Exploring Venus By Airship: Cool Concept, But Certainly Not New

An artist concept of the view from an airship orbiting Venus. Credit: NASA Langley HAVOC team.

Venus presents a special challenge to space explorers. Yes, there is a surface, but hellish temperatures and atmospheric pressure on the surface of Venus has a tendency to crush spacecraft fairly quickly. Short of building a submarine-rated surface explorer, maybe there’s a better way to look at the hothouse planet? A newly proposed NASA concept suggests using airships. Yes, airships with people in them.

But as you will see below, balloons and airships have been discussed extensively in the past decade by NASA and the Europeans as the best way of exploring Venus without needing to touch its hellish surface.

Venus may seem nothing but a distraction to an agency that is talking about exploring Mars in the 2030s (with Orion’s recent uncrewed test being the first advertised step of that, although critics say it won’t get us to the Red Planet). Leaving that aside, however, exploring Venus by balloon is not a new idea at all, even within NASA. The backers of the High Altitude Venus Operational Concept (HAVOC) even argue we should head to Venus before Mars, as one of the co-leads recently told Universe Today.

“A human mission to Venus is not on a lot of people’s radar, but we’ve really enjoyed working on the concepts for this mission,” said Langley’s Chris Jones, project co-lead, in an interview with Universe Today’s Nancy Atkinson. “This was an internal study: what does the future of humankind in space look like? Frankly, we see Venus as potentially no later than the second planetary destination that humans might go to, after Mars or even before Mars.”

Artist's conception of the High Altitude Venus Operational Concept (HAVOC) mission, a far-out concept being developed by NASA, approaching the planet. Credit: NASA Langley Research Center/YouTube (screenshot)
Artist’s conception of the High Altitude Venus Operational Concept (HAVOC) mission, a far-out concept being developed by NASA, approaching the planet. Credit: NASA Langley Research Center/YouTube (screenshot)

Why? Jones explained that because it takes a shorter time to get to Venus, that makes it a “stepping stone or practice run” to get humans to Mars. “The best would be a long lived surface lander, but technology issues for surface robotic missions are pretty significant, and a human mission to surface is nearly insurmountable. What’s left is a good platform for a science mission at mid-level altitudes, and it paints a good picture for a human mission in the atmosphere at 50 kilometers.”

The proposed flight profile of the HAVOC airship at Venus.  Credit: Space Mission Analysis Branch, NASA Langley Research Center.
The proposed flight profile of the HAVOC airship at Venus. Credit: Space Mission Analysis Branch, NASA Langley Research Center.

The clouds of Venus, Jones said, present an ideal spot for humans to roam from a spacecraft. The conditions at 50 kilometers (31 miles) above the surface are about the same pressure and atmosphere as Earth.

“Air itself is a lifting gas at those altitudes,” he added, “so you don’t have to bring some ridiculous supply of helium for this to work. And the rest of the environmental parameters at 50 kilometers are actually quite nice: the gravity is about the same as on Earth’s surface, the atmospheric pressure is about the same as Earth, and we can potentially manufacture a significant amount of that air by processing carbon dioxide. These are some of the facts we saw early on that inspired us to do this.”

There also would be more solar power and protection from radiation than Mars, and the temperature — although fairly hot — would be possible to account for fairly easily in spacecraft designs.

Jones provided some details on how the crew would spend about 30 days exploring the planet after a journey there and back (440 days total). Bear in mind that the mission is just in the early stages of even thinking about development. Cost, timeline, approvals and many other hurdles would need to be overcome before it could even become a reality.

Details of the proposed HAVOC airship mission to Venus. Credit: Space Mission Analysis Branch, NASA Langley Research Center.
Details of the proposed HAVOC airship mission to Venus. Credit: Space Mission Analysis Branch, NASA Langley Research Center.

“The big parameters of Venus’ atmosphere is the big longitudinal winds,” Jones said. “If you just rode them, it would take you about 110 hours to circle the planet. The other component of winds would push you towards the poles. In order to stay near the equator where there is less turbulence, the airship would ride the longitudinal winds while using a propulsion system to counter those winds pushing you towards the poles.”

The concept arose from science objectives for the planet out of NASA’s Venus Exploration Analysis Group, Jones said, whose aims include understanding the atmosphere and its interaction with the surface. NASA’s Langley Research Center also has human objectives they considered, such as showing how people can work in deep space and develop advanced technologies to accomplish that.

The proposed Venus exploration plan for HAVOC. Credit: Space Mission Analysis Branch, NASA Langley Research Center.
The proposed Venus exploration plan for HAVOC. Credit: Space Mission Analysis Branch, NASA Langley Research Center.

The HAVOC mission would start with a series of phased exploration sorties. The first phase would be examining the Venusian atmosphere with a robotic mission, and the second would be crewed ride to orbit that would include deploying an uncrewed robotic airship in the atmosphere.

