Biggest and Hottest (ESA)

After six months, the volcanic eruption in Holuhraun came to an end on Friday. Producing material for spectacular photographs and numerous articles, the eruption sure was thrilling to observe, but its also a relief that its over.

Heres a brief overview of the developments in the past six months:

The eruption in Holuhraun was preceded by a series of earthquakes which began in Brarbunga volcano, which lies under Vatnajkull glacier, on August 16 but gradually moved to the north.

The pattern of earthquakes indicated that magma was channeling its way underground, creating a 50-km long intrusive dike, which ended in the already existing Holuhraun lava field to the north of the glacier.

After a minor eruption which lasted a few hours on August 29, a 1.6-km (1-mile) long fissure opened up on August 31spewing 1,175C (2,150F) hot lava from three craters, Suri, Baugur and Norri, 100 meters into the air.

The lava spread out over the old lava field, flowing onto the sands and into the riverbed of glacial river Jkuls Fjllum, which retreated. Eventually, the new lava field stopped expanding and started thickening, while the edges around the craters grew taller.

The craters later merged and formed a bubbling lava lake. The eruption remained fairly stable until mid-January. One month later it was reported that the eruption was likely in its final days and on February 27 it came to an end, having lasted almost six months, or 181 days.

Notably, volcanologist Haraldur Sigursson predicted in October that the eruption would end on March 4 and was off only by five days.

With the help of his grandson, an engineering student at Reykjavk University, Haraldur based his prediction on a simple math formula calculating the curve of the decreasing subsidence of the Brarbunga caldera and hence reduced pressure of magma. Its the first time in history that the end of a volcanic eruption has been predicted with such accuracy, he says.

Here are a few facts about the eruption:

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Biggest and Hottest (ESA)

Astronomy – Ch. 7: The Solar Sys – Comparative Planetology (10 of 33) Planet Magnetic Field – Video


Astronomy - Ch. 7: The Solar Sys - Comparative Planetology (10 of 33) Planet Magnetic Field
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Astronomy – Ch. 7: The Solar Sys – Comparative Planetology (16 of 33) Planet’s Tilt – Video


Astronomy - Ch. 7: The Solar Sys - Comparative Planetology (16 of 33) Planet #39;s Tilt
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Astronomy - Ch. 7: The Solar Sys - Comparative Planetology (16 of 33) Planet's Tilt - Video

Astronomy – Ch. 7: The Solar Sys – Comparative Planetology (13 of 33) Planet Distance From the Sun – Video


Astronomy - Ch. 7: The Solar Sys - Comparative Planetology (13 of 33) Planet Distance From the Sun
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Astronomy – Ch. 7: The Solar Sys – Comparative Planetology (24 of 33) Chemical Composition 1 – Video


Astronomy - Ch. 7: The Solar Sys - Comparative Planetology (24 of 33) Chemical Composition 1
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New database a tool in groundwater, geothermal discussions

In a dry land with the highest utility rates in the country, conflicts over water and power generation are never far from hand.

Now, residents who want to wade into these sometimes hot waters or simply understand where they live have a new database at their disposal. The University of Hawaii at Manoa this week announced the creation of the Hawaii Groundwater &Geothermal Resource Center, an online clearing house of data on island and state water wells and also the volcanic hotspots where new geothermal ventures could be added to the often controversial existing ones.

Loaded with maps, data, studies and history, the site was designed by the Hawaii Institute for Geophysics and Planetology to help experts track and understand groundwater and how it is being used, and where geothermal potential exists.

The site is also a one-stop for amateurs to come up to speed on the hydrologic and volcanic dynamics of their island, provided they are willing to plow through the data.

Residents can find out how many wells are drilled in their area, or how water quality and salt content varies from region to region, said Donald Thomas, one of the leaders of the database initative and director of The Center for the Study of Active Volcanoes at the University of Hawaii at Hilo.

It will also help us if we can maintain it in operation for an extended period of time to recognize changes in the groundwater supply that may occur from climate change or increasing demand on the resources, Thomas said. If we can better understand the resources, we have a better chance of managing them sustainably.

