Universe Today

March 24, 2014December 23, 2015 by David Dickinson

Ready, Set, Messier Marathon: A 2014 Guide

Patiently awaiting darkness at the starting line... Credit and copyright: John Chumack.

Have YOU seen all 110?

The passage of the northward equinox last week on March 20^th means one thing in the minds of many a backyard observer: the start of Messier Marathon season. This is a time of year during which a dedicated observer can conceivably spot all of the objects in Charles Messier’s famous deep sky catalog in the span of one night.

We’ve written about some tips and tricks to completing this challenge previously, as well as the optimal dates for carrying a marathon out. Typically, the New Moon weekend nearest the March equinox is the best time of year for northern hemisphere observers to target all of the objects on Messier’s list. This works because a majority of the Messier objects are clustered into two regions: towards the core of our galaxy in Sagittarius — where the Sun sits during the December solstice — up through the summer triangle constellations of Cygnus, Aquila and Lyra, and in the bowl of Virgo asterism and its super cluster of galaxies that extends northward into the constellation of Coma Berenices. In March through early April the Sun sits in the constellation of Pisces, well away from the galactic plane.

The prospects for completing a Messier marathon in 2014 favor the last weekend on March on the 29^th-30^th. The Moon reaches New on Sunday, March 30^th at 18:45 Universal Time/2:45 PM EDT.

Messier marathons first came into vogue in the early 1970s right around the time Schmidt-Cassegrain and large Dobsonian “light bucket” telescopes came into general use.

Charles Messier began noting the curious objects that he would later incorporate into his famous catalog during the summer of 1758, with his description of the Crab Nebula in Taurus, which would become Messier object number one or M1. Messier was a prolific comet hunter and discovered 21 comets in his lifetime. The catalog was compiled over the span of 13 years from 1771 to 1784. Messier’s original list contained 45 objects, and was later expanded in subsequent editions 103, with Messier’s assistant Pierre Méchain adding six more objects to the catalog. The list is generally tallied at 110 objects, with one famous controversy being M102, which is generally cited as a re-observation of M101 or the galaxy NGC 5866.

The catalog itself contains a grab bag of open and globular clusters, galaxies, planetary and diffuse nebulae, and one double star (M40). The Messier catalog spans the sky down to M7, an object also known as the Ptolemy Cluster, which is the southernmost object on the list at latitude -34 degrees 48’ south.

The first page of Messier's third revision of his catalog describing M1 through M5. Image in th Public Domain. — The first page of Messier’s third revision of his catalog, describing M1 through M5. Image in the Public Domain.

Messier observed from Paris at latitude +48 degrees 51’ north using two primary telescopes of the almost one dozen that he owned for his discoveries: a 6.4” Gregorian reflector and a 3.5” refractor. Messier knew nothing of the nature of these “faint fuzzies” that he’d periodically stumbled across in his cometary vigil. His original intent was to compile a list of “comet imposters” in the night sky for comet hunters to be aware of in their quests. In his words:

“What made me produce this catalog was the nebula which I had seen in Taurus while I was observing the comet of that year (1758). The shape and brightness of that nebula reminded me so much of a comet, that I undertook to find more of its kind, to save astronomers from confusing these nebulae with comets.”

“Beware, here doth not lie comets,” Messier admonishes future generations of observers. Still, some peculiarities remain in the catalog: why did Messier, for example, include such obvious “non-comets” as the Pleiades (M45), but skip over the brilliant Double Cluster in Perseus?

Charles Messier's 1771 sketch of the Orion nebula, M42 in the Messier Catalog. Image in the public domain. — Charles Messier’s 1771 sketch of the Orion nebula, M42 in the Messier Catalog. Image in the public domain.

Alas, such mysteries are known only to Messier, who was interred at the famous Père Lachaise cemetery after his death in 1817. When we visit Paris, we’ll bypass Jim Morison to leave a copy of Burnham’s Celestial Handbook at Messier’s grave.

And just like the road variety, “running the Messier marathon” takes all of the stamina and pacing that a visual athlete can muster. You’ll want to grab M77 and M74 immediately after dusk, or the marathon will be over before it starts. From there, move on up north to the famous Andromeda galaxy (M31) and the scattering of objects around it before settling in for a more leisurely observing pace moving westward through the constellations of Orion, Leo and surrounding objects.

An all-sky map showing the distribution of Messier objects. (Click to enlarge). Credit: Jim Cornmell under a Wikimedia Commons Attribution-Share Alike 3.0 Unported license.

Now towards the approach of local midnight comes the first large group: the Virgo cluster of galaxies extending through Coma Berenices, rising to the east. After this batch, you can catch some quick shut-eye before bagging the Messier objects towards the galactic center and up through Cygnus in the pre-dawn. Plan ahead; M52, M2 and M30 are especially notoriously difficult in the spring dawn sky!

It’s also worth noting your “attitude versus latitude” plays a role as well. To this end, Ed Kotapish compiled this nifty perpetual chart of when the entire Messier catalog is visible from respective latitudes:

A chart calculating number of total Messier objects that are visible on the dates (vertical column in month-day format) versus north latitude (top row). Note that this chart is pertpetual for non-leap years, and does not take into account the pahse of the Moon. Click to enlarge. Credit: Edward Kotapish.

