The Bigelow Expandable Activity Module (BEAM) will be launched onboard a SpaceX Dragon on Friday April 8th for a 2-year mission. Astronauts will test the module during that time. Image Bigelow Aerospace.
Space habitats have long been an object of fascination for thinkers, dreamers, and engineers. Science fiction is littered with space habitats, whether in books or movies. And their designs have ranged from titanic, uber-engineered types to fanciful, organic types.
Bigelow Aerospace is one company that is focused on creating affordable, practical space habitats. Inflatability is the name of the game for Bigelow, and now, one of their habitat modules is going to be tested on the ISS for a 2-year period. The BEAM, or Bigelow Expandable Activity Module, will be launched aboard a SpaceX Dragon on Friday April 8th, for a 2-day journey to the ISS.
The BEAM travels as an 8 foot bundle, but once it’s attached to the ISS, and inflated by astronauts, it will be large enough to hold a car. However, astronauts won’t be living inside it; rather, the BEAM will be tested for 2 years to see how it holds up. The objectives for this 2 year mission include:
Demonstrating launch and deployment, as well as folding and packing techniques.
Determining radiation protection capability.
Demonstrating design performance such as thermal, structural, mechanical durability, long-term leak performance, etc.
Increasing Technology Readiness Level (TRL) of expandable habitat technology
The BEAM with human figure for scale. Image: Bigelow Aerospace.
“The International Space Station is a uniquely suited test bed to demonstrate innovative exploration technologies like the BEAM,” said William Gerstenmaier, associate administrator for human exploration and operations at NASA Headquarters in Washington. “As we venture deeper into space on the path to Mars, habitats that allow for long-duration stays in space will be a critical capability. Using the station’s resources, we’ll learn how humans can work effectively with this technology in space, as we continue to advance our understanding in all aspects for long-duration spaceflight aboard the orbiting laboratory.”
The obvious risk to an inflatable space habitat is puncturing; not only from meteoroids, but from the growing population of space junk that inhabits Earth’s orbit. But BEAM is designed with this hazard in mind. It’s a thick-walled design, made from multiple layers of fabric similar to Kevlar. As far as space junk goes, BEAM should be impenetrable.
The BEAM is just a test module. It will hold only monitoring equipment, and will be entered by astronauts retrieving data and performing inspections. Bigelow Aerospace’s design for a usable habitat is the B330, a module large enough for 6 occupants, with a projected lifespan of 20 years. Test results from BEAM’s 2 years in space will help refine the design of the B330.
After its 2 years are up, BEAM will be released from the ISS and will be destroyed when it enters Earth’s atmosphere.
Orbital ATK Cygnus CRS-6/OA-6 space freighter arrives for capture and berthing at the International Space Station on Saturday, March 26, 2016 at 6:51 a.m. EDT. Credit: NASA/ESA/Tim Peake
Orbital ATK Cygnus CRS-6/OA-6 space freighter arrives for capture and berthing at the International Space Station on Saturday, March 26, 2016 at 6:51 a.m. EDT. Credit: NASA/ESA/Tim Peake
KENNEDY SPACE CENTER, FL – Following a perfectly executed three day orbital rendezvous, NASA astronaut and Expedition 47 Commander Tim Kopra successfully reached out with the International Space Station’s robotic arm, Canadarm2, grabbed hold and captured Orbital ATK’s commercial Cygnus cargo freighter at 6:51 a.m. EDT, this morning, Saturday, March 26, 2016.
The ISS and Cygnus were soaring some 250 miles (400 kilometers) over the Indian Ocean at the time of capture following the cargo crafts blastoff atop a two stage United Launch Alliance (ULA) Atlas V at 11:05 p.m. EDT on Tuesday, March 22, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, Fl.
Robotics officers on the ground in Houston working with the station crew high above then maneuvered Cygnus – holding over 3.5 tons of critical cargo supplies and science – into position for final installation and berthing to the orbiting laboratory’s Earth-facing port on the Unity module a few hours later. It was finally bolted fully into place at approximately 10:52 a.m. EDT.
Orbital ATK Cygnus CRS-6/OA-6 space freighter arrives for capture and berthing at the International Space Station on Saturday, March 26, 2016 at 6:51 a.m. EDT. Credit: NASA TV
This Cygnus is named the S.S. Rick Husband in honor of Col. Rick Husband, the late commander of Space Shuttle Columbia, which was tragically lost with its crew of seven NASA astronauts during re-entry on its final flight on Feb. 1, 2003.
The crew plans to open the hatch to the SS Rick Husband tomorrow morning on Easter Sunday, March 26.
The Orbital ATK Cygnus CRS-6 space freighter is loaded with 3513 kg (7700 pounds) of science experiments and hardware, crew supplies, spare parts, gear and station hardware for the orbital laboratory in support of over 250 research experiments being conducted on board by the Expedition 47 and 48 crews.
A computer overlay with engineering data provides video of the Canadarm2 robotic arm maneuvering to capture the Orbital ATK Cygnus OA-6 space freighter on Saturday, March 26, 2016 at 651 a.m. EDT. Credit: NASA TV
All of Cygnus maneuvers were “executed to perfection for a flawless approach and rendezvous” after the three day trip from Florida to the ISS, as the vehicle closed in to within a few meters for grappling, said NASA commentator Rob Navius.
NASA TV showed spectacular HD views of Cygnus and its UltraFlex solar arrays – deployed 2 hours after launch – from station and robotic arm cameras during the final approach operation, as flight controllers closely monitored all spacecraft systems.
“The crew is ready for Cygnus approach to the capture point,” radioed Kopra.
“Station you are go for capture,” Mission Control radioed back.
Cygnus was placed into free drift mode before capture to prevent any accidental perturbations in the final seconds.
From his robotics work station in the Cupola, Kopra then put the arm in motion by about 6:40 a.m. EDT, during the final phase of the final approach. He extended the 57 foot long (19 meter long) arm to reach out and grab the aft end of Cygnus cargo craft at its grappling pin by closing the snares on the end effector.
ESA astronaut Tim Peake served as backup for arm operations while NASA astronaut Jeff Williams monitored Cygnus systems.
