A close encounter with Jupiter about four billion years ago may have resulted in another planet’s ejection from the solar system altogether, scientists have found.
The existence of a fifth giant gas planet at the time of the solar system’s formation — in addition to Jupiter, Saturn, Uranus and Neptune that we know of today — was first proposed in 2011, researchers said.
But the question remained: if it did exist, how did it get pushed out?
For years, scientists have suspected the ouster was either Saturn or Jupiter.
“Our evidence points to Jupiter,” said Ryan Cloutier, a PhD candidate in University of Toronto’s Department of Astronomy & Astrophysics and lead author of a new study published in The Astrophysical Journal.
Planet ejections occur as a result of a close planetary encounter in which one of the objects accelerates so much that it breaks free from the massive gravitational pull of the Sun.
However, earlier studies which proposed that giant planets could possibly eject one another did not consider the effect such violent encounters would have on minor bodies, such as the known moons of the giant planets, and their orbits.
So Cloutier and his colleagues turned their attention to moons and orbits, developing computer simulations based on the modern-day trajectories of Callisto and lapetus, the regular moons orbiting around Jupiter and Saturn respectively.
They then measured the likelihood of each one producing its current orbit in the event that its host planet was responsible for ejecting the hypothetical planet, an incident which would have caused significant disturbance to each moon’s original orbit.
“Ultimately, we found that Jupiter is capable of ejecting the fifth giant planet while retaining a moon with the orbit of Callisto,” said Cloutier.
“On the other hand, it would have been very difficult for Saturn to do so because Iapetus would have been excessively unsettled, resulting in an orbit that is difficult to reconcile with its current trajectory,” Cloutier said
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Navigation satellite system by March


Last three satellites of constellation to be launched next year.

India is expected to have its own satellite-based regional navigation system in place by next March, providing accurate position information service for terrestrial, aerial and marine navigation, disaster management, vehicle tracking, fleet management and visual and voice navigation for drivers.
A.S. Kiran Kumar, Chairman, Indian Space Research Organisation (ISRO), said here on Thursday that the constellation of seven satellites comprising the Indian Regional Navigation Satellite System (IRNSS) would be in orbit by March. The last three of the satellites were scheduled to be launched in January, February and March, he told the media on the sidelines of a function organised by the High Energy Materials Society of India.
Launched by PSLV rockets, the first four satellites of the constellation are already in orbit. ISRO has also established a satellite navigation centre at Byalalu in Karnataka. A network of ranging stations located across the country will provide data for the orbital determination of the satellites and monitoring of the navigation signal.
Mr. Kumar said the first experimental flight of the indigenously developed fully Reusable Launch Vehicle (RLV) would take place towards the beginning of 2016. The RLV-TD (Technology Demonstrator) was undergoing tests at VSSC from where it would be moved to Bengaluru and later to Srikarikotta for the launch. RLV has been conceived by ISRO as a space plane that will bring down the cost of satellite launch substantially.
In the first test flight, RLV-TD, weighing around 1.5 tonnes, would be launched to an altitude of 70 km atop a solid booster rocket and released. Re-entering the atmosphere, the thermally insulated vehicle will travel back to earth in a controlled descent, to be recovered from the sea. ISRO has plans to construct a 4-km runway at SHAR for the RLV to make a horizontal landing in the subsequent flights.
Mr. Kumar said preparations were underway for the first developmental flight of the GSLV Mark 3 scheduled to take place by December 2016.
The biggest rocket made in India, the Mk3 will be capable of launching four-tonne satellites into geosynchronous orbit. He said efforts were on to achieve the target of two launches per year, using the Mk2 configuration of GSLV that is currently capable of placing satellites up to 2.2 tonnes in orbit.
Mr. Kumar added that Chandrayaan 2, India’s second lunar exploration mission, was expected to be launched by 2018. The project involves the indigenous development of a lunar orbiter, lander and rover.

  • First four satellites are already in orbit
  • Chandrayaan 2 likely by 2018: ISRO Chairman

  • Last three satellites of constellation to be launched next year

    Scientists trigger artificial quake on Japanese mountain


    Researchers have triggered an artificial earthquake on a mountain in Japan in search of data to help find signs of possible volcanic eruptions.
    Mount Zao is a 1,841-metres high complex volcano on the border between Yamagata Prefecture and Miyagi Prefecture in Japan.
    It has become active since a magnitude-9.0 earthquake hit Japan in March 2011, with increased volcanic tremors.
    A team from Tohoku University, together with Japan Meteorological Agency, detonated about 200 kg of dynamite inside a 40-metre-deep hole dug on the mountain side.
    Water poured inside the hole spewed out with the force of the blast.
    Seismic waves from the blast were measured by about 150 seismometers placed on the mountain, ‘NHK World’ reported.
    Since seismic waves travel more slowly through water, analysis of seismometer data enables researchers to estimate pools and pathways of hot water up to about two km underground.
    Satoshi Miura, a Professor at Tohoku University, said finding out the locations of hot water is a key to guessing where the next steam-blast explosion could occur.