“The bounds of the chart are for a variety of objects,” Ed told Universe Today. “I used nautical twilight (when the Sun falls below -12 degrees in elevation) as the starting and ending condition.” Ed also notes that the top curve of the chart on the morning side is bounded by the difficulty in finding troublesome M30, while the left bottom evening boundary is limited by the observability of M110 and M74, which can be a problem for observers at higher latitudes.

Alternate versions of the Messier marathon exist as well, such as imaging or even sketching all 110 objects in one night.

Why complete a Messier marathon? Well, not only does such a feat hone your visual skills as an observer, but it also familiarizes you with the entire catalog… and there’s nothing that says you have to complete it all in one evening, except of course, for bragging rights at the next star party!

Good luck!

-Here’s a handy list of all 110 of the Messier objects in the catalog.

-Be sure to send those pics of Messier objects and more in to Universe Today’s Flickr forum!

March 24, 2014December 23, 2015 by Jason Major

Cosmologists Cast Doubt on Inflation Evidence

Some physicists still have questions on the true origin of the BICEP2 findings...

It was just a week ago that the news blew through the scientific world like a storm: researchers from the BICEP2 project at the South Pole Telescope had detected unambiguous evidence of primordial gravitational waves in the cosmic microwave background, the residual rippling of space and time created by the sudden inflation of the Universe less than a billionth of a billionth of a second after the Big Bang. With whispers of Nobel nominations quickly rising in the science news wings, the team’s findings were hailed as the best direct evidence yet of cosmic inflation, possibly even supporting the existence of a multitude of other universes besides our own.

That is, if they really do indicate what they appear to. Some theorists are advising that we “put the champagne back in the fridge”… at least for now.

Theoretical physicists and cosmologists James Dent, Lawrence Krauss, and Harsh Mathur have submitted a brief paper (arXiv:1403.5166 [astro-ph.CO]) stating that, while groundbreaking, the BICEP2 Collaboration findings have yet to rule out all possible non-inflation sources of the observed B-mode polarization patterns and the “surprisingly large value of r, the ratio of power in tensor modes to scalar density perturbations.”

“However, while there is little doubt that inflation at the Grand Unified Scale is the best motivated source of such primordial waves, it is important to demonstrate that other possible sources cannot account for the current BICEP2 data before definitely claiming Inflation has been proved. “

– Dent, Krauss, and Mathur (arXiv:1403.5166 [astro-ph.CO])

The history of the universe starting the with the Big Bang. Image credit: grandunificationtheory.com

Inflation may very well be the cause — and Dent and company state right off the bat that “there is little doubt that inflation at the Grand Unified Scale is the best motivated source of such primordial waves” — but there’s also a possibility, however remote, that some other, later cosmic event is responsible for at least some if not all of the BICEP2 measurements. (Hence the name of the paper: “Killing the Straw Man: Does BICEP Prove Inflation?”)

Not intending to entirely rain out the celebration, Dent, Krauss, and Mathur do laud the BICEP2 findings as invaluable to physics, stating that they “will be very important for constraining physics beyond the standard model, whether or not inflation is responsible for the entire BICEP2 signal, even though existing data from cosmology is strongly suggestive that it does.”

Now I’m no physicist, cosmologist, or astronomer. Actually I barely passed high school algebra (and I have the transcripts to prove it) so if you want to get into the finer details of this particular argument I invite you to read the team’s paper for yourself here and check out a complementary article on The Physics arXiv Blog.

And so, for better or worse (just kidding — it’s definitely better) this is how science works and how science is supposed to work. A claim is presented, and, regardless of how attractive its implications may be, it must stand up to any other possibilities before deemed the decisive winner. It’s not a popularity contest, it’s not a beauty contest, and it’s not up for vote. What it is up for is scrutiny, and this is just an example of scientists behaving as they should.

Still, I’d keep that champagne nicely chilled.

Source: The Physics arXiv Blog

_________

Want to read more about the BICEP2 findings from actual physicists? Read more in an article by Peter Coles, see what Matthew Francis has to say in his article on arstechnica here, and watch a video by Sean Carroll on PBS News Hour.

March 24, 2014March 8, 2017 by Fraser Cain

Can Light Orbit A Black Hole?

Since black holes are the most powerful gravitational spots in the entire Universe, can they distort light so much that it actually goes into orbit? And what would it look like if you could survive and follow light in this trip around a black hole?

I had this great question in from a viewer. Is it possible for light to orbit a black hole?

Consider this thought experiment, first explained by Newton. Imagine you had cannon that could shoot a cannonball far away. The ball would fly downrange and then crash into the dirt. If you shot the cannonball harder it would fly further before slamming into the ground. And if you could shoot the cannonball hard enough and ignore air resistance – it would travel all the way around the Earth. The cannonball would be in orbit. It’s falling towards the Earth, but the curvature of the Earth means that it’s constantly falling just over the horizon.

This works not only with cannonballs, astronauts and satellites, but with light too. This was one of the big discoveries that Einstein made about the nature of gravity. Gravity isn’t an attractive force between masses, it’s actually a distortion of spacetime. When light falls into the gravity well of a massive object, it bends to follow the curvature of spacetime.

