Pillars of light on a cold winter’s night

Photo: A display of ice pillars. Photo by Matt Franduto.

Beautiful ice pillars brighten a frigid night in Northeastern Ohio.

When the air is especially cold and conditions just right, ice crystals form and, suspended in the air, can do amazing things. This night (January 22) tiny plates of ice reflected artificial lights to make a brilliant display of ice pillars. CAA member Matt Franduto witnessed the show and braved single-digit temperatures (~7 degrees F) to record the scene. Ice pillars are often mistaken for auroras (“northern lights”) which are a whole other kind of phenomenon.

Notes: Sony A-500, manual focus, ISO 400, f/4.5, 8 sec., 18mm lens cropped.

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Moon and Jupiter dance on a cold night

Photo: Moon and Jupiter in close conjunction, January 21, 2013. Photo by James Guilford.

Moon and Jupiter in close conjunction, January 21, 2013

Despite the fact it was 9 degrees (F) and just before 11:00 PM, I simply had to go out and try a shot of the Monday night (January 21) close conjunction of the Moon and Jupiter. Skies had cleared and the day’s occasional snows stopped, so I had a good opportunity. I stepped out on to our sidewalk and, tolerating the frigid breeze as long as I could, shot several exposures, bracketing the shutter speed. I only got one or two that were acceptable to me mostly due to focus being off. The image I’m sharing is sharp enough that (in the uncompressed original) even shows hints of Jupiter’s cloud belts, diagonal here in its tiny disk. None of Jove’s moons show due to the short exposure needed to record Earth’s Moon, just hours away from apogee. Pictures done and shared, it was off to slumberland having witnessed a cold celestial dance before bed. — James Guilford

Notes: Single-exposure image — Canon EOS 50D: ISO 400, f/5.6, 1/500 sec., 400mm lens (600mm equiv.), cropped and adjusted in Adobe Photoshop.

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Still “clicking,” Opportunity finishes crater rim “walkabout”

Photo: Path taken by Mars Exploration Rover "Opportunity" NASA/JPL-Caltech/MSSS/NMMNHS

Opportunity’s Path. Image Credit: NASA/JPL-Caltech/MSSS/NMMNHS

SAN FRANCISCO — The latest work assignment for NASA’s long-lived Mars rover Opportunity is a further examination of an area where the robot just completed a walkabout.

“If you are a geologist studying a site like this, one of the first things you do is walk the outcrop, and that’s what we’ve done with Opportunity,” said Steve Squyres, the mission’s principal investigator at Cornell University in Ithaca, N.Y.

Coming up on its ninth anniversary, Opportunity still is a capable robotic explorer. It has been investigating a crater-rim site where observations from orbiting Mars spacecraft detected traces of clay minerals, which form under wet, non-acidic conditions that can be favorable for life. The rover’s current activities were presented at the Fall Meeting of the American Geophysical Union in San Francisco.

The rover team chose this site as a driving destination years earlier. The site is named Matijevic Hill in honor of the late Jacob Matijevic, who led the engineering team for the twin Mars exploration rovers Spirit and Opportunity for several years.

Opportunity drove about 1,160 feet (354 meters) in a counterclockwise circuit around Matijevic Hill in October and November, bringing the total miles driven on the mission to 22 miles (35.4 kilometers). Researchers used the rover to survey the extent of Matijevic Hill outcrops and identify the best places to investigate further.

“We’ve got a list of questions posed by the observations so far,” Squyres said. “We did this walkabout to determine the most efficient use of time to answer the questions. Now we have a good idea what we’re dealing with, and we’re ready to start the detailed work.”

The hill is on the western rim of Endeavour Crater, a bowl 14 miles (22 kilometers) in diameter. An impact from a celestial object dug this crater more than 3 billion years ago, pushing rocks onto the rim from a greater depth than Opportunity reached during its first several years on Mars. Since the impact, those rocks may have been altered by environmental conditions. Sorting out the relative ages of local outcrops is a key to understanding the area’s environmental history.

“Almost nine years into a mission planned to last for three months, Opportunity is fit and ready for driving, robotic-arm operations and communication with Earth,” said the mission’s deputy project scientist, Diana Blaney, of NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, Calif.

Two outcrops of high interest on Matijevic Hill are “Whitewater Lake” and “Kirkwood.” Whitewater Lake is light-toned material that science team members believe may contain clay. Kirkwood contains small spheres with composition, structure and distribution that differ from other iron-rich spherules, nicknamed blueberries, that Opportunity found at its landing site and throughout the Meridiani Planum area it has explored. Squyres calls the Kirkwood spheres “newberries.”