    Harvest rain water or pay penalty


    BWSSB aims to enforce its proposal from March 2016

    Not implementing Rain Water Harvesting (RWH) at home may land you in a soup forcing you to pay a fine of 25 per cent of your water bill for three months progressively hiked to half your monthly bill till you harvest rain water.
    Bangalore Water Supply and Sewerage Board (BWSSB), in its board meeting on Thursday, approved the proposal, which has been sent to Urban Development Department (UDD) for approval.
    BWSSB brought in guidelines in 2009 making all sites of 40 ft X 60 sq ft and above to implement RWH with a one-year deadline. Of around 55,000 properties that this applied to, only close to 25,000 implemented RWH.
    “It has been five years since its deadline expired. People have been making excuses and not implementing RWH, even as underground water levels are fast depleting. So we have decided to bring in this penalty regime,” said T.M. Vijay Bhaskar, Chairman, BWSSB.
    “Ideally, we want to see the regime operational as we speak. But we are working on a March 1, 2016 deadline after which we will start penalising residents. The government has to approve the proposal and notify it,” he said.
    However S. Vishwanath, who aided BWSSB in drafting the RWH policy, is sceptical of the new guidelines. He said it is yet to be seen whether the penalty regime will work to bring more properties into the fold. “The main issue is that there is no incentive to harvest rain water. BWSSB provides highly subsidised water at Rs. 8 a kilo litre while the capital cost of RWH is high,” he said.
    He also differed with BWSSB on its focus on the core city. BWSSB needs to concentrate more on the outskirts where underground water levels are pretty low, rather than the core city where underground water levels are high, he explained.
    Mini STP in all buildings with more than 5 flats
    The BWSSB has decided to make a mini-Sewage Treatment Plant (STP) mandatory for all buildings with more than five flats.
    The guidelines also include a mandatory two-piping policy for all bathrooms. One pipeline will be exclusively used for flushing toilets using recycled water from the STP.
    “An estimated 40 – 50 litres of water is wasted in flushing a toilet every day. Water recycled in the mini-STP can be used to flush toilets, saving that much water. This is safe as the water will not in any way come in contact with the human body,” said T.M. Vijay Bhaskar, Chairman, BWSSB.

    Centre sanctions Rs. 64 crore for Coastal Tourism Circuit in Nellore

    The Centre has sanctioned Rs. 64 crore for implementation of the Coastal Tourism Circuit for Nellore district.
    Responding to Andhra Pradesh Tourism Development Corporation’s (APTDC) proposals worth Rs. 100 crore for the project, the Union Ministry of Tourism has sanctioned Rs. 64 crore for the purpose under its Swadesh Darshan Scheme.
    The Swadesh Darshan programme is an integrated development of tourist circuits around specific themes and the Coastal Tourism Circuit for Nellore is one of the five circuits indentified under this scheme. Others are: Buddhist Circuit, Himalayan Circuit, Krishna Circuit and North-East Circuit.
    R. Amarendra Kumar, the Executive Director (Projects), APTDC, said the mega project would pave the way for beautification of the coastline comprising scenic beaches, destinations of heritage and cultural importance.
    Nellore region is strategically located as it is well connected to cities like Chennai, Tirupati and Bengaluru. The existing Sri City and the proposed Industrial Smart City under Vizag-Chennai Industrial Corridor will also help in attracting a large number of visitors to the district.
    The proposed tourism circuit in this region envisages linking all the attractive features like the Pulicat Lake (B V Palem, Irakkum and Venadu Islands, Atakanitippa), the Nelapattu Birds sanctuary, the Kandaleru reservoir, Nellore tank bund, the Kothakoduru and Mypadu beaches, Ramatheertham temple and beach, Iskapalli beach, Udayagiri Fort and Krishnapatnam cruise terminal.
    The Pulicat Lake is the second largest brackish water lake in India; the flamingos here are nature’s gift. The sight of winged beauties at Nelapattu bird sanctuary is a feast to the eyes; The satellite launch pad of India —Sriharikota — has a great significance while the Krishnapatnam Port is India’s largest port on the horizon.Besides sumptuous Nellore cuisine, the place offers fascinating green spaces and mesmerising temples.