Distant galaxies, the Sun, and even our own Earth will cause light to be deflected from its path by their distortion of spacetime. But it’s the incredible gravity of a black hole that can tie spacetime in knots. And yes, there is a region around a black hole where even photons are forced to travel in an orbit. In fact, this region is known as the “photon sphere”.

From far enough away, black holes act like any massive object. If you replaced the Sun with a black hole of the same mass, our Earth would continue to orbit in exactly the same way. But as you get closer and closer to the black hole, the orbiting object needs to go faster and faster as it whips around the massive object. The photon sphere is the final stable orbit you can have around a black hole. And only light, moving at, well, light speed, can actually exist at this altitude.

Artist impression of a black hole. Credit: ESO/L. Calçada

Imagine you could exist right at the photon sphere of a black hole. Which you can’t, so don’t try. You could point your flashlight in one direction, and see the light behind you, after it had fully orbited the black hole. You would also be bathed in the radiation of all the photons captured in this region. The visible light might be pretty, but the x-ray and gamma radiation would cook you like an oven.

Below the photon sphere you would see only darkness. Down there is the event horizon, light’s point of no return. And up above you’d see the Universe distorted by the massive gravity of the black hole. You’d see the entire sky in your view, even stars that would be normally obscured by the black hole, as they wrap around its gravity. It would be an awesome and deadly place to be, but it’d sure beat falling down below the event horizon.

If you could get down into the photon sphere, what kind of experiments would you want to do? Tell us in the comments below.

March 24, 2014December 23, 2015 by Elizabeth Howell

‘Yesterday’s Coffee’: Drinking Urine In Space Could Preview Mars Exploration Techniques

Expedition 10 commander Leroy Chiao is reflected in a water sphere on board the International Space Station in 2004. Credit: NASA

“Here on board the ISS, we turn yesterday’s coffee into tomorrow’s coffee” is a slogan that sounds a little like a Don Draper-led advertising campaign. Seriously, though, it’s a nifty way in which Expedition 39 commander Koichi Wakata describes in this video (also embedded below) how the astronauts drink purified urine on the station.

The water is perfectly hygienic once it runs through the system, and moreover, it could be a useful trick for future space colonists to remember.

Water is heavy, at about 8.3 pounds per gallon (or roughly 1 kg/liter) at room temperature. And astronauts in space do need to go through a lot of it to prevent dehydration and other illnesses. Throw in demanding activities such as exercising two hours a day or going on a spacewalk, and you can see how quickly people in space go through it.

Everything sent into space has an associated launch cost with it, and space engineers are always looking for ways to shave a few grams here or there. By installing the water purification system (which was completed in 2009 with Wakata on board), NASA said it would be able to reduce the amount sent up to station.

When people speak of space colonies on the Moon or Mars, they often talk about landing them near a large source of water ice and then using that to help support the people working there. As NASA once wrote in a worksheet, “Until an orbiting grocery store is opened, recycling of water and air will be crucial for crew survival.”

Check out Wakata’s explanation of the water recycling system below. For more information on recycling water in Mars colonies, one source to start with could be T. A. Heppenheimer’s “Colonies In Space”, published on the National Space Society website.

March 23, 2014December 23, 2015 by Ken Kremer

NASA Targeting Earth Observing Satellites and ISS Sensors to Aid Missing Malaysian Airline Search

Sensors aboard NASA’s Terra satellite are aiding the search for MH 370. Credit: NASA

NASA has actively joined the hunt for the missing Malaysian Airline flight MH-370 that mysteriously disappeared without a trace more than two weeks ago on March 8, 2014.

Sensors aboard at least two of NASA’s unmanned Earth orbiting global observation satellites as well as others flying on the manned International Space Station (ISS) are looking for signs of the jetliner that could aid the investigators from a multitude of nations and provide some small measure of comfort to the grieving families and loved ones of the passengers aboard.

“Obviously NASA isn’t a lead agency in this effort. But we’re trying to support the search, if possible,” Allard Beutel, NASA Headquarters, Office of Communications director, told Universe Today this evening.

NASA’s airplane search assistance comes in two forms; mining existing space satellite observing data and retargeting space based assets for new data gathering since the incident.

The Malaysian Airline Boeing 777-2H6ER jetliner went missing on March 8 while cruising en route from Kuala Lampur, Malaysia to Beijing, China. See cockpit photo below.

Accurate facts on why MH-370 vanished with 239 passengers aboard have sadly been few and far between.

Chinese satellite image of possible debris of MH 370. Credit: China/SASTIND

Last week, the search area shifted to a wide swath in the southern Indian Ocean when potential aircraft debris was spotted in a new series of separate satellite images from Australia and China government officials.

A prior set of official Chinese government satellite images at a different location yielded absolutely nothing.

The area is now focused 2,500 km (1,600 mi) south west of Perth, a city on the western coast of Australia.

NASA’s search support was triggered upon activation of the International Charter on Space and Major Disasters.

Available data from NASA’s Terra and Aqua satellites has already been transmitted to the U.S. Geological Survey and new data are now being collected in the search area.

