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     2017-02-22

    Russian Progress 66 Launches Cargo to Station

    Posted on February 22, 2017 at 1:14 am by dhuot.
    The Russian 66 Progress launched at 12:58 a.m. Wednesday (11:58 a.m. Baikonur time) from the Baikonur Cosmodrome in Kazakhstan.

    The Russian Progress 66 launched at 12:58 a.m. Wednesday (11:58 a.m. Baikonur time) from the Baikonur Cosmodrome in Kazakhstan.

     

    The unpiloted Russian Progress 66 launched at 12:58 a.m. Wednesday (11:58 a.m. Baikonur time) from the Baikonur Cosmodrome in Kazakhstan. It is now orbiting the planet on course for the International Space Station

    The vehicle will deliver almost three tons of food, fuel and supplies to the Expedition 50 crew.

    The spacecraft is set to dock to the Pirs docking compartment at 3:34 a.m. Friday, Feb. 24. NASA TV coverage of rendezvous and docking will begin at 2:45 a.m. Progress 66 will remain docked at the station for almost four months before departing in June for its deorbit into Earth’s atmosphere.

    This was the first launch of a Progress cargo ship from Baikonur since the Progress 65 supply craft was lost Dec. 1, 2016.

    ترجمه:
     
     
    پیشرفت روسیه راه اندازی 66 باری به ایستگاه
     
    Unpiloted روسی پیشرفت 66 ساعت 12:58 صبح چهارشنبه (ساعت 11:58 صبح پایگاه زمان) از پایگاه فضایی بایکونور در قزاقستان آغاز شد. آن در حال حاضر این سیاره در دوره برای ایستگاه فضایی بین المللی دور است

    خودرو تقریبا سه تن از مواد غذایی و سوخت و تجهیزات به خدمه 50 سفر ارائه کرده است.

    سفینه به اسکله به محفظه متصل کردن Pirs در 3:34 صبح جمعه 24 فوریه تنظیم شده است. تلویزیون ناسا پوشش قرار ملاقات گذاشتن و docking آغاز خواهد شد در ساعت 2:45 صبح پیشرفت 66 در ایستگاه حدود چهار ماه قبل در ماه ژوئن برای خود deorbit به جو زمین ترک شناوراشغال شده،پس باقی خواهد ماند.

    این اولین راه اندازی پیشرفت کشتی باری از پایگاه از پیشرفت 65 هنر و صنعت تامین 1 دسامبر 2016 را از دست داده بود.
     
     
     2017-02-22
     

    NASA & TRAPPIST-1: A Treasure Trove of Planets Found

    Seven Earth-sized planets have been observed by NASA's Spitzer Space Telescope around a tiny, nearby, ultra-cool dwarf star called TRAPPIST-1. Three of these planets are firmly in the habitable zone. Over 21 days, NASA's Spitzer Space Telescope measured the drop in light as each planet passed in front of the star. Spitzer was able to identify a total of seven rocky worlds, including three in the habitable zone, where liquid water might be found. The video features interviews with Sean Carey, manager of the Spitzer Science Center, Caltech/IPAC; Nikole Lewis, James Webb Space Telescope project scientist, Space Telescope Science Institute; and Michaël Gillon, principal investigator, TRAPPIST, University of Liege, Belgium. The system has been revealed through observations from NASA's Spitzer Space Telescope and the ground-based TRAPPIST (TRAnsiting Planets and PlanetesImals Small Telescope) telescope, as well as other ground-based observatories. The system was named for the TRAPPIST telescope. NASA's Jet Propulsion Laboratory, Pasadena, California, manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at Caltech in Pasadena. Spacecraft operations are based at Lockheed Martin Space Systems Company, Littleton, Colorado. Data are archived at the Infrared Science Archive housed at Caltech/IPAC. Caltech manages JPL for NASA. For more information about Spitzer, visit
     
    ترجمه:
    ناسا & TRAPPIST 1: گنج از سیارات یافت
    هفت سیاره به اندازه زمین  توسط تلسکوپ فضایی اسپیتزر ناسا اطراف کوچک، نزدیکی ستاره کوتوله های فوق العاده سرد به نام TRAPPIST 1 ديده شد. سه نفر از این سیارات بصورتی پایدار و محکم در منطقه قابل سکونت است. بیش از 21 روز تلسکوپ فضایی اسپیتزر ناسا کاهش نور به عنوان هر یک از سیاره گذشته مقابل ستاره اندازه گیری. اسپیتزر توانست شناسایی مجموع هفت دنیای سنگی شامل سه در منطقه قابل سکونت که در آن آب مایع ممکن است یافت. کلیپ های مصاحبه با کری شان، مدیر مرکز علوم اسپیتزر Caltech/IPAC؛ Nikole لوئیس، دانشمند پروژه تلسکوپ فضایی جیمز وب در مؤسسه علوم تلسکوپ فضایی; و Michaël Gillon، TRAPPIST، محقق اصلی دانشگاه فرودگاه لیژ بلژیک. سیستم از طریق مشاهدات از تلسکوپ فضایی اسپیتزر ناسا و تلسکوپ زمینی TRAPPIST (جابجایی سیارات و PlanetesImals تلسکوپ کوچک) و همچنین رصدخانه های دیگر نشان داده شده است. سیستم برای تلسکوپ TRAPPIST نامیده می شد. آزمایشگاه پیشرانش جت ناسا، پاسادنا کالیفرنیا ماموریت تلسکوپ فضایی اسپیتزر را برای ناسا علوم ماموریت ریاست واشنگتن اداره می کند. عملیات علمی در مرکز علمی اسپیتزر در Caltech در پاسادنا انجام شده است. فضاپیمای عملیات در فضای لاکهید مارتین اساس
     