“We don’t know yet whether Whitewood Lake and Kirkland are from before or after the crater formed,” he said. “One of the most important things to work out is the order and position of the rock layers to tell us the relative ages. We also need more work on the composition of Whitewater and debris shed by Whitewater to understand the clay signature seen from orbit, and on the composition of the newberries to understand how they formed.”

NASA launched Spirit and Opportunity in 2003. Both completed their three-month prime missions in April 2004 with Spirit ceasing operations in 2010. The mission’s goal is to learn about the history of wet environments on ancient Mars. JPL manages the Mars Exploration Rover Project for NASA’s Science Mission Directorate at NASA Headquarters in Washington.

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NASA Technology Days coming to Cleveland

WASHINGTON — Business leaders, space enthusiasts, students and the public are invited to attend NASA Technology Days. The free, three-day public technology showcase will take place at the Cleveland Public Auditorium and Conference Center Nov. 28-30. Participants from industry, academia and the U.S. Government will discuss strategy development, partnerships and methods to foster technology transfer and innovation.

The showcase will feature NASA-funded technologies available for transfer to the aerospace, advanced-energy, automotive, innovative manufacturing and human-health industries. The venue will provide opportunities for networking, business development and forging new relationships, including dialogue with NASA technology program leadership.

NASA officials will discuss the agency’s upcoming technology initiatives, technology transfer and strategic partnerships. NASA centers also will provide exhibits and information on how businesses can partner with the agency for technology development, transfer and innovation. Attendees also can learn about leading technologies contributing to American economic growth and innovation.

NASA Technology Days is free and open to the public, but registration is required. To register, visit:

http://www.aiaa.org/nasatechdays

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Space station spotting service announced

Photo: Arc of the International Space Station passing through the Big Dipper. Credit: Chris Christie.

The ISS passed through the “Big Dipper” August 23, 2012. Photo by Chris Christie.

WASHINGTON — On the 12th anniversary of crews continuously living and working aboard the International Space Station, NASA announced a new service to help people see the orbiting laboratory when it passes overhead. “Spot the Station” will send an email or text message to those who sign up for the service a few hours before they will be able to see the space station.

Nov. 2 marked 12 years of continuous human habitation of the space station.

“It’s really remarkable to see the space station fly overhead and to realize humans built an orbital complex that can be spotted from Earth by almost anyone looking up at just the right moment,” said William Gerstenmaier, NASA’s associate administrator for human exploration and operations. “We’re accomplishing science on the space station that is helping to improve life on Earth and paving the way for future exploration of deep space.”

When the space station is visible — typically at dawn and dusk — it is the brightest object in the night sky, other than the moon. On a clear night, the station is visible as a fast moving point of light, similar in size and brightness to the planet Venus. “Spot the Station” users will have the options to receive alerts about morning, evening or both types of sightings.

The International Space Station’s trajectory passes over more than 90 percent of Earth’s population. The service is designed to only notify users of passes that are high enough in the sky to be easily visible over trees, buildings and other objects on the horizon. NASA’s Johnson Space Center calculates the sighting information several times a week for more than 4,600 locations worldwide, all of which are available on “Spot the Station.”

To sign up for “Spot the Station,” visit:
http://spotthestation.nasa.gov

For information about the International Space Station and a full list of sightings, visit:
http://www.nasa.gov/station

Source: NASA Press Release

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Phenominal new view of our galaxy’s core

Photo: Central bulge of the Milky Way Galaxy. ESO/VVV Consortium Acknowledgement: Ignacio Toledo, Martin Kornmesser

Central portion of the Milky Way: ESO/VVV Consortium – Acknowledgement: Ignacio Toledo, Martin Kornmesser

Using a whopping nine-gigapixel image from the VISTA infrared survey telescope at ESO’s Paranal Observatory, an international team of astronomers has created a catalogue of more than 84 million stars in the central parts of the Milky Way. This gigantic dataset contains more than ten times more more stars than previous studies and is a major step forward for the understanding of our home galaxy. The image gives viewers an incredible, zoomable view of the central part of our galaxy. It is so large that, if printed with the resolution of a typical book, it would be 9 meters long and 7 meters tall.

“By observing in detail the myriads of stars surrounding the centre of the Milky Way we can learn a lot more about the formation and evolution of not only our galaxy, but also spiral galaxies in general,” explains Roberto Saito (Pontificia Universidad Católica de Chile, Universidad de Valparaíso and The Milky Way Millennium Nucleus, Chile), lead author of the study.

Most spiral galaxies, including our home galaxy the Milky Way, have a large concentration of ancient stars surrounding the centre that astronomers call the bulge. Understanding the formation and evolution of the Milky Way’s bulge is vital for understanding the galaxy as a whole. However, obtaining detailed observations of this region is not an easy task.
“Observations of the bulge of the Milky Way are very hard because it is obscured by dust,” says Dante Minniti (Pontificia Universidad Catolica de Chile, Chile), co-author of the study. “To peer into the heart of the galaxy, we need to observe in infrared light, which is less affected by the dust.”

