United Launch Alliance's Delta II rocket has been added to the National Launch Services II contract by NASA. Photo Credit: Alan Walters/awaltersphoto.com
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NASA announced that it has added the Delta II rocket, a launch vehicle that appeared to be slipping into history, to the NASA Launch Services (NLS) II contract. The Delta II, produced by United Launch Alliance, is one of the most successful expendable launch vehicles that has ever been produced.
This modification of the contract will allow ULA to add the Delta II rocket as part of the contract’s on-ramp provision. The modification allows United Launch Services to offer as much as five Delta II rockets.
The Delta II was most recently utilized to launch the GRAIL mission to study the Moon's composition. Photo Credit: Mike Killian/ARES Institute
“We are extremely pleased NASA has added the reliable Delta II to the NLS II contract and look forward to continuing the legacy of the program,” said Michael Gass, ULA’s president and CEO. “ULA has demonstrated its ability to fully integrate Atlas V, Delta IV and Delta II product lines allowing us to continue offering medium launch capability at the best value for our customers.”
The Delta II rocket, in its various configurations has been launched 150 times and has a success rate of 98.7 percent. The one notable failure was the 1997 launch of a U.S. Air Force Global Positioning IIR-1 satellite (GPS IIR-1). Within 13 seconds of launch the Delta II exploded causing severe destruction to the surrounding area. The cause of this mishap was determined to be a crack within one of the GEM-40 solid rocket boosters that are affixed to the base of the Delta II.
The Delta II rocket has a very extensive history of success and has been used to launch many famous missions. Image Credit: NASA/JPL
“While we count success one mission at a time, we have been able to count on the Delta II’s success 96 times in a row over the last decade,” Gass said. “This is a tribute to our dedicated ULA employees, our supplier teammates and our NASA Launch Services Program customer who ensures mission success is the focus of each and every launch.”
The planetary science missions that the rocket has sent into space reads like a “Who’s Who” of space exploration missions. The Mars Exploration Rovers Spirit and Opportunity, Mars Phoenix Lander, Genesis, Stardust, Mars Pathfinder, Mars Global Surveyor, Messenger, Deep Impact, Dawn, Kepler, Wise and the recent GRAIL mission to the Moon – all thundered to orbit atop a Delta II.
The Delta II rocket is launched from either Vandenberg Air Force Base in California or Cape Canaveral Air Force Station located in Florida. Photo Credit: NASA.gov
ULA’s next planned launch of a Delta II will carry the NPOESS Preparatory Project (NPP) mission for NASA. It is currently slated to launch Oct. 25, 2011 from Space Launch Complex-2 at Vandenberg Air Force Base, located in California. ULA launches from both Vandenberg as well as Cape Canaveral Air Force Station, located in Florida.
While this change does allow for at least five more launches of the Delta II, after those launches, the rocket will no longer be utilized and will be phased out of service.
The NLS II contracts are designed to provide for payloads weighing about 550 pounds or more to be sent to a minimum 124-mile-high circular orbit. The launch service providers signed into these contracts also may offer different launch vehicles to NASA to meet other requirements. NASA can also provide launch services to other agencies, such as the National Oceanic and Atmospheric Administration or NOAA.
Spirit and Opportunity, Pathfinder, Deep Impact, Dawn, Kepler, Stardust, Genesis and Wise - were all launched on the Delta II rocket. Photo Credit: NASA/George Shelton
NASA has stated that it cannot provide one of the Atlas rockets required to launch the ExoMars mission that it has partnered with ESA on. Image Credit: ESA
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The European Space Agency’s “ExoMars” mission is under threat of cancellation. NASA and ESA heads will meet on Monday, Oct. 3 to decide how much more can be cut from the rapidly slimming mission. This meeting comes on the heels of NASA’s latest round of cuts – which means that the U.S. space agency cannot provide ESA with the Atlas V rocket that was slated to launch part of the mission.
ESA still might be able to keep ExoMars going if it can acquire a Proton rocket under the trade system that the agency is working to negotiate with Russia. Barring that? ExoMars will more-than-likely be cancelled. ESA had been hoping to send a diverse science package to the red planet. ExoMars is currently comprised of a communications relay system, descent and landing modules and a rover that is similar in design to the Mars Exploration Rovers Spirit and Opportunity which have been operating on Mars for the past seven years.
The ExoMars Trace Gas Orbiter was originally set to launch in 2016, now its future is uncertain. Image Credit: ESA
NASA Administrator Charles Bolden and ESA Director-General Jean-Jacques Dordain are scheduled to meet in Cape Town, South Africa, during the International Astronautical Congress. During this meeting they are set to discuss one of two options that are left for their joint Mars expedition. The first is a single 2018 launch that will include a NASA-ESA rover and communications package. The second will be to try and maintain, despite the issues with the launch vehicle, the planned 2016 launch.
