Zero G Living: Tough To Sustain, Harder To Study

Expedition 40 NASA astronaut Reid Wiseman participates in a spacesuit fit-check prior to his scheduled flight to space in May 2014. Credit: NASA

Small populations make it really hard to do scientific studies, because the sample size may not be representative of the population being studied. And that’s the challenge with spaceflight, right before you start: only so many people head up there and take part of your experiments. With less than 20 people heading to space per year these days, that’s a tiny population to do medical studies from.

“One of the advantages that terrestrial medicine has is a lot of people to study,” said Jean Sibonga, the bone lead of NASA’s human spaceflight program. “While we’re acquiring our data using the conventional clinical methods for testing bone health here on Earth, terrestrial medicine is running these same studies and getting the results sooner.”

But for a small group being studied, the science is highly professionalized. NASA’s scientists are part of many professional societies ranging from anesthesia to bone science to nutrition. They collaborate with people all over the world. And slowly, as the results come in, they say they are making progress in understanding how space deconditions our bodies and how to make them stronger again.

With bone — where for decades, physicians have tried to figure out which populations are most at risk for fractures — comes an example of another hurdle. The astronauts are young, usually 50 or below, making them statistically one of the least at risk for fractures until they expose themselves to microgravity. This means that comparing them to seniors is “clearly not an appropriate test for our population,” Sibonga said.

One challenge of spaceflight is comparing data from astronauts, in the prime of their career, to seniors. Both groups can have similar health issues, but for different reasons: astronauts are exposed to microgravity, while seniors have aged. Pictured are Expedition 40's Maxim Surayev (age 41) and Reid Wiseman (age 38). Credit: NASA/Victor Zelentsov
One challenge of spaceflight is comparing data from astronauts, in the prime of their career, to seniors. Both groups can have similar health issues, but for different reasons: astronauts are exposed to microgravity, while seniors have aged. Pictured are Expedition 40’s Maxim Surayev (age 41) and Reid Wiseman (age 38). Credit: NASA/Victor Zelentsov

But for what it’s worth, NASA has adapted international clinical guidelines to identify astronauts who have optimal bone health, and to see if the “countermeasures” — weight-bearing exercises — are having any success. This also means looking at the astronaut’s entire picture of health, from family history to medication intake to hormone levels, to see if these variables have any sorts of effect. (More on the results of these tests tomorrow.)

The issue with astronauts, Sibonga said, is they go through very rapid bone losses — even faster than what postmenopausal women experience. Astronauts lose about 1% of their bone density on average per month from their hip and spine. In aging women, vertebrae are the most affected and they can find themselves with “compression fractures” where the vertebrae collapse and their backs are stooped over.

Astronauts may be at risk, but it’s hard with tests on the space station to see if this is happening real time. This work has to wait until they get back to Earth. Sibonga said NASA is trying to fix that. “We’re doing market surveys, and if we find a promising technology for inflight monitoring, we will work to develop and validate these tests in these astronauts.”

Regular exercise is one way that astronauts prepare for the rigors of orbit. Here, Expedition 32 JAXA astronaut Akihiko Hoshide does maintenance on the International Space Station during a spacewalk in 2012. Credit: NASA
Regular exercise is one way that astronauts prepare for the rigors of orbit. Here, Expedition 32 JAXA astronaut Akihiko Hoshide does maintenance on the International Space Station during a spacewalk in 2012. Credit: NASA

Sometimes that technology comes from other sectors. The idea of “loading” not only applies to human health, but also to engineering. So some of the same models could have relevancy between engineering and humans. One device NASA has been testing on the ground is a quantitative computed tomography (QCT), an imager that quantifies the amount of bone mass an astronaut has in true three dimensions. From these QCT data, engineers can develop models to estimate the mechanical loads that would cause a bone to fracture. But only a handful of people have applied this engineering model to biological systems, Sibonga said.

Naturally, NASA is also interested in how much bone mineral density (BMD) comes back after a mission. BMD tests are done every three years in astronauts from the time they are selected (bearing in mind the technology was not available until about the mid-1990s). Uniquely, NASA also invites its astronauts back after they leave or retire to continue the tests — a practice even the military branches in the United States don’t do. This allows the agency to do long-term population studies on its astronaut corps.

Sibonga added that NASA’s science is proceeding at an aggressive pace, given the small population and mission schedules, and cited a few examples of research papers on skeletal health and femoral strength as examples.

This begins a three-part series on astronaut health. Tomorrow: How to exercise in zero G. Two days from now: Battling against what space does to your health.

Opportunity Overlooks Ridge for Spectacular Vista of Vast Martian Crater and Habitable Zone Ahead

NASA’s Opportunity Mars rover captures sweeping panoramic vista near the ridgeline of 22 km (14 mi) wide Endeavour Crater’s western rim. The center is southeastward and also clearly shows the distant rim. See the complete panorama below. This navcam panorama was stitched from images taken on May 10, 2014 (Sol 3659) and colorized. Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Ken Kremer-kenkremer.com

NASA’s Opportunity Mars rover captures sweeping panoramic vista near the ridgeline of 22 km (14 mi) wide Endeavour Crater’s western rim. The center is southeastward and also clearly shows the distant rim. See the complete panorama below. This navcam panorama was stitched from images taken on May 10, 2014 (Sol 3659) and colorized. Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Ken Kremer-kenkremer.com
More mosaics and 10 year route map below[/caption]

NASA’s incredibly long lived Opportunity rover has driven to the ridgeline of a Martian mountain and captured spectacular panoramic vistas peering down into the vast expanse of huge Endeavour crater and out along the jagged rim segments leading to her next target – which scientists believe holds minerals indicative of a habitable zone. See mosaic views above and below.

Since departing the world famous ‘Jelly Doughnut’ rock by the summit of ‘Solander Point’ in February, Opportunity has spent the past several months driving south and exploring intriguing rock outcrops on ‘Murray Ridge’ located along the eroded western rim of Endeavour Crater.

The renowned robot is now exploring a region of outcrops atop the rims ridge that’s a possible site harboring deposits of hydrated clay minerals, formed in the ancient past when Mars was warmer and wetter.

