Five moon pictures based on data gathered by the Lunar Reconnaissance Orbiter. Credit: NASA
If you’re a fan of moon observation, it’s lucky for you that spacecraft such as the Lunar Reconnaissance Orbiter exist. For about the past five years, the NASA spacecraft has been in orbit around a closest large neighbor, taking images of the surface in high-definition.
To celebrate LRO’s fifth anniversary, NASA is asking members of the public to vote on which of those images (above) is their favorite. This isn’t so much a statement about the scientific data it has collected, NASA said, but more appreciating the images as art.
Voting runs from May 23 to June 6, and the winner will be announced with the full collection’s release on June 18 — the actual official fifth anniversary of the launch. You can find more information about the vote at this page.
By the way, LRO not only takes good pictures of the moon, but also of other spacecraft. You can check out its pictures of LADEE and Chang’e-3 in these past Universe Today articles.
Meanwhile, James Garvin — NASA’s chief scientist of the sciences and exploration directorate — eloquently weighs in below on his favorite images of the moon. His description of Aristarchus is interesting: “Here is Mother Nature’s expression of a gigantic landform made by a cosmic collision.” You can check out the other four below.
Images of Earth assembled from over 36,000 fan-submitted "selfless" on Earth Day, April 22, 2014 (NASA)
On Earth Day, April 22, NASA invited people around the world to share their “selfies” on social media sites like Twitter, Facebook, Google+, and Instagram, showing where on Earth they are and marking them with the hashtag #GlobalSelfie. Well, here we are a month later and the results have just been released… proof of what a beautiful world we all make up!
The image above was built using 36,422 fan-submitted self-portraits from 113 countries, and is based upon images of Earth acquired on April 22 by NASA/NOAA’s Visible Infrared Imaging Radiometer Suite instrument aboard the Suomi National Polar-orbiting Partnership (NPP) satellite. (See the original NPP images here.)
How cool is that? A picture of Earth, as seen from space, recomposed of pictures of people on Earth taken the very same day!
Did you send in a #GlobalSelfie? I’m in there somewhere too, but I haven’t located myself (yet). They’re organized by hue and tone, not location, so I could be representing a spot in the middle of the Peruvian jungle instead of along the Providence River.
The GlobalSelfie campaign was more than just a PR gimmick. 2014 is a big year for NASA Earth observation, with five missions launched to monitor our planet’s wind, oceans, soil, and atmosphere. GlobalSelfie was used to kick off the Earth Right Now campaign, helping to raise awareness about these missions and the data they’ll gather to ultimately benefit people around the world.
Scale model of the Sierra Nevada Corporation’s (SNC) Dream Chaser is readied for wind tunnel testing at high speeds that simulate the conditions it will encounter during its flight through the atmosphere returning from space. Credit: NASA/David C. Bowen
The private Dream Chaser mini-shuttle being developed by Sierra Nevada Corp. (SNC) has successfully completed a series of rigorous wind tunnel tests on scale models of the spacecraft – thereby accomplishing another key development milestone under NASA’s Commercial Crew Program to restore America’s human spaceflight access to low Earth orbit.
Engineers from SNC and NASA’s Langley Research Center in Hampton, Virginia conducted six weeks of intricate testing with several different Dream Chaser scale model spacecraft to study its reaction to subsonic, transonic and supersonic conditions that will be encountered during ascent into space and re-entry from low-Earth orbit.
The tests are among the milestones SNC must complete to receive continued funding from the Commercial Crew Integrated Capability initiative (CCiCAP) under the auspices of NASA’s Commercial Crew Program.
The Dream Chaser is among a trio of US private sector manned spaceships being developed with seed money from NASA’s Commercial Crew Program in a public/private partnership to develop a next-generation crew transportation vehicle to ferry astronauts to and from the International Space Station (ISS) by 2017 – a capability totally lost following the space shuttle’s forced retirement in 2011.
Since that day, seats on the Russian Soyuz are US astronauts only way to space and back.
The SpaceXDragon and BoeingCST-100 ‘space taxis’ are also vying for funding in the next round of contracts to be awarded by NASA around late summer 2014.
