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Showing posts with label Sci-Tech. Show all posts
Showing posts with label Sci-Tech. Show all posts

Mar 28, 2016

[CA] Highest Peak in Saturn

Scientists working on NASA’s Cassini mission have identified the highest point on Saturn’s largest moon Titan. Titan’s highest peak is 10, 948 feet high. It is found within a trio of mountainous ridges called the Mithrim Montes.
About Cassini Mission:
·       Cassini–Huygens is an unmanned spacecraft sent to the planet Saturn. Cassini is the fourth space probe to visit Saturn and the first to enter orbit.
·       Its design includes a Saturn orbiter and a lander for the moon Titan. The lander, called Huygens, landed on Titan in 2005. The spacecraft was launched on October 15, 1997. This was the first landing ever accomplished in the outer Solar System.

Objectives:
·       Determine the three-dimensional structure and dynamic behavior of the rings of Saturn.
·       Determine the composition of the satellite surfaces and the geological history of each object.
·       Determine the nature and origin of the dark material on Iapetus’s leading hemisphere.
·       Measure the three-dimensional structure and dynamic behavior of the magnetosphere.
·       Study the dynamic behavior of Saturn’s atmosphere at cloud level.
·       Study the time variability of Titan’s clouds and hazes.
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Jan 6, 2016

[CA - Notes] IUPAC adds new 4 elements

IUPAC announced addition of Four Elements to complete Seventh row of Periodic Table

The International Union of Pure and Applied Chemistry (IUPAC) announced discovery and assignment of elements with atomic numbers 113, 115, 117 and 118. The decision was taken by the IUPAC as the four elements met the discovery of elements of the IUPAP/IUPAC Transfermium Working Group (TWG) 1991 Discovery Criteria.
All these four elements are synthetic in nature. They were discovered by scientists belonging to the USA, Russian and Japan and complete the 7th row of the periodic table of the elements. Also, these four elements are the first to be added to the table since 2011, when elements 114 (Flerovium, FI) and 116 (Livermorium, LV) were added.



Naming of elements: After officially recognizing the elements, the IUPAC also invited suggestions related to permanent names and symbols from the scientists who discovered them. New elements can be named after a mythological concept, a mineral, a place or country, a property or a scientist.

Details of four elements

Element Number
Temporary Name
Temporary Symbol
Others
113
Ununtrium
Uut
Discovered by the scientists belonging to RIKEN research laboratory in Japan
115
Ununpentium
Uup
Discovered by scientists belonging to Russia and the USA in collaboration. In element 117, Indian scientist Susanta Lahiri played an important role
117
Unnseptium
Uus
118
Ununoctium
Uuo
Jointly discovered by scientists belonging to the Nuclear Research in Dubna, Russia and Lawrence Livermore National Laboratory, California, USA

How they were discovered?
They were discovered by slamming lighter ­nuclei into each other and tracking the following decay of the radioactive superheavy elements. Like other superheavy elements that populate the end of the periodic table, they only exist for fractions of a second before decaying into other elements.
About IUPAC
Ø It is an association of bodies, National Adhering Organizations, which represent the chemists of different member countries.
Ø It was formed in 1919 by chemists from industry and academia and headquartered in Zurich, Switzerland.
Ø It serves to advance the worldwide aspects of the chemical sciences and to contribute to the application of chemistry in the service of mankind.

Ø Over nearly eight decades, it has succeeded in fostering worldwide communications in the chemical sciences and in uniting academic, industrial and public sector chemistry in a common language.

