NASA's MESSENGER Spacecraft Headed For Mercury Impact

After three and a half years in orbit around Mercury the tiny shriveled and pockmarked orb that boasts temperatures in excess of 650 degrees NASAs MESSENGER mission to our solar systems innermost planet is headed for a controlled late March 2015 surface impact.

The spacecraft is getting closer to the planet than weve ever been which helps our [surface] composition measurements a lot, said David Lawrence, a MESSENGER science team member at Johns Hopkins Universitys Applied Physics Lab (APL). Between now and impact

Until the $450 million MESSENGER, Mercury rarely registered as a blip on most researchers radars. But scientists are now in the process of sorting through a plethora of new data about the planet.

Artists rendering of the MESSENGER spacecraft orbiting Mercury (Credit: Wikipedia)

Mercury is an oddball planet of contradictions, said David Blewett, a MESSENGER science team member also at APL, which NASA contracted to build and operate the mission. It has a huge iron core, but the surface rocks are almost totally bereft of iron. Mercury is the planet closest to the Sun, yet it has a polar cap in the form of ice(s) lurking in the eternal darkness of polar craters.

And although Mercury has no apparent current tectonic or volcanic activity; in its distant past, after formation and cooling; the planet did shrink in a manner not unlike a shriveled orange.

Mercurys surface also has hundreds of surface hollows no deeper than a km, says Lawrence, who notes that they cover the planet. You dont see these hollows on any other planet in the solar system, he said. Theyre not craters and they dont look like volcanoes.

Blewett says they have shapes similar to certain depressions found on the South polar cap of Mars Mars, who points out that as the Sun warms the Red Planets surface, these Martian features form from the transformation of carbon dioxide from ice and into a gaseous state. It appears that a similar process is happening on Mercury, says Blewett, but instead of ice being lost, it is solid rock.

As the planet closest to the Sun, however, Lawrence said he would have expected such volatile elements, like sodium, chlorine and sulfur, to have already been baked off the surface. Yet he notes that surprisingly thats not the case.

But compared to the Moon, Mercury doesnt have a lot of compositional surface variability, said Lawrence. In visible light, Mercury is kind of dark gray, bland and uniform.

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NASA's MESSENGER Spacecraft Headed For Mercury Impact

Astronomy club offers Starfest at Bays Mountain

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September 21st, 2014 2:00 pm by Matthew Lane

KINGSPORT -- Bays Mountain Park's astronomy club is holding its annual StarFest convention next month, featuring keynote speakers, planetarium programs, a solar viewing and the chance to spend the night in the park.

Planetarium Director Adam Thanz said the event is one of the finest astronomy events in the nation.

The 31st annual StarFest will run Oct. 17 to Oct. 19 and the deadline to register for the event is this Friday, Sept. 26. Thanz is reminding people who may want to attend StarFest that no walk-ups will be allowed on the day of the event and people must pre-register and pay by the end of the week.

Registration is $90 per person; full time students and people under 21 the cost is $80. Thanz said the fee includes access to all of the speakers, activities, five meals, the park's public programs (wildlife exhibits, planetarium shows, barge rides and trails), the opportunity to sleep/camp on the park grounds and a commemorative T-shirt.

The theme of this year's event is "Seeing the Sky" with a focus on how people see the sky differently, through art, literature, science and music.

On Friday night, Mark Littmann will present a dramatic reading in the planetarium theater of the play "Little Lessons for Lina" that tells the true story of Caroline Herschel -- the first woman to be a professional astronomer - and her older brother William, who discovered the planet Uranus, infrared radiation, our position in the Milky Way and more.

Littmann is the Hill Chair of Excellence Professorship in Science Writing at the University of Tennessee. He holds a doctorate in English from Northwestern University, has taught astronomy at six universities and written/produced 35 planetarium programs.

On Saturday morning, Littman returns with "Seeing the Sky Through Words," a program on the various writers through the ages and their efforts to describe the sky and celestial bodies -- the craters on the Moon, Saturn and its rings and a total eclipse of the Sun.

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Astronomy club offers Starfest at Bays Mountain

City College professor brings stars to her students

The universe may be mysterious, but Lisa Will can at least make it relatable.

Shes an astronomy and physics professor at San Diego City College, which recently opened a new science building and planetarium.

