Space and astronomy news
The Carnival of Space 182 is up at nextbigfuture
After a one month hiatus, the Carnival of Space is back. Nextbigfuture will be working with Universe today on the organization of the Carnival of Space. There are hosts signed up into April already.
This week Carnival of space has an animation video of the Mars moon Phobos, nuclear fusion for space propulsion, vacuum engineering, cataclysmic variables and much more.
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It’s comet ahoy! for the Stardust spacecraft, which is on its way to a Valentine’s Day meetup with comet Tempel 1. The images above were taken on Jan. 18 and 19 from a distance of 26.3 million kilometers (16.3 million miles), and 25.4 million kilometers (15.8 million miles). On Feb. 14, Stardust will fly within about 200 kilometers (124 miles) of the comet’s nucleus and for the first time we’ll get a second closeup look at Tempel 1.
“We were there in 2005 with the Deep Impact spacecraft, said Stardust-NExT Project Manager Tim Larson, speaking on today’s 365 Days of Astronomy podcast, “and this is a golden opportunity. It’s the first time we’ve ever been able to revisit a comet on a second pass near the sun.”
Larson said this encounter will give provide important information about how the surface of the comets change with each passage near the sun and whether the changes in the comet are global or just specific to certain areas on the surface.
From the Deep Impact mission, we already know that comet Tempel 1 has a wide variety of features on its surface.
“We have found smooth areas that look like material flows,” Larson said,” there are rough, pitted areas, there are craters on the surface, which we don’t know if they’re impact craters or if they’re caused by material coming out from the inside of the comet. So this is a very interesting comet in terms of variety of terrain.”
The exciting part will be comparing ‘before and after’ images of Tempel 1.
The spacecraft will be able to take up to 72 images and store them on board. Larson said the images will be carefully timed to center them around the closest approach to the comet, providing the best possible resolution.
“We should be able to get around three dozen images that are at better than 80 meters per pixel resolution and our closest approach images should be down below 20 meters per pixel resolution,” he said. “That will be good enough to resolve a lot of the key features on the surface of the comet and start that process of comparison.”
The repurposed Stardust spacecraft that flew past comet Wild 2 and brought back samples has just enough fuel to carry out maneuvers for the upcoming Tempel 1 flyby.
Larson said the preparations in designing the flyby sequences and software are almost complete and are being tested, and now the team is eagerly looking at the daily optical navigation images.
“We’re tracking where the comet is relative to the spacecraft,” he said, “and that will feed into our trajectory correction maneuvers. We have three more of those left before we arrive at the comet, and those will be used to target the spacecraft to the desired flyby point.”
The TCMs will occur on January 31, February 7, and then the last fully designed TCM will occur on February 12, two days before arrival.
There are challenges to using a recycled spacecraft.
“The primary challenge is, first of all, designing a new mission that it can accomplish with the fuel that it has left,” Larson said. “And through some clever mission design using some carefully timed trajectory correction maneuvers and taking advantage of some Earth gravity assists, we were able to modify the trajectory of the spacecraft to get it close to Tempel 1. So that’s been the primary challenge, and along with that is conserving the fuel that we have on board and making sure that we have enough fuel left to finish off this mission. Beyond that, there have been a few challenges in terms of aging equipment on board the spacecraft, — the spacecraft will be 12 years old in early February, and it’s well beyond its design life. And although everything is generally healthy on board, we have had a couple of pieces of equipment that were starting to age, and starting to degrade slightly. So we switched over to backup equipment so we were on fresh, healthy equipment, and we still have functioning equipment as backups.”
The closest approach will occur at 8:30 pm Pacific Time on February 14, 2011, where the spacecraft will be about 200 kilometers (125 miles) away from the surface of the comet, which is the closest any spacecraft has been to the surface of a comet.
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Christa McAuliffe never had the chance to fulfill her dream of teaching from space and in the aftermath of the accident, her lesson plans were filed away by NASA with sadness and grief. The lessons were incomplete, unfinished, and most regrettably, they were never were taught. I wrote an article two-and-a-half years ago how NASA engineer Jerry Woodfill — the same endearing engineer from our series “13 Things That Saved Apollo 13” — had come across McAuliffe’s unfinished lesson plans by accident and worked for several months to resurrect them and give them new life with current technology. On this 25th anniversary of the Challenger accident, I wanted to remind our readers of this engaging story, and how the Challenger Centers for Space Science Education are now using McAuliffe’s lessons. The lessons are also available for any teacher, or anyone who wants to view or use them.
Also, the Challenger Centers offer a wonderful education resource and experience for young people. Please consider donating to their mission, started by the families of the Challenger astronauts lost in the accident. Your donation will honor the Challenger 7 heroes and help inspire the next generation.
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In remembrance of the Challenger accident 25 years ago today, several notable people have issued statements in memory of the Challenger crew, as well as the crews of Apollo 1 and Columbia. Below are a few; add your own, if you like, in the comments section.
