Historic SpaceX Dragon Docking to ISS – Highlights Video

SpaceX has released a cool video (above) recapping the mission highlights of the historic May 22 blastoff of the firm’s Falcon 9 rocket with the Dragon spacecraft that went on to become the first privately developed vehicle in history to successfully dock to the International Space Station (ISS) on May 25, 2012.

Dragon was captured with a robotic arm operated by astronauts Don Pettit and Andre Kuipers working in tandem aboard the ISS as it approached the massive orbiting lab complex and was then berthed at an Earth facing port.

Dragon was the first US spacecraft to attach to the ISS since the retirement of NASA’s Space Shuttle program last July 2011 following the STS-135 mission of shuttle Atlantis. The 14.4 ft (4.4 meter) long resupply vehicle delivered over 1000 pounds of non-critical gear, food, clothing and science equipment to the ISS.

After spending six days at the ISS, the Dragon undocked and splashed down in the Pacific Ocean some 560 miles off the coast of California on May 31, 2012.

Image Caption: SpaceX Falcon 9 rocket clears the tower after liftoff at 3:44 a.m. on May 22, 2012 from Space Launch Complex-40 at Cape Canaveral Air Force Station, Fla.,on the first commercial mission to loft the Dragon cargo resupply vehicle to the International Space Station. Credit: Ken Kremer/www.kenkremer.com

The Falcon 9 rocket and Dragon cargo carrier were designed, developed and built by Hawthorne, Calif., based SpaceX Corporation, founded in 2002 by CEO and Chief Designer Elon Musk.

SpaceX signed a contract with NASA in 2006 to conduct twelve Falcon 9/Dragon resupply missions to carry about 44,000 pounds of cargo to the ISS at a cost of some $1.6 Billion over the next few years. The first operational Dragon CRS mission is slated to blast off around October 2012.

Read my Universe Today articles starting here for further details about the historic SpaceX Falcon 9/Dragon mission to the ISS.

Ken Kremer

Case Closed on the Pioneer Anomaly

Caption: An artist’s view of a Pioneer spacecraft heading into interstellar space. Both Pioneer 10 and 11 are on trajectories that will eventually take them out of our solar system. Image credit: NASA

The case of the Pioneer Anomaly has intrigued and perplexed scientists, engineers and the space-savvy public since 1980, when analysis of tracking data from the twin Pioneer spacecraft showed a small, unexplained slowing of the duo. The answer to this puzzle — now firmly found — lies not in weird physics or mysterious dark matter, but simply the effect of heat pushing back on the spacecraft – heat from the spacecraft itself, emanating from electrical current flowing through instruments and the thermoelectric power supply.

If you’re thinking, “hasn’t this mystery been solved before?” – you’d be right.

Slava Turyshev from the Jet Propulsion Laboratory has laboriously worked on the project since 2004, recovering files from back corners of NASA closets and boxes that were on their way to the trash, converting 1970s punch card data to today’s digital format, and poring over all the data that the spacecraft have beamed back to Earth from billions of miles away.

Along the way, Turyshev has published a couple of papers on his work (here’s one from 2011), and in April of this year, The Planetary Society – who was supporting in part Turyshev’s research – claimed victory that the Pioneer Anomaly was solved.

But now, Turyshev has officially published his findings in the journal Physical Review Letters, and JPL saw fit to put out a press release.

However, over the years other scientists figured out that the culprit might be the heat coming from the spacecraft’s components. In 2001, for example, a scientist named Louis K. Sheffer published a paper, “Conventional Forces can Explain the Anomalous Acceleration of Pioneer 10” and with some good number crunching, determined that “non-isotropic radiation of spacecraft heat” could account for the slowing and “that the entire effect can be explained without the need for new physics.”

Why Sheffer’s paper wasn’t considered more seriously is uncertain, but perhaps at that time the “new physics” idea – that we may have to revise our understanding of gravitational physics — was more intriguing than a mundane effect like heat from the spacecraft’s systems.

But nonetheless, it appears everyone is satisfied with the explanation dutifully resolved by Turyshev and his team of mostly volunteer helpers. And Turyshev’s description of the effect is beautiful in its simplicity:

“The effect is something like when you’re driving a car and the photons from your headlights are pushing you backward,” he said. “It is very subtle.”

