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GS Paper: GS3-17.Awareness in the fields of IT, Space, Computers, Robotics, Nano-technology, Bio-technology and issues relating to Intellectual Property Rights.

  • NASA-ISRO Synthetic Aperture Radar

    The NASA-ISRO Synthetic Aperture Radar satellite, aimed at making global measurement of land surface changes using advanced radar imaging, is proposed to be launched in early 2023, informed Earth Sciences Minister.

    Note the key features of the Mission. Every statement has a unique information.

    NASA-ISRO SAR

    • NISAR is a joint collaboration for a dual-frequency L and S-band SAR for earth observation.
    • NASA and Bengaluru-headquartered ISRO signed a partnership on September 30, 2014, to collaborate on and launch NISAR.
    • The mission is targeted to launch in early 2022 from ISRO’s Sriharikota spaceport in Andhra Pradesh’s Nellore district, about 100km north of Chennai.
    • It is capable of producing extremely high-resolution images for a joint earth observation satellite mission with NASA.
    • It will be the first satellite mission to use two different radar frequencies (L-band and S-band) to measure changes in our planet’s surface less than a centimeter across.

    Objectives of the NISAR

    • NISAR will observe Earth’s land and ice-covered surfaces globally with 12-day regularity on ascending and descending passes, sampling Earth on average every six days for a baseline three-year mission.
    • It will measure Earth’s changing ecosystems, dynamic surfaces, and ice masses, providing information about biomass, natural hazards, sea-level rise, and groundwater, and will support a host of other applications.
    • It would also provide data on natural hazards including earthquakes, tsunamis, volcanoes, and landslides.

    What are L and S Bands?

    • L band waves are used for GPS units because they are able to penetrate clouds, fog, rain, storms, and vegetation.
    • The S-band is used by airport surveillance radar for air traffic control, weather radar, surface ship radar, and some communications satellites, especially those used by NASA to communicate with the Space Shuttle and the International Space Station.
    • NISAR uses a sophisticated information-processing technique known as SAR to produce extremely high-resolution images.
    • Radar penetrates clouds and darkness, enabling NISAR to collect data day and night in any weather.

    What is collaboration?

    • NASA is providing the mission’s L-band SAR, a high-rate communication subsystem for science data, GPS receivers, a solid-state recorder, and payload data subsystem.
    • ISRO is providing the spacecraft bus, the S-band radar, the launch vehicle, and associated launch services for the mission, whose goal is to make global measurements of the causes and consequences of land surface changes using advanced radar imaging.
  • Stellar Mid-life Crisis: What ails the middle-aged Sun?

    Stars like our Sun can go through a mid-life crisis, according to new research carried out by scientists from IISER Kolkata.

    Stellar Middle Age

    • At about 4.6 billion years of age, the sun is middle-aged, that is, it will continue to live for roughly the same period.
    • There are accurate methods for estimating the age of the Sun, such as by using radioactive dating of very old meteorites that have fallen on the Earth.
    • However, for more distant stars which are similar in mass and age to the Sun, such methods are not possible.
    • One of the methods used is called gyrochronology.
    • There is a relationship between rotation rate and age, that is the rotation rate of a star slows down with age.

    How does it occur?

    • When the stellar wind escapes from the star, it carries away with it a part of the angular momentum of the star, which results in its slowing down.
    • The stellar wind has two drivers: one is the high temperature of the outer atmosphere of stars – the corona – which results in an outward expansion and hence plasma winds that emanate out.
    • The other is the magnetic field.
    • The magnetic field actually heats the corona and so when magnetic activity is strong the winds are strong and since wind carries away the internal (rotational) angular momentum of the star, it slows down its rotation.
    • This is called magnetic braking.
    • As the star ages, due to this mechanism, its rotation slows down and this relationship is used in gyrochronology to estimate the age of the star.

    Impact

    • This can lead to dramatic changes in their activity and rotation rates.
    • The study also provides an explanation for the breakdown of the long-established relation between rotation rate and age in middle-aged sunlike stars.
    • However, there is a breakdown of the gyrochronology relationship, because, after midlife, a star’s rate of spin does not slow down with age as fast as it was slowing down earlier.
    • Another intriguing fact is that the Sun’s activity level has been observed to be much lower than other stars of similar age.
  • [pib] Near-Surface Shear Layer (NSSL) of Sun

    Indian astronomers have found a theoretical explanation for the existence of the Near-Surface Shear Layer (NSSL) of the Sun for the first time.

    What is a Near-Surface Shear Layer?