Also, if you haven’t already, watch the new Challenger 25th anniversary tribute song and video by Stephen Kay.
NASA also has an interactive feature remember the three crews.
Additionally, a high-quality documentary about the accident has been produced by SnagFilms, an online library of more than 2000 documentary films available to view for free. The film, which you can access below, is called “Catastrophic Failure.”
Statement by Steven J. McAuliffe on the 25th Anniversary of the Challenger Accident
“That people across the country steadfastly remember the crew members of Challenger is both comforting and inspirational to our family. Scott, Caroline and I very much appreciate the kind thoughts and continuous support we have received over the years.
Christa confidently and joyfully embraced life, no less than her friends and colleagues on Challenger, and no less than the crews of Columbia , Apollo 1, and all of those people who courageously follow their own paths every day. I know Christa would say that that is the most precious lesson – ordinary people can make extraordinary contributions when they remain true to themselves and enthusiastically pursue their own dreams wherever they may lead. Our family knows that generations of students and teachers will continue to share her love of learning and love of life, and will do great things for our world. We believe Christa would be especially pleased by, and proud of the Challenger Center for Space Science Education and its mission. The Challenger Center honors each crew member’s devotion to learning and exploration, touching the lives of over 400,000 students and 40,000 teachers each year. In that way, Challenger Center continues the teaching mission of all the crew members of STS-51-L.”
(About Steven J. McAuliffe: Originally from Massachusetts , Steven McAuliffe now lives in Concord , New Hampshire , where he serves as a Federal judge. He is the widower of Christa McAuliffe, NASA’s Teacher in Space candidate. Steve continues to serve as a Founding Director for Challenger Center for Space Science Education. He has two children, Scott and Caroline, and has remarried.)
US President Barack Obama on NASA’s Day of Remembrance (January 27, 2011)
“Fifty years ago, a young President facing mounting pressure at home propelled a fledgling space agency on a bold, new course that would push the frontiers of exploration to new heights. Today, on this Day of Remembrance when NASA reflects on the mighty sacrifices made to push those frontiers, America’s space agency is working to achieve even greater goals. NASA’s new 21st Century course will foster new industries that create jobs, pioneer technology innovation, and inspire a new generation of explorers through education – all while continuing its fundamental missions of exploring our home planet and the cosmos.
Throughout history, however, we have seen that achieving great things sometimes comes at great cost and we mourn the brave astronauts who made the ultimate sacrifice in support of NASA missions throughout the agency’s storied history. We pause to reflect on the tragic loss of the Apollo 1 crew, those who boarded the space shuttle Challenger in search of a brighter future, and the brave souls who perished on the space shuttle Columbia.
Though triumph and tragedy, each of us has benefited from their courage and devotion, and we honor their memory by dedicating ourselves to a better tomorrow. Despite the challenges before us today, let us commit ourselves and continue their valiant journey toward a more vibrant and secure future.”
Message from NASA Administrator Charlie Bolden: Day of Remembrance
“The last week of January every year brings us the opportunity to reflect on the sobering realities of our space exploration enterprise. Each time men and women board a spacecraft, their actions carry great risk along with the opportunity for great discoveries and the chance to push the envelope of our human achievement. Today, we honor the Apollo 1, Challenger and Columbia crews, as well as other members of the NASA family who lost their lives supporting NASA’s mission of exploration. We thank them and their families for their extraordinary sacrifices in the service of our nation.
This year marks the 25th anniversary of the loss of Challenger — a tragedy that caused us to completely re-think our systems and processes as we worked to make the shuttle safer. The nation will never forget Jan. 28, 1986, nor its indelible images. The astronauts in that crew were personal friends of mine, as were the astronauts aboard Columbia when it was lost. The Apollo I crew perished while I was studying at the Naval Academy, and I mourned their loss in the line of duty with the nation. These brave men and women will always be a part of us, and we are still building on their legacies.
NASA has learned hard lessons from each of our tragedies, and they are lessons that we will continue to keep at the forefront of our work as we continuously strive for a culture of safety that will help us avoid our past mistakes and heed warnings while corrective measures are possible. In memory of our colleagues, I ask the NASA Family once again to always make its opinions known and to be unafraid to speak up to those in authority, so that safety can always be our guiding principle and the sacrifices of our friends and colleagues will not be in vain.
On this Day of Remembrance, as we honor our fallen heroes with tributes and public ceremonies, I will take part in a wreath-laying ceremony at Arlington National Cemetery. Across the country, flags at NASA Headquarters and the NASA centers will be flown at half-mast in memory of our colleagues lost in the cause of exploration.
The legacy of those who have perished is present every day in our work and inspires generations of new space explorers. Every day, with each new challenge we overcome and every discovery we make, we honor these remarkable men and women. Please join me in working to fulfill their dreams for the future.”