Launched in 1972 and 1973 respectively, Pioneer 10 and 11 are still heading on an outward trajectory from our Sun. In the early 1980s, navigators saw a deceleration on the two spacecraft, in the direction back toward the Sun, as the spacecraft were approaching Saturn. They dismissed it as the effect of small amounts of leftover propellant still in the fuel lines. But by 1998, as the spacecraft kept traveling on their journey and were over 13 billion kilometers (8 billion miles) away from the Sun, a group of scientists led by John Anderson of JPL realized there was an actual deceleration of about 300 inches per day squared (0.9 nanometers per second squared). They were the ones who raised the possibility that this could be some new type of physics that contradicted Einstein’s general theory of relativity.

After that, all sorts of theories surfaced, some fairly wacky, some more serious.

In 2004, Turyshev decided to really dig into the matter and started gathering records stored all over the country to analyze the data to see if he could definitively figure out the source of the deceleration. In part, according to JPL, Turyshev and his colleagues were contemplating a deep space physics mission to investigate the anomaly, and he wanted to be sure there was one before asking NASA for a spacecraft.

And so they went searching for Doppler data, telemetry data, and anything they could find about the spacecraft, including picking the brains of navigators who worked with the spacecraft over the years.

They collected more than 43 gigabytes of data, which may not seem like a lot now, but is quite a lot of data for the 1970s. He also managed to save a vintage tape machine that was about to be discarded, so he could play the magnetic tapes. Viktor Toth from Canada, heard about the effort and helped create a program that could read the telemetry tapes and clean up the old data.

They saw that what was happening to Pioneer wasn’t happening to other spacecraft, mostly because of the way the spacecraft were built. For example, the Voyager spacecraft are less sensitive to the effect seen on Pioneer, because its thrusters align it along three axes, whereas the Pioneer spacecraft rely on spinning to stay stable.

Turyshev and his colleagues were able to calculate the heat put out by the electrical subsystems and the decay of plutonium in the Pioneer power sources, which matched the anomalous acceleration seen on both Pioneers.

“The story is finding its conclusion because it turns out that standard physics prevail,” Turyshev said. “While of course it would’ve been exciting to discover a new kind of physics, we did solve a mystery.”

Turyshev’s paper: Finding the Origin of the Pioneer Anomaly.

Source: JPL

Looking Into the Heart of a Quasar

Caption: Artist’s impression of the quasar 3C 279. Credit: ESO/M. Kornmesser

From an ESO press release:

An international team of astronomers has observed the heart of a distant quasar with unprecedented sharpness, two million times finer than human vision. The observations, made by connecting the Atacama Pathfinder Experiment (APEX) telescope to two others on different continents for the first time, is a crucial step towards the dramatic scientific goal of the “Event Horizon Telescope” project: imaging the supermassive black holes at the centre of our own galaxy and others.

Astronomers connected APEX, in Chile, to the Submillimeter Array (SMA) in Hawaii, USA, and the Submillimeter Telescope (SMT) in Arizona, USA. They were able to make the sharpest direct observation ever of the center of a distant galaxy, the bright quasar 3C 279, which contains a supermassive black hole with a mass about one billion times that of the Sun, and is so far from Earth that its light has taken more than 5 billion years to reach us. APEX is a collaboration between the Max Planck Institute for Radio Astronomy (MPIfR), the Onsala Space Observatory (OSO) and ESO. APEX is operated by ESO.

The telescopes were linked using a technique known as Very Long Baseline Interferometry (VLBI). Larger telescopes can make sharper observations, and interferometry allows multiple telescopes to act like a single telescope as large as the separation — or “baseline” — between them. Using VLBI, the sharpest observations can be achieved by making the separation between telescopes as large as possible. For their quasar observations, the team used the three telescopes to create an interferometer with transcontinental baseline lengths of 9447 km from Chile to Hawaii, 7174 km from Chile to Arizona and 4627 km from Arizona to Hawaii. Connecting APEX in Chile to the network was crucial, as it contributed the longest baselines.

The observations were made in radio waves with a wavelength of 1.3 millimetres. This is the first time observations at a wavelength as short as this have been made using such long baselines. The observations achieved a sharpness, or angular resolution, of just 28 microarcseconds — about 8 billionths of a degree. This represents the ability to distinguish details an amazing two million times sharper than human vision. Observations this sharp can probe scales of less than a light-year across the quasar — a remarkable achievement for a target that is billions of light-years away.

The observations represent a new milestone towards imaging supermassive black holes and the regions around them. In future it is planned to connect even more telescopes in this way to create the so-called Event Horizon Telescope. The Event Horizon Telescope will be able to image the shadow of the supermassive black hole in the centre of our Milky Way galaxy, as well as others in nearby galaxies. The shadow — a dark region seen against a brighter background — is caused by the bending of light by the black hole, and would be the first direct observational evidence for the existence of a black hole’s event horizon, the boundary from within which not even light can escape.