    • It was long known the Sun’s equator spins faster than the poles.
    • However, a peek into the internal rotation of the Sun using sound waves revealed the existence of an intriguing layer where the rotation profile of the Sun changes sharply.
    • The layer is called as a near-surface shear layer (NSSL), and it exists very close to the solar surface, where there is an outward decrease in angular velocity.

    What have researchers found?

    • They have used an equation called the thermal wind balance equation to explain how the slight difference in temperature between solar poles and equator, called thermal wind term.
    • It is balanced by the centrifugal force appearing due to solar differential rotation.
    • They have noted that if this condition is true near the solar surface, it can explain the existence of NSSL, which is inferred in helioseismology (technique of using sound waves to peek inside the Sun) based observation.

    Why study NSSL?

    • Understanding NSSL is crucial for the study of several solar phenomena like sunspot formation, solar cycle, and it will also help in understanding such phenomena in other stars.
  • [pib] What are PRIDE Guidelines?

    The Union Ministry for Science & Technology has released “Biotech-PRIDE (Promotion of Research and Innovation through Data Exchange) Guidelines” developed by the Department of Biotechnology (DBT).

    Biotech-PRIDE

    • These guidelines aim at providing a well-defined framework and guiding principle to facilitate and enable sharing and exchange of biological knowledge, information and data.
    • They will facilitate this and enable the exchange of information to promote research and innovation in different research groups across the country.
    • They will be implemented through the Indian Biological Data Centre (IBDC) at Regional Centre for Biotechnology supported by the Department of Biotechnology.

    Creating a national repository: Bio-Grid

    • Other existing datasets/ data centres will be bridged to this IBDC which will be called Bio-Grid.
    • This Bio-Grid will be a National Repository for biological knowledge, information and data.
    • It will be responsible for enabling its exchange, developing measures for safety, standards and quality for datasets and establishing detailed modalities for accessing data.

     Why need such guidelines?

    • India ranks number 4 amongst the top 20 countries contributing biological databases.
    • The Government invests a large number of public funds for biosciences to gain deep insights into intricate biological mechanisms and other processes and for translation.
  • Geo-imaging satellite EOS-03

    Geo-imaging satellite for earth observation EOS-03, which would enable near real-time monitoring of natural disasters like floods and cyclones, is scheduled for launch in the third quarter of 2021.

    EOS-03

    • ISRO has realized a geo-imaging satellite, “EOS-03”, for Earth Observation from Geostationary Orbit.
    • EOS-03 is capable of imaging the whole country four-five times daily and would enable near real-time monitoring of natural disasters like floods and cyclones.
    • In addition to natural disasters, EOS-03 would also enable monitoring of water bodies, crops, vegetation condition, forest cover changes.

    Other developments: Small Satellite Launch Vehicle (SSLV)

    • The first developmental flight of the Small Satellite Launch Vehicle (SSLV) is scheduled for the fourth quarter of 2021 from the Satish Dhawan Space Centre, Sriharikota.
    • The SSLV is a cost-effective, three-stage and all-solid launch vehicle with a payload capability of 500 kg to 500 km planar orbit or 300 kg to Sun-Synchronous Polar Orbit.
    • It is ideal for the on-demand, quick turn-around launch of small satellites.
    • The major technologies developed as part of SSLV are flexible nozzle control with electro-mechanical actuators for all stages, miniaturized avionics, and a velocity trimming module in the upper stage for precise satellite injection.
  • Russia’s Nauka Module for ISS

    Pirs, a Russian module on the International Space Station (ISS) used as a docking port for spacecraft and as a door for cosmonauts to go out on spacewalks. In its place, Russia’s space agency Roscosmos will be attaching a significantly larger module called Nauka.

    What does Russia’s new Nauka module do?

    • Nauka, which is 42 feet long and weighs 20 tonnes, was supposed to be launched as early as 2007, as per the ISS’s original plan.
    • Nauka — meaning “science” in Russian — is the biggest space laboratory Russia has launched to date, and will primarily serve as a research facility.
    • It is also bringing to the ISS another oxygen generator, a spare bed, another toilet, and a robotic cargo crane built by the European Space Agency (ESA).
    • The new module was sent into orbit using a Proton rocket — the most powerful in Russia’s space inventory — on July 21 and will take eight days to reach the ISS.

    What kind of research goes on at the International Space Station?

    • A space station is essentially a large spacecraft that remains in low-earth orbit for extended periods of time.
    • It is like a large laboratory in space and allows astronauts to come aboard and stay for weeks or months to carry out experiments in microgravity.
    • For over 20 years since its launch, humans have continuously lived and carried out scientific investigations on the $150 billion ISS under microgravity conditions, being able to make breakthroughs in research not possible on Earth.

