A Match Made in Space

Rocketplane XP spaceplane. Credit: Rocketplane

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Rocketplane Global has announced they will be offering the opportunity for people to get married in space. On their upcoming planned suborbital flights, the space tourism company is making available specialty charter flights that include space wedding ceremonies. Billed as “the ultimate high-end celebrity wedding,” the package was first un”veiled” in Japan earlier this month by Rocketplane Japan and First Advantage Travel. With the shirtsleeve cabin environment of the XP spaceplane and its redundant life support systems, the wedding party can wear clothing of their own choosing. No need for “bulky helmets or pressure suits which would detract from the beauty of the ceremony and of course the Wedding Kiss,” said the press release. No mention if the happy couples can then become part of the 60 Mile High Club.

Rocketplane’s press release didn’t provide the price, and the website listed for further information is in Japanese, but Rocketplane’s suggested retail price on their first flights to space is $250,000 a person, so the cost for a bride, groom and wedding party would likely be astronomical, no pun intended.

Reportedly, the special wedding charter flight package includes the actual wedding ceremony in space for the bride, groom and three guests, the space marriage license and certificates, an original wedding dress, full picture and video coverage of the wedding flight and a live broadcast of the ceremony to the ground, premium hotels and transportation, and an original website developed for the wedding customers. Additional options include a space theme honeymoon in Hawaii with chartered jet transportation and a complete VIP lodging and activities package and private tour of the observatories on Mauna Kea.

Wow.

One couple from the US has already signed up for the first space wedding. Check out their website, which says they are planning to be married in 2010.

Rocketplane CEO George French said this package shows how the Rocketplane XP spaceplane can be adapted for a wide variety of unique and special uses. “We are developing a variety of additional charter flight packages involving artists, media and cultural themes as well as additional corporate promotional campaigns,” he said.

While cosmonaut Yuri Malenchenko got married via radio communication while he was on board the International Space Station (his fiancé was on Earth) no wedding ceremony has yet been performed with both the bride and groom in space.

Misuzu Onuki, Rocketplane’s Director of Asian Business Development said, “I believe that the wedding is one of the most important events in our lives, and getting married in the place closest to Heaven will be very appealing and be a key factor in the development of space tourism.”

Additional ways these charter flights could be used if for microgravity research payloads placed in racks with the scientists who developed the payload flying the mission and operating the experiments from on board. Also planned are Teacher in Space flights, which could include one or two teachers and dozens of student microgravity science experiments. A Japanese newspaper is sponsoring a contest for a Teacher in Space flight on board a Rocketplane flight.

Original News Source: Rocketplane Press Release

“Baby Red Spot” May Have Met Demise on Jupiter

The Great Red Spot on Jupiter has been observed for over 150 years, and it doesn’t appear this anti-cyclonic storm is showing any signs of letting up. How does it maintain its power? Well, like a planetary Pac-Man, it “eats up” other storms, zapping them of their power. The sequence of images here from the Hubble Space Telescope shows three different storms on Jupiter: The Great Red Spot, Red Spot Jr. (otherwise known as Oval BA, to the south of GRS), and Baby Red Spot, to the left of GRS in the first two images. Baby got a little too close to big brother GRS, and may have been snuffed out. But GRS keeps on keeping on. These three natural-color Jupiter images were made from data acquired on May 15, June 28, and July 8, 2008, by the Hubble’s Wide Field Planetary Camera 2.

Red Spot Jr. first appeared on Jupiter in early 2006 when a previously white storm turned red. This is the second time, since turning red, it has skirted past its big brother apparently unscathed. More on Jr. or Oval BA over at the BA himself, Phil Plait’s Bad Astronomy.

But poor little Baby Red Spot, which is in the same latitudinal band as the GRS. This new red spot first appeared earlier this year. The baby spot gets ever closer to the GRS in this picture sequence until it is caught up in GRS’s anticyclonic spin. In the final image the baby spot is deformed and pale in color and has been spun to the right (east) of the GRS. The prediction is that the baby spot will now get pulled back into the GRS “Cuisinart” and disappear for good. This is one possible mechanism that has powered and sustained the GRS for at least 150 years.

