven more than 21 miles (34 km). Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Kenneth Kremer

Segments of Endeavour’s rim at Cape York and Cape Tribulation about 6 kilometers further south offers scientifically rich motherlodes of phyllosilicate clay minerals and other water bearing minerals that formed Billions of years ago on Mars and that could possibly point to habitats favorable for the genesis and support of Martian microbial life forms if they ever existed in the past or present.

Opportunity is currently traversing about the hilltops and slopes of Cape York where she recently made landfall after an epic three year trek across the plains of the Meridiani Planum region of Mars.

Initial reconnaissance around the southern tip and then climbing on top of the central ridge of Cape York have already yielded a bonanza of new science data at rock types never seen before on Mars, according to Steve Squyres, the Mars Rover Principal Investigator of Cornell University.

The rover is now driving north and back down around the base while searching for a “winter haven” with more potential for great science and a northerly inclined slope to more efficiently catch the sun’s rays.

“Opportunity is heading north to find the best winter site,” Ray Arvidson told Universe Today. Arvidson is the rover’s deputy principal investigator, of Washington University in St. Louis.

“We are more than halfway toward the northern part of Cape York where there are slopes steep enough to provide an energy-valid winter site and where science can take place. Now we are driving away from the predicted outcrops [of smectite clay minerals] on Cape York and onto the bench on the western side because we have run out of time to investigate these outcrops.”

Opportunity - Wide panoramic view inside vast Endeavour Crater snapped ascending Cape York crater ridge on Sol 2754, October 23, 2011. Opportunity wheel tracks at center. Cape Tribulation and distant, far side Endeavour crater rim in background. Opportunity is now driving to the northern tip of Cape York in search of a winter haven to survive upcoming brutal Martian Antarctic winter temperatures. Credit: NASA/JPL/Cornell

However, the rover team was still hoping to catch a break for science opportunities along the way north and just chanced upon geologic veins potentially indicative of past flow of liquid water.

“The bench around the edge of Cape York looks like sedimentary rock that’s been cut and filled with veins of material possibly delivered by water,” says Arvidson.

3 D Opportunity Panorama - 3 D Wide panoramic view inside vast Endeavour Crater snapped ascending Cape York crater ridge on Sol 2754, October 23, 2011. Opportunity wheel tracks at center. Cape Tribulation and distant, far side Endeavour crater rim in background. Opportunity is now driving to the northern tip of Cape York in search of a winter haven to survive upcoming brutal Martian Antarctic winter temperatures. Credit: NASA/JPL/Cornell

Opportunity has just driven to a light toned vein at a spot dubbed “Homestake” and will spend a few sols (martian days) investigating with all the tools on the terminus of the robotic arm – including some Microscopic Imager (MI) images of the vein and placing the Alpha Particle X-ray Spectrometer (APXS) on top for overnight integrations.

“Opportunity will then continue traveling on the outboard side of Cape York (i.e. facing the plains),” Herrera told Universe Today.

“Plans are subject to change, but currently, Opportunity will travel to the north end of Cape York and stay there for the winter if suitable north facing slopes are found.”

“Our hope is that once a winter haven is identified, Opportunity will have enough power to make brief forays for science gathering in the vicinity of the winter haven,” Herrera informed me.

Homestake vein close up on Sol 2765- November 3, 2011. RAT (Rock Abrasion Tool) at lower left will target Homestake. Credit: NASA/JPL/Cornell

Opportunity Panorama at Cape York Ridge at Endeavour Crater - November 2011
Opportunity rover is exploring around the base of Cape York hill at the bench and vein features which may hold clues to the ancient flow of liquid water here on Mars. Opportunity drives North (ahead) from here in search of a sunny winter haven. Mosaic Credit: NASA/JPL/Cornell/Kenneth Kremer/Marco Di Lorenzo

Opportunity’s power levels have dropped by nearly 25 percent in the past few months – as Martian dust builds up – and are hovering around 300 watts-hours , which is less than a third of the maximum output possible from her life giving solar arrays.

Her sparkling wing-like solar panels boasted an output of some 950 watt-hours upon landing on Mars nearly 8 years ago – for a mission warrentied to last a mere 90 Martian Days, or Sols. That equates to 31 times beyond the design lifetime !

