Virgin Galactic Unveils SpaceShipTwo

Your trip to space is just around the corner now. In the next step in its goal of sending regular folk to space, Virgin Galactic today unveiled the vehicle that’s going to take them there: SpaceShipTwo. The announcement was made today at a press conference at the American Museum of Natural History in New York.

Actually, there were two vehicles revealed today: SpaceShipTwo, which will carry passengers on a suborbital trip into space, and the WhiteKnightTwo carrier.

The design, of course, is based on Scaled Composite’s SpaceShipOne vehicle, which won the $10 million Ansari X-Prize in October 2004.

According to Virgin Galactic, the WhiteKnightTwo mothership is almost complete, and should be ready for testing in summer, 2008. Once completed, it should be the world’s largest all carbon composite aircraft, capable of lifting SpaceShipTwo to high altitude.

Unlike SpaceShipOne, which had room for the pilot and two passengers, SpaceShipTwo will have room for eight paying passengers. Currently, the spacecraft is about 60% complete. Passengers will spent about 2.5 hours in the air, with about 5 minutes of actual weightlessness.
WhiteKnight2
There are some more differences. WhiteKnightTwo has an extra crew cabin; a recreation of the one inside SpaceShipTwo. This will give passengers a chance to experience a little taste of what the complete trip will be like. As part of its flight plan, WhiteKnightTwo spend some time taking a parabolic flight path – like NASA’s vomit comet – to give those passengers a little bit of weightlessness too.

The company says it’s already booked 200 people, with another 85,000 registrations of interest to fly. In fact, 80 of SpaceShipTwo’s potential passengers have already been through medical assessment and centrifuge training at a special facility in Philadelphia.

Sir Richard Branson, Founder of Virgin Galactic, was, of course, bubbling and enthusiastic in the press release: “The designs of both the mothership and the new spaceship are absolutely beautiful and surpass any expectations for the future of commercial spaceflight that we had when first registering the name Virgin Galactic in 1999. Burt and his team have done a fantastic job and I am also delighted with the wonderful vision that Foster and Partners, working with URS, have shown in the final designs for Spaceport America in New Mexico. Finally, we are all very excited about the prospect of being able to develop a bio-fuel solution for the space launch system and we are looking forward to working with Pratt and Whitney and Virgin Fuels to trial an appropriate bio mix for the PW308A engines that will be powering our new carrier aircraft.”

If all goes well, the first passengers will blast off on their suborbital journey in 2009.
Flight Process
Here’s a special treat. You can access all the press images if you like, to see all the different photographs released today.

Original Source: Virgin Galactic

Researchers Plan to Launch Paper Airplane from ISS

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This is from the “why is anyone spending money on this?” department. Researchers from the University of Tokyo have teamed up with members of the Japan Origami Airplane Association to develop a paper aircraft capable of surviving the flight from the International Space Station to the Earth’s surface. The only problem is that no one knows where the paper airplane might land, and no tracking device is in the works to be used. So, the plan is to do an experiment with no way of gathering any data.


The researchers began testing the strength and heat resistance of an 8 centimeter (3.1 in) long prototype on January 17 in an ultra-high-speed wind tunnel at the University of Tokyo. In the tests, the origami glider — which is shaped like the Space Shuttle and has been treated to withstand intense heat — will be subjected to wind speeds of Mach 7, or about 8,600 kilometers (5,300 miles) per hour.

The researchers claim this paper airplane will come down more slowly than say, a real spacecraft, and it is not expected to burn up on re-entry.

No launch date has been set for the paper spaceplane, but Shinji Suzuki, an aerospace engineering professor at the University of Tokyo, is thinking ahead. “We hope the space station crew will write a message of peace on the plane before they launch it,” says Suzuki. “We don’t know where in the world the plane will land, but it would be nice to send a message to whoever finds it.”

Even if the paper airplane does make it through the atmosphere unscathed, given that our planet is 70% water, don’t hold out much hope for it being found.

Original News Source: Pink Tentacle

Mercury in Living Color

The MESSENGER science team released more pictures from the Jan. 14 flyby, including what we’ve all been waiting for, the first one in color! But if you’re looking for spectacular, eye-catching color, well, sorry, its just not part of Mercury’s make-up.

The color image was created by combining three separate images taken through MESSENGER’s Wide Angle Camera (WAC) filters in the infrared, far red, and violet wavelengths (red, green, and blue filters for this image.) MESSENGER’s eyes can see far beyond the color range of the human eye, and the colors seen in this image are somewhat different from what a human would see.

Creating a false-color image in this way brings out color differences on Mercury’s surface that cannot be seen in the black and white images released earlier.