The third phase is the 30-day mission described above, while the fourth phase could potentially be as long as a year. If it gets to a Phase 5, that would be a “permanent presence in Venus’ atmosphere”, Jones said.

A size comparison of ships for the proposed HAVOC mission to Venus. Credit: Space Mission Analysis Branch, NASA Langley Research Center.
A size comparison of ships for the proposed HAVOC mission to Venus. Credit: Space Mission Analysis Branch, NASA Langley Research Center.

Of note: balloons have been discussed before within NASA, particularly by Venus exploration advocate Geoffrey Landis of NASA Glenn, and Jones told Universe Today that this new team found much inspiration from Landis’ previous work.

Universe Today interviewed Landis in 2008 about missions he proposed about human-colony airships and uncrewed solar-powered airplanes. And in this 2010 study, he suggested three ideas for exploring the surface using uncrewed low-altitude balloons. One would skim the clouds around 25 kilometers (15.6 miles) and two other concepts (more rigid, naturally), would fly about 5 kilometers (3 miles) high. This was presented at an American Institute of Aeronautics and Astronautics meeting that year.

The remaining core of the High Altitude Venus Operational Concept (HAVOC), a far-out mission being developed by NASA, in this artist's concept. Credit: NASA Langley Research Center/YouTube (screenshot)
The remaining core of the High Altitude Venus Operational Concept (HAVOC), a far-out mission being developed by NASA, in this artist’s concept. Credit: NASA Langley Research Center/YouTube (screenshot)

“A notable advantage of the carbon dioxide atmosphere of Venus is that this allows a much wider range of lifting gasses for a balloon; not merely the hydrogen or helium usually used for terrestrial balloons,” Landis wrote in the paper. “Oxygen and nitrogen, in fact, are lifting gasses in the Venus atmosphere (although not good ones). At the altitudes considered, two other lifting gasses are water (which is a gas at the temperatures considered) and ammonia.”

Landis was also not deterred by harsh surface conditions. While Venus’ surface is difficult — its  480 Celsius (900 Fahrenheit) thick atmosphere destroyed the Soviet Venera probes in minutes — he’s secured early-stage NASA funding for a robotic landsailing rover concept nicknamed “Zephyr”. “Sailing on Venus! How cool is that? The project will have an exceptional public engagement factor,” the description page for the Venus Landsailing Rover reads.

In a nutshell, Glenn has created electronics that can continue to function in temperatures similar to what are found on the surface. Simulations also show that solar cells would work, albeit at reduced efficiency. Hence the idea to use a heavily-reinforced landsail to take advantage of Venus’ 100-times-more-pressure-than-Earth atmosphere at the surface. Wind speeds are less than a meter of second, but have terrific force behind them. And at least some of Venus appears to be flat, with rocks only a centimeter thick in pictures from Venera.

Artist's concept for a landsail rover on Mars, based on an idea by NASA's Geoffrey Landis. Credit: NASA
Artist’s concept for a landsail rover on Mars, based on an idea by NASA’s Geoffrey Landis. Credit: NASA

Balloons have also been considered by the European Space Agency, particularly in the form of an uncrewed Venus Entry Probe discussed in detail in this presentation by Surrey Satellite Technology Ltd. It would include a Low Venus Orbiter that would map the planet to complement closer-to-ground measurements, a Venus Relay Satellite that would send information from the balloon, and the “aerobot” itself.

“The aerobot consists of a long-duration balloon and gondola … that will analyze the Venusian middle cloud layer at an altitude of ~55 km, where the environment is relatively benign. The balloon will deploy a swarm of active ‘ballast’ micro-sondes, which, once deployed, will determine vertical profiles of the lower atmosphere,” the presentation reads. More detailed information is available from this 2004 ESA workshop presentation by Surrey and this ESA webpage, which says the study was completed in 2005.

Students have even explored Venusian balloon ideas, such as in the 2014 Summer School Alpbach cosponsored by the European Space Agency. An uncrewed idea called EvolVe suggests a joint orbiter and balloon mission to see how tectonic activity and volcanoes affected the surface of Venus, among other scientific goals. The balloon would hover in the same general region, about 50 to 60 km (31 miles to 37 miles),  and probe the surface using radar and other tools. It’s one of two concepts selected for further investigation that could lead to a science conference presentation and/or science journal publication.

Look Out Below! Rosetta Will Give Its Comet A Close Buzz In February

A mosaic of images of Comet 67P/Churyumov–Gerasimenko taken from the Rosetta spacecraft Dec. 14. Credit: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0

Remember how breathless we felt when the Philae lander actually made it to the surface of its target comet a few weeks ago? Sure, the maneuvers didn’t go as planned, but the images the spacecraft obtained in its brief spurts of activity on the surface are still being shared and discussed eagerly by scientists (amid a controversial image release policy, to be sure.)

