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!
Breakthrough Listen will monitor the 1 million closest stars to Earth over a ten year period. Credit: Breakthrough Initiatives
In July of 2015, Breakthrough Initiatives – a non-profit dedicated to the search for extra-terrestrial intelligence, founded by Yuri Milner – announced the creation of Breakthrough Listen. A ten-year initiative costing $100 million, this program was aimed at using the latest in instrumentation and software to conduct the largest survey to date for extraterrestrial communications, encompassing the 1,000,000 closest stars and 100 closest galaxies.
On Thursday, April. 20th, at the Breakthrough Discuss conference, the organization shared their analysis of the first year of Listen data. Gathered by the Green Bank Radio Telescope, this data included an analysis of 692 stars, as well as 11 events that have been ranked for having the highest significance. The results have been published on the project’s website, and will soon be published in the Astrophysical Journal.
The Green Bank Telescope (GBT), a radio telescope located at the Green Bank Observatory in West Virginia. Credit: greenbankobservatory.org
While the results were not exactly definitive, this is just the first step in a program that will span a decade. As Dr. Andrew Siemion, the Director of the BSRC, explained in a BI press release:
“With the submission of this paper, the first scientific results from Breakthrough Listen are now available for the world to review. Although the search has not yet detected a convincing signal from extraterrestrial intelligence, these are early days. The work that has been completed so far provides a launch pad for deeper and more comprehensive analysis to come.”
The Green Bank Telescope searched for these signals using its “L-band” receiver, which gathers data in frequencies ranging from 1.1 to 1.9 GHz. At these frequencies, artificial signals can be distinguished from natural sources, which includes pulsars, quasars, radio galaxies and even the Cosmic Microwave Background (CMB). Within these parameters, the BSRC team examined 692 stars from its primary target list.
For each star, they conducting three five-minutes observation periods, while also conducting five-minute observations on a set of secondary targets. Combined with a Doppler drift search – a perceived difference in frequency caused by the motion of the source or receiver (i.e. the star and/or Earth) – the Listen science team identified channels where radio emission were seen for each target (aka. “hits”).
The Parkes radio telescope, one of the telescopes comprising CSIRO’s Australia Telescope National Facility. Credit: CSIRO/David McClenaghan
This led to a combined 400 hours and 8 petabytes worth of observational data. All together, the team found millions of hits from the sample data as a whole, and eleven events that rose above the threshold for significance. These events (which are listed here) took place around eleven distant stars and ranged from to 25.4 to 3376.9 SNR (Signal-to-Noise Ratio).
However, the vast majority of the overall hits were determined to be the result of radio frequency interference from local sources. What’s more, further analysis of the 11 events indicated that it was unlikely that any of the signals were artificial in nature. While these stars all exhibited their own unique radio “fingerprints”, this is not necessarily an indication that they are being broadcast by intelligent species.
But of course, finding localized and unusual radio signals is an excellent way to select targets for follow-up examination. And if there is evidence to be found out there of intelligent species using radio signals to communicate, Breakthrough Listen is likely to be the one that finds them. Of all the SETI programs mounted to date, Listen is by far the most sophisticated.
Not only do its radio surveys cover 10 times more sky than previous programs, but its instruments are 50 times more sensitive than telescopes that are currently engaged in the search for extra-terrestrial life. They also cover 5 times more of the radio spectrum, and at speeds that are 100 times as fast. Between now and when it concludes in the coming decade, the BSRC team plans to release updated Listen data once every six months.
Aerial view of the Automated Planet Finder at the Lick Observatory. Credit: Lick Observatory/Laurie Hatch
In the meantime, they are actively engaging with signal processing and machine learning experts to develop more sophisticated algorithms to analyze the data they collect. And while they continue to listen for extra-solar sources of life, Breakthrough Starshot continues to develop the first concept for a laser-driven lightsail, which they hope will make the first interstellar voyage in the coming years.
And of course, we here in the Solar System are looking forward to missions in the coming decade that will search for life right here, in our own backyard. These include missions to Europa, Enceladus, Titan, and other “ocean worlds” where life is believed to exist in some exotic form!
Breakthrough Listen‘s data analysis can be found here. Director Andrew Siemion also took to Facebook Live on Thursday, April 20th, to presents the results of Listen’s first year of study.And be sure to check out this video that marked the launch of Breakthrough Initiatives:
Artist's concept of Cassini diving between Saturn and its innermost ring. Credit: NASA/JPL-Caltech
One down, twenty-one to go! The Cassini spacecraft survived the first dive through the narrow gap between Saturn and its rings, and is now back communicating with Earth.