Endeavour Crater Panorama from Opportunity, Sol 2681, August 2011
Opportunity arrived at the rim of Endeavour on Sol 2681, August 9, 2011 and climbed up the ridge known as Cape York. Odyssey crater is visible at left. Opportunity is now driving to the northern tip of Cape York (to the left) and is investigating a geologic vein that indicates flow of liquid water. Opportunity was photographed from Mars orbit on Sept. 10, 2011.
Mosaic Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Kenneth Kremer

Cape York is a low ridge that belongs to the rim of humongous Endeavour crater, some 14 miles or 22 kilometers in diameter that offers spectacular panoramic vistas peering into the vast and beautiful crater sporting a huge central mound and mountainous rim segments both near and far.

Opportunity arrived at Cape York and Endeavour Crater in August 2011 after an overland expedition of more than 21 miles (34 km).

NASA’s Curiosity rover is on course to liftoff for Mars on Nov. 25

Traverse map showing the 7 Year Journey of Opportunity from Eagle Crater landing site to current location at Cape York ridge at Endeavour Crater rim. Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Kenneth Kremer

Read Ken’s continuing features about Opportunity starting here:
Opportunity spotted Exploring vast Endeavour Crater from Mars Orbit
Twin Towers 9/11 Tribute by Opportunity Mars Rover
NASA Robot arrives at ‘New’ Landing Site holding Clues to Ancient Water Flow on Mars
Opportunity Arrives at Huge Martian Crater with Superb Science and Scenic Outlook
Opportunity Snaps Gorgeous Vistas nearing the Foothills of Giant Endeavour Crater

November 3, 2011December 24, 2015 by Nancy Atkinson

Russia Considers Simulated Mars Mission on the Space Station

A view of the International Space Station as seen by the last departing space shuttle crew, STS-135. Credit: NASA

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Russia and ESA are just finishing up a 500-day simulated Mars mission here on Earth, and now Roscosmos, Russia’s Federal Space Agency is considering taking it to the next level and conducting a “virtual” Mars mission experiment in space, on board the International Space Station. This tentative plan would have two cosmonauts and/or astronauts staying on board the ISS for up to 18 months, matching the potential length of a manned Mars mission.

“We are interested in staging such an experiment in actual conditions of zero gravity,” Roscosmos’ deputy head Vitaly Davydov told Itar-Tass. While there are so specific plans at this time, Davydov added that such a project might be possible after 2014, since the schedule of ISS work and its crews for the next two years have already been plotted.

As of now, crews on the space station usually stay no longer than 6 months, to avoid long-term bone and muscle mass loss, as well as keeping the crews “fresh.” Davydov said Russia cannot make such a decision unilaterally, and would have to get consent from other international partners in the program.

The major issues in doing this would be how the costs would be divided by the 16 countries involved the ISS program and which countries the astronauts would be from. If such a mission would be approved, it will be interesting to see how much interest there is by astronaut and cosmonaut corps for staying in space for 18 months.

Source: Itar-Tass

November 3, 2011April 13, 2022 by Ken Kremer

Phobos and Jupiter Conjunction in 3 D and Amazing Animation – Blastoff to Martian Moon near

3 D view of the rare Phobos–Jupiter conjunction taken on 1 June 2011 by the High Resolution Stereo Camera on Mars Express. Credits: ESA/DLR/FU Berlin (G. Neukum)

Video Caption: Phobos and Jupiter in Conjunction – taken from Mars orbit !
A movie of the 1 June 2011 Phobos–Jupiter conjunction made by combining a sequence of 100 images of the encounter taken by the High Resolution Stereo Camera on ESA’s Mars Express orbiter. Mars Express is searching for safe landing zones on Phobos for Russia’s Phobos-Grunt lander blasting off on November 9. Credits: ESA/DLR/FU Berlin (G. Neukum)
3 D images of Phobos-Jupiter conjuction below
Update – Phobos-Grunt launch processing photo below

In just 7 days, Russia’s Phobos-Grunt sample return mission will blast off for Mars on November 9 on a daring mission to grab soil samples from the surface of the miniscule martian moon Phobos and return them back to Earth for analysis to give us breathtaking new insights into the formation and evolution of Mars, Phobos and our Solar System.

So, check out the amazing animation and 3 D stereo images of fish-like Phobos and banded Jupiter snapped by Europe’s Mars Express orbiter to get a bird’s eye feel for the battered terrain, inherent risks and outright beauty that’s in store for the Phobos -Grunt spaceship when it arrives in the Red Planet’s vicinity around October 2012. Whip out your red-cyan 3 D glasses – Now !

