This metallic "space fabric" was created using 3-D printed techniques that add different functionality to each side of the material. Credits: NASA/JPL-Caltech
One would think NASA was preparing for a some sword fights in space! At least, that’s the impression one might get when they see the new armor NASA is developing for the first time. Officially, they are referring to it as a new type of “space fabric“, one which will provide protection to astronauts, spaceships and deployable devices. But to the casual observer, it looks a lot like chain mail armor!
The new armor is the brainchild of Polit Casillas, a systems engineer from NASA’s Jet Propulsion Laboratory. Inspired by traditional textiles, this armor relies on advances made in additive manufacturing (aka. 3-D printing) to create woven metal fabrics that can fold and change shape quickly. And someday soon, it could be used for just about everything!
As the son of a fashion designer in Spain, Casillas grew up around fabrics and textiles, and was intrigued by how they are used for the sake of design. Much in the same way that textiles are produced by weaving together countless threads, Casilla’s prototype space fabric relies on 3-D printing to create metal squares in one piece, which are then strung together to form a coat of armor.
Another example of a 3-D-printed metallic “space fabric.” The bottom and top sides of the fabric are designed to have different functionality. Credits: NASA/JPL-Caltech
In addition to his work with this new space fabric, Casillas co-leads JPL’s Atelier workshop, which specialized in the rapid-prototyping of advanced concepts and systems. This fast-paced collaborative environment works with different technologies and looks for ways to incorporate new ones (such as 4-D printing) into existing designs. As Casillas described this concept in a NASA press release:
“We call it ‘4-D printing’ because we can print both the geometry and the function of these materials. If 20th Century manufacturing was driven by mass production, then this is the mass production of functions.”
The space fabrics have four essential functions, which includes reflectivity, passive heat management, foldability and tensile strength. With one side reflecting light and the other absorbing it, the material acts as a means of thermal control. It can also fold in many different ways and adapt to shapes, all the while maintaining tensile strength to ensure it can sustain forces pulling on it.
These fabrics could be used to protect astronauts and shield large antennas, deployable devices and spacecraft from meteorites and other hazards. In addition, they could be used to ensure that missions to extreme environments would be protected from the elements. Consider Jupiter’s moon Europa, which NASA is planning on exploring in the coming decade using a lander – aka. the Europa Clipper mission.
Artist’s concept of a Europa Clipper mission. Credit: NASA/JPL
Here, and on other “ocean worlds” – like Ceres, Enceladus, Titan and Pluto – this sort of flexible armor could provide insulation for spacecraft. They could be used on landing struts to ensure that they could change shape to fit over uneven terrain as well. This kind of material could also be used to build habitats for Mars or the Moon – like the South Pole-Aitken Basin, where permanently-shadowed craters allow for the existence of water ice.
Another benefit of this material is the fact that it is considerably cheaper to produce compared to materials made using traditional fabrication methods. Under ordinary conditions, designing and building spacecraft is a complex and costly process. But by adding multiple functions to a material at different stages of development, the whole process can be made cheaper and new designs can be implemented.
Andrew Shapiro-Scharlotta is a manager at the JPL’s Space Technology Office, an office responsible for funding early-stage technologies like the space fabric. As he put it, this sort of production process could enable all kinds of designs and new mission concepts. “We are just scratching the surface of what’s possible,” he said. “The use of organic and non-linear shapes at no additional costs to fabrication will lead to more efficient mechanical designs.”
In keeping with how 3-D printing has been developed for use aboard the ISS, the JPL team not only wants to use this fabric in space, but also manufacture it in space as well. In the future, Casillas also envisions a process whereby tools and structural materials can be printed from recycled materials, offering additional cost-savings and enabling rapid, on-demand production of necessary components.
Such a production process could revolutionize the way spacecraft and space systems are created. Instead of ships, suits, and robotic craft created from many different parts (which then have to be assembled), they could be printed out like “whole cloth”. The manufacturing revolution, it seems, loometh!
SpaceX Falcon 9 rocket carrying classified NROL-76 surveillance satellite for the National Reconnaissance Office successfully launches shortly after sunrise from Launch Complex 39A on 1 May 2017 from NASA’s Kennedy Space Center in Florida. 1st stage accomplished successful ground landing at the Cape nine minutes later. Credit: Ken Kremer/Kenkremer.com
SpaceX Falcon 9 rocket carrying classified NROL-76 surveillance satellite for the National Reconnaissance Office successfully launches shortly after sunrise from Launch Complex 39A on 1 May 2017 from NASA’s Kennedy Space Center in Florida. 1st stage accomplished successful ground landing at the Cape nine minutes later. Credit: Ken Kremer/Kenkremer.com
KENNEDY SPACE CENTER, FL – SpaceX today staged the stupendously successful Falcon 9 rocket launch at sunrise of a mysterious spy satellite in support of U.S. national defense for the National Reconnaissance Office (NRO) while simultaneously accomplishing a breathtaking pinpoint land landing of the boosters first stage that could eventually dramatically drive down the high costs of spaceflight.
Liftoff of the classified NROL-76 payload for the NRO took place shortly after sunrise this morning, Monday, May 1, at 7:15 a.m. EDT (1115 GMT), from SpaceX’s seaside Launch Complex 39A on NASA’s Kennedy Space Center in Florida.
The weather was near perfect and afforded a spectacular sky show for all those who descended on the Florida Space Coast for an up close eyewitness view of the rockets rumbling thunder.