Dream Chaser commercial crew vehicle built by Sierra Nevada Corp docks at ISS
“What we have seen from our industry partners is a determination to make their components and systems work reliably, and in turn they’ve been able to demonstrate the complex machinery that makes spaceflight possible will also work as planned,” said Kathy Lueders, NASA’s Commercial Crew Program manager. “These next few months will continue to raise the bar for achievement by our partners.”
To prepare for the wind tunnel testing, technicians first meticulously hand glued 250 tiny sand grains to the outer surface of the 22-inch long Dream Chaser scale model in order to investigate turbulent flow forces and flight dynamic characteristics along the vehicle that simulates what the actual spacecraft will experience during ascent and re-entry.
Dream Chaser awaits launch atop United Launch Alliance Atlas V rocket
Testing encompassed both the Dream Chaser spacecraft by itself as well as integrated in the stacked configuration atop the Atlas V launch vehicle that will boost the vehicle to space from Launch Complex 41 at Cape Canaveral Air Force Station in Florida.
The testing of the Dream Chaser model was conducted at different angles and positions and around the clock inside the Unitary Plan Wind Tunnel at NASA Langley to collect the data as quickly as possible.
“All the data acquired will be used to validate computer models and populate the Dream Chaser spacecraft performance database,” according to NASA test engineer Bryan Falman.
NASA says that the resulting data showed the existing computer models were accurate.
Additonal wind tunnel testing was done at NASA’s Ames Research Center in Moffett Field, California and the CALSPAN Transonic Wind Tunnel in New York.
The wind tunnel work will also significantly aid in refining the Dream Chaser’s design and performance as well as accelerate completion of the Critical Design Review (CDR) before the start of construction of the full scale vehicle for orbital flight tests by late 2016.
Video Caption: Engineers used a wind tunnel at NASA’s Langley Research Center in Hampton, Virginia, to evaluate the design of Sierra Nevada Corporation’s Dream Chaser spacecraft. Credit: NASA
“The aerodynamic data collected during these tests has further proven and validated Dream Chaser’s integrated spacecraft and launch vehicle system design. It also has shown that Dream Chaser expected performance is greater than initially predicted,” said Mark N. Sirangelo, corporate vice president and head of SNC’s Space Systems.
“Our program continues to fully complete each of our CCiCap agreement milestones assisted through our strong collaboration efforts with our integrated ‘Dream Team’ of industry, university and government strategic partners. We are on schedule to launch our first orbital flight in November of 2016, which will mark the beginning of the restoration of U.S. crew capability to low-Earth orbit.”
The Dream Chaser design builds on the experience gained from NASA Langley’s earlier exploratory engineering work with the HL-20 manned lifting-body vehicle.
“The NASA-SNC effort makes for a solid, complementary relationship,” said Andrew Roberts, SNC aerodynamics test lead. “It is a natural fit. NASA facilities and the extensive work they’ve done with the Dream Chaser predecessor, HL-20, combined with SNC’s engineering, is synergistic and provides great results.”
Dream Chaser will be reusable and can carry a mix of cargo and up to a seven crewmembers to the ISS. It will also be able to land on commercial runways anywhere in the world, according to SNC.
Left landing gear failed to deploy as private Dream Chaser spaceplane approaches runway at Edwards Air Force Base, Ca. during first free flight landing test on Oct. 26, 2103. Credit: Sierra Nevada Corp. See video below
Stay tuned here for Ken’s continuing Sierra Nevada, Boeing, SpaceX, Orbital Sciences, commercial space, Orion, Curiosity, Mars rover, MAVEN, MOM and more planetary and human spaceflight news.
Scale models of NASA’s Commercial Crew program vehicles and launchers; Boeing CST-100, Sierra Nevada Dream Chaser, SpaceX Dragon. Credit: Ken Kremer/kenkremer.com
When it comes to the Universe, things often go bump in the night. But whether two galaxies collide, a star explodes in a brilliant supernova, or a meteor hits a massive planet, we tend to catch the aftermath tens to hundreds of thousands of years later.
Of course, there’s always an exception to the rule. In today’s news, astronomers using NASA’s Mars Reconnaissance Orbiter have found a fresh meteor-impact crater. And it’s the biggest seen using before-and-after pictures.