Each image covers 58 degrees of Jovian latitude and 70 degrees of longitude (centered on 5 degrees South latitude and 110, 121, and 121.

Original News Source: HubbleSite

Geologists Predicted Mars Avalanche

A Mars Avalanche, taken by NASAs HiRISE instrument on the Mars Reconnaisance Orbiter (Credit: NASA/HiRISE)

Remember the amazing images of an avalanche on Mars back in March of this year from the HiRISE camera on the Mars Reconnaissance Orbiter? If not for two geologists studying landforms in Alaska, MRO scientists might not have been on the lookout for such an event, or may not have known what they were seeing. A serendipitous week-long trip to Alaska by Craig Kochel and Jeffrey Trop, geology professors at Bucknell University, helped them predict one of the most important, and breathtaking planetary observations ever made. Witnessing an avalanche, or landslide in action on Mars has helped us realize the Red Planet is still a dynamic, ever-changing planet.

The two geologists were in Alaska for an eight day trip in July 2006, studying geological features and the processes that create them. In preparing for the trip, they looked at photographs of the area they would be hiking through and noticed several features in the photographs that looked familiar. Kochel thought they reminded him of images he’d seen when working on the Viking missions to Mars in the 1970s. In both the photographs and while they were hiking they saw triangle-shaped landforms called “fans” that especially looked like features on Mars. But, at first they didn’t know what they were.

During their short time in Alaska they saw over 200 snow, ice and/or rock avalanches. They realized these events were creating the fan-like features in Alaska, and determined similar avalanches on Mars were creating those same features. Additionally, they believed avalanches could still occur on Mars due to changes in temperatures from sunlight hitting a cliff wall.

At a presentation at the Lunar and Planetary science conference, Kochel and Trop shared their findings and explained that with a bit of luck and good timing, it would be possible to snap photographs of Martian avalanches.

Amazingly, soon afterwards the orbiter sent back images of an ice flow avalanche in action on Mars. Pieces of ice, dust and possibly rocks crashed down from high, steep areas, sending clouds of fine material billowing upwards. The cloud itself was about 180 meters across. The exact cause of the avalanche isn’t known with certainty, but it could be because the sun warmed layers of ice. This was the first time an avalanche had been observed on another world, and was the perfect confirmation of Kochel and Trop’s ideas.

Studies like this show that although Earth and Mars are very different places, in many ways they can be astoundingly similar.

Here are more images of the Mars Avalanche.

Original News Source: Astrobiology Magazine

Snuggling Up to Venus

Artist's conception of Venus Express. Image credit: ESA

ESA’s Venus Express spacecraft will be cozying up to the planet it has been studying for over two years to begin new and more detailed observations of Venus. This week, engineers began executing a series of maneuvers to gradually bring the spacecraft to a new orbit, closer to Venus. In its new, modified orbit the spacecraft will be able to observe unexplored regions and investigate phenomena that were not within its reach before. The maneuvers will be executed through the month of July, settling it into its new orbit by August 4. Venus Express will eventually get close enough to the planet to dip slightly into the atmosphere, testing out its aerobraking capabilities to further alter its orbit, as well as evaluating the density of the upper atmosphere by measuring the drag on the spacecraft with its on-board accelerometers.

Until now, Venus Express has occupied a highly eccentric polar orbit: at its closest point (pericentre), the spacecraft is between 250 km and 400 km from the planet, and at its farthest (apocentre), it is about 66,000 km away. The pericentre is located at 84° north.

This eccentric orbit was designed to facilitate observation of the southern hemisphere for extended periods, while being able to obtain close observations of northern hemisphere and northern polar regions.
The lowering of the Venus Express orbit is the first step in for more ambitious explorations of Venus, especially of its atmosphere.

Venus Express has already found a highly variable quantity of the volcanic gas sulphur dioxide in the atmosphere of the planet. Scientists are trying to determine if this is evidence for active volcanoes on Venus, or by another unknown mechanism affecting the upper atmosphere.

