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December 20, 2013December 23, 2015 by Ken Kremer

Stunning Chang’e-3 Lunar Landing Video gives Astronauts Eye View of Descent & Touchdown

This screen shot from one photo of many of the moons surface snapped by the on-board descent imaging camera of the Chinese lunar probe Chang’e-3 on Dec. 14, 2013 shows the probe approaching the Montes Recti mountain ridge and approximate location of the landing site in Mare Imbrium. This marks the first time that China has sent a spacecraft to soft land on the surface of an extraterrestrial body. Image and video rotated 180 degrees.
Credit: Xinhua/CCTV/post processing and annotations Marco Di Lorenzo /Ken Kremer
See the entire stunning Chang’e-3 lunar landing video – below
Story updated
[/caption]

China accomplished a major technological and scientific feat when the country’s ambitious Chang’e-3 robotic spacecraft successfully soft landed on the Moon on Dec. 14 – on their very first attempt to conduct a landing on an extraterrestrial body.

Along the way the descent imaging camera aboard the Chang’e-3 lander was furiously snapping photos during the last minutes of the computer guided descent.

For a firsthand look at all the thrilling action, be sure to check out the stunning landing video, below, which gives an astronauts eye view of the dramatic descent and touchdown by China’s inaugural lunar lander and rover mission.

The video was produced from a compilation of descent camera imagery. The version here has been rotated 180 degrees – so you don’t have to flip yourself over to enjoy the ride.

And it truly harkens back to the glory days of NASA’s manned Apollo lunar landing program of the 1960’s and 1970’s.

The dramatic Chang’e-3 soft landing took place at Mare Imbrium at 8:11 am EST, 9:11 p.m. Beijing local time, 1311 GMT, which is to the east of the announced landing site on the lava filled plains of the Bay of Rainbows, or Sinus Iridum region.

The precise landing coordinates were 44.1260°N and 19.5014°W -located below the Montes Recti mountain ridge and about 40 kilometers south of the 6 kilometer diameter crater known as Laplace F – see image below.

Landing site of Chinese lunar probe Chang'e-3 on Dec. 14, 2013. — Landing site of Chinese lunar probe Chang’e-3 on Dec. 14, 2013.

The video begins as Chang’e-3 is approaching the Montes Recti mountain ridge which is about 90 km in length. Its peaks rise to nearly 2 km.

Chang’e-3 carried out the rocket powered descent to the Moon’s surface by firing the landing thrusters starting at the altitude of 15 km (9 mi) for a soft landing targeted to a preselected area in Mare Imbrium.

The vehicles thrusters then fire to pivot the lander towards the surface at about the 2:40 minute mark when it’s at an altitude of roughly 3 km.

Infographic shows the process of the soft-landing on the moon of China's lunar probe Chang'e-3 on Dec. 14, 2013. Credit: SASTIND/Xinhua /Zheng Yue — Infographic shows the process of the soft-landing on the moon of China’s lunar probe Chang’e-3 on Dec. 14, 2013. Credit: SASTIND/Xinhua /Zheng Yue

The powered descent was autonomous and preprogrammed and controlled by the probe itself, not by mission controllers on Earth stationed at the Beijing Aerospace Control Center (BACC) in Beijing.

Altogether it took about 12 minutes using the variable thrust engine which can continuously vary its thrust power between 1,500 to 7,500 newtons.

The variable thrust engine enabled Chang’e-3 to reduce its deceleration as it approached the moons rugged surface.

Photo taken on Dec. 14, 2013 shows the landing spot of lunar probe Chang'e-3 indicated on the screen of the Beijing Aerospace Control Center in Beijing, capital of China. Credit: Xinhua/Li — Photo taken on Dec. 14, 2013 shows the landing spot of lunar probe Chang’e-3 indicated on the screen of the Beijing Aerospace Control Center in Beijing, capital of China. Credit: Xinhua/Li

The 1200 kg lander was equipped with unprecedented terrain recognition equipment and software to hover above the landing site and confirm it was safe before proceeding.

This enabled the craft to avoid hazardous rock and boulder fields as well as craters in the pockmarked terrain that could spell catastrophe even in the final seconds before touchdown, if the vehicle were to land directly on top of them.

The descent engine continued firing to lower the lander until it was hovering some 100 meters above the lunar surface – at about the 5:10 minute mark.

Chang'e-3 hovered 100m high for 20 seconds before committing to land. This allows the on-board computer to make sure it doesn't land in a crater or an uneven place. Credit: China Space — Chang’e-3 hovered 100m high for 20 seconds before committing to land. This allows the on-board computer to make sure it doesn’t land in a crater or an uneven place. Credit: China Space

After hovering for about 20 seconds and determining it was safe to proceed, the lander descended further to about 3 meters. The engine then cut off and the lander free fell the remaining distance. The impact was cushioned by shock absorbers.

There is a noticeable dust cloud visible on impact as the Chang’e-3 mothership touched down atop the plains of Mare Imbrium.

Chang'e-3 lander imaged by the rover Yutu on the moon on Dec. 15, 2013. Note landing ramp at bottom. Credit: CCTV — Chang’e-3 lander imaged by the rover Yutu on the moon on Dec. 15, 2013. Note landing ramp at bottom. Credit: CCTV

Barely 7 hours later, China’s first ever lunar rover ‘Yutu’ rolled majestically down a pair of ramps and onto the Moon’s soil on Sunday, Dec. 15 at 4:35 a.m. Beijing local time.

The six wheeled ‘Yutu’, or Jade Rabbit, rover drove straight off the ramps and sped right into the history books as it left a noticeably deep pair of tire tracks behind in the loose lunar dirt.

The stunning feat was broadcast on China’s state run CCTV.

China thus became only the 3rd country in the world to successfully soft land a spacecraft on Earth’s nearest neighbor after the United States and the Soviet Union.

