The Chinese government has announced they will launch three taikonauts sometime in mid-June 2012, on the first manned mission to dock with their orbiting experimental module, and confirmed again that the crew might include China’s first female space traveler. A rocket carrying the Shenzhou 9 spacecraft was moved to a launch pad in China’s desert northwest over the weekend, China’s Xinhua News Agency reported.
The three-member crew will dock with and live inside the Tiangong 1 (or Heavenly Palace-1) orbital module launched last year. No word on how long the mission will be. We reported in March that the crew possibly could include a woman, and Niu Hongguang, deputy commander-in-chief of the country’s manned space program, said the final selection would depend on conditions nearer the time of launch.
This type of late announcement of the crew is not unprecedented – in the past, China’s space program has named the crew for the next mission just a few days before launch.
From previous reports, China picked two women and five men from thousands of candidates to become the second batch of seven astronaut trainees in 2010. Both of the women were former fighter jet pilots.
“The manned space program would not be complete without women’s participation,” Jiao Weixin, an earth and space scientist with Peking University, was quoted as saying.
China launched their first human mission in 2003. They have launched two other human missions, one of which included a space walk in 2008.
Zhou Jianping, chief designer of China’s human space program, said that the mission will be “a significant step in China’s space history”, because it’s the first time for a Chinese spacecraft to send astronauts into a space lab, instead of just carrying them to circle the Earth as in the previous three manned missions, the Chinese Daily reported.
During the flight, one crew member will remain aboard the Shenzhou 9 “as a precautionary measure in case of emergency” while the others enter Tiangong 1, Xinhua said.
We’ll keep you updated on any announcements of the crew or when the launch will take place.
The Chinese government last year announced a 5-year plan for space exploration that includes collecting samples from the Moon by 2016.
Images and video from the Transit of Venus on June 5/6, 2012 are still pouring in, and we needed to share just a few more. Here’s an awesome close-up look at the event in Hydrogen Alpha from accomplished astrophotographer John Chumack. He used a Lunt Solar Scope 60mm/50F H-Alpha filter and a DMK 21AF04 Fire-wire camera. This is 741 frames & 1/91 second exposure. John has more images on our Flickr page, and on his website, Galactic Images.
Venus transit with a transit of B747 jumbo across the solar disk which was captured by one of the members of the Tamilnadu Astronomical Society in India, Mr. Muralikrishna Kanagala during our transit event at Elliots Beach, Madras, India at 6.02 hrs IST, as the Sun rose. He used a Baader filtered Sony DSH H50 Camera.
Patrick Cullis put together this amazing time-lapse of the Transit, which features two telescopes, an airplane transit, sunset, and a few different angles of the view.
The above video is from the Solar Dynamics Observatory, a composite of the entire Transit, set to music.
And finally, this image and story from Blake Crosby and his son Orion from Charleston, South Carolina, displaying the lengths people would go to witness this event:
“This won’t be the best shot of the transit by a long shot, but my son and I jumped through a lot of hoops just to get it,” Crosby wrote in an email. “We live in Charleston, SC and our horizon is blocked by towering pine trees so we checked into the 9th floor of a Holiday Inn with a westward facing room. After lugging up all of our equipment, we found out that the doors to the balconies had been permanently closed, so we would have to shoot through a pane of glass with our Canon Rebel XS attached to a Celestron Nexstar 4SE with a Seymour filter. Furthermore, we were greeted, like many others, with a thick wall of clouds that just didn’t want to budge. Even worse, the hotel’s wifi was so shoddy we couldn’t stream any of the live views from the internet. However, we got a lucky break at about 8:00 EDT when the clouds parted for about 2 minutes and we were able to snap a couple of pics. My son Orion remarked that he was glad we endured those setbacks just so we could get a glimpse of an event that won’t happen again in our lifetimes.”
You can always see more images of many great astronomical views on our Flickr group page. Join us in sharing your images there and we may post them on Universe Today!
And if you’re interested in looking back, here’s an archive to all the past Carnivals of Space. If you’ve got a space-related blog, you should really join the carnival. Just email an entry to [email protected], and the next host will link to it. It will help get awareness out there about your writing, help you meet others in the space community – and community is what blogging is all about. And if you really want to help out, sign up to be a host. Send an email to the above address.
Despite a horrendous weather forecast, the clouds parted – at least partially – just in the nick of time for a massive crowd of astronomy and space enthusiasts gathered at Princeton University to see for themselves the dramatic start of the Transit of Venus shortly after 6 p.m. EDT as it arrived at and crossed the limb of the Sun.
And what a glorious view it was for the well over 500 kids, teenagers and adults who descended on the campus of Princeton University in Princeton, New Jersey for a viewing event jointly organized by the Astrophysics Dept and the Amateur Astronomers Association of Princeton (AAAP), the local astronomy club to which I belong.
See Transit of Venus astrophotos snapped from Princeton, above and below by Astrophotographer and Prof. Bob Vanderbei of Princeton U and a AAAP club member.