Nicole Lautze, another researcher spearheading the creation of the resource center, said high levels of public interest in water and geothermal spurred the initiative.

Our goal is to educate individuals and facilitate responsible management of these resources into the future, said Lautze, an assistant researcher at HIGP.

The searchable site is broken into four project areas which are still being developed. One is devoted entirely to research at the Humuula experimental wells in the Saddle area.

The Humuula Groundwater Research project contains online updates, photos and background on two exploratory wells where groundwater was found at unexpectedly high levels in the eastern corner of Pohakuloa Training Area. Hawaii State Water Wells features an interactive map of well sites, with information on depth, ownership and other data. The project digitalizes all water wells on file with the state Commission on Water Resource Management.

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New database a tool in groundwater, geothermal discussions

Astronomy – Ch. 7: The Solar Sys – Comparative Planetology (12 of 33) Planet Albedo – Video


Astronomy - Ch. 7: The Solar Sys - Comparative Planetology (12 of 33) Planet Albedo
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Astronomy – Ch. 7: The Solar Sys – Comparative Planetology (9 of 33) Planet Atomsphere – Video


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Astronomy – Ch. 7: The Solar Sys – Comparative Planetology (3 of 33) Terrestrial vs Gas Planets – Video


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Astronomy – Ch. 7: The Solar Sys – Comparative Planetology (7 of 33) Planet Density – Video


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Astronomy – Ch. 7: The Solar Sys – Comparative Planetology (21 of 33) Planet Escape Velocity – Video


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Astronomy – Ch. 7: The Solar Sys – Comparative Planetology (4 of 33) Basic Orbital Parameters – Video


Astronomy - Ch. 7: The Solar Sys - Comparative Planetology (4 of 33) Basic Orbital Parameters
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Astronomy – Ch. 7: The Solar Sys – Comparative Planetology (6 of 33) Planet Mass – Video


Astronomy - Ch. 7: The Solar Sys - Comparative Planetology (6 of 33) Planet Mass
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Astronomy – Ch. 7: The Solar Sys – Comparative Planetology (8 of 33) Planet Composition – Video


Astronomy - Ch. 7: The Solar Sys - Comparative Planetology (8 of 33) Planet Composition
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Dawn spacecraft captures sharper images of Ceres

February 17, 2015

These two views of Ceres were acquired by NASA's Dawn spacecraft on Feb. 12, 2015, from a distance of about 52,000 miles (83,000 kilometers) as the dwarf planet rotated. The images have been magnified from their original size. (Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA)

Provided by Elizabeth Landau,NASAs Jet Propulsion Laboratory

Craters and mysterious bright spots are beginning to pop out in the latest images of Ceres from NASAs Dawn spacecraft. These images, taken Feb. 12 at a distance of 52,000 miles (83,000 kilometers) from the dwarf planet, pose intriguing questions for the science team to explore as the spacecraft nears its destination.

As we slowly approach the stage, our eyes transfixed on Ceres and her planetary dance, we find she has beguiled us but left us none the wiser, said Chris Russell, principal investigator of the Dawn mission, based at UCLA. We expected to be surprised; we did not expect to be this puzzled.

Dawn will be gently captured into orbit around Ceres on March 6. As the spacecraft delivers better images and other data, the science team will be investigating the nature and composition of the dwarf planet, including the nature of the craters and bright spots that are coming into focus. The latest images, which have a resolution of 4.9 miles (7.8 kilometers) per pixel, represent the sharpest views of Ceres to date.

The spacecraft explored the giant asteroid Vesta for 14 months during 2011 and 2012. Scientists gained numerous insights about the geological history of this body and saw its cratered surface in fine detail. By comparing Vesta and Ceres, they will develop a better understanding of the formation of the solar system.