The rocket roared off pad 39A after ignition of the nine Merlin 1D first stage engines generated some 1.7 million pounds of thrust.
The Falcon sped skyward darting in and out of wispy white clouds and appeared to head in a northeasterly direction from the space coast.
“A National Reconnaissance Office (NRO) payload was successfully launched aboard a SpaceX Falcon 9 rocket from Launch Complex 39A (LC-39A), Kennedy Space Center (KSC), Florida, at 7:15 a.m. EDT, on May 1, 2017,” the NRO said in a post launch statement.
“Thanks to the SpaceX team for the great ride, and for the terrific teamwork and commitment they demonstrated throughout. They were an integral part of our government/industry team for this mission, and proved themselves to be a great partner,” said Betty Sapp, Director of the National Reconnaissance Office.
The launch of the two stage 229 foot tall Falcon 9 was postponed a day after a last moment scrub was suddenly called on Sunday by the launch director at just about T minus 52 seconds due to a sensor issue in the first stage.
SpaceX engineers were clearly able to fully resolve the issue in time for today’s second launch attempt of the super secret NROL-76 for the NRO customer.
Barely nine minutes after the launch, the 156 foot tall first stage of the SpaceX Falcon 9 rocket made an incredibly precise and thrilling soft touchdown on land at Cape Canaveral Air Force Station’s Landing Zone 1, located a few miles south of launch pad 39A.
SpaceX Falcon 9 deploys quartet of landing legs moments before precision propulsive ground touchdown at Landing Zone 1 on Canaveral Air Force Station barely nine minutes after liftoff from Launch Complex 39A on 1 May 2017 from NASA’s Kennedy Space Center in Florida. Credit: Ken Kremer/Kenkremer.com
The quartet of landing legs attached to the base of the first stage deployed only moments before touchdown – as can be seen in my eyewitness photos herein.
Multiple sonic booms screamed across the space coast as the 15 story first stage plummeted back to Earth and propulsively slowed down to pass though the sound barrier and safely came to rest fully upright.
This counts as SpaceX’s first ever launch of a top secret US surveillance satellite. It also counts as the fourth time SpaceX landed a first stage fully intact on the ground.
As is typical for NRO missions, nothing is publically known about the satellite nor has the NRO released any details about this mission in support of national security other than the launch window. SpaceX Falcon 9 deploys quartet of landing legs moments before precision propulsive ground touchdown at Landing Zone 1 on Canaveral Air Force Station barely nine minutes after liftoff from Launch Complex 39A on 1 May 2017 from NASA’s Kennedy Space Center in Florida. Credit: Ken Kremer/Kenkremer.com
Overall SpaceX has now recovered 10 first stages via either land or at sea on an oceangoing platform.
NROL-76 marks the fifth SpaceX launch of 2017 and the 33rd flight of a Falcon 9.
Blastoff of SpaceX Falcon 9 delivering NROL-76 spy satellite to orbit on 1 May 2017 for the U.S. National Reconnaissance Office. Credit: Julian Leek
NROL-76 is the second of five launches slated for the NRO in 2017. The next NRO launch is on schedule for August 14 from Vandenberg Air Force Base (VAFB), California by competitor ULA.
Until now launch competitor United Launch Alliance (ULA) and its predecessors have held a virtual monopoly on the US military’s most critical satellite launches.
The NRO is a joint Department of Defense–Intelligence Community organization responsible for developing, launching, and operating America’s intelligence satellites to meet the national security needs of our nation, according to the NRO.
Watch for Ken’s continuing onsite launch reports direct from the Kennedy Space Center and Cape Canaveral Air Force Station in Florida.
Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.
SpaceX Falcon 9 rocket carrying classified NROL-76 surveillance satellite for the National Reconnaissance Office stands raised erect poised for sunrise liftoff from Launch Complex 39A on 1 May 2017 from NASA’s Kennedy Space Center in Florida. Credit: Ken Kremer/Kenkremer.com
NASA astronaut Kate Rubins poses for a picture with the minION device during the first sample initialization run of the Biomolecular Sequencer investigation. Credits: NASA
Seeking to understand more about space-born microbes, NASA has initiated a program known as Genes in Space-3 – a collaborative effort that will prepare, sequence and identify unknown organisms, entirely from space. For those who might be thinking that this sounds a lot like the film Life – where astronauts revive an alien organism on the International Space Station and everyone dies! – rest assured, this is not the setup for some horror movie.
In truth, it represents a game-changing development that builds on recent accomplishments, where DNA was first synthesized by NASA astronaut Kate Rubin aboard the International Space Station in 2016. Looking ahead, the Genes in Space-3 program will allow astronauts aboard the ISS to collect samples of microbes and study them in-house, rather than having to send them back to Earth for analysis.
The previous experiments performed by Rubin – which were part of the Biomolecule Sequencer investigation – sought to demonstrate that DNA sequencing is feasible in an orbiting spacecraft. The Genes in Space-3 seeks to build on that by establishing a DNA sample-preparation process that would allow ISS crews to identify microbes, monitor crew health, and assist in the search for DNA-based life elsewhere in the Solar System.
