Opportunity Rover Starts Year 10 on Mars with Remarkable Science Discoveries

Image caption: Opportunity Celebrates 9 Years and 3200 Sols on Mars snapping this panoramic view from her current location on ‘Matijevic Hill’ at Endeavour Crater. The rover discovered phyllosilicate clay minerals and calcium sulfate veins at the bright outcrops of ‘Whitewater Lake’, at right, imaged by the Navcam camera on Sol 3197 (Jan. 20, 2013). “Copper Cliff” is the dark outcrop, at top center. Darker “Kirkwood” outcrop, at left, is site of mysterious “newberries” concretions. Credit: NASA/JPL-Caltech/Cornell/Marco Di Lorenzo/Ken Kremer

9 Years ago, NASA’s pair of identical twin sister rovers – christened Spirit & Opportunity- bounced to daunting airbag-cushioned landings on opposite sides of the Red Planet for what was supposed to be merely 90 day missions, or maybe a little bit longer scientists hoped.

Today, Opportunity celebrates a truly unfathomable achievement, starting Year 10 on Mars since she rolled to a bumpy stop on January 24, 2004 inside tiny Eagle crater. And she’s now at a super sweet spot for science (see our photo mosaic above) loaded with clays and veined minerals and making the most remarkable findings yet about the planets watery past – thus building upon a long string of previously unthinkable discoveries due to her totally unforeseen longevity.

“Regarding achieving nine years, I never thought we’d achieve nine months!” Principal Investigator Prof. Steve Squyres of Cornell University told Universe Today for this article commemorating Opportunity’s 9th anniversary.

Opportunity reached 3200 Sols, or Martian days, and counting , by her 9th birthday. She is now 108 months into the 3 month primary mission – that’s 36 times longer than the 3 month “warranty.”

“Every sol is a gift,” Squyres told me. He always refers to the rovers as our “Priceless assets on Mars”, that have to be taken good care of to wring out the maximum science data possible and for as long as humanly, or more aptly, robotically possible.

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Image Caption: ‘Matijevic Hill’ Panorama for Rover’s Ninth Anniversary. As Opportunity neared the ninth anniversary of its landing on Mars, the rover was working in the ‘Matijevic Hill’ area seen in this view from Opportunity’s panoramic camera (Pancam). Two of the features investigated at Matijevic Hill are “Copper Cliff,” the dark outcrop in the left center of the image, and “Whitewater Lake,” the bright outcrop on the far right. The component images for this mosaic were taken from Sol 3137 (Nov. 19, 2012) through Sol 3150 (Dec. 3, 2012). Credit: NASA/JPL-Caltech/Cornell/Arizona State Univ.

The resilient, solar powered Opportunity robot begins her 10th year roving around beautifully Earth-like Martian terrain where where she proved that potentially life sustaining liquid water once flowed billions of years ago when the planet was warmer and wetter.

Opportunity is healthy and has driven over 22 miles (35 kilometers )- marking the first overland expedition on another planet. See our photo mosaics and route map by Ken Kremer and Marco Di Lorenzo.

She is now working at the inboard edge of “Cape York” – a hilly segment of the eroded rim of 14 mile (22 km) wide Endeavour Crater, featuring terrain with older rocks than previously inspected and unlike anything studied before. It’s a place no one ever dared dream of reaching prior to launch in the summer of 2003 and landing on the Meridiani Planum region of Mars.

“It’s like a whole new mission since we arrived at Cape York,” says Squyres.

Opportunity Sol 3182_3Ba_Ken Kremer

Image caption: Opportunity Celebrates 9 Years on Mars snapping this panoramic view of the vast expanse of 14 mile (22 km) wide Endeavour Crater from atop ‘Matijevic Hill’ on Sol 3182 (Jan. 5, 2013). The rover then drove 43 feet to arrive at ‘Whitewater Lake’ and investigate clay minerals. Photo mosaic was stitched from Navcam images and colorized. Credit: NASA/JPL-Caltech/Cornell/Ken Kremer/Marco Di Lorenzo

Today Opportunity is poised for breakthrough science at deposits of phyllosilicates – clay minerals which stem from an earlier epoch when liquid water flowed on Mars eons ago and perhaps may have been more favorable to sustaining microbial life because they form in more neutral pH water. Endeavour Crater is more than 3 Billion years old.