    Pro-active measures mooted to mitigate human-animal conflicts

    Greater public awareness on animal behaviour, the protocol to handle conflict situations and pro-active initiatives to help people reduce their losses are some of the measures mooted to mitigate man-animal conflicts.
    Vidya Athreya, Senior Research Fellow, Wildlife Conservation Society (WCS) India Programme, who is studying leopards, said here on Thursday that some of these measures could help people reduce their losses while helping to save the wild cats as well.
    She was speaking at a workshop on human-animal interactions and the resulting conflicts, organised by WCS in collaboration with the Mysore District Journalists’ Association.
    Building effective pens or sheds to protect livestock from predators would go a long way in mitigating losses while reducing conflicts, said Ms. Athreya.
    In rural areas with leopard population, if the farmers have to go to fields at night, it was best to go in groups or by making noise, lest the leopard mistake them for prey.
    She said that though translocation of leopards has been adopted by the Forest Department, it has not worked as the space left vacant by the animals will be occupied by another cat or the conflict will be transferred to another region. Incidentally, about 20 leopards have been trapped, caged and released into the forests in Mysuru region in the last two years but it is not clear whether the problem has abated. But it is done to soothe the frayed nerves of the local community, who otherwise, may indulge in revenge killings.
    Citing from her own research in Maharashtra, she said that there has never been a human death due to leopard attack though there may have been accidental injury as leopards tend to shy away from humans.
    The conflict however was real as leopards outside national parks and wildlife sanctuaries preyed on domestic animals and almost 40 per cent of its diet consisted of dogs.

    Pay for causing pollution, SC to trucks entering Delhi

    Formal judicial orders on October 12

    Declaring that controlling Delhi's pollution has become the "requirement of the day", the Supreme Court agreed to formalise in a judicial order a series of directions to impose 'environment compensation charge' on all light and heavy duty commercial vehicles entering the National Capital.
    A three-judge bench led by Chief Justice of India in a special sitting at 10.30 a.m. said the formal order imposing the pollution charge would be passed on Monday.
    It directed the Delhi government to issue a separate notification in this regard based on the Supreme Court.
    The pollution charge would be collected from all 127 entry points into Delhi. The court said the "deterrent" mechanism is an experiment for two months and is subject to any modification after four months.
    The court directed neighbouring State governments of Haryana, Rajasthan and Utter Pradesh to fall in line and the respective chief secretaries to co-ordinate with Delhi government.
    The series of directions to regulate the entry of trucks into Delhi to combat air pollution was drafted by the Supreme Court's amicus curiae in the case, senior advocate Harish Salve, in consultation with Solicitor General Ranjit Kumar for the Centre and senior advocate Dushyant Dave, representing the Delhi government.
    The Supreme Court's order on Monday would super cede all past order on the issue, including a recent one by the National Green Tribunal, imposing additional tax on polluting trucks entering Delhi.
    As per the note which will become part of the apex court's judicial order on Monday, environment compenation charge will be imposed at the rate of Rs. 700 for light duty vehicles and two-axle trucks. Three and four axle trucks would be charged Rs. 1300.
    Passenger buses, emergency vehicles and vehicles carrying essential commodities would be exempted from payment. The payment would be collected by the toll operator.
    "A direction is needed that charges so collected shall be handed over to the Delhi government by the toll operator without any deduction on a weekly basis," the directions said.
    The money so collected would be used by the Delhi government to augment public transport and roads, particularly vulnerable users like cyclists and pedestrians.
    The direction also said that private toll tax operators should install Radio Frequency Identity system at their own cost at all 127 points. This facility should be installed in nine main entry points which sees 75 per cent commercial traffic by November 2015. CCTVS too have to be installed in the same nine points.