NASA astronaut Kate Rubins became the first person to sequence DNA in space and sequenced more than a billion bases during her time aboard the ISS. Credits: NASA
As Sarah Wallace – a NASA microbiologist and the project’s Principal Investigator (PI) at the Johnson Space Center – said in a recent press release:
“We have had contamination in parts of the station where fungi was seen growing or biomaterial has been pulled out of a clogged waterline, but we have no idea what it is until the sample gets back down to the lab. On the ISS, we can regularly resupply disinfectants, but as we move beyond low-Earth orbit where the ability for resupply is less frequent, knowing what to disinfect or not becomes very important.”
Developed in partnership by NASA’s Johnson Space Center and Boeing (and sponsored by the ISS National Lab), this project brings together two previously spaceflight-tested molecular biology tools. First, there is miniPCR, a device which copies targeted pieces of DNA in a process known as Polymerase Chain Reaction (PCR) to create thousands of copies.
This device was developed as part of the student-designed Genes in Space competition, and was successfully tested aboard the ISS during the Genes in Space-1 experiment. Running from September to March of 2016, this experiment sought to test if the alterations to DNA and the weakening of the immune system (both of which happen during spaceflight) are in fact linked.
Student Anna-Sophia Boguraev, winner of the Genes in Space competition, is pictured with the miniPCR device. Credits: NASA
This test will be followed-up this summer with Genes in Space-2 experiment. Running from April to September, this experiment will measure how spaceflight affects telomeres – the protective caps on our chromosomes that are associated with cardiovascular disease and cancers.
The MinION, meanwhile, is a handheld device developed by Oxford Nanopore Technologies. Capable of analyzing DNA and RNA sequences, this technology allows for rapid analysis that is also portable and scalable. It has already been used here on Earth, and was successfully tested aboard the ISS as part of the Biomolecule Sequencer investigation earlier this year.
Combined with some additional enzymes to demonstrate DNA amplification, the Genes in Space-3 experiment will allow astronauts to bring the lab to the microorganisms, rather than the reverse. This will consist of crew members collecting samples from within the space station and then culturing them aboard the orbiting laboratory. The samples will then be prepared for sequencing using the miniPCR and sequenced and identified using the MinION.
As Sarah Stahl, a microbiologist and project scientist, explained, this will allow crews to combat the spread of infectious diseases and bacteria. “The ISS is very clean,” she said. “We find a lot of human-associated microorganisms – a lot of common bacteria such as Staphylococcus and Bacillus and different types of familiar fungi like Aspergillus and Penicillium.”
In addition to being able to diagnose illnesses and infections in real-time, the experiment will allow for new and exciting research aboard the ISS. This could include identifying DNA-based life on other planets, the samples of which would be returned to the ISS via probe. In addition, if and hen microbes are found floating around in space, they could be returned to the ISS for swift analysis.
Another benefit of the program will come from Earth-based scientists being able to access the experiments going on aboard the ISS in real-time. And scientists here on Earth will also benefit from the tools being employed, which will allow for cheap and effective ways to diagnose viruses, especially in parts of the world where access to a laboratory is not possible.
Once more, the development of systems and tools for use in space – an environment that is not typically conducive to Earth-based technologies – is offering up applications that go far beyond space travel. And in the coming years, ISS-based genetic research could help in the ongoing search for extra-terrestrial life, as well as provide new insights into theories like panspermia (i.e. the cosmos being seeded with life by comets, asteroids and planetoids).
Be sure to enjoy this video titled “Cosmic Carpool”, courtesy of NASA’s Johnson Space Center:
Artist's impression of a pulsar siphoning material from a companion star. Credit: NASA
When massive stars reach the end of their life cycle, they explode in a massive supernova and cast off most of their material. What’s left is a “milliscond pulsar”, a super dense, highly-magnetized neutron star that spins rapidly and emit beams of electromagnetic radiation. Eventually, these stars lose their rotational energy and begin to slow down, but they can speed up again with the help of a companion.
According to a recent study, an international team of scientists witnessed this rare event when observing an ultra-slow pulsar located in the neighboring Andromeda Galaxy (XB091D). The results of their study indicated that this pulsar has been speeding up for the past one million years, which is likely the result of a captured a companion that has since been restoring its rapid rotational velocity.
Typically, when a pulsars pairs with an ordinary star, the result is a binary system consisting of a pulsar and a white dwarf. This occurs after the pulsar pulls off the outer layers of a star, turning it into a white dwarf. The material from these outer layer then forms an accretion disk around the pulsar, which creates a “hot spot” that radiates brightly in the X-ray specturum and where temperatures can reach into the millions of degrees.
As they state in their paper, the detection of this pulsar was made possible thanks to data collected by the XMM-Newton space observatory from 2000-2013. In this time, XMM-Newton has gathered information on approximately 50 billion X-ray photons, which has been combined by astronomers at Lomosov MSU into an open online database.
This database has allowed astronomers to take a closer look at many previously-discovered objects. This includes XB091D, a pulsar with a period of seconds (aka. a “second pulsar”) located in one of the oldest globular star clusters in the Andromeda galaxy. However, finding the X-ray photos that would allow them to characterize XB091D was no easy task. As Ivan Zolotukhin explained in a MSU press release:
“The detectors on XMM-Newton detect only one photon from this pulsar every five seconds. Therefore, the search for pulsars among the extensive XMM-Newton data can be compared to the search for a needle in a haystack. In fact, for this discovery we had to create completely new mathematical tools that allowed us to search and extract the periodic signal. Theoretically, there are many applications for this method, including those outside astronomy.”