The SS Rick Husband was rock steady during its capture as the station was flying over South Africa and the Indian Ocean.
“Capture confirmed,” reported Navius just moments before the video downlink was temporarily lost as the station communications moved between satellites.
“Excellent work gentleman. Much appreciated. Made that look easy,” radioed Jeremy Hansen, a Canadian Space Agency astronaut from Houston mission control.
“We’d also like to say we are really honored to bring aboard the SS Rick Husband to the International Space Station,” radioed Kopra. “He was a personal hero to many of us. This will be the first Cygnus honoree who was directly involved with the construction of this great station.”
A Cygnus cargo spacecraft named the SS Rick Husband is being prepared inside the Payload Hazardous Servicing Facility at NASA’s Kennedy Space Center for upcoming Orbital ATK CRS-6/OA-6 mission to deliver hardware and supplies to the International Space Station. The Cygnus is scheduled to lift off atop a United Launch Alliance Atlas V rocket on March 22, 2016. Credit: Ken Kremer/kenkremer.com
It took about 9 minutes to complete the approach from the 30 meter distant hold point to the final capture point where the SS Rick Husband Cygnus arrived at about 6:37 am EDT. NASA TV showed the grapple fixture gradually coming into view.
Cygnus approached precisely within the center of the approach corridor, said Peake, during continuing updates as the ship moved closer to the targeted berthing port. It was perfectly aligned for its capture point.
Cygnus grapple fixture is located at the bottom end of the vehicles service module, beside the thruster.
Kopra and Peake are spending their 103rd day on the station today. While Williams arrived just 8 days ago.
All burns to get to the initial rendezvous point in the keep out sphere 250 meters away were “right on the money. Every burn has been on course and on target, said NASA JSC commentator Navius in Houston, as Cygnus soared some 400 km over the Pacific.
“Everything has gone off without a hitch. A rock solid approach.”
Flight controllers in Houston and Orbital ATK’s Dulles control headquarters then gave the go ahead to resume moving and approach closer to the 30 meter hold point.
The actual berthing operation took place about an hour later than expected to double check that everything was precisely aligned and communications were fully established.
Controllers used the arm to move Cygnus in for capture. They commanded four gangs of four bolts to latch Cygnus to the common berthing mechanism (CBM) on the internally positioned Unity modules nadir or Earth-facing port.
The first and second stage captures were successfully completed by 10:52 a.m. EDT this morning, marking the official hard mating of Cygnus and the station.
When the ISS Expedition 47 crew members open the hatch, they will be greeted with a sign noting the spacecraft was named SS Rick Husband in honor of the STS-107 mission commander.
Orbital ATK #Cygnus mated to Unity module at 10:52 a.m. EDT (2:52 p.m. UTC). Graphic shows location of five spacecraft at station now. Credit: NASA
The SS Rick Husband Cygnus is actually at the vanguard of a “constellation” of three resupply ships arriving at the station over a three week period of three weekends.
Next comes the Russian Progress 63 which will dock at Russia’s Zvezda module next weekend after launching this Thursday from site 31 at Kaszakhstan carrying another three tons of supplies.
Following Progress is the SpaceX Return To Flight (RTF) mission dubbed SpaceX CRS-8.
It is slated to launch on April 8 and arrive at the ISS on April 10 for berthing to the Earth-facing port of the Harmony module – at the end of the station where NASA space shuttles formerly docked. It carries another 3.5 tons of supplies.
So altogether the trio of international cargo ships will supply over 12 tons of station supplies in rapid succession over the next 3 weeks.
This choreography will set up America’s Cygnus and Dragon resupply craft to simultaneously be present and reside attached at adjacent ports on the ISS for the first time in history.
A United Launch Alliance (ULA) Atlas V launch vehicle lifts off from Cape Canaveral Air Force Station carrying a Cygnus resupply spacecraft on the Orbital ATK CRS-6 mission to the International Space Station. Liftoff was at 11:05 p.m. EDT on March 22, 2016. The spacecraft will deliver 7,500 pounds of supplies, science payloads and experiments. Credit: Ken Kremer/kenkremer.com
Plans currently call for Cygnus to stay at station for approximately two months until May 20th, when it will be unbolted and unberthed for eventual deorbiting and reentry.
But first it will stay on orbit for about another eight days, said Orbital ATK’s Cygnus program manager Frank DeMauro in an interview with Universe Today.
After unberthing, Cygnus will be used to conduct several experiments including the Saffire-1 experiment, it will deploy nanosats from an externally mounted carrier, and the REBR experiment will monitor the burn-up of Cygnus during the fiery reentry into the Earth’s atmosphere, said DeMauro.
Orbital ATK’s attention then shifts to the next Cygnus launch on the Return to Flight, or RTF, mission of the firms Antares rocket from NASA Wallops on the eastern shore of Virginia.
OA-6 is only the second Cygnus to be launched atop a ULA Atlas V rocket, following the OA-4 mission last December.
The CRS-6/OA-6 flight is also the second flight of the enhanced Cygnus variant, that is over 1 meter longer and sports 50% more volume capability.
Thus it is capable of carrying a much heavier payload of some 3500 kg (7700 lbs) vs. a maximum of 2300 kg (5070 lbs) for the standard version.
Watch for Ken’s onsite launch reports direct from the Kennedy Space Center in Florida and continuing mission reports.
Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.
Video caption: Mobius video camera placed at Florida launch pad captures blastoff up close of Orbital ATK OA-6 (CRS-6) mission riding to orbit atop a United Launch Alliance Atlas V rocket on March 22, 2016 at 11:05 p.m. EDT from Space Launch Complex-41 on Cape Canaveral Air Force Station. Credit: Ken Kremer/kenkremer.com
A United Launch Alliance (ULA) Atlas V rocket carrying the Orbital ATK Cygnus OA-6 mission lifted off from Space Launch Complex 41 at 11:05 p.m. EDT on March 22, 2016 from Cape Canaveral Air Force Station, Fla. Credit: Ken Kremer/kenkremer.com
A United Launch Alliance (ULA) Atlas V rocket carrying the OA-6 mission lifted off from Space Launch Complex 41 at 11:05 p.m. EDT on March 22, 2016 from Cape Canaveral Air Force Station, Fla. The first stage is powered by RD-180 engines that shut down 6 seconds early for an undetermined reason. Credit: Ken Kremer/kenkremer.com
KENNEDY SPACE CENTER, FL – This week’s Atlas V rocket launch of a Cygnus cargo ship to the International Space Station (ISS) apparently experienced a first stage engine anomaly during the climb to space that required a longer firing of the boosters upper stage engine so the payload could successfully achieve the required orbit.