Well, the truck delivery for Philae — the Rosetta spacecraft, still doing maneuvers above — is going to do something special in February. The machine is going to scoot down real close to the comet, just before heating from the Sun could make it dangerous to do so due to gas and dust emissions.

The plan is to bring Rosetta to an astounding four miles (six kilometers) above Comet 67P/Churyumov–Gerasimenko, so close that the images sent back to Earth will have a resolution of just a few inches per pixel. Scientists hope to learn more about how reflective the comet is and also to better understand how gas is emitted as 67P draws close to the Sun.

A mosaic of images of Comet 67P/Churyumov–Gerasimenko taken from the Rosetta spacecraft Dec. 14. Credit: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0
A mosaic of images of Comet 67P/Churyumov–Gerasimenko taken from the Rosetta spacecraft Dec. 14. Credit: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0

“As the comet becomes more and more active, it will not be possible to get so close to the comet. So this opportunity is very unique,” stated Matt Taylor, the Rosetta project scientist from the European Space Research and Technology Center, in a NASA press release.

Rosetta’s closest view of the comet previous to this was a six-mile (10 kilometer) mapping orbit that it did for a short time before moving to release the Philae lander. After that, its orbit was expected to range between 20 km and 50 km (12.4 miles and 18.6 miles) through the end of this month.

Philae, meanwhile, made it down to the surface and did manage to send pictures back during its approximately 60 hours of activity, before shutting down due to a lack of sunlight hitting its solar panels. Philae is now wedged in a shady spot on the comet, but it’s possible more sunlight could fall in that area when the comet nears its closest approach to the Sun in 2015, between the orbits of Earth and Mars.

A handful of pictures from Philae were released or re-released publicly last week through ESA and NASA, with far more being shown at the American Geophysical Union annual meeting (see video above, and this link that requires free registration).

The European Space Agency is saying that about 20% of the mission’s science is expected to flow from Philae (at most), and 80% from Rosetta. Early results from both spacecraft present some intriguing properties about the comet. Based on the ratio of isotopes (types) of hydrogen on the comet, it’s more likely that it was asteroids that delivered water to Earth. Also, Philae was unable to dig very far into the surface, implying that underneath the dust must be something like a thick layer of ice.

A recent Rosetta blog post on the European Space Agency says that the team expects to take a break for the holidays from posting — unless, of course, they manage to track down the Philae lander in pictures. The location of the spacecraft is still unknown, but it’s believed that Rosetta’s high-resolution camera may be able to catch the lander or its glint — coupled with clues Philae’s experiments gave to its location.

Star Trekking: We Humans Can Beam Tools Into Space Without A Transporter

Expedition 42 astronaut Butch Wilmore holds up a 3-D-printed rachet, the first such tool made in space. Credit: NASA

In the 1960s, we thought the best way of sending stuff between Earth and space was through a transporter. These days, turns out all it takes is an e-mail and a special 3-D printer. The first tool created in space, a rachet, was made last week on the International Space Station using plans beamed from Earth. Now, we get to see if it actually works.

The printer has been active for a few weeks, making test items that had already been done on Earth. But for this particular item, manufacturer Made In Space chose to take an additional risk: creating a tool from plans that were done almost at the last minute, similar to how a real mission would work when astronauts have a sudden need for a part.

“Made In Space uplinked a design which did not exist when the printer was launched. In fact the ratchet was designed, qualified, tested, and printed in space in less than a week,” the company wrote on its blog.

NASA astronaut Butch Wilmore (Expedition 42 commander on the International Space Station) holds the first 3-D printed part made in space, which was created on Nov. 25, 2014. Credit: NASA
NASA astronaut Butch Wilmore (Expedition 42 commander on the International Space Station) holds the first 3-D printed part made in space, which was created on Nov. 25, 2014. Credit: NASA

And it wasn’t as simple as just sending up the plans and hoping for the best. NASA had to give the safety thumbs-up before it went up there. Also, the plans (once sent to the space station) were verified as okay to go by Made In Space engineers before the crew got the okay to print last week.

The rachet took about four hours to print in space, which is a heck of a lot faster than sitting around waiting for a cargo ship — especially when said ship is delayed, as what happened recently to the SpaceX Dragon that was supposed to launch on Friday (Dec. 19) and has now been pushed back to at least Jan. 6.

While the rachet could be of use for simple repairs in space, it won’t be staying up there long. Just as with all the other parts printed so far, it’s going to be sent back to Earth for analysis to make sure it can stand up to the rigors of a space mission. Made In Space will soon have a more robust printer going up to station, and wants to make sure all the kinks are worked out before then.