I asked Squyres to discuss the discovery of the phyllosilicates – which have never before been analyzed up close on the Martian surface and are actually a main target of NASA’s new Curiosity rover at Gale Crater.

“We have found the phyllosilicates at Cape York: they’re in the Whitewater Lake materials,” Squyres explained. Spectral data collected from Mars orbit by the CRISM spectrometer aboard NASA’s MRO circling spacecraft allowed the researchers to direct Opportunity to this exact spot.

“Whitewater Lake” is an area of bright local outcrops currently being investigated and providing information about a different and apparently less acidic environment compared to other areas and craters visited earlier in the mission – and potentially more conducive to life.

Opportunity also discovered more mineral veins at “Whitewater Lake”, in addition to those hydrated mineral veins discovered earlier at Cape York at a spot named “Homestake” – see our mosaic below.

“We have investigated the veins in these materials, and we have determined that they are calcium sulfate,” Squyres confirmed to me.

Opportunity Sol 2761_2a_Ken Kremer

Image caption: Opportunity discovers hydrated Mineral Vein at Endeavour Crater – November 2011. Opportunity determined that the ‘Homestake’ mineral vein was composed of calcium sulfate,or gypsum, while exploring around the base of Cape York ridge at the western rim of Endeavour Crater. The vein discovery indicates the ancient flow of liquid water at this spot on Mars. This panoramic mosaic of images was taken on Sol 2761, November 2011, and illustrates the exact spot of the mineral vein discovery. Featured on NASA Astronomy Picture of the Day (APOD) on 12 Dec 2011. Credit: NASA/JPL/Cornell/Kenneth Kremer/Marco Di Lorenzo.

How do the new mineral veins compare to those at ‘Homestake’ and those just found by Curiosity at Yellowknife Bay inside Gale crater? I asked Sqyures.

“Much narrower, and possibly older,” he said compared to the Homestake calcium sulfate veins .

“It’s too early to say how they compare to the veins at Gale, though.”

The local area at “Cape York” is called “Matijevic Hill” – in honor of a recently deceased team member who played a key role on NASA’s Mars rovers.

The rover has already spent a few months at “Matijevic Hill” on a ‘walk about’ scouting survey and also found concretions dubbed “newberries” that are different from the “blueberry” concretions found earlier in the mission.

How widespread are the phyllosilicates ?

“Matijevic Hill is the only exposure of phyllosilicates we know of at Cape York, so in order to find more we’re going to have to go elsewhere,” Squyres replied. “We haven’t figured out what the “newberries” are yet, but attempting to do that will be our next task.”

It is likely to take many more weeks and even months to “figure out” what this all means for science.

Therefore, no one should expect the robot to move much in the near future. Since the rover made landfall at the western rim of Endeavour crater at Spirit Point in August 2011, she has been circling around Cape York ever since.

Opportunity Sol 2678c_Ken Kremer

Image caption: Opportunity rover first arrived at the western rim of Endeavour Crater (14 miles, 22 km wide) in August 2011. This photo mosaic of navcam images shows portions of the segmented rim of Endeavour crater on Sol 2678. Large ejecta blocks from a smaller nearby crater are visible in the middle. At Endeavour, Opportunity will investigate the oldest minerals deposits she has ever visited from billions of years ago and which may hold clues to environments that were potentially habitable for microbial life. The rover may eventually drive to Cape Tribulation at right if she survives. Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Ken Kremer (kenkremer.com)

What is the next destination for Opportunity?

“Once we’re done at Cape York, our next destination will be Solander Point [to the south],” Squyres confirmed. It’s the next rim segment south of Cape York (see map).

Eventually, if Opportunity continues to function and survives the next Martian winter, she may be directed several miles even further south, along the crater rim to a spot called Cape Tribulation – because it also harbors caches of phyllosilicate clay minerals. But there is no telling when that might be.