When it comes to the red planet, we’ve seen evidence of fresh craters before, but usually the impact can’t be nailed down to better than a few years’ time. The constant sweep of the obiter’s weather-monitoring camera, the Mars Color Imager (MARCI), however, allowed us to pinpoint the impact to within a day.
The orbiter began its systematic observation of Mars in 2006. Ever since, Bruce Cantor, MARCI’s principle investigator, has examined the camera’s daily images, searching for evidence of dust storms and other observable weather events. Cantor’s findings help NASA operators plan for weather events that may be harmful to the solar-powered rover, Opportunity.
Nearly two months ago, Cantor noticed a black smudge — a telltale sign of an impact — on the red planet. “It wasn’t what I was looking for,” Cantor said in a NASA press release. “I was doing my usual weather monitoring and something caught my eye. It looked usual, with rays emanating from a central spot.”
So Cantor dug through earlier images, discovering that the dark spot wasn’t visible on March 27, 2012, but appeared on March 28, 2012.
MARCI is a low resolution camera, which is what allows it to see a large area of Mars constantly. But without a high resolution image, we can’t pick out the details of the impact-like black smudge. So Cantor performed follow-up observations with the orbiter’s telescope Context Camera (CTX) and the High Resolution Imaging Science Experiment (HiRISE).
CTX has imaged nearly the entire surface of Mars at least once during the orbiter’s seven-plus years of observations. It photographed the site of the newly-discovered crater in January 2012, revealing nothing prior to the impact. But two new craters appear in the recent image.
The largest crater is slightly elongated and spans 48.5 by 43.5 meters, roughly half the length of a football field. “The biggest crater is unusual, quite shallow compared to other fresh craters we have observed,” said HiRISE Principal Investigator Alfred McEwen of the University of Arizona, Tucson.
The impacting object is likely a few meters across. Something that small would burn up in the Earth’s atmosphere, but with a much thinner atmosphere (about 1% as thick as Earth’s), Mars lets most debris right on through.
To add to the details, images from HiRISE revealed more than a dozen smaller craters near the two larger ones seen by CTX. It’s likely that Mars’ atmosphere, as thin as it is, supplied enough pressure to break the incoming meteoroid into smaller pieces, leaving multiple impacts behind.
This image from the HiRISE camera, on board NASA’s Mars Reconnaissance Orbiter reveals the two impact craters and many smaller craters around them. Image Credit: NASA / JPL-Caltech / University of Arizona
“Studies of fresh impact craters on Mars yield valuable information about impact rates and about subsurface material exposed by the excavations,” said Leslie Tamppari, deputy project scientist for the Mars Reconnaissance Orbiter mission at NASA’s Jet Propulsion Laboratory. “The combination of HiRISE and CTX has found and examined many of them, and now MARCI’s daily coverage has given great precision about when a significant impact occurred.”
The initial NASA press release can be viewed here.
The new Type II supernova is nestled up to the nucleus of the galaxy in this photo taken May 21 with a 17-inch telescope. Credit: Gianluca Masi, Francesca Nocentini and Patrick Schmeer
A supergiant star exploded 23.5 million years ago in one of the largest and brightest nearby galaxies. This spring we finally got the news. In April, the Katzman Automatic Imaging Telescope (KAIT) as part of the Lick Observatory Supernova Search, photographed a faint “new star” very close to the bright core of M106, a 9th magnitude galaxy in Canes Venatici the Hunting Dogs.
The inner core of a red or blue supergiant moments before exploding as a supernova looks like an onion with multiple elements “burning” through the fusion process to create the heat and pressure that stays the force of gravity. Fusion stops at iron. With no energy pouring from the central core to keep the other elements cooking, the star collapses and the rebounding shock wave tears it apart.
A study of its light curve indicated a Type II supernova – the signature of a rare supergiant star ending its life in the most violent way imaginable. A typical supergiant star is 8 to 12 times more massive than the sun and burns at a much hotter temperature, rapidly using up its available fuel supply as it cooks lighter elements like hydrogen and helium into heavier elements within its core. Supergiant lifetimes are measured in the millions of years (10-100 million) compared to the frugal sun’s 11 billion years. When silicon fuses to create iron, a supergiant reaches the end of the line – iron can’t be fused or cooked into another heavier element – and its internal “furnace” shuts down. Gravity takes over and the whole works collapses in upon itself at speeds up to 45,000 miles per second.