Source: Made In Space

NASA’s First Orion Crew Module Arrives Safely Back at Kennedy Space Center

Homecoming view of NASA’s first Orion spacecraft after returning to NASA’s Kennedy Space Center in Florida on Dec. 19, 2014 after successful blastoff on Dec. 5, 2014. Credit: Ken Kremer - kenkremer.com

KENNEDY SPACE CENTER, FL – After a history making journey of more than 66,000 miles through space, ocean splash down and over 2700 mile cross country journey through the back woods of America, NASA’s pathfinding Orion crew capsule has returned to its home base at the Kennedy Space Center in Florida.

“The Orion mission was a spectacular success,” said Jules Schneider, Lockheed Martin Program manager for Orion at KSC, during a homecoming event attended by space journalists including Universe Today on Friday, Dec. 19, 2014.

“We achieved 85 of 87 test objectives,” noted Schneider. “Only an up righting air bag did not deploy fully after splashdown. And we are looking into that. Otherwise the mission went extremely well.”

Orion’s early homecoming was unexpected and a pleasant surprise since it hadn’t been expected until next week just prior to Christmas.

Orion flew on its two orbit, 4.5 hour flight maiden test flight on the Exploration Flight Test-1 (EFT-1) mission that started NASA’s long road to send astronauts beyond Earth and eventually to Mars in the 2030s.

The media were able to see the entire Orion capsule from top to bottom, including the exposed, blackened and heat scorched heat shield which had to protect the vehicle from fiery reentry temperatures exceeding 4000 F (2200 C).

 Top view of NASA’s maiden Orion spacecraft after returning to NASA’s Kennedy Space Center in Florida on Dec. 19, 2014.   Credit: Ken Kremer - kenkremer.com

Top view of NASA’s maiden Orion spacecraft after returning to NASA’s Kennedy Space Center in Florida on Dec. 19, 2014. Credit: Ken Kremer – kenkremer.com

Orion is being stored for now inside the Launch Abort System Facility (LASF)

“The heat shield worked extremely well and did its job,” Schneider told Universe Today.

Engineers took three samples from the 16.5 foot diameter heat shield and they are in for analysis.

“I don’t know if you can tell, we’ve actually taken a few core samples off the heat shield already and we’re looking at those,” said Schneider. “We will be removing the heat shield from this vehicle later in February so we will get an ever better look at it.”

One of the main objectives was to test the heat shield during the high speed atmospheric plummet of about 20000 mph (32000 kph) that reached approximately 85% of what astronauts will experience during a return from future voyages to Mars and Asteroids in the next decade and beyond.

“All of Orion’s system performed very well,” Schneider told me in an interview beside Orion.

“And the capsule used only about 90 pounds of its about 300 pounds of hydrazine propellant stored on board.”

“All of the separation events went beautifully and basically required virtually no maneuvering fuel to control the attitude of the capsule. The expected usage was perhaps about 150 pounds.”

“Therefore there is a lot more hydrazine fuel on board than we expected. And we had to be cautious in transporting Orion across the country.”

Up close view of three core samples taken from the heat shield of NASA’s first Orion spacecraft after returning to NASA’s Kennedy Space Center in Florida on Dec. 19, 2014.   Credit: Ken Kremer - kenkremer.com
Up close view of three core samples taken from the heat shield of NASA’s first Orion spacecraft after returning to NASA’s Kennedy Space Center in Florida on Dec. 19, 2014. Credit: Ken Kremer – kenkremer.com

Lockheed Martin is the Orion prime contractor.

The Orion arrived module arrived back at KSC, Thursday afternoon after being hauled across our country mostly on back country roads, and with no publicity or fanfare, on an unmarked flat bed truck to minimize interaction with the public.

“It was like a black ops operation,” said one of the team members responsible to safely transporting Orion from Naval Base San Diego to KSC.

NASA obtained special permits to move Orion from all the states travelled between California and Florida.

“We didn’t want any publicity because the capsule was still loaded with residual toxic chemicals like ammonia and hydrazine.” These were used to power and fuel the capsule.”

Orion’s test flight began with a flawless launch on Dec. 5 as it roared to orbit atop the fiery fury of a 242 foot tall United Launch Alliance Delta IV Heavy rocket – the world’s most powerful booster – at 7:05 a.m. EST from Space Launch Complex 37 (SLC-37) at Cape Canaveral Air Force Station in Florida.

The unpiloted test flight of Orion on the EFT-1 mission ignited NASA’s roadmap to send Humans to Mars by the 2030s by carrying the capsule farther away from Earth than any spacecraft designed for astronauts has traveled in more than four decades.

Humans have not ventured beyond low Earth orbit since the launch of Apollo 17 on NASA’s final moon landing mission on Dec. 7, 1972.

Watch for more details and photos later.