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Japans critical new resupply spaceship – nicknamed Kounotori2, (HTV2) – was successfully berthed today (Jan. 27) at the International Space Station (ISS). Kounotori2 – which translates as ‘White Stork’ in Japanese – was grappled by the ISS crew and then manually nested to an Earth facing docking port on the Harmony module.
Kounotori2 was launched aboard a Japanese H-IIB rocket from the Tanegashima Space Center in southern Japan at 12:37 a.m. (2:27 p.m. Japan time) on Jan. 22 to begin a five day orbital chase of the station.
View the Video and a Photo album below of the rendezvous and docking sequence
The two ships became one as Astronaut Cady Coleman grappled the free flying ‘White Stork’ at 6:41 a.m. EST with the stations robotic arm while the vessels were flying in formation about 220 miles above the south Indian Ocean in an easterly direction.
After an automatic rendezvous early this morning, the unmanned HTV2 cargo carrier slowly approached the space station from below to a series of ever closer hold points- 250 m, 30 m and 10 m.
Mission controllers on Earth carefully maneuvered the 35,000 pound ship to the final capture distance of about 33 feet (10 meters). The HTV thrusters were disabled and it was placed into ‘free drift’ mode.
ISS astronauts Paolo Nespoli, Cady Coleman and Commander Mark Kelly crew monitored the approach from inside the ISS. The crew was deftly working at the controls of the robotics work station of the Cupola Observation dome.
Finally, Coleman gently grabbed the ‘White Stork’ with the 58 foot long Space Station Robotic arm, built and contributed by Canada.
“Grapple completed, Kounotori is grappled!” tweeted and twitpiced Paolo Nespoli from the ISS.
“This demonstrates what we can do when humans and robots work together,” radioed Cady Coleman.”We look forward to bringing HTV 2 – Kounotori – aboard the International Space Station.”
Video caption: Japanese Cargo Craft Arrives at ISS.
From: NASAtelevision | January 27, 2011
An unpiloted Japanese resupply ship, the “Kounotori”2 H-2B Transfer Vehicle (HTV2 ), was captured and berthed to the Earth-facing port of the Harmony module of the International Space Station Jan. 27, 2011. The berthing took place after an automated five-day flight following its launch on the Japan Aerospace Exploration Agency’s H-2B rocket Jan. 22 from the Tanegashima Space Center in southern Japan. The ‘Kounotori’, which means “white stork” in Japanese, is loaded with more than four tons of supplies and spare parts for the six crew members on the orbital laboratory. Expedition 26 Flight Engineers Cady Coleman and Paolo Nespoli were at the controls of the robotic work station in the space station’s Cupola module to maneuver the Canadarm2 robotic arm for the grapple and berthing of the HTV2, which will remain at the orbital outpost until the end of March
Italian astronaut Paolo Nespoli had the honor of driving Kounotori2 to a hard dock at the station. The attachment was completed at 9:51 a.m. EST after Kelly inspected the docking mechanism and confirmed it was clear of debris and ready. 16 bolts firmly latched the cargo freighter into place a few hours later.
The crew will open the hatch to Kounotori2 on Friday, (Jan. 28) at about 7:30 a.m. This is only the second flight of the Kounotori. The barrel shaped vehicle is coated with 57 solar panels.
Kounotori2 is loaded with over 4 tons of pressurized and unpressurized cargo, including science experiments, research gear, space parts, clothing, food and water and other provisions from Japan, NASA and Canada.
HTV2 will remain docked at the ISS for about two months until late March. During that time the ISS crew will retrieve all the equipment and supplies for transfer to locations both inside and outside the ISS.
Using the Canadian robotic arm and Dextre robot, a pallet loaded with large spare parts for the station will be extracted from a slot on the side of the cargo ship robot and attached to an experiment platform outside the Japanese Kibo module.
On Feb. 18, the ISS crew will move the HTV from the Earth facing port. They will relocate it 180 degrees to the other side of the Harmony module to the space facing zenith port. This maneuver is required to provide enough clearance for Space Shuttle Discovery so that the orbiter can also safely dock at the Harmony module in late February. Discovery is set to launch on Feb. 24.
The HTV2 docking marks the start of an extremely busy time of orbital comings and goings at the ISS.
A Russian Progress resupply ship launches later today, at 8:31 p.m. EST. Following a two day chase, the Progress will dock on Saturday night (Jan. 29) at 9:39 p.m. and deliver over 6000 pounds of cargo to the station. Watch NASA TV
The European ATV cargo ship – named ‘Johannes Kepler – blasts off on Feb. 15.
HTV2 Rendezvous & Docking Photo Album: Jan 27, 2011
All photos Credit NASA and NASA TV
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Today, Jan. 24, 2011 marks the 7th anniversary of the safe landing of the Opportunity Mars Exploration Rover (MER). Opportunity will soon celebrate another remarkable milestone – 2500 Sols, or Martian days, roving the red planet. Together with her twin sister Spirit, the NASA rovers surely rank as one of the greatest feats in the annals of space exploration.