Now, the altitude of the pericentre will now be lowered to between 185 and 300 km. This modification will enable the following science advantages:
• Study of the magnetic field in the northern polar region
• Study of the plasma environment deeper in the ionosphere
• To indirectly deduce the density of the planet’s atmosphere by measuring the force, or drag, exerted by the planet’s atmosphere on the body of the spacecraft as it moves closer to the planet

Venus Express is European Space Agency’s first mission to Venus. Launched in November 2005, the spacecraft arrived at the planet on 11 April 2006 and began science observations within a month. Since then, it has continuously been making new discoveries and revising our knowledge of Venus.

As of April of this year the spacecraft had returned over 1277 gigabits of data to Earth.

Where In The Universe Challenge #12

It’s time once again for another “Where In The Universe” challenge. See if you can guess where in our vast universe this picture was taken. Give yourself extra points if you can name the spacecraft responsible for the image, too. We’ve been getting a lot of positive feedback on this challenge, and readers seem to enjoy this weekly test of their visual space-themed recognition skills. And we’ve been enjoying the reader comments on their successful and the not-so-successful identification of these space images. We’ve learned so much about the universe by the images taken by all the different spacecraft, and scientists can refer again and again images to study the fine details. And sometimes, they see something they didn’t even know was there.

Alright, its time to make your guess, and no peeking below before your guess has been made.

This is an image of Jupiter’s rings, taken by the Voyager 2 spacecraft, from the dark side of Jupiter. The faint ring system is shown in this color composite as two light orange lines protruding from the left side of Jupiter’s limb. This picture was taken in Jupiter’s shadow through orange and violet filters. Voyager 2 was at a range of 1,450,000 kilometers (900,000 miles), and about 2 degrees below the plane of the ring.

We didn’t know Jupiter had rings until the Voyagers found them in 1979. Jupiter’s rings are very dark, unlike Saturn’s rings which contain lots of ice and are very reflective. Not until the Galileo mission which orbited Jupiter from 1995 to 2003, did scientists figure out the rings were made of dust and materials kicked up by meteoroids slamming into Jupiter’s inner moons.


Voyager 1 flew by Jupiter on March 5, 1979, taking more than 18,000 images of planet and its moons. Voyager 2 flew by Jupiter on July 9, 1979, taking about the same number. Between the two Voyager spacecraft, three new moons and a thin, dark ring were discovered. Voyager images of Jupiter’s moon Io revealed active volcanoes, the first ever discovered on another body besides Earth.

How did you do on this challenge?

Take Up a Collection For NASA

A NASA contractor needs urine. And lots of it, too, about 30 liters (8 gallons) a day, even on weekends. All the details, if you need to know or need to go, of how to collect the specimens are over at SpaceRef, but the quick scoop is that contractor Hamilton Sundstrand is seeking urine from workers at the Johnson Space Center. The company is working on the new Orion space capsule that will replace the shuttle and eventually take astronauts to the moon. This is nothing new. NASA has a long-standing tradition of collecting samples from its workers to help design better space toilets because “you can’t make fake urine,” said John Lewis, NASA’s head of life support systems for Orion.

The contractor is working on how to deal with pee up in space and on the moon. “Urine is a mess because urine is full of solids,” said Lewis. Those solids clog the venting system for dumping pee, so keeping the waste disposal system clear is “really a challenge,” he said.

Here’s an article we did a few months ago about recycling urine on long duration space flights.

An email soliciting urine was sent out to JSC employees, but wasn’t meant to go public, Lewis said. In part the email said:

The Orion Program will be holding a urine collection study starting Monday, July 21 and running through Thursday, July 31, 2008. We are looking for donors as we need to collect a large amount of urine per day for the entire 11 day period. Please contact [deleted] at [deleted]@hs.utc.com to express interest in donating or to get answers to any questions you have regarding the study. We will be hosting an informational meeting with encouraged attendance for potential urine donors from 11-11:30 a.m. Thursday, July 17, 2008 in the first floor conference room. In this meeting we will go over instructions and guidelines for the study and introduce volunteers to the equipment that will be used in the study. If you are unable to attend this meeting due to scheduling conflicts, we can set up another time to clarify the study operations on an individual basis.”

Again, if you need to know more, see the entire email here.

Don’t we just love to read other people’s mail?