It’s been nearly four decades since the prior lunar landing was accomplished by the Soviet Union’s Luna 24 sample return spacecraft back in 1976.

America’s last visit to the Moon’s surface occurred with the manned Apollo 17 landing mission – crewed by astronauts Gene Cernan and Harrison ‘Jack’ Schmitt , who coincidentally ascended from the lunar soil on Dec. 14, 1972 – exactly 41 years ago.

China’s Chang’e-3 probe joins NASA’s newly arrived LADEE lunar probe which entered lunar orbit on Oct. 6 following a spectacular night time blastoff from NASA’s Wallops Flight Facility in Virginia.

Stay tuned here for Ken’s continuing Chang’e-3, LADEE, MAVEN, MOM, Mars rover and more news.

Ken Kremer Moon map showing landing site of Chinese lunar probe Chang’e-3 on Dec. 14, 2013 below Montes Recti in Mare Imbrium beside Sinus Iridum, or the Bay of Rainbows . Credit: China Space[/caption]

Image shows the trajectory of the lunar probe Chang'e-3 approaching the landing site on Dec. 14. — Image shows the trajectory of the lunar probe Chang’e-3 approaching the landing site on Dec. 14.

December 20, 2013December 23, 2015 by Elizabeth Howell

After Facing Down Ammonia Leak, This Astronaut Will Help Crew During Spacewalks

NASA astronaut Doug Wheelock, who was commander of Expedition 25. This 2010 picture of him also shows the Sabatier system that extracts drinkable water from the International Space Station's atmosphere. Credit: NASA

When you learned to drive a car for the first time, remember how comforting it was to have an experienced driver beside you, able to anticipate the hazards and keep you on schedule?

That’s surely how the Expedition 38 crew feels about one of the voices “on the line” as two astronauts prepare to venture outside to replace a crippled ammonia pump. One of the “CapComs” or people communicating with the crew on Saturday, Monday and Wednesday will be astronaut Doug Wheelock — who just happens to be known for co-replacing a broken ammonia tank himself in 2010. (The other CapCom is Japanese astronaut Aki Hoshide, who will chat through robotic procedures with Koichi Wakata).

Wheelock is the visible edge of hundreds — likely thousands — of people working feverishly at NASA and its international partners this past week to get the spacewalks ready through pool simulations, a virtual reality lab and other means. Several backup and non-critical space station systems are offline because of that pump, which has to regulate temperatures properly for vital electronics to work.

“I am their choreographer,” Wheelock told Universe Today of his plan for the astronauts. While spacewalkers Mike Hopkins and Rick Mastracchio already know what they are supposed to do when, Wheelock said he will be “their eyes and ears on the timeline.” If something needs to be stopped or changed, he’ll help them figure out what to do next.

NASA astronaut Doug Wheelock anchored to Canadarm2 during an August 2010 spacewalk. He and Tracy Caldwell Dyson ventured outside three times during Expedition 24 to swap out and replace a broken ammonia pump. Credit: NASA

Wheelock and fellow astronaut Tracy Caldwell Dyson had to spring into action themselves in August 2010. A pump in the same location broke, forcing space station systems offline and requiring them to go outside a few days later. With astronaut Shannon Walker piloting Canadarm2, the astronauts accomplished their tasks in three spacewalks — but encountered obstacles along the way.

During the first spacewalk, as Wheelock disconnected lines from the broken pump, he not only faced a pipe that wouldn’t let go, but a shower of ammonia snowflakes. That was “what got me on the EVA [extra-vehicular activity],” he recalled. That’s why NASA plans to lower the line pressure on the cooling system before the astronauts head outside this time. Normally the lines are pressurized at 360 pounds per square inch, but they’ll be lowered to 120 psi through commands from the ground.

Other “lessons learned” are more recent. Italian astronaut Luca Parmitano was wearing a NASA spacesuit in July when he experienced a water leak in his helmet, putting him at risk and terminating the spacewalk early. This will be the first spacewalk since that time. NASA believes it has replaced the part of the suit that failed, but the agency has new backups in place. Hopkins and Mastracchio will have soaker pads in their helmets as well as a “snorkel”-like device, or tube that will let them breathe oxygen from a different part of the suit if water flows into the helmet again.

Allison Bolinger, NASA's lead U.S. spacewalk officer, holds up a snorkel-like device that astronauts began using in spacesuits in December 2013. The pipe (modified from spacesuit parts) is supposed to be a backup if a helmet fills with water, as what occurred during a July 2013 spacewalk. Credit: NASA (YouTube/screenshot) — Allison Bolinger, NASA’s lead U.S. spacewalk officer, holds up a snorkel-like device that astronauts began using in spacesuits in December 2013. The pipe (modified from spacesuit parts) is supposed to be a backup if a helmet fills with water, as what occurred during a July 2013 spacewalk. Credit: NASA (YouTube/screenshot)

So what are some key parts of the spacewalks to look for? Wheelock identified a few spots.

‘HAP’ check. That soaker pad is called a “helmet absorption pad”, and as a matter of course the astronauts will be asked to verify that the pad is not wet at the same time that they also check their gloves for tears (another lesson learned from a past spacewalk.) So you will hear Wheelock calling “HAP check” from time to time to the crew.

Unlatching and latching the ammonia connectors on the pumps. Because this is when leaks are most likely to occur — posing a risk to Mastracchio, who is performing the work — Wheelock is going to do a “challenge and response” procedure. He will read up the step, the astronaut will verify it and will do the work. There will be “a lot more chatter on the [voice] loop” during those times, Wheelock said, with everyone on the ground watching through Mastracchio’s head camera feed (visible at the front of the room) to see what is happening. “There will be a lot of people standing in Mission Control at that point,” he joked, himself included.