The slowest spinning X-ray pulsar in a globular star cluster has been discovered in the Andromeda galaxy. Credit: A. Zolotov
Based on a total of 38 XMM-Newton observations, the team concluded that this pulsar (which was the only known pulsar of its kind beyond our galaxy at the time), is in the earliest stages of “rejuvenation”. In short, their observations indicated that the pulsar began accelerating less than 1 million years ago. This conclusion was based on the fact that XB091D is the slowest rotating globular cluster pulsar discovered to date.
The neutron star completes one revolution in 1.2 seconds, which is more than 10 times slower than the previous record holder. From the data they observed, they were also able to characterize the environment around XB091D. For example, they found that the pulsar and its binary pair are located in an extremely dense globular cluster (B091D) in the Andromeda Galaxy – about 2.5 million light years away.
This cluster is estimated to be 12 billion years old and contains millions of old, faint stars. It’s companion, meanwhile, is a 0.8 solar mass star, and the binary system itself has a rotation period of 30.5 hours. And in about 50,000 years, they estimate, the pulsar will accelerate sufficiently to once again have a rotational period measured in the milliseconds – i.e. a millisecond pulsar.
A diagram of the ESA XMM-Newton X-Ray Telescope. Delivered to orbit by a Ariane 5 launch vehicle in 1999. Credit: ESA/XMM-Newton
Interestingly, XB910D’s location within this vast region of super-high density stars is what allowed it to capture a companion about 1 million years ago and commence the process “rejuvenation” in the first place. As Zolotukhin explained:
“In our galaxy, no such slow X-ray pulsars are observed in 150 known globular clusters, because their cores are not big and dense enough to form close binary stars at a sufficiently high rate. This indicates that the B091D cluster core, with an extremely dense composition of stars in the XB091D, is much larger than that of the usual cluster. So we are dealing with a large and rather rare object—with a dense remnant of a small galaxy that the Andromeda galaxy once devoured. The density of the stars here, in a region that is about 2.5 light years across, is about 10 million times higher than in the vicinity of the Sun.”
Thanks to this study, and the mathematical tools the team developed to find it, astronomers will likely be able to revisit many previously-discovered objects in the coming years. Within these massive data sets, there could be many examples of rare astronomical events, just waiting to be witnessed and properly characterized.
Gaze into Gaia’s crystal ball and you will see the future. This video shows the motion of 2,057,050 stars in the coming 5 million years from the Tycho-Gaia Astrometric Solutionsample, part of the first data release of European Space Agency’s Gaia mission.
Gaia is a space observatory parked at the L2 Lagrange Point, a stable place in space a million miles behind Earth as viewed from the Sun. Its mission is astrometry: measuring the precise positions, distances and motion of 1 billion astronomical objects (primarily stars) to create a three-dimensional map of the Milky Way galaxy. Gaia’s radial velocity measurements — the motion of stars toward or away from us — will provide astronomers with a stereoscopic and moving-parts picture of about 1% of the galaxy’s stars.
Think about how slowly stars move from the human perspective. Generations of people have lived and died since the days of ancient Greece and yet the constellations outlines and naked eye stars appear nearly identical today as they did then. Only a few stars — Arcturus, Sirius, Aldebaran — have moved enough for a sharp-eyed observer of yore to perceive their motion.
Given enough time, stars do change position, distorting the outlines of the their constellations. This view shows the sky looking north in 91,000 A.D. Both Lyra and the Big Dipper are clearly bent out of shape! Created with Stellarium
We know that stars are constantly on the move around the galactic center. The Sun and stars in its vicinity orbit the core at some half-million miles an hour, but nearly all are so far away that their apparent motion has barely moved the needle over the time span of civilization as we know it.
This video shows more than 2 million stars from the TGAS sample, with the addition of 24,320 bright stars from the Hipparcos Catalogue that weren’t included in Gaia’s first data release back in September 2016. The video starts from the positions of stars as measured by Gaia between 2014 and 2015, and shows how these positions are expected to evolve in the future, based on the stars’ proper motions or direction of travel across space.
This frame will help you get your footing as you watch the video. Orion (at right) and the Alpha Persei stellar association and Pleiades (at left) are shown. Credit: ESA/Gaia/DPAC
Watching the show
The frames in the video are separated by 750 years, and the overall sequence covers 5 million years. The dark stripes visible in the early frames reflect the way Gaia scans the sky (in strips) and the early, less complete database. The artifacts are gradually washed out as stars move across the sky.
Using the map above to get oriented, it’s fun to watch Orion change across the millennia. Betelgeuse departs the constellation heading north fairly quickly, but Orion’s Belt hangs in there for nearly 2 million years even if it soon develops sag! The Pleiades drift together to the left and off frame and then reappear at right.
Stars seem to move with a wide range of velocities in the video, with stars in the galactic plane moving quite slow and faster ones speeding across the view. This is a perspective effect: most of the stars we see in the plane are much farther from us, and thus seem to be moving slower than the nearby stars, which are visible across the entire sky.
Artist’s impression of The Milky Way Galaxy to provide context for the video. The Sun and solar system are located in the flat plane of the galaxy, so when we look into the Milky Way (either toward the center or toward the edge), the stars pile up across the light years to form a band in the sky. If we could rise above the disk and see the galaxy from the halo, we’d be able to look down (or up) and see the galaxy as a disk with winding spiral arms. Credit: NASA
Some of the stars that appear to zip in and out of view quickly are passing close to the Sun. But motion of those that trace arcs from one side of the sky to the other while passing close to the galactic poles (top and bottom of the frame) as they speed up and slow down, is spurious. These stars move with a constant velocity through space.