The WAC has 11 narrow-band color filters, in contrast to the two visible-light filters and one ultraviolet filter that were on Mariner 10’s camera. By combining images taken through different filters in the visible and infrared, the MESSENGER data allow Mercury to be seen in a variety of high-resolution color views not previously possible. This visible-infrared image shows an incoming view of Mercury, about 80 minutes before MESSENGER’s closest pass of the planet from a distance of about 27,000 kilometers (17,000 miles).


I love this image of Mercury’s south pole limb. It shows the terminator; the transition from the sunlit, day side of Mercury to the dark, night side of the planet. In the region near the terminator, the sun shines on the surface at a low angle, causing the rims of craters to cast long shadows, which brings out the height differences of the surface features. This image was acquired about 98 minutes after MESSENGER’s closest approach to Mercury, when the spacecraft was at a distance of about 33,000 kilometers (21,000 miles).

Mercury Spectra.  Image Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington/Laboratory for Atmospheric and Space Physics, University of Colorado
And here’s one for the scientist in you: the first data returned from MESSENGER’s Mercury Atmospheric and Surface Composition Spectrometer (MASCS). What the image on the right shows with the bar-graph type lines is a high-resolution spectra of the planet’s surface in ultraviolet, visible, and near-infrared light. The image on the left shows a portion of the ground-track along which the MASCS instrument took over 650 observations of the surface. The area is about 300 kilometers (190 miles) across. For those of you not fluent in spectra-ese, this shows the relative amount of sunlight reflected from the surface at wavelengths from the ultraviolet to the visible (rainbow) to the infrared.

Original News Source: MESSENGER Press Releases

Astrosphere for January 22, 2008

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The Lunar News Network is concerned about the potentially faltering plans to return to the Moon, and has some suggestions if you want to take action.

Chris Lintott wonders if the United Kingdom should contribute to the International Space Station.

Centauri Dreams discusses how long it takes Earth to recover from extinction events.

A Mars Odyssey reports on a booming business, in moon dirt.

Have there been UFOs over Texas? I was just in Texas, and would have loved to see UFOs. Anyway, back to the question… no. No aliens. Astroprof gives a much more detailed answer.

Instead of the Moon, some space enthusiasts are suggesting we visit asteroids instead. Personally, I like both ideas.

This isn’t exactly space, but it’s so well written that I couldn’t resist. Pamela Gay talks about the digital divide, and how she’s greeted with blank stares when she talks technology with others.

Phil hits the pseudoscientists with a one-two punch. No, asteroid 2007 TU24 isn’t going to hit the Earth. And no, that’s not bigfoot on the surface of Mars.

Pop quiz. Mercury or the Moon, which is which?

Should NASA Overhaul Its Vision?

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Is the moon really “so yesterday?” An article in the Jan. 18 issue of Aviation Week and Space Technology reported that a group of influential people in the space community will meet in early February to discuss alternatives to NASA’s current Vision for Space Exploration of returning to the moon to prepare for future missions to Mars. But a subsequent letter to the editor in AWST written by Planetary Society President Lou Friedman and Scott Hubbard of Stanford University tried to put the brakes on any notion that the group has already come to a consensus that NASA’s VSE should change direction and destination.

In the letter, Friedman and Hubbard state that the article created “the misperception that the workshop we are organizing at Stanford University has already decided upon a new path for the human and robotic exploration of space. We wish to make it clear that the purpose of the workshop is to examine critically the Vision for Space Exploration in order to prepare for future space policy considerations in a new Administration and new Congress.”

The Aviation Week article reported that the purpose of the February meeting is “to offer the next U.S. president an alternative to President Bush’s ‘vision for space exploration’–one that would delete a lunar base and move instead toward manned missions to asteroids along with a renewed emphasis on Earth environmental spacecraft.”

But Friedman and Hubbard’s letter said, “This point of view is undoubtedly the personal opinion of some participants – but such an opinion is neither a premise nor a presumed outcome of the workshop.” Instead, they said, the workshop will address a many issues of space exploration and the workshop has no predetermined conclusions.

“We have deliberately included a wide range of participants with disparate views, including those who would maintain the status quo. We personally do not know what the conclusions of the workshop will be – or even if there will be a definitive consensus,” said Friedman and Hubbard.

Examining the current Vision is surely a good idea. A Business 101 rule is that once a plan is put into action, you should always stay on top of changing conditions and adjust your plan accordingly, constantly updating and improving. Should NASA consider missions to asteroids instead of the moon? Will going to asteroids get us to Mars more quickly, or is the moon a good, safe place to get our space legs back before moving on?

Hopefully the group meeting at Stanford University in February, as well as the upcoming new political administration in the US, will examine the VSE with open minds, considering both human and robotic missions, and without political agendas.

Another Business 101 tenet is that communication is vital to success. It’s good to see that space exploration is something people are talking about.”