“No one expected Spirit or Opportunity to go on this long,” says Ray Arvidson in an interview from Washington University in St. Louis. Arvidson is the deputy principal investigator for the Spirit and Opportunity rovers.
7 Years ago today on Jan. 24, 2004, NASA’s Opportunity rover daringly smashed into the Martian atmosphere at about 12,000 MPH on a one shot, do or die mission with no certainty as to the outcome. Thus began “The Six Minutes of Terror” as the plummeting probes heat shield endured temperatures exceeding 1400°C (2600 F) during the fiery entry, descent and landing phase (EDL).
The spectacular plunge was slowed by atmospheric friction on the heat shield and a complex pre-programmed combination of parachutes and retro rockets, and in the last moments by inflatable airbags designed to allow the robot to bounce about two dozen times and gently and gradually roll to a complete stop.
Ultimately, Opportunity survived intact just like her twin sister Spirit who landed safely three weeks earlier on Jan. 3, 2004. EDL was the culmination of a seven month interplanetary cruise of over 250 million miles from Earth. Both rovers were launched from Cape Canaveral, Florida in the summer of 2003 on board Delta 2 rockets. The dynamic duo landed on opposite sides of the Red planet.
Opportunity is now 84 months into the 3 month mission – still alive and blazing a trail of Exploration and Discovery across the Meridiani Planum region of Mars.
The amazing Martian robot has driven more than 16.5 miles (26.7 km) and snapped over 148,000 pictures. She has suffered remarkable few mechanical failures and they have only minimally impaired her ability to traverse across the surface and conduct science operations.
Both rovers survived far beyond the mere 3 month “warranty” proclaimed by NASA as the mission began with high hopes following the nail biting “Six Minutes of Terror”. At the time, team members and NASA officials hoped they might function a few months longer.
“The rovers are our priceless assets” says Steve Squyres, of Cornell University who is the Principal Scientific Investigator for the mission. Squyres and the entire rover team treat every day with a “sense of urgency” and as “a gift to science”.
Since 2004, the rover’s longevity has surpassed all expectations and nobody on the science and engineering teams that built and operate the twins can believe they lasted so long and produced so much science.
“We have a new Opportunity overview article publishing shortly in the Journal of Geophysical Research (JGR). The Spirit overview paper appeared recently. In addition, there will be about 24 new scientific papers coming out in the new few months as JGR special issues covering more of the MER results. ”
The incredible longevity is “way beyond the wildest expectations of even the people who built the twin sisters” according to fellow Cornell University Professor Jim Bell. “To say the rovers have surpassed expectations is an understatement. We’ve blown them out of the water”. Bell is the lead scientist responsible for the rovers’ high resolution color imaging system called Pancam.
“After 7 years it is still very exciting,“ Arvidson told me. “I am delighted to come to work every day. It’s great to work on the engineering plan for driving and operating the rovers and then see the results the next day.”
Spirit and Opportunity have accomplished a remarkable series of scientific breakthroughs, far surpassing the wildest dreams of all the researchers and NASA officials. Indeed both Mars rovers are currently stationed at scientific goldmines.
Opportunity is currently exploring the outskirts of the stadium sized ‘Santa Maria’ Carter – some 295 feet wide (90 m) – which holds deposits of water bearing minerals that will further elucidate the potential for habitability on the red planet.
The rover arrived at the western edge of the relatively fresh impact crater on Dec. 16, 2010 (Sol 2451). This intermediate stop on the rovers 19 km long journey from Victoria Crater to giant 22 km wide Endeavour Crater will provide important ground truth observations to compare with the orbital detection of exposures of hydrated sulfate minerals. Read more on Santa Maria in the next feature story.
Santa Maria is just 6 km from the western rim of Endeavour which shows spectral signatures of phyllosilicates, or clay bearing minerals, which formed in water about 4 billion years ago and have never before been directly analyzed on the Martian surface.
Phyllosilicates form in neutral aqueous conditions that could have been more habitable and conducive to the formation of life than the later Martian episodes of more harshly acidic conditions in which the sulfates formed that Opportunity has already been exploring during her 7 year long overland expedition.
Since the moment she landed inside ‘Eagle’ crater, Opportunity has been on a Martian crater tour her entire lifetime.
Opportunity “scored a 300-million mile interplanetary hole in one,” Steve Squyres said at that time, by improbably rolling to a stop smack inside the small 66 foot wide ‘Eagle’ crater (see map) after bouncing across the virtually flat and featureless dusty plains of Meridiani. She has been a lucky princess from the moment of her birth, spying layered sedimentary rocks in a bedrock outcrop from first light in her cameras a mere 26 feet or so away. That’s unlike any previous lander.
Seven days later she drove off the landing pad, drilled into the outcrops and collected the “ground truth” science data to prove that hematite was present and liquid water had indeed flowed at Meridiani as a lake or shallow sea on ancient Mars.