The Pacific Beach resident is also the resident astronomer at the Reuben H. Fleet Science Center, where she presents monthly Sky Tonight planetarium shows.

Will, 43, was born in Northern California, lived in Arizona while she earned her doctorate from Arizona State and landed in San Diego in 2007. She tells us about her star-filled life.

Q: What inspired you to study astronomy?

A: Star Trek. I vividly remember being around 5 years old and looking up Vulcan in the encyclopedia, expecting to learn more about the planet. Instead I found the Roman god of fire and forge. That led me to looking up other things, like planets and stars, saddened that interstellar space travel and aliens were not, in fact, a part of our reality. But it also set me on a path of learning about astronomy.

Q: Youre also a physics professor. Can you explain, in layman terms, how physics and astronomy work together?

A: Physics is the study of how the things work. In astronomy, we use physics to study how the universe functions. The most amazing thing about physics is how widely applicable it is. For example, the Doppler effect used to track the path of storms is the same physics that describes the redshifts of galaxies, which is how we first learned the universe is expanding. I try to stress that breadth to help my students appreciate physics.

Q: Tell us a bit about City Colleges new planetarium.

A: Due to the generosity of voters who passed Propositions S and N, City College now has a new science building, which first opened for classes in spring 2014. This facility provides the modern classrooms and science laboratories that the hardworking students of City College deserve. As part of this building, an 80-seat Spitz SciDome HD planetarium was included to serve both as the Astronomy 101 lecture hall and a space for public-outreach events.

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City College professor brings stars to her students

Astronomy – Ch. 3: Motion of the Moon (12 of 12) Aristarchus: Distance to the Sun? – Video


Astronomy - Ch. 3: Motion of the Moon (12 of 12) Aristarchus: Distance to the Sun?
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Astronomy - Ch. 3: Motion of the Moon (12 of 12) Aristarchus: Distance to the Sun? - Video

Astronomy – Ch. 3: Motion of the Moon (10 of 12) The Phases of the Moon Explained – Video


Astronomy - Ch. 3: Motion of the Moon (10 of 12) The Phases of the Moon Explained
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Astronomy - Ch. 3: Motion of the Moon (10 of 12) The Phases of the Moon Explained - Video

Astronomy Update: Jupiter's moon has the potential for life

Editors note: With the exception of today, Astronomy Update is published on the third Saturday of the month and provided by the Chippewa Valley Astronomical Society and the L.E. Phillips Planetarium. It is compiled by Lauren Likkel of the UW-Eau Claire physics and astronomy department.

Perhaps one of the most fascinating locales in our solar system is Jupiters moon Europa.

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Astronomy Update: Jupiter's moon has the potential for life

Hunting the Wild Nutrinos

The forbidding Antarctic ice cap has become a new Mecca for astronomers looking to take advantage of the continents many months of darkness and pristine skies. Yet perhaps the most revolutionary astronomy project now under way at the South Pole plans to make use not of its clear views but its surprisingly clear ice.

If they are right, the repercussions would be enormous. Neutrino astronomy could give scientists a view straight to the heart of some of the most violent and energetic processes in the universe, including quasars and active galactic nuclei (distant galaxies believed to be powered by massive black holes), as well as the sources of mysterious gamma ray bursts and perhaps even the universes origin in the Big Bang.

What makes neutrinos such a good subject for astronomy is that unlike visible light or other forms of radiation they zip through the universe virtually unimpeded. Produced as a byproduct of the nuclear fusion that occurs at the heart of every star, they have no electric charge and-as far as anyone can tell so far-no mass. So if astronomers could detect neutrinos and measure their energy levels they could learn more about what goes on in those stars.

Neutrino detection is also important for studying high-energy sources such as active galactic nuclei. The powerful gravitational pull of these objects and the interstellar dust and gas surrounding them prevent most other forms of energy from escaping. It is as if astronomers, even with radio telescopes and instruments that capture other wavelengths of radiation, were viewing them through a dense fog. Researchers expect that Amanda will see through this turbulence to reveal a sky dotted with heretofore unknown sources of intense energy, thus opening a new chapter in astronomy.

The only problem with neutrinos is that the very property that makes them such valuable sources of information also makes them devilishly difficult to detect. The earth is constantly bathed in a flood of neutrinos, yet astronomers have no way of detecting them directly. Instead, they look for evidence that high-energy neutrinos have collided with the atomic nuclei of surrounding matter. When collisions occur, they give off muons-negatively charged particles that are like electrons but have more than 200 times the mass. These muons give off a bluish light called Cherenkov radiation that cascades away from the crash site like waves from the bow of a boat.

