Oh, Canada! Yes, we can see you from here!

Photo: Lights of Canada. Photo by Reynolds & Dills.

Lights of Canada, seen across Lake Erie from Ohio.

by Jay Reynolds

For years, Suzie Dills has told me about seeing lights across the lake when she walks her dog at night. I always joked that she was making it up (knowing full well that she wasn’t). It wasn’t long before we looked on the map and determined that they were lights from Canada (or Narnia).

Well, I’ve always told her to call me when they are happening, Sunday night (May 5) was the night.

When I arrived at Huntington Beach, I knew exactly where to look, but didn’t really see much. (I know what you may be thinking.) I saw a few lights but not the lights, cars, houses, and small children that she’d planted in my anticipation.

But when I raised my binoculars… “Ole Eagle-Eyes Suzie” was correct!

The horizon was littered with many, many red lights and the occasional building light as well. This easily spanned 30 degrees along the horizon. You could clearly make out the thermal boundary layer above the lights. Video would show the scintillation of the lights.

It was terrific to see this across the lake on such a grand scale!

Those of us old enough to remember antenna TV, Sunday night would have been great fun to pick up signals from Toledo, Detroit, and maybe even Erie, Penn. (only to learn they are watching the same “Lost in Space” I was watching).

Higher up, through the haze, you could see Procyon, Pollux, and Castor taking their final bow of the spring; farewell winter friends, we’ll see you soon enough.

The warmer air temperatures had led us to this optical refraction across Lake Erie the previous two nights. This happens in the spring and autumn when the lake water temperature is radically different than the air temperature! Cold lake temps (43 degrees) and warm air temps (65 degrees) set up a trap/ducting which bends/refracts the light over the horizon. The effect is somewhat similar to a hot summer day when blacktop has that mirror/mirage look to it. The pavement is very hot, the air is much cooler.

The measured distance from Bay Village to Canada is approximately 50 miles. Because of the curvature of the Earth, we are usually limited to approximately 16-20 miles line-of-sight.

Bottom line, science is fun, nature can fool us into thinking “a bridge to Canada would be half the cost we thought,” and Suzie has binocular eyes after all!

Jay Reynolds is the CAA’s Observatory Director, astronomy instructor at CSU, and well-known as a NASA Solar System Ambassador.

Photo: Stars through thin clouds. Photo by Reynolds & Dills.

Stars above, Canada’s lights below.

Photos: Jay Reynolds & Suzie Dills: Canon 400 (Xti) Single shot, 10 sec, ISO 1600, Processing MaxIm D/L

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M42: The Great Orion Nebula

Image: M42: The Great Orion Nebula, by Keven Tag.

M42: The Great Orion Nebula, by Keven Tag.

CAA member Keven Tag shared this lovely image of M42, the Orion Nebula, with us. His techniques and results are pretty advanced. Here’s what he said: “Thought I’d send this along. The skies were fairly clear last night {March 14} and I was able to get a nice shot of M42. This was captured from my Strongsville driveway so considering the amount of light pollution, results aren’t bad. It helps that it’s a nice bright target.” Technical stuff: a light pollution (Astronomik CLS-CCD) filter. Also, I use a modified Canon Rebel XSi which has the two native Canon filters removed. Here are some other details…. This was from a stack of (1600 ISO) Subs: Lights: 5X20, 5X40; Darks: 5X30; Flats: 5X30. Equipment and processing details — Mount: CGEM, Scope: Stellarvue SVR90, Camera: Canon XSi(Honis modified), Filter: Astronomik CLS-CCD, Mount Control: TheSkyX, Camera Control: BackYardEOS, Processing: Deep Sky Stacker.”

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Planck mission results shake cosmology’s basics

Image: Artist's concept: Planck spacecraft. Credit: ESA/NASA

Artist’s concept: Planck spacecraft. Credit: ESA/NASA

WASHINGTON — The Planck space mission has released the most accurate and detailed map ever made of the oldest light in the universe, revealing new information about its age, contents and origins.

The map results suggest the universe is expanding more slowly than scientists thought, and is 13.8 billion years old, 100 million years older than previous estimates. The data also show there is less dark energy and more matter, both normal and dark matter, in the universe than previously known. Dark matter is an invisible substance that only can be seen through the effects of its gravity, while dark energy is pushing our universe apart. The nature of both remains mysterious.

The map, based on the mission’s first 15.5 months of all-sky observations, reveals tiny temperature fluctuations in the cosmic microwave background, ancient light that has traveled for billions of years from the very early universe to reach us. The patterns of light represent the seeds of galaxies and clusters of galaxies we see around us today.