When the outer layers reached the core, they crushed it into a dense ball of subatomic particles and send a powerful shock wave back towards the surface that rips the star to shreds. A supernova is born! Newly-minted radioactive forms of elements like nickel and cobalt are created by the tremendous pressure and heat of the explosion. Their rapid decay into stable forms releases energy that contributes to the supernova’s light.
This Hubble Space Telescope image shows how spectacular M106 truly is. Dark filaments of dust are silhouetted against billions of unresolved suns. Young star clusters rich with hot, blue stars and tufts of pink nebulosity swaddling newborn stars ornament the galaxy’s spiral arms. A supermassive black hole rumbles at the heart of the galaxy. M106 is the 106th entry in Charles Messier’s famous catalog created in the 18th century. It’s located 23.5 million light years away. Credit: NASA / ESA
For two weeks, the supernova in M106 remained pinned at around magnitude +15, too faint to tease out from the galaxy’s bright, compact nucleus for most amateur telescopes. But a photograph taken by Gianluca Masi and team on May 21 indicate it may have brightened somewhat. They estimated its red magnitude – how bright it appears when photographed through a red filter – at +13.5. A spectrum made of the object reveals the ruby emission of hydrogen light, the telltale signature of a Type II supernova event.
At magnitude +9, M106 visible in almost any telescope and easy to find. Start just above the Bowl of the Big Dipper which stands high in the northwestern sky at nightfall in late May. The 5th magnitude stars 5 CVn (5 Canes Venatici) and 3 CVn lie near the galaxy. Star hop from the Bowl to these stars and then over to M106. Stars plotted to mag. +8. Click to enlarge. Stellarium
Visually the supernova will appear fainter because our eyes are more sensitive to light in the middle of the rainbow spectrum (green-yellow) than the reds and purple that bracket either side. I made a tentative observation of the object last night using a 15-inch (37-cm) telescope and hope to see it more clearly tonight from a darker sky. We’ll keep you updated on our new visitor’s brightness as more observations and photographs come in. You can also check Dave Bishop’s Latest Supernovae site for more information and current images.
Even if the supernova never gets bright enough to see in your telescope, stop by M106 anyway. It’s big, easy to find and shows lots of interesting structure. Spanning 80,000 light years in diameter, M106 would be faintly visible with the naked eye were it as close as the Andromeda Galaxy. In smaller scopes the galaxy’s bright nucleus stands out in a mottled haze of pearly light; 8-inch(20-cm) and larger instrument reveal the two most prominent spiral arms. M106 is often passed up for the nearby more famous Whirlpool Galaxy (M51). Next time, take the detour. You won’t be disappointed.
Artist's impression of an asteroid breaking up. Credit: NASA/JPL-Caltech
Do you lack a telescope, but have a burning desire to look for asteroids near Earth? No problem! NASA and the Slooh telescope network will soon have you covered, as the two entities have signed a new agreement allowing citizen scientists to look at these objects using Slooh.
This is all related to NASA’s Asteroid Grand Challenge (which includes the agency’s desire to capture and redirect an asteroid for further study.) What the two entities want to do is show citizen astronomers how to study asteroids after they are discovered by professionals, looking at properties such as their size and rotation and light reflectivity.
Additionally, Slooh will add 10 new telescopes to the Institute of Astrophysics of the Canary Islands, the facility it is using until at least 2020. The hope is to add to the total of 10,957 discovered near-Earth asteroids, which include 1,472 that are “potentially hazardous.” Astronomers believe only about 30% of the 140-meter sized asteroids near Earth have been discovered, and less than 1% of 30-meter sized asteroids. (Bigger ones more than a kilometer across are about 90% discovered.)
Screenshot from a live webcast from SLOOH Space Camera.