    Notification on ESZ around Okhla sanctuary challenged


    As environmentalists see red over the Centre's notification limiting the eco-sensitive zone (ESZ) around Okhla Bird Sanctuary, activist and birder Anand Arya challenged the decision before the National Green Tribunal (NGT) on Thursday.
    Mr. Arya challenged the August 19 notification of the Centre setting the extent of eco-sensitive zone around the sanctuary as 100 metres on all sides, except northern, and 1.27 km on the northern boundary.
    His counsel Rahul Choudhary told the Bench that the notification is in violation of all legislative policies, including the provisions of the Environment (Protection) Act.
    The notification on the sanctuary, which is one among the several ornithologically-significant sites along the 50-km stretch of the Yamuna, had rejoiced many big builders and investors, who have projects or have brought homes in the area.
    “The notification will not only adversely affect the community at large, but will also result in the violation of the Environment (Protection) Act, 1986; Biological Diversity Act, 2002; precautionary principle; principle of sustainable development; inter-generational equity; and the principle of eco-centrism, all of which are law of the land as propounded by the Supreme Court,” Mr. Choudhary said.
    A Bench headed by NGT chairperson Justice Swatanter Kumar issued notices to the Centre, the State of Uttar Pradesh, chief wildlife warden, and the government of NCT of Delhi seeking their response in two weeks.

    Wild pandas in China turn carnivorous, fight for meat

    In a clip captured by infrared cameras, a panda was seen gnawing at the bones of a dead calf.

    Wild pandas at a national nature reserve in northwest China’s Gansu province have been captured by infrared cameras in an unusual behaviour such as fighting and eating meat.
    Since the beginning of 2014, staff at Baishuijiang National Nature Reserve have been observing the habits of the reserve’s 110 pandas with over 200 infrared cameras.
    Reserve manager Yuan Fengxiao said, “In the past, even our staff seldom saw wild pandas, but the infrared cameras have helped us record many valuable images of the animals.”
    Over 99 per cent of pandas’ diet consists of bamboo. In one clip, a panda was seen gnawing at the bones of a dead calf.
    Researcher He Liwen said that besides bamboo, wild pandas are scavengers and eat meat, but rarely find carcasses of dead animals.
    Another panda was seen with a bleeding forehead shortly after appearing on another camera with its forehead intact, probably as a result of fighting with other pandas or bears, state-run Xinhua news agency reported.
    In another clip, a pair of pandas were wandering in the woods when one discovered the camera and started to chew on it.
    Spread over 2,00,000 hectares, the Baishuijiang reserve is one of China’s largest reserves for wild pandas.
    Mr. Yuan said that about 500 species of animals and over 2,000 kinds of wild plants have been recorded there.
    The infrared cameras have also captured footage of other rare species including the golden monkey and Takin.

    Surprising discovery of oxygen in 67P comet’s atmosphere

    The Comet 67P/Churyumov-Gerasimenko has thrown a very big surprise — its atmosphere contains molecular oxygen. Based on our current thinking, the presence of molecular oxygen in a comet had been ruled out. But chemical analysis of its atmosphere using ROSINA mass spectrometer on board the Rosetta spacecraft has shown that molecular oxygen is not only present but is also found in high proportion.
    In fact, molecular oxygen level in the comet was found to range from one per cent to 10 per cent relative to water with a mean value of 3.8 per cent (with an error margin of 0.85 per cent). It has turned out that oxygen is the fourth most common gas in the comet’s atmosphere, after water, carbon monoxide and carbon dioxide.
    The results were published today (October 29) in the journal Nature.
    “It is the most surprising finding as molecular oxygen was not among the molecules expected to be found in a comet,” Prof. Kathrin Altwegg, project leader of the ROSINA mass spectrometer from the University of Bern, Switzerland and a co-author of the study said during a press briefing.
    Since molecular oxygen is highly reactive, it was assumed that it would have combined with hydrogen then present to form water. “We had never thought that oxygen could ‘survive’ for billions of years without combining with other substances,” said Prof. Altwegg. Alas, the discovery of molecular oxygen has shaken the very foundation of our understanding of oxygen in comets.
    “Molecular oxygen was constant over a long period of time. When the comet is orbiting the Sun, it loses more material from the surface. So a fresh layer gets exposed over time. Since the ratio of water to oxygen is remaining constant [in different locations on the comet], it means that molecular oxygen must be present in the whole body [of the comet]. If it is present only on the top surface then there would be a decrease [in amount] over a period of time,” Prof. A. Bieler the first author of the paper from the University of Michigan, U.S. told during the briefing.
    During the period of study — August 2014 to March 2015 — the authors estimate that several centimetres thick layer of material must have been lost from the surface areas of the comet.
    Since the ratio of water to oxygen has not changed in different locations on the comet or over time (nearly 4.6 billion years), there is a stable correlation between water and oxygen.
    Since oxygen is present in the whole body of the comet, the oxygen must be primordial and must be present even before or at the formation of the comet, Prof. Bieler said. In other words, the oxygen originated very early, before the formation of the Solar System.
    “Specifically, high-energy particles struck grains of ice in the cold and dense birthplaces of stars, the so-called dark nebulae, and split water into oxygen and hydrogen. The oxygen was then not further “processed” in the early solar system. The oxygen measurements show that at least a significant part of the comet’s material is older than our solar system and has a composition typical of dark nebulae, from which solar nebulae and later planetary systems originate,” notes a University of Bern release.
    The molecular oxygen has been trapped in the water ice of the comet 67P. The ice has never been heated up to get reprocessed. “[You have] ice grains with oxygen embedded into it and you have them even today means that the ice was never sublimated, never went back into the gas phase,” Prof. Altwegg said.
    According to her, most of the Solar System info models predict heavy inflow of material from outside to the centre of the Solar System and then also a heavy outflow of material leading to a mixing of intrasolar system during formation. “But these [models] are not compatible with ice grains containing oxygen. They must have stayed out, never mixed, or never come close to the young Sun,” she said.
    “The preferred explanation of our observations is the incorporation of primordial oxygen into the cometary nucleus,” they note in the paper.
    Radiolysis of icy grains before accretion is one of the possible mechanisms that the author think could have preserved the oxygen over a long period of time. “When produced by radiolysis in water ice, oxygen can remain trapped in voids, while hydrogen can diffuse out. This prevents the hydrogenation of oxygen, which is otherwise a dominant reaction for the destruction of molecular oxygen, and could lead to increased and stable levels of oxygen in the solid ice,” they write.