The ten year old Red Planet rover first reached the rim of Endeavour Crater in August 2011. She has captured numerous sweeping gorgeous vistas during her first of its kind expedition on the surface of another planet by an alien probe from Earth.

Read my earlier story detailing the top 10 discoveries from twin sisters Spirit and Opportunity according to Deputy Principal Investigator Prof. Ray Arvidson – here.

The gigantic crater spans 14 miles (22 kilometers) in diameter.

So there is endless enthralling terrain to investigate – for at least another 10 years!

The floor of Endeavour crater is filled with dark sand, brighter dust, and, in the distance, dusty haze, says NASA.

This vista of the Endeavour Crater rim was acquired by NASA's Mars Exploration Rover Opportunity's panoramic camera on April 18, 2014, from the southern end of "Murray Ridge" on the western rim of the crater. In mid-May, the rover approached the dark outcrops on the flank of the hill at right. The high peak in the distance on the right is informally named "Cape Tribulation" and is about 1.2 miles (2 kilometers) to the south of Opportunity's position when this view was recorded Credit: NASA/JPL-Caltech/Cornell Univ./Arizona State Univ.
This vista of the Endeavour Crater rim was acquired by NASA’s Mars Exploration Rover Opportunity’s panoramic camera on April 18, 2014, from the southern end of “Murray Ridge” on the western rim of the crater. In mid-May, the rover approached the dark outcrops on the flank of the hill at right. The high peak in the distance on the right is informally named “Cape Tribulation” and is about 1.2 miles (2 kilometers) to the south of Opportunity’s position when this view was recorded Credit: NASA/JPL-Caltech/Cornell Univ./Arizona State Univ.

Opportunity’s goal all the while has been to doggedly trek southwards towards exposures of aluminum-rich clays detected from orbit by NASA’s powerful Martian ‘Spysat’ – the Mars Reconnaissance Orbiter (MRO) – while gathering context data at rock outcrops at Murray Ridge along the winding way.

These aluminum-rich clay minerals, or phyllosilicates, likely formed billions of years ago in flowing liquid neutral water which is more conducive to life, compared to more acidic environments explored earlier in the mission, and is therefore potentially indicative of a Martian habitable zone and a scientific goldmine.

The science and engineering team has used the high resolution MRO spectral and imaging data to more efficiently direct Opportunity southwards along the Endeavour crater rim and towards the biggest caches of the clay minerals – which were detected at a mountainous rim segment called ‘Cape Tribulation’ and which is seen in the panoramic vistas.

Although Cape Tribulation still lies some 1.2 miles (2 kilometers) further south, the rover has just arrived at a region which the team believes shows the first signatures of the clay minerals.

NASA’s Opportunity Mars rover captures sweeping panoramic vista near the ridgeline of 22 km (14 mi) wide Endeavour Crater's western rim. The center is southeastward and the distant rim is visible in the center. An outcrop area targeted for the rover to study is at right of ridge.  This navcam panoram was stitched from images taken on May 10, 2014 (Sol 3659) and colorized.  Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Ken Kremer-kenkremer.com
NASA’s Opportunity Mars rover captures sweeping panoramic vista near the ridgeline of 22 km (14 mi) wide Endeavour Crater’s western rim. The center is southeastward and the distant rim is visible in the center. An outcrop area targeted for the rover to study is at right of ridge. This navcam panorama was stitched from images taken on May 10, 2014 (Sol 3659) and colorized. Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Ken Kremer-kenkremer.com

“The rover is exploring the region of aluminum-hydroxyl clay minerals seen from orbit,” said NASA in a mission update.

The six wheeled robot will utilize her mast mounted cameras and arm mounted microscopic imager (MI) and APXS spectrometer to gather images and measurements to unlock the mysteries of Mars ability to support life – past or present.

“The more we explore Mars, the more interesting it becomes. These latest findings present yet another kind of gift that just happens to coincide with Opportunity’s 10th anniversary on Mars,” said Michael Meyer, lead scientist for NASA’s Mars Exploration Program.

“We’re finding more places where Mars reveals a warmer and wetter planet in its history. This gives us greater incentive to continue seeking evidence of past life on Mars.”

Opportunity Mars rover peers over mountain ridge for gorgeous vista into floor and out to distant rim of 22 km (14 mi) wide Endeavour Crater.  This pancam camera view was assembled from images taken on May 16, 2014 (Sol 3665) with false color sky.  Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Ken Kremer-kenkremer.com
Opportunity Mars rover peers over mountain ridge for gorgeous vista into floor and out to distant rim of 22 km (14 mi) wide Endeavour Crater. This pancam camera view was assembled from images taken on May 16, 2014 (Sol 3665) with false color sky. Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Ken Kremer-kenkremer.com

And Opportunity is now power-rich following a series of fortuitous wind cleaning events that substantially cleared the dust off the power generating solar wing arrays.

The solar array energy production has reached 761 watt-hours compared to about 900 watt-hours at landing in 2004 and only about 270 watt-hours just before Christmastime in December 2013.

“Solar panels [are] cleanest since about sol 1600 [September 2008],” says mission science team member Larry Crumpler.

More power means more work time and more bonus science studies and data return.

So the robot survived magnificently through her 6th harsh Martian winter with plenty of science rich targets planned ahead during the southern hemisphere Martian spring and summer.

Opportunity by Solander Point peak – 2nd Mars Decade Starts here!  NASA’s Opportunity rover captured this panoramic mosaic on Dec. 10, 2013 (Sol 3512) near the summit of “Solander Point” on the western rim of Endeavour Crater where she starts Decade 2 on the Red Planet. She is currently investigating outcrops of potential clay minerals formed in liquid water on her 1st mountain climbing adventure. Assembled from Sol 3512 navcam raw images. Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Ken Kremer-kenkremer.com
Opportunity by Solander Point peak – 2nd Mars Decade Starts here!
NASA’s Opportunity rover captured this panoramic mosaic on Dec. 10, 2013 (Sol 3512) near the summit of “Solander Point” on the western rim of Endeavour Crater where she starts Decade 2 on the Red Planet. She is currently investigating outcrops of potential clay minerals formed in liquid water on her 1st mountain climbing adventure. Assembled from Sol 3512 navcam raw images. Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Ken Kremer-kenkremer.com

Today, May 24, marks Opportunity’s 3673nd Sol or Martian Day roving Mars – compared to a warranty of just 90 Sols.