After completing her science campaign, she climbed up and over the rim, departed ‘Eagle’ and arrived at ‘Endurance’ about 3 months after landing day.
After numerous tests, Opportunity was commanded to slowly crawl down into the crater. She gradually descending about 30 vertical feet, frequently drilling into the sedimentary rocks and layers to reveal Mars watery past in unprecedented scientific detail for about six months.
In Dec. 2004, Opportunity departed for “Victoria” crater, which many believed would be her final destination. The robot nearly perished in a sand trap at Purgatory along the way during a nearly two year drive across the treacherous martian sand dunes.
Opportunity arrived in Sept. 2006 to unveil Victoria’s Secrets in color. The rover actually wound up spending two years driving to different vantage points around the rim of and then inside the half mile wide crater before departing in Sept 2008 for the unimaginable goal of giant ‘Endeavour’ crater.
The rover team hopes to reach the slopes of Endeavour sometime later in 2011 if all goes well – before her 8th anniversary !
See below some of the best images taken by Opportunity during her 7 Year Martian Trek
This Opportunity panorama reveals 2,500 ft-wide, 230 ft-deep Victoria Crater from the lip at Duck Bay alcove. Geologic layers reveal the history of Martian water here. The panorama was taken about 8 feet from the crater rim on Sol 952 (28 Sept 2006) as the rover sat between two steep promontories, Cape Verde and Cabo Frio. This vista exposes a thick stack of geologic layers which revealed the hidden watery secrets of the Martian environment farther back in time than any other location visited previously by the rovers. One can see a ½ mile to the distant cliff walls of the crater, above a windswept dune field in the center. This mosaic was assembled from navcam images and featured in Aviation Week & Space Technology magazine and on the Astronomy Picture of the Day (APOD) on 2 Oct. 2006 in high resolution. Credit: NASA/JPL/Cornell, Bernhard Braun, Marco Di Lorenzo, Kenneth Kremer. http://antwrp.gsfc.nasa.gov/apod/ap061002.html
Check out this spherical projection panorama of Opportunity descending inside Victoria Crater on Sol 1332. Credit: NASA/JPL/Cornell/Nasatech.net
Relive Opportunity’s landing:
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A Japanese rocket successfully blasted off early this morning (Jan. 22) on a vital mission bound for the International Space Station (ISS). The launcher carried the Kounotori2 – which means ‘White Stork’ in Japanese – cargo resupply vessel. Kounotori2, also dubbed HTV2, is stocked with over 3800 kilograms (8000 pounds) of crucial science experiments, research gear, food and provisions for the six person international crew living aboard the Earth orbiting outpost.
Liftoff of the unmanned H-IIB rocket from Launch Pad No. 2 at the Tanegashima Space Center occurred earlier today at 2:37:57 p.m. on January 22, local Japan Standard Time (12:37:57 a.m. EST), from a remote island rocket base located in southern Japan.
Watch 2 Videos of the launch below. Especially be sure to view the Japanese version (interspersed with English) which captured dramatic rear-looking video of the receding Earth and its curvature and the separation of the Solid Rocket Boosters (SRBs) – during the ascent to orbit.
The launch was flawless in all respects. The Japanese Space Agency – JAXA – confirmed that the Kounotori2 cargo carrier separated from the launch vehicle as expected at about 15 minutes and 13 seconds after liftoff.
Blast off of the 186 foot tall rocket had been delayed two days by poor weather. By the time of Saturday’s launch, the weather had cleared with a wind speed of 8.3 meters/second from the north-west and the temperature was 10.6 degrees Celsius according to JAXA.
The H-IIB is a two-stage rocket powered by liquid oxygen and liquid hydrogen with four strap-on solid rocket boosters (SRBs) powered by polybutadiene. The SRB’s were jettisoned as planned about two minutes into the flight (see video).
Rendezvous at the ISS is scheduled to take place on Jan. 27.
After the HTV2 arrives in close proximity, astronauts on board will manually dock the cargo ship to the station. Using the stations Canadian built robotic arm, known as Canadarm2, the Expedition 26 crew of Cady Coleman and Scott Kelly from the US and Paolo Nespoli from Italy will grapple HTV2 and berth it to the Earth-facing port on the Harmony module.
Japanese Space Agency – JAXA – HTV Launch Video. In Japanese – interspersed with English
Video Caption: The H-IIB Launch Vehicle No. 2 with the KOUNOTOR 2 (HTV 2) cargo transporter onboard launched from the Tanegashima Space Center in southern Japan at 2:37:57 p.m. on January 22, Sat., Japan Standard Time, (12:37:57 a.m. EST) and is bound for the International Space Station (ISS). KOUNOTORI 2 translates as ‘White Stork’ in Japanese.
HTV Launch with NASA Commentary
This was the second launch of the HTV cargo carrier which was developed by the Japan Aerospace Exploration Agency (JAXA). The maiden launch occurred in September 2009 and was a test flight to demonstrate the autonomous and remotely-controlled rendezvous capabilities while also delivering cargo and supplies to the ISS.