We talk about Slooh frequently on Universe Today because it is one of the go-to locations for live events happening in the cosmos, such as when a solar eclipse occurs. NASA also plans to work with Slooh on these live events, beginning with looking at Comet 209P/LINEAR and its meteor shower when it goes past our planet Friday (May 23).
“This partnership is a great validation of our approch to engage the public in the exploration of space,” stated Michael Paolucci, the founder and CEO of Slooh.
“NASA understands the importance of citizen science, and knows that a good way to get amateur astronomers involved is to offer them ways to do productive astronomy. Slooh does that by giving them remote access to great telescopes situated at leading observatory sites around the world.”
"Cosmic clumps" seen in NASA's Spitzer Space Telescope throw the deepest shadows scientists have ever seen. Credit: NASA/JPL-Caltech/University of Zurich
When gas and dust squeeze tightly enough together in space, no light can get through and the place is black as pitch. But this dusty cloud seen about 16,000 light-years away from us will eventually generate new stars, with the darkest parts creating powerful O-type stars — a star-type poorly known to scientists.
“The map of the structure of the cloud and its dense cores we have made in this study reveals a lot of fine details about the massive star and star cluster formation process,” stated Michael Butler, a postdoctoral researcher at the University of Zurich in Switzerland who led the study.
The new study, which included observations from NASA’s Spitzer Space Telescope, examined the shadows these clumps cast and concluded this cloud is about 7,000 times more massive than the sun, and about 50 light-years in diameter. Because Spitzer examines the universe in infrared light, this allows it to peer through dusty areas that are difficult or impossible to see in visual light, allowing Spitzer to examine different astronomical phenomena.
Artist’s concept of NASA’s Spitzer Space Telescope surrounded by examples of exoplanets it has looked at. Credit: NASA/JPL-Caltech
Looking at clouds such as this one are expected to shed more light (so to speak) on how O-type stars are created. This stellar type is at least 16 times as massive as the sun (but can be much more) and is known for its wind and powerful radiation, that clean out the neighborhood of any dust or gas that could have formed other planets or stars.
Once these stars reach the end of their short lives, they explode as supernovas and also create heavier elements that are found in rocky planets and in the case of Earth (as far as we know), living beings. Researchers are still unclear on how the stars are able to pick up mass that is so much more the mass of our sun without breaking apart.
An artist's impression of a magnetar, a highly magnetic, slowly rotating neutron star. Credit: ESO/L. Calçada
Astronomy is a discipline of extremes. We’re constantly searching for the most powerful, the most explosive, and the most energetic objects in the Universe. Magnetars — extremely dense and highly magnetic neutron stars — are no exception to the rule. They’re the strongest known magnets in the Universe, millions of times more powerful than the strongest magnets on Earth.
But their origin has eluded astronomers for 35 years. Now, an international team of astronomers think they’ve found the partner star of a magnetar for the first time, an observation that suggests magnetars form in binary star systems.
When the core of a massive star runs out of energy, it collapses to form an incredibly dense neutron star or black hole. Meanwhile the outer layers of the star blow away in a stupendously powerful explosion, known as a supernova. A teaspoon of “neutron star stuff” would have a mass of about a billion tonnes, and a few cups would outweigh Mount Everest.
Magnetars are an unusual form of neutron stars with powerful magnetic fields. While there are roughly a dozen known magnetars in the Milky Way, one stands out as being the most peculiar. CXOU J164710.2-455216 — located 16,000 light-years away in the young star cluster Westerlund 1 — is unlike any other magnetar because astronomers can’t see how it formed in the first place.
Astronomers estimate that this magnetar must have been born in the explosive death of a star about 40 times the mass of the Sun. “But this presents its own problem, since stars this massive are expected to collapse to form black holes after their deaths, not neutron stars,” said Simon Clark, lead author on the paper, in a press release. “We did not understand how it could have become a magnetar.”
So astronomers went back to the drawing board. The most promising solution suggested that the magnetar formed through the interactions of two massive stars orbiting one another. Once the more massive star began to run out of fuel, it transferred mass to the less massive companion, causing it to rotate more and more rapidly — a crucial ingredient to creating ultra-strong magnetic fields.