Original News Sources: CNN, NASA Watch

Phoenix’s Rasp Works to Create Ice Shavings

The Phoenix Mars Lander successfully used a rasp on the end of its robotic arm to drill into the frozen soil on Mar’s arctic tundra. This effort loosened the icy material, which was then scraped up and collected in the lander’s scoop. Images and data sent from Phoenix early today indicated the shaved material in the scoop had changed slightly over time during the hours after it was collected, which is a sign that the material includes water ice. Water ice sublimates, or evaporates on Mars surface because of the low surface pressure on the Red Planet. It can exist just under the surface, however, protected by the soil.

The motorized rasp — located on the back of the lander’s robotic arm scoop — made two distinct holes in a trench informally named “Snow White.” The material loosened by the rasp was collected in the scoop and documented by the Robotic Arm Camera. The activity was a test of the rasping method of gathering an icy sample, in preparation for using that method in coming days to collect a sample for analysis in an oven of Phoenix’s Thermal and Evolved-Gas Analyzer (TEGA).

“This was a trial that went really well,” said Richard Morris, a Phoenix science team member from NASA’s Johnson Space Center, Houston. “While the putative ice sublimed out of the shavings over several hours, this shows us there will be a good chance ice will remain in a sample for delivery” to Phoenix’s laboratory ovens.

The motorized rasp bit extends from the back of the scoop on the end of Phoenix’s 2.35-meter-long (7.7-foot-long) robotic arm. The tool works just a rasp for woodworking, which coarsely files or shaves material.

‘While Phoenix was in development, we added the rasp to the robotic arm design specifically to grind into very hard surface ice,’ said Barry Goldstein, Phoenix project manager at NASA’s Jet Propulsion Laboratory, Pasadena, Calif. ‘This is the exactly the situation we find we are facing on Mars, so we believe we have the right tool for the job. Honeybee Robotics in New York City did a heroic job of designing and delivering the rasp on a very short schedule.'”

The past few days, Phoenix used its robotic arm to clear the top layer of dirt from a trench it dug called Snow White. On Tuesday, Phoenix used the rasp to dig into two spots at the bottom of the trench.

Mission scientists have been working on techniques to quickly obtain the sample and then deliver it to the TEGA before too much ice has sublimated away. The TEGA test will “bake” the soil, releaseing gases present to help sciencists learn more about the ice’s composition.

Today, (Wednesday) Phoenix will be commanded to continue scraping and enlarging the “Snow White” trench and to conduct another series of rasp tests. The lander’s cameras will again be used to monitor the sample in the scoop after its collection.

Original News Source: Phoenix Press Release

Colonizing Venus With Floating Cities

Cloud city of Bespin, from Stars Wars. Credit and copyright: Ralph McQuarrie

Seemingly, people in the space community have a tendency to push the boundaries of thought about all the possibilities that await us in the universe. Case in point: Geoffrey Landis. Landis is a scientist at NASA’s Glenn Research Center who writes science fiction in his spare time. Last week Landis shared with us his ideas for using a solar powered airplane to study Venus.

This week, Landis goes a step farther (actually, several steps farther) with his ideas about colonizing Venus. Yes, Venus, our hot, greenhouse-effect-gone-mad neighboring planet with a crushing surface pressure that has doomed the few spacecraft that have attempted to reach the planet’s mysterious landscape. Landis knows Venus’ surface itself is pretty much out of the question for human habitation.

But up about 50 kilometers above the surface, Landis says the atmosphere of Venus is the most Earth-like environment, other than Earth itself, in the solar system. What Landis proposes is creating floating cities on Venus where people could live and work, as well as study the planet below.

“There’s been a lot of people who have been proposing space colonies, such as colonies that are in free space, separate from any planet,” said Landis. “And I said, well, if you’re thinking that far into the future why don’t we think of some more groundbreaking, or perhaps we should say atmosphere-breaking possibilities.”

50 km above the surface, Venus has air pressure of approximately 1 bar and temperatures in the 0°C to 50°C range, a quite comfortable environment for humans. Humans wouldn’t require pressurized suits when outside, but it wouldn’t quite be a shirtsleeves environment. We’d need air to breathe and protection from the sulfuric acid in the atmosphere.

