First look inside SpaceX Dragon V2 next generation astronaut spacecraft unveiled by CEO Elon Musk on May 29, 2014. Credit: Robert Fisher/America Space
Would you ‘Enter the Dragon’?
First look inside SpaceX Dragon V2 next generation astronaut spacecraft unveiled by CEO Elon Musk on May 29, 2014. Credit: Robert Fisher/AmericaSpace[/caption]
We’ve shown you lots of exterior shots of SpaceX’s next generation manned Dragon V2 spacecraft after Billionaire entrepreneur and SpaceX CEO Elon Musk pulled the curtain off to reveal his future plans for human spaceflight on May 29 during a live webcast from SpaceX HQ in Hawthorne, Calif.
And we’ve shown you the cool animation to see exactly ‘How it Works!’ from launch to landing.
Now we’ve compiled a stunning collection of imagery revealing what it’s like to actually stand within the gleaming walls of the futuristic Dragon spaceship from an astronauts perspective.
Check out the gallery of Dragon V2 imagery above and below.
Elon Musk seated inside Dragon V2 explaining consoles at unveiling on May 29, 2014. Credit: SpaceX
Experience this exciting new chapter of American ‘Commercial Human Spaceflight’ coming to fruition.
NASA’s Commercial Crew Program (CCP) is a public private partnership between NASA and a trio of amazing American aerospace companies – SpaceX, Boeing amd Sierra Nevada – to create inexpensive but reliable new astronaut spaceships to the High Frontier.
And NASA’s unprecedented commercial crew program is so far ahead of any international competitors that I think they’ll soon be knocking at the door and regret not investing in a similar insightful manner.
The goal is to get American’s back in space on American rockets from American soil – rather than being totally dependent on Russian rocket technology and Soyuz capsules for astronaut rides to the International Space Station (ISS) and back.
Potential crew members check out the seats of the new SpaceX Dragon V2 next generation astronaut spacecraft. Credit: Robert Fisher/America Space
“We need to have our own capability to get our crews to space. Commercial crew is really, really, really important,” NASA Administrator Charles Bolden told me in an exclusive interview – here.
SpaceX CEO Elon Musk pulls open the hatch to ‘Enter the Dragon’. Credit: Robert Fisher/America Space
Boeing and Sierra Nevada are competing with SpaceX to build the next generation spaceship to ferry astronauts to and from the ISS by 2017 using seed money from NASA’s CCP.
The BoeingCST-100 and Sierra Nevada Dream Chaser ‘space taxis’ are also vying for funding in the next round of contracts to be awarded by NASA around late summer 2014. A look through the open hatch of the Dragon V2 reveals the layout and interior of the seven-crew capacity spacecraft. Credit: NASA/Dimitri Gerondidakis
Stay tuned here for Ken’s continuing SpaceX, Boeing, Sierra Nevada, Orbital Sciences, commercial space, Orion, Mars rover, MAVEN, MOM and more planetary and human spaceflight news.
The Dragon V2 spacecraft’s seating arrangement with the control panel swung up to allow crewmembers to get into their seats. Once the crew is in place, the control panel swings down and locks in launch position. Credit: NASA/Dimitri Gerondidakis
A look through the open hatch of the Dragon V2 reveals the layout and interior of the seven-crew capacity spacecraft. Credit: NASA/Dimitri Gerondidakis
SpaceX CEO Elon Musk unveils SpaceX Dragon V2 next generation astronaut spacecraft on May 29, 2014. Credit: Robert Fisher/America Space
Asteroids of various sizes whiz past our planet all the time. Some we know about, but many we don’t, and new ones are identified on an almost weekly basis. (In fact one such recently-discovered asteroid named 2014 HQ214, an object the length of an aircraft carrier, will pass us at a mere 3 lunar distances today June 8… watch live coverage here.) And, of course, some actually do impact Earth, and if they are large enough the results can be quite… energetic, to put it lightly.
While there aren’t yet any programs in place that can prevent a large asteroid impact from happening, there are some that are at least on the lookout for potential impactors. The B612 Foundation’s privately-funded Sentinel mission is one of them and, once launched and placed in orbit around the Sun in 2018, will hunt for near-Earth asteroids down to about 140 meters in size using the most advanced infrared imaging technology… and no federal budget cuts or red tape to worry about.
The video above, produced by B612 Foundation’s primary contractor Ball Aerospace, shows how Sentinel will work, and why development has been going so well.