The experiment marks the first time that APEX has taken part in VLBI observations, and is the culmination of three years hard work at APEX’s high altitude site on the 5000-metre plateau of Chajnantor in the Chilean Andes, where the atmospheric pressure is only about half that at sea level. To make APEX ready for VLBI, scientists from Germany and Sweden installed new digital data acquisition systems, a very precise atomic clock, and pressurized data recorders capable of recording 4 gigabits per second for many hours under challenging environmental conditions. The data — 4 terabytes from each telescope — were shipped to Germany on hard drives and processed at the Max Planck Institute for Radio Astronomy in Bonn.

The successful addition of APEX is also important for another reason. It shares its location and many aspects of its technology with the new Atacama Large Millimeter/submillimeter Array (ALMA) telescope. ALMA is currently under construction and will finally consist of 54 dishes with the same 12-metre diameter as APEX, plus 12 smaller dishes with a diameter of 7 metres. The possibility of connecting ALMA to the network is currently being studied. With the vastly increased collecting area of ALMA’s dishes, the observations could achieve 10 times better sensitivity than these initial tests. This would put the shadow of the Milky Way’s supermassive black hole within reach for future observations.

Shimmering Aurora Australis Timelapse

Our friends in the Southern Hemisphere have been enjoying some lovely auroral displays following the Sun’s recent activity. Here’s a new timelapse video of the night sky view on July 17, 2012, compiled by Maki Yanagimachi at Mt. John University Observatory in New Zealand. Enjoy the multi-colored aurora shimmering across the sky.

CosmoQuest Offering Online Astronomy Course

Want to brush up on your astro-knowledge? Wishing you had taken that Astronomy 101 course in college? CosmoQuest – the citizen science and web-based astronomy community — is offering online astronomy courses, and their first offering is now open for signups! “CQX 001: Solar System Science” is an 8-session, 4-week course, exploring the solar system, planetary geology, and extrasolar planets.

“Not everyone has access to astronomy and space science classes,” said Dr. Pamela Gay, the founder of CosmoQuest. “With CosmoQuest, we’re looking to make the universe accessible to everyone at a cost comparable to what you might pay for dance or music lessons.”

The classes will be offered online through a Google+ Hangout, and this first course offering will be taught by someone familiar to Universe Today readers: Ray Sanders, who contributes to UT and also answers astronomy questions at his blog, Dear Astronomer. Ray is a research assistant at Arizona State University.

“By combining Hangout technology with educational content, we’ll be able to deliver an outstanding classroom experience,” Ray said. “In this first course, CosmoQuest students will be able to participate in typical “Astro 101” solar system course material – our Sun and its planets. We’ll also briefly explore Pluto’s status, astrobiology, geology, and planetary systems outside our solar system.”

“Solar System Science” is just the first of many classes that CosmoQuest has planned.

“In the coming months, we’ll be opening courses on data reduction, observing, stars, galaxies, and more,” said Pamela. “Our goal is to prepare people to take part in more and more advanced citizen science programs over time.”

If you’ve ever participated in a Google+ Hangout, you know how fun they can be. Here’s a chance to use a Hangout to really put your brain to work over the summer!

“By keeping the classes small and meeting “face-to-face” using Google Hangouts, CosmoQuest’s online classes let students engage in content-rich real-time dialogue with their instructor and fellow classmates,” said Georgia Bracey, who is with the Education & Public Outreach team at Cosmoquest. “This brings a high level of flexibility, depth, and student-centeredness to the class in a way that’s not usually possible in a traditional lecture course.”

The cost for the class is $240, and the class is limited to 8 participants. This first CosmoQuest Academy class begins on July 24, 2012. You can find out more information and sign up at this link.

Barnstorming the Moon’s Giordano Bruno Crater

Caption: Southern rim of Giordano Bruno crater seen obliquely by LROC. Credit: NASA/GSFC/Arizona State University

At the 2012 Lunar Science Forum going on this week at the NASA Lunar Science Institute, scientist Mark Robinson presented some new stunning images from the Lunar Reconnaissance Orbiter’s cameras (LROC), including this oblique view Giordano Bruno crater, and a wonderful video (below) that allows viewers to “barnstorm” over the crater to witness the stark beauty of this impact basin.

“I could spend weeks and months looking at the preserved materials in the crater,” Robinson said, adding that views like this are helping scientists to understand the impact process. “Until astronauts visit Giordano Bruno, this gives a view about as close as you can get to standing on the surface to the west of the crater.”

Robinson is the Principal Investigator for LROC, and in his talk today said all systems on LROC are working nominally. “That’s NASA-speak for everything is fantastic,” he joked.