Leak procedures. If ammonia does start to shower out, Mastracchio will quickly close the valve and wait a few minutes as it could be just residual ammonia in the line. If that doesn’t work out, Mastracchio is trained on a procedure to attach a device to the front end of the connector and move a lever that prevents a cavity in the line from filling with ammonia. Then he can open the valve again, bleed out the ammonia that’s left over and keep going.

NASA astronaut Rick Mastracchio inspects two spacesuits to be used during spacewalks in December 2013. The spacewalks were to remove and replace a faulty ammonia pump. Credit: NASA TV

Decontamination procedures. The ammonia makes a distinctive “ping” when it hits the helmet, says Wheelock (who yes, heard that happen himself.) You can also see ammonia on the suit, he said, as it looks a bit like candle wax and obscures the stitching. All of which to say, NASA has procedures in place if the agency suspects or can confirm large amounts of ammonia got on Mastracchio’s suit. (Small amounts would essentially fleck off in the sun.) Hopkins, who will be out of the line of fire, can do a thorough inspection of Mastracchio and scrape off any ammonia with a warm metal tool — without hurting the suit underneath. The astronauts could also do a “bakeout” in the airlock — 30 minutes if suspected, an hour if confirmed — where they will sit with the hatch open and wait for any ammonia to sublimate off the suit. Once they close the hatch, the astronauts can verify if the ammonia is gone using Drager tubes, which have gold crystals inside that turn “purpleish blue” in the presence of ammonia, Wheelock said.

Margin calls. Because NASA needs to make sure the astronauts have 30 to 60 minutes to decontaminate at the end of their spacewalks, officials will preserve a margin of oxygen available for the astronauts to walk through that work. So it’s possible the agency may terminate a spacewalk before all tasks are completed just because they need that bit of margin at the end.

To learn more, Wheelock has been answering questions occasionally on his Twitter account from followers, and you can read through what he posts when he finds the time. Universe Today will also cover the spacewalks (currently planned for Saturday, Monday and Wednesday) as they occur.

December 18, 2013December 23, 2015 by Elizabeth Howell

Leaky Spacesuit Fixed For Christmas Spacewalk Blitz On Station, NASA Says

NASA astronaut Rick Mastracchio during a spacewalk on STS-118. Credit: NASA

When NASA astronaut Mike Hopkins steps into space for the first time this week, he will wear a spacesuit that previously sprung a water leak and forced Italian astronaut Luca Parmitano back to station in July, NASA officials said Wednesday (Dec. 18).

While at first glance this sounds like an extra bit of drama as Hopkins and Rick Mastracchio make contingency spacewalks Dec. 21, 23 and 25 to kickstart a shut-down cooling loop, NASA officials say the suit is ready to go for another trip outside because astronauts (under NASA’s direction) have made a bunch of changes to the unit.

Repurposing spacesuit parts, a new pad will be added to the back of all NASA spacesuit helmets to soak up water, should one leak again. Astronauts also velcroed a pipe into each suit — a sort of snorkel — that in the worst case, would give an astronaut with a water leak an alternate route for drawing in air.

Also, the Expedition 38 crew swapped out a fan pump separator that likely malfunctioned and caused the spacesuit leak. The cause is still under investigation, but NASA believes that a problem in the water chemistry caused contamination that plugged a tiny hole inside the water separation part of the unit. This allowed the water to escape, enter the air loop and get into the helmet.

Finally, there are new procedures in place for the astronauts themselves. They will monitor the helmet pad for fluid. NASA additionally plotted out its spacewalk procedures — which include the use of a Canadian robotic arm on station — to make sure the astronauts are always within reasonable reach of an airlock.

NASA astronauts Rick Mastracchio and Mike Hopkins will do spacewalks in December 2013 to swap out a cooling pump on the International Space Station. Credit: : NASA — NASA astronauts Rick Mastracchio and Mike Hopkins will do spacewalks in December 2013 to swap out a cooling pump on the International Space Station. Credit: NASA

So here’s why the spacewalks are happening: a week ago (Dec. 11), a flow control valve inside of a pump — the pump is located outside of the station — stopped regulating ammonia temperatures inside of an external cooling loop. The loop is required to, as the name implies, cool down space station electronics. The loop got too cold, it shut down automatically, and NASA took science experiments and redundant systems offline to deal with the problem. (The main problem is NASA can’t run a heat exchanger on Node 2, which affects experiments in the U.S. Columbus laboratory and Japanese Experiment Module. No completed research has been lost to date, however.)

After figuring out that it couldn’t control the valve again, NASA shifted its attention to an isolation valve upstream. That valve is only designed to be in two positions — opened or closed — but the hardware vendor said it could be used at spots in between to regulate the ammonia flow. So software engineers created a patch to make this happen, and uploaded it to station.

Throw in another element, however: the station is about to enter what’s called an annual “high beta” period, when orbital dynamics mean the sun will be shining on it for longer periods of time than usual. (Read more technical details here.) When the angle exceeds 60 degrees, for safety reasons NASA suspends all cargo flights to station as well as spacewalks. This year, it will happen between about Dec. 30, 2013 and Jan. 9, 2014.

The International Space Station in 2010. Credit: NASA

So if NASA spent time playing with the valve and found out it couldn’t work in the long run, a couple of problems could happen. First, it would be harder to do a spacewalk to fix it.

Also, the agency was weighing whether to allow Orbital Sciences to fly a Cygnus cargo flight this month, and felt that they could run into a problem where the spacecraft was ready to go, but NASA needed more time to fix the problem. So that’s why the spacewalk is happening.