The findings also test theories describing inflation, a dramatic expansion of the universe that occurred immediately after its birth. In far less time than it takes to blink an eye, the universe blew up by 100 trillion trillion times in size. The new map, by showing that matter seems to be distributed randomly, suggests that random processes were at play in the very early universe on minute “quantum” scales. This allows scientists to rule out many complex inflation theories in favor of simple ones.

The newly-estimated expansion rate of the universe, known as Hubble’s constant, is 67.15 plus or minus 1.2 kilometers/second/megaparsec. A megaparsec is roughly 3 million light-years. This is less than prior estimates derived from space telescopes, such as NASA’s Spitzer and Hubble, using a different technique. The new estimate of dark matter content in the universe is 26.8 percent, up from 24 percent, while dark energy falls to 68.3 percent, down from 71.4 percent. Normal matter now is 4.9 percent, up from 4.6 percent.

Planck launched in 2009 and has been scanning the skies ever since, mapping the cosmic microwave background, the afterglow of the theorized big bang that created our universe. Complete results from Planck, which still is scanning the skies, will be released in 2014.

For more information about Planck, visit: http://www.nasa.gov/planck

From a NASA/JPL News Release, 3/21/2013

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“Awesome” PANSTARRS viewed and photographed

Photo: Comet & Moon, by Christopher Christie.

Moon & PANSTARRS by Christopher Christie, March 13, 2013, from Rocky River, Ohio.
Canon EOS Rebel T3: ISO 400, f/4.5, 2.5 sec.

Mid-March saw a good bit of interest in Comet C/2011 L4 (PANSTARRS). As it approached perihelion the comet put on a good show for observers in the Southern Hemisphere. It was known PANSTARRS would, after its close passage to the Sun, become an object for Northerners to admire, perhaps naked-eye, and excitement grew.

Photo: Comet PANSTARRS by Matt Franduto.

Two Trails: Comet PANSTARRS and Airplane, by Matt Franduto.
Sony A500: ISO 400, f/4.5, 4 seconds. March 14, 2013. Brunswick, Ohio.

After its March 10 perihelion, die-hard comet-spotters looked to the west every evening, hoping for an opening in the clouds. Most tries were met with disappointment. Sometimes an opening would appear and the comet would glow forth in the dimming twilight. Then, after the sunset of March 14, it seemed the weather would cooperate. Mostly-clear skies greeted observers and crowds gathered in several places affording views of a distant horizon. One such place was Mapleside Farms, an orchard and restaurant in Brunswick, Ohio. The view from their parking lot is splendid, with the terrain dropping away rapidly to lowland orchards and a miles-wide valley. Astronomer-folk, including a group of CAA members, and the curious stood transfixed watching the western horizon, waiting for the sunset to fade, hoping distant clouds would remain far off.

Comet PANSTARRS by David Nuti.

PANSTARRS over Avon, Ohio, by David Nuti. Nikon D5000: ISO 1600, f/5.6, 4 sec., March 14, 2013.

Eventually, around 8:30 PM, observers began to pick out the comet from Earthly twilight, cloud-streaks, and jet contrails. “Does the comet blink?” someone asked, apparently seeing a far-away aircraft. I don’t know if they were serious. The first to spot and the only viewers to see PANSTARRS did so through binoculars and/or digital cameras. For us, the little comet was just a notch too dim to pick out with the unaided eye. Through binoculars, PANSTARRS had a small and well-defined nucleus and a lovely, cone-shaped, feathered tail. Overall, because of its low elevation, the comet had a golden coloration. Observing time in Brunswick was brief. Not long after first sightings, PANSTARRS began fading in and out as thin bands of clouds floated over the area. “I expected the comet to move faster,” commented one gentleman. Finally, just before 9:00, after only 20 to 30 minutes of visibility, it was gone. Casual visitors who did see PANSTARRS seemed excited. It was probably the first comet they had ever seen and was proclaimed as “awesome!”

Photo: Comet PANSTARRS, by Jay Reynolds.

PANSTARRS over Avon by Jay Reynolds. Canon EOS Digital Rebel XTi: ISO 800, f/2.8, 1 sec., March 14, 2013.

Photo: PANSTARRS & Mars, by Jay Reynolds.

‘STARRS & Mars by Jay Reynolds. The faint dot of the Red Planet may be seen
in some of the photos by other CAA members.

Photo: PANSTARRS by Bruce Lane.

In Dark Skies, Comet PANSTARRS over Avon, by Bruce Lane.
Canon EOS Digital Rebel XT: ISO 800, f/6.3, 1.6 sec., March 14, 2013.