The stunningly beautiful nighttime blastoff of the United Launch Alliance (ULA) Atlas V from the Florida space coast on Tuesday, March 22, was not quite as flawless as initially thought and marred by the early engine shutdown which has now forced a postponement of the next planned Atlas V launch as company engineers painstakingly evaluate the data.
“The Centaur [upper stage] burned for longer than planned,” Lyn Chassagne, spokesperson for rocket maker ULA, told Universe Today.
“The ULA engineering team is reviewing the data to determine the root cause of the occurrence.”
The Centaur RL10C-1 powerplant had to make up for a thrust and velocity deficiency resulting from a 6 second shorter than planned firing of the Atlas V’s first stage RD-180 engines.
Indeed the Centaur had to fire for a minute longer than planned to inject Cygnus into its target orbit.
“The first stage cut-off occurred approximately 6 seconds early, however the Centaur was able to burn an additional approximately 60 seconds longer and achieve mission success, delivering Cygnus to its required orbit.”
“The team is evaluating the occurrence as part of the standard post-flight data analysis. Following successful spacecraft separation, Centaur performed a disposal burn,” Chessagne elaborated.
The two stage ULA Atlas V lifted off on time at 11:05 p.m. EDT on Tuesday, March 22, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, Fl, under a picturesque moonlit sky carrying an Orbital ATK Cygnus spacecraft on a resupply mission for NASA to the ISS.
Following a 21-minute ascent, the S.S. Rick Husband Cygnus spacecraft was successfully deployed into its intended orbit approximately 144 miles above the Earth, inclined at 51.6 degrees to the equator, Orbital ATK confirmed in a statement.
The Russian-made RD AMROSS RD-180 engines power the Atlas V first stage and the dual nozzle powerplants have been completely reliable in 62 Atlas launches to date.
The RD-180s were supposed to fire for 255.5 seconds, or just over 4 minutes. But instead they shut down prematurely resulting in decreased velocity that had to be supplemented by the Centaur RL10C-1 to get to the intended orbit need to reach the orbiting outpost.
The liquid oxygen/liquid hydrogen fueled Aerojet Rocketdyne RL10C-1 engine was planned to fire for 818 seconds or about 13.6 minutes. The single engine produces 22,900 lbf of thrust.
The cause of the first stage engine shortfall has not been announced. ULA has launched a thorough investigation to determine root cause as to whether for example it’s the RD-180 engine itself, a faulty sensor, fuel related, ground support equipment or a myriad of some other rocket components or issues.
A United Launch Alliance (ULA) Atlas V launch vehicle lifts off from Cape Canaveral Air Force Station carrying a Cygnus resupply spacecraft on the Orbital ATK CRS-6 mission to the International Space Station. Liftoff was at 11:05 p.m. EDT on March 22, 2016. The spacecraft will deliver 7,500 pounds of supplies, science payloads and experiments. Credit: Ken Kremer/kenkremer.com
Although the Atlas V did successfully launch and deploy the commercial Cygnus CRS-6/OA-6 spacecraft into the required orbit, the Centaur was pressed into extra duty in real time to propel the payload.
The Atlas V first and second stages are preprogrammed to swiftly react to a wide range of anomalous situations to account for the unexpected. The rocket and launch teams conduct countless simulations to react to off nominal situations.
“The Atlas V’s robust system design, software and vehicle margins enabled the successful outcome for this mission,” Chassagne said.
“As with all launches, we will continue to focus on mission success and work to meet our customer’s needs.”
At the post launch media briefing, ULA program manager for NASA missions Vern Thorp, said that “ in a little over 20 minutes we went from liftoff to delivering Cygnus into exactly the orbit that it wanted to be in. This was our second successful cargo mission [for Orbital ATK] since December.”
“We were targeting a 230 kilometer circular orbit and we came very close to that as we normally do, just a fraction of a kilometer off. Well within the normal dispersions.”
“We nailed it. We got Cygnus where it wants to go.”
Asked about the Centaur he said that the prelaunch predictions are based on preliminary trajectories and can vary depending on the actual conditions at launch.
“What I do know is that Centaur nailed the orbit. Like every mission, we’re going to do a very, very detailed post-flight review. We always do and we always have done that. That’s to make sure that everything performed properly. From everything we’ve seen so far, the mission was pretty nominal.”
Now as a result of the post-flight review into the engine anomaly and velocity shortfall, the next launch of the “Atlas V carrying the MUOS-5 mission for the U.S. Navy and the U.S. Air Force has been delayed to no earlier than May 12,” Chassagne added.
ULA needs to “further review the data anomaly experienced during the OA-6 mission.”
“The delay will allow additional time to review the data and to confirm readiness for the MUOS-5 mission.”
The Atlas V/MUOS-5 mission will lift off from the same pad at Space Launch Complex 41 on Cape Canaveral Air Force Station, Fl, whenever a launch target date is announced by ULA.
ULA Atlas V rockets to orbit with Orbital ATK Cygnus OA-6 from Space Launch Complex 41 on Cape Canaveral Air Force Station in Florida at 11:05 p.m. EDT on March 22, 2016. Credit: Julian Leek
Meanwhile the Cygnus CRS-6/OA-6 spacecraft continues chasing down the ISS for a planned arrival early Saturday morning, March 26.
The spacecraft will arrive at the station on Saturday, March 26. At that time Expedition 47 Commander Tim Kopra of NASA and Flight Engineer Tim Peake of ESA (European Space Agency) will grapple Cygnus, using the space station’s robotic arm, at approximately 6:40 a.m.