Original News Source: Planetary Society Press Release

Branson Outlines His Vision For Virgin Galactic, Video Interview

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Things are moving quickly for Virgin Galactic. The world’s first commercial space tourism company has gone from strength to strength since developing Scaled Composite’s X-Prize-winning space ship design into Virgin Galactic’s SpaceShipTwo. Now, as Virgin Galactic is well on its way to building the world’s first space port in the New Mexico desert, Richard Branson discusses his vision the company’s direction and very exciting future.

In a video interview by the Telegraph Online, Richard Branson shows why he’s best guy to be at the helm of Virgin Galactic: he has a vision. So far, the development of Virgin Galactic has been astonishing, but then again, having an international company as successful as Virgin supporting it, there is room for huge aspirations.

Among the first space tourists to fly Virgin Galactic will be Richard himself, his 90 year old parents and two kids. In successive flights, big names such as Stephen Hawking have been sent their £100,000 ($200,000) tickets. Hawking has already been taken up in a parabolic flight (the “vomit comet” as used for astronaut zero-gravity training), and according to Branson, Hawking passed with flying colors.

In his interview, Branson discusses his hopes for the future. In one plan he hopes Virgin will establish a space hotel where people can use as a base and take tours on automated spacecraft to the Moon and back. The additional possibility of using the SpaceShipTwo concept as a means to transport passengers around the globe is especially interesting. The flight from London to Sydney would only take 30 minutes for a vehicle traveling into a low-Earth orbit, and emissions from such a plan would be at a minimum (almost nil when compared with the current long-haul jet flights that burn tons of fuel).

Interestingly the Virgin boss briefly mentions colonization (but stops at where he was thinking about colonizing), citing the ever present threat of a global catastrophe as reason enough to live beyond the Earth. So, will the first commercial Mars colonial spaceships be red and branded “Virgin Galactic“? Watch this space…

Watch the full interview.

Source: Telegraph.co.uk

Forget Black Holes, How Do You Find A Wormhole?

An artists impression of what it would look like inside a wormhole. Pretty. (credit: Space.com)

Finding a black hole is an easy task… compared with searching for a wormhole. Suspected black holes have a massive gravitational effect on planets, stars and even galaxies, generating radiation, producing jets and accretion disks. Black holes will even bend light through gravitational lensing. Now, try finding a wormhole… Any ideas? Well, a Russian researcher thinks he has found an answer, but a highly sensitive radio telescope plus a truckload of patience (I’d imagine) is needed to find a special wormhole signature…

A wormhole connecting two points within spacetime.
Wormholes are a valid consequence of Einstein’s general relativity view on the universe. A wormhole, in theory, acts as a shortcut or tunnel through space and time. There are several versions on the same theme (i.e. wormholes may link different universes; they may link the two separate locations in the same universe; they may even link black and white holes together), but the physics is similar, wormholes create a link two locations in space-time, bypassing normal three dimensional travel through space. Also, it is theorized, that matter can travel through some wormholes fuelling sci-fi stories like in the film Stargate or Star Trek: Deep Space Nine. If wormholes do exist however, it is highly unlikely that you’ll find a handy key to open the mouth of a wormhole in your back yard, they are likely to be very elusive and you’ll probably need some specialist equipment to travel through them (although this will be virtually impossible).

Alexander Shatskiy, from the Lebedev Physical Institute in Moscow, has an idea how these wormholes may be observed. For a start, they can be distinguished from black holes, as wormhole mouths do not have an event horizon. Secondly, if matter could possibly travel through wormholes, light certainly can, but the light emitted will have a characteristic angular intensity distribution. If we were viewing a wormhole’s mouth, we would be witness to a circle, resembling a bubble, with intense light radiating from the inside “rim”. Looking toward the center, we would notice the light sharply dim. At the center we would notice no light, but we would see right through the mouth of the wormhole and see stars (from our side of the universe) shining straight through.

For the possibility to observe the wormhole mouth, sufficiently advanced radio interferometers would be required to look deep into the extreme environments of galactic cores to distinguish this exotic cosmic ghost from its black hole counterpart.

However, just because wormholes are possible does not mean they do exist. They could simply be the mathematical leftovers of general relativity. And even if they do exist, they are likely to be highly unstable, so any possibility of traveling through time and space will be short lived. Besides, the radiation passing through will be extremely blueshifted, so expect to burn up very quickly. Don’t pack your bags quite yet…

Source: arXiv publication

When Do Asteroids Turn Dangerous?

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One of the most spectacular sights in the night sky is a fireball; a rock from space impacts the atmosphere and blazes a trail that can last seconds or even minutes. These burn up harmlessly, but when do they turn dangerous? When do asteroids get large enough that they can actually get through the atmosphere and cause some destruction here on the ground?

During an invited talk at the Meteoroids 2007 conference held in Barcelona, Spain, Clark R. Chapman from the Southwest Research Institute delivered a presentation about how to define this line between harmless explosion in the sky and an impact that causes destruction here on the ground. The paper, entitled Meteoroids, Meteors, and the Near-Earth Object Impact Hazard was later published in the journal Earth, Moon and Planets.