Stars located in the Milky Way’s halo, a roughly spherical structure centered on the galaxy’s spiral disk, also appear to move quite fast because they slice through the galactic plane with respect to the Sun. In reality, halo stars move very slowly with respect to the center of the galaxy.
Early in the the visualization, we see clouds of interstellar gas and dust that occupy vast spaces within the galaxy and block the view of more distant suns. That these dark clouds seem to disappear over time is also a spurious effect.
After a few million years, the plane of the Milky Way appears to have shifted towards the right as a consequence of the motion of the Sun with respect to that of nearby stars in the Milky Way. Regions that are depleted of stars in the video will not appear that way to future stargazers but will instead be replenished by stars not currently sampled by Gaia. So yes, there are a few things to keep in mind while watching these positional data converted into stellar motions, but the overall picture is an accurate one.
I find the video as mesmerizing as watching fireflies on a June night. The stars seem alive. Enjoy your ride in the time machine!
SpaceX Falcon 9 rocket carrying classified NROL-76 surveillance satellite for the National Reconnaissance Office stands raised erect poised for sunrise liftoff from Launch Complex 39A on 30 April 2017 from NASA’s Kennedy Space Center in Florida. Credit: Ken Kremer/Kenkremer.com
SpaceX Falcon 9 rocket carrying classified NROL-76 surveillance satellite for the National Reconnaissance Office stands raised erect poised for sunrise liftoff from Launch Complex 39A on 30 April 2017 from NASA’s Kennedy Space Center in Florida. Credit: Ken Kremer/Kenkremer.com
KENNEDY SPACE CENTER, FL – A classified surveillance for the nation’s spymasters is set for blastoff shortly after sunrise on Sunday, Apr. 30 by SpaceX in a space first by the firm founded by billionaire entrepreneur Elon Musk that also features a ground landing attempt by the booster. Update: Scrub reset to May 1
Liftoff of the still mysterious NROL-76 classified payload for the National Reconnaissance Office, or NRO, is slated Sunday morning, April 30 from SpaceX’s seaside Launch Complex 39A on NASA’s Kennedy Space Center in Florida.
The Falcon 9 rocket and NROL-76 payload have been mated and rolled about a quarter mile up the ramp at pad 39A.
The 229-foot-tall (70-meter) Falcon 9/NROL-76 were raised erect this morning, Saturday, April 29 and are poised for liftoff and undergoing final prelaunch preparations.
The breakfast time launch window on Sunday, April 30 opens at 7 a.m. EDT (1100 GMT). It extends for two hours until 9.a.m. EDT.
#NROL76 will carry a classified payload designed, built and operated by @NatReconOfc. @SpaceX @45thSpaceWing. Credit: NRO
The exact time of the spy satellite launch within the two hour window is classified at less than T Minus one day.
Spectators have been gathering from across the globe to witness the exciting launch and landing and area hotels are filling up.
A brand new Falcon 9 is being used for the launch unlike the recycled rocket utilized for the prior launch of the SES-10 mission involving history’s first reflown orbit class booster.
As is typical for NRO missions, nothing is publicly known about the satellite nor has the NRO released any details about this mission in support of national security other than the launch window.
We also know that this is the first launch of a spy satellite for the US governments super secret NRO spy agency by SpaceX and a source of pride for Musk and all SpaceX employees.
However you can watch the launch live on a SpaceX dedicated webcast starting about 20 minutes prior to the 7:00 am EDT opening of the window.
As is customary for all national security launches live coverage of the launch will cease approximately five minutes after liftoff as the secret payload makes it way to orbit.
However, SpaceX will continue their live webcast with complete coverage of the ground landing attempt back at the Cape which is a secondary objective of the launch.
#NROL76 Mission Patch depicts Lewis & Clark heading into the great unknown to discover and explore the newly purchased Louisiana Territory. Launch slated for 30 April 2017 from KSC pad 39A. Credit: NRO
Everything is on track for Sunday’s launch of the 229 foot tall SpaceX Falcon 9 on the NRO launch of NROL-76.
And the weather looks promising at this time.
Sunday’s weather outlook is currently forecasting an 80% chance of favorable conditions at launch time. The concerns are for cumulus clouds according to Air Force meteorologists with the 45th Space Wing at Patrick Air Force Base.
SpaceX Falcon 9 rocket carrying classified NROL-76 surveillance satellite for the National Reconnaissance Office stands raised erect poised for sunrise liftoff from Launch Complex 39A on 30 April 2017 from NASA’s Kennedy Space Center in Florida. Credit: Ken Kremer/Kenkremer.com
In case of a scrub for any reason on April 30, the backup launch opportunity Monday, May 1.
The path to launch was paved following a successful static hotfire test of the first stage booster on pad 39A which took place shortly after 3 p.m. Tuesday, April 25, as I reported here.
SpaceX conducts successful static hot fire test of Falcon 9 booster atop Launch Complex 39A at the Kennedy Space Center on 25 Apr. 2017 as seen from Merritt Island National Wildlife Refuge, Titusville, FL. The Falcon 9 is slated to launch the NROL-76 super secret spy satellite for the U.S. National Reconnaissance Office (NRO) on 30 April 2017. Credit: Ken Kremer/Kenkremer.com
Until now launch competitor United Launch Alliance (ULA) and its predecessors have held a virtual monoploy on the US military’s most critical satellite launches.