Photo: PANSTARRS by Joe Hamlin.

Comet PANSTARRS over Huntington Park, Bay Village, by Joe Hamlin, March 15, 2013.

Image: Pan-STARRS LogoComet PANSTARRS images shown here were created and shared by CAA members. In many cases we have modified their original efforts a bit to present via this Web site. As a matter of style, we have settled on an all-caps, non-hyphenated form for the name. PANSTARRS is a non-periodic comet discovered in June 2011 using the Pan-STARRS telescope located near the summit of Haleakala, on the island of Maui in Hawaii. Pan-STARRS stands for: Panoramic Survey Telescope and Rapid Response System. Because Pan-STARRS is used in cometary discovery, other comets also bear the program moniker. Wikipedia on Pan-STARRS.

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Curiosity result: Mars could have supported microbial life

PASADENA, Calif. — An analysis of a rock sample collected by NASA’s Curiosity rover shows ancient Mars could have {emphasis added — ed.} supported living microbes.

Scientists identified sulfur, nitrogen, hydrogen, oxygen, phosphorus and carbon — some of the key chemical ingredients for life — in the powder Curiosity drilled out of a sedimentary rock near an ancient stream bed in Gale Crater on the Red Planet last month.

“A fundamental question for this mission is whether Mars could have supported a habitable environment,” said Michael Meyer, lead scientist for NASA’s Mars Exploration Program at the agency’s headquarters in Washington. “From what we know now, the answer is yes.”

Clues to this habitable environment come from data returned by the rover’s Sample Analysis at Mars (SAM) and Chemistry and Mineralogy (CheMin) instruments. The data indicate the Yellowknife Bay area the rover is exploring was the end of an ancient river system or an intermittently wet lake bed that could have provided chemical energy and other favorable conditions for microbes. The rock is made up of a fine-grained mudstone containing clay minerals, sulfate minerals and other chemicals. This ancient wet environment, unlike some others on Mars, was not harshly oxidizing, acidic or extremely salty.

The patch of bedrock where Curiosity drilled for its first sample lies in an ancient network of stream channels descending from the rim of Gale Crater. The bedrock also is fine-grained mudstone and shows evidence of multiple periods of wet conditions, including nodules and veins.

Curiosity’s drill collected the sample at a site just a few hundred yards away from where the rover earlier found an ancient streambed in September 2012.

“Clay minerals make up at least 20 percent of the composition of this sample,” said David Blake, principal investigator for the CheMin instrument at NASA’s Ames Research Center in Moffett Field, Calif.

These clay minerals are a product of the reaction of relatively fresh water with igneous minerals, such as olivine, also present in the sediment. The reaction could have taken place within the sedimentary deposit, during transport of the sediment, or in the source region of the sediment. The presence of calcium sulfate along with the clay suggests the soil is neutral or mildly alkaline.

Scientists were surprised to find a mixture of oxidized, less-oxidized, and even non-oxidized chemicals, providing an energy gradient of the sort many microbes on Earth exploit to live. This partial oxidation was first hinted at when the drill cuttings were revealed to be gray rather than red.

“The range of chemical ingredients we have identified in the sample is impressive, and it suggests pairings such as sulfates and sulfides that indicate a possible chemical energy source for micro-organisms,” said Paul Mahaffy, principal investigator of the SAM suite of instruments at NASA’s Goddard Space Flight Center in Greenbelt, Md.

An additional drilled sample will be used to help confirm these results for several of the trace gases analyzed by the SAM instrument.

“We have characterized a very ancient, but strangely new ‘gray Mars’ where conditions once were favorable for life,” said John Grotzinger, Mars Science Laboratory project scientist at the California Institute of Technology in Pasadena, Calif. “Curiosity is on a mission of discovery and exploration, and as a team we feel there are many more exciting discoveries ahead of us in the months and years to come.”

NASA/JPL News Release

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March comet comes to (low) northern skies

Image: Mid-March sky positions for Comet PANSTARRS. Credit: NASA

For those in search of comet L4 PANSTARRS, look to the west after sunset in early and mid-March. This graphic shows the comet’s expected positions in the sky. Image credit: NASA

Comets visible to the naked eye are a rare delicacy in the celestial smorgasbord of objects in the nighttime sky.  Scientists estimate that the opportunity to see one of these icy dirtballs advertising their cosmic presence so brilliantly they can be seen without the aid of a telescope or binoculars happens only once every five to 10 years.  That said, there may be two naked-eye comets available for your viewing pleasure this year.