NASA’s first Orion spacecraft blasts off at 7:05 a.m. atop United Launch Alliance Delta 4 Heavy Booster at Space Launch Complex 37 (SLC-37) at Cape Canaveral Air Force Station in Florida on Dec. 5, 2014.   Launch pad remote camera view.   Credit: Ken Kremer - kenkremer.com
NASA’s first Orion spacecraft blasts off at 7:05 a.m. atop United Launch Alliance Delta 4 Heavy Booster at Space Launch Complex 37 (SLC-37) at Cape Canaveral Air Force Station in Florida on Dec. 5, 2014. Launch pad remote camera view. Credit: Ken Kremer – kenkremer.com

Watch for Ken’s ongoing Orion coverage from onsite at the Kennedy Space Center about the historic launch on Dec. 5.

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer

Jules Schneider, Lockheed Martin Program manager for Orion at KSC, and Ken Kremer/Universe Today discuss Orion during arrival event at NASA’s Kennedy Space Center in Florida on Dec. 19, 2014.   Credit: Ken Kremer - kenkremer.com
Jules Schneider, Lockheed Martin Program manager for Orion at KSC, and Ken Kremer/Universe Today discuss Orion during arrival event at NASA’s Kennedy Space Center in Florida on Dec. 19, 2014. Credit: Ken Kremer – kenkremer.com

Rocket Issues force SpaceX and NASA to Postpone Falcon 9 Rocket Launch to January 2015

SpaceX Falcon 9 erect at Cape Canaveral launch pad 40 awaiting launch on Sept 20, 2014 on the CRS-4 mission. Credit: Ken Kremer - kenkremer.com

KENNEDY SPACE CENTER, FL – Due to technical problems encountered during a hot fire test of the first stage engines this week with the SpaceX Falcon 9 rocket, the planned Dec. 19 launch of the commercial rocket and NASA contracted Dragon cargo freighter to the International Space Station (ISS) on a critical resupply mission has been postponed a few weeks into the new year to Jan. 6 at the earliest “out of an abundance of caution,” SpaceX officials told Universe Today.

Prior to every launch, SpaceX performs an internally required full countdown dress rehearsal and hot fire test of the first stage propulsion systems.

The hot fire test attempted on Tuesday “did not run for its full duration” of about three seconds, SpaceX spokesman John Taylor confirmed to me.

Therefore SpaceX and NASA managers decided to postpone the launch in order to run another static fire test.

“We are opting to execute a second static fire test prior to launch,” Taylor said.

In light of the catastrophic failure of the Orbital Sciences Antares rocket and Cygnus cargo freighter, everything must be done to ensure a launch success.

Due to the large amount of work required to test and analyze all rocket systems and the impending Christmas holidays, the earliest opportunity to launch is Jan. 6.

SpaceX Falcon 9 first stage rocket will attempt precison landing on this autonomous spaceport drone ship soon after launch set for Dec. 19, 2014 from Cape Canaveral, Florida.  Credit: SpaceX/Elon Musk
SpaceX Falcon 9 first stage rocket will attempt precision landing on this autonomous spaceport drone ship soon after launch now reset for Jan. 6, 2015, from Cape Canaveral, Florida. Credit: SpaceX/Elon Musk

The SpaceX Falcon 9 rocket carrying the Dragon cargo freighter had been slated to liftoff on its next unmanned cargo run dubbed CRS-5 to the ISS under NASA’s Commercial Resupply Services (CRS) contract.

Here is the full update from SpaceX.

“While the recent static fire test accomplished nearly all of our goals, the test did not run the full duration. The data suggests we could push forward without a second attempt, but out of an abundance of caution, we are opting to execute a second static fire test prior to launch.”

“Given the extra time needed for data review and testing, coupled with the limited launch date availability due to the holidays and other restrictions, our earliest launch opportunity is now Jan. 6 with Jan. 7 as a backup.

New countdown clock at NASA’s Kennedy Space Center displays SpaceX Falcon 9 CRS-5 mission and recent Orion ocean recovery at the Press Site viewing area on Dec. 18, 2014.  Credit: Ken Kremer – kenkremer.com
New countdown clock at NASA’s Kennedy Space Center displays SpaceX Falcon 9 CRS-5 mission and recent Orion ocean recovery at the Press Site viewing area on Dec. 18, 2014. Credit: Ken Kremer – kenkremer.com

“The ISS orbits through a high beta angle period a few times a year. This is where the angle between the ISS orbital plane and the sun is high, resulting in the ISS’ being in almost constant sunlight for a 10 day period.

“During this time, there are thermal and operational constraints that prohibit Dragon from being allowed to berth with the ISS. This high beta period runs from 12/28/14-1/7/15”

“Note that for a launch on 1/6 , Dragon berths on 1/8.”