Originally, researchers focused their efforts on the largest asteroids: the objects 2 km (1.2 miles) and above. These are the space rocks that could cause wide scale devastation across the planet, affecting the climate and leading the the deaths of hundreds of millions of people. It was calculated that an individual might have a 1-in-25,000 chance of dying in an asteroid impact.

Now that the Spaceguard Survey has discovered 75% of the asteroids 1 km and larger, your chances of dying have dropped to about 1-in-720,000. About the same chance as dying from a fireworks accident or amusement park ride.

According to Chapman, astronomers are now shifting their focus from the largest impacts – like the one that wiped out the dinosaurs 65 million years ago – to the smaller, but still dangerous space rocks. For example, the rock that detonated in the air above Tunguska, Siberia in 1908. That object was probably only between 20-100 metres (65-325 feet) across.

And yet, it leveled the forest for thousands of square kilometres and would have caused immense destruction if it had hit a populated area.

A new survey, informally called the Spaceguard Two Survey, will begin soon with the goal of finding 90% of the near-Earth asteroids larger than 140 metres (460 feet) within the next 15 years.

There are many variables that go into calculating the resulting destruction from an impact. You have to consider the velocity, if it’s a metallic or rocky asteroid, and whether it’s fragmented or not.

What should the response be of national and international emergency management officials to a prediction that a 35 m NEA will strike a populated country a decade in the future? Following current interpretations, we would simply tell people near ground-zero to stay inside and not look directly at the high-altitude explosion. But if objects of that size could cause Tunguska-like damage, we might not only evacuate people for 100 km surrounding ground-zero but we would certainly consider a space mission to move or blow-up the threatening NEA.

Originally, researchers thought that Tunguska level events happened once in 4,000 years, but it might be more common, maybe as often as 1-in-700. And perhaps even smaller, more common, asteroids could still cause destruction on the ground – 1-in-200 years.

If Spaceguard Two Survey gets going, it should locate most of the larger asteroids, but even 50% of the Tunguska-sized impactors. It will even be tracking 1-2 million 30 metre objects.

And if one of those rocks is on a collision course with Earth, governments and space agencies will be able to work out an evacuation or prevention strategy.

Or at least encourage people to avert their eyes.

Original Source: SWRI

Podcast: Cosmic Rays

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We’re going to return to a long series of episodes we like to call: Radiation that Can Turn You Into a Superhero. This time we’re going to look at cosmic rays, which everyone knows made the Fantastic Four. These high-energy particles are streaming from the Sun and even intergalactic space, and do a wonderful job of destroying our DNA, giving us radiation sickness, and maybe (hopefully!) turning us into superheroes.

Click here to download the episode

Cosmic Rays – Show notes and transcript

Or subscribe to: astronomycast.com/podcast.xml with your podcatching software.

Using GPS Could Better Tsunami Warning System

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When there is a tsunami coming towards your home, you want to know about it as far in advance as possible. An early warning about such a disaster could save countless lives, and using Global Positioning System information may just be the way to speed up our reaction time in the future.

The traditional tsunami warning system relies on measuring the magnitude of the earthquake that causes the tsunami. This method is not always reliable, though, as calculating accurately the power of the resulting ocean waves takes hours or days.

For example, 2005 Nias quake near Indonesia was estimated to cause about the same size of tsunami as the powerful 2004 Indian Ocean quake, which destroyed cities in portions of Indonesia, India and Thailand and killed more than 225,000 people. The 2005 tsunami did not nearly meet the same proportions as the earlier quake. There have been five false tsunami alarms between 2005 and 2007, which can reduce the effectiveness of the warnings in the eye of the public.

In a study published in the December Geophysical Research Letters, researcher Y. Tony Song of NASA’s Jet Propulsion Laboratory in Pasadena, California, showed that using GPS from coastal areas near the epicenter of the quake could help more accurately and quickly determine the scale of a tsunami.

Here’s how it would potentially work: data from seismometers near the earthquake’s epicenter is first registered, as in the traditional system. After that, GPS data of the seafloor displacement is factored in, which gives a more complete picture of the extent and power of the earthquake. The size of the predicted tsunami is then quickly calculated and given a number between 1 and 10 – 1 being the lowest – much like the Richter scale. This information could then be passed through the tsunami warning system to evacuate people to safety.

GPS data helps create a 3-dimensional model of the tsunami by giving details about the horizontal and vertical displacement of the seafloor, and this data can be sent and analyzed in minutes from coastal GPS stations. Song’s methods have accurately modeled three previous tsunamis: one in Alaska in 1964, the Indian Ocean tsunami in 2004, and the 2005 Nias tsunami.

Source: JPL Press Release