“I see this as the wave of the future — the ability for non-governmental organizations to put together the funding, working with outstanding technical organizations like Ball Aerospace, and produce space missions where the government isn’t involved and where the price is much, much less, and we still get the same kind of great information.”
– Dr. Scott Hubbard, B612 Program Architect and former director of the NASA Ames Research Center
Hydrogen’s electron and proton have oppositely charged antimatter counterparts in the antihydrogen: the positron and antiproton. Image credit: NSF.
The best science — the questions that capture and compel any human being — is enshrouded in mystery. Here’s an example: scientists expect that matter and antimatter were created in equal quantities shortly after the Big Bang. If this had been the case, the two types of particles would have annihilated each other, leaving a Universe permeated by energy.
As our existence attests, that did not happen. In fact, nature seems to have a one-part in 10 billion preference for matter over antimatter. It’s one of the greatest mysteries in modern physics.
But the Large Hadron Collider is working hard, literally pushing matter to the limit, to solve this captivating mystery. This week, CERN created a beam of antihydrogen atoms, allowing scientists to take precise measurements of this elusive antimatter for the first time.
Antiparticles are identical to matter particles except for the sign of their electric charge. So while hydrogen consists of a positively charged proton orbited by a negatively charged electron, antihydrogen consists of a negatively charged antiproton orbited by a positively charged anti-electron, or a positron
While primordial antimatter has never been observed in the Universe, it’s possible to create antihydrogen in a particle accelerator by mixing positrons and low energy antiprotons.
In 2010, the ALPHA team captured and held atoms of antihydrogen for the first time. Now the team has successfully created a beam of antihydrogen particles. In a paper published this week in Nature Communications, the ALPHA team reports the detection of 80 antihydrogen atoms 2.7 meters downstream from their production.
“This is the first time we have been able to study antihydrogen with some precision,” said ALPHA spokesperson Jeffrey Hangst in a press release. “We are optimistic that ALPHA’s trapping technique will yield many such insights in the future.”
One of the key challenges is keeping antihydrogen away from ordinary matter, so that the two don’t annihilate each other. To do so, most experiments use magnetic fields to trap antihydrogen atoms long enough to study them.
However, the strong magnetic fields degrade the spectroscopic properties of the antihydrogen atoms, so the ALPHA team had to develop an innovative set-up to transfer antihydrogen atoms to a region where they could be studied, far from the strong magnetic field.
To measure the charge of antihydrogen, the ALPHA team studied the trajectories of antihydrogen atoms released from the trap in the presence of an electric field. If the antihydrogen atoms had an electric charge, the field would deflect them, whereas neutral atoms would be undeflected.
The result, based on 386 recorded events, gives a value of the antihydrogen electric charge at -1.3 x 10-8. In other words, its charge is compatible with zero to eight decimal places. Although this result comes as no surprise, since hydrogen atoms are electrically neutral, it is the first time that the charge of an antiatom has been measured to such high precision.
In the future, any detectable difference between matter and antimatter could help solve one of the greatest mysteries in modern physics, opening up a window into a new realm of science.
The paper has been published in Nature Communications.
A large crater in Meridiani Planum on Mars, about 20 kilometers (12.4 miles) northwest of Opportunity's landing site and 42 kilometers (24.6 miles) northwest of Endeavour Crater, where Opportunity is right now. The crater is older than Victoria Crater (another target of Opportunity's), which is clear because it is more filled in with sediments and eroded. Credit: NASA/JPL/University of Arizona
Mars, that ever-changing and beautiful Red Planet practically next door to us, is one of the most well-studied places humans have in the universe. We’ve sent spacecraft there for about 50 years. Yet there’s still a lot of mysteries out there.
NASA’s Mars Reconnaissance Orbiter is among the investigating spacecraft in the area checking out the planet’s past and looking for any interesting clues to tell us more about how Mars — and the Earth, and the solar system, and planets in general — formed. Mars had a wetter past (as the rovers have showed us), but where the water went and why its atmosphere are so thin are among the things scientists are trying to understand.
Luckily for us, the catalog of the University of Arizona’s High Resolution Imaging Science Experiment (HiRISE) is easily available online for all of us to marvel at. Here are just some of the pictures sent back from across the solar system. To see more, look below and check out this HiRISE web page.