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ESA’s Mars Express orbiter (MEX) was tasked to help Russia locate suitable and safe landing sites on Phobos’ pockmarked terrain. MEX was built by ESA, the European Space Agency and has been in Mars orbit since 2003.

To capture this impressive series of rare photos of Jupiter and Phobos in conjunction, Mars Express performed a special maneuver to observe an unusual alignment of Jupiter and Phobos on 1 June 2011.

Mars Express High Resolution Stereo Camera (HRSC) snapped a total of 104 images over 68 seconds when the distance from the spacecraft to Phobos was 11,389 km and the distance to Jupiter was 529 million km.

Phobos- Jupiter Conjunction: before, during and after on 1 June 2011 from Mars Express. Credits: ESA/DLR/FU Berlin (G. Neukum)

Enjoy the exquisite views of the bands of Jupiter and imagine exploring the deep pockets and mysterious grooves on Phobos – which may be a captured asteroid.

The camera was kept fixed on Jupiter, to ensure it remained static as Phobos passed in front and which afforded an improvement in our knowledge of the orbital position of Phobos.

Phobos in 3 D during flyby of 10 March 2010. Image taken from a distance of 278 km. Russia’s Phobos-Grunt will retrieve rogolith and rock for return to Earth. Credit: ESA/DLR/FU Berlin (G. Neukum)

NASA’s twin Mars rovers Spirit and Opportunity have also occasionally photographed both of Mars’ moons to further refine their orbital parameters.

NASA’s Curiosity rover remains on track to liftoff for Mars on Nov. 25

Orbital Paths of Phobos and Mars Express. The trajectories of Phobos and Mars Express at the time of the conjunction with Jupiter on 1 June 2011. The letter ‘S’ denotes the South Pole of Mars.

Technicians at Baikonur Cosmodrome prepare Phobos-Grunt for upper stage attachment. Credit: Roscosmos

Read Ken’s continuing features about Phobos-Grunt here:
Russia Fuels Phobos-Grunt and sets Mars Launch for November 9
Phobos-Grunt and Yinghou-1 Arrive at Baikonur Launch Site to tight Mars Deadline
Phobos-Grunt: The Mission Poster
Daring Russian Sample Return mission to Martian Moon Phobos aims for November Liftoff

November 2, 2011December 24, 2015 by Nancy Atkinson

Mars Likely Not Ever Warm and Wet Enough for Life – At Least on Surface

Impact cratering and erosion combine to reveal the composition of the Martian underground by exposing materials from the subsurface. Image credit: NASA/JPL-Caltech/JHUAPL

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Mars’ surface was probably not ever warm and wet long enough to support life, a new study published today in Nature concludes. But underground on the Red Planet might be a different story. By taking a look at several years of data from orbiting spacecraft and examining more than 350 sites on Mars, a team of researchers determined that Martian environments with abundant liquid water on the surface existed only in short episodes. But liquid and likely warm water more likely lasted for longer periods of time below the surface, and this would have been occurring at about the same time that life was developing on Earth.

“If surface habitats were short-term, that doesn’t mean we should be glum about prospects for life on Mars, but it says something about what type of environment we might want to look in,” said Bethany Ehlmann from Caltech and JPL, who is the lead author of the study. “The most stable Mars habitats over long durations appear to have been in the subsurface. On Earth, underground geothermal environments have active ecosystems.”

And so, the best place to look for signs of past life on Mars may be underground.

The researchers’ findings seem to indicate that Mars’ surface was almost always cold and dry, and any appearances of water – and the salts they left behind – occurred during geologically brief periods. This is certainly not the first time research has suggested brief periods of water flowing on Mars, or that underground water may have persisted, but the news study does help to provide a better picture of the history of water on Mars and even if it could possibly be there today.

Clays are crucial to understanding past water on Mars, as they form only when water is around long enough to change the chemical structure of rocks into clay, and different types of clay minerals result from different types of wet conditions.