NASA TV coverage of rendezvous and grapple will begin at 5:30 a.m.
The Cygnus CRS-6/OA-6 payload of more than 16,000 pounds (7200 kg) weighed in as the heaviest payload to launch on an Atlas V to date.
A Cygnus cargo spacecraft named the SS Rick Husband is being prepared inside the Payload Hazardous Servicing Facility at NASA’s Kennedy Space Center for upcoming Orbital ATK CRS-6/OA-6 mission to deliver hardware and supplies to the International Space Station. The Cygnus is scheduled to lift off atop a United Launch Alliance Atlas V rocket on March 22, 2016. Credit: Ken Kremer/kenkremer.com
The Cygnus has been named the S.S. Rick Husband in honor of Col. Rick Husband, the late commander of Space Shuttle Columbia, which was tragically lost with its crew of seven NASA astronauts during re-entry on its final flight on Feb. 1, 2003.
Watch for Ken’s ongoing Cygnus launch reports.
Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.
Orbital ATK CRS-6 launch vehicle with the Cygnus cargo spacecraft bolted to the top of the Atlas V rocket is poised for launch at Space Launch Complex 41 at Cape Canaveral Air Force Station on March 22, 2016. Credit: Ken Kremer/kenkremer.com
These radar images of comet P/2016 BA14 were taken on March 23, 2016, by scientists using an antenna of NASA's Deep Space Network at Goldstone, California. At the time, the comet was about 2.2 million miles (3.5 million kilometers) from Earth. Credit: NASA/JPL-Caltech/GSSR
These radar images of comet P/2016 BA14 were taken on March 23, 2016, by scientists using an antenna of NASA’s Deep Space Network at Goldstone, California. At the time, the comet was about 2.2 million miles (3.5 million kilometers) from Earth. Credit: NASA/JPL-Caltech/GSSR
On March 22, Comet P/2016 BA14 (Pan-STARRS) flew just 2.2 million miles (3.5 million kilometers) from Earth, making it the third closest comet ever recorded. The last time a comet appeared on our doorstep was in 1770, when Lexell’s Comet breezed by at about half that distance. Through a telescope, comet BA14 looked (and still looks) like a faint star, though time exposures reveal a short, weak tail. With an excellent map and large amateur telescope you might still find it making a bead across the Big Dipper and constellation Bootes tonight through the weekend.
Flyby Comet Imaged by Radar
While normal telescopes show few details, NASA’s Goldstone Solar System Radar in California’s Mojave Desert pinged P/2016 BA14 with radar over three nights during closest approach and created a series of crisp, detailed images from the returning echoes. They show a bigger comet than expected — about 3,000 feet (one kilometer) across — and resolve features as small as 26 feet (8 meters) across.
“The radar images show that the comet has an irregular shape: looks like a brick on one side and a pear on the other,” said Shantanu Naidu, a researcher at NASA’s Jet Propulsion Laboratory. “We can see quite a few signatures related to topographic features such as large flat regions, small concavities and ridges on the surface of the nucleus.”
I honestly thought we’d see a more irregular shape assuming that astronomers were correct in thinking that BA14 broke off from its parent 252P/LINEAR though it’s possible it happened so long ago that the “damage” has been repaired by vaporizing ice softening its contours.
Comets are as dark as charcoal but appear light only because the sun illuminates them against the blackness of outer space. I shone a flashlight on a charcoal briquette (left) to simulate comet lighting. The same charcoal when viewed in normal light appears black. Credit: Bob King
Radar also shows that the comet is rotating on its axis once every 35 to 40 hours. While radar eyes focused on BA14, Vishnu Reddy, of the Planetary Science Institute, Tucson, Arizona, used the NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawaii to examine the comet in infrared light. He discovered its dark surface reflects less than 3% of the sunlight that falls on it. The infrared data is expected to yield clues of the comet’s composition as well.
Illustration of Comet 67P/Churyumov-Gerasimenko brought down to Earth in the city of Los Angeles, Calif. Not only can we appreciate its size but also its truly dark surface. Credit: ESA and anosmicovni
Comets are exceptionally dark objects often compared to the appearance of a fresh asphalt road or parking lot. They appear bright in photos because seen against the blackness of space, they’re still reflective enough to stand out. Comet 67P/Churyumov-Gerasimenko, still the apple of the orbiter Rosetta’s eye, is similarly dark, reflecting about 4% of sunlight.
What makes comets so dark even though they composed primarily of ice? Astronomers believe a comet grows a dark ‘skin’ both from accumulated dust and irradiation of its pristine ices by cosmic rays. Cosmic rays loosen oxygen atoms from water ice, freeing them to combine with simple carbon molecules present on comets to form larger, more complex and darker compounds resembling tars and crude oil. Dust settles on a comet’s surface after it’s set free from ice that vaporizes in sunlight.
What a view! Comet 67P/C-G photographed from a distance of just 7.5 miles (12 kilometers) on March 19, 2016 by Rosetta’s Navcam. The largest boulder to the right is Cheops, which stands about 82 feet (25 meters) high. Credit: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0
I live in Minnesota, where our annual State Fair features every kind of deep-fried food you can imagine: deep-fried Twinkies, deep-fried fruit, deep-fried bacon and even deep-fried Smores. Just now, I can’t shake the thought that comets are just another deep-fried confection made of pristine, 4.5-billion-year-old ice toasted by eons of sunlight and cosmic bombardment.