So far she has snapped over 192,600 amazing images on the first overland expedition across the Red Planet.

Her total odometry stands at over 24.49 miles (39.41 kilometers) since touchdown on Jan. 24, 2004 at Meridiani Planum.

Meanwhile on the opposite side of Mars, Opportunity’s younger sister rover Curiosity is trekking towards gigantic Mount Sharp and just drilled into her 3rd Red Planet rock at Kimberley.

Stay tuned here for Ken’s continuing Curiosity, Opportunity, Orion, SpaceX, Boeing, Orbital Sciences, MAVEN, MOM, Mars and more planetary and human spaceflight news.

Ken Kremer

Traverse Map for NASA’s Opportunity rover from 2004 to 2014 - A Decade on Mars.  This map shows the entire path the rover has driven during a decade on Mars and over 3660 Sols, or Martian days, since landing inside Eagle Crater on Jan 24, 2004 to current location along Murray Ridge south of Solander Point summit at the western rim of Endeavour Crater and heading to clay minerals at Cape Tribulation.  Opportunity discovered clay minerals at Esperance - indicative of a habitable zone.  Credit: NASA/JPL/Cornell/ASU/Marco Di Lorenzo/Ken Kremer
Traverse Map for NASA’s Opportunity rover from 2004 to 2014 – A Decade on Mars
This map shows the entire path the rover has driven during a decade on Mars and over 3660 Sols, or Martian days, since landing inside Eagle Crater on Jan 24, 2004 to current location along Murray Ridge south of Solander Point summit at the western rim of Endeavour Crater and heading to clay minerals at Cape Tribulation. Opportunity discovered clay minerals at Esperance – indicative of a habitable zone. Credit: NASA/JPL/Cornell/ASU/Marco Di Lorenzo/Ken Kremer

Antares Rocket Engine Suffers Significant Failure During Testing

Hotfire test of Aerojet Rocketdyne AJ26 engines on the E-1 Test Stand at NASA’s Stennis Space Center on Jan 17, 2014. Credit: NASA

Hotfire test of Aerojet Rocketdyne AJ26 engines on the E-1 Test Stand at NASA’s Stennis Space Center on Jan 17, 2014. Credit: NASA
See up close AJ26 photos below[/caption]

A Russian built rocket engine planned for future use in the first stage of Orbital Sciences Corp. commercial Antares rocket launching to the International Space Station failed during pre-launch acceptance testing on Thursday afternoon, May 22, at NASA’s Stennis Space Center in Mississippi.

“There was a test failure at Stennis yesterday afternoon (May 22),” Orbital Sciences spokesman Barry Beneski told Universe Today.

The Aerojet Rocketdyne AJ26 rocket engine failed with extensive damage about halfway through the planned test aimed at qualifying the engine for an Antares flight scheduled for early next year.

“Engineers are examining data to determine the cause of the failure,” Beneski told me.

The test was initiated at about 3:00 p.m. EDT on Thursday and the anomaly occurred approximately 30 seconds into the planned 54-second test.

“It terminated prematurely, resulting in extensive damage to the engine,” Orbital said in a statement.

An investigation into the incident by Aerojet and NASA has begun. The cause of the failure is not known.

“During hot-fire testing on May 22 at NASA’s Stennis Space Center, Aerojet Rocketdyne’s AJ26 engine experienced a test anomaly. The company is leading an investigation to determine the cause,” Aerojet spokesperson Jessica Pieczonka told Universe Today.

Up close view of two AJ26 first stage engines at the base of an Antares rocket during exclusive visit by Ken Kremer/Universe Today.  These engines powered the successful Antares  liftoff on Jan. 9, 2014 at NASA Wallops, Virginia.  Credit: Ken Kremer - kenkremer.com
Up close view of two AJ26 first stage engines at the base of an Antares rocket at NASA Wallops during exclusive visit by Ken Kremer/Universe Today. These engines powered the successful Antares liftoff on Jan. 9, 2014 at NASA Wallops, Virginia. Credit: Ken Kremer – kenkremer.com

Fortunately no one was hurt.

“There were no injuries,” Pieczonka confirmed to me.

A team of NASA, Orbital Sciences Corporation, Aerojet Rocketdyne and Lockheed Martin engineers tests all of the AJ26 engines on the E-1 Test Stand at NASA’s Stennis Space Center before delivering them to the launch site at NASA’s Wallops Flight Facility in Virginia.

The testing program began in November 2010.

“Stennis will perform checkouts to the facility to ensure its operational integrity,” NASA Stennis spokesperson Rebecca Strecker told me.

Antares first stage is powered by a pair of liquid oxygen and kerosene fueled AJ26-62 engines that deliver a combined 734,000 pounds (3265 kilonewtons) of sea level thrust.

To date, the AJ26 engines have performed flawlessly through a total of three Antares launches from NASA’s Wallops Flight Facility in Virginia.

They measure 3.3 meters (10.9 feet) in height and weigh 1590 kg (3,500 lb.).

Side view of two AJ26 first stage engines at the base of an Antares rocket during exclusive visit by Ken Kremer/Universe Today.  These engines powered the successful Antares  liftoff on Jan. 9, 2014 at NASA Wallops, Virginia.  Credit: Ken Kremer - kenkremer.com
Side view of two AJ26 first stage engines at the base of an Antares rocket during exclusive visit by Ken Kremer/Universe Today. These engines powered the successful Antares liftoff on Jan. 9, 2014 at NASA Wallops, Virginia. Credit: Ken Kremer – kenkremer.com

The next Antares rocket is slated to blastoff on June 10 with the Cygnus cargo freighter on the Orb-2 resupply mission to the ISS.

As of today, it’s not known whether the June flight will have to be postponed.

“It is too early to tell if upcoming Antares flights will be affected,” Beneski said.

The most recent launch of the two stage rocket took place this past winter on Jan. 9, 2014 on the Orb-1 resupply mission.