It was gratifying to see so many children and whole families come out at dinner time to witness this ultra rare celestial event with their own eyes – almost certainly a last-in-a-lifetime experience that won’t occur again for another 105 years until 2117. The crowd gathered on the roof of Princeton’s Engineering Dept. parking deck – see photos
For the next two and a half hours until sunset at around 8:30 p.m. EDT, we enjoyed spectacular glimpses as Venus slowly and methodically moved across the northern face of the sun as the racing clouds came and went on numerous occasions, delighting everyone up to the very end when Venus was a bit more than a third of the way through the solar transit.
Indeed the flittering clouds passing by in front of Venus and the Sun’s active disk made for an especially eerie, otherworldly and constantly changing scene for all who observed through about a dozen AAAP provided telescopes properly outfitted with special solar filters for safely viewing the sun.
As part of this public outreach program, NASA also sent me special solar glasses to hand out as a safe and alternative way to directly view the sun during all solar eclipses and transits through your very own eyes – but not optical aids such as cameras or telescopes.
Altogether the Transit lasted 6 hours and 40 minutes for those in the prime viewing locations such as Hawaii – from where NASA was streaming a live Transit of Venus webcast.
You should NEVER look directly at the sun through any telescopes or binoculars not equipped with special eye protection – because that can result in severe eye injury or permanent blindness!
We in Princeton were quite lucky to observe anything because other astro friends and fans in nearby areas such as Philadelphia, PA and Brooklyn, NY reported seeing absolutely nothing for this last-in-a-lifetime celestial event.
Princeton’s Astrophysics Department organized a series of lectures prior to the observing sessions about the Transit of Venus and how NASA’s Kepler Space Telescope currently uses the transit method to detect and discover well over a thousand exoplanet and planet candidates – a few of which are the size of Earth and even as small as Mars, the Red Planet.
NASA’s Curiosity rover is currently speeding towards Mars for an August 6 landing in search of signs of life. Astronomers goal with Kepler’s transit detection method is to search for Earth-sized planets in the habitable zone that could potentially harbor life !
So, NASA and astronomers worldwide are using the Transit of Venus in a scientifically valuable way – beyond mere enjoyment – to help refine their planet hunting techniques.
Historically, scientists used the Transit of Venus over the past few centuries to help determine the size of our Solar System.
See more event photos from the local daily – The Trenton Times – here
And those who stayed late after sunset – and while the Transit of Venus was still visibly ongoing elsewhere – were treated to an extra astronomical bonus – at 10:07 p.m. EDT the International Space Station (ISS) coincidentally flew overhead and was visible between more break in the clouds.
Of course clouds are no issue if you’re watching the Transit of Venus from the ISS or the Hinode spacecraft. See this Hinode Transit image published on APOD on June 9 and enhanced by Marco Di Lorenzo.
This week, local NY & NJ residents also had another extra special space treat – the chance to see another last-in-a-lifetime celestial event: The Transit of Space Shuttle Enterprise across the Manhattan Skyline on a seagoing voyage to her permanent new home at the Intrepid Sea, Air and Space Museum.
Well, not the sky exactly, but definitely in the clouds!
This image, acquired by NASA’s Aqua satellite on June 5, shows an enormous oval hole in the clouds above the southern Pacific Ocean, approximately 500 miles (800 km) off the southwestern coast of Tasmania. The hole itself is several hundred miles across, and is the result of high pressure air in the upper atmosphere.
According to Rob Gutro of NASA’s Goddard Space Flight Center, “This is a good visible example of how upper-level atmospheric features affect the lower atmosphere, because the cloud hole is right under the center of a strong area of high pressure. High pressure forces air down to the surface blocking cloud formation. In addition, the altocumulus clouds are rotating counter-clockwise around the hole, which in the southern hemisphere indicates high pressure.”
The northwestern tip of Tasmania and King Island can be seen in the upper right of the image.
The Aqua mission is a part of the NASA-centered international Earth Observing System (EOS). Launched on May 4, 2002, Aqua has six Earth-observing instruments on board, collecting a variety of global data sets about the Earth’s water cycle. Read more about Aqua here.
I’m not sure how often this happens, but I’ve never seen it before: crepuscular rays on both the west and east horizon at the same time — or crepuscular and anti-crepuscular rays occurring simultaneously. I’m staying out in the wilds of Minnesota this summer, with great views of both horizons and captured these images last evening, June 9, 2012. The word crepuscular means “relating to twilight,” and these rays occur when objects such as mountain peaks or clouds partially shadow the Sun’s rays, usually when the Sun is low on the horizon. These rays are visible only when the atmosphere contains enough haze or dust particles so that sunlight in unshadowed areas can be scattered toward the observer.
Then occasionally, light rays scattered by dust and haze sometimes appear on “antisolar” point, (the horizon opposite to the setting sun). These rays, called anti-crepuscular rays, originate at the Sun, cross over the sky to the opposite horizon, and appear to converge toward the antisolar point.
Anyone else ever seen this before?