Long exposure streak shot of blastoff of United Launch Alliance Atlas V rocket carrying Orbital ATK's Cygnus spacecraft at 11:05 p.m. EDT on March 22, 2016, with foreground view of world famous Vehicle Assembly Building (VAB) at NASA’s Kennedy Space Center in Florida. Atlas V lifted off from nearby Space Launch Complex 41 on Cape Canaveral Air Force Station in Florida. Credit: Alex Polimeni/Spaceflight Now
Long exposure streak shot of blastoff of United Launch Alliance Atlas V rocket carrying Orbital ATK’s Cygnus spacecraft at 11:05 p.m. EDT on March 22, 2016, with foreground view of world famous Vehicle Assembly Building (VAB) at NASA’s Kennedy Space Center in Florida. Atlas V lifted off from nearby Space Launch Complex 41 on Cape Canaveral Air Force Station in Florida. Credit: Alex Polimeni/Spaceflight Now
KENNEDY SPACE CENTER, FL – Tuesday evening, March 22, turned into ‘streaks galore’ on Florida’s space coast, as the nighttime launch of an Orbital ATK Cygnus cargo freighter atop an Atlas V rocket was captured in unforgettable fashion by talented space photographers as it chases down the International Space Station (ISS), loaded with hundreds of science experiments.
Check out this expanding gallery of breathtaking photos and videos collected from many of my photojournalist friends and colleagues – who collectively count as the best space photographers worldwide!
We all descended on the sunshine state to record the Tuesday’s blastoff of the United Launch Alliance Atlas V rocket carrying Orbital ATK’s Cygnus CRS-6 (OA-6) spacecraft from an array of locations ringing Cape Canaveral’s seaside launch pad as well as remote cameras we all set as media directly at the launch pad.
The two stage ULA Atlas V lifted off right on time at 11:05 p.m. EDT from Space Launch Complex 41 on Cape Canaveral Air Force Station, Fl, into a picturesque moonlit sky on a resupply mission to the ISS.
ULA Atlas V rockets to orbits with Orbital ATK Cygnus OA-6 in this long exposure streak shot taken from the roof of the world famous Vehicle Assembly Building (VAB) at NASA’s Kennedy Space Center in Florida. Liftoff from nearby Space Launch Complex 41 on Cape Canaveral Air Force Station in Florida occurred at 11:05 p.m. EDT on March 22, 2016. Credit: Julian Leek
One could not have asked for better weather. Conditions were near perfect at launch time with virtually no winds and clouds.
Cygnus rode to orbit on a fountain of fire. And right now she is in hot pursuit of the million pound orbiting outpost crewed by an international team of six astronauts and cosmonauts.
The streak shots vividly show how the rocket magnificently illuminated the scattered thin clouds hovering over the seaside launch pad as it ascended and arced over eastwards towards Africa.
Streak shot shows United Launch Alliance Atlas V rocket carrying Orbital ATK’s Cygnus spacecraft soaring over Space Launch Complex- 37 housing upcoming Delta IV Heavy rocket after lift off from nearby Space Launch Complex 41 on Cape Canaveral Air Force Station in Florida at 11:05 p.m. EDT on March 22, 2016. The Cygnus is on a resupply mission to the International Space Station and scheduled to arrive at the orbiting laboratory Saturday, March 26. Credit: United Launch Alliance
The Orbital ATK Cygnus CRS-6 (OA-6) mission launched aboard an Atlas V Evolved Expendable Launch Vehicle (EELV) in the 401 configuration vehicle. This includes a 4-meter-diameter payload fairing in its longest, extra extended configuration to accommodate the Cygnus.
The first stage of the Atlas V booster is powered by the RD AMROSS RD-180 engine. The Centaur upper stage was powered by the Aerojet Rocketdyne RL10C-1 engine.
It was the ULA’s 62nd straight success with the Atlas V as well as the firms third launch in 2016 and the 106th launch since the company formed in 2006.
Gorgeous launch of ULA Atlas V with Cygnus OA-6 mission in this streak shot taken over Cocoa Beach on March 22, 2016! Weather couldn’t have cooperated better! Credit: Talia Landman/AmericaSpace
The Cygnus CRS-6 (OA-6) mission is being launched under terms of the firm’s Commercial Resupply Services (CRS) contract with NASA. It also counts as Orbital ATK’s fifth cargo delivery mission to the space station.
Watch these launch videos from remote video cameras set right at the launch pad showing the full fury of liftoff sounding off with the deafening thunder of some one million pounds of liftoff thrust.
Video caption: Flame trench view of the Orbital/ATK OA-6 resupply module launch to the ISS on a ULA Atlas 5 rocket from Pad 41 of the CCAFS on March 22, 2016. Credit: Jeff Seibert/AmericaSpace
Video caption: Mobius video camera placed at Florida launch pad captures blastoff up close of Orbital ATK OA-6 (CRS-6) mission riding to orbit atop a United Launch Alliance Atlas V rocket on March 22, 2016 at 11:05 p.m. EDT from Space Launch Complex-41 on Cape Canaveral Air Force Station. Credit: Ken Kremer/kenkremer.com
OA-6 is loaded with 3513 kg (7700 pounds) of science experiments and hardware, crew supplies, spare parts, gear and station hardware to the orbital laboratory in support over 250 research experiments being conducted on board by the Expedition 47 and 48 crews.
Among the research highlights are experiments like Strata-1 which will evaluate how soil on airless bodies like asteroids moves about in microgravity, Gecko Gripper to test adhesives similar those found on geckos’ feet, Meteor will evaluate the chemical composition of meteors entering the Earth’s atmosphere, Saffire will purposely set a large fire inside Cygnus after it unberths from the ISS to examine how fires spread in space, and a nanosat deployer mounted externally will deploy over two dozen nanosats also after unberthing.
A new 3D printer featuring significantly upgraded capabilities is also on board.
Atlas V Cygnus OA-6 streak shot on March 22, 2016. 246 second exposure from Satellite Beach. Credit: John Kraus
The spacecraft will arrive at the station on Saturday, March 26, at which time Expedition 47 Commander Tim Kopra of NASA and Flight Engineer Tim Peake of ESA (European Space Agency) will grapple Cygnus, using the space station’s robotic arm, at approximately 6:40 a.m.
NASA TV coverage of rendezvous and grapple will begin at 5:30 a.m.
The Cygnus has been named the S.S. Rick Husband in honor of Col. Rick Husband, the late commander of Space Shuttle Columbia, which was tragically lost with its crew of seven NASA astronauts during re-entry on its final flight on Feb. 1, 2003.
Watch for Ken’s onsite launch reports direct from the Kennedy Space Center in Florida.
Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.