In looking at Venus, the fact that struck Landis the most is that Earth’s atmosphere of nitrogen and oxygen would actually float in Venus’ atmosphere of carbon dioxide. “Because the atmosphere of Venus is CO2, the gases that we live in all the time, nitrogen and oxygen, would be a lifting gas,” he said. “On Earth, we know to get something to lift, you need something lighter than air. Well, on Venus, guess what? Our air is lighter than air, or at least lighter than the Venus atmosphere.”

So, create a bubble, fill it with Earth-like atmosphere, and it would float on Venus. “If you could just take the room you’re sitting in and replace the walls with something thinner, the room would float on Venus,” said Landis.

The biggest challenge would be using a substance resistant to sulfuric acid to form the outer layer of the bubble; ceramics or metal sulfates could possibly serve in this role, but of course, you’d want to be able to see outside, as well. “Just think of the great pictures you could get,” said Landis.

Asked if he has ever thought about terraforming Venus, Landis said, “Oh, yes, of course! That’s one of the reasons I started thinking about the floating cities on Venus. The more you look at Venus, the more you say, ‘oh my goodness, terraforming would be a really hard project.'”

Back in about 1962 when Carl Sagan first talked about the concept of terraforming Venus, it wasn’t known what a challenge Venus would be.

“They didn’t quite know how difficult Venus is, they didn’t know how thick the atmosphere was on Venus and how hot it was,” said Landis. “They knew it had a greenhouse effect, but they didn’t know how bad. But the more we look at the problems, the more we say, goodness, terraforming is a very difficult proposition.”

But Landis thinks Venus already has a very nice environment.

“What I like to say, the problem with Venus is if you define sea level as the place in the atmosphere where it’s the same as Earth, the place of “sea level” on Venus is just too far above the ground.”

While Landis’ plans for a solar powered airplane are a true possibility for an upcoming mission to Venus, his ideas about colonizing that planet are a little more speculative. “This is really just a thought exercise,” said Landis, “an exercise in imagination rather than something we’re likely to do in the near term. I don’t expect people will be building cities on Venus, at least probably not in this century.”

Anyone having visions of Bespin and Lando Calrissian from “The Empire Strikes Back”?

Maybe that should be “Landis” Calrissian.

More information about Geoffrey Landis.

New Evidence for a Wetter, Warmer Ancient Mars

A 3-D image of a trough in the Nili Fossae region of Mars shows phyllosilcates (in magenta and blue hues) on slopes of mesas and canyon walls, showing water played a role in Mars’ past.

For all the Mars romanticists out there, we (yes, that means me, too) hope and maybe even dream that Mars once harbored water. And not just a little spurt of groundwater every once in awhile; we want the water to have been there in abundance and for enough time to make an impact on the planet and its environment. Now, proof of copious amounts of water in Mars’ past may have been found. Two new papers based on data from the Mars Reconnaissance Orbiter (MRO) found that vast regions of the ancient southern highlands of Mars hosted a water-rich environment, and that water played a sizable role in changing the minerals of a variety of terrains in the Noachian period – about 4.6 billion to 3.8 billion years ago.

John Mustard, a professor of planetary geology at Brown University and deputy principal investigator for the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) on MRO investigated the pervasive presence of phyllosilicates, clay-like minerals that preserve a record of water’s interaction with rocks.

Specifically, Mustard and his team from 13 other institutions focused on phyllosilicate deposits in areas like craters, valleys and dunes all over the planet. Among the highlights, he detected the clay-like minerals in fans and deltas within three regions, most notably the Jezero crater. That discovery marks the first time hydrated silicates have been found in sediments “clearly lain by water,” Mustard said.

The team also found phyllosilicate deposits in thousands of places in and around craters, including the pointed peaks located at the center of some of the depressions. This suggests that water was present 4-5 kilometers below the ancient Martian surface, the team wrote, due to the generally accepted principle that crater-causing collisions excavate underground minerals that are then exposed on the crater peaks.

“Water must have been creating minerals at depth to get the signatures we see,” Mustard said.

The clay minerals were formed at low temperatures (100-200°C) – an important clue to understanding the Red Planet’s potential for habitability during the Noachian period.