The last first stage booster during the SES-10 launch of the first recycled rocket landed on a droneship barge at sea last month.
SpaceX will also attempt to achieve the secondary mission goal of landing the 156 foot tall first stage of the Falcon 9 rocket on land at Cape Canaveral Air Force Station’s Landing Zone 1, located a few miles south of launch pad 39A.
This counts as the fourth time SpaceX will attempt a dramatic land landing potentially visible to hundreds of thousands of locals and tourists.
NROL-76 will be the fifth SpaceX launch of 2017.
Watch for Ken’s continuing onsite launch reports direct from the Kennedy Space Center and Cape Canaveral Air Force Station in Florida.
Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.
The New LEGO Apollo Saturn V set displayed in horizontal position. Credit: LEGO
LEGO Saturn V in launch configuration. Credit: LEGO Yesterday LEGO announced that their new LEGO Apollo Saturn V set will be available to buy on June 1, 2017. And let me tell you, this thing is going to be a monster. In fact, it’ll be the tallest LEGO set ever made from their crowdsourced LEGO Ideas competition, with a total height of 1 meter (39 inches). It’s going have a total of 1969 pieces (got to assume this isn’t a coincidence), and it contains all the separate parts to run your own simulated Moon mission (LEGO Moon not included).
The LEGO Ideas competitions allow LEGO builders to propose construction ideas to the LEGO community. Fans vote up their favorite designs, and then winning sets are chosen by LEGO to be turned into actual sets. At any time, there are a bunch of space-related LEGO sets in the running, including a Hubble Space Telescope (not approved), Cassini-Huygens (expired), and the Mars Curiosity Rover (approved and in stores now).
LEGO NASA Apollo 11 Set. Credit: LEGO
The NASA Apollo Saturn V set was originally created by Felix Stiessen (saabfan) and Valérie Roche (whatsuptoday), and pitched to the LEGO Ideas community back in 2014. It gained enough votes to pass through each stage of approval, and yesterday, LEGO announced it’ll be available as a full set on June 1, 2017.
What’s going to be in the set? According to LEGO, it can be stacked up in its original launch profile, with all the stages attached, service module and command module attached. Or, you can display it horizontally, with the three stages separately on stands. You’ll actually be able to extract the lunar lander, dock it with the various modules, descend to your own LEGO Moon (again, you’re going to need to supply your own Moon here, maybe that’ll be a future set?), and return the command module back to an ocean landing on Earth (again, Earth not supplied).
Command, Service and Lunar Lander Modules in various configurations. Credit: LEGO
This is the tallest set to ever come out of the LEGO Ideas Community, and the one with the most pieces – 1969, which coincidentally, was the same year that humans first walked on the Moon with Apollo 11. The initial prototype set was crated by Stiessen and Roche, but then the LEGO team took over when the idea was approved, enhancing it and preparing it for its final release as an official LEGO set.
It’s going to have a scale of 1:110. Since the set will be 1-metre high, that’ll give you a sense of just how big the original Saturn V rocket really was: 110 metres (or 363 feet). Regular LEGO minifigs have a scale of 1:47 or so, which means that regular minifigs won’t fit as astronauts into the set, but LEGO is planning to release a team of 3 new astronaut minifigs so you can play out the lunar landings.
This won’t be the tallest LEGO set ever built, though, that honor goes to the Eiffel Tower which is 7cm taller. That’s not much, though, they should have considered building the launch pad too, but now I’m just getting greedy.
Artist's impression of rocky exoplanets orbiting Gliese 832, a red dwarf star just 16 light-years from Earth. Credit: ESO/M. Kornmesser/N. Risinger (skysurvey.org).
Back in February of 2017, NASA announced the discovery of a seven-planet system orbiting a nearby star. This system, known as TRAPPIST-1, is of particular interest to astronomers because of the nature and orbits of the planets. Not only are all seven planets terrestrial in nature (i.e. rocky), but three of the seven have been confirmed to be within the star’s habitable zone (aka. “Goldilocks Zone”).
But beyond the chance that some of these planets could be inhabited, there is also the possibility that their proximity to each other could allow for life to be transferred between them. That is the possibility that a team of scientists from the University of Chicago sought to address in a new study. In the end, they concluded that bacteria and single-celled organisms could be hopping from planet to planet.
Special Guest:
Tim Blais is the founder of A Capella Science, an “educational and utterly nerdy online video project.” You can find his videos online on YouTube at A Capella Science.
We use a tool called Trello to submit and vote on stories we would like to see covered each week, and then Fraser will be selecting the stories from there. Here is the link to the Trello WSH page (http://bit.ly/WSHVote), which you can see without logging in. If you’d like to vote, just create a login and help us decide what to cover!
Announcements:
On Friday, May 12, the WSH will welcome authors Michael Summers and James Trefil to the show to discuss their new book, Exoplanets: Diamond Worlds, Super Earths, Pulsar Planets and the New Search for Life Beyond Our Solar System. In anticipation of their appearance, the WSH Crew is pleased to offer our viewers a chance to win one of two hard cover copies of Exoplanets. Two winners will be drawn live by @fraser during our show on May 12th. To enter for a chance to win a copy of Exoplanets, send an email to: [email protected] with the Subject: Exoplanets. Be sure to include your name and email address in the body of your message so that we can contact the winners afterward. All entries must be electronically postmarked by 23:59 EST on May 10, 2017, in order to be eligible. No purchase necessary. Two winners will be selected at random from all eligible entries. Good luck!