Photo: Center of the Milky Way with VISTA region indicated. ESO/Nick Risinger (skysurvey.org)

Central portion of the Milky Way with VISTA region indicated. ESO/Nick Risinger (skysurvey.org)

The large mirror, wide field of view and very sensitive infrared detectors of ESO’s 4.1-meter Visible and Infrared Survey Telescope for Astronomy (VISTA) make it by far the best tool for this job. The team of astronomers is using data from the VISTA Variables in the Via Lactea program (VVV), one of six public surveys carried out with VISTA. The data have been used to create a monumental 108 200 by 81 500 pixel color image containing nearly nine billion pixels. This is one of the biggest astronomical images ever produced. The team has now used these data to compile the largest catalogue of the central concentration of stars in the Milky Way ever created.

To help analyze this huge catalog the brightness of each star is plotted against its color for about 84 million stars to create a color–magnitude diagram. This plot contains more than ten times more stars than any previous study and it is the first time that this has been done for the entire bulge. Color–magnitude diagrams are very valuable tools that are often used by astronomers to study the different physical properties of stars such as their temperatures, masses and ages.

“Each star occupies a particular spot in this diagram at any moment during its lifetime. Where it falls depends on how bright it is and how hot it is. Since the new data gives us a snapshot of all the stars in one go, we can now make a census of all the stars in this part of the Milky Way,” explains Dante Minniti.

The new color–magnitude diagram of the bulge contains a treasure trove of information about the structure and content of the Milky Way. One interesting result revealed in the new data is the large number of faint red dwarf stars. These are prime candidates around which to search for small exoplanets using the transit method.

“One of the other great things about the VVV survey is that it’s one of the ESO VISTA public surveys. This means that we’re making all the data publicly available through the ESO data archive, so we expect many other exciting results to come out of this great resource,” concludes Roberto Saito. For access to much larger versions of these images, visit the ESO Web site.

Source: ESO News Release

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Earth-sized planet discovered in Alpha Centauri system

European astronomers have discovered a planet with about the mass of the Earth orbiting a star in the Alpha Centauri system — the nearest to Earth. It is also the lightest exoplanet ever discovered around a star like the Sun. The planet was detected using the HARPS instrument on the 3.6-metre telescope at ESO’s La Silla Observatory in Chile. The results appeared online in the journal Nature on October 17, 2012.

Alpha Centauri is one of the brightest stars in the southern skies and is the nearest stellar system to our Solar System — only 4.3 light-years away. It is actually a triple star — a system consisting of two stars similar to the Sun orbiting close to each other, designated Alpha Centauri A and B, and a more distant and faint red component known as Proxima Centauri. Since the 19th century astronomers have speculated about planets orbiting these bodies, the closest possible abodes for life beyond the Solar System, but searches of increasing precision had revealed nothing. Until now.

“Our observations extended over more than four years using the HARPS instrument and have revealed a tiny, but real, signal from a planet orbiting Alpha Centauri B every 3.2 days,” says Xavier Dumusque (Geneva Observatory, Switzerland and Centro de Astrofisica da Universidade do Porto, Portugal), lead author of the paper. “It’s an extraordinary discovery and it has pushed our technique to the limit!”

The European team detected the planet by picking up the tiny wobbles in the motion of the star Alpha Centauri B created by the gravitational pull of the orbiting planet. The effect is minute — it causes the star to move back and forth by no more than 51 centimetres per second (1.8 km/hour), about the speed of a baby crawling. This is the highest precision ever achieved using this method.

Alpha Centauri B is very similar to the Sun but slightly smaller and less bright. The newly discovered planet, with a mass of a little more than that of the Earth, is orbiting about six million kilometres away from the star, much closer than Mercury is to the Sun in the Solar System. The orbit of the other bright component of the double star, Alpha Centauri A, keeps it hundreds of times further away, but it would still be a very brilliant object in the planet’s skies.

The first exoplanet around a Sun-like star was found by the same team back in 1995 and since then there have been more than 800 confirmed discoveries, but most are much bigger than the Earth, and many are as big as Jupiter. The challenge astronomers now face is to detect and characterise a planet of mass comparable to the Earth that is orbiting in the habitable zone around another star. The first step has now been taken.

“This is the first planet with a mass similar to Earth ever found around a star like the Sun. Its orbit is very close to its star and it must be much too hot for life as we know it,” adds Stéphane Udry (Geneva Observatory), a co-author of the paper and member of the team, “but it may well be just one planet in a system of several. Our other HARPS results, and new findings from Kepler, both show clearly that the majority of low-mass planets are found in such systems.”

Source: European Southern Observatory

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