In turn, the companion star became so massive that it shed a large amount of its recently gained mass. This caused it “to shrink to low enough levels that a magnetar was born instead of a black hole — a game of stellar pass-the-parcel with cosmic consequences” said coauthor Francisco Najarro from the Centro de Astrobiología in Spain.
This image shows both the magnetar and its former binary companion, which has been kicked far away. Image Credit: ESO
There was only one slight problem: no companion star had been found. So Clark and colleagues set out to search for a star in other parts of the cluster. They used ESO’s Very Large Telescope to hunt for a hypervelocity star — an object escaping the cluster at an incredible speed — that might have been kicked out of orbit by the supernova explosion that formed the magnetar.
One star, known as Westerlund 1-5, matched their prediction.
“Not only does this star have the high velocity expected if it is recoiling from a supernova explosion, but the combination of its low mass, high luminosity and carbon-rich composition appear impossible to replicate in a single star — a smoking gun that shows it must have originally formed with a binary companion,” said coauthor Ben Ritchie from Open University.
The discovery suggests that double star systems may be essential for forming these enigmatic stars.
The paper has been published in Astronomy & Astrophysics, and is available for download here.
The Mars Hand Lens Imager on NASA's Curiosity Mars rover provided this nighttime view of a hole produced by the rover's drill and, inside the hole, a line of scars produced by the rover's rock-zapping laser. The hole is 0.63 inch (1.6 centimeters) in diameter. The camera used its own white-light LEDs to illuminate the scene on May 13, 2014. Credit: NASA/JPL-Caltech/MSSS
NASA’s rover Curiosity said ‘Goodbye Kimberley’ having fulfilled her objectives of drilling into a cold red sandstone slab, sampling the tantalizing grey colored interior and pelting the fresh bore hole with a pinpoint series of parting laser blasts before seeking new adventures on the road ahead towards the inviting slopes of Mount Sharp, her ultimate destination.
Curiosity successfully drilled her 3rd hole deep into the ‘Windjama’ rock target at the base of Mount Remarkable and within the science waypoint at a region called “The Kimberley” on May 5, Sol 621.
Since then, the 1 ton robot carefully scrutinized the resulting 2.6 inches (6.5 centimeters) deep bore hole and the mound of dark grey colored drill tailings piled around for an up close examination of the texture and composition with the MAHLI camera and spectrometers at the end of her 7-foot-long (2 meters) arm to glean every last drop of science before moving on.
Curiosity’s panoramic view departing Mount Remarkable and ‘The Kimberley Waypoint’ where rover conducted 3rd drilling campaign inside Gale Crater on Mars. The navcam raw images were taken on Sol 630, May 15, 2014, stitched and colorized. Credit: NASA/JPL-Caltech/Ken Kremer – kenkremer.com/Marco Di Lorenzo
Multiple scars clearly visible inside the drill hole and on the Martian surface resulting from the million watt laser firings of the Mast mounted Chemistry and Camera (ChemCam) instrument left no doubt of Curiosity’s capabilities or intentions.
Furthermore she successfully delivered pulverized and sieved samples to the pair of onboard miniaturized chemistry labs; the Chemistry and Mineralogy instrument (CheMin) and the Sample Analysis at Mars instrument (SAM) – for chemical and compositional analysis.
Curiosity completed an “intensive investigation of ‘The Kimberley’, having successfully drilled, acquired and dropped samples into CheMin and SAM,” wrote science team member Ken Herkenhoff in an update.
“MAHLI has taken lots of excellent images of the drill hole, including some during the night with LEDs on, nicely showing the ChemCam LIBS spots.”
“The initial analysis of this new sample by Chemin is ongoing, requiring repeated overnight integration to build up high-quality data,” says Herkenhoff.
The rover’s earth bound handlers also decided that one drill campaign into Kimberley was enough.
So the rover will not be drilling into any other rock targets here.
Composite photo mosaic shows deployment of NASA Curiosity rovers robotic arm and two holes after drilling into ‘Windjana’ sandstone rock on May 5, 2014, Sol 621, at Mount Remarkable as missions third drill target for sample analysis by rover’s chemistry labs. The navcam raw images were stitched together from several Martian days up to Sol 621, May 5, 2014 and colorized. Credit: NASA/JPL-Caltech/Ken Kremer – kenkremer.com/Marco Di Lorenzo
And it may be a very long time before the next drilling since the guiding team of scientists and engineers wants desperately to get on and arrive at the foothills of Mount Sharp as soon as possible.
