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JPL News - Day in Review

 

DAY IN REVIEW New Clues to Ceres' Bright Spots and Origins Ceres reveals some of its well-kept secrets in two new studies in the journal Nature, thanks to data from NASA's Dawn spacecraft. They include highly anticipated insights about mysterious bright features found all over the dwarf planet's surface. In one study, scientists identify this bright material as a kind of salt. The second study suggests the detection of ammonia-rich clays, raising questions about how Ceres formed. About the Bright Spots Ceres has more than 130 bright areas, and most of them are associated with impact craters. Study authors, led by Andreas Nathues at Max Planck Institute for Solar System Research, Göttingen, Germany, write that the bright material is consistent with a type of magnesium sulfate called hexahydrite. A different type of magnesium sulfate is familiar on Earth as Epsom salt. Nathues and colleagues, using images from Dawn's framing camera, suggest that these salt-rich areas were left behind when water-ice sublimated in the past. Impacts from asteroids would have unearthed the mixture of ice and salt, they say. "The global nature of Ceres' bright spots suggests that this world has a subsurface layer that contains briny water-ice," Nathues said. A New Look at Occator The surface of Ceres, whose average diameter is 584 miles (940 kilometers), is generally dark -- similar in brightness to fresh asphalt -- study authors wrote. The bright patches that pepper the surface represent a large range of brightness, with the brightest areas reflecting about 50 percent of sunlight shining on the area. But there has not been unambiguous detection of water ice on Ceres; higher-resolution data are needed to settle this question. The inner portion of a crater called Occator contains the brightest material on Ceres. Occator itself is 60 miles (90 kilometers) in diameter, and its central pit, covered by this bright material, measures about 6 miles (10 kilometers) wide and 0.3 miles (0.5 kilometers) deep. Dark streaks, possibly fractures, traverse the pit. Remnants of a central peak, which was up to 0.3 miles (0.5 kilometers) high, can also be seen. With its sharp rim and walls, and abundant terraces and landslide deposits, Occator appears to be among the youngest features on Ceres. Dawn mission scientists estimate its age to be about 78 million years old. Study authors write that some views of Occator appear to show a diffuse haze near the surface that fills the floor of the crater. This may be associated with observations of water vapor at Ceres by the Herschel space observatory that were reported in 2014. The haze seems to be present in views during noon, local time, and absent at dawn and dusk, study authors write. This suggests that the phenomenon resembles the activity at the surface of a comet, with water vapor lifting tiny particles of dust and residual ice. Future data and analysis may test this hypothesis and reveal clues about the process causing this activity. "The Dawn science team is still discussing these results and analyzing data to better understand what is happening at Occator," said Chris Russell, principal investigator of the Dawn mission, based at the University of California, Los Angeles. The Importance of Ammonia In the second Nature study, members of the Dawn science team examined the composition of Ceres and found evidence for ammonia-rich clays. They used data from the visible and infrared mapping spectrometer, a device that looks at how various wavelengths of light are reflected by the surface, allowing minerals to be identified. Ammonia ice by itself would evaporate on Ceres today, because the dwarf planet is too warm. However, ammonia molecules could be stable if present in combination with (i.e. chemically bonded to) other minerals. The presence of ammoniated compounds raises the possibility that Ceres did not originate in the main asteroid belt between Mars and Jupiter, where it currently resides, but instead might have formed in the outer solar system. Another idea is that Ceres formed close to its present position, incorporating materials that drifted in from the outer solar system - near the orbit of Neptune, where nitrogen ices are thermally stable. "The presence of ammonia-bearing species suggests that Ceres is composed of material accreted in an environment where ammonia and nitrogen were abundant. Consequently, we think that this material originated in the outer cold solar system," said Maria Cristina De Sanctis, lead author of the study, based at the National Institute of Astrophysics, Rome. In comparing the spectrum of reflected light from Ceres to meteorites, scientists found some similarities. Specifically, they focused on the spectra, or chemical fingerprints, of carbonaceous chondrites, a type of carbon-rich meteorite thought to be relevant analogues for the dwarf planet. But these are not good matches for all wavelengths that the instrument sampled, the team found. In particular, there were distinctive absorption bands, matching mixtures containing ammoniated minerals, associated with wavelengths that can't be observed from Earth-based telescopes. The scientists note another difference is that these carbonaceous chondrites have bulk water contents of 15 to 20 percent, while Ceres' content is as much as 30 percent. "Ceres may have retained more volatiles than these meteorites, or it could have accreted the water from volatile-rich material," De Sanctis said. The study also shows that daytime surface temperatures on Ceres span from minus 136 degrees to minus 28 degrees Fahrenheit (180 to 240 Kelvin). The maximum temperatures were measured in the equatorial region. The temperatures at and near the equator are generally too high to support ice at the surface for a long time, study authors say, but data from Dawn's next orbit will reveal more details. As of this week, Dawn has reached its final orbital altitude at Ceres, about 240 miles (385 kilometers) from the surface of the dwarf planet. In mid-December, Dawn will begin taking observations from this orbit, including images at a resolution of 120 feet (35 meters) per pixel, infrared, gamma ray and neutron spectra, and high-resolution gravity data. Dawn's mission is managed by the Jet Propulsion Laboratory for NASA. 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 ATK Inc., in Dulles, Virginia, designed and built the spacecraft. The German Aerospace Center, Max Planck Institute for Solar System Research, Italian Space Agency and Italian National Astrophysical Institute are international partners on the mission team. For a complete list of mission participants, visit: http://dawn.jpl.nasa.gov/mission More information about Dawn is available at the following sites: http://dawn.jpl.nasa.gov http://www.nasa.gov/dawn