This image from Mars shows a variety of sandy features: ripples, transverse aeolian ridges (which are larger and lighter), dunes (dark) and draa (very large bedforms that are greater than 1 kilometer or 0.62 miles). Credit: NASA/JPL/University of ArizonaA Martian alluvial fan on the floor of a 60-kilometer (38-mile) crater near the equator of Mars. Scientists commonly study these features to learn more about the Red Planet’s wet past. Credit: NASA/JPL/University of ArizonaShiny dunes on Mars taken by the HiRISE camera on the Mars Reconnaissance Orbiter. Credit: NASA/JPL/University of ArizonaDunes migrating across the surface of Mars. Picture taken by the HiRISE camera on the Mars Reconnaissance Orbiter. Credit: NASA/JPL/University of Arizona
The cover of the new book "Space Hoax" by Paul Gillebaard.
Space Hoax, written by Paul Gillebaard, is the adventure filled sequel to his book Moon Hoax (read our review of that book here.) This space thriller begins right where Moon Hoax left off.
Our hero, Peter Novak, living a certainly less than boring life, is on his way back from the Moon. He had launched on what was supposed to be a suicide mission to the Moon in a race to disprove China’s lies. Peter proved our country did go to the Moon; the Apollo missions were not faked. China’s machinations to humiliate the USA in a dizzying plot failed. Saving face and doing the right thing, the two Taikonauts in orbit around the Moon allow Peter Novak to use their Chinese spacecraft as a lifeboat home.
The stage is now set for Peter’s next challenge.
Executives in China are not pleased with their lies being exposed. Ideally, they would love to put an end to Peter Novak. They still wish to embarrass the USA, cripple our space program, and push their own country ahead into the future of spaceflight. Their next possible target: A commercial spaceflight company and the International Space Station (ISS). Any terrorism against the ISS would be incredibly damaging to the USA and the other cooperating space faring nations.
In Space Hoax, Peter is torn. He wants to develop his relationship with the love of his life. She is the daughter of a Cosmonaut, his father’s ally and friend from years past. Once back on Earth, Peter must contend with staying grounded in life and the inevitable pull of his job. He’s trying to move forward with his girlfriend and stay safe for her sake. On the other hand, he is an accomplished astronaut and trusted government agent. When the Space Intelligence Division has a credible threat that a prominent commercial rocket company has a spy within its ranks, Peter Novak is recruited for the job. How much will Peter have to risk this time to complete the mission?
Space Hoax is chock full of rockets, launches, harrowing landings, and spacewalks that all space geeks will love. Paul Gillebaard has a commanding knowledge of aerospace technology and sprinkles the book’s pages with credible tech. As a female reader, Peter Novak’s male swagger can be a bit much, but the plot pulls you in and weaves a plausible tale of high stakes, space race deceit. If you enjoyed Moon Hoax, you will be pleased with its sequel.
After nearly four decades of of listening for for signs of life in the cosmos, astronomer Jill Tarter is one of a handful of true experts on the Search for Extraterrestrial Intelligence (SETI). And since 1995 we’ve known for certain there are other planets out there; the goal now is to find one that’s habitable.
“Exoplanets are real,” Tarter said recently, talking about how the Kepler planet-hunting mission has changed the concept of SETI. “We are now observing stars where we KNOW there are planets. We’ve gone from having 20-30 potential targets to having thousands of targets. Kepler is telling us WHERE to look, and we are focusing there.”
But so far the search has come up empty. After so long with no luck, why continue? Tarter recently appeared on PBS’s “Secret Lives of Scientists” and she gave them an answer in less than 30 seconds.
An infrared image of N103B, the remainders of a supernova that exploded about 1,000 years ago in the Large Magellanic Cloud, which is one of the closest galaxies to the Milky Way. Credit: NASA/JPL-Caltech/Goddard
It might be a bad idea to get close to dead stars. Like a White Walker from Game of Thrones, this “cosmic zombie” white dwarf star was dangerous even though it was just a corpse of a star like our own. The result from this violence is still visible in the Spitzer Space Telescope picture you see above.
Astronomers believe the giant star was shedding material (a common phenomenon in older stars), which fell on to the white dwarf star. As the gas built up on the white dwarf over time, the mass became unstable and the dwarf exploded. What’s left is still lying in a pool of gas about 160,000 light-years away from us.
“It’s kind of like being a detective,” stated Brian Williams of NASA’s Goddard Space Flight Center, who led the research. “We look for clues in the remains to try to figure out what happened, even though we weren’t there to see it.”