Orbital Sciences technicians at work on two AJ26 first stage engines at the base of an Antares rocket during exclusive visit by Ken Kremer/Universe Today at NASA Wallaps.  These engines powered the successful Antares  liftoff on Jan. 9, 2014 at NASA Wallops, Virginia bound for the ISS.  Credit: Ken Kremer - kenkremer.com
Orbital Sciences technicians at work on two AJ26 first stage engines at the base of an Antares rocket during exclusive visit by Ken Kremer/Universe Today at NASA Wallaps. These engines powered the successful Antares liftoff on Jan. 9, 2014 at NASA Wallops, Virginia bound for the ISS. Credit: Ken Kremer – kenkremer.com

The AJ26 engines were originally known as the NK-33 and built in the Soviet Union for their manned moon landing program.

Aerojet extensively modified, checked and tested the NK-33 engines now designated as the AJ26-62 to qualify them for use in the first stage Antares core, which is manufactured in Ukraine by the Yuznoye Design Bureau and based on the Zenit launch vehicle.

“Each test of an AJ26 engine is exciting and affirming because it is in direct support of NASA’s commercial space flight efforts, as well as a continuation of a very successful Stennis partnership with Orbital and Aerojet Rocketdyne,” Stennis Director Rick Gilbrech said in an earlier statement.

Antares soars to space on Jan. 9, 2014 from NASA Wallops on Virginia coast on the Orb-1 mission to the ISS.  Photo taken by remote camera at launch pad. Credit: Ken Kremer - kenkremer.com
Antares soars to space on Jan. 9, 2014 from NASA Wallops on Virginia coast on the Orb-1 mission to the ISS. Photo taken by remote camera at launch pad. Credit: Ken Kremer – kenkremer.com

Orbital Sciences was awarded a $1.9 Billion supply contract by NASA to deliver 20,000 kilograms of research experiments, crew provisions, spare parts and hardware for 8 flights to the ISS through 2016 under the Commercial Resupply Services (CRS) initiative.

The June mission would be the second operational Antares/Cygnus flight.

SpaceX has a similar resupply contract using their Falcon 9 rocket and Dragon cargo carrier and just completed their 3rd operational mission to the ISS.

Ken Kremer

Antares rocket powered by AJ26 1st stage engines successfully launched on Jan. 9, 2014. Here it undergoes processing at the Horizontal Integration Facility at NASA Wallops, Virginia, during exclusive visit by  Ken Kremer/Universe Today.   Credit: Ken Kremer - kenkremer.com
Antares rocket powered by AJ26 1st stage engines successfully launched on Jan. 9, 2014. Here it undergoes processing at the Horizontal Integration Facility at NASA Wallops, Virginia, during exclusive visit by Ken Kremer/Universe Today. Credit: Ken Kremer – kenkremer.com

Private Dream Chaser Crewed Mini-Shuttle Design Advances through Rigorous Wind Tunnel Tests

Scale model of the Sierra Nevada Corporation’s (SNC) Dream Chaser is readied for wind tunnel testing at high speeds that simulate the conditions it will encounter during its flight through the atmosphere returning from space. Credit: NASA/David C. Bowen

The private Dream Chaser mini-shuttle being developed by Sierra Nevada Corp. (SNC) has successfully completed a series of rigorous wind tunnel tests on scale models of the spacecraft – thereby accomplishing another key development milestone under NASA’s Commercial Crew Program to restore America’s human spaceflight access to low Earth orbit.

Engineers from SNC and NASA’s Langley Research Center in Hampton, Virginia conducted six weeks of intricate testing with several different Dream Chaser scale model spacecraft to study its reaction to subsonic, transonic and supersonic conditions that will be encountered during ascent into space and re-entry from low-Earth orbit.

The tests are among the milestones SNC must complete to receive continued funding from the Commercial Crew Integrated Capability initiative (CCiCAP) under the auspices of NASA’s Commercial Crew Program.

The Dream Chaser is among a trio of US private sector manned spaceships being developed with seed money from NASA’s Commercial Crew Program in a public/private partnership to develop a next-generation crew transportation vehicle to ferry astronauts to and from the International Space Station (ISS) by 2017 – a capability totally lost following the space shuttle’s forced retirement in 2011.

Since that day, seats on the Russian Soyuz are US astronauts only way to space and back.

The SpaceX Dragon and Boeing CST-100 ‘space taxis’ are also vying for funding in the next round of contracts to be awarded by NASA around late summer 2014.

Dream Chaser commercial crew vehicle built by Sierra Nevada Corp docks at ISS
Dream Chaser commercial crew vehicle built by Sierra Nevada Corp docks at ISS

“What we have seen from our industry partners is a determination to make their components and systems work reliably, and in turn they’ve been able to demonstrate the complex machinery that makes spaceflight possible will also work as planned,” said Kathy Lueders, NASA’s Commercial Crew Program manager. “These next few months will continue to raise the bar for achievement by our partners.”

To prepare for the wind tunnel testing, technicians first meticulously hand glued 250 tiny sand grains to the outer surface of the 22-inch long Dream Chaser scale model in order to investigate turbulent flow forces and flight dynamic characteristics along the vehicle that simulates what the actual spacecraft will experience during ascent and re-entry.

Dream Chaser awaits launch atop United Launch Alliance Atlas V rocket
Dream Chaser awaits launch atop United Launch Alliance Atlas V rocket

Testing encompassed both the Dream Chaser spacecraft by itself as well as integrated in the stacked configuration atop the Atlas V launch vehicle that will boost the vehicle to space from Launch Complex 41 at Cape Canaveral Air Force Station in Florida.

The testing of the Dream Chaser model was conducted at different angles and positions and around the clock inside the Unitary Plan Wind Tunnel at NASA Langley to collect the data as quickly as possible.

“All the data acquired will be used to validate computer models and populate the Dream Chaser spacecraft performance database,” according to NASA test engineer Bryan Falman.

NASA says that the resulting data showed the existing computer models were accurate.

Additonal wind tunnel testing was done at NASA’s Ames Research Center in Moffett Field, California and the CALSPAN Transonic Wind Tunnel in New York.