     
    ============================================================================================================

    Crystal Growth, Earth Science and Tech Demo Research Launching to Orbiting Laboratory

    Terry Virts and Scott Kelly
    NASA astronauts Scott Kelly and Terry Virts work within the Microgravity Science Glovebox during a previous Rodent Research investigation. Rodent Research 4 could provide a more thorough understanding of humans’ inability to grow a lost limb at the wound site and could lead to tissue regeneration efforts in space.
    Credits: NASA
    The SAGE III instrument integrated on the EXPRESS Pallet Adapter
    The SAGE III instrument integrated on the EXPRESS Pallet Adapter (ExPA) after its final sharp edge inspection before its launch on Space X 10. This investigation will measure the stratospheric ozone, aerosols, and other trace gases by locking onto the sun or moon and scanning a thin profile of the atmosphere.
    Credits: NASA
    During Expedition 45, ESA astronaut Andreas Mogensen captured pictures of blue jets
    During Expedition 45, ESA astronaut Andreas Mogensen captured pictures of blue jets, elusive electrical discharges in the upper atmosphere, with the most sensitive camera on the orbiting outpost to look for these brief features
    Credits: ESA/NASA

    The tenth SpaceX cargo resupply launch to the International Space Station, targeted for launch Feb. 18, will deliver investigations that study human health, Earth science and weather patterns. Here are some highlights of the research headed to the orbiting laboratory:

    Crystal growth investigation could improve drug delivery, manufacturing

    Monoclonal antibodies are important for fighting off a wide range of human diseases, including cancers. These antibodies work with the natural immune system to bind to certain molecules to detect, purify and block their growth. The Microgravity Growth of Crystalline Monoclonal Antibodies for Pharmaceutical Applications (CASIS PCG 5) investigation will crystallize a human monoclonal antibody, developed by Merck Research Labs, that is currently undergoing clinical trials for the treatment of immunological disease.

    Preserving these antibodies in crystals allows researchers a glimpse into how the biological molecules are arranged, which can provide new information about how they work in the body. Thus far, Earth-grown crystalline suspensions of monoclonal antibodies have proven to be too low-quality to fully model. With the absence of gravity and convection aboard the station, larger crystals with more pure compositions and structures can grow. 

    The results from this investigation have the potential to improve the way monoclonal antibody treatments are administered on Earth. Crystallizing the antibodies could enable methods for large-scale delivery through injections rather than intravenously, and improve methods for long-term storage.

    Understanding crystal growth in space could benefit researchers on Earth

    Without proteins, the human body would be unable to repair, regulate or protect itself. Crystallizing proteins provides better views of their structure, which helps scientists to better understand how they function. Often times, proteins crystallized in microgravity are of higher quality than those crystallized on Earth. LMM Biophysics 1 explores that phenomena by examining the movement of single protein molecules in microgravity. Once scientists understand how these proteins function, they can be used to design new drugs that interact with the protein in specific ways and fight disease.

    Identifying proteins that benefit from microgravity crystal growth could maximize research efficiency

    Much like LMM Biophysics 1, LMM Biophysics 3 aims to use crystallography to examine molecules that are too small to be seen under a microscope, in order to best predict what types of drugs will interact best with certain kinds of proteins. LMM Biophysics 3 will look specifically into which types of crystals thrive and benefit from growth in microgravity, where Earth’s gravity won’t interfere with their formation. Currently, the success rate is poor for crystals grown even in the best of laboratories. High quality, space-grown crystals could improve research for a wide range of diseases, as well as microgravity-related problems such as radiation damage, bone loss and muscle atrophy.

    X Prize-winning device seeks insight into how deadly bacteria become drug-resistant

    Microgravity accelerates the growth of bacteria, making the space station an ideal environment to conduct a proof-of-concept investigation on the Gene-RADAR® device developed by Nanobiosym. This device is able to accurately detect, in real time and at the point of care, any disease that leaves a genetic fingerprint.

    Nanobiosym Predictive Pathogen Mutation Study (Nanobiosym Genes) will analyze two strains of bacterial mutations aboard the station, providing data that may be helpful in refining models of drug resistance and support the development of better medicines to counteract the resistant strains.

    Microgravity may hold key to scaling up stem cell cultivation for research, treatment

    Stem cells are used in a variety of medical therapies, including the treatment of stroke. Currently, scientists have no way of efficiently expanding the cells, a process that may be accelerated in a microgravity environment.

    During the Microgravity Expanded Stem Cells investigation, crew members will observe cell growth and morphological characteristics in microgravity and analyze gene expression profiles of cells grown on the station. This information will provide insight into how human cancers start and spread, which aids in the development of prevention and treatment plans. Results from this investigation could lead to the treatment of disease and injury in space, as well as provide a way to improve stem cell production for human therapy on Earth.