“Both Falcon 9 and Dragon remain in good health, and our teams are looking forward to launch just after the New Year.”

Watch for Ken’s ongoing SpaceX launch coverage from onsite at the Kennedy Space Center.

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer

SpaceX Falcon 9 Rocket to Attempt Daring Ocean Platform Landing with Next Launch

SpaceX Falcon 9 first stage rocket will attempt precison landing on this autonomous spaceport drone ship soon after launch set for Dec. 19, 2014 from Cape Canaveral, Florida. Credit: SpaceX/Elon Musk

KENNEDY SPACE CENTER, FL – In a key test of rocket reusability, SpaceX will attempt a daring landing of their Falcon 9 first stage rocket on an ocean platform known as the “autonomous spaceport drone ship” following the planned Friday, Dec. 19, blastoff on a high stakes mission to the International Space Station (ISS).

The SpaceX Falcon 9 rocket carrying the Dragon cargo freighter is slated to liftoff on its next unmanned cargo run, dubbed CRS-5, to the ISS under NASA’s Commercial Resupply Services (CRS) contract. In a late development, there is a possibility the launch could be postponed to January 2015.

The instantaneous launch window for the Falcon 9/Dragon is slated for 1:20 p.m from Space Launch Complex 40 at Cape Canaveral Air Force Station in Florida.

As the Dragon proceeds to orbit, SpaceX engineers will attempt to recover the Falcon 9 first stage via a precision landing for the first time “on a custom-built ocean platform known as the autonomous spaceport drone ship,” according to a SpaceX statement.

Testing operation of Falcon 9 hypersonic grid fins (x-wing config) launching on next Falcon 9 flight, CRS-5.   Credit: SpaceX/Elon Musk
Testing operation of Falcon 9 hypersonic grid fins (x-wing config) launching on next Falcon 9 flight, CRS-5. Credit: SpaceX/Elon Musk

“While SpaceX has already demonstrated two successful soft water landings, executing a precision landing on an unanchored ocean platform is significantly more challenging.”

SpaceX rates the chances of success at “perhaps 50% at best.”

Of course since this has never been attempted before, tons of planning is involved and lots can go wrong.

But this is space exploration, and it’s not for the meek and mild.

It’s time to go boldly where no one has gone before and expand the envelope if we hope to achieve great things.

SpaceX Falcon 9 erect at Cape Canaveral launch pad 40  awaiting launch on Sept 20, 2014 on the CRS-4 mission. Credit: Ken Kremer - kenkremer.com
A SpaceX Falcon 9 erect at Cape Canaveral launch pad 40 prior to launch on Sept 20, 2014, on the CRS-4 mission. Credit: Ken Kremer – kenkremer.com

The 14 story Falcon 9 will be zooming upwards at 1300 m/s (nearly 1 mi/s). Engineers will then relight the Merlin 1D first stage engines to stabilize and lower the rocket.

Four hypersonic grid fins had been added to the first stage and placed in an X-wing configuration. They will be deployed only during the reentry attempt and will be used to roll, pitch, and yaw the rocket in concert with gimballing of the engines.

Here’s a description from SpaceX:

“To help stabilize the stage and to reduce its speed, SpaceX relights the engines for a series of three burns. The first burn—the boostback burn—adjusts the impact point of the vehicle and is followed by the supersonic retro propulsion burn that, along with the drag of the atmosphere, slows the vehicle’s speed from 1300 m/s to about 250 m/s. The final burn is the landing burn, during which the legs deploy and the vehicle’s speed is further.”

“To complicate matters further, the landing site is limited in size and not entirely stationary. The autonomous spaceport drone ship is 300 by 100 feet, with wings that extend its width to 170 feet. While that may sound huge at first, to a Falcon 9 first stage coming from space, it seems very small. The legspan of the Falcon 9 first stage is about 70 feet and while the ship is equipped with powerful thrusters to help it stay in place, it is not actually anchored, so finding the bullseye becomes particularly tricky. During previous attempts, we could only expect a landing accuracy of within 10km. For this attempt, we’re targeting a landing accuracy of within 10 meters.”

Watch for Ken’s ongoing SpaceX launch coverage from onsite at the Kennedy Space Center.

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer

………….

Learn more about SpaceX, Orion, Antares, NASA missions and more at Ken’s upcoming outreach events:

Dec 18: “SpaceX CRS-5, Orion EFT-1, Antares Orb-3 launch, Curiosity Explores Mars,” Kennedy Space Center Quality Inn, Titusville, FL, evenings

New Pictures Of Philae’s Lonely Resting Spot On The Comet Emerge

This (in blue) is where the Philae lander came to rest on Comet 67P/Churyumov-Gerasimenko. The graphic is based on topographic modelling of the comet's nucleus and Philae's picture of a nearby cliff (in white). Credit: ESA/Rosetta/Philae/CNES/FD/CIVA

In scientific style, researchers are slowly narrowing down where the Philae lander arrived on Comet 67P/Churyumov-Gerasimenko. Earlier today (Dec. 17) at the American Geophysical Union meeting, more pictures from the European spacecraft were released showing its landing site and also what the terrain looked like underneath Philae as it bounced to its destination. The pictures were also placed on NASA’s website.