If a rocket can somehow be procured and the current schedule maintained, ExoMars would be a two launch affair with the Atlas V launching one of the mission’s components and another launch vehicle transporting the remainder. If the mission is saved, but scaled back further, only a single launch would take place in 2018. The Proton rocket scenario appears to be a last-ditch effort to salvage the program at this time. The final deciding factor as to whether-or-not ESA can save the program, to some degree, in its current configuration – depends on ESA obtaining a rocket to replace the Atlas V which NASA says it can no longer provide.
NASA had originally stated that it would provide two Atlas V rockets for the mission, the space agency has taken at least one of these off off the table recently. Photo Credit: ULA
ESA has estimated that either way, the mission will cost them the same 850 million euros ($1.36 billion) that it has already garnered from the nations that comprise the European Union. This is largely due to the fact that ESA has already spent the money to procure the materials and services needed for the orbiter component of the mission.
The primary issue that has continued to threaten mission is the poor state of the economy – both in the U.S. and Europe.
ExoMars started out as a rover and a separate ground station, and was originally set to launch in 2011 on a Soyuz Fregat rocket. In 2009 ESA signed into the Mars Joint Exploration Initiative with NASA. This agreement with NASA both pushed back the launch of the mission considerably and started ExoMars down the path to where it currently finds itself. ExoMars has been changed repeatedly since its inception and now it is facing possible cancellation. Image Credits: ESA
Dr. Ed Weiler retired on Sept 30, 2011 as the NASA Associate Administrator for the Science Mission Directorate at NASA HQ, Washington, DC after 33 distinguished years at NASA, including 10 years as Chief of all NASA Space Science and nearly 20 years as Chief Scientist for the Hubble Space Telescope. In this photo, Weiler ‘Hugs Hubble' after launch of STS-125 on the final shuttle mission to repair and upgrade the Hubble Space Telescope in May 2009. A happy and relieved Weiler chats post-launch inside the KSC Press Center about Hubble and NASA Space Science. Credit: Ken Kremer
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Ed Weiler, NASA’s Science leader in charge of the robotic missions that continually produce scientific breakthroughs that amaze all humanity and longtime Chief Scientist on the Hubble Space Telescope that has completely revolutionized our understanding of humanities place in the Universe, retired today (Sept. 30) from NASA after a distinguished career spanning almost 33 years.
Weiler is departing NASA during what has been dubbed the “Year of Space Science”- the best year ever for NASA Space Science research. The two most recent successes are the launch of JUNO to Jupiter and the twin GRAIL probes to the Moon. Blastoff of the Curiosity Mars Science Laboratory rover is slated for late November 2011.
Weiler’s official title is associate administrator of NASA’s Science Mission Directorate (SMD) at agency Headquarters in Washington, DC. In that capacity he was responsible for overseeing NASA’s science and research programs in Earth science, heliophysics, planetary science and astrophysics.
Weiler was appointed to lead SMD in 2008. He holds this position now for the second time after serving in between as Director of NASA Goddard Spaceflight Center in Greenbelt, Maryland from 2004 to 2008. His earlier stint as associate administrator lasted from 1998 to 2004 for what was then called the Space Science Enterprise.
Dr. Ed Weiler, NASA Associate Administrator for the Science Mission Directorate. Credit: NASA/Bill Ingalls
Probably the job he loved best was as Chief Scientist of the Hubble Space Telescope from 1979 to 1998, until he was promoted to the top rung of NASA management.
I was very lucky to meet and chat with Ed Weiler while I was covering the final space shuttle flight – STS-125 – to repair and upgrade Hubble. STS 125 blasted off in May 2009 and accomplished every single objective to catapult Hubble to the apex of its capabilities.
At the recent launch of the twin GRAIL lunar mapping probes, I spoke with Weiler about a wide range of NASA missions. Watch for my upcoming interview with Ed.
Weiler is very hopeful that Hubble will continue to operate for several more years at least.
NASA issued this statement from NASA Administrator Charles Bolden, “Ed leaves an enduring legacy of pride and success that forever will remain a part of NASA’s science history. His leadership helped inspire the public with each new scientific discovery, and enabled NASA to move forward with new capabilities to continue to explore our solar system and beyond.”
The successes under Weiler’s leadership include NASA’s great observatory missions, unprecedented advances in Earth science and extensive exploration of Mars and other planets in our solar system. These advances have rewritten science textbooks and earned enormous support for NASA’s science programs from the general public.
The Mars rovers Spirit and Opportunity are just one example of the science missions approved and funded during Weiler’s tenure.