“One step at a time,” said Squyres as always. He is not making any guesses or predictions. The mission is totally discovery driven.

Well after so many great science discoveries over the past 9 years, I asked Squyres to describe the context and significance of the phyllosilicates discovery?

“Impossible to say, I’m afraid… we’re still figuring this place out; I can’t put it in context yet,” Squyres concluded.

Thus, there is still so much more bountiful science research still to be done by Opportunity – and nobody is making any forecasts on how long she might yet survive.

So just keep praying to the Martian weather gods for occasional winds and “dust devils” to clean off those life giving solar panels – and to the US Congress to provide the essential funding.

Ken Kremer

Opportunity Sol 2852a_Ken Kremer

Image caption: Opportunity Phones Home – Dusty Self Portrait from Endeavour Crater on Mars on Sol 2852, February 2012. NASA’s rover Opportunity snaps self-portrait where she endured 5th frigid Martian winter at Greeley Haven. Opportunity is currently investigating Cape York ridge and Matijevic Hill at right. Vast expanse of Endeavour Crater and rim in background with dusty solar panels and full on view of the High Gain Antenna (HGA) in the foreground. Mosaic: NASA/JPL/Cornell/ASU/Marco Di Lorenzo/Ken Kremer

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Image caption: Endeavour Crater Panorama from Opportunity, Sol 2681, August 2011 on arrival at the rim of Endeavour and Cape York ridge. Odyssey crater visible at left. Mineral veins were later found to surround Cape York. Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Ken Kremer

Opportunity Route map_3187s_Ken Kremer

Image caption: Traverse Map for NASA’s Opportunity rover from 2004 to 2013 – shows the entire path the rover has driven over 9 years, 3200 Sols and more than 22 miles (35 km) from Eagle Crater landing site to current location at Cape York ridge at Endeavour Crater. Credit: NASA/JPL/Cornell/ASU/Marco Di Lorenzo/Ken Kremer (kenkremer.com)

Weekly Space Hangout – January 25, 2013

Back by popular demand… the Weekly Space Hangout has returned. This is a weekly broadcast on Google+, where I’m joined by a wide and varied team of space and astronomy journalists to discuss the big breaking stories this week.

This week, we talked about:

We record the Weekly Space Hangout every Friday on Google+ at 12:00 pm PST / 3:00 pm EST / 2000 GMT. You’ll want to circle Cosmoquest on Google+ to find out when we’re recording next. The audio for the Weekly Space Hangout is also released to the Astronomy Cast podcast feed.

NASA: Reaches for New Heights – Greatest Hits Video

Video Caption: At NASA, we’ve been a little busy: landing on Mars, developing new human spacecraft, going to the space station, working with commercial partners, observing the Earth and the Sun, exploring our solar system and understanding our universe. And that’s not even everything.Credit: NASA

Check out this cool action packed video titled “NASA: Reaching for New Heights” – to see NASA’s ‘Greatest Hits’ from the past year

The 4 minute film is a compilation of NASA’s gamut of Robotic Science and Human Spaceflight achievements to explore and understand Planet Earth here at home and the heavens above- ranging from our Solar System and beyond to the Galaxy and the vast expanse of the Universe.

Image caption: Planets and Moons in perspective. Credit: NASA

The missions and programs featured include inspiringly beautiful imagery from : Curiosity, Landsat, Aquarius, GRACE, NuSTAR, GRAIL, Dawn at Asteroid Vesta, SDO, X-48C Amelia, Orion, SLS, Apollo, SpaceX, Sierra Nevada Dream Chaser, Boeing CST-100, Commercial Crew, Hurricane Sandy from the ISS, Robonaut and more !

And even more space exploration thrills are coming in 2013 !

Ken Kremer

IMG_3760a_SpaceX launch 22 May 2012

Image caption: SpaceX Falcon 9 rocket blasts off on May 22, 2012 with Dragon cargo capsule from Space Launch Complex-40 at Cape Canaveral Air Force Station, Fla., on the first commercial mission to the International Space Station. The next launch is set for March 1, 2013. Credit: Ken Kremer

Incredible Astrophoto: Thor’s Helmet in Canis Major

Thor’s Helmet Nebula (NGC 2359) in the constellation of Canis Major. Credit and copyright: Rolf Wahl Olsen.