Japan expects to construct and launch about one HTV per year with the capability to ramp up production to two vehicles per year if necessary and if the Japanese government approves funding.
JAXA is evaluating the possibility to convert the HTV into a vehicle capable of flying humans to space.
China, the other Asian superpower, has already established a human spaceflight program.
China has successfully launched three manned capsules to space and is vigorously moving forward with plans to orbit a manned space station.
After the forced retirement of the Space Shuttle later this year, NASA will be completely dependent on commercial companies and foreign governments to launch all of its future cargo requirements to the ISS.
More HTV 2 launch and launch processing photos below from JAXA
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After a more than decade long journey of 6 billion kilometers, hopes are high for a celestial date in space between an icy comet and a thrusting probe on Valentine’s Day 2011. The rendezvous in space between NASA’s approaching Stardust-NExT spacecraft and Comet Tempel 1 takes place nearly on the exact opposite side of the Sun on Feb 14, 2011 at approximately 11:37 p.m. EST (8:37 p.m. PST).
The top science goal is to find out “how much the comet’s surface has changed between two close passages to the sun” since it was last visited in 2005, said principal investigator Joe Veverka of Cornell University, Ithaca, N,Y at a media briefing today, Jan 19, at NASA Headquarters. Indeed it’s the first time in history that a comet has been visited twice by space probes from Earth.
The lead scientists and engineers outlined the plans for the cometary flyby at the briefing. See a video of the entire briefing below.
Since the last visit in 2005, the comet has completed another orbit around the sun. “It will be the first time we’ll be able to see changes after a comet has passed through one perihelion,” explained Veverka. Tempel 1 belongs to the Jupiter family of comets and orbits between Mars and Jupiter.
Comet Tempel 1 suffered a cosmic collision during that first encounter with an emissary from Earth when NASA’s Deep Impact smashed a copper projectile directly into the comets nucleus. The blast created an impact crater and ejected an enormous cloud of gas and debris. Reflected light off the dust particles totally obscured the view of the crater and prevented any images from being taken. Researchers had hoped to determine the size of the crater. A lot of bets hinge on that determination.
“We have a chance to complete the Deep Impact experiment. We hope to see how big the impact crater is and what that tells us about the mechanical properties, ” said Veverka.
With just over 3 weeks remaining, the craft is approximately 24.6 million kilometers (15.3 million miles) away from its encounter. Stardust-NExT will zoom past the nearly 6-kilometer-wide comet (3.7 miles) at a distance of approximately 200 kilometers (124 miles) and at a speed of 10 km/sec according to Tim Larson, the mission’s project manager from the Jet Propulsion Laboratory (JPL), Pasadena, Calif.
“The spacecraft is still working well 12 years after launch. This is a bonus mission with a scientifically desirable target which we can get close to,” said Larson.
“Everything will happen autonomously,” stated Larson. “The craft will be about 2 AU away from Earth at encounter. Since the round trip signals will take about 40 minutes there is no chance for any real time changes.”
“Stardust-NExT will take 72 high resolution images during the close approach encounter. These will be stored in an onboard computer and relayed back to Earth starting about an hour later. It will take about 12 hours to get them all back.”
NASA says that after processing, the images are expected to be available at approximately 4:30 a.m. EST (1:30 a.m. PST) on Feb. 15.
“For the first time we’ll go back to see what happens to a comet since our last visit,” explained Pete Schultz, co-investigator of Brown University, Providence, R.I. “The comet has been out to the orbit of Jupiter and back to Mars and had several outbursts of gas and dust. In 2005 we saw old and new surfaces. So it has a complicated geologic history. We hope to resolve the crater and see ejecta. But there are many unknowns. What we see – whether its the crater or the other unseen side – all depends on the rotation of the comet nucleus.”
“The comet dynamics are complex and erratic, not inert,” said Steve Chesley, a co-investigator at JPL. “They are like a rocket with no one at the controls. The orbit can change. So it is a huge challenge to target a spacecraft for a flyby or rendezvous.”
Stardust-NeXT is a repurposed spacecraft. The Valentine’s Day encounter will be the last hurrah for the aging probe. Stardust was originally launched way back in 1999. It flew by Comet Wild 2 on Jan. 2, 2004 and collected cometary dust particles which were returned to Earth in a sample return capsule in Jan. 2006. Since then it has continued its solitary voyage through the void of the space.
The craft is nearly out of fuel and all movements consume fuel. It is totally dependent on the reaction control thrusters for navigating through space and pointing its camera and science instruments, said Larson.
“We are confident that we will have enough fuel to finish up this mission. It has been a big, big challenge to maintain a reserve supply. After the mission there won’t be much left that the spacecraft can do. The last trajectory correction maneuver is two days before arrival. That is also when we will take our last optical navigation images for targeting the spacecraft.”