Dawns mission to Vesta and Ceres is managed by the Jet Propulsion Laboratory for NASAs Science Mission Directorate in Washington. Dawn is a project of the directorates Discovery Program, managed by NASAs Marshall Space Flight Center in Huntsville, Alabama. UCLA is responsible for overall Dawn mission science. Orbital ATK, Inc., of Dulles, Virginia, designed and built the spacecraft. JPL is managed for NASA by the California Institute of Technology in Pasadena. The framing cameras were provided by the Max Planck Institute for Solar System Research, Gottingen, Germany, with significant contributions by the German Aerospace Center (DLR) Institute of Planetary Research, Berlin, and in coordination with the Institute of Computer and Communication Network Engineering, Braunschweig. The visible and infrared mapping spectrometer was provided by the Italian Space Agency and the Italian National Institute for Astrophysics, built by Selex ES, and is managed and operated by the Italian Institute for Space Astrophysics and Planetology, Rome. The gamma ray and neutron detector was built by Los Alamos National Laboratory, New Mexico, and is operated by the Planetary Science Institute, Tucson, Arizona.

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Dawn spacecraft captures sharper images of Ceres

Astronomy – Ch. 7: The Solar Sys – Comparative Planetology (2 of 33) Introduction 2 – Video


Astronomy - Ch. 7: The Solar Sys - Comparative Planetology (2 of 33) Introduction 2
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Weekly Calendar, Feb. 15, 2015

By Staff Saturday, February 14, 2015

Feb. 15

Knights of Columbus Council 13621 pancake breakfast, 7:30 a.m.noon, third Sunday of each month, 790 26 1/2 Road, $5 adults, $3 ages 6-12, younger than 6 free, proceeds benefit the fund for local charities, 260-7664.

Feb. 16

Healing Hearts Cardiac Support Group, 67:30 p.m., Grand Mesa Room, St. Marys Life Center, 2686 Patterson Road, program features exercise plans, stress management and heart physiology with St. Marys cardiac rehab therapists, family members welcome, 298-2769.

Fruita Seniors Food for Thought, 2 p.m., Senior Center at the Fruita Community Center, 324 N. Coulson St., Fruita, in honor of Valentines Day, bring a food you love to share with the group, 858-0360.

Grand Valley Rebekah Lodge No. 40, 7:30 p.m. first and third Monday of each month, Clifton IOOF Hall, 202 Second St., Clifton, 985-4754.

Rainbow for Girls Grand Junction Assembly No. 12, 7 p.m. first and third Monday of each month, Masonic Center, 2400 Consistory Court, 434-4608.

Orchard Mesa Lions Club, 7 p.m. first and third Monday of each month, A Taste of Heaven Catering, 2817 North Ave., 242-0860.

Eagle Riders, 6:30 p.m. third Monday of each month, 243-6454, foe595.com.

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Weekly Calendar, Feb. 15, 2015

planet – definition of planet in English from the Oxford …

noun 1A celestial body moving in an elliptical orbit round a star. Example sentences Kepler showed that a planet moves round the Sun in an elliptical orbit which has the Sun in one of its two foci. Nasa astronomers said they had found the smallest planets yet orbiting stars beyond our Sun. The planets all orbit the Sun in the same direction, with orbital planes inclined slightly to the ecliptic. Get more examples 1.1 (the planet) The earth: no generation has the right to pollute the planet More example sentences The high tax on petrol was put on in the first place to encourage people to use less of something which is polluting the planet. Ten years ago at the Rio earth summit the world accepted the need to manage the planet as a single whole for the whole of the human race. The idea behind the relay is to unite the world and infuse the planet with the Olympic spirit. Get more examples

The planets of the solar system are either gas giantsJupiter, Saturn, Uranus, and Neptuneor smaller rocky bodiesMercury, Venus, Earth, and Mars. Pluto, formerly regarded as the ninth planet, was in 2006 reclassified as a dwarf planet. The minor planets, or asteroids, orbit mainly between the orbits of Mars and Jupiter. Only Earth and Venus have substantial atmospheres

Middle English: from Old French planete, from late Latin planeta, planetes, from Greek plants 'wanderer, planet', from planan 'wander'.

Early Greek astronomers observed certain heavenly bodies moving around the night sky in contrast to the stars, which stayed permanently in a fixed position in relation to one another. This is why they are called planets, from Greek plants wanderer. The Sun and the Moon were once thought of as planets too. Plankton, the term for small and microscopic organisms floating in the sea, comes via German from the related Greek word planktos, wandering or drifting. See also aeroplane

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Teacher Page: Viscosity – Hawai’i NASA Space Grant Consortium

Hawai'i Space Grant Consortium, Hawai'i Institute of Geophysics and Planetology, University of Hawai'i, 1996 Viscosity Teacher Page Purpose

To determine how fluid a liquid really is by measuring its viscosity.