Weiler’s leadership has been instrumental in securing continued support and funding for NASA Space Science from Congress and the White House. He has received numerous prestigious awards including the NASA Distinguished Service Medal and several Presidential Rank Awards for Meritorious Executive and Distinguished Executive.
Ed Weiler remembers Spirit at JPL symposium. Credit: AP
Planet Mercury as seen from the MESSENGER spacecraft in 2008. Credit: NASA/JPL
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According to data from the The Fast Imaging Plasma Spectrometer (FIPS) onboard NASA’s MESSENGER spacecraft, the solar wind is “sandblasting” the surface of Mercury at its polar regions.
Based on findings from one of seven different papers from the MESSENGER mission to be published in the Sept. 30th edition of Science, sodium and oxygen particles are charged in a manner similar to Earth’s own Aurora Borealis.
How are the University of Michigan researchers able to detect and study this phenomenon?
Using the FISP, the scientists at the University of Michigan have taken measurements of Mercury’s exosphere and magnetosphere. The data collected has provided researchers with a better understanding of interactions between Mercury and our Sun. FIPS data has also confirmed theories regarding the composition and source of particles in Mercury’s space environment.
“We had previously observed neutral sodium from ground observations, but up close we’ve discovered that charged sodium particles are concentrated near Mercury’s polar regions where they are likely liberated by solar wind ion sputtering, effectively knocking sodium atoms off Mercury’s surface,” said FIPS project leader Thomas Zurbuchen (University of Michigan).
In a UM press release, Zurbuchen added, “We were able to observe the formation process of these ions, and it’s comparable to the manner by which auroras are generated in Earth’s atmosphere near polar regions.”
Given that Earth and Mercury are the only two magnetized planets in the inner solar system (Mars is believed to have had a magnetic field in its past), the solar wind is deflected around them. The solar wind has made recent news due to recent outbursts from the Sun causing visible aurorae, caused by the interaction of charged particles from the Sun and Earth’s relatively strong magnetosphere. While Mercury does have a magnetosphere, compared to Earth’s it is relatively weak. Given Mercury’s weak magnetosphere and close proximity to the Sun, the effects of the solar wind have a more profound effect.
The Fast Imaging Plasma Spectrometer on board MESSENGER has found that the solar wind is able to bear down on Mercury enough to blast particles from its surface into its wispy atmosphere. Image Credit: Shannon Kohlitz, Media Academica, LLC
“Our results tell us is that Mercury’s weak magnetosphere provides very little protection of the planet from the solar wind,” Zurbuchen said.
Jim Raines, FIPS operations engineer (University of Michigan) added, “We’re trying to understand how the sun, the grand-daddy of all that is life, interacts with the planets. It is Earth’s magnetosphere that keeps our atmosphere from being stripped away. And that makes it vital to the existence of life on our planet.”
A high-resolution monochrome image has been combined with a lower-resolution enhanced-color image. The hollows appear in cyan, a result of their high reflectance and bluish color relative to other parts of the planet. The large pit in the center of the crater may be a volcanic vent, from which the orange material erupted. Credit: Courtesy of Science/AAAS
The MESSENGER team also released other results from the mission, including new evidence that flood volcanism has been widespread on Mercury, the first close-up views of Mercury’s “hollows,” and the first direct measurements of the chemical composition of Mercury’s surface.
MESSENGER, as well the the Mariner 10 flyby mission saw unusual features on the floors and central mountain peaks of some impact craters which were very bright and have a blue color relative to other areas of Mercury. This type of feature is not seen on the Moon, and were nicknamed “hollows.”
Now, with the latest MESSENGER data, hollows have been found over a wide range of latitudes and longitudes, suggesting that they are fairly common across Mercury. Many of the depressions have bright interiors and halos.
“To the surprise of the science team, it turns out that the bright areas are composed of small, shallow, irregularly shaped depressions that are often found in clusters,” says David Blewett, a staff scientist at the Johns Hopkins University Applied Physics Laboratory (APL) in Laurel, Md., and lead author of one of the Science reports. “The science team adopted the term ‘hollows’ for these features to distinguish them from other types of pits seen on Mercury.”
Blewett added the hollows detected so far have a fresh appearance and have not accumulated small impact craters, indicating that they are relatively young.
NASA announces student Essay Naming Contest for the twin GRAIL Lunar spaceships. The essay writing contest is open to students in Grades K - 12 at schools in the United States. Submission Deadline is November 11, 2011. GRAIL A & B are twin science robots that will explore the gravity field of the moon like never before.
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Student Alert ! – Here’s your once in a lifetime chance to name Two NASA robots speeding at this moment to the Moon on a super science mission to map the lunar gravity field. They were successfully launched from the Earth to the Moon on September 10, 2011. Right now the robots are called GRAIL A and GRAIL B. But, they need real names that inspire. And they need those names real soon. The goal is to “capture the spirit and excitement of lunar exploration”, says NASA – the US Space Agency.