“You might have heard of a comet ISON, which may become a spectacular naked-eye comet later this fall,” said Amy Mainzer, the principal investigator of NASA’s NEOWISE mission at the Jet Propulsion Laboratory (JPL) in Pasadena, Calif., and self-described cosmic icy dirtball fan.  ”But if you have the right conditions you don’t have to wait for ISON. Within a few days, comet PANSTARRS will be making its appearance in the skies of the Northern Hemisphere just after twilight.”

Discovered in June 2011, comet 2011 L4 (PANSTARRS) bears the name of the telescopic survey that discovered it — the less than mellifluous sounding “Panoramic Survey Telescope and Rapid Response System” which sits atop the Haleakala volcano in Hawaii.

Since its discovery a year-and-a-half ago, observing comet PANSTARRS has been the exclusive dominion of comet aficionados in the Southern Hemisphere, but that is about to change.  As the comet continues its well-understood and safe passage through the inner solar system, its celestial splendor will be lost to those in the Southern Hemisphere, but found by those up north.

“There is a catch to viewing comet PANSTARRS,” said Mainzer. “This one is not that bright and is going to be low on the western horizon, so you’ll need a relatively unobstructed view to the southwest at twilight and, of course, some good comet-watching weather.”

Well, there is one more issue — the time of day, or night, to view it.

“Look too early and the sky will be too bright,” said Rachel Stevenson, a NASA Postdoctoral Fellow at JPL. “Look too late, the comet will be too low and obstructed by the horizon.  This comet has a relatively small window.”

By March 8, comet PANSTARRS may be viewable for those with a totally unobstructed view of the western horizon for about 15 minutes after twilight.  On March 10, it will make its closest approach to the sun about 28 million miles (45 million kilometers) away. As it continues its nightly trek across the sky, the comet may get lost in the sun’s glare but should return and be visible to the naked eye by March 12. As time marches on in the month of March, the comet will begin to fade away slowly, becoming difficult to view (even with binoculars or small telescopes) by month’s end.  The comet will appear as a bright point of light with its diffuse tail pointing nearly straight up from the horizon like an exclamation point.

What, if any, attraction does seeing a relatively dim naked-eye comet with the naked eye hold for someone who works with them every day, with file after file of high-resolution imagery spilling out on her computer workstation?

“You bet I’m going to go look at it!” said Mainzer. “Comet PANSTARRS may be a little bit of a challenge to find without a pair of binoculars, but there is something intimately satisfying to see it with your own two eyes.  If you have a good viewing spot and good weather, it will be like the Sword of Gryffindor, it should present itself to anyone who is worthy.”

NASA detects, tracks and characterizes asteroids and comets passing relatively close to Earth using both ground- and space-based telescopes. The Near-Earth Object Observations Program, commonly called “Spaceguard,” discovers these objects, characterizes a subset of them, and predicts their paths to determine if any could be potentially hazardous to our planet.

Article courtesy JPL

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February asteroids: A hit and a miss!

NASA Statement, 2/15/2013

New information provided by a worldwide network of sensors has allowed scientists to refine their estimates for the size of the object that entered that atmosphere and disintegrated in the skies over Chelyabinsk, Russia, at 7:20:26 p.m. PST, or 10:20:26 p.m. EST on Feb. 14 (3:20:26 UTC on Feb. 15).

The estimated size of the object, prior to entering Earth’s atmosphere, has been revised upward from 49 feet (15 meters) to 55 feet (17 meters), and its estimated mass has increased from 7,000 to 10,000 tons. Also, the estimate for energy released during the event has increased by 30 kilotons to nearly 500 kilotons of energy released. These new estimates were generated using new data that had been collected by five additional infrasound stations located around the world – the first recording of the event being in Alaska, over 6,500 kilometers away from Chelyabinsk. The infrasound data indicates that the event, from atmospheric entry to the meteor’s airborne disintegration took 32.5 seconds. The calculations using the infrasound data were performed by Peter Brown at the University of Western Ontario, Canada.

“We would expect an event of this magnitude to occur once every 100 years on average,” said Paul Chodas of NASA’s Near-Earth Object Program Office at the Jet Propulsion Laboratory in Pasadena, Calif. “When you have a fireball of this size we would expect a large number of meteorites to reach the surface and in this case there were probably some large ones.”

The trajectory of the Russia meteor was significantly different than the trajectory of the asteroid 2012 DA14, which hours later made its flyby of Earth, making it a completely unrelated object. The Russia meteor is the largest reported since 1908, when a meteor hit Tunguska, Siberia.

20130216-084351.jpg

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