If you’d like to join Fraser and Paul Matt Sutter on their Tour to Iceland in February 2018, you can find the information at astrotouring.com.
If you would like to join the Weekly Space Hangout Crew, visit their site here and sign up. They’re a great team who can help you join our online discussions!
We record the Weekly Space Hangout every Friday at 12:00 pm Pacific / 3:00 pm Eastern. You can watch us live on Universe Today, or the Universe Today YouTube page<
Planning on a little space tourism? Better start training! Credit: barfology.com
It’s a new era for space travel. And if there’s one thing that sets it apart from the previous one, it is the spirit of collaboration that exists between space agencies and between the public and private sector. And with commercial aerospace (aka. NewSpace) companies looking to provide everything from launch services to orbital and lunar tourism, a day is fast-approaching when ordinary people will be able to go into space.
Because of this, many aerospace companies are establishing safety and training programs for prospective clients. If civilians plan on going into space, they need to have the benefit of some basic astronaut training. In short, they will need to learn how to go safely conduct themselves in a zero-gravity environment, with everything from how to avoid blowing chunks to how to relieve oneself in a tidy fashion.
In recent years, companies like Blue Origin, Virgin Galactic, Space Adventures, Golden Spike, and SpaceX have all expressed interest in making space accessible to tourists. The proposed ventures range from taking passengers on suborbital spaceflights – a la Virgin Galactic’s SpaceShipTwo – to trips into orbit (or the Moon) aboard a space capsule – a la Blue Origins’ New Shepard launch system.
Virgin Galactic’s SpaceShipTwo’s performing a glide flight. Credit: Virgin Galactic
And while these trips will not be cheap – Virgin Galactic estimates that a single seat aboard SpaceShipTwo will cost $250,000 – they absolutely have to be safe! Luckily, space agencies like NASA already have a very well-established and time-honored practice for training astronauts for zero-g. Perhaps the most famous involves flying them around in a Zero-Gravity Aircraft, colloquially known as the “Vomit Comet”.
This training program is really quite straightforward. After bringing astronaut trainees to an altitude of over 10,000 meters (32,000 feet), the plane begins flying in a parabolic arc. This consists of it climbing and falling, over and over, which causes the trainees to experience the feeling of weightlessness whenever the plane is falling. The name “vomit comet” (obviously) arises from the fact that passengers tend to lose their lunch in the process.
The Soviet-era space program also conducted weightlessness training, which Roscomos has continued since the collapse of the Soviet Union. Since 1984, the European Space Agency (ESA) has also conducts parabolic flights using a specially-modified Airbus A300 B2 aircraft. The Canadian Space Agency (CSA) has done the same since it was founded in 1989, relying on the Falcon 20 twin-engine jet.
Given the fact that NASA has been sending astronauts into space for nearly 60 years, they have certainly accrued a lot of experience in dealing with the effects of weightlessness. Over the short-term, these include space adaptation syndrome (SAS), which is also known as “space sickness”. True to its name, the symptoms of SAS include nausea and vomiting, vertigo, headaches, lethargy, and an overall feeling of unease.
Hawking has experienced zero gravity before, when he flew on Zero Gravity Corp’s modified Boeing 727 in 2007. Credit: Jim Campbell/Aero-News Network
Roughly 45% of all people who have flown in space have suffered from space sickness. The duration of varies, but cases have never been shown to exceed 72 hours, after which the body adapts to the new environment. And with the benefit of training, which includes acclimating to what weightlessness feels like, both the onset and duration can be mitigated.
Beyond NASA and other space agencies, private companies have also offered reduced gravity training to private customers. In 2004, the Zero Gravity Corporation (Zero-G, based in Arlington, Virginia) became the first company in the US to offer parabolic flights using a converted Boeing 727. In 2008, the company was acquired by Space Adventures, another Virginia-based space tourism company.
Much like Virgin Galactic, Space Adventures began offering clients advance bookings for sub-orbital flights, and has since expanded their vision to include lunar spaceflights. As such, the Zero-G experience has become their training platform, allowing clients the ability to experience weightlessness before going into space. In addition, some of the 700 clients who have already booked tickets with Virgin Galactic have used this same training method to prepare.
Similarly, Virgin Galactic is taking steps to prepare its astronauts for the day when they begin making regular flights into sub-orbit. According to the company, this will consist of astronauts taking part in a three day pre-flight preparation program that will be conducted onsite at Spaceport America – Virgin Galactic’s spaceflight facility, located in New Mexico.
Aside from microgravity, their astronaut training will also emphasize how to function when experiencing macrogravity (i.e. multi-g forces), which occur during periods of acceleration. The training will also include medical check-ups, psychological evaluations, and other forms of pre-flight prepation – much in the same way that regular astronauts are prepared for their journey. As they state on their website:
“Pre-flight preparation will ensure that each astronaut is mentally and physically prepared to savor every second of the spaceflight. Basic emergency response training prescribed by our regulators will be at the forefront. Activities to aid familiarity with the spaceflight environment will follow a close second.”
Blue Origin, meanwhile, has also been addressing concerns with regards to its plan to start sending tourists into suborbit in their New Shepard system. After launching from their pad outside of El Paso, Texas, the rocket will fly customers to an altitude of 100 km (62 mi) above the Earth. During this phase, the passengers will experience 3 Gs of acceleration – i.e. three times what they are used to.