The wind tunnel work will also significantly aid in refining the Dream Chaser’s design and performance as well as accelerate completion of the Critical Design Review (CDR) before the start of construction of the full scale vehicle for orbital flight tests by late 2016.



Video Caption: Engineers used a wind tunnel at NASA’s Langley Research Center in Hampton, Virginia, to evaluate the design of Sierra Nevada Corporation’s Dream Chaser spacecraft. Credit: NASA

“The aerodynamic data collected during these tests has further proven and validated Dream Chaser’s integrated spacecraft and launch vehicle system design. It also has shown that Dream Chaser expected performance is greater than initially predicted,” said Mark N. Sirangelo, corporate vice president and head of SNC’s Space Systems.

“Our program continues to fully complete each of our CCiCap agreement milestones assisted through our strong collaboration efforts with our integrated ‘Dream Team’ of industry, university and government strategic partners. We are on schedule to launch our first orbital flight in November of 2016, which will mark the beginning of the restoration of U.S. crew capability to low-Earth orbit.”

The Dream Chaser design builds on the experience gained from NASA Langley’s earlier exploratory engineering work with the HL-20 manned lifting-body vehicle.

“The NASA-SNC effort makes for a solid, complementary relationship,” said Andrew Roberts, SNC aerodynamics test lead. “It is a natural fit. NASA facilities and the extensive work they’ve done with the Dream Chaser predecessor, HL-20, combined with SNC’s engineering, is synergistic and provides great results.”

Dream Chaser will be reusable and can carry a mix of cargo and up to a seven crewmembers to the ISS. It will also be able to land on commercial runways anywhere in the world, according to SNC.

Left landing gear failed to deploy as private Dream Chaser spaceplane approaches runway at Edwards Air Force Base, Ca. during first free flight landing test on Oct. 26, 2103.   Credit: Sierra Nevada Corp.  See video below
Left landing gear failed to deploy as private Dream Chaser spaceplane approaches runway at Edwards Air Force Base, Ca. during first free flight landing test on Oct. 26, 2103. Credit: Sierra Nevada Corp. See video below

Stay tuned here for Ken’s continuing Sierra Nevada, Boeing, SpaceX, Orbital Sciences, commercial space, Orion, Curiosity, Mars rover, MAVEN, MOM and more planetary and human spaceflight news.

Ken Kremer

Scale models of NASA’s Commercial Crew program vehicles and launchers; Boeing CST-100, Sierra Nevada Dream Chaser, SpaceX Dragon. Credit: Ken Kremer/kenkremer.com
Scale models of NASA’s Commercial Crew program vehicles and launchers; Boeing CST-100, Sierra Nevada Dream Chaser, SpaceX Dragon. Credit: Ken Kremer/kenkremer.com

Curiosity says ‘Goodbye Kimberley’ after Parting Laser Blasts and Seeking New Adventures Ahead

The Mars Hand Lens Imager on NASA's Curiosity Mars rover provided this nighttime view of a hole produced by the rover's drill and, inside the hole, a line of scars produced by the rover's rock-zapping laser. The hole is 0.63 inch (1.6 centimeters) in diameter. The camera used its own white-light LEDs to illuminate the scene on May 13, 2014. Credit: NASA/JPL-Caltech/MSSS

NASA’s rover Curiosity said ‘Goodbye Kimberley’ having fulfilled her objectives of drilling into a cold red sandstone slab, sampling the tantalizing grey colored interior and pelting the fresh bore hole with a pinpoint series of parting laser blasts before seeking new adventures on the road ahead towards the inviting slopes of Mount Sharp, her ultimate destination.

Curiosity successfully drilled her 3rd hole deep into the ‘Windjama’ rock target at the base of Mount Remarkable and within the science waypoint at a region called “The Kimberley” on May 5, Sol 621.

Since then, the 1 ton robot carefully scrutinized the resulting 2.6 inches (6.5 centimeters) deep bore hole and the mound of dark grey colored drill tailings piled around for an up close examination of the texture and composition with the MAHLI camera and spectrometers at the end of her 7-foot-long (2 meters) arm to glean every last drop of science before moving on.

Curiosity’s panoramic view departing Mount Remarkable and ‘The Kimberley Waypoint’ where rover conducted 3rd drilling campaign inside Gale Crater on Mars. The navcam raw images were taken on Sol 630, May 15, 2014, stitched and colorized. Credit: NASA/JPL-Caltech/Ken Kremer – kenkremer.com/Marco Di Lorenzo
Curiosity’s panoramic view departing Mount Remarkable and ‘The Kimberley Waypoint’ where rover conducted 3rd drilling campaign inside Gale Crater on Mars. The navcam raw images were taken on Sol 630, May 15, 2014, stitched and colorized. Credit: NASA/JPL-Caltech/Ken Kremer – kenkremer.com/Marco Di Lorenzo

Multiple scars clearly visible inside the drill hole and on the Martian surface resulting from the million watt laser firings of the Mast mounted Chemistry and Camera (ChemCam) instrument left no doubt of Curiosity’s capabilities or intentions.

Furthermore she successfully delivered pulverized and sieved samples to the pair of onboard miniaturized chemistry labs; the Chemistry and Mineralogy instrument (CheMin) and the Sample Analysis at Mars instrument (SAM) – for chemical and compositional analysis.

Curiosity completed an “intensive investigation of ‘The Kimberley’, having successfully drilled, acquired and dropped samples into CheMin and SAM,” wrote science team member Ken Herkenhoff in an update.

“MAHLI has taken lots of excellent images of the drill hole, including some during the night with LEDs on, nicely showing the ChemCam LIBS spots.”

“The initial analysis of this new sample by Chemin is ongoing, requiring repeated overnight integration to build up high-quality data,” says Herkenhoff.

The rover’s earth bound handlers also decided that one drill campaign into Kimberley was enough.

So the rover will not be drilling into any other rock targets here.