At first glance, you might expect this beautiful image to be from a big ground-based observatory or even one of the space telescopes. But this image was taken by “amateur” astronomer Rolf Wahl Olsen. We’ve featured his work before, and he’s done amazing stuff – such as the first amateur image of another solar system — but even he says this latest image of an emission nebula might be his best image to date.

It’s a stunning look at what is known as Thor’s Helmet. This helmet-shaped feature (complete with wings!) is an emission nebula is located in the constellation of Canis Major, about 15,000 light years from Earth. The nebula is a large expanding bubble illuminated by a central star in its last stage of life — a massive Wolf-Rayet star which is shedding its outer layers of gas at an extremely high rate due to intense radiation pressure. Wolf-Rayet stars are thought to represent a brief stage of evolution near the end of life for giant super massive stars; the last unstable phase before the star explodes as a brilliant supernova.

The nebula is some 30 light years in diameter is embedded among a dense star field consisting of thousands of multi-colored stars, adding more beauty to the scene.

Thanks to Rolf for sharing this gorgeous image with Universe Today.

Here’s more details from Rolf:
Date: 8th, 14th, 19th December 2012 and 5th, 6th, 9th January 2013
Exposure: LRGB: 530:44:33:33m, total 10hrs 40mins @ -28C
Telescope: 10″ Serrurier Truss Newtonian f/5
Camera: QSI 683wsg with Lodestar guider
Filters: Astrodon LRGB E-Series Gen 2
Taken from his observatory in Auckland, New Zealand

A wider view:

Thor's Helmet in Canis Major. Credit and copyright: Rolf Wahl Olsen.
Thor's Helmet in Canis Major. Credit and copyright: Rolf Wahl Olsen.

Want to get your astrophoto featured on Universe Today? Join our Flickr group or send us your images by email (this means you’re giving us permission to post them). Please explain what’s in the picture, when you took it, the equipment you used, etc.

Dry Ice Drives Dramatic Changes on Mars

Mars may not be tectonically active but that doesn’t mean there’s nothing happening on the Red Planet’s surface. This video from NASA’s Jet Propulsion Laboratory shows the dramatic seasonal changes that take place in Mars’ polar regions when the frozen carbon dioxide — called “dry ice”  — coating the basalt sand dunes begins to thaw and cracks, releasing jets of sublimating CO2 gas that carry dark material upwards and outwards, staining the frozen surface of the dunes. Imagine what it would be like to be standing nearby when these jets erupt!

This process occurs around the upper latitudes of Mars every spring and is responsible for the dark (and sometimes light) mottled discolorations observed across sandy and dune-covered terrain.

Bright fans are created when surface conditions cause escaping CO2 gas to condense back onto the surface. (NASA/JPL/University of Arizona)

If a prevailing wind happens to be blowing when the gases are escaping the cracks in the ice, whatever material they are carrying will be spread by the wind across the dunes in long streaks and fans. Read more about this process here.

“It’s an amazingly dynamic process. We had this old paradigm that all the action on Mars was billions of years ago. Thanks to the ability to monitor changes with the Mars Reconnaissance Orbiter, one of the new paradigms is that Mars has many active processes today.”

– Candice Hansen, Planetary Science Institute

The images in the video were acquired by the HiRISE camera aboard the Mars Reconnaissance Orbiter, which has been orbiting and observing Mars in unprecedented detail for over six years. See more HiRISE images of the Martian surface here.

