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November 6, 2011April 13, 2022 by Ken Kremer

Curiosity Rover Bolted to Atlas Rocket – In Search of Martian Microbial Habitats

The payload fairing containing Curiosity, NASA's Mars Science Laboratory (MSL) rover rises from the transporter below as it is lifted up the side of the Vertical Integration Facility At Space Launch Complex 41. The fairing, which protects the payload during launch, was attached to the Atlas V rocket already stacked inside the facility. Credit: NASA/Kim Shiflett

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Only time now stands in the way of Curiosity’s long awaited date with the Red Planet. NASA’s next, and perhaps last Mars rover was transported to the launch pad at Cape Canaveral Air Force Station and then hoisted on top of the mighty Atlas V rocket that will propel her on a 10 month interplanetary journey to Mars to seek out the potential habitats of Extraterrestrial life.

In less than three weeks on November 25 – the day after Thanksgiving – the Curiosity Mars Science Laboratory (MSL) rover will soar to space aboard the Atlas V booster. Touchdown astride a layered mountain at the Gale Crater landing site is set for August 2012.

Collage showing transport of Curiosity inside nose cone to Space Launch Complex 41 at Cape Canaveral, Florida. Credit: NASA

The $2.5 Billion rover must liftoff by Dec. 18 at the latest, when the launch window to Mars closes for another 26 months. Any delay would cost hundreds of millions of dollars.

Curiosity represents a quantum leap in science capabilities and is by far the most advanced robotic emissary sent to the surface of another celestial body. MSL will operate for a minimum of one Martian year, equivalent to 687 days on earth.

After years of meticulous design work and robotic construction by dedicated scientists and engineers at NASA’s Jet Propulsion Laboratory in California and months of vigilant final assembly and preflight processing at the Payload Hazardous Servicing Facility (PHSF) at NASA’s Kennedy Space Center in Florida, Curiosity was finally moved the last few miles (km) she’ll ever travel on Earth – in the dead of night – to Space Launch Complex 41 at the Cape.

Curiosity inside the Nose Cone to Mars. In the Payload Hazardous Servicing Facility at the Kennedy Space Center in Florida, the Atlas V rocket's payload fairing containing the Mars Science Laboratory (MSL) spacecraft stands securely atop the transporter that will carry it to Space Launch Complex 41. Credit: NASA/Kim Shiflett

The robo behemoth was tucked inside her protective aeroshell Mars entry capsule and clamshell-like nose cone, gingerly loaded onto the payload transporter inside the PHSF and arrived – after a careful drive – at Pad 41 at about 4:35 a.m. EDT on Nov. 3. The move was delayed one day by high winds at the Cape.

Employees at Space Launch Complex 41 keep watch as the payload fairing containing NASA's Mars Science Laboratory (MSL) spacecraft is lifted up the side of the Vertical Integration Facility. Credit: NASA/Kim Shiflett

Teams from rocket builder United Launch Alliance then hoisted MSL by crane on top of the Atlas V rocket already assembled inside the launch gantry known as the Vertical Integration Facility, or VIF, and bolted it to the venerable Centaur upper stage. Technicians also attached umbilicals for mechanical, electrical and gaseous connections.

Curiosity’s purpose is to search for evidence of habitats that could ever have supported microbial life on Mars and determine whether the ingredients of life exist on Mars today in the form of organic molecules – the building blocks of life.

We are all made of organic molecules – which is one of the essential requirements for the genesis of life along with water and an energy source. Mars harbors lots of water and is replete with energy sources, but confirmation of organics is what’s lacking.

Curiosity, inside the payload fairing at Pad 41, has been attached to a lifting device in order to be raised and attached to the Atlas V rocket inside the Vertical Integration Facility. The fairing will protect the payload from heat and aerodynamic pressure generated during ascent. Credit: NASA/Kim Shiflett

The Atlas V will launch in the configuration known as Atlas 541. The 4 indicates a total of four solid rocket motors (SRM) are attached to the base of the first stage. The 5 indicates a five meter diameter payload fairing. The 1 indicates use of a single engine Centaur upper stage.

One of the last but critical jobs remaining at the pad is installation of Curiosity’s MMRTG (Multi-Mission Radioisotope Thermoelectric Generator) power source about a week before launch around Nov. 17. Technicians will install the MMRTG through small portholes on the side of the payload fairing and aeroshell.

The nuclear power source will significantly enhance the driving range, scientific capability and working lifetime of the six wheeled rover compared to other solar powered landed surface explorers like Pathfinder, Spirit, Opportunity, Phoenix and Phobos-Grunt.