The lander is sleeping in a shady spot on the comet’s surface after the dramatic touchdown — actually, three touchdowns — on Nov. 12, when it flew for more than two hours across the surface and bounced as high as two miles (3.2 kilometers). This was partly because harpoons expected to secure it to the surface failed to deploy, and also because the comet crust was icier than expected, according to Gizmodo.

You can see in the diagram above Philae’s predicament; it’s wedged in a spot that doesn’t get a lot of sunlight, at least for now. That could change as 67P draws closer to the Sun in the late winter or early spring, but nobody yet knows for sure. And yes, the search for the landing site still continues in earnest, but the challenge now is the orbiting Rosetta spacecraft only has so much bandwidth to send back images, according to Wired. As more high-resolution OSIRIS (Optical, Spectroscopic, and Infrared Remote Imaging System) pictures arrive, scientists hope to figure out where it went.

Two pictures from Philae highlighted in today’s release are below. Will the lander take more? Scientists certainly hope so, but even if that doesn’t happen, the lander was only expected to return 20% of the science results in any case. Rosetta is still active and will stick with the comet through mid-2015, when 67P gets closest to the Sun.

The Philae lander captured a picture of a nearby cliff, nicknamed "Perihelion Cliff", on the nucleus of Comet 67P/Churyumov-Gerasimenko. Credit: ESA/Rosetta/Philae/CIVA
The Philae lander captured a picture of a nearby cliff, nicknamed “Perihelion Cliff”, on the nucleus of Comet 67P/Churyumov-Gerasimenko. Reports say this picture had been released before, but was processed to show more detail (such as the glare, believed to be reflection from the lander). Credit: ESA/Rosetta/Philae/CIVA
Philae's blurred view of the surface during its first bounce from Comet 67P/Churyumov-Gerasimenko on Nov. 12, 2014. The lander sailed for about two hours in the first bounce, made contact briefly, then bounced again before coming to rest. The black squares represent areas where data was not collected. Credit: ESA/Rosetta/Philae/CIVA
Philae’s blurred view of the surface during its first bounce from Comet 67P/Churyumov-Gerasimenko on Nov. 12, 2014. The lander sailed for about two hours in the first bounce, made contact briefly, then bounced again before coming to rest. The black squares represent areas where data was not collected. Credit: ESA/Rosetta/Philae/CIVA

Morning Star, We Hardly Knew Ya: Venus Express’ Best Discoveries In 8 Years

Artist's impression of Venus Express entering orbit in 2006. Credit: ESA - AOES Medialab

Venus Express is mostly dead. The spacecraft spent more than eight years faithfully relaying information from the Morning Star/Evening Star planet, but it’s now out of fuel, out of control and within weeks of burning up in the atmosphere.

While we mourn the end of the productive mission, the European Space Agency spacecraft showed us a lot about the planet that we once considered a twin to Earth. Some of the surprises, as you can see below, including a possibly slowing-down rotation, and the realization that volcanoes may still be active on the hellish planet.

False colour composite of a rainbow-like feature known as a ‘glory’, seen on Venus on 24 July 2011. The image is composed of three images at ultraviolet, visible, and near-infrared wavelengths from the Venus Monitoring Camera. The images were taken 10 seconds apart and, due to the motion of the spacecraft, do not overlap perfectly. The glory is 1200 km across, as seen from the spacecraft, 6000 km away. It's the only glory ever seen on another planet. Credit: ESA/MPS/DLR/IDA.
False color composite of a rainbow-like feature known as a ‘glory’, seen on Venus on 24 July 2011. The image is composed of three images at ultraviolet, visible, and near-infrared wavelengths from the Venus Monitoring Camera. The images were taken 10 seconds apart and, due to the motion of the spacecraft, do not overlap perfectly. The glory is 1200 km across, as seen from the spacecraft, 6000 km away. It’s the only glory ever seen on another planet. Credit: ESA/MPS/DLR/IDA.

Quick video summary: Venus Express found that the spacecraft’s rotation may have slowed down by 6.5 minutes between 1996 (when the Magellan spacecraft was in orbit) and 2012. The surprising information emerged when scientists discovered surface features weren’t in the expected areas, and couldn’t find any calculation errors between the data.