But the robot will undoubtedly be busy with further analysis of the ‘Windjana’ sample along the way, since there’s plenty of leftover sample material stored in the CHIMRA sample processing mechanism to allow future delivery of samples when the rover periodically pauses during driving.
This May 12, 2014, view from the Mars Hand Lens Imager (MAHLI) in NASA’s Curiosity Mars Rover shows the rock target “Windjana” and its immediate surroundings after inspection of the site by the rover by drilling and other activities. Credit: NASA/JPL-Caltech/MSSS
“Windjana” is named after a gorge in Western Australia.
It’s been a full year since the first two drill campaigns were conducted during 2013 at the ‘John Klein’ and ‘Cumberland’ outcrop targets inside Yellowknife Bay. They were both mudstone rock outcrops and the interiors were markedly different in color.
“The drill tailings from this rock are darker-toned and less red than we saw at the two previous drill sites,” said Jim Bell of Arizona State University, Tempe, deputy principal investigator for Curiosity’s Mast Camera (Mastcam).
“This suggests that the detailed chemical and mineral analysis that will be coming from Curiosity’s other instruments could reveal different materials than we’ve seen before. We can’t wait to find out!”
The science team chose Windjana for drilling “to analyze the cementing material that holds together sand-size grains in this sandstone,” says NASA.
Curiosity’s Panoramic view of Mount Remarkable at ‘The Kimberley Waypoint’ where rover conducted 3rd drilling campaign inside Gale Crater on Mars. The navcam raw images were taken on Sol 603, April 17, 2014, stitched and colorized. Credit: NASA/JPL-Caltech/Ken Kremer – kenkremer.com/Marco Di Lorenzo
Featured on APOD – Astronomy Picture of the Day on May 7, 2014
“The Kimberley Waypoint was selected because it has interesting, complex stratigraphy,” Curiosity Principal Investigator John Grotzinger, of the California Institute of Technology, Pasadena, told me.
Curiosity departed the ancient lakebed at the Yellowknife Bay region in July 2013 where she discovered a habitable zone with the key chemical elements and a chemical energy source that could have supported microbial life billions of years ago – and thereby accomplished the primary goal of the mission.
Windjama lies some 2.5 miles (4 kilometers) southwest of Yellowknife Bay.
Curiosity still has about another 4 kilometers to go to reach the foothills of Mount Sharp sometime later this year.
The sedimentary layers of Mount Sharp, which reaches 3.4 miles (5.5 km) into the Martian sky, is the six wheeled robots ultimate destination inside Gale Crater because it holds caches of water altered minerals. Such minerals could possibly indicate locations that sustained potential Martian life forms, past or present, if they ever existed.
Stay tuned here for Ken’s continuing Curiosity, Opportunity, Orion, SpaceX, Boeing, Orbital Sciences, LADEE, MAVEN, MOM, Mars and more planetary and human spaceflight news.
Illustration of the ESA Planck Telescope in Earth orbit (Credit: ESA)
In 1964 the European Launcher Development Organisation (ELDO) and the European Space Research Organisation (ESRO) were founded, on February 29 and March 20 respectively, marking the beginning of Europe as a major space power and player in the new international venture to explore beyond our planet. A decade later these two entities merged to become ESA, and the rest, as it’s said, is history.
The video above commemorates ESA’s service to the cooperation and innovation of European nations in space, and indeed the entire world with many of the far-reaching exploration missions its member states have developed, launched and maintained. From advanced communications and observational satellites to its many missions exploring the worlds of the Solar System to capturing the light from the beginning of the Universe, ELDO, ESRO, and ESA have pushed the boundaries of science and technology in space for half a century… and are inspiring the next generation to continue exploring into the decades ahead. So happy anniversary, ESA — I can only imagine what we might be looking back on in another 50 years!
Source: ESA. See more key dates from ESA’s history here.