The minivan sized rover measures three meters in length, roughly twice the size of the MER rovers; Spirit and Opportunity. MSL is equipped with 10 science instruments for a minimum two year expedition across Gale crater. The science payload weighs ten times more than any prior Mars rover mission.

The Atlas V rocket and Curiosity will roll out to the launch pad on Wednedsay, November 23, the day before Thanksgiving.

Meanwhile, Russia’s Phobos-Grunt mission to Mars and Phobos is on target to blast off on November 9, Moscow time [Nov 8, US time].

Curiosity Mars Science Laboratory Rover - inside the Cleanroom at KSC. Credit: Ken Kremer

Read Ken’s continuing features about Curiosity 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

Read Ken’s continuing features about Phobos-Grunt upcoming Nov 9 launch here:
Phobos-Grunt and Yinghuo-1 Encapsulated for Voyage to Mars and Phobos
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

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, 2011April 26, 2016 by Jason Major

Asteroid 2005 YU55: An Expert’s Explanation

A radar image an asteroid, 2005 YU55, acquired in April 2010. (This is not the asteroid that will pass by Earth on Jan. 27, 2012)Credit: NASA

NASA’s Jet Propulsion Laboratory released this video today featuring more information about the much-discussed 2005 YU55, a 400-meter-wide asteroid that will pass by Earth next Tuesday at a distance closer than the Moon. The video features research scientist Lance Benner, an expert in radio imaging of near-Earth objects.

While YU55 will come closer than any object we’ve been aware of in the past 35 years, it poses no risk to Earth.

“2005 YU55 cannot hit Earth, at least over the interval that we can compute the motion reliably, which extends for several hundred years.”

– Lance Benner, JPL Research Scientist

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While we can’t state enough that there’s no danger from YU55, this close pass will offer a fantastic opportunity for scientists to acquire detailed radar images of this ancient C-type asteroid.

NASA’s Near-Earth Objects Observation Program will continue tracking YU55 using the 70-meter radar telescope at the Deep Space Network in Goldstone, California, as well as with the Arecibo Planetary Radar Facility in Puerto Rico.

“This is the closest approach by an asteroid this large that we’ve known about in advance,” said Benner. “The Goldstone telescope has a new radar imaging capability which has just become available that will enable us to see much finer detail than has previously been possible.”

Radar imaging allows scientists to better study the surface features and composition of fast-moving, dark objects like YU55 which reflect very little visible light.

Space.com has provided a great infographic that shows exactly where this asteroid will pass by Earth. Note that the side view plainly shows that the path of the asteroid is well above the plane of the Earth/Moon orbit.

Source: SPACE.com: All about our solar system, outer space and exploration

Video: JPL

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 4, 2011April 26, 2016 by Jason Major

Asteroid 2005 YU55 Gets Closer to Earth; “No Chance of an Impact”

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Yes, it’s coming. Yes, it’s big. Yes, it will be even closer than the Moon. And yes… we’re completely safe.

The 400-meter-wide asteroid 2005 YU55 is currently zipping through the inner Solar System at over 13 km (8 miles) a second. On Tuesday, November 8, at 6:28 p.m. EST, it will pass Earth, coming within 325,000 km (202,000 miles). This is indeed within the Moon’s orbit (although YU55’s trajectory puts it a bit above the exact plane of the Earth-Moon alignment.) Still, it is the closest pass by such a large object since 1976… yet, NASA scientists aren’t concerned. Why?

Because its orbit has been well studied, there’s nothing in its way, and frankly there’s simply nothing it will do to affect Earth.

2005_YU55_approach_movie — Animation of 2005 YU55's trajectory on Nov. 8. (NASA/JPL) Click to play.

Period.

2005 YU55’s miniscule gravity will not cause earthquakes. It has no magnetic field. It will not strike another object, or the Moon, or the Earth. It will not come into contact with cometary debris, Elenin, a black dwarf, Planet X, or Nibiru. (Not that those last three even exist.) No, YU55 will do exactly what it’s doing right now: passing through the Solar System. It will come, it will go, and hopefully NASA scientists – as well as many amateur astronomers worldwide – will have a chance to get a good look at it as it passes.

Scientists with NASA’s Near-Earth Objects Observation Program will begin tracking YU55 on Friday, November 4 using the 70-meter radar telescope at the Deep Space Network in Goldstone, California , as well as with the Arecibo Planetary Radar Facility in Puerto Rico beginning November 8. These facilities will continue to track it until the 10th.

This close pass will offer a great opportunity to get detailed radar imaging of YU55, an ancient C-type asteroid literally darker than coal. Since these objects can be difficult to observe using visible light, radar mapping can better reveal details about their surface and composition.