“In response to activation of the International Charter on Space and Major Disasters last week regarding the missing Malaysia Airlines jetliner, NASA sent relevant space-based data to the U.S. Geological Survey’s Earth Resources Observations and Science Hazard Data Distribution System that facilitates the distribution of data for Charter activations,” according to a NASA statement.

And it’s important to note that NASA satellites and space-based cameras are designed for long-term scientific data gathering and Earth observation.

“They’re really not meant to look for a missing aircraft,” Beutel stated.

“The archive of global Earth-observing satellite data is being mined for relevant images. These include broad-area views from the MODIS [instrument] on NASA’s Terra and Aqua satellites,” Beutel informed me.

The next step was to retarget both satellites and another high resolution camera aboard the ISS.

“In addition, two NASA high-resolution assets have been targeted to take images of designated search areas: the Earth Observing-1 satellite and the ISERV camera on the International Space Station,” Beutel explained.

Sensors aboard NASA’s Aqua satellite are aiding the search for MH 370. Credit: NASA

Aqua and Terra were already gathering new observations with the MODIS instrument in the search area off Australia last week. MODIS measures changes in Earth’s cloud cover.

Here are the satellite observation times and capabilities:

• MODIS on the Aqua satellite observed at about 1:30 p.m. local time as it passes overhead from pole-to-pole
• MODIS on the Terra satellite observed at about 10:30 a.m. local time
• The width (field of view) of a MODIS observation is 2,300 kilometers
• One pixel of a MODIS image – the limit of how small a feature it can see – is about 1 kilometer.

A new set of high resolution Earth imaging cameras are being sent to the ISS and are loaded aboard the SpaceX CRS-3 Dragon resupply capsule now slated for blastoff on March 30.

The newly launched NASA/JAXA GPM precipitation monitoring satellite which will cover this ocean area in the future is still in the midst of science instrument checkout.

The International Space Station (ISS) in low Earth orbit. Credit: NASA

Ships and planes from at least 26 countries have been being dispatched to the new based on the new satellite imagery to search for debris and the black boxes recording all the critical engineering data and cockpit voices of the pilot and copilot and aid investigators as to what happened.

No one knows at this time why the Malaysia Airlines flight mysteriously disappeared.

Ken Kremer

Map of possible MH 370 debris locations published 1: 12 March (disproved), 2: 20–23 March 2014. Credit: Wikipedia

Flight deck view of the missing MH 370 aircraft, showing many of the communication systems now under investigation. Credit: Chris Finney

March 23, 2014December 23, 2015 by Bob King

Sirius, UFO trickster extraordinaire

Pilot Kenneth Arnold with an illustration of a UFO he saw in 1947. The modern run of UFO sightings began when Arnold reported seeing nine objects flying in a V-formation over Mt. Ranier in Washington. Click for more on the story.

Scintillating Sirius is sometimes mistaken for a UFO

I’ve never seen a UFO that stayed a UFO. I remember certain moving lights as a kid but they turned out to be airplanes or geese aglow with light pollution. And who hasn’t been tricked into thinking they’ve discovered the next Milky Way supernova only to realize it was a distant aircraft in your line of sight?

For all the hours of dark sky time amateur astronomers accumulate, few of us have seen a UFO. It makes sense. We’re generally familiar with the stars and their movements, where the planets happen to be and the atmosphere’s uncanny ability to distort and parse light into strange and beautiful phenomena. Not that some skywatchers haven’t seen a few things that defy immediate explanation.

While some might say this takes away the magic of the night sky, rendering us blind to the possibility of UFOs, I’d argue the contrary. Knowledge deepens our appreciation of all we see, hear, smell and touch.

Sirius, nicknamed the Dog Star is the brightest star in Canis Major and brightest in the night sky. This map show Sirius about 1/3 of the way up in the southern sky during late twilight this month. Stellarium — Sirius, nicknamed the Dog Star, is the brightest star in Canis Major and brightest in the night sky. This map show Sirius about 1/3 of the way up in the southern sky during late twilight this month. Stellarium

Familiar objects often mistaken for UFOs include bright stars, planets and satellites, but high – if not highest – on the list is Sirius in the constellation Canis Major the Greater Dog.

Sirius has attained UFO status for several good reasons: at magnitude -1.5 it’s the brightest star in the sky, it “moves” both slowly and rapidly and shoots out light of different colors.

Because it’s bright, and for many of us, falls along an easy line of sight on March evenings, we’re bound to notice it. No star sparkles more intensely especially when hovering low in the sky.

For skywatchers at mid-northern latitudes, Sirius is the bright, often flashing star in the southern sky at nightfall. Credit: Bob King

Stars. So big but yet so tiny. Despite their enormous size, distance reduces stars to tiny pinpoints even in the largest telescopes. When a star beam hits our atmosphere, it gets yanked around by parcels of air of varying density, speed and size. Each parcel acts like a individual lens, refracting or bending the star’s light into a tiny image. As the air churns overhead, the positions of all those individual images continually change, zigging the star in random directions. While our eyes aren’t keen enough to distinguish the many tiny images moving to and fro, we sense the starlight’s tortured path as sputtering light or twinkling. All stars flitter around – just ask telescopic observers – but twinkling is most noticeable in bright stars like Vega, Canopus, Rigel and especially Sirius.