“No spacecraft has ever been this close to Saturn before. We could only rely on predictions, based on our experience with Saturn’s other rings, of what we thought this gap between the rings and Saturn would be like,” said Cassini Project Manager Earl Maize of NASA’s Jet Propulsion Laboratory in Pasadena, California. “I am delighted to report that Cassini shot through the gap just as we planned and has come out the other side in excellent shape.”
It was a long day for Cassini scientists and engineers at the Jet Propulsion Laboratory while the spacecraft was out of contact for 20 hours during this first dive, signaling the beginning of the end for the mission.
Cassini, running out of fuel, is heading toward its ultimate death by crashing into Saturn on September 15, 2017. But during the next few months, Cassini will make twenty-one more passes through the gap, and in doing so, further our understanding of how giant planets, and planetary systems everywhere, form and evolve.
A raw image of Saturn’s polar vortex, taken on April 26, 2017 by the Cassini spacecraft during the first close pass between Saturn and its rings. Credit: NASA/JPL-Caltech.
Project Scientist Linda Spilker said Cassini will be able to make close up measurements of Saturn and its rings to finally help us understand the mass and internal structure of Saturn. And the images should be absolutely stunning.
Contact was lost as the ring-plane crossing started at 2 a.m. PDT (5 a.m. EDT) on April 26. NASA’s Deep Space Network Goldstone Complex in California’s Mojave Desert acquired Cassini’s signal at 11:56 p.m. PDT on April 26, 2017 (2:56 a.m. EDT on April 27) and data began flowing at 12:01 a.m. PDT (3:01 a.m. EDT) on April 27.
Cassini was programmed to collect science data while close to the planet. As a protective measure, the spacecraft used its large, dish-shaped high-gain antenna (13 feet or 4 meters across) as a deflector shield, orienting it in the direction of oncoming ring particles. This orientation put the spacecraft out of contact with Earth.
“In the grandest tradition of exploration, NASA’s Cassini spacecraft has once again blazed a trail, showing us new wonders and demonstrating where our curiosity can take us if we dare,” said Jim Green, director of the Planetary Science Division at NASA Headquarters.
We did it! Cassini is in contact with Earth and sending back data after a successful dive through the gap between Saturn and its rings. pic.twitter.com/cej1yO7T6a
The gap between the rings and the top of Saturn’s atmosphere is about 1,500 miles (2,000 kilometers) wide, and Cassini came within about 1,000 miles (1,600 kilometers) of Saturn’s cloud tops.
The best models for the region suggested that if there were ring particles in the area where Cassini crossed the ring plane, they would be tiny, on the scale of smoke particles. However, the spacecraft was traveling at speeds of about 77,000 mph (124,000 kph) relative to the planet, so small particles hitting a sensitive area could potentially have disabled the spacecraft.
The spacecraft is being destroyed after a successful 13 year mission at Saturn, as NASA needs to follow the protocol of planetary protection, and not allow a spacecraft with possible microbes from Earth to crash into a potentially habitable moon such as Enceladus or Titan.
Cassini’s next dive through the gap is scheduled for May 2.
Multi-dome lunar base being constructed, based on the 3D printing concept. Once assembled, the inflated domes are covered with a layer of 3D-printed lunar regolith by robots to help protect the occupants against space radiation and micrometeoroids.
Credits: ESA/Foster + Partners
In recent years, multiple space agencies have shared their plans to return astronauts to the Moon, not to mention establishing an outpost there. Beyond NASA’s plan to revitalize lunar exploration, the European Space Agency (ESA), Rocosmos, and the Chinese and Indian federal space agencies have also announced plans for crewed missions to the Moon that could result in permanent settlements.
As with all things in this new age of space exploration, collaboration appears to be the key to making things happen. This certainly seems to be the case when it comes to the China National Space Administration (CNSA) and the ESA’s respective plans for lunar exploration. As spokespeople from both agencies announced this week, the CNSA and the ESA hope to work together to create a “Moon Village” by the 2020s.
The announcement first came from the Secretary General of the Chinese space agency (Tian Yulong). On earlier today (Wednesday, April 26th) it was confirmed by the head of media relations for the ESA (Pal A. Hvistendahl). As Hvistendahl was quoted as saying by the Associated Press:
“The Chinese have a very ambitious moon program already in place. Space has changed since the space race of the ’60s. We recognize that to explore space for peaceful purposes, we do international cooperation.”
Multi-dome lunar base being constructed, based on the 3D printing concept. Credits: ESA/Foster + Partners
Yulong and Hvistendahl indicated that this base would aid in the development of lunar mining, space tourism, and facilitate missions deeper into space – particularly to Mars. It would also build upon recent accomplishments by both agencies, which have successfully deployed robotic orbiters and landers to the Moon in the past few decades. These include the CNSA’s Chang’e missions, as well as the ESA’s SMART-1 mission.