With the wide angle camera, LROC has mapped the entire Moon nearly 33 times. “Every map has a different photometric geometry, so this is not a redundant dataset,” Robinson said, adding that the different lighting provides different ways to study the Moon. “And to be able to do follow-up observations, I can’t tell you how great it is.”

Just about every month, the science team is able to take new mosaics of both the north and south pole, and they’ve also found 160 pits – lunar caves – so far. These caves with “skylights” are intriguing because they would offer potential protective habitats for future lunar explorers.

Now in its extended mission, LRO is still going strong, and has provided incredible details of the lunar surface. LRO project scientist Richard Vondrak said since the start of the mission, LRO has uploaded 325 terabytes of data into the Planetary Data System, the digital storehouse for NASA science mission, through June 2012.


Caption: Close-up detail of the rim of Giordano Crater. Credit: NASA/GSFC/Arizona State University

“Thanks to LRO, the Moon’s topography is now better understood than the Earth, since two-thirds of Earth is covered by water,” Vondrak said.
But both scientists agrees LRO is just getting started.

“The Moon is one of the most engaging bodies in the Solar System and we’ve still got a lot of work to do,” Robinson said

Robinson suggests scrolling through all of the details of this beautiful impact crater by looking at the full-resolution version of Giordano Crater — “not to be missed!” he said. Also, the full resolution version of the video can be downloaded here.

Sources: NLSI Lunar Forum, LROC website

Where Has the Spirit of Exploration Gone?

Noted space author Andrew Chaikin has started a video series in response to the drastic cuts proposed for planetary science. This second video in the series features Mars scientist Nathalie Cabrol, who urges America to explore space even in difficult economic times.

Chaikin says he is fighting back against the proposed cuts “with passion — passion for the incredible adventure that began half a century ago and has given us countless wonders and amazing discoveries. I’m making these videos as a call to action.”

Postcards From The (Inner) Edge

As the world turns its gaze outward in anticipation of the arrival of Mars Science Laboratory — with its hair-raising “seven minutes of terror” landing — let’s take a moment to look back inward, where MESSENGER is still faithfully orbiting the first rock from the Sun, Mercury, and sending back images that could only have been imagined just a few years ago.

The image above shows the graben-gouged terrain around Balanchine crater, within Mercury’s vast Caloris Basin impact crater. Named for the co-founder of the New York City Ballet, Balanchine crater is 41 km (25.5 miles) in diameter and filled with the curious erosion features known as hollows. Graben — basically sunken troughs in the surface — are the result of extensional forces that have pulled sections of the planet’s upper crust apart.

This image shows the peak-ring structure located within the much larger crater Rustaveli, which is 180 km (112 miles) in diameter. One of the more recently-named craters (the IAU convention for new features on Mercury has them titled after renowned artists, writers and composers from history) Rustaveli is named for a 12th-century Georgian poet who wrote the epic “The Knight in the Panther’s Skin”. The crater that now bears his namesake is located on Mercury’s northern hemisphere.

These two craters — also located within Caloris Basin — don’t yet have names but are no less interesting. Their overlapping positions works like an optical illusion, making the newer,sharper-edged crater on the right seem to almost float above the surface. The false-color of the image highlights the difference in surface composition of the two craters, which are both about 40 km (24 miles) wide. (The Caloris Basin in which they reside, however, is one of the largest known impact sites in our solar system, measuring at 1550 km — 963 miles — across!)

Now we zoom out for a wider view of our solar system’s second-densest planet (Earth is the first) and take a look at an image that’s night and day — literally! This is Mercury’s terminator, the twilit dividing line between night and day. More than just making a pretty picture, data on this transition is valuable to scientists as some atmospheric phenomena can only be observed at the terminator, such as the interaction between surface dust and charged particles from the Sun (which, at less than half the distance to the Sun than we are, Mercury is constantly bathed in.)

And now to zoom back in, we get a good look at an unnamed central-peaked crater about 85 km (52 miles) across in an oblique view  that highlights the hollows and depressions within its floor. Acquired as part of what’s called a “targeted observation”, high-resolution images like this (79 meters/pixel) allow scientists to closely investigate specific features — but sadly there’s just not enough mission time to image all of Mercury at this level of detail.

On March 17, 2011 (March 18, 2011, UTC), MESSENGER became the first spacecraft ever to orbit Mercury. The mission has provided the first data from Mercury since Mariner 10, over 30 years ago. After over 1,000 orbits, 98 percent of Mercury is now imaged in detail, allowing us to know more about our solar system’s innermost world than ever before.

Keep up with MESSENGER updates (and the latest images) on the mission website here.