Signs of deep water, deep life? Erosion has exposed clays (light blue) that subterranean waters favorable to life may have formed eons ago in the Nili Fossae region of Mars. Credit: NASA/JPL/JHUAPL/University of Arizona/Brown University

In 2005, clay minerals were discovered in many regions of Mars by the OMEGA spectrometer on the ESA’s Mars Express. This finding seemed to indicate the planet was once warm and wet. But there’s a problem with Mars’ atmosphere – it is not thick enough now for water to be retained on Mars’ surface, and there is not scientific consensus that it was ever thick enough in the past to have allowed water to remain on the surface.

But this new study supports an alternative hypothesis that warm water persisted under Mars surface and many erosional features seen by the orbiting spacecraft were carved during brief periods when liquid water was stable at the surface.

“The types of clay minerals that formed in the shallow subsurface are all over Mars,” said John Mustard, professor at Brown University in Providence, R.I. Mustard a co-author of the study. “The types that formed on the surface are found at very limited locations and are quite rare.”

During the past five years, researchers used OMEGA and NASA’s Compact Reconnaissance Imaging Spectrometer, or CRISM, instrument on the Mars Reconnaissance Orbiter to identify clay minerals at thousands of locations on Mars. Clay minerals that form with small amounts of water usually retain the same chemical elements as those found in the original volcanic rocks later altered by the water.

The study interprets this to be the case for most terrains on Mars with iron and magnesium clays. In contrast, surface environments with higher ratios of water to rock can alter rocks further. Soluble elements are carried off by water, and different aluminum-rich clays form.

Another clue is detection of a mineral called prehnite. It forms at temperatures above about 400 degrees Fahrenheit (about 200 degrees Celsius). These temperatures are typical of underground hydrothermal environments rather than surface waters.

Two upcoming missions will help decipher the water clues left behind on Mars. The Curiosity rover, or the Mars Science Laboratory will be heading towards Gale Crater, to investigate a large, layered hill that contain clay and sulfate minerals. Curiosity is scheduled to launch later this month.

These new findings also have implications for how Mars’ atmosphere may have evolved over time, and the Mars Atmosphere and Volatile Evolution Mission, or MAVEN, in development for a 2013 launch, may provide evidence for or against this new interpretation of the Red Planet’s environmental history. This new study predicts MAVEN findings will beconsistent with the atmosphere not having been thick enough to provide warm, wet surface conditions for a prolonged period.

Source: JPL

November 1, 2011December 24, 2015 by Nancy Atkinson

Mars Express Experiences Multiple ‘Safe Mode’ Events

An illustration showing the ESA's Mars Express mission. Credit: ESA/Medialab)

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Mars Express has been a fixture in orbit around the Red Planet for almost eight years, but problems with the spacecraft’s computer memory has put the orbiter into safe mode and science observations have been halted for the time being. The spacecraft has gone into safe mode three times since mid-August, twice being recovered successfully. It has also had additional problems with its memory during this time. ESA says a technical work-around is being investigated that will enable the resumption of a number of observations, which will hopefully evolve into a long-term solution.

Safe mode is operational mode designed to safeguard both the spacecraft itself and its instrument payload in the event of faults or errors.

The portion of Mars Express’s computer the Solid-State Mass Memory (SSMM) system, which stores data before sending it on to Earth was not able to either write new data or read the previous data already in memory. The SSMM is a critical subsystem, central to all spacecraft and instrument operations.

This is not the first time the spacecraft has gone into safe mode. Three years ago a similar event took place, but now this multiple occurrence of problems has the Mars Express team looking for inventive solutions. The memory system has been switched to the “B” side or redundant computer, but the same fault took place, putting the spacecraft back in safe mode.

Another issue with the spacecraft going into safe mode is that is uses a lot of reserve fuel – as much as is required for six months of normal operations — so the frequent instances of this mode has engineers looking for a long-term solution. Most of the fuel consumption when entering safe mode is the ‘Sun acquisition’ process for letting the spacecraft know where it is in space, which requires a significant amount of spacecraft maneuvering.

ESA says they are making good progress with finding an alternative approach to commanding Mars Express, and will test it soon, and work continues on the finding a full solution to the memory problems.

Source: ESA

October 31, 2011April 13, 2022 by Ken Kremer

Closing the Clamshell on a Martian Curiosity

In the Payload Hazardous Servicing Facility at NASA's Kennedy Space Center in Florida, sections of an Atlas V rocket payload fairing engulf NASA's Mars Science Laboratory (MSL) as they close in around it. The blocks on the interior of the fairing are components of the fairing acoustic protection (FAP) system, designed to protect the payload by dampening the sound created by the rocket during liftoff. Launch of MSL aboard a United Launch Alliance Atlas V rocket is planned for Nov. 25 from Space Launch Complex-41 on Cape Canaveral Air Force Station. Credit: NASA/Jim Grossmann

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Curiosity’s clamshell has been closed.