As part of the Chang’e program, the Chinese landers explored the lunar surface in part to investigate the prospect of mining Helium-3, which could be used to power fusion reactors here on Earth. Similarly, the SMART-1 mission created detailed maps of the northern polar region of the Moon. By charting the geography and illumination of the lunar north pole, the probe helped to identify possible base sites where water ice could be harvested.
In addition, its is likely that the construction of this base will rely on additive manufacture (aka. 3-d printing) techniques specially developed for the lunar environment. In 2013, the ESA announced that they had teamed up with renowned architects Foster+Partners to test the feasibility of using lunar soil to print walls that would protect lunar domes from harmful radiation and micrometeorites.
Artist’s impression of a lunar base created with 3-d printing techniques. Credits: ESA/Foster + Partners
This agreement could signal a new era for the CNSA, which has enjoyed little in the way of cooperation with other federal space agencies in the past. Due to the agency’s strong military connections, the U.S. government passed legislation in 2011 that barred the CSNA from participating in the International Space Station. But an agreement between the ESA and China could open the way for a three-party collaboration involving NASA.
The ESA, NASA and Roscosmos also entered into talks back in 2012 about the possibility of creating a lunar base together. Assuming that all four nations can agree on a framework, any future Moon Village could involve astronauts from all the world’s largest space agencies. Such a outpost, where research could be conducted on the long-term effects of exposure to low-g and extra-terrestrial environments, would be invaluable to space exploration.
In the meantime, the CNSA hopes to launch a sample-return mission to the Moon by the end of 2017 – Chang’e 5 – and to send the Chang’e 4 mission (whose launch was delayed in 2015) to the far side of the Moon by 2018. For its part, the ESA hopes to conduct a mission analysis on samples brought back by Chang’e 5, and also wants to send a European astronaut to Tiangong-2 (which just conducted its first automated cargo delivery) at some future date.
As has been said countless times since the end of the Apollo Era – “We’re going back to the Moon. And this time, we intend to stay!”
You might think you’re reading an educational website, where I explain fascinating concepts in space and astronomy, but that’s not really what’s going on here.
What’s actually happening is that you’re tagging along as I learn more and more about new and cool things happening in the Universe. I dig into them like a badger hiding a cow carcass, and we all get to enjoy the cache of knowledge I uncover.
Okay, that analogy got a little weird. Anyway, my point is. Squirrel!
Fast radio bursts are the new cosmic whatzits confusing and baffling astronomers, and now we get to take a front seat and watch them move through all stages of process of discovery.
Stage 1: A strange new anomaly is discovered that doesn’t fit any current model of the cosmos. For example, strange Boyajian’s Star. You know, that star that probably doesn’t have an alien megastructure orbiting around it, but astronomers can’t rule that out just yet?
Stage 2: Astronomers struggle to find other examples of this thing. They pitch ideas for new missions and scientific instruments. No idea is too crazy, until it’s proven to be too crazy. Examples include dark matter, dark energy, and that idea that we’re living in a
Stage 3: Astronomers develop a model for the thing, find evidence that matches their predictions, and vast majority of the astronomical community comes to a consensus on what this thing is. Like quasars and gamma ray bursts. YouTuber’s make their videos. Textbooks are updated. Balance is restored.
Today we’re going to talk about Fast Radio Bursts. They just moved from Stage 1 to Stage 2. Let’s dig in.
Fast radio bursts, or FRBs, or “Furbys” were first detected in 2007 by the astronomer Duncan Lorimer from West Virginia University.
He was looking through an archive of pulsar observations. Pulsars, of course, are newly formed neutron stars, the remnants left over from supernova explosions. They spin rapidly, blasting out twin beams of radiation. Some can spin hundreds of times a second, so precisely you could set your watch to them.
Lorimer’s archive of pulsar observations was captured at the Parkes radio dish in Australia. Credit: CSIRO (CC BY 3.0)
In this data, Lorimer made a “that’s funny” observation, when he noticed one blast of radio waves that squealed for 5 milliseconds and then it was gone. It didn’t match any other observation or prediction of what should be out there, so astronomers set out to find more of them.
Over the last 10 years, astronomers have found about 25 more examples of Fast Radio Bursts. Each one only lasts a few milliseconds, and then fades away forever. A one time event that can appear anywhere in the sky and only last for a couple milliseconds and never repeats is not an astronomer’s favorite target of study.
Actually, one FRB has been found to repeat, maybe.
The question, of course, is “what are they?”. And the answer, right now is, “astronomers have no idea.”