Composite photo mosaic shows deployment of NASA Curiosity rovers robotic arm and two holes after drilling into ‘Windjana’ sandstone rock on May 5, 2014, Sol 621, at Mount Remarkable as missions third drill target for sample analysis by rover’s chemistry labs.  The navcam raw images were stitched together from several Martian days up to Sol 621, May 5, 2014 and colorized.   Credit: NASA/JPL-Caltech/Ken Kremer - kenkremer.com/Marco Di Lorenzo
Composite photo mosaic shows deployment of NASA Curiosity rovers robotic arm and two holes after drilling into ‘Windjana’ sandstone rock on May 5, 2014, Sol 621, at Mount Remarkable as missions third drill target for sample analysis by rover’s chemistry labs. The navcam raw images were stitched together from several Martian days up to Sol 621, May 5, 2014 and colorized. Credit: NASA/JPL-Caltech/Ken Kremer – kenkremer.com/Marco Di Lorenzo

And it may be a very long time before the next drilling since the guiding team of scientists and engineers wants desperately to get on and arrive at the foothills of Mount Sharp as soon as possible.

But the robot will undoubtedly be busy with further analysis of the ‘Windjana’ sample along the way, since there’s plenty of leftover sample material stored in the CHIMRA sample processing mechanism to allow future delivery of samples when the rover periodically pauses during driving.

This May 12, 2014, view from the Mars Hand Lens Imager (MAHLI) in NASA's Curiosity Mars Rover shows the rock target "Windjana" and its immediate surroundings after inspection of the site by the rover by drilling and other activities.  Credit:   NASA/JPL-Caltech/MSSS
This May 12, 2014, view from the Mars Hand Lens Imager (MAHLI) in NASA’s Curiosity Mars Rover shows the rock target “Windjana” and its immediate surroundings after inspection of the site by the rover by drilling and other activities. Credit: NASA/JPL-Caltech/MSSS

“Windjana” is named after a gorge in Western Australia.

It’s been a full year since the first two drill campaigns were conducted during 2013 at the ‘John Klein’ and ‘Cumberland’ outcrop targets inside Yellowknife Bay. They were both mudstone rock outcrops and the interiors were markedly different in color.

“The drill tailings from this rock are darker-toned and less red than we saw at the two previous drill sites,” said Jim Bell of Arizona State University, Tempe, deputy principal investigator for Curiosity’s Mast Camera (Mastcam).

“This suggests that the detailed chemical and mineral analysis that will be coming from Curiosity’s other instruments could reveal different materials than we’ve seen before. We can’t wait to find out!”

The science team chose Windjana for drilling “to analyze the cementing material that holds together sand-size grains in this sandstone,” says NASA.

Curiosity’s Panoramic view of Mount Remarkable at ‘The Kimberley Waypoint’ where rover conducted 3rd drilling campaign inside Gale Crater on Mars. The navcam raw images were taken on Sol 603, April 17, 2014, stitched and colorized. Credit: NASA/JPL-Caltech/Ken Kremer – kenkremer.com/Marco Di Lorenzo.  Featured on APOD - Astronomy Picture of the Day on May 7, 2014
Curiosity’s Panoramic view of Mount Remarkable at ‘The Kimberley Waypoint’ where rover conducted 3rd drilling campaign inside Gale Crater on Mars. The navcam raw images were taken on Sol 603, April 17, 2014, stitched and colorized. Credit: NASA/JPL-Caltech/Ken Kremer – kenkremer.com/Marco Di Lorenzo
Featured on APOD – Astronomy Picture of the Day on May 7, 2014

“The Kimberley Waypoint was selected because it has interesting, complex stratigraphy,” Curiosity Principal Investigator John Grotzinger, of the California Institute of Technology, Pasadena, told me.

Curiosity departed the ancient lakebed at the Yellowknife Bay region in July 2013 where she discovered a habitable zone with the key chemical elements and a chemical energy source that could have supported microbial life billions of years ago – and thereby accomplished the primary goal of the mission.

Windjama lies some 2.5 miles (4 kilometers) southwest of Yellowknife Bay.

Curiosity still has about another 4 kilometers to go to reach the foothills of Mount Sharp sometime later this year.

The sedimentary layers of Mount Sharp, which reaches 3.4 miles (5.5 km) into the Martian sky, is the six wheeled robots ultimate destination inside Gale Crater because it holds caches of water altered minerals. Such minerals could possibly indicate locations that sustained potential Martian life forms, past or present, if they ever existed.

Stay tuned here for Ken’s continuing Curiosity, Opportunity, Orion, SpaceX, Boeing, Orbital Sciences, LADEE, MAVEN, MOM, Mars and more planetary and human spaceflight news.

Ken Kremer

ESA Marks 50 Years of Cooperative Space Innovation

Illustration of the ESA Planck Telescope in Earth orbit (Credit: ESA)

In 1964 the European Launcher Development Organisation (ELDO) and the European Space Research Organisation (ESRO) were founded, on February 29 and March 20 respectively, marking the beginning of Europe as a major space power and player in the new international venture to explore beyond our planet. A decade later these two entities merged to become ESA, and the rest, as it’s said, is history.

The video above commemorates ESA’s service to the cooperation and innovation of European nations in space, and indeed the entire world with many of the far-reaching exploration missions its member states have developed, launched and maintained. From advanced communications and observational satellites to its many missions exploring the worlds of the Solar System to capturing the light from the beginning of the Universe, ELDO, ESRO, and ESA have pushed the boundaries of science and technology in space for half a century… and are inspiring the next generation to continue exploring into the decades ahead. So happy anniversary, ESA — I can only imagine what we might be looking back on in another 50 years!

Source: ESA. See more key dates from ESA’s history here

Watch the Trailer for “The Last Man on the Moon”

Gene Cernan on the Moon during the final EVA of the Apollo 17 mission, Dec. 13, 1972 (NASA/JSC scan)

On December 14, 1972, at about 5:40 a.m. GMT, Apollo 17 astronaut Eugene Andrew “Gene” Cernan returned to the lunar module Challenger after the end of the third mission EVA to join Harrison “Jack” Schmitt, completing nearly two and a half days of surface operations within the Taurus-Littrow site and officially becoming the last human to set foot upon the lunar surface. No one has returned since, and to this day the 80-year-old Cernan still holds the title of “last man on the Moon.”

If that’s not the perfect setup for a documentary film, I don’t know what is. Luckily for us there’s one in the works.