NASA needs your help and has just announced an essay writing contest open to students in Grades K – 12 at schools in the United States. The deadline to submit your essay is November 11, 2011. GRAIL stands for “Gravity Recovery And Interior Laboratory.”
The rules state you need to pick two names and explain your choices in 500 words or less in English. Your essay can be any length up to 500 words – even as short as a paragraph. But, DO NOT write more than 500 words or your entry will be automatically disqualified.
Learn more about the GRAIL Essay Naming Contest here:
Students: NASA Wants You to Name that GRAIL !
Write an Essay and name these twin Lunar mapping satellites. NASA’s twin GRAIL A & B science probes are now streaking to the Moon and arrive on New Year’s Day 2012. This picture shows how they looked, mounted side by side, during launch preparations prior to blasting off for the Moon on Sept. 10, 2011 from Florida. Credit: Ken Kremer
The GRAIL A and B lunar spaceships are twins – just like those other awe inspiring robots “Spirit” and “Opportunity” , which were named by a 10 year old girl student and quickly became famous worldwide and forever because of their exciting science missions of Exploration and Discovery.They arrive in Lunar Orbit on New Year’s Day 2012.
Blastoff of twin GRAIL A and B lunar gravity mapping spacecraft on a Delta II Heavy rocket on Sept. 10 from Pad 17B Cape Canaveral Air Force Station in Florida at 9:08 a.m. EDT. Credit: Ken Kremer
And there is another way that students can get involved in NASA’s GRAIL mission.
GRAIL A & B are both equipped with four student-run MoonKAM cameras. Students can suggest targets for the cameras. Then the cameras will take close-up views of the lunar surface, taking tens of thousands of images and sending them back to Earth.
“Over 1100 middle schools have signed up to participate in the MoonKAM education and public outreach program to take images and engage in exploration,” said Prof. Maria Zuber of MIT.
Prof. Zuber is the top scientist on the mission and she was very excited to announce the GRAIL Essay Naming contest right after the twin spaceships blasted off to the Moon on Sep 10, 2011 from Cape Canaveral in Florida.
What is the purpose of GRAIL ?
“GRAIL simply put, is a ‘Journey to the Center of the Moon’,” says Dr. Ed Weiler, NASA Associate Administrator of the Science Mission Directorate in Washington, DC.
“It will probe the interior of the moon and map its gravity field by 100 to 1000 times better than ever before. We will learn more about the interior of the moon with GRAIL than all previous lunar missions combined. Precisely knowing what the gravity fields are will be critical in helping to land future human and robotic spacecraft. The moon is not very uniform. So it’s a dicey thing to fly orbits around the moon.”
“There have been many missions that have gone to the moon, orbited the moon, landed on the moon, brought back samples of the moon,” said Zuber. “But the missing piece of the puzzle in trying to understand the moon is what the deep interior is like.”
So, what are you waiting for.
Start thinking and writing. Students – You can be space explorers too !
Opportunity captured at Endeavour Crater rim on Sept 10, 2011, Sol 2712. Opportunity is visible at the end of the white arrow, sitting atop some light toned outcrops on the rim of Endeavour Crater located at the southern tip of a rim segment named Cape York. Opportunity is ascending Endeavour at Cape York ridge and positioned to the right of the small crater named Odyssey. This image was taken by the HiRISE camera aboard NASA’s Mars Reconnaissance Orbiter (MRO), Opportunity travelled nearly three years to reach this rim because it contains rocks even more ancient than the rocks of Meridiani Planum, which the rover has been exploring since 2004, and hence may teach us something about an even more ancient era in Martian history. Click to enlarge. Credit: NASA/JPL/University of Arizona
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Opportunity has just been imaged in high resolution at Endeavour crater by a powerful NASA camera orbiting overhead in Mars orbit. The new image (see above) was snapped while NASA’s long lived robot was climbing a hilltop offering spectacular panoramic vistas peering into the vast crater which is some 14 miles (22 km) wide.
The HiRiSE camera aboard NASA’s Mars Reconnaissance Orbiter photographed Opportunity and her wheel tracks on September 10, 2011, or Martian Sol 2712 for a mission warrentied to last only 90 Sols ! The rover is sitting to the right of another small crater known as Odyssey. Click to enlarge the image.
Look very closely and you’ll even be able to easily discern the rovers pair of tire tracks showing the path traversed by the robot as she explores the crater and the ejecta rocks and boulders excavated and strewn about by an ancient impact.
Opportunity imaged at Endeavour crater rim with wheel tracks exploring Odyssey crater, rocks and boulders climbing up Cape York ridge. Credit: NASA/JPL/University of Arizona
Opportunity is ascending up the rim of Endeavour crater at the southern tip of a low ridge dubbed Cape York – a location that has already yielded a bonanza of new science data since her recent arrival in August 2011 after a more than 20 mile (33 km) epic trek.