    Space-based lightning sensor could improve climate monitoring

    Lightning flashes somewhere on Earth about 45 times per second, according to space-borne lightning detection instruments. This investigation continues those observations using a similar sensor aboard the station.

    The Lightning Imaging Sensor (STP-H5 LIS) will measure the amount, rate and energy of lightning as it strikes around the world. Understanding the processes that cause lightning and the connections between lightning and subsequent severe weather events is a key to improving weather predictions and saving life and property. From the vantage of the station, the LIS instrument will sample lightning over a swider geographical area than any previous sensor.

    Raven seeks to save resources with versatile autonomous technologies 

    Future robotic spacecraft will need advanced autopilot systems to help them safely navigate and rendezvous with other objects, as they will be operating thousands of miles from Earth. The Raven (STP-H5 Raven) studies a real-time spacecraft navigation system that provides the eyes and intelligence to see a target and steer toward it safely.

    Raven uses a complex system to image and track the many visiting vehicles that journey to the space station each year. Equipped with three separate sensors and high-performance, reprogrammable avionics that process imagery, Raven’s algorithm converts the collected images into an accurate relative navigation solution between Raven and the other vehicle. Research from Raven can be applied toward unmanned vehicles both on Earth and in space, including potential use for systems in NASA’s future human deep space exploration.

    Understanding Earth’s atmosphere health could inform policy, protection

    The Stratospheric Aerosol and Gas Experiment (SAGE) program is one of NASA’s longest running Earth-observing programs, providing long-term data to help scientists better understand and care for Earth’s atmosphere. SAGE was first operated in 1979 following the Stratospheric Aerosol Measurement (SAM), on the Apollo-Soyuz mission.

    SAGE III will measure stratospheric ozone, aerosols, and other trace gases by locking onto the sun or moon and scanning a thin profile of the atmosphere.

    Understanding these measurements will allow national and international leaders to make informed policy decisions regarding the protection and preservation of Earth’s ozone layer. Ozone in the atmosphere protects Earth’s inhabitants, including humans, plants and animals, from harmful radiation from the sun, which can cause long-term problems such as cataracts, cancer and reduced crop yield.

    Studying tissue regeneration in space could improve injury treatment on Earth

    Only a few animals, such as tadpoles and salamanders, can regrow a lost limb, but the onset of this process exists in all vertebrates. Tissue Regeneration-Bone Defect (Rodent Research-4) a U.S. National Laboratory investigation sponsored by the Center for the Advancement of Science in Space (CASIS) and the U.S. Army Medical Research and Materiel Command, studies what prevents other vertebrates such as rodents and humans from re-growing lost bone and tissue, and how microgravity conditions impact the process. Results will provide a new understanding of the biological reasons behind a human’s inability to grow a lost limb at the wound site, and could lead to new treatment options for the more than 30% of the patient population who do not respond to current options for chronic non-healing wounds.  

    Crew members in orbit often experience reduced bone density and muscle mass, a potential consequence of microgravity-induced stress. Previous research indicates that reduced gravity can promote cell growth, making microgravity a potentially viable environment for tissue regeneration research. This investigation may be able to shed more light on why bone density decreases in microgravity and whether it may be possible to counteract it.

    These investigations will join many others recurring around the clock aboard the station, all benefitting future spaceflight and life on Earth. For more information about the science happening on station, visit International Space Station Research and Technology.

    ترجمه:

    کریستال رشد علوم زمین و فناوری تحقیقات آزمایشی راه اندازی به آزمايشگاه مدار

    Virts تری و کلی اسکات
    فضانوردان ناسا اسکات کلی و Virts تری در میکروگرانشی گلاو باکس علم در طول تحقیقات جوندگان تحقیقات قبلی کار می کنند. جوندگان تحقیقات 4 می درک کاملتری از ناتوانی انسان در رشد اندام از دست داده در محل زخم را فراهم می کند و می تواند منجر به تلاش های بازسازی بافت در فضا.
    اعتبار: ناسا
    یکپارچه ساز سوم سیج در آداپتور پالت اکسپرس
    یکپارچه ساز سوم سیج در اکسپرس پالت آداپتور (ExPA) پس از بازرسی نهایی لبه های تیز خود را قبل از راه اندازی آن در فضای X 10. این تحقیق ازن استراتوسفر ذرات معلق در هوا و گازهای دیگر اثری قفل بر روی خورشید و یا ماه و اسکن مشخصات نازک اتمسفر اندازه گیری خواهد شد.
    اعتبار: ناسا
    در طول سفر 45 فضانورد ESA آندریاس Mogensen اسیر تصاویر جت آبی
    در طول سفر 45 ESA فضانورد Mogensen آندریاس تصاویر جت آبی گریزان ترشحات الکتریکی در جو بالا با حساس ترین دوربین در پایگاه orbiting به دنبال این ویژگی مختصر اسیر
    اطلاعات نمایشی: ESA/ناسا

    دهم SpaceX محموله resupply دسترسی به ایستگاه فضایی بین المللی، هدفمند برای راه اندازی 18 فوریه ارائه تحقیقات است که مطالعه سلامت انسان، علوم زمین و

     
    -------------------==============================================================================------------------------------

    NASA’s Juno Mission to Remain in Current Orbit at Jupiter

    Jupiter's south pole
    NASA’s Juno spacecraft soared directly over Jupiter’s south pole when JunoCam acquired this image on Feb. 2, 2017, from an altitude of about 62,800 miles (101,000 kilometers) above the cloud tops. This image was processed by citizen scientist John Landino. This enhanced color version highlights the bright high clouds and numerous meandering oval storms.
    Credits: NASA/JPL-Caltech/SwRI/MSSS/John Landino

    NASA’s Juno mission to Jupiter, which has been in orbit around the gas giant since July 4, 2016, will remain in its current 53-day orbit for the remainder of the mission. This will allow Juno to accomplish its science goals, while avoiding the risk of a previously-planned engine firing that would have reduced the spacecraft’s orbital period to 14 days.