This ‘Frankenstein’ liftoff image is the result of a 160+ image time lapse sequence compiled from Atlas V rocket launch carrying the OA-6 ISS resupply #Cygnus capsule, showing streak shot and star trails as captured at the NASA causeway at KSC/CCAFS. Launched by United Launch Alliance for Orbital ATK on March 22, 2016 at 11:05 p.m. EDT. Credit: Michael SeeleyULA Atlas V carrying Orbital ATK Cygnus CRS-6/OA-6 streaks skyward on March 22, 2016. Credit: Ben Smegelsky ULA Atlas V/Cygnus OA-6 intermittent streak shot following launch on March 22, 2016 is taken from roof of Vehicle Assembly Building (VAB) at NASA’s Kennedy Space Center in Florida. Credit: Ken Kremer/kenkremer.com Photographers on the VAB roof at KSC, preparing for Atlas V/Cygnus launch on March 22, 2016. Credit: Jared HaworthA Cygnus cargo spacecraft named the SS Rick Husband is being prepared inside the Payload Hazardous Servicing Facility at NASA’s Kennedy Space Center for upcoming Orbital ATK CRS-6/OA-6 mission to deliver hardware and supplies to the International Space Station. Cygnus is scheduled to lift off atop a United Launch Alliance Atlas V rocket on March 22, 2016. Credit: Ken Kremer/kenkremer.com
Based on a series of articles that were recently made available to the public, NASA predicts it could build a base on the Moon by 2022, and for cheaper than expected. Credit: NASA
Returning to the Moon has been the fevered dream of many scientists and astronauts. Ever since the Apollo Program culminated with the first astronauts setting foot on the Moon on July 20th, 1969, we have been looking for ways to go back to the Moon… and to stay there. In that time, multiple proposals have been drafted and considered. But in every case, these plans failed, despite the brave words and bold pledges made.
However, in a workshop that took place in August of 2014, representatives from NASA met with Harvard geneticist George Church, Peter Diamandis from the X Prize Foundation and other parties invested in space exploration to discuss low-cost options for returning to the Moon. The papers, which were recently made available in a special issue of New Space, describe how a settlement could be built on the Moon by 2022, and for the comparatively low cost of $10 billion.
Data from New Horizons supports the theory that Pluto's 4 small moons were formed as a result of a collision. Image by NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute
The high albedo (reflectivity) of some of Pluto’s moons supports the theory that those moons were formed as a result of a collision, rather than being Kuiper Belt Objects (KBOs) that wandered too close and were captured by Pluto’s gravity. Data supporting the collision theory came from NASA’s New Horizons spacecraft as it flew by Pluto in July 2015.
The Pluto system is a complex one. Pluto has 5 moons: Charon, Styx, Nix, Kerberos, and Hydra. Charon is the only moon that is tidally locked with Pluto, and the two are sometimes called a double dwarf planet. The system’s barycenter lies between Pluto and Charon, though much closer to Pluto. The objects in the system move in near-circular orbits, rather than ellipses.
Pluto and Charon were thought to have formed the same way the other planets formed in the Solar System; by coalescing out of a ring of debris left over after the Sun formed. Then, it was thought, the other Plutonian moons were captured from the Kuiper Belt. Pluto resides in the Kuiper Belt, so this made sense. Some of the other moons in our Solar System, like Neptune’s Triton and Saturn’s Phoebe, are also thought to be captured Kuiper Belt Objects (KBOs).
A competing theory for the formation of the Pluto system is the collision theory. This theory states that Pluto and Charon did indeed coalesce out of the ring of debris around the Sun, and that Charon was itself a dwarf planet. But a collision occurred after that, about 4 or 4.5 billion years ago, between Pluto and an object about the same size as Pluto.
This collision left Pluto and Charon in their binary state, but created a circumbinary disk of debris out of which the other 4 moons formed. There are competing versions of these theories, one of which suggests that all of Pluto’s 5 moons were formed by this collision, and none coalesced out of the circumstellar disk of debris that the other planets were formed from.
New Horizons has delivered measurements and data showing that the albedo of Pluto’s 4 smallest moons is much too high for captured KBOs. Their surface reflectivity is highly suggestive of a water-ice composition. Measured KBOs have a geometric albedo of less than .20, while Styx, Nix, Hydra, and Kerberos have values of .40, .57, .56, and .45 respectively. This points to the idea that the object that collided with Pluto 4 to 4.5 billion years ago had at least some icy surface layers.
Pluto’s 4 small moons, Styx, Nix, Kerberos, and Hydra, are all non-spheroidal. This also points to their origins as conglomerated objects which formed from a collision-induced debris disk, rather than as captured Kuiper Belt objects.
These results were published in the journal Science, on March 18th, 2016. They were gathered using the Long-Range Reconnaissance Imager (LORRI), and the Multispectral Visible Imaging Camera (MVIC) instruments on board New Horizons.
Half of the data from New Horizons’ visit to Pluto is yet to arrive, including data from the Linear Etalon Imaging Spectral Array (LEISA). Scientists are hopeful that this data, and all the existing data which together will take years to analyze, will answer some of the questions surrounding the formation of the Pluto system.
A United Launch Alliance (ULA) Atlas V launch vehicle lifts off from Cape Canaveral Air Force Station carrying a Cygnus resupply spacecraft on the Orbital ATK CRS-6 mission to the International Space Station. Liftoff was at 11:05 p.m. EDT on March 22, 2016. The spacecraft will deliver 7,500 pounds of supplies, science payloads and experiments. Credit: Ken Kremer/kenkremer.com
A United Launch Alliance (ULA) Atlas V launch vehicle lifts off from Cape Canaveral Air Force Station carrying a Cygnus resupply spacecraft on the Orbital ATK CRS-6 mission to the International Space Station. Liftoff was at 11:05 p.m. EDT on March 22, 2016. The spacecraft will deliver 7,500 pounds of supplies, science payloads and experiments. Credit: Ken Kremer/kenkremer.com
KENNEDY SPACE CENTER, FL – A stunningly beautiful nighttime launch mesmerized delighted spectators as it roared off a Florida space coast launch pad late Tuesday night, March 22, on a mission for NASA stocked with over three tons of science and supplies bound for the multinational crews working aboard the International Space Station (ISS).