Twinkling is caused by moving air pockets in our atmosphere. Twinkling is much stronger and more noticeable near the horizon, because our line of sight passes through a much greater thickness of air. Illustration: Bob King - See more at: http://astrobob.areavoices.com/2011/09/04/why-stars-twinkle-and-sputter-in-color/#sthash.MNP51ROv.dpuf — Twinkling is caused by moving air pockets in our atmosphere. Twinkling is much stronger and more noticeable near the horizon, because our line of sight passes through a much greater thickness of air. Illustration: Bob King

Mind you, it doesn’t necessarily matter how calm it is on the ground. Some 10 miles of relatively thick air between you and Sirius provide plenty of opportunities for fluttering images on many otherwise tranquil nights. Bright planets generally don’t twinkle because they’re close enough to show actual disks. Tiny shifts induced by atmospheric turbulence can bodily move a star with ease, but planets are big enough compared to the size of the air cells to hold their own and beam forth a steady light.

For some, Sirius’ twinkling creates the sense that a star is moving or shooting about, making it that much more mysterious. Superimposed on this apparent rapid movement is the slow westward drift of the stars caused by Earth’s rotation. People have contacted me about brilliant, slow-moving objects, and it’s clear they’ve been watching a star get a free ride from our revolving planet.

The color and brightness of Sirius can change rapidly as it twinkles. I shot these slightly out of focus to spread the color out and show it more clearly. Not only are the hues striking but brightness changes are obvious, too. Photo: Bob King — The color and brightness of Sirius changes rapidly as it twinkles. I shot these individual 1/30″ photos slightly out of focus to spread the color out and show it more clearly. Not only are the hues striking but brightness changes are obvious, too. The short video at the top of this story captures Sirius’ twinkling “live”.Credit: Bob King

So we’ve got brightness and movement going for us – what about color? Colors come from the air, too. Just as white light is composed of a rainbow or spectrum of individual colors from indigo to red, so is starlight. When Sirius is low above the horizon, refraction (bending of light) is strong enough to create images of the star in every color of the rainbow and cast them about in different directions. Split-second variations in air density and flow make for continuous multi-color sparkles.

Sirius’ colors are fairly obvious with the naked eye, but I’ve found binoculars show them even better. By the way, the jerkiness induced in holding binoculars steady adds another motion factor to the UFO equation.

Sirius is hotter, brighter and 1.75 times the size of our own sun. It's located nearby as stars go at a distance of 8.7 light years, the main reason it appears so bright in the sky. Credit: Wikipedia — Sirius is hotter, brighter and 1.75 times the size of our own sun. As stars go, it’s practically in our backyard at just 8.7 light years away – the main reason it appears so bright in the nighttime sky. Credit: Wikipedia

Once, a fellow came to our local planetarium with video he’d taken of a UFO, hoping for help in identifying the object. We watched it change from a star to a bloated disk and back to a star again as the image jumped wildly about in the shaky, hand-held camera. Knowing the date and time of the footage, we instantly knew it was the camera struggling to maintain autofocus on Sirius.

Sirius is orbited by an Earth-sized, superdense white dwarf nicknamed the "Pup". Credit: NASA/ESA — Sirius is orbited by an Earth-sized, superdense white dwarf nicknamed the “Pup”. Credit: NASA/ESA

I remember thinking, “wow, we really helped this guy out”, but he was less than pleased. We tried to explain that he was seeing not only the brightest star in the sky but one twice as massive as the sun and nearly twice its size. But facts were of no use. Convinced he had recorded a UFO anyway, he took his video and promptly left!

I’d love to see a real space ship UFO powered by alien biology. Deep down many of us suspect they exist. With 1,779 extra-solar planets confirmed to date, habitats for potential life seem more certain than ever. But what are the odds of little green men dropping by anything soon? Not only are the distances between stars daunting, but intelligent species may have no interest in outer space or leaving the home planet. After all, whales don’t build space ships.

March 22, 2014April 26, 2016 by Ken Kremer

Curiosity Pulls into Kimberley and Spies Curvy Terrain For Drilling Action

Martian landscape with rows of curved rock outcrops at ‘Kimberly’ in the foreground and spectacular Mount Sharp on the horizon. NASA’s Curiosity Mars rover pulled into Kimberly waypoint dominated by layered rock outcrops as likely drilling site. This colorized navcam camera photomosaic was assembled from imagery taken on Sol 576 (Mar. 20, 2014). Credit: NASA/JPL-Caltech/Marco Di Lorenzo/Ken Kremer-kenkremer.com

Martian landscape with rows of curved rock outcrops at ‘Kimberley’ in the foreground and spectacular Mount Sharp on the horizon. NASA’s Curiosity Mars rover pulled into Kimberly waypoint dominated by layered rock outcrops as likely drilling site. This colorized navcam camera photomosaic was assembled from imagery taken on Sol 576 (Mar. 20, 2014).
Credit: NASA/JPL-Caltech/Marco Di Lorenzo/Ken Kremer-kenkremer.com
See additional Curiosity Mars photomosaics below[/caption]

KENNEDY SPACE CENTER, FL – NASA’s Curiosity rover has just pulled into gorgeous terrain chock full of curvy rock outcrops at Kimberley that’s suitable for contact science and drilling action, according to the mission team.