    Back2Basics: International Space Station (ISS)

    • The International Space Station, which launched its first piece in 1998, is a large spacecraft that orbits around the Earth and is home to the astronauts.
    • The ISS is currently the only active space station in the earth’s orbit.
    • The first crew on the space station arrived on November 2, 2000.
    • The space station is home to a minimum of six astronauts, with two bathrooms, a gymnasium, and a big bay window.
    • It is a joint project between five participating space agencies -NASA (USA), Roscosmos (Russia), JAXA (Japan), ESA (Europe), and CSA (Canada).
  • Moon-forming region seen around an exoplanet for the first time

     

    Scientists for the first time have spotted a Moon-forming region around an exo-planet beyond our solar system.

    What are Exoplanets?

    • More than 4,400 planets have been discovered outside our solar system, called exoplanets.
    • Most orbit other stars, but free-floating exoplanets, called rogue planets, orbit the galactic center and are untethered to any star.
    • No circumplanetary discs had been found until now because all the known exoplanets resided in “mature” – fully developed – solar systems, except the two infant gas planets orbiting PDS 70.

    What is the new finding?

    • The researchers have detected a disc of swirling material accumulating around one of two newborn planets.
    • They were seen orbiting a young star called PDS 70, located a relatively close 370 light-years from Earth.
    • It is called a circumplanetary disc, and it is from these those moons are born.
    • The discovery offers a deeper understanding of the formation of planets and moons.

    Focus of the finding: Formation of disc

    • In our solar system, the impressive rings of Saturn, a planet around which more than 80 moons orbit, represent a relic of a primordial moon-forming disc.
    • The orange-colored star PDS 70, roughly the same mass as our Sun, is about 5 million years old– a blink of the eye in cosmic time.
    • The two planets are even younger. Both planets are similar (although larger) to Jupiter, a gas giant.
    • It was around one of the two planets, called PDS 70c, that a Moon-forming disc was observed.

    Observing birth of a moon: Core Accretion

    • Stars burst to life within clouds of interstellar gas and dust scattered throughout galaxies.
    • Leftover material spinning around a new star then coalesces into planets, and circumplanetary discs surrounding some planets similarly yield moons.
    • The dominant mechanism thought to underpin planet formation is called “core accretion”.
    • In this scenario, small dust grains, coated in ice, gradually grow to larger and larger sizes through successive collisions with other grains.
    • This continues until the grains have grown to a size of a planetary core, at which point the young planet has a strong enough gravitational potential to accrete gas which will form its atmosphere.
    • Some nascent planets attract a disc of material around them, with the same process that gives rise to planets around a star leading to the formation of moons around planets.
    • The disc around PDS 70c, with a diameter about equal to the distance of the Earth to the sun, possesses enough mass to produce up to three moons the size of Earth’s moon.
  • What is Monkey B virus?

    China has reported the first human death case with the Monkey B virus (BV).

    What is Monkey B virus?

    • The virus, initially isolated in 1932, is an alphaherpesvirus enzootic in macaques of the genus Macaca.
    • B virus is the only identified old-world-monkey herpes virus that displays severe pathogenicity in humans.

    Answer this question from our AWE initiative:

    There is been an increase in occurance of zoonotic human infectious diseases are zoonotic . Give reasons for this. Also suggest ways to contain and decrease the frequency of such events.(250 Words)

    How is it transmitted?

    • The infection can be transmitted via direct contact and exchange of bodily secretions of monkeys and has a fatality rate of 70 per cent to 80 per cent.
    • According to the Centre for Disease Control and Prevention, Macaque monkeys commonly have this virus, and it can be found in their saliva, feces, urine, or brain or spinal cord tissue.
    • The virus may also be found in cells coming from an infected monkey in a lab. B virus can survive for hours on surfaces, particularly when moist.

    When can a human get infected with B virus?

    • Humans can get infected if they are bitten or scratched by an infected monkey.

    Symptoms

    • Symptoms typically start within one month of being exposed to B virus but could appear in as little as three to seven days.
    • The first indications of B virus infection are typically flu-like symptoms such as fever and chills, muscle ache, fatigue and headache.
    • Following this, a person may develop small blisters in the wound or area on the body that came in contact with the monkey.
    • Some other symptoms of the infection include shortness of breath, nausea and vomiting, abdominal pain and hiccups.
    • As the disease progresses, the virus spreads to and causes inflammation (swelling) of the brain and spinal cord, leading to neurologic and inflammatory symptoms.

    Is there a vaccine against B virus?

    • Currently, there are no vaccines that can protect against B virus infection.

    Who are at higher risk for infection?