And it won’t open up again until a few minutes after she blasts off for the Red Planet in just a little more than 3 weeks from now on Nov. 25, 2011 – the day after Thanksgiving celebrations in America.

The two halves of the payload fairing serve to protect NASA’s next Mars rover during the thunderous ascent through Earth’s atmosphere atop the powerful Atlas V booster rocket that will propel her on a fantastic voyage of hundreds of millions of miles through interplanetary space.

Spacecraft technicians working inside the Payload Hazardous Servicing Facility at NASA’s Kennedy Space Center (KSC) in Florida have now sealed Curiosity and her aeroshell inside the payload fairing shroud. The fairing insulates the car sized robot from the intense impact of aerodynamic pressure and heating during ascent. At just the right moment it will peal open and be jettisoned like excess baggage after the rocket punches through the discernable atmosphere.

Clamshell-like payload fairing about to be closed around Curiosity at KSC. Credit: NASA/Jim Grossmann

The next trip Curiosity takes will be a few miles to the Launch Pad at Space Launch Complex 41 at adjacent Cape Canaveral Air Force Station. She will be gingerly loaded onto a truck for a sojourn in the dead of night.

Curiosity in front of one payload fairing shell. Credit: NASA/Jim Grossmann

“Curiosity will be placed onto the payload transporter on Tuesday and goes to Complex 41 on Wednesday, Nov. 2,” KSC spokesman George Diller told Universe Today. “The logo was applied to the fairing this weekend.”

At Pad 41, the payload will then be hoisted atop the United Launch Alliance Atlas V rocket and be bolted to the Centaur upper stage.

Installation of Curiosity’s MMRTG (Multi-Mission Radioisotope Thermoelectric Generator) power source is one of the very last jobs and occurs at the pad just in the very final days before liftoff for Mars.

The MMRTG will be installed through a small porthole in the payload fairing and the aeroshell (see photo below).

MMRTG power source will be installed on Curiosity through the porthole at right just days before Nov. 25 launch. Credit: NASA/Jim Grossmann

The plutonium dioxide based power source has more than 40 years of heritage in interplanetary exploration and will significantly enhance the driving range, scientific capability and working lifetime of the six wheeled rover compared to the solar powered rovers Spirit and Opportunity.

After a 10 month voyage, Curiosity is due to land at Gale Crater in August 2012 using the revolutionary sky crane powered descent vehicle for the first time on Mars.

Camera captures one last look at Curiosity before an Atlas V rocket payload fairing is secured around it. Credit: NASA/Jim Grossmann

Curiosity has 10 science instruments to search for evidence about whether Mars has had environments favorable for microbial life, including chemical ingredients for life. The unique rover will use a laser to look inside rocks and release the gasses so that its spectrometer can analyze and send the data back to Earth.

Technicians monitor Curiosity about to be engulfed by the two halves of the payload fairing. Credit: NASA/Jim Grossmann

Payload fairing sealed around Curiosity at the Payload Hazardous Servicing Facility at KSC. Credit: NASA/Jim Grossmann

Atlas V rocket at Launch Complex 41 at Cape Canaveral, Florida
An Atlas V rocket similar to this one utilized in August 2011 for NASA’s Juno Jupiter Orbiter will blast Curiosity to Mars on Nov. 25, 2011 from Florida. Credit: Ken Kremer

Phobos-Grunt, Earth’s other mission to Mars courtesy of Russia is due to blast off first from the Baikonur Cosmodrome on November 9, 2011.