The intrepid rover discovered a rock unlike any other since she safely landed at the Meridiani Planum region of Mars nearly eight years ago on Jan. 24, 2004.
Opportunity is now searching Endeavour crater and Cape York for signatures of phyllosilicates – clay minerals that formed in the presence of pH neutral water flowing on Mars surface billions of years ago. Cape York ridge at Endeavour Crater - From Orbit
This image taken from Mars orbit shows the path driven by NASA's Mars Exploration Rover Opportunity in the weeks around the rover's arrival at the rim of Endeavour crater and up to Sol 2688. Opportunity has since driven a short distance to the right. Credit: NASA/JPL-Caltech/University of Arizona
Endeavour Crater Panorama from Opportunity, Sol 2681, August 2011
Opportunity arrived at the rim of Endeavour on Sol 2681, August 9, 2011 and climbed up the ridge known as Cape York. Odyssey crater is visible at left. Opportunity has since driven a short distance beyond Odyssey crater and was photographed from Mars orbit on Sept. 10, 2011.
Mosaic Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Kenneth Kremer
3 D Anaglyph of Craters at Rheasilvia - the South Polar Region of Vesta. This 3-D image shows the topography, craters and grooves of Vesta’s south polar region obtained by the framing camera instrument aboard NASA’s Dawn spacecraft on Aug. 23 and 28, 2011. The image has a resolution of about 260 meters per pixel.
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Try not to plummet off a steep crater cliff or be buried under a landslide while gazing at the irresistibly alluring curves of beautiful Rheasilvia – the mythical mother of Romulus and Remus – whose found a new home at the South Pole of the giant Asteroid Vesta.
3 D is undoubtedly the best way to maximize your pleasure. So whip out your cool red-cyan anaglyph glasses to enhance your viewing experience of Rheasilvia, the Snowman and more – and maximize your enjoyment of this new 3 D collection showcasing the heavily cratered, pockmarked, mountainous and groovy terrain replete at Vesta.
3D Details of Wave-Like Terrain in the South Pole of Vesta
This image was obtained by NASA’s Dawn spacecraft from an orbit of about 1,700 miles (2,700 kilometers) above the surface of the giant asteroid Vesta. Topography in the area surrounding Vesta's south pole area shows impact craters, ridges and grooves. These images in 3D provide scientists with a realistic impression of the solid surface of the celestial body.
Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
Can you find the location of the 3 D image above in the 2 D South Pole image below?
Scientists and mortals have been fascinated by the enormous impact crater Rheasilvia and central mountain unveiled in detail by NASA’s Dawn Asteroid Orbiter recently arrived at Vesta, the 2nd most massive object in the main asteroid belt. Ceres is the largest object and will be Dawn’s next orbital target in 2015 after departing Vesta in 2012.
3D - A Big Mountain at Asteroid Vesta’s South Pole
Scientists were fascinated by this enormous mound inside a big circular depression at the south pole- dubbed Rheasilvia. This stereo image was recorded from an altitude of about 1,700 miles (2,700 kilometers) above the surface and shows the structure of the mountain, displayed in the right half of this 3D image. The base of the mountain has a diameter of about 125 miles (200 kilometers), and its altitude above the surroundings is about 9 miles (15 kilometers). The vicinity of the peak of the mountain shows landslides that occurred when material from the flanks of the mountain were slipping down. Also visible are tectonic structures from tension in Vesta's crust. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
“Vesta is the smallest terrestrial planet in our Solar System”, said Chris Russell in an interview with Universe Today. “We do not have a good analog to Vesta anywhere else in the Solar System.”
And the best is yet to come. In a few days, Dawn begins snapping images from a much lower altitude at the HAMO mapping orbit of ca. 685 km vs the initial survey orbit of ca, 2700 km. where most of these images were taken.
Can you find the location of the 3 D South Pole images above in the 2 D South Pole image below?