    • The virus might pose a potential threat to laboratory workers, veterinarians, and others who may be exposed to monkeys or their specimens.
    • To date, only one case has been documented of an infected person spreading the B virus to another person.
  • Near-Earth Asteroid Scout Mission

    Last week, NASA announced that its new spacecraft, named NEA Scout, has completed all required tests and has been safely tucked inside the Space Launch System (SLS) rocket.

    For landing on Moon

    • NEA Scout is one of several payloads that will hitch a ride on Artemis I, which is expected to be launched in November.
    • Artemis I will be an uncrewed test-flight of the Orion spacecraft and SLS rocket.
    • Under the Artemis programme, NASA has aimed to land the first woman on the Moon in 2024 and also establish sustainable lunar exploration programs by 2030.

    What is NEA Scout?

    • Near-Earth Asteroid Scout, or NEA Scout, is a small spacecraft, about the size of a big shoebox. Its main mission is to fly by and collect data from a near-Earth asteroid.
    • It will also be America’s first interplanetary mission using special solar sail propulsion.
    • This type of propulsion is especially useful for small, lightweight spacecraft that cannot carry large amounts of conventional rocket propellant.
    • NEA Scout will use stainless steel alloy booms and deploy an aluminium-coated sail measuring 925 square feet.
    • The large-area sail will generate thrust by reflecting sunlight.
    • Energetic particles of sunlight bounce off the solar sail to give it a gentle, yet constant push.

    How will it study the asteroid?

    • NEA Scout is equipped with special cameras and can take pictures ranging from 50 cm/pixels to 10 cm/pixels.
    • It can also process the image and reduce the file sizes before sending them to the earth-based Deep Space Network via its medium-gain antenna.
    • The spacecraft will take about two years to cruise to the asteroid and will be about 93 million miles away from Earth during the asteroid encounter.

    Why should we study near-Earth asteroids?

    • Despite their size, some of these small asteroids could pose a threat to Earth.
    • Understanding their properties could help us develop strategies for reducing the potential damage caused in the event of an impact.
    • Scientists will use this data to determine what is required to reduce risk, increase effectiveness, and improve the design and operations of robotic and human space exploration.
  • Why does Mercury have such a big iron core?

    Researchers have developed a model showing that the density, mass and iron content of a Mercury’s core is influenced by its distance from the Sun’s magnetic field.

    About Mercury

    • Mercury is the first and the smallest planet in our solar system.
    • It is also the closest planet to Earth.
    • Like the other three terrestrial planets, Mercury contains a core surrounded by a mantle and a crust.
    • But unlike any other planet, Mercury’s core makes up a larger portion of the planet.
    • MESSENGER was a NASA robotic space probe that orbited the planet Mercury between 2011 and 2015, studying Mercury’s chemical composition, geology, and magnetic field.
    • It was the analysis from the MESSENGER mission that tells: Mercury’s core is solid.

    Mystery over the core

    • It has long been known that Mercury’s core composition is made of liquid metal.
    • The core itself is about 3,600 km across. Surrounding that is a 600 km thick mantle.
    • And around that is the crust, which is believed to be 100-200 km thick.
    • The crust is known to have narrow ridges that extend for hundreds of kilometres.
    • This large core has long been one of the most intriguing mysteries about Mercury.

    Why does Mercury have a large core?

    • A new study reveals that the sun’s magnetism is the reason.
    • The sun’s magnetic field influences the density, mass, and iron content of Mercury’s core.
    • The four inner planets of our solar system—Mercury, Venus, Earth, and Mars—are made up of different proportions of metal and rock.
    • A gradient in which the metal content in the core drops off as the planets get farther from the sun.
    • The researchers explain how this happened by showing that the sun’s magnetic field controlled the distribution of raw materials in the early forming solar system.

    What are the key propositions?

    • During the early formation of the solar system, when a swirling dust storm and gas encircled the sun, iron’s grain was drawn toward the centre by the sun’s magnetic field.
    • At the time of planet formation from clumps of that dust and gas, planets nearer to the sun consolidated more iron into their centres than those farther away.
    • Scientists also found that the density and proportion of iron in the planet’s core correlate with the strength of the magnetic field around the sun during planetary formation.
    • Existing models on planetary formation were used to determine the speed at which gas and dust were pulled into the centre of our solar system during its formation.
    • The magnetic field that the sun would have generated as it burst into being and calculated how that magnetic field would draw iron through the dust and gas cloud.

    Cooling led solidification

    • As the early solar system began to cool, dust and gas that were not drawn into the sun started to clump together.
    • The clumps closer to the sun would have been exposed to a stronger magnetic field and thus would contain more iron than those farther away from the sun.
    • As the clumps coalesced and cooled into spinning planets, gravitational forces drew the iron into their core.