    “Juno is healthy, its science instruments are fully operational, and the data and images we’ve received are nothing short of amazing,” said Thomas Zurbuchen, associate administrator for NASA’s Science Mission Directorate in Washington. “The decision to forego the burn is the right thing to do – preserving a valuable asset so that Juno can continue its exciting journey of discovery.”

    Juno has successfully orbited Jupiter four times since arriving at the giant planet, with the most recent orbit completed on Feb. 2. Its next close flyby of Jupiter will be March 27.

    The orbital period does not affect the quality of the science collected by Juno on each flyby, since the altitude over Jupiter will be the same at the time of closest approach. In fact, the longer orbit provides new opportunities that allow further exploration of the far reaches of space dominated by Jupiter’s magnetic field, increasing the value of Juno’s research.

    During each orbit, Juno soars low over Jupiter’s cloud tops – as close as about 2,600 miles (4,100 kilometers). During these flybys, Juno probes beneath the obscuring cloud cover and studies Jupiter’s auroras to learn more about the planet's origins, structure, atmosphere and magnetosphere.

    The original Juno flight plan envisioned the spacecraft looping around Jupiter twice in 53-day orbits, then reducing its orbital period to 14 days for the remainder of the mission. However, two helium check valves that are part of the plumbing for the spacecraft’s main engine did not operate as expected when the propulsion system was pressurized in October. Telemetry from the spacecraft indicated that it took several minutes for the valves to open, while it took only a few seconds during past main engine firings.

    “During a thorough review, we looked at multiple scenarios that would place Juno in a shorter-period orbit, but there was concern that another main engine burn could result in a less-than-desirable orbit,” said Rick Nybakken, Juno project manager at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California. “The bottom line is a burn represented a risk to completion of Juno’s science objectives.”

    Juno’s larger 53-day orbit allows for “bonus science” that wasn’t part of the original mission design. Juno will further explore the far reaches of the Jovian magnetosphere – the region of space dominated by Jupiter’s magnetic field – including the far magnetotail, the southern magnetosphere, and the magnetospheric boundary region called the magnetopause. Understanding magnetospheres and how they interact with the solar wind are key science goals of NASA’s Heliophysics Science Division.

    "Another key advantage of the longer orbit is that Juno will spend less time within the strong radiation belts on each orbit,” said Scott Bolton, Juno principal investigator from Southwest Research Institute in San Antonio. “This is significant because radiation has been the main life-limiting factor for Juno.”

    Juno will continue to operate within the current budget plan through July 2018, for a total of 12 science orbits. The team can then propose to extend the mission during the next science review cycle. The review process evaluates proposed mission extensions on the merit and value of previous and anticipated science returns. 

    The Juno science team continues to analyze returns from previous flybys. Revelations include that Jupiter's magnetic fields and aurora are bigger and more powerful than originally thought and that the belts and zones that give the gas giant’s cloud top its distinctive look extend deep into the planet’s interior. Peer-reviewed papers with more in-depth science results from Juno’s first three flybys are expected to be published within the next few months. In addition, the mission's JunoCam – the first interplanetary outreach camera – is now being guided with assistance from the public. People can participate by voting on which features on Jupiter should be imaged during each flyby.

    “Juno is providing spectacular results, and we are rewriting our ideas of how giant planets work,” said Bolton. “The science will be just as spectacular as with our original plan.”

    JPL manages the Juno mission for NASA. The mission’s principal investigator is Scott Bolton at Southwest Research Institute in San Antonio. The Juno mission is part of the New Frontiers Program managed by NASA's Marshall Space Flight Center in Huntsville, Alabama, for the Science Mission Directorate. Lockheed Martin Space Systems, Denver, built the spacecraft. JPL is managed for NASA by Caltech in Pasadena, California.

     
    ترجمه
     
    Jupiter's south pole
    NASA’s Juno spacecraft soared directly over Jupiter’s south pole when JunoCam acquired this image on Feb. 2, 2017, from an altitude of about 62,800 miles (101,000 kilometers) above the cloud tops. This image was processed by citizen scientist John Landino. This enhanced color version highlights the bright high clouds and numerous meandering oval storms.
    Credits: NASA/JPL-Caltech/SwRI/MSSS/John Landino

    NASA’s Juno mission to Jupiter, which has been in orbit around the gas giant since July 4, 2016, will remain in its current 53-day orbit for the remainder of the mission. This will allow Juno to accomplish its science goals, while avoiding the risk of a previously-planned engine firing that would have reduced the spacecraft’s orbital period to 14 days.