Video: NASA/JPL

Curiosity’s Robotic Arm Camera Snaps 1st Night Images

Image caption: This image of a Martian rock illuminated by white-light LEDs (light emitting diodes) is part of the first set of nighttime images taken by the Mars Hand Lens Imager (MAHLI) camera at the end of the robotic arm of NASA’s Mars rover Curiosity. The image was taken on Jan. 22, 2013, after dark on Sol 165. It covers an area about 1.3 inches by 1 inch (3.4 by 2.5 centimeters). Credit: NASA/JPL-Caltech/MSSS

Curiosity’s high resolution robotic arm camera has just snapped the 1st set of night time images of a Martian rock of the now 5 1/2 month long mission – using illumination from ultraviolet and white light emitting LED’s. See the images above and below.

The Mars Hand Lens Imager (MAHLI) camera is located on the tool turret at the end of Curiosity’s 7 foot (2.1 m) long robotic arm.

MAHLI took the close-up images of a rock target named “Sayunei” on Jan. 22 (Sol 165), located near the front-left wheel after the rover had driven over and scuffed the area to break up rocks in an effort to try and expose fresh material, free of obscuring dust.

“Sayunei” is at the site of the “John Klein” outcrop in “Yellowknife Bay” where the team hopes to commence the 1st rock drilling operations here in the coming days. Curiosity drove a few meters several sols ago to reach “John Klein”.

See below our Sol 157 mosaic showing the “John Klein” outcrop – where the rover snapped these night images of “Sayunei”.

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Image caption: This image of a Martian rock illuminated by ultraviolet LEDs (light emitting diodes) is part of the first set of nighttime images taken by the MAHLI camera on the robotic arm. The image was taken on Jan. 22, 2013, after dark on Sol 165. It covers an area about 1.3 inches by 1 inch (3.4 by 2.5 centimeters). Credit: NASA/JPL-Caltech/MSSS

“The purpose of acquiring observations under ultraviolet illumination was to look for fluorescent minerals,” said MAHLI Principal Investigator Ken Edgett of Malin Space Science Systems, San Diego. “These data just arrived this morning. The science team is still assessing the observations. If something looked green, yellow, orange or red under the ultraviolet illumination, that’d be a more clear-cut indicator of fluorescence.”

Analysis is still in progress to determine whether fluorescent minerals are present. Certain classes of organic compounds are also fluorescent.

MAHLI is an adjustable focus camera that works over a wide range. It can focus on targets just a few centimeters away or on distant objects like Mount Sharp, over 6 miles (10 km) away.

The LED’s surround the MAHLI lens.

Curiosity has discovered widespread evidence for the ancient flow of liquid water at “Yellowknife Bay” in the form of water bearing mineral veins, cross-bedded layering, nodules and spherical sedimentary concretions.

Ken Kremer

Curiosity & Yellowknife Bay Sol 157_4Ca_Ken Kremer

Image caption: Curiosity found widespread evidence for flowing water in the highly diverse, rocky scenery shown in this photo mosaic from the edge of Yellowknife Bay on Sol 157 (Jan 14, 2013). The rover will soon conduct 1st Martian rock drilling operation at flat, light toned rocks at the outcrop called “John Klein”, at center, the site where she is now located. ‘John Klein’ drill site and ‘Sheep Bed’ outcrop ledges to right of rover arm are filled with numerous mineral veins and spherical concretions which strongly suggest precipitation of minerals from liquid water. ‘Snake River’ rock formation is the linear chain of rocks protruding up from the Martian sand near rover wheel. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo

27 Years Ago: Voyager 2’s Visit to Uranus

Image of Uranus’ crescent taken by a departing Voyager 2 on January 25, 1986 (NASA/JPL)

27 years ago today, January 24, 1986, NASA’s Voyager 2 spacecraft sped past Uranus, becoming simultaneously the first and last spacecraft to visit the blue-tinged gas giant, third largest planet in the Solar System.

The image above shows the crescent-lit Uranus as seen by Voyager 2 from a distance of about 965,000 km (600,000 miles.) At the time the spacecraft had already passed Uranus and was looking back at the planet on its way outwards toward Neptune.

Although composed primarily of hydrogen and helium, trace amounts of methane in Uranus’ uppermost atmosphere absorb most of the red wavelengths of light, making the planet appear a pale blue color.