Here’s a diagram of the pump that Mastracchio and Hopkins plan to replace:

A view of a pump module aboard the International Space Station that is used to maintain ammonia at the correct temperature in an external cooling loop. Credit: NASA

The “nominal” plan is for three spacewalks, but it could range anywhere from two to four depending on how things go. To put things simply, here’s how the spacewalks would go:

EVA 1: The pump with the broken valve would be disconnected and a spare pump (which is some distance away, but reachable using Canadarm2) would be prepped for the swap.
EVA 2: The pump with the broken valve would be removed and set aside while the spare pump is partially installed (meaning, only the bolts and electrical connections would be put in.)
EVA 3: The spare pump’s installation would be finished, and the pump with the broken valve would be stowed more permanently outside. NASA thinks that eventually, it could use that first pump again if astronauts installed a new valve on it, but that isn’t a need for the time being.

Flying Canadarm2 would be Japanese astronaut Koichi Wakata, who has operated every type of robotics currently in orbit. Mastracchio has six spacewalks under his belt already, while Hopkins will be on his first go.

If all goes to plan, NASA will not only swap out the pump, but also preserve the option for the Russians to proceed with a planned Dec. 27 spacewalk that is less urgent. In that case, the cosmonauts plan to swap out experiments, put in a foot restraint and install some cameras.

We’ll cover the spacewalks as they happen. They’re scheduled for Dec. 21, 23 and 25 at 7:10 a.m. EST (12:10 p.m. UTC) and should run about 6.5 hours each. Broadcasts will run live on NASA Television.

By the way, the pump with the problem is just three years old — astronauts had to make three spacewalks in 2010 to install it after a more severe failure. NASA characterized this situation as a more unusual failure and said this is not a symptom of an aging station at all.

Overview of the tasks that Rick Mastracchio and Mike Hopkins will perform during three spacewalks in December 2013 to remove and replace a pump with a faulty valve inside of it. The pump is required to maintain the external cooling system at the right temperature. Credit: NASA

December 17, 2013December 23, 2015 by Ken Kremer

How to See Spectacular Prime Time Night Launch of Antares Commercial Rocket to ISS on Dec. 19

Antares Launch – Maximum Elevation Map
The Antares nighttime launch will be visible to millions of spectators across a wide area of the Eastern US -weather permitting. This map shows the maximum elevation (degrees above the horizon) that the Antares rocket will reach during the Dec 19, 2013 launch depending on your location along the US east coast. Credit: Orbital Sciences[/caption]

UPDATE: The launch of Cygnus has been delayed until no earlier than January 7, 2014 due to the coolant leak at the International Space Station and necessary spacewalks to fix the problem. You can read more about the issue here and here.

WALLOPS ISLAND, VA – Orbital Sciences Corp. is marching forward with plans for a spectacular night blastoff of the firms privately developed Antares rocket and Cygnus cargo spacecraft on Thursday, Dec. 19 from a seaside pad at Wallops Island, Virginia on a mission for NASA that’s bound for the International Space Station (ISS).

The nighttime Antares liftoff is currently scheduled for prime time – at 9:19 p.m. EST from Launch Pad 0A at the Mid-Atlantic Regional Spaceport (MARS) at NASA Wallops Island, Virginia. It should be easily visible to tens of millions of residents along a wide swath of the US East Coast spanning from South Carolina to southern Maine – weather permitting.

Here’s our guide on “How to See the Antares/Cygnus Dec. 19 Night Launch” – with your own eyes – complete with viewing maps and trajectory graphics from a variety of prime viewing locations; including Philadelphia, NYC, Baltimore and historic landmarks in Washington, DC.

Update: launch postponed to mid-January 2014 to allow NASA astronauts to conduct 3 EVA’s to swap out the ammonia pump module and restore full cooling capacity to the ISS

It will be visible to spectators inland as well, stretching possibly into portions of West Virginia and western Pennsylvania.

For example; Here’s the expected view from Rocky’s famous workout on the steps of the Philadelphia Art Museum.

The viewing maps are courtesy of Orbital Sciences, the private company that developed both the Antares rocket and Cygnus resupply vessel aimed at keeping the ISS fully stocked and operational for science research.

Up top is the map showing the maximum elevation the rocket will reach in the eastern United States.

The flight is designated the Orbital-1, or Orb-1 mission.

Orb-1 is the first of eight commercial cargo resupply missions to the ISS by Orbital according to its Commercial Resupply Services (CRS) contract with NASA.

Of course you can still view the launch live via the NASA TV webcast.

This marks the maiden night launch of the two stage Antares rocket following a pair of daytime test and demonstration launches earlier this year, in April and September.

It’s important to note that the Dec. 19 liftoff is still dependent on NASA engineers resolving the significant issue with the ammonia cooling system that popped up late last week when a critical flow control valve malfunctioned.

If the pump valve can’t be brought back online, two American astronauts may make two or three unscheduled spacewalks starting later this week.

So in the event spacewalks are required, Antares launch could still slip a few days to the end of the launch window around Dec. 21 or Dec. 22. Thereafter the launch would be postponed until January 2014.

Here’s your chance to witness a mighty rocket launch – from the comfort of your home and nearby locations along the east coast.

And its smack dab in the middle of the Christmas and holiday season resplendent with shining bright lights.

Weather outlook appears rather promising at this time – 95% favorable chance of lift off.

The rocket was rolled out to the Wallops launch pad this morning by Orbital’s technicians.

Cygnus is loaded with approximately 1465 kg (3,230 lbs.) of cargo for the ISS crew for NASA.

NASA Television coverage of the Antares launch will begin at 8:45 p.m. on Dec. 19 – www.nasa.gov/ntv

Stay tuned here for Ken’s Antares launch reports from NASA Wallops Flight Facility, VA.