To help inform the public about YU55 NASA’s Jet Propulsion Laboratory in Pasadena recently hosted a live Q&A session on Ustream featuring specialists Marina Brozovic, a Goldstone Radar Team scientist, and Don Yeomans, manager of NASA’s Near-Earth Object Program. They fielded questions sent in via chat and Twitter… a recording of the event in its entirety can be seen below:

Video streaming by Ustream

Undoubtedly there will still be those who continue to spread misinformation about 2005 YU55. After all, they did the same with the now-disintegrated comet Elenin. But the truth is out there… and the truth is that there’s no danger, no cover-ups, no “plots”, and simply no cause for concern.

“It’s completely safe… no chance of an impact.”

– Don Yeomans, JPL

Read more about YU55 on our previous post or on NASA’s Near-Earth Object Program site.

UPDATE: JPL has released a brief video about YU55 featuring research scientist Lance Benner, who specializes in radar imaging of near-Earth objects:

Although classified as a potentially hazardous object, 2005 YU55 poses no threat of an Earth collision over at least the next 100 years. However, this will be the closest approach to date by an object this large that we know about in advance and an event of this type will not happen again until 2028 when asteroid (153814) 2001 WN5 will pass to within 0.6 lunar distances. – Near-Earth Object Program, JPL

November 3, 2011December 24, 2015 by Jason Major

A Night Flight Over the Mideast

India-Pakistan Border from ISS — India-Pakistan Border from orbit. Credit: NASA.

The cities of the Middle East and southern Asia shine bright in the night beneath the International Space Station as it passed high overhead on October 21, 2011.

This video, an animation made from dozens of still images taken by the Expedition 29 crew, was assembled by the Image Science and Analysis Laboratory at Johnson Space Center in Houston. It was uploaded to the Gateway to Astronaut Photography of Earth site on October 27.

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Some glare from the Moon (off screen to the upper left) can be seen in the Plexiglas of the ISS window. The strobe-like flashes are lightning in clouds. Airglow is also visible as a band of hazy green light surrounding the planet.

Another particularly noticeable feature visible in this video is the bright orange line of the border between India and Pakistan. Erected by the Indian government to prevent smuggling, nearly 1200 miles (1930 km) of floodlights and fences separate the two countries, creating a geopolitical feature easily visible from orbit.

The website’s description states:

The sequence of shots was taken October 21, 2011 from 19:53:26 to 20:25:24 GMT, on a pass beginning over Turkmenistan, east of the Caspian Sea to southeastern China, just northwest of Hong Kong. City lights show at the beginning of the video as the ISS travels southeastward towards the India-Pakistan borderline (click here for the Earth Observatory article to learn more about this area). Pakistan’s second largest city, Lahore, can be easily seen as the brightly lit area left of track. Immediately downtrack of Lahore is New Delhi, India’s capital city, with the Kathiawar Peninsula right of track dimly lit. Smaller cities in southern India can be seen as the pass continues southeastward through southern India, into the Bay of Bengal. Lightning storms are also present, represented by the flashing lights throughout the video. The pass ends over western Indonesia, looking left of track at the island of Sumatra.

I particularly like the way the stars shine so prominently beyond Earth’s limb, and how the moonlight illuminates the clouds… not to mention the bloom of dawn at the end. What an incredible sight this must be for the ISS crew members! I can’t imagine ever getting tired of seeing this outside the Station windows.

Watch more ISS videos here.

Video courtesy of the Image Science & Analysis Laboratory, NASA Johnson Space Center.

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 1, 2011April 26, 2016 by Jason Major

Senate Approves Bill Funding JWST

Full scale model of the JWST at the EADS Astrium in Munich. Credit: EADS Astrium

This afternoon the U.S. Senate approved H.R. 2112, a FY 2012 bill from Maryland Senator Barbara Mikulski that would fund the James Webb Space Telescope to launch in 2018. This is another step forward for the next-generation space telescope, which many have called the successor to Hubble… all that now remains is for the House to reconcile.

“We are creating the building blocks that we need for a smarter America. Our nation is in an amazing race – the race for discovery and new knowledge, the race to remain competitive,” Chairwoman Mikulski said. “This bill includes full funding of the James Webb Telescope to achieve a 2018 launch. The Webb Telescope supports 1,200 jobs and will lead to the kind of innovation and discovery that have made America great. It will inspire America’s next generation of scientists and innovators that will have the new ideas that lead to new products and new jobs.”

The bill was approved by a vote of 69 to 30.

Thanks to everyone who contacted their representatives in support of the JWST and to all the websites out there that helped make it simple to do so… and of course to all the state representatives who listened and stood behind the JWST!