“The Last Man on the Moon,” from UK-based Mark Stewart Productions, tells the story of Gene Cernan and his accomplishments against the backdrop of the Apollo era, when superpowers competed for dominance in space and hotshot flyboys became international heroes. With firsthand accounts from Cernan himself and his family, along with several other astronauts and NASA celebrities, it’s an emotional and intimate account of America’s last lunar voyage.

Watch the trailer below:

According to IMDB the 99-minute documentary directed by Mark Craig is slated for release in the UK (and hopefully U.S.!) sometime this year, although an exact date isn’t listed. There have been advance screenings very recently, at some of which Cernan was present for Q&A sessions. Some viewers are calling it “the best space documentary they have seen” so needless to say I’m pretty excited about it!

You can keep up with the status of the film (and see some exclusive astronaut photos) by liking the Facebook page here and joining the mailing list on the official site.

And yes, we do need more films like this.

“I really wanted to reach out, stick it in my spacesuit and bring it home and show it to everybody: this is what it feels like.
– Gene Cernan

Earth over the LM seen from the Apollo 17 landing site (NASA/JSC scan)
Earth over the LM seen from the Apollo 17 landing site (NASA/JSC scan)

Video © Mark Stewart Productions. All rights reserved.

NASA Mars Lander InSight ‘Go’ For Construction

Artist's conception of the NASA InSight Mars lander. Credit: NASA/JPL-Caltech

It’s time to get ready for Mars, again! NASA has given the approval to begin construction on its 2016 mission, the Interior Exploration Using Seismic Investigations, Geodesy and Heat Transport (InSight) mission.

As the mission implies, the lander (which isn’t moveable) will focus on learning more about the inside of Mars. The idea is to figure out how terrestrial planets are “differentiated” inside between core, mantle and crust. Also, watchers of the Mars program may recognize some parts of the lander, as it will borrow the design from the successful Phoenix mission in 2008.

“We will incorporate many features from our Phoenix spacecraft into InSight, but the differences between the missions require some differences in the InSight spacecraft,” stated Stu Spath, InSight program manager at Lockheed Martin.

“For example, the InSight mission duration is 630 days longer than Phoenix, which means the lander will have to endure a wider range of environmental conditions on the surface.”

View of Mars' surface near the north pole from the Phoenix lander. Credit: NASA/JPL-Calech/University of Arizona
View of Mars’ surface near the north pole from the Phoenix lander. Credit: NASA/JPL-Calech/University of Arizona

NASA mission planners are still determining where InSight will go, but they expect it will be a site near the equator of Mars and that it will last at least two years on the surface.

The Mars lander will include a robotic arm with “surface and burrowing” instruments whose projects are led by the French and German space agencies, which are CNES (National Center of Space Studies) and DLR (German Center for Aerospace), respectively. CNES will contribute a seismic experiment to look at “Marsquakes” and when meteors smack the surface, while DLR’s science experiment will look at interior planetary heat.

Mars on March 8, 2014 shows not only clouds over Hellas but evening limb clouds. Credit: W.L. Chin
Mars on March 8, 2014 shows not only clouds over Hellas but evening limb clouds. Credit: W.L. Chin

The seismometer will sit on the surface, covered up to protect it from the cold and wind, while the heat-flow probe will be hammered in about three to five yards or meters. Investigators also plan an experiment that will communicate with NASA’s Deep Space Network antenna network to see how much the rotation of Mars wobbles, which could hint if the core of the Red Planet is solid or liquid. The mission will also include wind, temperature and pressure sensors, as well as a magnetometer.

“Mars actually offers an advantage over Earth itself for understanding how habitable planetary surfaces can form,” stated Bruce Banerdt, InSight principal investigator at NASA’s Jet Propulsion Laboratory. “Both planets underwent the same early processes. But Mars, being smaller, cooled faster and became less active while Earth kept churning. So Mars better preserves the evidence about the early stages of rocky planets’ development.”

Construction will be led by Lockheed Martin. You can check out more information about InSight at this website. NASA has several missions working at Mars right now, such as the Mars Curiosity rover, the Opportunity rover and the orbiting Mars Reconnaissance Orbiter and Mars Odyssey spacecraft.

Source: Jet Propulsion Laboratory

Saturn Aurora Sparkles In New Hubble Images

Several images of an aurora on Saturn's north pole taken in April and May 2013 by the Hubble Space Telescope. Credit: NASA/ESA, Acknowledgement: J. Nichols (University of Leicester)

It’s amazing to see what some flashes of light can tell us. New images the Hubble Space Telescope took of Saturn not only reveal auroras dancing in the north pole, but also reveal some interesting things about the giant planet’s magnetic field.

“It appears that when particles from the Sun hit Saturn, the magnetotail collapses and later reconfigures itself, an event that is reflected in the dynamics of its auroras,” the European Space Agency wrote in a description of the image.

“Saturn was caught during a very dynamic light show – some of the bursts of light seen shooting around Saturn’s polar regions traveled more than three times faster than the speed of the gas giant’s roughly 10-hour rotation period.”

And for those readers that remember the music video from Saturn that the Cassini spacecraft took — also of auroras — ESA said this new research complements what the other spacecraft did, too.

The research has been accepted for publication in Geophysical Research Letters.

Source: ESA

Return of the SpaceX-3 Dragon to Earth Caps Super Science Mission for NASA

SpaceX-3 Dragon cargo freighter was detached from the ISS at 8 AM ET on May 18, 2014 and released by station crew at 9:26 AM for splashdown in the Pacific Ocean with science samples and cargo. Credit: NASA

SpaceX-3 Dragon commercial cargo freighter was detached from the ISS at 8 AM EDT on May 18, 2014 and released by station crew at 9:26 AM for splashdown in the Pacific Ocean with science samples and cargo. Credit: NASA
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The 30 day flight of the SpaceX-3 Dragon commercial cargo freighter loaded with a huge cache of precious NASA science experiments including a freezer packed with research samples ended today with a spectacular departure from the orbiting lab complex soaring some 266 miles (428 km) above Earth.

Update 3:05 PM EDT May 18: SpaceX confirms successful splashdown at 3:05 p.m. EDT today.

“Splashdown is confirmed!! Welcome home, Dragon!”