    “Juno is healthy, its science instruments are fully operational, and the data and images we’ve received are nothing short of amazing,” said Thomas Zurbuchen, associate administrator for NASA’s Science Mission Directorate in Washington. “The decision to forego the burn is the right thing to do – preserving a valuable asset so that Juno can continue its exciting journey of discovery.”

    Juno has successfully orbited Jupiter four times since arriving at the giant planet, with the most recent orbit completed on Feb. 2. Its next close flyby of Jupiter will be March 27.

    The orbital period does not affect the quality of the science collected by Juno on each flyby, since the altitude over Jupiter will be the same at the time of closest approach. In fact, the longer orbit provides new opportunities that allow further exploration of the far reaches of space dominated by Jupiter’s magnetic field, increasing the value of Juno’s research.

    During each orbit, Juno soars low over Jupiter’s cloud tops – as close as about 2,600 miles (4,100 kilometers). During these flybys, Juno probes beneath the obscuring cloud cover and studies Jupiter’s auroras to learn more about the planet's origins, structure, atmosphere and magnetosphere.

    The original Juno flight plan envisioned the spacecraft looping around Jupiter twice in 53-day orbits, then reducing its orbital period to 14 days for the remainder of the mission. However, two helium check valves that are part of the plumbing for the spacecraft’s main engine did not operate as expected when the propulsion system was pressurized in October. Telemetry from the spacecraft indicated that it took several minutes for the valves to open, while it took only a few seconds during past main engine firings.

    “During a thorough review, we looked at multiple scenarios that would place Juno in a shorter-period orbit, but there was concern that another main engine burn could result in a less-than-desirable orbit,” said Rick Nybakken, Juno project manager at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California. “The bottom line is a burn represented a risk to completion of Juno’s science objectives.”

    Juno’s larger 53-day orbit allows for “bonus science” that wasn’t part of the original mission design. Juno will further explore the far reaches of the Jovian magnetosphere – the region of space dominated by Jupiter’s magnetic field – including the far magnetotail, the southern magnetosphere, and the magnetospheric boundary region called the magnetopause. Understanding magnetospheres and how they interact with the solar wind are key science goals of NASA’s Heliophysics Science Division.

    "Another key advantage of the longer orbit is that Juno will spend less time within the strong radiation belts on each orbit,” said Scott Bolton, Juno principal investigator from Southwest Research Institute in San Antonio. “This is significant because radiation has been the main life-limiting factor for Juno.”

    Juno will continue to operate within the current budget plan through July 2018, for a total of 12 science orbits. The team can then propose to extend the mission during the next science review cycle. The review process evaluates proposed mission extensions on the merit and value of previous and anticipated science returns. 

    The Juno science team continues to analyze returns from previous flybys. Revelations include that Jupiter's magnetic fields and aurora are bigger and more powerful than originally thought and that the belts and zones that give the gas giant’s cloud top its distinctive look extend deep into the planet’s interior. Peer-reviewed papers with more in-depth science results from Juno’s first three flybys are expected to be published within the next few months. In addition, the mission's JunoCam – the first interplanetary outreach camera – is now being guided with assistance from the public. People can participate by voting on which features on Jupiter should be imaged during each flyby.

    “Juno is providing spectacular results, and we are rewriting our ideas of how giant planets work,” said Bolton. “The science will be just as spectacular as with our original plan.”

    JPL manages the Juno mission for NASA. The mission’s principal investigator is Scott Bolton at Southwest Research Institute in San Antonio. The Juno mission is part of the New Frontiers Program managed by NASA's Marshall Space Flight Center in Huntsville, Alabama, for the Science Mission Directorate. Lockheed Martin Space Systems, Denver, built the spacecraft. JPL is managed for NASA by Caltech in Pasadena, California.

     
     
    ترجمه:
     

    جونو ناسا ماموریت به مشتری که در مدار اطراف گاز غول پیکر از 4 ژوئیه 2016 در آن جریان مدار 53 روز باقی مانده از ماموریت باقی می ماند. این جونو برای به انجام رساندن آن اهداف علم در حالی که اجتناب از خطر از پیش برنامه ریزی موتور که شلیک فضاپیما تناوب مداری به 14 روز کاهش می دهد.

    "جونو سالم است، ابزار علم خود به طور کامل عملیاتی است و اطلاعات و تصاویر دریافتی ما هیچ چیزی کوتاهی شگفت انگیز،" توماس Zurbuchen مدیر دیپلم برای ریاست ماموریت علمی ناسا در واشنگتن، گفت. "تصمیم به سوختگی چشم پوشی کار درست انجام – که جونو قادر به ادامه سفر هیجان انگیز خود را کشف می تواند یک دارایی با ارزش حفظ است."

    ===============================================================================================

    JunoCamNASA's OSIRIS-REx Takes Closer Image of Jupiter

     

    black and white jupiter with moons

    During Earth-Trojan asteroid search operations, the PolyCam imager aboard NASA’s OSIRIS-REx spacecraft captured this image of Jupiter (center) and three of its moons, Callisto (left), Io, and Ganymede. The image, which shows the bands of Jupiter, was taken at 3:34 a.m. EST, on Feb. 12, when the spacecraft was 76 million miles (122 million kilometers) from Earth and 418 million miles (673 million kilometers) from Jupiter. PolyCam is OSIRIS-REx’s longest range camera, capable of capturing images of the asteroid Bennu from a distance of two million kilometers.