A United Launch Alliance (ULA) Atlas V rocketed raced to orbit from Cape Canaveral Air Force Station, Fl, carrying an enlarged Cygnus commercial resupply spacecraft on the Orbital ATK CRS-6 mission to the ISS.
The venerable Atlas V lifted off right on target at 11:05 p.m. EDT from Space Launch Complex 41 into a picturesque moonlit sky that magnificently illuminated the scattered thin clouds hovering over the seaside launch pad for the hordes of excited folks and families lining the beaches and lucky to witness what may be history’s last launch of a Cygnus from Florida.
A United Launch Alliance (ULA) Atlas V rocket carrying the OA-6 mission lifted off from Space Launch Complex 41 at 11:05 p.m. EDT on March 22, 2016 from Cape Canaveral Air Force Station, Fla. Credit: Ken Kremer/kenkremer.com
Future liftoffs of the private Orbital ATK Cygnus supply truck designed to stock the station will return to their original launch site on Virginia’s eastern shore starting with the next mission for their NASA customer sometime this summer.
Cygnus launches to the ISS normally start from NASA’s Wallops Flight Facility in Virginia.
But a catastrophic failure of the Orbital ATK Antares rocket moments after liftoff on Oct. 28, 2014, forced Orbital to seek and book an alternative launch vehicle while the company redesigned and reengined Antares first stage with new powerful powerplants for the ride to orbit.
A United Launch Alliance (ULA) Atlas V launch vehicle lifts off from Cape Canaveral Air Force Station carrying a Cygnus resupply spacecraft on the Orbital ATK CRS-6 mission to the International Space Station. Liftoff was at 11:05 p.m. EDT on March 22, 2016. The spacecraft will deliver 7,500 pounds of supplies, science payloads and experiments. Credit: Ken Kremer/kenkremer.com
The Cygnus spacecraft will arrive at the station on Saturday, March 26, at which time Expedition 47 Commander Tim Kopra of NASA and Flight Engineer Tim Peake of ESA (European Space Agency) will grapple Cygnus, using the space station’s robotic arm, at approximately 6:40 a.m. NASA TV coverage of rendezvous and grapple will begin at 5:30 a.m.
The commercial Cygnus cargo freighter was built by Orbital ATK, based in Dulles, Virginia.
A Cygnus cargo spacecraft named the SS Rick Husband is being prepared inside the Payload Hazardous Servicing Facility at NASA’s Kennedy Space Center for upcoming Orbital ATK CRS-6/OA-6 mission to deliver hardware and supplies to the International Space Station. Cygnus is scheduled to lift off atop a United Launch Alliance Atlas V rocket on March 22, 2016. Credit: Ken Kremer/kenkremer.com
The Cygnus has been named the S.S. Rick Husband in honor of Col. Rick Husband, the late commander of Space Shuttle Columbia, which was tragically lost with its crew of seven NASA astronauts during re-entry on its final flight on Feb. 1, 2003.
This flight is also known as OA-6 and is being launched under terms of the firm’s Commercial Resupply Services (CRS) contract with NASA. It also counts as Orbital ATK’s fifth cargo delivery mission to the space station.
OA-6 is loaded with 3513 kg (7700 pounds) of science experiments and hardware, crew supplies, spare parts, gear and station hardware to the orbital laboratory in support over 250 research experiments being conducted on board by the Expedition 47 and 48 crews.
About a quarter of the cargo is devoted to science and research gear. The cargo includes 3279 kg of science investigations, 1139 kg of crew supplies, 1108 kg of vehicle hardware, 157 kg of spacewalk equipment, and 98 kg of computer resources.
Here a NASA description of a few of the scientific highlights:
– Gecko Gripper, testing a mechanism similar to the tiny hairs on geckos’ feet that lets them stick to surfaces using an adhesive that doesn’t wear off,
– Strata-1, designed to evaluate how soil on small, airless bodies such as asteroids behaves in microgravity.
– Meteor, an instrument to evaluate from space the chemical composition of meteors entering Earth’s atmosphere. The instrument is being re-flown following its loss on earlier supply missions.
– Saffire, which will set a large fire inside the Cygnus in an unprecedented study to see how large fires behave in space. The research is vital to selecting systems and designing procedures future crews of long-duration missions can use for fighting fires.
– Cygnus is carrying more than two dozen nanosatellites that will be ejected from either the spacecraft or the station at various times during the mission to evaluate a range of technology and science including Earth observations.
Here a cool video prelaunch look at Cygnus and me in the NASA Kennedy Space Center clean room discussing the Meteor experiment:
Video Credit: Thaddeus Cesari/VideoShampoo.com
When the ISS Expedition 47 crew members open the hatch, they will be greeted with a sign noting the spacecraft was named ‘SS Rick Husband’ in honor of the STS-107 mission commander.
Cygnus will spend approximately two months docked at the ISS.
OA-6 is only the second Cygnus to be launched atop a ULA Atlas V rocket, following the OA-4 mission last December.
The CRS-6/OA-6 flight is also the second flight of the enhanced Cygnus variant, that is over 1 meter longer and sports 50% more volume capability.
Thus it is capable of carrying a much heavier payload of some 3500 kg (7700 lbs) vs. a maximum of 2300 kg (5070 lbs) for the standard version.
A United Launch Alliance (ULA) Atlas V rocket carrying the OA-6 mission lifted off from Space Launch Complex 41 at 11:05 p.m. EDT on March 22, 2016 from Cape Canaveral Air Force Station, Fla. Credit: Ken Kremer/kenkremer.com
Watch for Ken’s onsite launch reports direct from the Kennedy Space Center in Florida.
Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.