Topography of Densely Cratered Deformed Terrain
This 3 D anaglyph image shows the topography of Vesta's densely cratered terrain obtained by the framing camera instrument aboard NASA's Dawn spacecraft on August 6, 2011. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDAAnaglyph of the ‘Snowman' Crater. This anaglyph image shows the topography of Vesta's three craters, informally named the "Snowman," obtained by the framing camera instrument aboard Dawn on August 6, 2011. The camera has a resolution of about 260 meters per pixel. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDAVesta's Ancient, Cratered Surface in 3D
This image of the giant asteroid Vesta obtained by NASA's Dawn spacecraft shows the surface of the asteroid from an orbit of about 1,700 miles (2,700 kilometers) above the surface. Numerous impact craters illustrate the asteroid's violent youth. By counting craters on distinct geological surfaces scientists can deduce relative ages of the asteroid's surface. This 3D view provides scientists the opportunity to learn more about the morphology of craters on asteroids and physical properties of the material at Vesta's surface.. Image resolution is about 260 meters per pixel. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDAViewing the South Pole of Vesta and Rheasilvia Impact Basin
This image obtained by Dawns framing camera shows the south pole of the giant asteroid Vesta. Scientists are discussing whether the Rheasilvia circular structure that covers most of this image originated by a collision with another asteroid, or by internal processes early in the asteroid's history. Images in higher resolution from Dawn's next lowered orbit might help answer that question. The image was recorded from a distance of about 1,700 miles (2,700 kilometers). The image resolution is about 260 meters per pixel. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDARhea Silvia, torso from the amphitheatre at Cartagena in Spain that was rediscovered in 1988. Rhea Silvia was the mother of Romulus and Remus, the mythical founders of Rome. Source: Wikipedia
Read Ken’s continuing features about Dawn and Vesta
A False-Color Topography of Vesta's South Pole. This false-color map of the giant asteroid Vesta was created from stereo images obtained by the framing camera aboard NASA’s Dawn spacecraft. The image shows the elevation of surface structures with a horizontal resolution of about 750 meters per pixel. The terrain model of Vesta's southern hemisphere shows a big circular structure with a diameter of about 300 miles (500 kilometers), its rim rising above the interior of the structure for more than 9 miles (15 kilometers.) Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
Video caption: Rheasilvia Impact Basin and Vesta shape model. This false-color shape model video of the giant asteroid Vesta was created from images taken by the framing camera aboard NASA’s Dawn spacecraft. Rheasilvia – South Pole Impact Basin – shown at bottom (left) and head on (at right). Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
‘Rheasilvia’ – that’s the brand new name given to the humongous and ever more mysterious South Pole basin feature being scrutinized in detail by Dawn, according to the missions top scientists in a Universe Today exclusive. Dawn is NASA’s newly arrived science orbiter unveiling the giant asteroid Vesta – a marvelously intriguing body unlike any other in our Solar System.
What is Rheasilvia? An impact basin? A crater remnant? Tectonic action? A leftover from internal processes? Or something completely different? That’s the hotly debated central question consuming loads of attention and sparking significant speculation amongst Dawn’s happily puzzled international science team. There is nothing closely analogous to Vesta and Rhea Silvia – and thats a planetary scientists dream come true.
“Rheasilvia – One thing that we all agree on is that the large crater should be named ‘Rheasilvia’ after the mother of Romulus and Remus, the mythical mother of the Vestals,” said Prof. Chris Russell, Dawns lead scientist, in an exclusive interview with Universe Today. Russell, from UCLA, is the scientific Principal Investigator for Dawn.
“Since we have never seen any crater just like this one it is difficult for us to decide exactly what did happen,” Russell told me. “The name ‘Rheasilvia’ has been approved by the IAU and the science team is using it.”
Craters on Vesta are being named after the Vestal Virgins—the priestesses of the Roman goddess Vesta. Other features will be named for festivals and towns of that era. Romulus and Remus were the mythical founders of Rome.
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‘Rheasilvia’ has the science team in a quandary, rather puzzled and reevaluating and debating long held theories as they collect reams of new data from Dawn’s three science instruments – provided by the US, Germany and Italy. That’s the scientific method in progress and it will take time to reach a consensus.
Prior to Dawn’s orbital insertion in July 2011, the best views of Vesta were captured by the Hubble Space Telescope and clearly showed it wasn’t round. Scientists interpreted the data as showing that Vesta’s southern hemisphere lacked a South Pole! And, that it had been blasted away eons ago by a gargantuan cosmic collision that excavated huge amounts of material that nearly utterly destroyed the asteroid.
The ancient collision left behind a colossal 300 mile (500 km) diameter and circular gaping hole in the southern hemisphere – nearly as wide as the entire asteroid (530 km) and leaving behind an as yet unexplained and enormous central mountain peak, measuring some 9 miles (15 km) high and over 125 miles (200 km) in diameter. The mountain has one of the highest elevations in the entire solar system.
“We are trying to understand the high scarps that we see and the scarps that should be there and aren’t,” Russell explained. “We are trying to understand the landslides we think we see and why the land slid. We see grooves in the floor of the basin and want to interpret them.
“And the hill in the center of the crater remains as mysterious today as when we first arrived.”