Once it reaches space, the capsule will then detach from the rocket. During this time, the passengers will experience a few minutes of weightlessness. Between the intense acceleration and the feeling of freefall, many have wondered if potential clients should be worried about space sickness. These questions have been addressed by former NASA astronaut Nicholas Patrick, who now serves as Blue Origin’s human integration architect.
During an interview with Geekwire in January of 2017, he indicated that they plan to provide barf bags for customers to tuck into their flight suits, just in case. This is similar to what astronauts do aboard the International Space Station (see video above) and during long-term spaceflights. When asked about what customers could do to prepare for space sickness, he also emphasized that some training would be provided:
“It’s a short flight, so we won’t be asking people to train for a year, the way NASA astronauts trained for a shuttle flight, or three years, the way they train for a long space station mission. We’re going to get this training down to a matter of days, or less. That’s because we don’t have very many tasks. You need to know how to get out of your seat gracefully, and back into your seat safely.
“We’ll teach you a few safety procedures, like how to use the fire extinguisher – and maybe how to use the communication system, although that will come naturally to many people. What we’ll probably spend some time on is training people how to enjoy it. What are they going to take with them and use up there? How are they going to play? How are they going to experiment? Not too much training, just enough to have fun.”
“Getting sick to your stomach can be a problem on zero-G airplane flights like NASA’s “Vomit Comet,” but motion sickness typically doesn’t come up until you’ve gone through several rounds of zero-G. Blue Origin’s suborbital space ride lasts only 11 minutes, with a single four-minute dose of weightlessness.”
Bezos also addressed these questions in early April during the 33rd Space Symposium in Colorado Springs, where his company was showcasing the New Shepard crew capsule. Here too, audience members had questions about what passengers should do if they felt the need to vomit (among the other things) in space.
“They don’t throw up right away,” he said, referring to astronauts succumbing to space sickness. “We’re not going to worry about it… It takes about three hours before you start to throw up. It’s a delayed effect. And this journey takes ten or eleven minutes. So you’re going to be fine.”
On April 27th, during a special Q&A session of Twitch Science Week, Universe Today’s own Fraser Cain took part in a panel discussion about the future of space exploration. Among the panelists were and Ariane Cornell, the head of Astronaut Strategy and Sales for Blue Origin. When the subject of training and etiquette came up, she described the compact process Blue Origins intends to implement to prepare customers for their flight:
“[T]he day before flight is when we give you a full – intense, but very fun – day of training. So they are going to teach you all the crucial things that you need. So ingress, how do you get into the capsule, how do you buckle in. Egress, how do you get out of the seat, out of the hatch. We’re going to teach you some emergency procedures, because we want to make sure that you guys are prepared, and feel comfortable. We’re also going to teach you about zero-g etiquette, so then when we’re all up there and we’re doing our somersaults, you know… no Matrix scenes, no Kung Fu fighting – you gotta make sure that everybody gets to enjoy the flight.”
When asked (by Fraser) if people should skip breakfast, she replied:
“No. It’s the most important meal of the day. You’re going to want to have your energy and we’re pretty confident that you’re going to have a good ride and you’re not going to feel nauseous. It’s one parabola. And when we’ve seen people, for example, when they go on rides on NASA’s “Vomit Comet”… What we’ve seen from those types of parabolic flights is that people – if they get sick – its parabola six, seven, eight. It’s a delayed effect, really. We think that with that one parabola – four minutes – you’re going to enjoy every second of it.”
Another interesting issue was addressed during the 33rd Space Symposium was whether or not the New Shepard capsule would have “facilities”. When asked about this, Bezos was similarly optimistic. “Go to the bathroom in advance,” he said, to general laughter. “If you have to pee in 11 minutes, you got problems.” He did admit that with boarding, the entire experience could take up to 41 minutes, but that passengers should be able to wait that long (fingers crossed!)
But in the event of longer flights, bathroom etiquette will need to be an issue. After all, its not exactly easy to relieve oneself in an environment where all things – solid and liquid – float freely and therefore cannot simply be flushed away. Luckily, NASA and other space agencies have us covered there too. Aboard the ISS, where astronauts have to relieve themselves regularly, waste-disposal is handled by “zero-g toilets”.
Similar to what astronauts used aboard the Space Shuttle, a zero-g toilet involves an astronaut fastening themselves to the toilet seat. Rather than using water, the removal of waste is accomplished with a vacuum suction hole. Liquid waste is transferred to the Water Recovery System, where it is converted back into drinking water (that’s right, astronauts drink their own pee… sort of).
Solid waste is collected in individual bags that are stored in an aluminum container, which are then transferred to the docked spacecraft for disposal. Remember that scene in The Martian where Mark Watney collected his crew members solid waste to use as fertilizer? Well, its much the same. Poo in a bag, and then let someone remove it and deal with it once you get home.
When it comes to lunar tourism, space sickness and waste disposal will be a must. And when it comes to Elon Musk’s plan to start ferrying people to Mars in the coming decades – aboard his Interplanetary Transportation System – it will be an absolute must! It will certainly be interesting to see how those who intend to get into the lunar tourism biz, and those who want to colonize Mars, will go about addressing these needs.
In the meantime, keep your eyes on the horizon, keep your barf bags handy, and make sure your zero-g toilet has a tight seal!