Ken Kremer

December 14, 2013December 23, 2015 by Ken Kremer

China’s Maiden Lunar Rover ‘Yutu’ Rolls 6 Wheels onto the Moon – Photo and Video Gallery

China’s first lunar rover separates from Chang’e-3 moon lander early Dec. 15, 2013. Screenshot taken from the screen of the Beijing Aerospace Control Center in Beijing. Credit: Xinhua/post processing by Marco Di Lorenzo/Ken Kremer
Updated- See below Photo Gallery of Yutu’s descent to lunar surface on Dec. 15, 2013[/caption]

China’s first ever lunar rover rolled majestically onto the Moon’s soil on Sunday, Dec. 15, barely seven hours after the Chang’e-3 mothership touched down atop the lava filled plains of the Bay of Rainbows.

Check out the gallery of stunning photos and videos herein from China’s newest space spectacular atop stark lunar terrain.

The six wheeled ‘Yutu’, or Jade Rabbit, rover drove straight off a pair of ramps at 4:35 a.m. Beijing local time and sped right into the history books as it left a noticeably deep pair of tire tracks behind in the loose lunar dirt.

The stunning feat was broadcast on China’s state run CCTV using images transmitted to Earth from cameras mounted on the Chang’e-3 lander and aimed directly at the rear of the departing moon buggy.

Watch this YouTube video from CCTV showing the separation of ‘Yutu’ from the lander:

The scene was reminiscent of NASA’s Mars Sojourner rover driving of the Mars Pathfinder lander back in 1997.

Chinese space engineers based at the Beijing Aerospace Control Center (BACC) carefully extended a pair of ramps out from the lander in a complex process, drove Yutu onto the ramps and then gently lowered them onto the moon’s soil.

China’s Change’-3 mission had just safely soft landed on the Moon hours only earlier on Saturday, Dec. 14 at 9:11 p.m. Beijing time, 8:11 EST at the Sinus Iridum region, or Bay of Rainbows.

China thus became only the 3rd country in the world to successfully land a spacecraft on Earth’s nearest neighbor after the United States and the Soviet Union.

A video grab shows China's first moon rover, Yutu, or Jade Rabbit, separating from Chang'e-3 moon lander early Dec. 15, 2013. The six-wheeled rover separated from the lander early on Sunday, several hours after the Chang'e-3 probe soft-landed on the lunar surface. Credit: Xinhua — A video grab shows China’s first moon rover, Yutu, or Jade Rabbit, separating from Chang’e-3 moon lander early Dec. 15, 2013. The six-wheeled rover separated from the lander early on Sunday, several hours after the Chang’e-3 probe soft-landed on the lunar surface. Credit: Xinhua

It’s been nearly four decades since the prior lunar landing was accomplished by the Soviet Union’s Luna 24 sample return spacecraft.

Read my detailed account of the Chang’e-3 landing on Dec. 14 – here.

1st post landing image transmitted from the Moon’s surface by China’s Chang’e-3 lunar lander on Dec. 14, 2013. Credit: CCTV/post processing by Marco Di Lorenzo/Ken Kremer

Watch this YouTube video compilation of CCTV’s Dec. 14 landing coverage:

Over 4600 images have already been transmitted by Chang’e-3 in less than a day on the Moon.

Tomorrow, the 120 kg Yutu rover will begin driving in a circle around the 1200 kg lander.

And the pair of lunar explorers will snap eagerly awaited portraits of one another!

The rover and lander are equipped with 8 science instruments multiple cameras, spectrometers, an optical telescope, ground penetrating radar and other sensors to investigate the lunar surface and composition.

The radar instrument installed at the bottom of the rover can penetrate 100 meters deep below the surface to study the Moon’s structure and composition in unprecedented detail, according to Ouyang Ziyuan, senior advisor of China’s lunar probe project, in an interview on CCTV.

Stay tuned here for Ken’s continuing Chang’e-3, LADEE, MAVEN, MOM, Mars rover and more news.

Ken Kremer

Yutu moves towards drive off ramp still atop the Chang’e-3 lander, shown in this screen shot from early Dec. 15, 2013. Credit: CCTV

Yutu atop the transfer ramp to lunar surface. Credit: CCTV

Yutu descends down the transfer ramp to lunar surface. Credit: CCTV

December 14, 2013December 23, 2015 by Ken Kremer

China Scores Historic Success as Chang’e-3 Rover Lands on the Moon Today

Photo taken on Dec. 14, 2013 shows a picture of the moon surface taken by the on-board camera of lunar probe Chang’e-3 on the screen of the Beijing Aerospace Control Center in Beijing. This marks the first time that China has sent a spacecraft to soft land on the surface of an extraterrestrial body. Credit: Xinhua/CCTV
Story updated[/caption]

China scored a stunning, history making success with the successful touchdown of the ambitious Chang’e-3 probe with the ‘Yutu’ rover on the surface of the Moon today, Dec. 14, on the country’s first ever attempt to conduct a landing on an extraterrestrial body.

The dramatic Chang’e-3 soft landing on the lava filled plains of the Bay of Rainbows occurred at about 8:11 am EST, 9:11 p.m. Beijing local time, 1311 GMT today.

The monumental feat is the first landing on the Moon by any entity in nearly four decades. It was broadcast live on CCTV, China’s state run television network.

Note: Read my related new story with a photo gallery of Yutu’s 6 wheels rolling onto lunar soil – here

This maiden Chinese moon landing marks a milestone achievement for China and clearly demonstrates the country’s technological prowess.

A tidal wave of high fives was unleashed by the huge teams of Chinese space engineers teams controlling the flight from the Beijing Aerospace Control Center (BACC).

There was also a huge sense of relief from the nail biting tension upon confirmation of the successful soft landing following many years of hard work and intense planning.

The Chang’e-3 mission entails the first soft landing on the Moon by anyone since the Soviet Union’s unmanned Luna 24 sample return vehicle touched down back in 1976.

Artists concept of the rocket assisted landing of China’s lunar probe Chang'e-3. — Artists concept of the rocket assisted landing of China’s lunar probe Chang’e-3.