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Jun 26, 2015

[CA] India based Neutrino Observatory (INO): Part 2


Current Affairs

India based Neutrino Observatory (INO) 
Part 2
Part 1
[What is INO? / Nodal agency of INO / Location of INO / What is Neutrino and their types]  CLICK HERE  

Neutrino Oscillation:
·        Neutrinos (Electron / Muon / Tau) can morph from one type or flavour to another as they pass through space, people, matter and the earth itself. This phenomenon is called as Neutrino Oscillation.
·        While the details of two oscillations – the electron type to the muon type and muon type to tau type are known fairly well, the third, the switching of the tau type to electron type is not well characterised and forms one of the main objectives of the INO

Why is Neutrino study important?
·        Since Neutrinos are abound in the universe, even their tiny masses can have an effect on the evolution of the universe through their gravitational effects.
·        Thus, neutrinos hold the key to fundamental questions on the origin of the universe and energy production in stars.
·        INO is an experimental project in basic sciences seeking to expand our knowledge horizon.
·        Scientists firmly says that, INO has nothing to do with radioactivity or any other dangerous nuclear activity, nor does it have any defence or strategic objectives

History of INO:
·        India was at the forefront of neutrino research in the 1960s. One of the earliest laboratories established to detect neutrinos in the world was located more than 2 km deep at the Kolar Gold Field mines in Karnataka. It was at this laboratory that the atmospheric neutrinos were first detected in 1965. Unfortunately, this laboratory had to be shut down with the closure of the mines in the 1990s.
·        The INO was proposed in 2000 at an international conference in Chennai. The proposal was further refined and consolidated at the 2001 neutrino meeting in Chennai, when the INO consortium of collaborating Indian institutions was formed.

Oct 18, 2010
Ministry of Environment & Forests approved both environment and forest clearance for setting up the observatory in the Bodi West Hills Reserved Forest in the Theni district of Tamil Nadu
Feb 2012
The land was allocated to the INO collaboration by the government of Tamil Nadu and the excavation work was about to start.
Naba K Mondal, chief spokesperson of INO project and a senior scientist at the Tata Institute of Fundamental Research, Mumbai, told that the pre-project work will start in April 2012 and Rs. 66 crores has been sanctioned for the work.
The first task will be to have a road connectivity from Rasingapuram to Pottipuram village.
The project is expected to be completed in 2015 at an estimated cost of Rs 1,500 crores.
Sep 18, 2012
Kerala’s octogenarian Opposition leader and CPI(M) central committee member VS Achuthanandan expressed anxiety over establishing a neutrino observatory on the Theni-Idukki border between Tamil Nadu and Kerala, citing environmental and radiological issues.
Soon the INO collaboration clarified on all the issues raised by him and the responses are on the INO website.
Jan 05, 2015
Union Cabinet headed by Prime Minister Narendra Modi approved to set up the India-based Neutrino Observatory (INO)
Feb 20, 2015
The southern bench of National Green Tribunal ordered notices to the central and state governments on a petition challenging the environmental clearance granted to the India-based Neutrino Observatory (INO) project.
Mar 26, 2015
The Madurai bench of the Madras high court restrained the central government from commencing the work on the proposed India-based Neutrino Observatory (INO).The court directed the government to get permission from the Tamil Nadu Pollution Control Board (TNPCB) before commencing the work.


Why Bodi Hills chosen as site for INO?:
·        Bodi Hills was chosen as a suitable site for locating the underground detector as the steep slopes of the Western Ghats provide ideal and stable rock conditions to build a large underground cavern for long-term use
·        The main detector, which will detect both natural and man-made neutrinos, is an indigenously built 50 kiloton magnetized iron calorimeter (ICAL) detector.
·        It will be world’s most massive neutrino detector. This will be located in a cavern 1.3 km below the mountain peak so that there is a material overburdern of about 1200 metres in all directions to filter out cosmic rays

2 Phases of INO:
·        Phase I: INO will study neutrinos produced by cosmic rays in the earth’s atmosphere
·        Phase II: will be at least 10-15 years down the line, the INO could be used as a far detector for using beams from future accelerator – based ‘neutrino factories’ in Japan, Europe and USA in what is called as Long Baseline Neutrino Experiment (LBNE)

Neutrino Factories:
·        Unlike the sporadic neutrinos flying in all directions that a particle accelerator normally produces, a neutrino factory will create a focused beam of neutrinos at one site on the earth and fire it downwards until the beams resurface at other points.