 

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Teacher Workshop This Weekend! Physics of Sound

 

Physics of Sound When: Saturday, Dec. 12, 10 a.m. to 12 p.m. Where: Columbia Memorial Space Center, Downey, California Target Audience: Teachers for grades K-12 Overview:This hands-on workshop illustrates how sound moves through solids, liquids and gases. By teaching students about the physics of sound, you can illustrate why there is no sound in the vacuum of space. Plus, learn how we communicate with spacecraft at the edges of the solar system with NASA's Deep Space Network. Participants are invited to participate in a simulated space mission in the Challenger Learning Center after the workshop from 1 p.m. to 3 p.m. Reserve your spot today! Register online Call (562) 231-1200 during operating hours OR email Reservations@DowneySpaceCenter.org (include your full name, phone number, address and class title) Workshops are FREE for all pre-service and fully credentialed teachers. Pre-registration is required. Participants are required to bring in their teacher or student ID the day of each workshop. Lunch will be provided. This free workshop is offered through the City of Downey Columbia Memorial Space Center, a hands-on learning center dedicated to bringing the wonder and excitement of science and innovation to audiences of all ages and backgrounds, in partnership with NASA/JPL Education. Discover more upcoming educator workshops and events from NASA/JPL Education.

 

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If you choose our pharmacy you get best customer service and most effective medications! View this email in your browser Bet you'll never find better offer. If you tired of buying expensive useless medications try visiting our online pharmacy now! Only in our online drugstore! Also we have - Blood Pressure - Cancer - Stomach - Stop Smoking ... and more than 2.000 positions Only in our online shop! Copyright ©noquieras.com, All rights reserved. Want to change how you receive these emails? You can update your preferences or unsubsc ribe from this list Friday, December 4, 2015 JPL News - Day in Review   DAY IN REVIEW To Jupiter with JunoCam! When NASA's Juno mission arrives at Jupiter on July 4, 2016, new views of the giant planet's swirling clouds will be sent back to Earth, courtesy of its color camera, called JunoCam. But unlike previous space missions, professional scientists will not be the ones producing the processed views, or even choosing which images to capture. Instead, the public will act as a virtual imaging team, participating in key steps of the process, from identifying features of interest to sharing the finished images online. "This is really the public's camera. We are hoping students and whole classrooms will get involved and join our team," said Scott Bolton, Juno principal investigator at the Southwest Research Institute in San Antonio. The Juno team has kicked off the first stage of JunoCam activity with the launch of a new Web platform on the mission's website. Now and throughout the mission, amateur astronomers are invited to submit images of Jupiter from their own telescopes. These views will be the basis for online discussions about which of Jupiter's swirls, bands and spots JunoCam should image as it makes repeated, close passes over the planet. The ground-based views will be essential for identifying and tracking changes in the planet's cloud features as Juno approaches. "In between our close Jupiter flybys, Juno goes far from the planet, and Jupiter will shrink in JunoCam's field of view to a size too small to be useful for choosing which features to capture. So we really are counting on having help from ground-based observers," said Candy Hansen, a member of the Juno science team who leads planning for the camera. Juno will get closer to Jupiter than any previous orbiting spacecraft, giving JunoCam the best close-up views yet of the planet's colorful cloud bands. Every 14 days, the spinning, solar-powered spacecraft will dive past the planet in just a couple of hours, gathering huge amounts of science data, plus about a dozen JunoCam images. At closest approach, Juno will snap photos from only 3,100 miles (5,000 kilometers) above Jupiter's clouds. "JunoCam will capture high-resolution color views of Jupiter's bands, but that's only part of the story," said Diane Brown, Juno program executive at NASA Headquarters in Washington. "We'll also be treated to the first-ever views of Jupiter's north and south poles, which have never been imaged before." Unlike most spacecraft cameras, JunoCam was specially designed to work on a spinning spacecraft. Typically, spacecraft must point very precisely at their subjects while taking a picture to avoid smearing their images. Since Juno rotates twice per minute, the Juno team designed a camera that images several