Learn more about Orbital ATK Cygnus, ISS, ULA Atlas rocket, SpaceX, Boeing, Space Taxis, Mars rovers, Orion, SLS, Antares, NASA missions and more at Ken’s upcoming outreach events:
Mar 21-23: “Orbital ATK Atlas/Cygnus launch to the ISS, ULA, SpaceX, SLS, Orion, Commercial crew, Curiosity explores Mars, Pluto and more,” Kennedy Space Center Quality Inn, Titusville, FL, evening Mar 21 /late afternoon Mar 22/23
The Orbital ATK CRS-6 launch vehicle with the Cygnus cargo spacecraft bolted to the top of the Atlas V rocket is poised for launch at Space Launch Complex 41 at Cape Canaveral Air Force Station on March 22, 2016. Credit: Ken Kremer/kenkremer.com
The New Horizons team used "principal component analysis" to get this false-color image that highlights the different regions of Pluto. Image: NASA/New Horizons/JHAPL
The New Horizons probe revealed the surface features of Pluto in rich detail when it reached the dwarf planet in July 2015. Some of the features look like snapshots of rivers and lakes that are locked firmly in place by Pluto’s frigid temperatures. But now scientists studying the data coming back from New Horizons think that those frozen lakes and rivers could once have been liquid nitrogen.
Pluto has turned out be a surprisingly active place. New Horizons has shown us what might be clouds in Pluto’s atmosphere, mountains that might be ice volcanoes, and cliffs made of methane ice that melt away into the plains. If there were oceans and rivers of liquid nitrogen on the surface of Pluto, that would fit in with our evolving understanding of Pluto as a much more active planet than we thought.
Richard Binzel, a New Horizons team member from MIT, thinks that lakes of liquid nitrogen could have existed some 800 or 900 million years ago. It all stems from Pluto’s axial tilt, which at 120 degrees is much more pronounced than Earth’s relatively mild 23 degree tilt. And computer modelling suggests that this tilt could have even been more extreme many millions of years ago.
The result of this extreme tilt is that much more of Pluto’s surface would have been exposed to sunlight. That may have warmed Pluto enough to allow liquid nitrogen to flow over the planet’s surface. These kinds of changes to a planet’s axial tilt, (and precession and eccentricity) affect a planet’s climate in what are called Milankovitch cycles. The same cycles are thought to have a similar effect on Earth’s climate, though not as extreme as on Pluto.
According to Binzel, Pluto could be somewhere in between its temperature extremes, meaning that if Pluto will ever be warm enough for liquid nitrogen again, it could be hundreds of millions of years from now. “Right now, Pluto is between two extreme climate states,” Binzel says.
Alan Stern is a planetary scientist at the Southwest Research Institute, and New Horizons’ Principal Investigator. He thinks that these long-cycle climate changes could have a very pronounced effect on Pluto, which has a nitrogen-rich atmosphere. In ancient times, Pluto’s atmosphere could have been more dense than Mars’. “This opens up the possibility that liquid nitrogen may have once or even many times flowed on Pluto’s surface,” he said.
More data from New Horizons is still on its way. About half is yet to arrive. That data, and further analysis, might discredit the fledgling idea that Pluto had and will have again lakes of liquid nitrogen. “We are just beginning to understand the long-term climate of Pluto,” said Binzel.
This week is the 47th Lunar and Planetary Science Conference (LPSC) in Houston. Members of the New Horizons team will be presenting almost 40 reports on Pluto and its system of moons at this conference. Stern’s lecture, titled “The Exploration of Pluto,” will be archived online at http://livestream.com/viewnow/LPSC2016.
“Life exists because of supernovae,” said Steve Howell, project scientist for NASA’s Kepler and K2 missions at NASA’s Ames Research Center. “All heavy elements in the universe come from supernova explosions. For example, all the silver, nickel, and copper in the earth and even in our bodies came from the explosive death throes of stars.”
So a glimpse of a supernova explosion is of intense interest to astronomers. It’s a chance to study the creation and dispersal of the life-enabling elements themselves. A greater understanding of supernovae will lead to a greater understanding of the origins of life.
Stars are balancing acts. They are a struggle between the pressure to expand, created by the fusion in the star, and the gravitational urge to collapse, caused by their own enormous mass. When the core of a star runs out of fuel, the star collapses in on itself. Then there is a massive explosion, which we call a supernova. And only very large stars can become supernovae.
The brilliant flashes that accompany supernovae are called shock breakouts. These events last only about 20 minutes, an infinitesimal amount of time for an object that can shine for billions of years. But when Kepler captured two of these events in 2011, it was more than just luck.
Peter Garnavich is an astrophysics professor at the University of Notre Dame. He led an international team that analyzed the light from 500 galaxies, captured every 30 minutes over a period of 3 years by Kepler. They searched about 50 trillion stars, trying to catch one as it died as a supernova. Only a fraction of stars are large enough to explode as supernovae, so the team had their work cut out for them.
“In order to see something that happens on timescales of minutes, like a shock breakout, you want to have a camera continuously monitoring the sky,” said Garnavich. “You don’t know when a supernova is going to go off, and Kepler’s vigilance allowed us to be a witness as the explosion began.”
An artist’s concept of a shock breakout. Image: NASA Ames/STScl/G. Bacon
In 2011 Kepler caught two gigantic stars as they died their supernova death. Called KSN 2011a, and KSN 2011d, the two red super-giants were 300 times and 500 times the size of our Sun respectively. 2011a was 700 million light years from Earth, and 2011d was 1.2 billion light years away.
The intriguing part of the two supernovae is the difference between them; one had a visible shock breakout and one did not. This was puzzling, since in other respects, both supernovae behaved much like theory predicted they would. The team thinks that the smaller of the two, KSN 2011a, may have been surrounded by enough gas to mask the shock breakout.
The Kepler spacecraft is well-known for searching for and discovering extrasolar planets. But when some components on board Kepler failed in 2013, the mission was re-cast as the K2 Mission. “While Kepler cracked the door open on observing the development of these spectacular events, K2 will push it wide open, observing dozens more supernovae,” said Tom Barclay, senior research scientist and director of the Kepler and K2 guest observer office at Ames. “These results are a tantalizing preamble to what’s to come from K2!”
(For a brilliant and detailed look at the life-cycle of stars, I recommend “The Life and Death of Stars” by Kenneth R. Lang.)