Image credits: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

New Crew Welcomed Aboard the Space Station

On the 37th anniversary of the Apollo-Soyuz docking, a new international crew of three arrived at the International Space Station. Veteran Russian cosmonaut Yuri Malenchenko, NASA astronaut Suni Williams, and JAXA astronaut Aki Hoshide and joined their Expedition 32 crewmates early Tuesday, bringing the crew compliment on the station back to six.

Williams compared the Soyuz flight to camping and being on the ISS like a coming to a nice hotel.
Continue reading “New Crew Welcomed Aboard the Space Station”

Problems with Mars Odyssey Could Impact Telemetry for Curiosity Rover’s Landing

Caption: NASA’s Mars Odyssey spacecraft passes above Mars’ south pole in this artist’s illustration. The spacecraft has been orbiting Mars since October 24, 2001. Image credit: NASA/JPL

The “seven minutes of terror” could stretch into a longer time of trepidation for the hopeful Mars rover team and fans waiting back on Earth to find out if the Curiosity rover has landed safely. A problem with the Mars Odyssey orbiter means there could be a delay in the telemetry relayed to Earth as the Mars Science Laboratory descends and lands on Mars on August 5/6, 2012.

“There’s no impact to landing itself,” said NASA’s Mars exploration program chief Doug McCuistion at a press briefing on Monday. “It’s simply how that data gets returned to us and how timely that data is.”

McCuistion said the Odyssey team is assessing why the orbiter has gone into safe mode several times since early June, as well as having problems with its attitude control system. The glitches possibly could mean the spacecraft may not be in position to track and relay real-time data from MSL as it descends through Mars’ atmosphere and lands, possibly delaying the telemetry to Earth by several hours.

Curiosity’s automated landing sequence won’t be affected; it’s just that the data won’t be sent immediately – and the 14-minute communications lag between Earth and Mars means that the MSL team won’t be getting real-time updates about the rover’s perilous journey anyway; however, now it might be an even longer delay.

Caption: This artist’s concept from an animation depicts Curiosity, the rover to be launched in 2011 by NASA’s Mars Science Laboratory, as it is being lowered by the mission’s rocket-powered descent stage during a critical moment of the “sky crane” landing in 2012. Image Credit: NASA/JPL-Caltech

The rover is scheduled to land at 10:31 p.m. PDT on Aug. 5 (05:31 UTC, 1:31 a.m. EDT on Aug. 6).

Under normal circumstances, it’s a challenge for the orbiters to get in position to welcome another spacecraft to Mars, and provide tracking data and telemetry relay.

“If we were not to do anything, the Mars’ orbiting spacecraft may be on the other side of the planet,” said MSL navigation team chief Tomas Martin-Mur, during a previous interview with UT. “So as soon as we launch, we tell the other spacecraft where we are going to be by the time of entry so they can change their orbits over time, so they will be flying overhead as MSL approaches the planet.”

The orbiters – which also includes NASA’s Mars Reconnaissance Orbiter and ESA’s Mars Express – have been doing special maneuvers to be aligned in just the right place, nearby to MSL’s point of entry into Mars’ atmosphere.

But the glitches for Odyssey means it may not be in the right place.

MRO will be attempting to image the rover as it descends and lands — with possible hopes of catching the rover as it is descending on the “sky-crane” landing system — but MRO can only record data for later playback, whereas Odyssey could provide immediate relay. Mars Express won’t be aligned to see the last minute of flight, McCuistion said.

The Odyssey orbiter put itself in the precautionary, Earth-pointed status called safe mode on July 11, as it finished a maneuver adjusting, or trimming, its orbit. Odyssey’s computer did not reboot, so diagnostic information was subsequently available from the spacecraft’s onboard memory. Based on analysis of that information, the mission’s controllers sent commands yesterday morning taking Odyssey out of safe mode and reorienting it to point downward at Mars.

“We are on a cautious path to resume Odyssey’s science and relay operations soon,” said Gaylon McSmith, Odyssey project manager. “We will also be assessing whether another orbit trim maneuver is warranted.”

The landing is one of the most perilous times for a rover. “Those seven minutes are the most challenging part of this entire mission,” said Pete Theisinger, MSL’s project manager. “For the landing to succeed, hundreds of events will need to go right, many with split-second timing and all controlled autonomously by the spacecraft. We’ve done all we can think of to succeed. We expect to get Curiosity safely onto the ground, but there is no guarantee. The risks are real.”

We’ll provide updates as to Odyssey’s status. Here’s a look at the seven minutes of terror MSL will experience:

Sources: JPL, NASA