The six wheeled Martian dune buggy drove into the dazzling Kimberley waypoint this week after traversing a swath of otherworldly dune fields since passing through a gateway known as the ‘Dingo Gap’ sand dune some six weeks ago.

The robot’s arm has been deployed to investigate the most scientifically productive spots to touch Kimberley’s textured outcrops for detailed scrutiny.

The science team has been hunting for tasty rock outcrops suitable for the first drilling campaign since she departed the dried out lakebed at Yellowknife Bay in July 2013 and began her epic trek across the floor of Gale Crater towards the base of Mount Sharp.

With each passing Sol, or Martian day, Mount Sharp looms larger and larger and the historical layers with deposits of hydrated minerals potentially indicative of an alien habitable zone come ever clearer into focus.

About a month ago on Feb. 19 (Sol 548), Curiosity couldn’t resist the urge to pause mid dune drive, just like a tourist, and snap fabulous imagery of multiple rows of striated rocks at the Junda outcrop – see our mosaics below.

Junda appeared remarkably similar to Kimberley, about 1 kilometer back.

Curiosity looks back at Martian sand dunes and rover tracks after passing by Junda outcrop (right) on Sol 548 (Feb. 19, 2014) with Gale Crater rim and Mount Sharp on the distant horizon. Navcam colorized photomosaic. Credit: NASA/JPL-Caltech/Ken Kremer- kenkremer.com/Marco Di Lorenzo

So after executing a final series of short bumps edging ever closer to the outcrops this week, Curiosity parked at the periphery of Kimberley on Thursday, March 20, Sol 576, and captured breathtaking imagery of the rocky rows dominated by towering Mount Sharp on the distant horizon.

See our photomosaics showing the spectacularly inviting terrain around Kimberley and Junda – above and below by Marco Di Lorenzo and Ken Kremer.

“The images [at Kimberley] show nice outcrops in front of the rover, suitable for contact science,” according to science team member Ken Herkenhoff in a mission update.

NASA’s Curiosity Mars rover will likely drill into this layered rock outcrop, near the center of the mosaic, at the Kimberly waypoint. This photomosaic was assembled from high resolution Mastcam 34 camera images taken on Sol 574 (March 18, 2014). Credit: NASA/JPL-Caltech/Marco Di Lorenzo/Ken Kremer-kenkremer.com

This weekend, the state of the art robot is conducting contact science with the cameras and spectrometers on the terminus of the 7 foot long robotic arm and the mast mounted ChemCam laser and high resolution cameras to determine the best spot for drilling and sampling.

The team commanded Curiosity to clean out the arms CHIMRA sample handling mechanism in anticipation of boring into the Martian outcrops and delivering powdery, pulverized samples of cored Martian rocks to the SAM and CheMin miniaturized chemistry labs waiting patiently inside the robots belly to eat something exciting from the Red Planet.

“The arm will be deployed to “thwack” and vibrate CHIMRA to clean out any remnants of the “John Klein” [drilling] sample, followed by Mastcam and RMI imaging of the CHIMRA sieve,” says Herkenhoff.

Scientists directed Curiosity on a pinpoint drive to Kimberly after their interest was piqued by orbital images taken by the powerful telescopic camera on NASA’s Mars Reconnaissance Orbiter (MRO) circling overhead.

“At Kimberly, we see three terrain types exposed and a relatively dust-free surface,” said science team collaborator Katie Stack of the California Institute of Technology, Pasadena.

Flattened fisheye hazcam camera view of Kimberly rock outcrop and Mount Sharp backdrop, taken on Sol 576 (Mar. 20, 2014) and colorized. Credit: NASA/JPL-Caltech/Marco Di Lorenzo/Ken Kremer - kenkremer.com — Flattened fisheye hazcam camera view of Kimberly rock outcrop and Mount Sharp backdrop, taken on Sol 576 (Mar. 20, 2014) and colorized. Credit: NASA/JPL-Caltech/Marco Di Lorenzo/Ken Kremer – kenkremer.com

The missions science focus has shifted to “search for that subset of habitable environments which also preserves organic carbon,” says Curiosity Principal Investigator John Grotzinger, of the California Institute of Technology in Pasadena.

Organic molecules are the building blocks of life as we know it.

The sedimentary foothills of Mount Sharp, which reaches 3.4 miles (5.5 km) into the Martian sky, is the 1 ton 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.

Curiosity discovered a habitable zone at Yellowknife via two drilling operations at the John Klein and Cumberland outcrops and thereby accomplished the primary goal of the mission.