China now joins an elite club of three, including the United States, who have mastered the critical technology required to successfully touch down on Earth’s nearest neighbor.

China’s space vision also stands in total contrast to the utter lack of vision emanating from so called political leaders in Washington, DC who stymie NASA and US science at every opportunity!

‘Yutu’ could very well serve as a forerunner for testing the key technologies required for a Chinese manned lunar landing in the next decade.

In one of its first acts from the surface, the landers life giving solar panels were deployed as planned within minutes of touchdown

The Chang’e-3 mission is comprised of China’s ‘Yutu’ lunar lander riding piggyback atop a much larger four legged landing vehicle.

The Chang’e-3 lander transmitted its first images of the moon in real time during its approach to the lunar surface during the final stages of the ongoing landing operation carried live by CCTV.

A total of 59 images were received instead of the 10 expected, said a CCTV commentator.

The voyage from the Earth to the Moon began 12 days ago with the flawless launch of Chang’e-3 atop China’s Long March 3-B booster at 1:30 a.m. Beijing local time, Dec. 2, 2013 (12:30 p.m. EST, Dec. 1) from the Xichang Satellite Launch Center, in southwest China.

Chang’e-3 made a rocket powered descent to the Moon’s surface today by firing the landing thrusters starting at the altitude of 15 km (9 mi) for a soft landing targeted to a preselected area on the Bay of Rainbows.

The powered descent was autonomous and took about 12 minutes.

The variable thrust engine can continuously vary its thrust power between 1,500 to 7,500 newtons. It was the biggest ever used by China in space said a commentator on CCTV.

The variable thrust engine enabled Chang’e-3 to reduce its deceleration as it approached the moon.

The descent was preprogrammed and controlled by the probe itself, not from the ground.

A descent camera was mounted on the lander’s belly

The 1200 kg lander is equipped with unprecedented terrain recognition equipment and software to hover above the landing site and confirm it was safe. This enabled the craft to avoid rock and boulder fields that could spell catastrophe even in the final seconds before touchdown if the vehicle were to land directly on top of them.

The descent engine fired until the lander was about hovering 100 meters above the lunar surface.

After determining it was safe to proceed, the lander descended further to about 3 meters. The engine then cut off and the lander free fell the remaining distance. The impact was cushioned by shock absorbers.

The solar panels soon unfurled. They are the most efficient Chinese solar panels available, said a CCTV commentator.

The Bay of Rainbows, or Sinus Iridum region, is located in the upper left portion of the moon as seen from Earth. You can see the landing site with your own eyes.

It was imaged in high resolution by China’s prior lunar mission – the Chang’e-2 lunar orbiter – and is shown in graphics herein.

The Yutu rover is also unfurling its solar panels and mast today.

Yutu, which translates as Jade Rabbit, stands 150 centimeters high, or nearly 5 feet – human height.

It weighs approximately 120 kilograms and sports a robotic arm equipped with advanced science instruments.

On Sunday, the six-wheeled ‘Yutu’ rover with a rocker bogie suspension similar to NASA’s Mars rovers will be lowered in stages to the moon’s surface in a complex operation and then drive off a pair of landing ramps to explore the moon’s terrain for at least three months.

In what promises to be a space spectacular, the lander and rover are expected to photograph one another soon after Yutu rolls onto the Bay of Rainbows.

They will work independently.

The rover and lander are equipped with multiple cameras, spectrometers, an optical telescope, ground penetrating radar and other sensors to investigate the lunar surface and composition.

The Chang’e-3 lander is powered by a combination of solar arrays and a nuclear battery said CCTV, in order to survive the two week long lunar nights.

Chinese space officials expect the lander will function a minimum of 1 year.

ESA’s network of tracking stations are providing crucial support to China for Chang’e-3 from launch to landing.

Stay tuned here for Ken’s continuing Chang’e-3, LADEE, MAVEN, MOM, Mars rover and more news.

Ken Kremer

December 13, 2013December 23, 2015 by Ken Kremer

China’s Chang’e-3 Moon Rover Descends to Lower Orbit Sets Up Historic Soft Landing

All systems appear to be “GO” for the world’s first attempt to soft land a space probe on the Moon in nearly four decades.

China’s maiden moon landing probe – Chang’e-3 – is slated to attempt the history making landing this weekend on a lava plain in the Bay of Rainbows, or Sinus Iridum region.

Chinese space engineers at the Beijing Aerospace Control Center (BACC) paved the way for the historic touchdown by successfully commanding Chang’e-3 to descend from the 100 km-high lunar circular orbit it reached just one week ago on Dec. 6, to “an elliptical orbit with its nearest point about 15 km away from the moon’s surface”, according to a statement from China’s State Administration of Science, Technology and Industry for National Defense (SASTIND).

UPDATE: CCTV is providing live landing coverage

The first pictures taken from the alien lunar surface in some 37 years are expected to be transmitted within days or hours of touchdown planned as early as Saturday, Dec. 14, at 9:40 p.m. Beijing local time, 8:40 a.m. EST.

CCTV, China’s state run network, carried the launch live. It remains to be seen whether they will have live coverage of the landing since there have been no programming announcements.

SASTIND said the orbit lowering thruster firing was “conducted above the dark side of the moon at 9:20 p.m.” on Dec. 10, Beijing local time.

Confirmation of the Chang’e-3 probes new, lower orbit was received four minutes later.

China's lunar probe Chang'e-3 entered an orbit closer to the moon on Dec. 10, 2013. (Xinhua) — China’s lunar probe Chang’e-3 entered an orbit closer to the moon on Dec. 10, 2013. Credit: Xinhua

If successful, the Chang’e-3 mission will mark the first soft landing on the Moon since the Soviet Union’s unmanned Luna 24 sample return vehicle landed back in 1976.