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Only about a third of the surface of Tempel 1 was photographed by Deep Impact in 2005. “We’ll be looking at old territory and new and some overlap,” explained Veverka. “The science team is awfully excited and just can’t wait to see the pictures on Valentine’s day.”
“We have no idea how quickly the surface features change and whether its millions of years or days,” concluded Veverka.
“We expect new discoveries no matter what we see,” Larson summed up
Jan. 19, 2010: Science Team Media Briefing
The Stardust spacecraft has been repackaged for the Stardust-NexT mission. Stardust-NExT will rendezvous with Comet Tempel 1 on February 14, giving scientists an opportunity, for the first time, to search a comet’s surface for changes following its orbit around the sun. Mission scientists discussed the relevance of the mission at a briefing at NASA headquarters in Washington
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Spectacular eruptions from Mt Etna are spewing massive quantities of lava, smoke and ash many hundreds of meters high into the skies above the island of Sicily. Mt Etna is the most active volcano in Europe and one of the most active on all of Earth. The volcano rumbled to life again this week on the evening of January 12, 2011 and lit up the night sky. Mt Etna is 3350 meters high and located on the northeast coast of Sicily near the boot of Italy (see above, below).
Updated: comment or send me your Etna erupting photos/accounts to post below.
This fearsome natural wonder is providing an awe inspiring show from both Earth and Space. Local residents and lucky tourists nearby took stunning videos and photos (below) showing fountains of brilliant lava eruptions streaming mightily from the volcano.
Click to Enlarge all images
Amazing photos from space were captured by Earth orbiting satellites from NASA and ESA. NASA’s Terra satellite took the above image on Jan. 11 as Mt Etna was spewing forth smoke or ash just prior to the volcanic eruptions on Jan. 12. The photo of Etna is NASA’s Earth Observatory Image of the Day, today, Jan. 15, 2011.
ESA’s Envisat likewise snapped a gorgeous view of the billowing plume of smoke rising to space (photo at left) and the international crew aboard the ISS, which currently includes Italian astronaut Paolo Nespoli. Perhaps he’ll send us a shot !
Local news and eyewitness accounts say that tremors from the volcano began increasing on Jan. 11. Emissions of volcanic gases and water vapor have been ongoing since late September 2010. The sounds of explosive tremors from deep inside were also detected months ago.
This sizzling hot video – “Etna at Maximum Activity” – is set to music and records the magnificent flowing streams of lava and the thunderous sounds of the crackling, explosive eruptions. Be sure to view at full screen, then just sit back and enjoy !
Plumes of volcanic ash from the eruptions spread across Sicily and forced the closure of the local Fontanarossa airport – nearby to the city of Catania, which is 24 kilometers away.
Rumblings of Mt Etna have been recorded in historical documents dating back to about 1500 BC.
Another short, dramatic video with the raw sounds of the eruption from a group of German tourists visiting the beautiful city of Taormina, Sicily
Eyewitness Description:
“Mount Etna erupted in the evening of January 12, 2011 for around four hours, providing an amazing scenery. We shot this unique video from Taormina on January 12, 2011 at 11.45 p.m. and uploaded it on YouTube.
On the evening of 11th January 2011 an increase in volcanic tremor was recorded at the summit of the volcano. The recorded seismic activity reached a peak at 7 a.m. on 12th January when the source moved from north of NE crater to the SE crater. The eruption started with strombolian explosive activity at SE crater at around 9.p.m. Lava overflowed the eastern rim of SE crater and fed a flow that moved toward the western wall of the Valle del Bove (Valley of the oxen), an ancient huge uninhabited depression on the NE side of the volcano.
The Sicilian communities near the volcano were not threatened by this latest fascinating eruption. Best place to watch the fascinating eruptions of Mount Etna is the town of Taormina, nestled on a hill at 220 meters / 722 feet above the sea level and at a safe linear distance of approx. 28 Km / 17,4 miles from the top craters of the Sicilian volcano.”
A few years back, I visited Mt Etna and was incredibly lucky to witness this spectacle of nature myself. It was an unforgettable experience to see the glowing red-orange colored lava flowing out from the bowels of the Earth. It was like a living being with circulating blood.
In the excitement, I did something that in retrospect was incredibly stupid. I stood on a ledge, perhaps 50 cm thick, right above the porthole of the scalding hot lava erupting from the earth beneath my feet. Many others did too.
Sicily is a lovely place of manmade and natural wonders. Don’t pass up an opportunity to see Etna aflame
Look at Etnaweb (in Italian, but Universal) for a fantastic collection of local photos and webcams of the eruption.
Volcanic eruptions are breathtaking events to behold. The residual plumes of smoke and ash can stay aloft for many years and can also effect how we see other astronomical events such as our view of solar and lunar eclipses.