Viewing the South Pole of Vesta and Rheasilvia Impact Basin
This image obtained by Dawns framing camera and shows the south pole of the giant asteroid Vesta. Scientists are discussing whether the Rheasilvia circular structure that covers most of this image originated by a collision with another asteroid, or by internal processes early in the asteroid's history. Images in higher resolution from Dawn's lowered orbit might help answer that question. The image was recorded from a distance of about 1,700 miles (2,700 kilometers). The image resolution is about 260 meters per pixel. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
Another top Dawn scientist described Rheasilvia in this way:
“I would say that the floor of the impact feature contains chaotic terrain with multiple sets of intersecting grooves, sometimes fairly straight and often curvy, said Carol Raymond to Universe Today. Raymond is Dawn’s Deputy Principal Investigator from NASA’s Jet Propulsion Laboratory in Pasadena, Calif.
“The crater rim is not well-expressed”, Raymond told me. “We see strong color variations across Vesta, and the south pole impact basin appears to have a distinct spectral signature.
“The analysis is still ongoing,” Russell said.
“The south is distinctly different than the north. The north has a varied spectrum and the south has a distinct spectral feature but it has little variation.” Time will tell as additional high resolution measurements are collected from the forthcoming science campaign at lower orbits.
Russell further informed that the team is rushing to pull all the currently available data together in time for a science conference and public briefing in mid-October.
“We have set ourselves a target to gather everything we know about the south pole impact feature and expect to have a press release from what ever we conclude at the GSA (Geological Society of America) meeting on October 12. “We will tell the public what the options are.”
“We do not have a good analog to Vesta anywhere else in the Solar System and we’ll be studying it very intently.”
Impressive South Pole MountainTop at Rheasilvia Crater on Vesta
This mountain, which measures about 125 miles (200 kilometers) in diameter at its base, is one of the highest elevations on all known bodies with solid surfaces in the solar system. The image has been recorded with the framing camera aboard NASA's Dawn spacecraft from a distance of about 1,700 miles (2,700 kilometers). The image resolution is about 260 meters per pixel. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
Right now Dawn is using its ion propulsion system to spiral down four times closer to Vesta, as it descends from the initlal survey orbit(about 2700 km, 1700 mi) to the new science orbit, elegantly named HAMO – or High Altitude Mapping Orbit (about 685 km.)
“Our current plan is to begin HAMO on Sept. 29, but we will not finalize that plan until next week,” Dr. Marc Rayman told Universe Today. Rayman, of NASA’s JPL, is Dawn’s Chief Engineer.
“Dawn’s mean altitude today (Sept. 20) is around 680 km (420 miles),” said Rayman .
“Dawn successfully completed the majority of the planned ion thrusting needed to reach its new science orbit and navigators are now measuring its orbital parameters precisely so they can design a final maneuver to ensure the spacecraft is in just the orbit needed to begin its intensive mapping observations next week.”
Watch for lots more stories upcoming on Vesta and the Dawn mission
Infrared image of Neptune from Keck Observatory in Hawaii. Credit: Mike Brown/CalTech
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The confessed (and remorseless) “Pluto Killer” Mike Brown has turned his gaze – and the 10-meter telescope at the Keck Observatory in Hawaii – on Neptune, our solar system’s furthest “official” planet. But no worries for Neptune – Mike isn’t after its planetary status… he’s taken some beautiful infrared images instead!
Normally only visible as a featureless blue speck in telescopes, Brown’s image of Neptune — along with its largest moon Triton — shows the icy gas giant in infrared light, glowing bright red and orange.
Neptune and Triton in infrared. Credit: Mike Brown/CalTech.
Brown’s initial intention was not just to get some pretty pictures of planets. The target of the imaging mission was Triton and to learn more about the placement of its methane, nitrogen and seasonal frosts, and this sort of research required infrared imaging. Of course, Neptune turned out to be quite photogenic itself.
“The big difference is doing the imaging in the infrared where methane absorbs most of the photons,” said Brown. “So the bright places are high clouds where the sunlight reflects off of them before it had a chance to pass through much of the atmosphere. Dark is clear atmosphere full of methane absorption.
“I just thought it was so spectacular that I should post it.”
No argument here, Mike!
Neptune, now officially the outermost planet in our solar system, is the fourth largest planet and boasts the highest wind speeds yet discovered — 1,250 mph winds scream around its frigid skies! Like the other gas giants Neptune has a system of rings, although nowhere near as extravagant as Saturn’s. It has 13 known moons, of which Triton is the largest.
With its retrograde orbit, Triton is believed to be a captured Kuiper Belt Object now in orbit around Neptune. Kuiper Belt Objects are Mike Brown’s specialty, as he is the astronomer most well-known for beginning the whole process that got Pluto demoted from the official planet list back in 2006.
Jason Major is a graphic designer, photo enthusiast and space blogger. Visit his website Lights in the Dark and follow him on Twitter @JPMajor or on Facebook for the most up-to-date astronomy awesomeness!