Robotics officers at Mission Control at NASA’s Johnson Space Center detached Dragon from the Earth-facing port of the Harmony module at 8 a.m. EDT (1300 GMT) this morning, Sunday, May 18, 2014 using the stations Canadian-built robotic arm.

Engineers had earlier unbolted all 16 hooks and latches firmly connecting the vehicle to the station in preparation.

NASA astronaut Steve Swanson then commanded the gum dropped shaped Dragon capsule’s release from Canadarm2 as planned at 9:26 a.m. EDT (1326 GMT) while the pair were flying majestically over southern Australia.

The undocking operation was shown live on NASA TV.

The SpaceX Dragon commercial cargo craft was in the grips of the Canadarm2 before being released for a splashdown in the Pacific Ocean.  Credit: NASA
The SpaceX Dragon commercial cargo craft was in the grips of the Canadarm2 before being released for a splashdown in the Pacific Ocean. Credit: NASA

Swanson was assisted by Russian cosmonaut Alexander Skvortsov as the US- Russian team were working together inside the domed Cupola module.

Following the cargo ships release by the 57 foot long arms grappling snares, Swanson carefully maneuvered the arm back and away from Dragon as it moved ever so slowly in free drift mode.

It was already four feet distant within three minutes of release.

Three departure burns by the Dragon’s Draco maneuvering thrusters followed quickly in succession and occurred precisely on time at 9:29, 9:30 and 9:38 a.m. EST.

Dragon exited the 200 meter wide keep out zone – an imaginary bubble around the station with highly restricted access – at the conclusion of the 3rd departure burn.

“The Dragon mission went very well. It was very nice to have a vehicle take science equipment to the station, and maybe some day even humans,” Swanson radioed after the safe and successful departure was completed.

“Thanks to everyone who worked on the Dragon mission.”

The private SpaceX Dragon spent a total of 28 days attached to the ISS.

The six person international crew from Russia, the US and Japan on Expeditions 39 and 40 unloaded some 2.5 tons of supplies aboard and then repacked it for the voyage home.

The SpaceX resupply capsule is carrying back about 3500 pounds of spacewalk equipment, vehicle hardware, science samples from human research, biology and biotechnology studies, physical science investigations and education activities, as well as no longer needed trash.

“The space station is our springboard to deep space and the science samples returned to Earth are critical to improving our knowledge of how space affects humans who live and work there for long durations,” said William Gerstenmaier, associate administrator for human exploration and operations.

“Now that Dragon has returned, scientists can complete their analyses, so we can see how results may impact future human space exploration or provide direct benefits to people on Earth.”

Among the research investigations conducted that returned samples in the cargo hold were an examination of the decreased effectives of antibiotics in space, better growth of plants in space, T-Cell activation in aging and causes of human immune system depression in the microgravity environment.

The 10 minute long deorbit burn took place as scheduled at 2:10 p.m. EDT (1810 GMT) today.

Dragon returned to Earth for a triple parachute assisted splash down today at around 3:02 p.m. EDT (19:02 GMT) in the Pacific Ocean – some 300 miles west of Baja California.

Dragon is free flying after release from ISS at 9:26 a.m. EDT on May 18, 2014. Credit: NASA
Dragon is free flying after release from ISS at 9:26 a.m. EDT on May 18, 2014. Credit: NASA

It will be retrieved by recovery boats commissioned by SpaceX. The science cargo will be extracted and then delivered to NASA’s Johnson Space Center within 48 hours.

Dragon thundered to orbit atop SpaceX’s powerful new Falcon 9 v1.1 rocket on April 18, from Cape Canaveral, Fla.

This unmanned Dragon delivered about 4600 pounds of cargo to the ISS including over 150 science experiments, a pair of hi tech legs for Robonaut 2, a high definition Earth observing imaging camera suite (HDEV), the laser optical communications experiment (OPALS), the VEGGIE lettuce growing experiment as well as essential gear, spare parts, crew provisions, food, clothing and supplies to the six person crews living and working aboard in low Earth orbit.

Robonaut 2 engineering model equipped with new legs like those heading to the ISS on upcoming SpaceX CRS-3 launch were on display at the Kennedy Space Center Visitor Complex on March 15, 2014. Credit: Ken Kremer - kenkremer.com
Robonaut 2 engineering model equipped with new legs like those delivered to the ISS on the SpaceX CRS-3 launch were on display at the Kennedy Space Center Visitor Complex on March 15, 2014. Credit: Ken Kremer – kenkremer.com

It reached the ISS on April 20 for berthing.

Dragon is the only unmanned resupply vessel supply that also returns cargo back to Earth.

The SpaceX-3 mission marks the company’s third resupply mission to the ISS under the $1.6 Billion Commercial Resupply Services (CRS) contract with NASA to deliver 20,000 kg (44,000 pounds) of cargo to the ISS during a dozen Dragon cargo spacecraft flights through 2016.

The SpaceX Dragon is among a trio of American vehicles, including the Boeing CST-100 and Sierra Nevada Dream Chaser vying to restore America’s capability to fly humans to Earth orbit and the space station by late 2017, using seed money from NASA’s Commercial Crew Program (CCP) in a public/private partnership. The next round of contracts will be awarded by NASA about late summer 2014.

Another significant milestone was the apparently successful attempt by SpaceX to accomplish a controlled soft landing of the Falcon 9 boosters first stage in the Atlantic Ocean for eventual recovery and reuse. It was a first step in a guided 1st stage soft landing back at the Cape.

The next unmanned US cargo mission to the ISS is set for early morning on June 10 with the launch of the Orbital Sciences Cygnus freighter atop an Antares booster from a launch pad at NASA’s Wallops Flight Facility on the eastern shore of Virginia.

Stay tuned here for Ken’s continuing SpaceX, Orbital Sciences, Boeing, commercial space, Orion, Chang’e-3, LADEE, Curiosity, Mars rover, MAVEN, MOM and more planetary and human spaceflight news.

Ken Kremer

………

Ken’s upcoming presentation: Mercy College, NY, May 19: “Curiosity and the Search for Life on Mars” and “NASA’s Future Crewed Spaceships.”