     

    This image was produced by taking two copies of the same image, adjusting the brightness of Jupiter separately from the significantly dimmer moons, and compositing them back together so that all four objects are visible in the same frame.

    NASA’s Goddard Space Flight Center in Greenbelt, Maryland provides overall mission management, systems engineering and the safety and mission assurance for OSIRIS-REx. Dante Lauretta of the University of Arizona, Tucson, is the principal investigator, and the University of Arizona also leads the science team and the mission’s observation planning and processing. Lockheed Martin Space Systems in Denver built the spacecraft and is providing flight operations. Goddard and KinetX Aerospace are responsible for navigating the OSIRIS-REx spacecraft. OSIRIS-REx is the third mission in NASA’s New Frontiers Program. NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the agency’s New Frontiers Program for its Science Mission Directorate in Washington.

     

    ترجمه:

    عملیات جستجو سیارک زمین تروجان ها imager PolyCam داخل فضاپیما اوزیریس رکس ناسا این تصویر مشتری (مرکز) و سه تن از آن ماه Callisto (چپ) یو و Ganymede اسیر. تصویر است که گروههای مشتری را نشان می دهد، در 3:34 صبح به وقت شرق، در 12 فوریه, زمانی که فضاپیمای 76 میلیون مایل (122 میلیون کیلومتر) از زمین و 418 میلیون مایل (673 میلیون کیلومتر) از مشتری بود گرفته شده است. PolyCam اوزیریس رکس طولانی ترین محدوده دوربین, قادر به گرفتن تصاویر از سیارک Bennu از فاصله دو میلیون کیلومتر است.

    این تصویر با در نظر گرفتن دو نسخه از همان تصویر، تنظیم روشنایی مشتری به طور جداگانه از اقمار قابل توجهی دیمر و ترکیب آنها با هم عقب طوری که همه اشیاء در چهار در قاب همان تولید شد.

    مرکز پرواز فضایی گودارد ناسا در Greenbelt مریلند فراهم می کند به طور کلی ماموریت مدیریت سیستم های مهندسی و تضمین ایمنی و ماموریت برای اوزیریس رکس. دانته Lauretta از دانشگاه آریزونا در توسان، محقق اصلی است و دانشگاه آریزونا نیز منجر به تیم علم و مشاهده این ماموریت برنامه ریزی و پردازش. لاکهید مارتین سیستم های فضایی در دنور ساخت سفینه و عملیات پرواز ارائه شده است. گودارد و KinetX هوا و فضا برای مرور هستند

     
     
     
     
     
     
     
     
     
     
     
     
     
     
     
     
     
     
     
     
    Artist's concept of what a
     
     

    NASA-funded Website Lets Public Search for New Nearby Worlds

    NASA is inviting the public to help search for possible undiscovered worlds in the outer reaches of our solar system and in neighboring interstellar space. A new website, called Backyard Worlds: Planet 9, lets everyone participate in the search by viewing brief movies made from images captured by NASA's Wide-field Infrared Survey Explorer (WISE) mission. The movies highlight objects that have gradually moved across the sky.

    ترجمه به فارسی :

    ناسا قادر به دعوت عمومی به کمک جستجو ممکن است جهان ناشناخته می رسد بیرونی منظومه شمسی و فضای میان ستاره ای همسایه است. وب سایت جدید به نام حیاط خلوت جهان: 9 سیاره, اجازه می دهد تا همه در جستجوی با مشاهده فیلم های کوتاه ساخته شده از تصاویر گرفته شده توسط ناسا ماموریت میدان وسیع مادون قرمز بررسی اکسپلورر (حکیم) شرکت می کنند. فیلم برجسته کردن اشیاء است که به تدریج در سراسر آسمان نقل مکان کرد.

    ==================================================================================================================

     

    NASA Selects Proposals for First-Ever Space Technology Research Institutes

    High performance materials and structures are needed for safe and affordable next generation exploration systems.
    High performance materials and structures are needed for safe and affordable next generation exploration systems such as transit vehicles, habitats, and power systems.
    Credits: NASA
    Advanced biological engineering
    Advanced biological engineering techniques are rapidly emerging that can lead to innovative approaches for in situ biological manufacturing techniques using microbes and plants, and provide the means to create sustainable technologies for both future space exploration and terrestrial applications.
    Credits: NASA

    NASA has selected proposals for the creation of two multi-disciplinary, university-led research institutes that will focus on the development of technologies critical to extending human presence deeper into our solar system.

    The new Space Technology Research Institutes (STRIs) created under these proposals will bring together researchers from various disciplines and organizations to collaborate on the advancement of cutting-edge technologies in bio-manufacturing and space infrastructure, with the goal of creating and maximizing Earth-independent, self-sustaining exploration mission capabilities.

    “NASA is establishing STRIs to research and exploit cutting-edge advances in technology with the potential for revolutionary impact on future aerospace capabilities," said Steve Jurczyk, associate administrator for NASA’s Space Technology Mission Directorate in Washington. "These university-led, multi-disciplinary research programs promote the synthesis of science, engineering and other disciplines to achieve specific research objectives with credible expected outcomes within five years. At the same time, these institutes will expand the U.S. talent base in areas of research and development with broader applications beyond aerospace." 