For a more tranquil view of Earth and inspiration from Carl Sagan, click here
NASA’s Spirit robot is positioned next to an ancient and extinct volcanic feature on Mars. Learn more here
Can you envision a place hotter than Etna ? … A scorching, molten hellish world where the temperatures are unimaginably hot
Read about a newly detected Earth-sized planet with lava flows vastly hotter than Etna – or anywhere on Earth for that matter – in this story about a historic new discovery from NASA’s Kepler space telescope
Comment or send me your photos and eyewitness accounts of erupting Mt Etna
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Intriguing details about the physical properties and characteristics of a recently discovered asteroid have just been unveiled in amazing images obtained using a large radar dish in California. The radar dish serves as a key component of NASA’s Deep Space Network (DSN). The Near Earth asteroid, dubbed 2010 JL33, was imaged by radar on Dec. 11 and 12, 2010 at NASA’s Goldstone Solar System Radar in California’s Mojave Desert when a close approach to Earth offered an outstanding opportunity for high quality science.
Asteroids studies have taken on significantly increased importance at NASA ever since President Obama decided to cancel the Constellation ‘Return to the Moon’ program and redirect NASA’s next human spaceflight goal to journeying to an Asteroid by around 2025.
Update: Orbital diagram added below
A sequence of 36 amazingly detailed images has been assembled into a short movie (see below) by the science team at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, Calif. The movie shows about 90 percent of one rotation.
The data gathered by radar revealed that the asteroid measures roughly 1.8 kilometers (1.1 miles) in diameter and rotates once every nine hours.
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“Asteroid 2010 JL33 approached within 17 Earth-Moon distances [some 7 million km] in December 2010 and offered an outstanding opportunity to study it with radar,” said Lance Benner, a scientist at JPL who studies asteroids.
“To get detailed radar images, an asteroid must be close to Earth,” Benner told me, for Universe Today.
The object was only discovered on May 6 by the Mount Lemmon Survey in Arizona. The radar observations were led by a team headed by JPL scientist Marina Brozovic.
Video Caption: While safely passing Earth, NASA’s Goldstone Solar System Radar captured the rotation of asteroid 2010 JL33 — an irregular, elongated object roughly 1.8 kilometers (1.1) miles wide. The video consists of 36 frames.
“The radar images we got enabled us to estimate the asteroid’s size, rotation period, and to see features on its surface, most notably, the large concavity that appears as a dark region in the collage,” Benner elaborated.
“It was discovered so recently that little else is known about it.”
The object was revealed to be elongated and irregularly shaped.
The 70-meter (230-foot) diameter antenna is the largest, and therefore most sensitive, DSN antenna, and is capable of tracking a spacecraft travelling more than 16 billion kilometers (10 billion miles) from Earth.
The surface of the 70-meter reflector must remain accurate within a fraction of the signal wavelength, meaning that the precision across the 3,850-square-meter (41,400 sq. ft.) surface is maintained within one centimeter (0.4 in.). Credit: NASA
The large concavity is clearly visible in the images and may be an impact crater. It took about 56 seconds for the radio signals from the 70-meter (230-foot) diameter Goldstone radar dish to make the roundtrip from Earth to the asteroid and back to Earth again.
“When we get deeper into our analysis of the data, we will use the images to estimate the three-dimensional shape of the asteroid as well,” Benner added.
Benner belongs to a team that is part of a long-term NASA program to study asteroid physical properties and to improve asteroid orbits using radar telescopes at Goldstone and also at the Arecibo Observatory in Puerto Rico. The 1,000-foot-diameter (305 meters) Arecibo radar dish antenna is operated by the National Science Foundation.
“Each close approach by an asteroid provides an important opportunity to study it, so we try to exploit as many such opportunities as possible to investigate the physical properties of many asteroids. In the bigger picture, this helps us understand how the asteroids formed,” Benner told me.
“Asteroid 2010 JL33 is in an elongated orbit about the Sun. On average, it’s about 2.7 times farther from the Sun than the Earth is, but its distance from the Sun varies from 0.7 to 4.6 times that of the Earth.” That takes the asteroid nearly out to Jupiter at Aphelion. It takes about 4.3 years to complete one orbit around the sun.
But, there’s no need to fret about disaster scenarios. “The probability of impact with Earth is effectively zero for the foreseeable future,” Benner explained.
“On rare occasions it approaches closely to Vesta,” he said. Vesta is the second most massive asteroid and will be visited for the first time by NASA’s Dawn spacecraft later this year.
In addition to the ground based radar imaging, the tiny space rock was investigated by an Earth orbiting telescope.
“This asteroid was also studied by NASA’s Wide-field Infrared Survey Explorer (WISE) spacecraft,” according to Benner. “Our observations will help WISE scientists calibrate their results because we provided an independent means to estimate the size of this object.”
More at this JPL press release. The NASA-JPL Near-Earth Object Program website has an interactive map that allows you to see the asteroid’s position at any time you desire. Go to here
To see the trajectory of any other near-Earth asteroid, go to here
For more information about asteroid radar research, go to here
Information about the Deep Space Network is here