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Image of the 1,500-km-wide Oberon acquired by Voyager 2 on Jan. 24, 1986 (NASA/JPL)

The second of NASA’s twin space explorers (although it launched first) Voyager 2 came within 81,800 kilometers (50,600 miles) of Uranus on January 24, 1986, gathering images of the sideways planet, its rings and several of its moons. Voyager 2 also discovered the presence of a magnetic field around Uranus, as well as 10 new small moons.

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Three moons discovered by Voyager 2 in 1986 (NASA/JPL)

Data gathered by Voyager 2 revealed that Uranus’ rate of rotation is 17 hours, 14 minutes.

At the time of this writing, Voyager 2 is 15,184,370,900 km from Earth and steadily moving toward the edge of the Solar System at a speed of about 3.3 AU per year. At that distance, signals from Voyager take just over 14 hours and 4 minutes to reach us.

See images from Voyager 2’s visit of Uranus here, and check out a video of the August 20, 1977 launch below along with more images from the historic Voyager mission’s “Grand Tour” of the outer Solar System.

Don’t Tell Bones: Are We One Step Closer to “Beaming Up?”

It’s a crazy way to travel, spreading a man’s molecules all over the Universe…

While we’re still a very long way off from instantly transporting from ship to planet à la Star Trek, scientists are still relentlessly working on the type of quantum technologies that could one day make this sci-fi staple a possibility. Just recently, researchers at the University of Cambridge in the UK have reported ways to simplify the instantaneous transmission of quantum information using less “entanglement,” thereby making the process more efficient — as well as less error-prone.

(Because nobody wants a transporter mishap.)

In a paper titled Generalized teleportation and entanglement recycling, Cambridge researchers Sergii Strelchuk, Michal Horodecki and Jonathan Oppenheim investigate a couple of previously-developed protocols for quantum teleportation.

“Teleportation lies at the very heart of quantum information theory, being the pivotal primitive in a variety of tasks. Teleportation protocols are a way of sending an unknown quantum state from one party to another using a resource in the form of an entangled state shared between two parties, Alice and Bob, in advance. First, Alice performs a measurement on the state she wants to teleport and her part of the resource state, then she communicates the classical information to Bob. He applies the unitary operation conditioned on that information to obtain the teleported state.” (Strelchuk et al.)

In order for the teleportation to work, the process relies on entanglement — the remote connection between particles or individual bits of information regardless of the physical space separating them. This was what Einstein referred to as “spooky action at a distance.” But getting particles or information packets entangled is no simple task.

“Teleportation crucially depends on entanglement, which can be thought as a ‘fuel’ powering it,” Strelchuk said in an article on ABC Science. “This fuel… is hard to generate, store and replenish. Finding a way to use it sparingly, or, ideally, recycling it, makes teleportation potentially more usable.”

Read: Beam Me Up, Obama: Conspiracy Theory Claims President Teleported to Mars

Considering the sheer amount of information that makes up the also-difficult-to-determine state of a single object (in the case of a human, even simplistically speaking, about 10^28 kilobytes worth of data) you’re obviously going to want to keep the amount of entanglement fuel needed at a minimum.

Of course, we’re not saying we can teleport red-shirted security officers anywhere yet. But if.

Still, with a more efficient method to reduce — and even recycle — entanglement, Strelchuk and his team are bringing us a little closer to making quantum computing a reality. And it may very well take the power of a quantum computer to even make the physical teleportation of large-scale objects possible… once the technology becomes available.

“We are very excited to show that recycling works in theory, and hope that it will find future applications in areas such as quantum computation,” said Strelchuk. “Building a quantum computer is one of the great challenges of modern physics, and it is hoped that the new teleportation protocol will lead to advances in this area.”

(I’m sure Dr. McCoy would still remain skeptical.)

You can find the team’s full paper here (chock full of maths!) and read the article on ABC Science by Stephen Pincock here.

Transporter room image from TOS “Obsession” episode. © 2013 CBS Studios Inc. All Rights Reserved.