China would join an elite club of three, including the United States, who have mastered the critical technology to successfully touch down on Earth’s nearest neighbor.

The Chang’e-3 mission is comprised of China’s ‘Yutu’ lunar lander riding piggyback atop a much larger four legged landing probe.

Artists concept of the Chinese Chang'e 3 lander and rover on the lunar surface. Credit: Beijing Institute of Spacecraft System Engineering — Artists concept of the Chinese Chang’e-3 lander and rover on the lunar surface. Credit: Beijing Institute of Spacecraft System Engineering

Chang’e-3 will make a powered descent to the Moon’s surface on Dec. 14 by firing the landing thrusters at the altitude of 15 km (9 mi) for a soft landing in a preselected area on the Bay of Rainbows.

The powered descent will take about 12 minutes.

The variable thrust engine can continuously vary its thrust power between 1,500 to 7,500 newtons, according to Xinhua.

The Bay of Rainbows is located in the upper left portion of the moon as seen from Earth. It was imaged in high resolution by China’s prior lunar mission – the Chang’e-2 lunar orbiter.

The 1200 kg lander is equipped with terrain recognition equipment and software to avoid rock and boulder fields that could spell catastrophe even in the final seconds before touchdown if the vehicle were to land directly on top of them.

Chang’e-3 is powered by a combination of solar arrays and a nuclear device in order to survive the two week long lunar nights.

The six-wheeled ‘Yutu’ rover, with a rocker bogie suspension, will be lowered in stages to the moon’s surface in a complex operation and then drive off a pair of landing ramps to explore the moon’s terrain.

Yutu measures 150 centimeters high and weighs approximately 120 kilograms and sports a robotic arm equipped with science instruments.

The rover and lander are equipped with multiple cameras, spectrometers, an optical telescope, ground penetrating radar and other sensors to investigate the lunar surface and composition.

The radar instrument installed at the bottom of the rover can penetrate 100 meters deep below the surface to study the Moon’s structure and composition in unprecedented detail.

Stay tuned here for Ken’s continuing Chang’e-3, LADEE, MAVEN, MOM, Mars rover and more news.

Ken Kremer

December 13, 2013December 23, 2015 by Elizabeth Howell

This Picture Symbolizes The Changing Mission Of One Plucky Spacecraft

The Helix nebula is visible in the center of this image, surrounded by tracks of asteroids that are much closer to Earth (yellow dots). Click on the image to see them. The streaks you see are from satellites or cosmic rays. Credit: NASA/JPL-Caltech/UCLA

Besides being a darn pretty picture of the Helix nebula, this snapshot is a bit of symbolism for NASA. The spacecraft that nabbed this view is called the Wide-field Infrared Survey Explorer, or WISE. If you look very carefully — you may have to click on the picture for a closer view — you can see little dots showing the paths of asteroids in the picture. (The streaks are cosmic rays and satellites.)

WISE has an interesting history. It began as a telescope seeking secrets of the universe in infrared light, but ran out of coolant in 2010 and was repurposed for asteroid searching under the NEOWISE mission. It wrapped up its mission, was put into hibernation in February 2011, then reactivated this August to look for asteroids again for at least the next three years. You can see some pictures and data WISE collected during its mission below the jump.

It’s a nice way, NASA said, to celebrate the fourth anniversary of WISE’s launch. “WISE is the spacecraft that keeps on giving,” said Ned Wright of UCLA, who was the principal investigator of WISE before it transitioned into NEOWISE.

New results from NASA's NEOWISE survey find that more potentially hazardous asteroids, or PHAs, are closely aligned with the plane of our solar system than previous models suggested. Image credit: NASA/JPL-Caltech — Results from NASA’s NEOWISE survey find that more potentially hazardous asteroids, or PHAs, are closely aligned with the plane of our solar system than previous models suggested. Image credit: NASA/JPL-Caltech

This enormous section of the Milky Way galaxy is a mosaic of images from NASA's Wide-field Infrared Survey Explorer, or WISE. The constellations Cassiopeia and Cepheus are featured in this 1,000-square degree expanse. Image credit: NASA/JPL-Caltech/UCLA — This enormous section of the Milky Way galaxy is a mosaic of images from NASA’s Wide-field Infrared Survey Explorer, or WISE. The constellations Cassiopeia and Cepheus are featured in this 1,000-square degree expanse. Image credit: NASA/JPL-Caltech/UCLA

This oddly colorful nebula is the supernova remnant IC 443 as seen by WISE. Image credit: NASA/JPL-Caltech/UCLA

December 13, 2013December 23, 2015 by Elizabeth Howell

Why Exoplanet-Hunting Is ‘Like Seeing A Flea In A Lightbulb’

Artist's conception of the Kepler Space Telescope. Credit: NASA/JPL-Caltech

Exoplanets are really tiny compared to their host star, and it’s hard to imagine sometimes how astronomers can even find one of these worlds — let alone thousands of them. This nifty two-part series from PBS explains how it’s possible in an easy-to-understand and hilarious way. As an example, this is how they describe the Kepler space telescope’s capabilities:

“It can’t actually see those exoplanets because the stars that they surround are so big and bright. Instead, it looks for the tiny shadow of the planet as it passes in front of its parent star. If that sounds hard, that’s because it is. It’s like seeing a flea in a lightbulb in Los Angeles from New York City,” said host Joe Hanson in the video.

Near the end, he provides an interesting segway into the question of life beyond Earth: “The question we’re really interested in is not how common are planets, but how common are we.” That gets tackled in part 2 of the video, which you can see below the jump.

Remember that 2014 will be an interesting year for Kepler as NASA figures out what to do next with the observatory. It isn’t able to perform its primary mission (seeking exoplanets in Cygnus) because two of its four reaction wheels or pointing devices are malfunctioning. NASA, however, has an innovative fix on the books that could allow it to swing different fields of view during the year — check out this infographic for more details.