Mars rock rows and Mount Sharp. Martian landscape scene with rows of striated rocks in the foreground and Mount Sharp on the horizon. NASA's Curiosity Mars rover paused mid drive at the Junda outcrop to snap the component images for this navcam camera photomosaic on Sol 548 (Feb. 19, 2014) and then continued traveling southwards towards mountain base. UHF Antenna at right. Credit: NASA/JPL-Caltech/Marco Di Lorenzo/Ken Kremer-kenkremer.com — Mars rock rows and Mount Sharp. Martian landscape scene with rows of striated rocks in the foreground and Mount Sharp on the horizon. NASA’s Curiosity Mars rover paused mid drive at the Junda outcrop to snap the component images for this navcam camera photomosaic on Sol 548 (Feb. 19, 2014) and then continued traveling southwards towards mountain base. UHF Antenna at right. Credit: NASA/JPL-Caltech/Marco Di Lorenzo/Ken Kremer-kenkremer.com

To date Curiosity’s odometer stands at 6.2 kilometers. She has taken over 132,000 images.

The robot has somewhat over another 4 kilometers to go to reach the base of Mount Sharp.

She may arrive at the lower reaches of Mount Sharp sometime in mid 2014, but must first pass through a potentially treacherous dune field.

Meanwhile, NASA’s sister Opportunity rover is exploring clay mineral outcrops by the summit of Solander Point on the opposite side of Mars at the start of her 2nd Decade investigating the Red Planet’s mysteries.

A pair of new orbiters are streaking to the Red Planet to fortify Earth’s invasion fleet- NASA’s MAVEN and India’s MOM.

Stay tuned here for Ken’s continuing Curiosity, Opportunity, Chang’e-3, SpaceX, Orbital Sciences, LADEE, MAVEN, MOM, Mars and more planetary and human spaceflight news.

Learn more at Ken’s upcoming presentations at the NEAF convention on April 12/13 and at Washington Crossing State Park, NJ on April 6. Also evenings at the Quality Inn Kennedy Space Center, Titusville, FL, March 24/25 and March 29/30.

Ken Kremer

NASA Curiosity Mars rover Traverse Map from Landing Zone in Gale Crater to Kimberly Waypoint. Credit: NASA

March 22, 2014April 26, 2016 by Nancy Atkinson

Check Out These Online Astronomy Classes and Contests

Here are a few upcoming and ongoing astronomy classes and photography contests that our readers may be interested in.

Once a year, the One-Minute Astronomer — aka Brian Ventrudo — offers a detailed course called “The Art of Stargazing,” and you need to act fast on this one, as the final signup date is March 24, 2014. This 12-month course breaks down everything you need to know about stargazing into bite-sized pieces… detailed sky tours, choosing and using the best binoculars and telescope for you, and a smattering of science to help you understand a little about your place in the universe. It also shows you how to find and enjoy hundreds of achingly beautiful sights you will remember for the rest of your life.”

You have until noon (GMT) this Monday, March 24 to begin your personal odyssey through the heavens. As the Brian says, “You’ll come away from The Art of Stargazing with everything you need to become a skilled backyard stargazer.”

The cost is $197 USD, and there are payment plans, as well as a lifetime of followup information and email advisories. Get all the details here.

As always, you can find other ongoing classes at the CosmoQuest Academy. They regularly have new classes as well as opportunities for citizen science with their Moon Mappers, Asteroid Mappers and Planet Mappers programs.

There are also two astrophotography contests going on right now:

Ciel et Espace Photos in France is having their Photo Nightscape Awards, and are looking for submissions of Earth and night sky photos. Photos must be taken between January 1, 2014 and August 31, 2014. One photo submission per photographer, and all formats are accepted: panoramic, square, mosaics.

Prizes will be awarded Sunday, November 9, 2014 at the Rencontres Sky and Space (NCE) which will take place from 8 to 11 November 2014 at the Cité des Sciences et de l’Industrie.

They have two categories: pro and amateur. Prizes include a trip to the Very Large Telescope from ESO, a trip to the Alqueva Dark Sky Resever in Portugal for first prizes, and second prizes are a pair of Binocular from Nikon.

The judge for the contest is Miguel Claro, whose astrophotography we feature often here on Universe Today.

Get more information and find all the rules here.

A second photo contest comes from our friends at TWAN—The World At Night with their 5th annual International Earth and Sky Photo Contest, which is part of Global Astronomy Month in April 2014. The TWAN the contest is open to anyone of any age, anywhere around the world.

This year’s contest theme, “Dark Skies Importance,” has two categories: “Beauty of the Night Sky” and “Against the Lights.” Photos submitted to the contest should address either category: either to impress people on how important and amazing the starry sky is or to impress people on how bad the problem of light pollution has become. Both categories illustrate how light pollution affects our lives. Photographers can submit images to one or both categories.

Submitted photographs must be created in the “TWAN style” — showing both the Earth and the sky — by combining elements of the night sky (e.g., stars, planets, the Moon or celestial events) in the backdrop of a beautiful, historic, or notable location or landmark. This style of photography is called “landscape astrophotography”. This is similar to general “Nightscape Photography” but with more attention to the sky, astronomical perspectives, and celestial phenomena.

Find out more here.

March 22, 2014April 26, 2016 by Ken Kremer

SpaceX Resets Space Station Launch with Revolutionary Rocket Legs and Robonaut Legs to March 30

The Dragon spacecraft, filled with about 4,600 lbs of cargo bound for the space station, is mated with Falcon 9. Credit: SpaceX

KENNEDY SPACE CENTER, FL – Following last week’s sudden and late in the processing flow postponement of the SpaceX Falcon 9 rocket launch, SpaceX announced a reset of its next cargo mission launch for NASA to the International Space Station (ISS) to a new target date of Sunday, March 30.