Read Ken’s continuing features about Curiosity starting here:
Curiosity Buttoned Up for Martian Voyage in Search of Life’s Ingredients
Assembling Curiosity’s Rocket to Mars
Encapsulating Curiosity for Martian Flight Test
Dramatic New NASA Animation Depicts Next Mars Rover in Action

Read Ken’s continuing features about Russia’s Phobos-Grunt Mars mission here:
Russia Fuels Phobos-Grunt and sets Mars Launch for November 9
Phobos-Grunt and Yinghou-1 Arrive at Baikonur Launch Site to tight Mars Deadline
Phobos-Grunt: The Mission Poster
Daring Russian Sample Return mission to Martian Moon Phobos aims for November Liftoff

October 29, 2011April 13, 2022 by Ken Kremer

Russia Fuels Phobos-Grunt and sets Mars Launch for November 9

The Phobos-Grunt spacecraft is scheduled blastoff on November 9, 2011 from Baikonur Cosmodrome. It will reach Mars orbit in 2012 and eventually land on Phobos and return the first ever soil samples back to Earth in 2014. Credit Roscosmos

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Russia’s Space Agency, Roscosmos, has set November 9 as the launch date for the Phobos-Grunt mission to Mars and its tiny moon Phobos. Roscosmos has officially announced that the audacious mission to retrieve the first ever soil samples from the surface of Phobos will blastoff from the Baikonur Cosmodrome in Kazakhstan atop a Zenit-2SB rocket at 00:16 a.m. Moscow time.

Roscosmos said that engineers have finished loading all the propellants into the Phobos-Grunt main propulsion module (cruise stage), Phobos lander and Earth return module at Facility 31 at Baikonur.

Phobos-Grunt is Russia’s first mission to Mars in almost two decades and a prelude to an ambitious program of even more interplanetary Russian science flights.

Russian Phobos-Grunt spacecraft is set to launch to Mars on November 9, 2011.
L-shaped soil sample transfer tube extends from Earth return module ( top -yellow) and solar panel to bottom (left) of lander module. 2 landing legs, communications antenna, sampling arm, propulsion tanks and more are visible. Credit Roscosmos

Technicians also fueled the companion Yinghou-1 mini-satellite, provided by China, that will ride along inside a truss segment between the MDU propulsion module and the Phobos-Grunt lander.

The 12,000 kg Phobos-Grunt interplanetary spacecraft is being moved to an integration and test area at Facility 31 for integration with the departure segments of the Zenit rocket.

The next step is to enclose Phobos-Grunt inside the protective payload fairing and transport it to Facility 42 for mating atop the upper stage of the stacked Zenit-2SB booster rocket.

After about an 11 month journey, the spaceship will enter Mars orbit and spend several months searching for a suitable landing site on Phobos. The goal of the bold mission is to retrieve up to 200 grams of soil and rock from Phobos and return them to Earth in August 2014. The samples will help unlock the mysteries of the origin and evolution of Phobos, Mars and the Solar System.

Scientists hope that bits of Martian soil will be mixed in with Phobos soil.

Phobos-Grunt is equipped with a powerful 50 kg payload of some 20 international science instruments.

The 110 kg Yinghou-1, which translates as Firefly-1, is China’s first spaceship to voyage to Mars. It will be jettisoned by Phobos-Grunt into a separate orbit about Mars. The probe will photograph the Red planet with two cameras and study it with a magnetometer to explore Mars’ magnetic field and science instruments to explore its upper atmosphere.

Earth’s other mission to Mars in 2011, NASA’s Curiosity rover, is set to blast off for Mars on Nov. 25

Labeled Schematic of Phobos-Grunt and Yinghou-1 (YH-1) orbiter

Read Ken’s continuing features about Russia’s Phobos-Grunt Mars mission here::
Phobos-Grunt and Yinghou-1 Arrive at Baikonur Launch Site to tight Mars Deadline
Phobos-Grunt: The Mission Poster
Daring Russian Sample Return mission to Martian Moon Phobos aims for November Liftoff

October 23, 2011April 13, 2022 by Ken Kremer

Curiosity Buttoned Up for Martian Voyage in Search of Life’s Ingredients

Curiosity Mars Science Laboratory (MSL)- all elements assembled into flight configuration in the Payload Hazardous Servicing Facility at NASA’s Kennedy Space Center in Florida. The top portion is the cruise stage attached to the aeroshell (containing the compact car-sized rover) with the heat shield on the bottom. Launch of MSL aboard a United Launch Alliance Atlas V rocket is scheduled for Nov. 25 from Space Launch Complex 41 on Cape Canaveral Air Force Station in Florida. Credit: NASA/Glenn Benson

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Take a good last, long look at the magnificent robot that is Curiosity, because she’s been all buttoned up for her long Martian voyage in search of the ingredients of life. After years of exhaustive work, the most technologically advanced surface robotic rover ever to be sent beyond Earth has been assembled into the flight configuration, a NASA spokesperson informed Universe Today.

