Scott Kelly, NASA Astronaut, Tweets Picture of Manhattan From International Space Station
Get an Astronaut's-Eye View of SpaceX's Dragon Launch Abort Test
SpaceX's Crew Dragon spaceship is being built to zoom astronauts out of harm's way in the event of a launch pad emergency — but based on newly released video that was captured during this month's pad abort test, it could be the kind of ride people would pay for, even if they're not going into space.
The May 6 test flight at Cape Canaveral Air Force Station in Florida marked the first on-the-pad trial for the Crew Dragon "pusher" system, powered by the next-gen capsule's eight SuperDraco thrusters. The Dragon accelerated from zero to 100 mph (160 kilometers per hour) in just 1.2 seconds and reached a top speed of 345 mph (555 kilometers per hour).
SpaceX's two-minute video, recorded by cameras mounted on the Dragon, shows the Florida landscape falling away as the craft rises about a mile (1.5 kilometers) above the pad. There are some thrilling moments as the Dragon slowly tumbles, the "trunk" separates and flies away, and the parachutes unfurl. Then there's a nice and easy drift down to the Atlantic.
The latest video doesn't show the splashdown, but you can watch that part of the ride at the end of a video that SpaceX released just a couple of days after the test.
So how would the ride feel? "Had there been people on board, they would have been in great shape," SpaceX's founder and CEO, Elon Musk, told reporters just after the test.
The only one who could contradict Musk on that score was the crash-test dummy that was strapped into the Dragon — and the dummy isn't giving interviews. For a true first-person account, we'll probably have to wait until 2017, when crewed tests of the Crew Dragon are due to begin.
The Boeing Co. is developing its own crew vehicle for NASA's use, known as the CST-100. Both companies are receiving billions of dollars from the space agency to support the projects, and they're expected to start flying NASA astronauts to the International Space Station in 2017.
IN-DEPTH
- SpaceX Dragon Capsule Splashes Down
- Dragon Pad Abort Test Is a Real Blast
- Here's What It's Like Inside SpaceX's Dragon Capsule
SOCIAL
Cosmic Cannibal: Massive 'Nasty' Star Observed by Hubble Telescope
An ongoing act of cosmic cannibalism may be responsible for the strange appearance and unprecedented behavior of a gigantic star nicknamed "Nasty 1," a new study reports.
Observations by NASA's Hubble Space Telescope have revealed a disk of gas nearly 3 trillion miles (4.8 trillion kilometers) wide surrounding Nasty 1, which is a massive, rapidly aging object known as a Wolf-Rayet star.
Wolf-Rayet stars start out big, initially containing at least 20 times more mass than the sun. But their hydrogen-dominated outer layers soon puff up and are lost, exposing the objects' helium-burning cores to space. Astronomers aren't exactly sure how this process unfolds, but they have a few ideas. [Top 10 Strangest Things in Space]
For example, some scientists think these massive stars' powerful stellar winds blow away their own hydrogen envelopes. Another idea holds that the outer layers are siphoned off by a cannibalistic companion star.
"That's what we think is happening in Nasty 1," study lead author Jon Mauerhan, of the University of California, Berkeley, said in a statement, referring to the second hypothesis. "We think there is a Wolf-Rayet star buried inside the nebula, and we think the nebula is being created by this mass-transfer process. So this type of sloppy stellar cannibalism actually makes Nasty 1 a rather fitting nickname."
Such a disc had never before been seen surrounding a Wolf-Rayet star, researchers said. The nebula is likely only a few thousand years old and lies about 3,000 light-years from Earth, they added.
Several other factors further bolster the cannibalism idea over the stellar-wind hypothesis, study team members said. For one thing, at least 70 percent of all massive stars belong to binary systems. And modeling work suggests that such a star's own winds may not be strong enough to push it to Wolf-Rayet status.
"We're finding that it is hard to form all the Wolf-Rayet stars we observe by the traditional wind mechanism, because mass loss isn't as strong as we used to think," co-author Nathan Smith, of the University of Arizona, said in the same statement.
"Mass exchange in binary systems seems to be vital to account for Wolf-Rayet stars and the supernovae they make, and catching binary stars in this short-lived phase will help us understand this process," Smith added.
The new study was published online Thursday (May 21) in the Monthly Notices of the Royal Astronomical Society.
This is a condensed version of a report from Space.com. Read the full report. Follow Mike Wall on Twitter @michaeldwall and Google+. Follow us @Spacedotcom, Facebook or Google+.
More from Space.com
Most Luminous Known Galaxy Shines Brighter Than Light of 300 Trillion Suns
NASA researchers have identified the brightest galaxy ever encountered, which shines in the infrared wavelength with the equivalent light of 300 trillion suns.
The "extremely luminous infrared galaxy," or ELIRG, was encountered in data from 2010's Wide-field Infrared Survey Explorer. The WISE space telescope has revealed a number of strange and unique galaxies. This one, the astronomers theorize, may have a supermassive black hole at the center, which draws immense amounts of gas and matter into itself and releases a veritable rainbow of electromagnetic energy.
The energy is blocked by thick a halo of dust, which absorbs it and heats up, emitting infrared light instead — and in unprecedented amounts.
What's more, this particular galaxy is so far away that the light we're receiving on Earth was given off about 12.5 billion years ago. That means it grew that large and that bright during the infancy of the universe itself. To the researchers, that suggests that the black hole forming the center of the galaxy is breaking the rules somehow. For example, it may have started out bigger than any others we've encountered,.
"Another way for a black hole to grow this big is for it to have gone on a sustained binge, consuming food faster than typically thought possible," the University of Leicester's Andrew Blain, co-author of the report describing the galaxy, said in a NASA news release.
"It's like winning a hot-dog-eating contest lasting hundreds of millions of years." (The term hot DOGs does appear in the paper, but in reference to "hot dust-obscured galaxies" like this one.)
Understanding the galaxy's formation will help shed light on the early history of the universe and set a precedent for studying similar objects. The report appears in the May 22 issue of The Astrophysical Journal, and can be read on the ArXiv preprint server.
IN-DEPTH
- Scientists Map Halo of Gas Around Andromeda Galaxy
- Dead Galaxies Perished by 'Strangulation,' Astronomers Find
- Crashing Galaxies Shed New Light on Dark Matter Mystery
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