    Each STRI will receive up to $15 million over the five-year period of performance. The selected new institutes are:

    Center for the Utilization of Biological Engineering in Space (CUBES)

    As NASA shifts its focus from low-Earth orbit to deep space missions, the agency is investing in the development of technologies that will allow long-duration mission crews to manufacture the products they need, rather than relying on the current practice of resupply missions from Earth.

    The CUBES institute will advance research into an integrated, multi-function, multi-organism bio-manufacturing system to produce fuel, materials, pharmaceuticals and food. While the research goals of the CUBES institute are to benefit deep-space planetary exploration, these goals also lend themselves to practical Earth-based applications. For example, the emphasis on using carbon dioxide as the base component for materials manufacturing has relevance to carbon dioxide management on Earth.

    The CUBES team is led by Adam Arkin, principal investigator at the University of California, Berkeley, in partnership with Utah State University, the University of California, Davis, Stanford University, and industrial partners Autodesk and Physical Sciences, Inc. 

    Institute for Ultra-Strong Composites by Computational Design (US-COMP)

    Affordable deep space exploration will require transformative materials for the manufacturing of next-generation transit vehicles, habitats, power systems, and other exploration systems. These building materials need to be lighter and stronger than those currently used in even the most advanced systems.

    US-COMP aims to develop and deploy a carbon nanotube-based, ultra-high strength, lightweight aerospace structural material within five years. Success will mean a critical change to the design paradigm for space structures. Through collaboration with industry partners, it is anticipated that advances in laboratories could quickly translate to advances in manufacturing facilities that will yield sufficient amounts of advanced materials for use in NASA missions.

    Results of this research will have broad societal impacts, as well. Rapid development and deployment of the advanced materials created by the institute could support an array of Earthly applications and benefit the U.S. manufacturing sector.

    US-COMP is a multidisciplinary team of 22 faculty members led by Gregory Odegard, principal investigator at the Michigan Technological University, in partnership with Florida State University, University of Utah, Massachusetts Institute of Technology, Florida A&M University, Johns Hopkins University, Georgia Institute of Technology, University of Minnesota, Pennsylvania State University, University of Colorado and Virginia Commonwealth University. Industrial partners include Nanocomp Technologies and Solvay, with the U.S. Air Force Research Lab as a collaborator. 

    These awards are funded by NASA’s Space Technology Mission Directorate, which is responsible for developing the cross-cutting, pioneering, new technologies and capabilities needed by the agency to achieve its current and future missions.

    For more information about STMD, visit:

     

    ترجه به فارسی:

     

    ناسا طرح نخستین فضا از موسسات تحقیقاتی فناوری را انتخاب می کند.

    بالا عملکرد مواد و سازه های امن و مقرون به صرفه بعدی نسل اکتشاف مورد نیاز.
    بالا عملکرد مواد و سازه های امن و مقرون به صرفه بعدی نسل اکتشاف مانند حمل و نقل وسایل نقلیه زیستگاه و تغذیه سیستم های مورد نیاز.
    اعتبار: ناسا
    پیشرفته مهندسی زیستی
    روشهای پیشرفته مهندسی زیستی هستند به سرعت در حال ظهور که می تواند منجر به روش های نوآورانه برای روشهای تولید بیولوژیکی درجا با استفاده از میکروب ها و گیاهان، و وسیله برای ایجاد فن آوری های پایدار برای اکتشاف فضا در آینده و برنامه های زمینی.
    اعتبار: ناسا

    ناسا قادر به انتخاب طرح برای ایجاد دو موسسه تحقیقاتی چند رشته ای، دانشگاه منجر خواهد شد که در توسعه فن آوری های بحرانی گسترش حضور انسان عمیق تر به منظومه شمسی ما است.

    جدید فضای فناوری تحقیقات موسسه (STRIs) ایجاد شده تحت این طرح با هم محققان از رشته ها و سازمان های مختلف برای همکاری در پیشرفت فن آوری لبه برش در زیستی تولید و زیرساخت های فضایی با هدف ایجاد و به حداکثر رساندن قابلیت ماموریت اکتشاف زمین مستقل، خود کفا به ارمغان بیاورد.

    "ناسا STRIs برای پژوهش و بهره برداری از برش لبه پیشرفت در ایجاد است

    ======================================================================================

    NASA's Fermi Sees Gamma Rays from 'Hidden' Solar Flares

    An international science team says NASA's Fermi Gamma-ray Space Telescope has observed high-energy light from solar eruptions located on the far side of the sun, which should block direct light from these events. This apparent paradox is providing solar scientists with a unique tool for exploring how charged particles are accelerated to nearly the speed of light and move across the sun during solar flares.

    "Fermi is seeing gamma rays from the side of the sun we're facing, but the emission is produced by streams of particles blasted out of solar flares on the far side of the sun," said Nicola Omodei, a researcher at Stanford University in California. "These particles must travel some 300,000 miles within about five minutes of the eruption to produce this light."

    Omodei presented the findings on Monday, Jan. 30, at the American Physical Society meeting in Washington, and a paper describing the results will be published online in The Astrophysical Journal on Jan. 31.