The next time Curiosity opens her eyes she will have touched down at the foot of a layered mountain inside the planet’s Gale crater.

Curiosity Mars rover folded for flight and mated to the cruise stage. The cruise stage provides solar power, thrusters for navigation, and heat exchangers to the rover during its flight from Earth to Mars. Credit: NASA/Glenn Benson

Curiosity – NASA’s next Mars rover – is formally known as the Mars Science Laboratory (or MSL) and has entered the final stages of preflight processing.

After extensive quality assurance testing, Curiosity has been encapsulated for the final time inside the aeroshell that will be her home during the 10 month long interplanetary cruise to Mars. Furthermore, she’s been attached to the cruise stage that will guide her along the path from the home planet to the red planet.

Curiosity Mars Science Laboratory (MSL) assembled into flight configuration in the Payload Hazardous Servicing Facility at NASA’s Kennedy Space Center in Florida. The rover Curiosity has 10 science instruments designed to search for evidence on whether Mars has had environments favorable to microbial life, including chemical ingredients for life. Credit: NASA/Glenn Benson

The work to combine all the components into an integrated assembly was carried out inside the clean room facilities of the Payload Hazardous Servicing Facility at NASA’s Kennedy Space Center (KSC) in Florida.

The aeroshell is comprised of the heat shield and back shell.

The job of the aeroshell is to protect Curiosity from the intense heat of several thousand degrees F(C) generated by friction as the delicate assemblage smashes into the Martian atmosphere at about 13,200 MPH (5900 m/s) and plummets some 81 miles during the terrifying seven minute long entry, descent and landing (EDL) on the surface.

See Video animation below

The massive 2000 lb (900 kg) rover is folded up and mated to the back shell powered descent vehicle, known as the PDV or Sky Crane. The spacecraft is designed to steer itself through a series of S-curve maneuvers to slow the spacecraft’s descent through the Martian atmosphere.

In the final moments, the rocket powered Sky crane will lower the robot on tethers and then safely set Curiosity down onto the ground at a precise location inside the chosen landing site astride a layered mountain in Gale Crater believed to contain phyllosilicate clays and hydrated sulfate minerals that formed in liquid water.

The robot is the size of a compact car and measures three meters in length, roughly twice the size of the MER rovers; Spirit and Opportunity. It is equipped with 10 science instruments for a minimum two year expedition across Gale crater.

NASA's Curiosity Mars Science Laboratory Rover
Inside the Clean room at the Payload Hazardous Servicing Facility at the Kennedy Space Center.
The science payload weighs ten times more than any prior Mars rover mission. Curiosity will zap rocks with a laser and deftly maneuver her outstretched robotic arm to retrieve and analyze dozens of Martian soil samples. Credit: Ken Kremer

Curiosity will search for the ingredients of life including water and organic molecules and environmental conditions that could have been hospitable to sustaining Martian microbial life forms if they ever existed in the past or survived to the present through dramatic alterations in Mars climatic and geologic history.

Liftoff of the $2.5 Billion Curiosity rover is slated for Nov. 25 from Cape Canaveral Air Force Station in Florida on a United Launch Alliance Atlas V booster rocket. The launch window to Mars extends until Dec. 18.

This coming week, Curiosity will be encapsulated into the clamshell like payload fairing and the MSL logo will then be applied to the fairing, KSC spokesman George Diller told Universe Today. It will then be hoisted onto the payload transporter and carefully conveyed to Space Launch Complex 41 on Nov. 2, for mating atop the Atlas V rocket.

Mars Science Laboratory Aeroshell with Curiosity enclosed inside. Credit: NASA

Read Ken’s continuing features about Curiosity starting here:
Assembling Curiosity’s Rocket to Mars
Encapsulating Curiosity for Martian Flight Test
Dramatic New NASA Animation Depicts Next Mars Rover in Action

Read Ken’s features about Russia’s upcoming Phobos-Grunt, Earth’s other 2011 Mars mission here::
Phobos-Grunt and Yinghou-1 Arrive at Baikonur Launch Site to tight Mars Deadline
Phobos-Grunt: The Mission Poster
Daring Russian Sample Return mission to Martian Moon Phobos aims for November Liftoff