December 12, 2013December 23, 2015 by David Dickinson

IRIS Glimpses an Elusive Region of the Sun

An innovative solar observatory is adding a key piece to the puzzle of the enigma that is our Sun.

Its two of key questions in heliophysics: why does our Sun have a corona? And why is the temperature of the corona actually higher than the surface of the Sun?

This week, researchers released results from the preliminary first six months of data from NASA’s Interface Region Imaging Spectrograph, known as IRIS. The findings were presented at the Fall American Geophysical Union Meeting this past Monday.

IRIS was launched on June 27^th of this year on a Pegasus-XL rocket deployed from the belly of a Lockheed L-1011 aircraft flying out of Vandenberg Air Force Base. IRIS can focus in on a very specific interface region of the Sun sandwiched between the dazzling solar photosphere and the transition to the corona. To accomplish this, IRIS employs an ultraviolet slit spectrograph looking at ionized gas spectra.

IRIS in the clean room. The spacecraft is only about 2 metres in length, about the height of a person. (Credit: Lockheed Martin).

“The quality of images and spectra we are receiving is amazing,” IRIS Principal Investigator Alan Title said in a recent press release from the NASA Goddard Space Flight Center. While other missions may take over a decade to go from the drawing board to the launch pad, IRIS was developed and deployed into Low Earth Orbit in just 44 months.

IRIS offers scientists a new tool to probe the Sun and a complimentary instrument to platforms such as Hinode, the Solar Heliospheric Observatory (SOHO) and NASA’s Solar Dynamics Observatory. In fact, IRIS has a better resolution than SDO’s AIA imagers or Hinode when it comes to this key solar interface region. IRIS has a 20x greater resolution in time, and 25x the spatial resolution of any former space-based UV spectrometer deployed.

“We are seeing rich and unprecedented images of violent events in which gases are accelerated to very high velocities while being rapidly heated to hundreds of thousands of degrees,” said Lockheed Martin science lead on the IRIS mission Bart De Pontieu. These observations are key to backing up theoretical models of solar dynamics as well as testing and formulating new ones of how our Sun works.

IRIS bridges this crucial gap between the photosphere and the lower chromosphere of the Sun. While the solar surface roils at relatively placid 6,000 degrees Celsius, temperatures rise into the range of 2-3 million degrees Celsius as you move up through the transition region and into the corona.

Two key solar phenomena that are of concern to solar researchers can be examined by IRIS in detail. One is the formation of prominences, which show up as long looping swirls of solar material rising up from the surface of the Sun. Prominences can be seen from backyard telescopes at hydrogen alpha wavelengths. IRIS can catch and track their early modeling with unprecedented resolution. Images released from IRIS show the fine structure of targeted prominences as they evolve and rise off the surface of the Sun. When a prominence and accompanying coronal mass ejection is launched in our direction, disruption of our local space environment caused by massive solar storm can result.

Slit jaw spectra images (the two strips to the left) and imaging a spicules 9to the right as seen by IRIS. (Credit: NASA/IRIS). — Slit jaw spectra images (the two strips to the left) and imaging of spicules (to the right) as seen by IRIS. (Credit: NASA/IRIS).

The second phenomenon targeted by IRIS is the formation of spicules, which are giant columns of gas rising from the photosphere. Although the spicules look like hair-fine structures through Earth-based solar telescopes, they can be several hundred kilometres wide and as long as the Earth. Short-lived, spicules race up from the surface of the Sun at up to 240,000 kilometres per hour and seem to play a key role in energy and heat transfer from the solar surface up through the atmosphere. IRIS is giving us a view of the evolution of spicules for the first time, and they’re proving to be even more complex than theory previously suggested.

“We see discrepancies between these observations and the models, and that is great news for advancing knowledge. By seeing something we don’t understand, we have a chance of learning something new,” Said University of Oslo astrophysicist Mats Carlsson.

Like SDO and SOHO, data and images from IRIS are free for the public to access online. Though the field of view for IRIS is a narrow 2’ to 4’ arc minutes on a side – the solar disk spans about 30’ as seen from the Earth – IRIS gives us a refined view of “where the action is.”

Where is IRIS looking? This snapshot gives some context of the IRIS field of view (green and red boxes) and black and white insets versus SDO's AIA full disk view of the Sun. (Credit: NASA/SDO/IRIS). — Where is IRIS looking? This snapshot gives some context of the IRIS field of view (green and red boxes) and black and white insets versus SDO’s AIA full disk view of the Sun. (Credit: NASA/SDO/IRIS).

And this all comes at an interesting time, as our nearest star crosses the sputtering solar maximum for Cycle #24.

The equivalent of 50 million CPU hours were utilized in constructing and modeling what IRIS sees. The reconstruction was an international effort, spanning the Partnership for Advanced Computing in Europe, the Norwegian supercomputing collaboration, and NASA’s Ames Research Center.

IRIS also faced the additional challenge of weathering a 2.5 week period of inactivity due to the U.S. government shutdown this fall. Potential impacts due to sequestration remain an issue, though small explorer missions such as IRIS demonstrate how we can do more with less.

“We’ve made a giant step forward in characterizing the heat transfer properties of this region between the visible surface and the corona, which is key to understanding how the outer atmosphere of the Sun exists, and is key to understanding the outer atmosphere that the Earth lies in,” said Alan Title, referring to the tenuous heliosphere of the Sun extending out through the solar system.

Understanding the inner working of our Sun is vital: no other astronomical body has as big an impact on life here on Earth.

IRIS is slated for a two-year mission, though as is the case with most space-based platforms, researchers will work to get every bit of usefulness out of the spacecraft that they can. And it’s already returning some first-rate science at a relatively low production cost. This is all knowledge that will help us as a civilization live with and understand our often tempestuous star.