     
    On three occasions, NASA's Fermi Gamma-ray Space Telescope has detected gamma rays from solar storms on the far side of the sun, emission the Earth-orbiting satellite shouldn't be able to detect. Particles accelerated by these eruptions somehow reach around to produce a gamma-ray glow on the side of the sun facing Earth and Fermi. Watch to learn more.
    Credits: NASA's Goddard Space Flight Center/Scott Wiessinger, producer

    Fermi has doubled the number of these rare events, called behind-the-limb flares, since it began scanning the sky in 2008. Its Large Area Telescope (LAT) has captured gamma rays with energies reaching 3 billion electron volts, some 30 times greater than the most energetic light previously associated with these "hidden" flares.

    Thanks to NASA's Solar Terrestrial Relations Observatory (STEREO) spacecraft, which were monitoring the solar far side when the eruptions occurred, the Fermi events mark the first time scientists have direct imaging of beyond-the-limb solar flares associated with high-energy gamma rays.

    triptych of satellite solar flare observations
    These solar flares were imaged in extreme ultraviolet light by NASA's STEREO satellites, which at the time were viewing the side of the sun facing away from Earth. All three events launched fast coronal mass ejections (CMEs). Although NASA's Fermi Gamma-ray Space Telescope couldn't see the eruptions directly, it detected high-energy gamma rays from all of them. Scientists think particles accelerated by the CMEs rained onto the Earth-facing side of the sun and produced the gamma rays. The central image was returned by the STEREO A spacecraft, all others are from STEREO B.
    Credits: NASA/STEREO

    "Observations by Fermi's LAT continue to have a significant impact on the solar physics community in their own right, but the addition of STEREO observations provides extremely valuable information of how they mesh with the big picture of solar activity," said Melissa Pesce-Rollins, a researcher at the National Institute of Nuclear Physics in Pisa, Italy, and a co-author of the paper. 

    composite animation of CME as observed by satellites
    Combined images from NASA's Solar Dynamics Observatory (center) and the NASA/ESA Solar and Heliospheric Observatory (red and blue) show an impressive coronal mass ejection departing the far side of the sun on Sept. 1, 2014. This massive cloud raced away at about 5 million mph and likely accelerated particles that later produced gamma rays Fermi detected.
    Credits: NASA/SDO and NASA/ESA/SOHO

    The hidden flares occurred Oct. 11, 2013, and Jan. 6 and Sept. 1, 2014. All three events were associated with fast coronal mass ejections (CMEs), where billion-ton clouds of solar plasma were launched into space. The CME from the most recent event was moving at nearly 5 million miles an hour as it left the sun. Researchers suspect particles accelerated at the leading edge of the CMEs were responsible for the gamma-ray emission.

    Large magnetic field structures can connect the acceleration site with distant part of the solar surface. Because charged particles must remain attached to magnetic field lines, the research team thinks particles accelerated at the CME traveled to the sun's visible side along magnetic field lines connecting both locations. As the particles impacted the surface, they generated gamma-ray emission through a variety of processes. One prominent mechanism is thought to be proton collisions that result in a particle called a pion, which quickly decays into gamma rays.

    In its first eight years, Fermi has detected high-energy emission from more than 40 solar flares. More than half of these are ranked as moderate, or M class, events. In 2012, Fermi caught the highest-energy emission ever detected from the sun during a powerful X-class flare, from which the LAT detected high­energy gamma rays for more than 20 record-setting hours.

    NASA's Fermi Gamma-ray Space Telescope is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy and with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden and the United States.

    For more information on Fermi, visit:

    ترجمه به فارسی:

    فرمی ناسا می بیند اشعه گاما از شعله های خورشیدی 'مخفی'

    تیم علمی می گوید فرمی ناسا اشعه گاما تلسکوپ فضایی تا به مشاهده نور پر انرژی از فوران های خورشیدی قرار گرفته در سمت خورشید باید نور مستقیم از این وقایع را مسدود است. این تناقض آشکار قادر به ارائه خورشیدی دانشمندان با ابزار منحصر به فرد برای کشف چگونه می کنند؛ به نزدیک سرعت نور شتاب و حرکت در سراسر خورشید در شعله های خورشیدی است.

    گفت: نیکولا Omodei محقق دانشگاه استنفورد در کالیفرنیا "فرمی به دیدن اشعه گاما از طرف خورشید با آن مواجه هستیم، اما انتشار توسط جریانهای ذرات لعنتی از شعله های خورشیدی در سمت خورشید تولید می شود". "این ذرات حدود 300000 مایل در حدود پنج دقیقه فوران به تولید نور این سفر باید."

    Omodei ارائه یافته های در دوشنبه, 30 ژانویه در نشست انجمن فیزیک آمریکا در واشنگتن و مقاله توصیف نتایج آنلاین در مجله The Astrophysical در تاریخ 31 ژانویه منتشر خواهد شد.
    در سه تلسکوپ فضایی ناسا فرمی اشعه گاما اشعه گاما از طوفان های خورشیدی در سمت خورشید را شناسایی کرده است، انتشار ماهواره ای زمین به دور باید قادر به تشخیص. ذرات شتاب توسط فوران این نوعی رسیدن به تولید اشعه گاما تب و تاب بودن در حدود

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