The Shuttle Enterprise. In 1976, NASA's space shuttle Enterprise rolled out of the Palmdale manufacturing facilities and was greeted by NASA officials and cast members from the 'Star Trek' television series. From left to right they are: NASA Administrator Dr. James D. Fletcher; DeForest Kelley, who portrayed Dr. "Bones" McCoy on the series; George Takei (Mr. Sulu); James Doohan (Chief Engineer Montgomery "Scotty" Scott); Nichelle Nichols (Lt. Uhura); Leonard Nimoy (Mr. Spock); series creator Gene Rodenberry; an unnamed NASA official; and, Walter Koenig (Ensign Pavel Chekov). Credit: NASA
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‘Enterprise’, the first of NASA’s Space Shuttle orbiters to be assembled, was unveiled 35 Years ago on Sept. 17, 1976 to the soaring theme song and fanfare of the immortal science fiction television series – ‘Star Trek’. Members of the original cast (photo above) were on hand for the celebratory rollout at the Rockwell International manufacturing plant in Palmdale, California.
Today, the Enterprise is housed as the centerpiece at the Smithsonian’s National Air & Space Museum (NASM) Udvar-Hazy Annex in Chantilly, Virginia.
Check out these webcams for live views of shuttle Enterprise at NASM from the front and aft.
Space Shuttle Enterprise on display at the Smithsonian’s National Air & Space Museum Udvar-Hazy Annex in Chantilly, Virginia
NASA originally selected ‘Constitution’ as the orbiter’s name – in honor of the U.S. Constitution’s Bicentennial . That was until avid fans of ‘Star Trek’ mounted a successful letter writing campaign urging the White House to select the name ‘Enterprise’ – in honor of the popular TV shows starship of exploration. The rest is history.
Many scientists and space enthusiasts found inspiration from Star Trek and were motivated to become professional researchers by the groundbreaking science fiction show.
Space Shuttle Enterprise on display as the centerpiece at the Smithsonian’s National Air & Space Museum Udvar-Hazy Annex in Chantilly, Virginia. Credit: NASA
Enterprise was a prototype orbiter, designated as OV-101, and not built for spaceflight because it lacked the three space shuttle main engines necessary for launch and the thermal protection systems required for reentry into the Earth’s atmosphere.
Enterprise did however play a very key role in preparing NASA’s other shuttles for eventual spaceflight. The orbiter was tested in free flight when it was released from a Boeing 747 Shuttle Carrier Aircraft for a series of five critical approach and landing tests in 1977.I was fortunate to see Enterprise back in 1977 on top of a 747 during a cross country stop near the Johnson Space Center.
Enterprise in free flight during approach and landing test in 1977
In 1979 Enterprise was mated to an External Tank and a pair of Solid Rocket Boosters for several weeks of fit checks and procedural test practice in launch configuration at Launch Complex 39 at NASA’s Kennedy Space Center in Florida.
These efforts helped pave the way for the first ever flight of a space shuttle by her sister orbiter ‘Columbia’ on the STS-1 mission by John Young and Bob Crippen. Columbia blasted off on April 12, 1981 on a gutsy 54 hour test flight.
Enterprise in free flight during approach and landing test in 1977
In 1984, the Enterprise was ferried to Vandenberg Air Force Base for similar pad configuration checks at Space Launch Complex- 6 (SLC-6) for what was then planned to be the shuttle’s west coast launch site. All California launches were cancelled following the destruction of Space Shuttle Challanger in Jan 1986.
After three decades of flight, the Space Shuttle Era came to a historic end with the majestic predawn touchdown of Space Shuttle Atlantis on Jul 21, 2011. The STS-135 mission was the Grand Finale of NASA’s three decade long Shuttle program.
Following the retirement of all three remaining shuttle orbiters, Enterprise will soon be moved to her new permanent home at the Intrepid Air, Sea and Space Museum in New York City to make way for NASA’s new gift of Space Shuttle Discovery.
First Appearance of Enterprise
Space shuttle Enterprise made its first appearance mated to supportive propellant containers/boosters cluster, as it was rolled from the Vehicle Assembly Building at Kennedy Space Center en route to the launch pad, some 3.5 miles away, on May 1, 1979. Enterprise underwent several weeks of fit and function checks on the pad in preparation for STS-1, on which its sister craft Columbia took astronauts John Young and Robert Crippen into space for a 54-hour test mission. Credit: NASA First Appearance of EnterpriseSpace Shuttle Enterprise at Space Launch Complex 6 (SLC-6 ) at Vandenberg Air Force Base, on February 1, 1985. Credit: Tech. Sgt. Bill Thompson/USAF
Read Ken’s continuing features here about Discovery, Endeavour and Atlantis
Send Ken your pictures of Enterprise to publish at Universe Today.