The commercially developed Falcon 9 booster and Dragon cargo vessel are slated for a spectacular night time liftoff from Cape Canaveral Air Force Station in Florida at 10:50 p.m. EDT on March 30, SpaceX announced on Friday.

This mission, soaring to space under a resupply contract to NASA, could ignite a revolution in both rocketry and robotics.

The first stage of the Falcon 9 rocket sports a quartet of never before tried landing legs and the Dragon freighter is loaded with a set of lanky legs to enable mobility in space for NASA’s Robonaut 2 standing at the cutting edge of space robotics technology.

Launch preparations were suddenly halted less than 72 hours prior to the then planned March 16 early morning launch because of unspecified technical issues concerning the sudden discovery of “contamination,” sources told me.

The Falcon 9 rocket with landing legs in SpaceX’s hangar at Cape Canaveral, Fl, preparing to launch Dragon to the space station this Sunday March 30. Credit: SpaceX

“To ensure the highest possible level of mission assurance and allow additional time to resolve remaining open items, the team is taking additional time to resolve open items and ensure SpaceX does everything possible on the ground to prepare for a successful launch,” according to a statement from SpaceX.

Several sources told me that the problem related to “contamination” that was found in the “unpressurized truck section” at the rear of the Dragon spacecraft.

“An unknown contaminant of unknown origin was found on a blanket in the Dragon trunk,” independent sources said to Universe Today soon after the postponement was announced.

“After careful review and analysis, engineering teams representing both the ISS and SpaceX have determined Dragon is ready to fly ‘as-is.’ All parties agree that the particular constituents observed in Dragon’s trunk are in line with the previously defined environments levels and do not impose additional risk to the payloads,” SpaceX announced in a new statement.

With the contamination issues now resolved, the launch is back on track.

Robonaut 2 engineering model equipped with new legs like those heading to the ISS on upcoming SpaceX CRS-3 launch were on display at the Kennedy Space Center Visitor Complex on March 15, 2014. Credit: Ken Kremer - kenkremer.com — Robonaut 2 engineering model equipped with new legs like those heading to the ISS on upcoming SpaceX CRS-3 launch were on display at the Kennedy Space Center Visitor Complex on March 15, 2014. Credit: Ken Kremer – kenkremer.com

NASA Television will air live coverage on Sunday.

In case the launch is delayed, the backup launch opportunity is at 9:39 p.m. Wednesday, April 2.

Altogether, this unmanned SpaceX CRS-3 mission will deliver over 5000 pounds of science experiments, a pair of legs for Robonaut 2, a high definition imaging camera suite, an optical communications experiment and essential gear, spare parts, crew provisions, food, clothing and supplies to the six person crews living and working aboard the ISS soaring in low Earth orbit under NASA’s Commercial Resupply Services (CRS) contract.

SpaceX is under contract to NASA to deliver 20,000 kg (44,000 pounds) of cargo to the ISS during a dozen Dragon cargo spacecraft flights over the next few years at a cost of about $1.6 Billion.

To date SpaceX has completed two operational cargo resupply missions and a test flight. The last flight dubbed CRS-2 blasted off a year ago on March 1, 2013 atop the initial version of the Falcon 9 rocket.

Following the rescheduled March 30 launch and a series of orbit raising and course corrections over the next two days, Dragon will rendezvous and dock at the Earth facing port on the station’s Harmony module on Wednesday, April 2.

Falcon 9 SpaceX CRS-2 launch of Dragon spacecraft on March 1, 2013 to the ISS from pad 40 at Cape Canaveral, Florida.- shot from the roof of the Vehicle Assembly Building. During 2014, SpaceX plans two flight tests simulating Dragon emergency abort scenarios launching from pad 40. Credit: Ken Kremer/www.kenkremer.com — Falcon 9 SpaceX CRS-2 launch of Dragon spacecraft on March 1, 2013 to the ISS from pad 40 at Cape Canaveral, Florida.- shot from the roof of the Vehicle Assembly Building. Credit: Ken Kremer/www.kenkremer.com

Stay tuned here for Ken’s continuing SpaceX, Orbital Sciences, commercial space, Orion, Chang’e-3, LADEE, Mars rover, MAVEN, MOM and more planetary and human spaceflight news.

Learn more at Ken’s upcoming presentations at the NEAF astro/space convention on April 12/13 and at Washington Crossing State Park, NJ on April 6. Also evenings at the Quality Inn Kennedy Space Center, Titusville, FL, March 24/25 and March 29/30
.

And watch for Ken’s upcoming SpaceX launch coverage at Cape Canaveral & the Kennedy Space Center press site.

Ken Kremer

March 21, 2014December 29, 2015 by Fraser Cain

Weekly Space Hangout – March 21, 2014: Cosmos & Gravitational Waves!

Host: Fraser Cain
Guests: Matthew Francis, Nicole Gugliucci, Brian Koberlein, Morgan Rehnberg, Mike Simmons
Continue reading “Weekly Space Hangout – March 21, 2014: Cosmos & Gravitational Waves!”