This explosion in the Large Magellanic Cloud — one of the closest satellite galaxies to Earth — is known as a Type 1a supernova, but it’s a rare breed of that kind. Type 1as are best known as “standard candles” because their explosions have a consistent luminosity. Knowing how luminous the supernova type is allows astronomers to estimate distance based on its apparent brightness; the fainter the supernova is, the further away it is.
Most Type 1as happen when two orbiting white dwarfs smash into each other, but this scenario is more akin to something that Earthlings saw in 1604. Informally called Kepler’s supernova, because it was discovered by astronomer Johannes Kepler, astronomers believe this arose from a red giant and white dwarf interaction. The evidence left for this conclusion showed the supernova leftovers embedded in dust and gas.
Investigators have submitted their results to the Astrophysical Journal.
A graphic illustrating the ISEE-3 spacecraft's history. Courtesy Tim Reyes.
What is it like to make contact with a 36-year old dormant spacecraft?
“The intellectual side of you systematically goes through all the procedures but you really end up doing a happy dance when it actually works,” Keith Cowing told Universe Today. Cowing, most notably from NASA Watch.com, and businessman Dennis Wingo are leading a group of volunteer engineers that are attempting to reboot the International Sun-Earth Explorer (ISEE-3) spacecraft after it has traveled 25 billion kilometers around the Solar System the past 30 years.
Its initial mission launched in 1978 to study Earth’s magnetosphere, and the spacecraft was later repurposed to study two comets. Now, on its final leg of a 30-plus year journey and heading back to the vicinity of Earth, the crowdfunding effort ISEE-3 Reboot has been working to reactivate the hibernating spacecraft since NASA wasn’t able to provide any funds to do so.
The team awakened the spacecraft by communicating from the Arecibo radio telescope in Puerto Rico, using a donated transmitter. While most of the team has been in Puerto Rico, Cowing is back at home in the US manning the surge of media attention this unusual mission has brought.
Those at Arecibo are now methodically going through all the systems, figuring out what the spacecraft can and can’t do.
“We did determine the spin rate of spacecraft is slightly below what it should be,” Cowing said, “but the point there is that we’re now understanding the telemetry that we’re getting and its coming back crystal clear.”
For you tech-minded folks, the team determined the spacecraft is spinning at 19.16 rpm. “The mission specification is 19.75 +/- 0.2 rpm. We have also learned that the spacecraft’s attitude relative to the ecliptic is 90.71 degrees – the specification is 90 +/- 1.5 degrees. In addition, we are now receiving information from the spacecraft’s magnetometer,” Cowing wrote in an update on the website.
The next task will be looking at the propulsion system and making sure they can actually fire the engines for a trajectory correction maneuver (TCM), currently targeted for June 17.
One thing this TCM will do is to make sure the spacecraft doesn’t hit the Moon. Initial interactions with the ISEE-3 from Arecibo showed the spacecraft was not where the JPL ephemeris predicted it was going to be.
“That’s a bit troublesome because if you look at the error bars, it could hit Moon, or even the Earth, which is not good,” Cowing said, adding that they’ve since been able to refine the trajectory and found the ephemeris was not off as much as initially thought, and so such an impact is quite unlikely.
“However, it’s not been totally ruled out, — as NASA would say it’s a not a non-zero chance,” Cowing said. “The fact that it was not where it was supposed to be shows there were changes in its position. But assuming we can fire the engines when we want to, it shouldn’t be a problem. As it stands now, if we didn’t do anything, the chance of it hitting the Moon is not zero. But it’s not that likely.”
But the fact that the predicted location of the spacecraft is only off by less than 30,000 km is actually pretty amazing.
Consider this, the spacecraft has completed almost 27 orbits of the sun since the last trajectory maneuver. That is 24.87 billion kilometers. They are off course by less than 30,000 km. I can’t even come up with an analogy to how darn good that is!! That is almost 1 part in ten million accuracy! We need to confirm this with a DSN ranging, but if this holds, the fuel needed to accomplish the trajectory change is only about 5.8 meters/sec, or less than 10% of what we thought last week!
We truly stand on the shoulders of steely eyed missile men giants..
Dennis Wingo and ISEE-3 Reboot engineers at Arecibo. Image courtesy ISEE-3 Reboot.