lines of pixels at a time, at the right speed to cancel out the rotation and avoid smear. Previously, the best images of Jupiter were taken by NASA's two Voyager spacecraft, which flew past the planet in 1979. JunoCam's field of view is much wider than that of Voyager's narrow-angle camera. This means every JunoCam image is a kind of panorama, and its highest-resolution images will show wide swaths of clouds. The camera also benefits from decades of technology advancement, making it lighter, less power-hungry and lower in cost. After JunoCam data arrive on Earth, members of the public will process the images to create color pictures. The Juno team successfully tested this approach when JunoCam acquired its first high-resolution views, showing our home planet during the spacecraft's Earth flyby in October 2013. Since the mission's beginnings, JunoCam was intended almost entirely as a public outreach tool, in contrast to the spacecraft's other instruments that will address Juno's core science questions. Juno scientists will ensure JunoCam returns a few great shots of Jupiter's polar regions, but the overwhelming majority of the camera's image targets will be chosen by the public, with the data being processed by them as well. "We want to give people an opportunity to participate with NASA, and public involvement is key to JunoCam's success," said Bolton. "This is citizen science at its best." Information about JunoCam's new features for amateur astronomer engagement is available at: http://www.missionjuno.swri.edu/junocam The JunoCam Web platform will soon add a discussion section to begin identifying features of interest on the planet for JunoCam to image. The Juno mission website, designed and developed by Radical Media since 2011, has been augmented and updated to include new features in addition to the site's interactive JunoCam section. Launched in 2011, the Juno mission uses every known technique to probe beneath the obscuring cloud cover of Jupiter to learn more about the planet's origins, structure, atmosphere and magnetosphere. NASA's Jet Propulsion Laboratory, Pasadena, California, manages the Juno mission for the principal investigator, Scott Bolton, of Southwest Research Institute in San Antonio. Juno is part of NASA's New Frontiers Program, which is managed at NASA's Marshall Space Flight Center in Huntsville, Alabama. Lockheed Martin Space Systems, Denver, built the spacecraft. JPL is a division of the California Institute of Technology, in Pasadena, which manages the laboratory for NASA. For more information about Juno visit: http://www.nasa.gov/juno http://missionjuno.swri.edu   This message was sent to chantybanty1.chanti@blogger.com from: NASA Jet Propulsion Laboratory | jplnewsroom@jpl.nasa.gov | NASA's Jet Propulsion Laboratory | 4800 Oak Grove Dr | Pasadena, CA 91109 Manage Your Subscription Thursday, December 3, 2015 JPL News - Day in Review   DAY IN REVIEW LISA Pathfinder Carries Advanced NASA Thruster Tech The LISA Pathfinder spacecraft is on its way to space, having successfully launched from Kourou, French Guiana (Dec. 3 local time/Dec. 2 PST). › Read the full story NASA Space Telescopes See Magnified Image of Faintest Galaxy from Early Universe Astronomers harnessing the combined power of NASA's Hubble and Spitzer space telescopes have found the faintest object ever seen in the early universe. › Read the full story JPL CubeSat Clean Room: A Factory For Small Spacecraft JPL CubeSat clean room is doing big things for space explorations smallest inhabitants. › Read the full story   This message was sent to chantybanty1.chanti@blogger.com from: NASA Jet Propulsion Laboratory | jplnewsroom@jpl.nasa.gov | NASA's Jet Propulsion Laboratory | 4800 Oak Grove Dr | Pasadena, CA 91109 Manage Your Subscription Tuesday, December 1, 2015 Medications from World reliable sources Buying medications wt our well-known online pharmacy you save your time and money! 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Call the Educator Resource Center at 818-393-5917 to reserve your spot. This free workshop is offered through the NASA/JPL Educator Resource Center, which provides formal and informal educators with NASA resources and materials that support STEM learning. Discover more upcoming educator workshops and events from NASA/JPL Education.     This message was sent to chantybanty1.chanti@blogger.com from: NASA Jet Propulsion Laboratory | jplnewsroom@jpl.nasa.gov | NASA's Jet Propulsion Laboratory | 4800 Oak Grove Dr | Pasadena, CA 91109 Manage Your Subscription Subscribe to: Posts (Atom) Blog Archive ▼  2026 (67) ▼  September (5) Duck Cloth Weight Explained: Ounces, GSM, Numbered... Twill Fabric Weave: Structure, Types, Characterist... Duck Cloth: What It Is, How It Is Woven, and How I... Day in Review: NASA Watches Earth’s Weight, Finds ... 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