In addition to continued funding for the telescope the 2012 bill also allots the National Aeronautics and Space Administration $17.9 billion (still a reduction of $509 million or 2.8 percent from the 2011 enacted level) and preserves NASA’s portfolio balanced among science, aeronautics, technology and human space flight investments, including the Orion Multipurpose Crew Vehicle, the heavy lift Space Launch System, and commercial crew development.

It also supports funding for the NOAA.

“We are creating the building blocks that we need for a smarter America. Our nation is in an amazing race – the race for discovery and new knowledge, the race to remain competitive.”

– U.S. Senator Barbara A. Mikulski

Of course, we must remember that spending and allocation of funds is not necessarily creating funds. As with everything, money has to come from somewhere and it remains to be seen how this will affect other programs within NASA. Not everyone is in agreement that this is the best course of action for the Administration at this point, not with the overall reduction of budget being what it is.

Read the bill summary here.

You can show your continued support for the JWST by liking the Save the James Webb Space Telescope Facebook page and – even more importantly – by contacting your congressperson and letting them know you care!

October 31, 2011April 13, 2022 by Ken Kremer

Shenzhou-8 rolled out for Blastoff to China’s 1st Space Station on November 1

Shenzhou 8 spaceship and its launch vehicle Long March 2F/Y8 were transferred to the Jiuquan launch pad. Liftoff is scheduled for Nov. 1. China’s VAB in the background. Credit: CMSE

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China’s Shenzhou-8 capsule and the Long March booster rocket have been rolled out to the Gobi desert launch pad and will blast off early on November 1 bound for the 1st orbiting Chinese prototype space station – named Tiangong-1 (which translates as Heavenly Palace-1).

If successful, the Shenzhou -8/Tiangong -1 combined orbital complex will certainly be a ‘great leap forward’ for China’s space program ambitions and technological prowess while NASA’s current and future ambitions are being significantly curtailed by relentless budget cuts directed by politicians in Washington, D.C. – a fact noted by Chinese media.

Shenzhou-8, an unmanned spacecraft, and its carrier, Long March 2-F, are transported to the launch pad at the Jiuquan Satellite Launch Center in Northwest China's Gansu province. It is expected to perform China's first space docking with Tiangong-1, a lab module that went up in September from the same facility. Credit: Su Dong/China Daily

The unmanned Shenzhou- 8 capsule will lift off at 5:58 a.m. local time from the Jiuquan Satellite Launch Center located in Gansu province in northwest China.

Propellants are being loaded into the upgraded Long March 2F/Y8 carrier rocket today (Oct. 31). All launch preparations and tests are proceeding on schedule according to to the China Manned Space Engineering (CMSE) office – the state run government agency responsible for China’s human spaceflight program.

Prelaunch exercises are being coordinated by the Beijing Aerospace Flight Control Center, the command center for the Chinese space program.

The fully assembled vehicles were vertically transported some 1500 meters over about 2 hours along rail tracks from China’s version of NASA’s VAB, or the Vehicle Assembly Building.

The 8 ton Tiangong-1 target module was launched from Jiuquan on September 29 and is functioning perfectly

The Shenzhou VIII spacecraft is assembled with the Long-March II-F rocket at the Jiuquan Satellite Launch Center in Northwest China's Gansu province on Oct 23, 2011. Credit: CFP

The Long March 2F booster is the tallest, heaviest and most powerful in China’s arsenal of rockets.

Tiangong-1 has been maneuvered to rotate 180 degrees in orbit in anticipation of the upcoming launch according to CMSE.

The emergency escape tower is hoisted to Shenzhou-8 at the Jiuquan Satellite Launch Center on Oct 23, 2011. Credit: CFP

Shenzhou is China’s human rated capsule but is flying in an unmanned configuration for this flight – #8 – which will be China’s first ever attempt at critical Rendezvous & Docking maneuvers in earth orbit that are required to construct a Space Station- China’s long term goal by 2020 .

Shenzhou-8 will conduct at least two docking practice tests. After the first docking, the two ships will remain joined for about 12 days and then separate to carry out another docking.

So far China has conducted 3 manned flights, the first in 2003. Currently the US has no capability to launch astronauts to earth orbit and the ISS and is totally reliant on Russian Soyuz rockets and capsules to hitch a ride to space.

Two crewed flights to Tiangiong-1 are planned for 2012. The multi-person crews aboard Shenzhou 9 & Shenzhou 10 are likely to include China’s first woman astronaut. The chinese crews would float into Tiangong 1 from their capsules and remain on board for short duration missions of a few days or weeks. They will check out the space systems and conduct medical, space science and technology tests and experiments.

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