Viscosity is an internal property of a fluid that offers resistance to flow. For example, pushing a spoon with a small force moves it easily through a bowl of water, but the same force moves mashed potatoes very slowly. In fact, one of the major differences between styles of mashed potatoes is the viscosity of the starchy mass: some people like their potatoes running and teeming with milk and butter (they are fans of low-viscosity potatoes), while others like their potatoes drier and stickier, so they almost crack rather than flow (these people are devoted to high-viscosity potatoes).

Viscosity is important in volcanology. The more fluid a magma, the more likely it is to erupt. On the other hand, when more viscous (higher viscosity) lavas do erupt, they usually do so explosively. Viscosity also affects the shapes of lava flows and the mountains they erupt from. The more viscous the magma, the fatter the lava flow. Also, the more viscous the magmas a volcano erupts, the steeper the volcano. Thus, shield volcanoes like we have in Hawai'i have gentle slopes (less than 10 degrees), while stratovolcanoes like the Cascades in the northwestern mainland are much steeper (roughly 25 degrees). As expected, hawaiian volcanoes erupt more fluid lavas (called basalt) than do the Cascade volcanoes, which erupt a lava called andesite.

There are many ways to measure viscosity, including attaching a torque wrench to a paddle and twisting it in a fluid, using a spring to push a rod into a fluid, and seeing how fast a fluid pours through a hole. This exercise uses one of the oldest and easiest ways: we will simply see how fast a sphere falls through a fluid. The faster the sphere falls, the lower the viscosity. This makes sense: if the fluid has a high viscosity it strongly resists flow, so the sphere falls slowly. If the fluid has a low viscosity, it offers less resistance to flow, so the ball falls faster.

The measurement involves determining the velocity of the falling sphere. This is accomplished by dropping each sphere through a measured distance of fluid and measuring how long it takes to traverse the distance. Thus, you know distance and time, so you also know velocity, which is distance/time.

The formula for determining the viscosity is impressive, decorated with Greek letters and a squared term, but simply amounts to multiplying some numbers and then dividing by some others:

delta p = difference in density between the sphere and the liquid

g = acceleration of gravity

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Teacher Page: Viscosity - Hawai'i NASA Space Grant Consortium

Dawn gets closer views of Ceres

NASA on Friday said its Dawn spacecraft, on approach to dwarf planet Ceres, has acquired its latest and closest-yet snapshot of this mysterious world.

After the spacecraft arrives and enters into orbit around the dwarf planet, it will study the intriguing world in great detail. Ceres, with a diameter of 590 miles (950 kilometers), is the largest object in the main asteroid belt, located between Mars and Jupiter.

Dawn's mission to Vesta and Ceres is managed by the Jet Propulsion Laboratory for NASA's Science Mission Directorate in Washington.

Dawn is a project of the directorate's Discovery Program, managed by NASA's Marshall Space Flight Center in Huntsville, Alabama.

UCLA is responsible for overall Dawn mission science. Orbital Sciences Corp. of Dulles, Virginia, designed and built the spacecraft. JPL is managed for NASA by the California Institute of Technology in Pasadena.

The framing cameras were provided by the Max Planck Institute for Solar System Research, Gottingen, Germany, with significant contributions by the German Aerospace Center (DLR) Institute of Planetary Research, Berlin, and in coordination with the Institute of Computer and Communication Network Engineering, Braunschweig.

The visible and infrared mapping spectrometer was provided by the Italian Space Agency and the Italian National Institute for Astrophysics, built by Selex ES, and is managed and operated by the Italian Institute for Space Astrophysics and Planetology, Rome.

The gamma ray and neutron detector was built by Los Alamos National Laboratory, New Mexico, and is operated by the Planetary Science Institute, Tucson, Arizona.

Image Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

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Dawn gets closer views of Ceres