For both crepuscular and anti-crepsucular, the light rays are actually parallel, but appear to converge to the horizon due to “perspective,” the same visual effect that makes parallel railroad tracks appear to converge in the distance. One of the astronauts on the International Space Station actually captured crepuscular rays from orbit, showing how the rays are actually parallel. You can see that image and the description here.
Below are the two images separately. It was a beautiful evening and a thrilling sight.
Here’s a quick look at one of my favorite cosmic photo subjects – the varying layers of atmosphere that enshroud Saturn’s enormous moon Titan. The image above is a color-composite made from three raw images acquired by Cassini during its latest flyby.
On June 7 Cassini approached Titan within 596 miles (959 km) and imaged portions of the moon’s northwest quadrant with its radar instrument, as well as conducted further investigations of areas near the equator where surface changes were detected in 2010.
The image here was assembled from three raw images captured in red, green and blue visible light channels. It reveals some structure in the upper hydrocarbon haze layers that extend upwards above the moon’s opaque orange clouds — reaching 400-500 km in altitude, Titan’s atmosphere is ten times thicker than Earth’s!
The June 6 flyby was the second in a series of passes that will take Cassini into a more inclined orbit, where it will reside for the next three years as it investigates Saturn’s polar regions and obtains better views of its ring system.
Remember the Norway Spiral back in 2009 and the Australian Spiral in 2010? On June 7, 2012 there was another swirling spiral of light, this time see in the skies over the Middle East. People across the region reported seeing a “UFO” and soon videos began showing up on YouTube.
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During the May 20 annular eclipse, two teams sent a duo of high altitude balloons to simultaneously capture the event, and they got some amazing pictures. Not only did the two imaging systems on the balloons take pictures of the eclipse, but they also took pictures of each other, with both balloons near the edge of space. “Our goal was to launch 2 capsules to the edge of space to shoot photos and high-definition videos during the annular solar eclipse,” David Gonzales of Project Soar told Universe Today.
Project Soar has sent seven balloon launches with their reusable PURSUIT capsule to take images of Earth and space. They teamed up with Larry Grater who sent his North Texas Near Space capsule NTNS-1 on its maiden flight.
“In several of the images, you can see NTNS-1 under its balloon as shot from PURSUIT against a pitch black sky,” Gonzales said via email. “Despite the sun being high in the sky during the flights, you can see how dark the ground got in some of the images due to sun being mostly covered by our moon. Unlike a total eclipse though, there is no obvious dark spot as the transition between full annular and partial eclipse around the center-line is very gradual and not as sharp as in a total eclipse.”
Also visible is the eclipse in various stages as Sun-shaped lens flare in many the images.
The launch sites were chosen just hours before launch to ensure the trajectories would stay on the center-line for the eclipse and avoid overflying any restricted airspace, Gonzales said.
“We had a particularly challenging countdown as 2 balloons had to be filled with Hydrogen for a very narrow launch window,” he said.
Both capsules took to the skies on time from an East Albuquerque hiking park, and then had to immediately clear the Sandia mountains right after liftoff before continuing their journeys to the edge of space. As the team and other onlookers enjoyed the annular eclipse from the ground, the two balloons shot photos and videos from near space.
Here’s a compilation of the HD video that was shot, with an amazing view of the PURSUIT capsule falling after burst at high altitude (at 8:53). “NTNS-1 caught PURSUIT right after burst in the video,” Gonzales said. “I don’t think I’ve ever seen imagery of a capsule falling after burst at high altitude before.” Other key events in the video are NTNS-1 and PURSUIT close pass at 0:52, the PURSUIT Capsule visible at 7:24, PURSUIT descent at 8:53, NTNS-1 Burst at 11:41
Eclipse Soar was a collaborative effort between Project Soar of San Antonio and North Texas Near Space of Dallas.
Editor’s note: This guest post was written by Andy Tomaswick, an electrical engineer who follows space science and technology.
If humans are planning on spending any significant amount of time on the surface of another planet in the solar system, they’re going to need a specially made habitat to live in. Developing a prototype of that habitat is the goal of the NASA Advanced Exploration Systems Habitation Systems project, which sponsors the annual eXploration Habitat (X-Hab) challenge. To achieve this, NASA and the National Space Grant Foundation solicited ideas for module design ideas from universities back in March. On May 30th, the X-Hab challenge organizers selected 5 university teams to participate in the competition. The winning teams and their research concepts are:
California State Polytechnic University – “Vertical Habitability Layout and Fabrication Studies”
Oklahoma State University- “Horizontal Habitability Layout Studies”
Texas A&M University – “Wireless Smart Plug for DC Power”
University of Alabama at Huntsville – “Design and Development of a Microgravity Random Access Stowage and Rack System”
University of Colorado at Boulder – “Remote Plant Food Production Capability”
The teams are comprised primarily of undergraduate students, which NASA hopes will help train the next generation of scientists and engineers to work on future projects. They have a challenging journey ahead of them, as their selection is the first step in a process that will see the teams developing, delivering and testing their concepts within a year. The technologies from this year will add to the technologies from previous years, giving NASA a growing collection of ideas to draw from. With the continued success of the program, NASA’s next habitation module might primarily be designed by students.