TN political parties oppose:
·        The campaigners against the INO project have projected the proposed facility variously as a nuclear weapon facility.
·        Also they says it is a facility being built at the behest of Fermilab ( a US based particle accelerator facility, which has proposed to build a neutrino factory)
·        MDMK Chief Mr. Vaiko said that, INO is more or less like a hospital undertaking drug trials
·        Petition filed in Madurai Bench of Madras High Court.
·        Scientists argue that: Neutrinos are products of radioactive decays, they themselves are not radioactive

China and Neutrino:
·        Only in 2004, two years after India’s proposal did China propose an experiment to study neutrinos from the Daya Bay nuclear reactor using a detector located in an underground tunnel in a nearby hill.
·        In March 2012, that experiment succeeded in measuring a key parameter relating to the tau-neutrino / electron-neutrino oscillation.
·        Scientists believe that, no major science project can take off and succeed in India
  
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Jun 25, 2015

[CA] India based Neutrino Observatory (INO): Part 1

Current Affairs
India based Neutrino Observatory (INO)

What is INO?
·        Mega science project (Rs. 1584 crore by Hindu; Rs. 1350 crore by TIFR) under 12th Five year plan.
·        To setup an underground lab for pure science.
·        INO is the first mega collaborative experimental project to be undertaken in India and could set a precedent for large-scale collaborative efforts in basic sciences
Function on INO
·        INO lab has 50,000 tonnes magnetic detector and an Iron Calorimeter (ICAL) detector.
·        To study neutrinos and particle physics.
·        Later can be used for doing under-ground experiments in pure research in biology, physics and chemistry as well.
Where is INO?
·        Bodi west hills, Theni district, Tamil Nadu
·        When completed, the INO will house the world's most massive magnet, four times larger than the 12,500-tonne magnet in the Compact Muon Solenoid detector at CERN in Geneva, Switzerland
Who owns INO?
·        Jointly funded by the Department of Atomic Energy (DAE) and the Department of Science and Technology (DST)
·        BARC, Tata institute of Fundamental research (TIFR) and dozen other Indian research institutes.
·        26 Indian institutions and 100 scientists are involved in this project with TIFR as the nodal institute



Location factors
·        To detect Neutrino and their reactions, the lab has to be at least 1000 m below surface, to reduce natural cosmic radiation.
·        Mountains of South India, are most ideal for this lab, because they’ve dense rock (mostly gneiss) while the Himalayas are mostly metamorphic sedimentary rock with only pockets of gneiss.
·        Bodi west hills is made up of Charnockite (hardest rock known.) Earthquake risk minimum.

·        Hence better than hills in Karnataka, because they’ve more schistic type rocks, the rocks.



What is Neutrino?
·        Neutrinos are subatomic particles and, like photons and electrons, are one of the fundamental particles of nature
·        Neutrinos are products of radioactive decay
·        Neutrinos are streaming all over the universe in great abundance
·        After Photons, neutrinos are the most abundant particles in the universe
·        Scientists believe that the majority of the neutrinos that are floating around were born around 15 million years ago
·        Neutrinos are also being produced constantly – from terrestrial sources such as nuclear power stations and particle accelerators; in the atmosphere due to interactions of cosmic rays with nuclei resulting in what are called as ‘atmospheric neutrinos’
·        Like Photons, neutrinos do not carry any electric charge
·        Neutrinos have tiny mass (Photos do not have any mass)
·        Among the fundamental particles, neutrinos are a bit strange
·        About 100 trillion neutrinos from the sun and other cosmic sources pass through our bodies every second without us even realizing it
·        Neutrinos are elusive and not easily detected
·        Frederick Reines (in 1956) led the discovery of neutrino
·        Neutrino detectors are usually placed deep underground, typically a kilometer or still deeper. The large overburden of rock or earth above the detectors reduces the background cosmic ray particles by a million times or more.

Types of Neutrinos:
Neutrinos are known to come in three types –
Ø  Electron
Ø  Muon
Ø  Tau
Which of the above neutrino is heaviest? – result is not known; scientists are 'investigating'…

Neutrinos - types
Neutrino
Ve
Charged partner
Electron
Muon
Tau




Part 2
[Why Bodi Hills chosen as site? Neutrino Oscillation / History of INO / TN Political Parties oppose / China and Neutrino]  CLICK HERE 
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