In fact, until very recently, astronomers weren’t ever certain they were coming from space at all. We’re surrounded by radio signals all the time, so a terrestrial source of fast radio bursts seems totally logical.
About a week ago, astronomers from Australia announced that FRBs are definitely coming from outside the Earth. They used the Molonglo Observatory Synthesis Telescope (or MOST) in Canberra to gather data on a large patch of sky.
Then they sifted through 1,000 terabytes of data and found just 3 fast radio bursts. Three.
Since MOST is farsighted and can’t perceive any radio signals closer than 10,000 km away, the signals had to be coming outside planet Earth. They were “extraterrestrial” in origin.
Right now, fast radio bursts are infuriating to astronomers. They don’t seem to match up with any other events we can see. They’re not the afterglow of a supernova, or tied in some way to gamma ray bursts.
In order to really figure out what’s going on, astronomers need new tools, and there’s a perfect instrument coming. Astronomers are building a new telescope called the Canadian Hydrogen Intensity Mapping Experiment (or CHIME), which is under construction near the town of Penticton in my own British Columbia.
CHIME under construction in Penticton, British Columbia. Credit: Mateus A. Fandiño (CC BY-SA 4.0)
It looks like a bunch of snowboard halfpipes, and its job will be to search for hydrogen emission from distant galaxies. It’ll help us understand how the Universe was expanding between 7 and 11 billion years ago, and create a 3-dimensional map of the early cosmos.
In addition to this, it’s going to be able to detect hundreds of fast radio bursts, maybe even a dozen a day, finally giving astronomers vast pools of signals to study.
What are they? Astronomers have no idea. Seriously, if you’ve got a good suggestion, they’d be glad to hear it.
In these kinds of situations, astronomers generally assume they’re caused by exploding stars in some way. Young stars or old stars, or maybe stars colliding. But so far, none of the theoretical models match the observations.
This artist’s conception illustrates one of the most primitive supermassive black holes known (central black dot) at the core of a young, star-rich galaxy. Image credit: NASA/JPL-Caltech
Another idea is black holes, of course. Specifically, supermassive black holes at the hearts of distant galaxies. From time to time, a random star, planet, or blob of gas falls into the black hole. This matter piles upon the black hole’s event horizon, heats up, screams for a moment, and disappears without a trace. Not a full on quasar that shines for thousands of years, but a quick snack.
The next idea comes with the only repeating fast radio burst that’s ever been found. Astronomers looked through the data archive of the Arecibo Observatory in Puerto Rico and found a signal that had repeated at least 10 times in a year, sometimes less than a minute apart.
Since the quick blast of radiation is repeating, this rules out a one-time collision between exotic objects like neutron stars. Instead, there could be a new class of magnetars (which are already a new class of neutron stars), that can release these occasional shrieks of radio.
An artist’s impression of a magnetar. Credit: ESO/L. Calçada
Or maybe this repeating object is totally different from the single events that have been discovered so far.
Here’s my favorite idea. And honestly, the one that’s the least realistic. What I’m about to say is almost certainly not what’s going on. And yet, it can’t be ruled out, and that’s good enough for my fertile imagination.
Avi Loeb and Manasvi Lingam at Harvard University said the following about FRBs:
“Fast radio bursts are exceedingly bright given their short duration and origin at distances, and we haven’t identified a possible natural source with any confidence. An artificial origin is worth contemplating and checking.”
Artificial origin. So. Aliens. Nice.
Loeb and Lingam calculated how difficult it would be to send a signal that strong, that far across the Universe. They found that you’d need to build a solar array with twice the surface area of Earth to power the radio wave transmitter.
And what would you do with a transmission of radio or microwaves that strong? You’d use it to power a spacecraft, of course. What we’re seeing here on Earth is just the momentary flash as a propulsion beam sweeps past the Solar System like a lighthouse.
But in reality, this huge solar array would be firing out a constant beam of radiation that would propel a massive starship to tremendous speeds. Like the Breakthrough Starshot spacecraft, but for million tonne spaceships.
Credit: NASA/Pat Rawlings (SAIC)
In other words, we could be witnessing alien transportation systems, pushing spacecraft with beams of energy to other worlds.
And I know that’s probably not what’s happening. It’s not aliens. It’s never aliens. But in my mind, that’s what I’m imagining.
So, kick back and enjoy the ride. Join us as we watch astronomers struggle to understand what fast radio bursts are. As they invalidate theories, and slowly unlock one of the most thrilling mysteries in modern astronomy. And as soon as they figure it out, I’ll let you know all about it.
What do you think? Which explanation for fast radio bursts seems the most logical to you? I’d love to hear your thoughts and wild speculation in the comments.