Animation of Venus’ southern polar vortex made from VIRTIS thermal infrared images; white is cooler clouds at higher altitudes. Credit: ESA/VIRTIS-VenusX/INAF-IASF/LESIA-Obs. de Paris (G. Piccioni, INAF-IASF)

Quick video summary: Volcanic flows may still be active on Venus’ surface, according to 2010 data from the mission. Scientists looked at surface areas that had not been “weathered” very much (indicating that they are relatively young) and detected at least nine spots where the heat in those zones is much higher than the areas around it.

Venus Express picture of clouds on the planet. Despite the planet being extremely hot, the spacecraft found a cold layer in the atmosphere at temperatures of about -175 degrees Celsius (-283 Fahrenheit) that is colder than anything on Earth. It's so chilling that carbon dioxide may freeze and fall as snow or ice. Credit: ESA/MPS/DLR/IDA
A picture of Venus’ clouds. Despite the planet being extremely hot, Venus Express found a cold layer in the atmosphere at temperatures of about -175 degrees Celsius (-283 Fahrenheit) that is colder than anything on Earth. It’s so chilling that carbon dioxide may freeze and fall as snow or ice. Credit: ESA/MPS/DLR/IDA
Artist's impression of Venus with the solar wind flowing around the planet, which has little magnetic protection. Venus Express found that a lot of water has bled into space over the years from the planet, which happens when the sun's ultraviolet radiation breaks oxygen and hydrogen molecules apart and pushes them into space. Credit: ESA - C. Carreau
Artist’s impression of Venus with the solar wind flowing around the planet, which has little magnetic protection. Venus Express found that a lot of water has bled into space over the years from the planet, which happens when the sun’s ultraviolet radiation breaks oxygen and hydrogen molecules apart and pushes them into space. Credit: ESA – C. Carreau

Gallery: Saturn Moons Show How Not To Be Seen In Cassini Images

Tethys is mostly obscured behind Rhea as the moons orbit Saturn. The picture was captured by the Cassini spacecraft in April 2012 and highlighted in December 2014. Credit: NASA/JPL-Caltech/Space Science Institute

Peekaboo! Tethys makes a (mostly in vain) attempt to hide behind Rhea in this picture taken by the Cassini spacecraft a couple of years ago, but highlighted by NASA in a recent picture essay. Besides the neat view of the orbital dance, one thing that is clearly visible between the two moons is the different colors — a product of their different surfaces. It turns out that Tethys’ bright surface is due to geysers from another moon.

“Scientists believe that Tethys’ surprisingly high albedo is due to the water ice jets emerging from its neighbor, Enceladus,” NASA stated. “The fresh water ice becomes the E ring [of Saturn] and can eventually arrive at Tethys, giving it a fresh surface layer of clean ice.”

Saturn has an astounding number of moons — 62 moons discovered so far, and 53 of them named, if you don’t count the spectacular ring that surrounds the planet. The collection of celestial bodies includes Titan, the second-biggest moon in the Solar System. It’s so big that it includes a thick atmosphere. (Ganymede, around Jupiter, is the biggest.)

Below are some other pictures of moons dancing around Saturn — some harder to spot than others. All images were taken by the Cassini spacecraft since it arrived at the planet in 2004.

Titan peeks from behind two of Saturn's rings. Another small moon Epimetheus, appears just above the rings. Credit: NASA/JPL/Space Science Institute
Titan peeks from behind two of Saturn’s rings. Another small moon Epimetheus, appears just above the rings. Credit: NASA/JPL/Space Science Institute
Saturn's moons Dione and Rhea appear conjoined in this optical illusion-like image taken by the Cassini spacecraft.  Credit: NASA/JPL/Space Science Institute
Saturn’s moons Dione and Rhea appear conjoined in this optical illusion-like image taken by the Cassini spacecraft. Credit: NASA/JPL/Space Science Institute
Saturn's rings, made dark in part as the planet casts its shadow across them, cut a striking figure before Saturn's largest moon, Titan.  Credit: NASA/JPL/Space Science Institute
Saturn’s rings, made dark in part as the planet casts its shadow across them, cut a striking figure before Saturn’s largest moon, Titan. Credit: NASA/JPL/Space Science Institute
Three of Saturn's moons bunch together in this image by Cassini.  Credit: NASA/JPL/Space Science Institute.  Click for larger image.
Three of Saturn’s moons bunch together in this image by Cassini. Credit: NASA/JPL/Space Science Institute. Click for larger image.
Saturns rings with Saturns moon Mimas in the foreground (credit: NASA)
Saturn’s rings with Saturn’s moon Mimas in the foreground (credit: NASA)
Titan and Tethys line up for a portrait of 'sibling' moons. Credit: NASA/JPL/Space Science Institute
Titan and Tethys line up for a portrait of ‘sibling’ moons. Credit: NASA/JPL/Space Science Institute