Fortunately, the direction of muons aligns closely with the direction of the neutrinos that produced them. So a three-dimensional Cherenkov light detector, such as that provided by Amandas array of detectors buried beneath the South Pole, could not only confirm that high-energy neutrinos passed through, but also identify their trajectory with better than a 1-degree resolution: good enough to pinpoint their sources in the sky.

An early indication of the promise of muon detection came on February 24, 1987, when astronomers at an observatory in Chile spotted a new supernova. At the same time, neutrino detectors in Kamioka, Japan, and Cleveland, Ohio, registered a sudden flurry of activity, confirming that high-energy neutrino showers are associated with violent astronomical events.

Encouraged by these findings, the U.S. Department of Energy funded DUMAND, the Deep Underwater Muon and Neutrino Detector, which attempted to drop detectors into the deep ocean off Hawaii to hunt for neutrinos in December 1993. But technical problems stalled the project, which was eventually canceled last fall.

Another deepwater project is now under construction by European and U.S. scientists in the Mediterranean Sea. Yet, as Amanda scientists point out, the problem all oceanic detectors face is in filtering out the noise of background radiation from radioactive potassium, which is present in small amounts in ocean water, as well as from bioluminescent bacteria and higher organisms, not to mention the dangers to the instruments from currents and storms.

Conversely, Antarctic ice, which is essentially pure freshwater containing no such contaminants, produces virtually no background radiation. Moreover, once detectors are frozen in the ice, they will not be disturbed.

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Hunting the Wild Nutrinos

Astronomy – Ch. 3: Motion of the Moon (4 of 12) Why do we have 3 Types of Solar Eclipses? – Video


Astronomy - Ch. 3: Motion of the Moon (4 of 12) Why do we have 3 Types of Solar Eclipses?
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Astronomy - Ch. 3: Motion of the Moon (4 of 12) Why do we have 3 Types of Solar Eclipses? - Video

Astronomy – Ch. 3: Motion of the Moon (5 of 12) Moon’s Shadow and Different Solar Eclipses – Video


Astronomy - Ch. 3: Motion of the Moon (5 of 12) Moon #39;s Shadow and Different Solar Eclipses
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Astronomy - Ch. 3: Motion of the Moon (5 of 12) Moon's Shadow and Different Solar Eclipses - Video

Astronomy – Ch. 3: Motion of the Moon (9 of 12) Difference Between Sidereal & Synodic Month – Video


Astronomy - Ch. 3: Motion of the Moon (9 of 12) Difference Between Sidereal Synodic Month
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Astronomy - Ch. 3: Motion of the Moon (9 of 12) Difference Between Sidereal & Synodic Month - Video

Astronomy – Ch. 3: Motion of the Moon (11 of 12) Why Do We Only See One Side of the Moon? – Video


Astronomy - Ch. 3: Motion of the Moon (11 of 12) Why Do We Only See One Side of the Moon?
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Astronomy - Ch. 3: Motion of the Moon (11 of 12) Why Do We Only See One Side of the Moon? - Video

Winning images of Astronomy Photographer of the Year revealed

Overall winner was photographer James Woodend who took an image of aurora in Iceland's Vatnajokull Park The judges were also impressed by a rarely seen hybrid solar eclipse, taken by Eugen Kamenew from Germany Another stunning image shows the Horsehead Nebula standing out against a red glow 1500 light-years from Earth Images will be shown in free exhibition in the Royal Observatory's Astronomy Centre in London underFebruary

By Ellie Zolfagharifard for MailOnline

Published: 06:05 EST, 18 September 2014 | Updated: 05:31 EST, 19 September 2014

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From clouds dancing across the Milky Way to a stunning solar eclipse over Kenya, the annual competition showcasing the mysterious depths of our universe has revealed some incredible images.

West Midlands-based photographer James Woodend beat over a thousand amateur and professional photographers from around the world to win the title of Astronomy Photographer of the Year 2014.

As well as securing the 1,500 ($2,440) top prize, his image takes pride of place in the exhibition of winning photographs opening today at the Royal Observatory Greenwich.

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Winning images of Astronomy Photographer of the Year revealed