Noctilucent Clouds Imaged by Astronaut Chris Hadfield

Noctilucent clouds, also known as “night shining” clouds imaged by Chris Hadfield. Image credit: NASA

What a perspective! Canadian astronaut Chris Hadfield captured this stunning image of noctilucent clouds above the Pacific South Ocean on January 5th, 2013. Also known as “night shining”, or noctilucent clouds, they form at the edge of much larger polar mesospheric clouds.

Endeavour_silhouette_STS-130Polar mesospheric clouds form at an altitude of 76 to 85 kilometers, near the boundary between the mesosphere and the thermosphere. The mesosphere is the layer of the atmosphere above the stratosphere (where airplanes fly), and the thermosphere is above that, where solar radiation causes a significant spike in temperature. (The Space Shuttle photo over on the right is positioned right between those two layers).

Northpoleclouds_AIMData_cThese clouds are typically seen between 70°-75° in latitude, and last for a season of 60-80 days during the late Spring and early Summer. The clouds themselves are made up of ice crystals which measure up to 100 nm in diameter. Scientists are still working out exactly what causes noctilucent clouds; they’re still a bit of a mystery. But their appearance has become more frequent, increasing in brightness and extent, so it’s possible they’re an indication of increasing climate change.

In this photograph, the Sun is below the horizon, and the ground is dark. Those clouds are still partially illuminated by the Sun, and so we see them with this ethereal wispy structure. Hadfield used a Nikon D35 camera with a 400 mm telephoto lens. At the very bottom of the image, you can see the pale orange color of the stratosphere.

Canadian astronaut Chris Hadfield (did I mention he’s Canadian?) launched to the International Space Station on December 19, 2012 to participate in Expedition 34. He has been returning wondering pictures and sharing them on Twitter and Google+.

Original Source: NASA Earth Observatory

In Orion, There Really is a Hole in the Sky

Clouds of cosmic dust in the region of Orion. Credit: ESO

A new image from ESO’s APEX instrument shows a cloud of gas and dust in the Orion region. Image credit: ESO

When astronomers see dark regions in nebula in visible light, they know there’s something going on. There’s got to be some kind of star forming activity pumping out material that obscures the view to the newly forming starts. Switch to infrared and you can peer through that intervening dust to see the young stars at work.

Astronomers using the European Southern Observatory’s Atacama Pathfinder Experiment (APEX) telescope in Chile were surprised to see a dark region in the nebula NGC 1999, even in infrared, when the cause of the dark region should have been apparent.

Ooo, mystery.

These dark regions in nebulae have been observed for hundreds of years. Even William Herschel found one in the constellation Scorpius back in 1774.”Truly there is a hole in the sky here!” he noted. But it wasn’t a hole. It was a region where star formation is actively happening.

Under construction, nothing to see here, come back in a million years when the newly formed stars have generated powerful solar winds and are clearing out their stellar neighborhoods.

Bok_globules_in_IC2944
Here, I’ve attached an image of bok globules (dark nebulae in IC 2944), which can contain 2 to 50 solar masses of material contained within a volume of about a light-year. Often these dark regions can result in double or even multiple star systems.

But in the case of NGC 1999, astronomers used the APEX instrument to peer at this region in infrared; the perfect wavelength to see through all that dust.

And the hole, this dark region, was still there.

The wide-field area around NGC 1999 in Orion

This is a widefield view of the region around NGC 1999. The nebula itself is right at the middle of this image, with the more famous Orion Nebula up at the top of the picture. Image credit: ESO/Digitized Sky Survey 2. Acknowledgement: Davide De Martin

Thanks to multiple observations from different instruments, astronomers think they’ve puzzled out the nature of this dark hole. It’s actually a cavity carved out by the star V380 Orionis. It really is a dark hole in the nebula, and not a secret star forming region at all.

ngc-1999
V380 Orionis is the brightest star in the region of NGC 1999 – it’s actually the brightest member of a triple star system. It’s got a surface temperature of about 10,000 Kelvin and contains about 3.5 times the mass of the Sun. Back in 2010, researchers uncovered that a powerful jet from V380 Ori is probably responsible for carving out this gap in the nebula.

Original Source: ESO News Release

P.S. Pixies running through my head as I’m writing this.