“What does this mean for habitability? It’s very strong,” Mustard said. “It wasn’t this hot, boiling cauldron. It was a benign, water-rich environment for a long period of time.”

In another paper, graduate student Bethany Ehlmann and colleagues from Brown and other institutions analyzed sediment deposits in two exquisitely preserved deltas in the Jezero crater, which held an ancient lake slightly larger than Lake Tahoe. The deltas suggest a flow from rivers carrying the clay-like minerals from an approximate 15,000-square kilometer watershed during the Noachian period.
Ehlmann said scientists cannot determine whether the river flow was sporadic or sustained, but they do know it was intense and involved a lot of water.

The deltas appear to be excellent candidates for finding stored organic matter, Ehlmann said, because the clays brought in from the watershed and deposited in the lake would have trapped any organisms, leaving in essence a cemetery of microbes.

“If any microorganisms existed on ancient Mars, the watershed would have been a great place to live,” Ehlmann said. “So not only was water active in this region to weather the rocks, but there was enough of it to run through the beds, transport the clays and run into the lake and form the delta,” she said.

Original News Source: Brown University Press Release

Eta Vs. Peony: Which Star Will Go Supernova First?

The reigning champion for brightest star in the Milky Way is Eta Carinae, a highly unstable star prone to violent outbursts. Astronomers say Eta Car’s life will probably end in 100,000 years or so with a supernova explosion. That’s relatively soon in cosmic terms. But the Spitzer Space Telescope has unearthed a contender, both in brightness and in the supernova competition, found in the dusty depths of our galaxy’s center. Astronomers say the Peony nebular star might be as bright as Eta. But the biggest question may be, which star will be the first to go supernova?

Eta Carinae has the luminosity of 4.7 million times the brightness of our sun. And the new challenger, Peony, burns with the brightness of an estimated 3.2 million suns. But astronomers say it’s hard to pin down the exact brightness for these blazing stars, so they might shine with a similar amount of light.

Scientists already knew the Peony nebula star was out there, but they couldn’t get a good look at it to estimate its luminosity because of its sheltered location in the dusty central hub of our galaxy. Spitzer’s dust-piercing infrared eyes can penetrate the dust, and look into areas not visible with optical telescopes. Spitzer data was teamed up with infrared data from the European Southern Observatory’s New Technology Telescope in Chile to calculate the Peony nebula star’s luminosity.

“Infrared astronomy opens extraordinary views into the environment of the central region of our galaxy,” said Lidia Oskinova of Potsdam University in Germany. “The Peony nebula star is a fascinating creature. It appears to be the second-brightest star that we now know of in the galaxy. There are probably other stars just as bright if not brighter in our galaxy that remain hidden from view.”

Peony, with its rather delicate sounding name, is really a Big Bertha of a star. Astronomers estimate the Peony nebula star started its life with a hefty mass of roughly 150 to 200 times that of our sun. It is a type of giant blue star called a Wolf-Rayet star, with a diameter roughly 100 times that of our sun. That means this star, if placed where our sun is, would extend out to about the orbit of Mercury.

Stars this massive are rare and puzzle astronomers because they push the limits required for stars to form. Theory predicts that if a star starts out too massive, it can’t hold itself together and must break into a double or multiple stars instead.

Peony (maybe in an effort to control her weight) sheds an enormous amount of stellar matter in the form of strong winds. This matter is pushed so hard by strong radiation from the star that the winds speed up to about 1.6 million kilometers per hour (one million miles per hour) in only a few hours.

Ultimately, the Peony nebula star will live a short life of a few million years and will blow up in the most fantastic of cosmic explosions called a supernova. In fact, Oskinova and her colleagues say that the star is ripe for exploding soon, which in astronomical terms mean anytime from now to millions of years from now.

When this star blows up, it will evaporate any planets orbiting stars in the vicinity,” said Oskinova. “Farther out from the star, the explosion could actually trigger the birth of new stars.”

In addition to the star itself, the astronomers noted a cloud of dust and gas, called a nebula, surrounding the star. The team nicknamed this cloud the Peony nebula because it resembles the ornate flower.

Eta and Peony. Deceptively petite and delicate names for such big stars about to go boom.

Let the competition begin!

News Source: JPL