In 1982, NASA engineers at Goddard Space Flight Center, led by Robert Farquhar devised the maneuvers needed to send the spacecraft ISEE-3 out of the Earth-Moon system. It was renamed the International Cometary Explorer (ICE) to rendezvous with two comets – Giacobini-Zinner in 1985 and Comet Halley in 1986.
“Bob Farquhar and his team initially did it with pencils on the back of envelopes,” Cowing said, “so it is pretty amazing. And we’re really happy with the trajectory because we’ll need less fuel – we have 150 meters per second of fuel available, and we’ll only need about 6 meters per second of maneuvering, so that will give us a lot of margin to do the other things in terms of the final orbit, so we’re happy with that. But we have to fire the engines first before we pat ourselves on the back.”
And that’s where the biggest challenge of this amateur endeavor lies.
“The biggest challenge will be getting the engines to fire,” Cowing said. “The party’s over if we can’t get it to do that. The rest will be gravy. So that’s what we’re focusing on now.”
After the June 17 TCM, the next big date is August 10, when the team will attempt to put the spacecraft in Earth orbit and then resume its original mission that began back in 1978 – all made possible by volunteers and crowdfunding.
We’ll keep you posted on this effort, but follow the ISEE-3 Reboot Twitter feed, which is updated frequently and immediately after anything happens with the spacecraft. Also, for more detailed updates, check out the SpaceCollege website.
One has never been spotted for sure in the wild jungle of strange stellar objects out there, but astronomers now think they have finally found a theoretical cosmic curiosity: a Thorne-Zytkow Object, or TZO, hiding in the neighboring Small Magellanic Cloud. With the outward appearance of garden-variety red supergiants, TZOs are actually two stars in one: a binary pair where a super-dense neutron star has been absorbed into its less dense supergiant parter, and from within it operates its exotic elemental forge.
First theorized in 1975 by physicist Kip Thorne and astronomer Anna Zytkow, TZOs have proven notoriously difficult to find in real life because of their similarity to red supergiants, like the well-known Betelgeuse at the shoulder of Orion. It’s only through detailed spectroscopy that the particular chemical signatures of a TZO can be identified.
Portrait of the Small Magellanic Cloud, made by NASA’s Spitzer Space Telescope
Observations of the red supergiant HV 2112 in the Small Magellanic Cloud*, a dwarf galaxy located a mere 200,000 light-years away, have revealed these signatures — unusually high concentrations of heavy elements like molybdenum, rubidium, and lithium.
While it’s true that these elements are created inside stars — we are all star-stuff, like Carl Sagan said — they aren’t found in quantity within the atmospheres of lone supergiants. Only by absorbing a much hotter star — such as a neutron star left over from the explosive death of a more massive partner — is the production of such elements presumed to be possible.
“Studying these objects is exciting because it represents a completely new model of how stellar interiors can work,”said Emily Levesque, team leader from the University of Colorado Boulder and lead author on the paper. “In these interiors we also have a new way of producing heavy elements in our universe.”
Definitive detection of a TZO would provide direct evidence for a completely new model of stellar interiors, as well as confirm a theoretically predicted fate for massive star binary systems and the existence of nucleosynthesis environments that offer a new channel for heavy-element and lithium production in our universe.
– E.M. Levesque et al., Discovery of a Thorne-Zytkow object candidate in the Small Magellanic Cloud
One of the original proposers of TZOs, Dr. Anna Zytkow, is glad to see her work resulting in new discoveries.
“I am extremely happy that observational confirmation of our theoretical prediction has started to emerge,” Zytkow said. “Since Kip Thorne and I proposed our models of stars with neutron cores, people were not able to disprove our work. If theory is sound, experimental confirmation shows up sooner or later. So it was a matter of identification of a promising group of stars, getting telescope time and proceeding with the project.”
The findings were first announced in January at the 223rd meeting of the American Astronomical Society. The paper has now been accepted for publication in the Monthly Notices of the Royal Astronomical Society Letters, and is co-authored by Philip Massey, of Lowell Observatory in Flagstaff, Arizona; Anna Zytkow of the University of Cambridge in the U.K.; and Nidia Morrell of the Carnegie Observatories in La Serena, Chile. Read the team’s paper here.
Source: University of Colorado, Boulder. Illustration by ‘Digital Drew.’
__________________________ *In the paper the team notes that it’s not yet confirmed that HV 2112 is part of the SMC and could be associated with our own galaxy. If so it would rule out it being a TZO, but would still require an explanation of its observed spectra.