    Eating bacon, sausages poses cancer risk: WHO

    Ham, hot dogs also in group 1 list alongside tobacco, diesel fumes, asbestos for causes of cancer

    Eating processed meat can lead to bowel cancer in humans while red meat is a likely cause of the disease, World Health Organisation (WHO) experts said on Monday in findings that could sharpen debate over the merits of a meat-based diet.
    The France-based International Agency for Research on Cancer (IARC), part of the WHO, put processed meat such as hot dogs and ham in its group 1 list, which already includes tobacco, asbestos and diesel fumes, for which there is "sufficient evidence" of cancer links.
    "For an individual, the risk of developing colorectal (bowel) cancer because of their consumption of processed meat remains small, but this risk increases with the amount of meat consumed," Dr Kurt Straif of the IARC said in a statement.
    Red meat, under which the IARC includes beef, lamb and pork, was classified as a "probable" carcinogen in its group 2A list that also contains glyphosate, the active ingredient in many weed-killers.
    The lower classification for red meat reflected "limited evidence" that it causes cancer. The IARC found links mainly with bowel cancer, as was the case for processed meat, but it also observed associations with pancreatic and prostate cancer.
    The agency, whose findings on meat followed a meeting of health experts in France earlier this month, estimated each 50 gram portion of processed meat eaten daily increases the risk of colorectal cancer by 18 percent.
    The IARC, which was assessing meat for the first time and reviewed some 800 studies, does not compare the level of cancer risk associated with products in a given category, so does not suggest eating meat is as dangerous as smoking, for example.
    Health policy in some countries already calls for consumers to limit intake of red and processed meat, but the IARC said such advice to consumers was in certain cases focused on heart disease and obesity.
    The preparation of the IARC's report has already prompted vigorous reactions from meat industry groups, which argue meat forms part of a balanced diet and that cancer risk assessments need to be set in a broader context of environmental and lifestyle factors.
    The IARC, which does not make specific policy recommendations, cited an estimate from the Global Burden of Disease Project - an international consortium of more than 1,000 researchers - that 34,000 cancer deaths per year worldwide are attributable to diets high in processed meat.
    This compares with about 1 million cancer deaths per year globally due to tobacco smoking, 600,000 a year due to alcohol consumption, and more than 200,000 each year due to air pollution, it said.
    If the cancer link with red meat were confirmed, diets rich in red meat could be responsible for 50,000 deaths a year worldwide, according to the Global Burden of Disease Project.

    First insect-size robot that can fly, swim

    For the first time, scientists have designed an insect-like robot smaller than a paperclip that can both fly and swim — paving the way for future dual aerial aquatic robotic vehicles.
    The biggest challenge is conflicting design requirements: aerial vehicles require large airfoils like wings or sails to generate lift while underwater vehicles need to minimise surface area to reduce drag.
    To solve this engineers at the Harvard University’s John A Paulson School of Engineering and Applied Science (SEAS) took a clue from puffins.
    The birds with flamboyant beaks are one of nature’s most adept hybrid vehicles, employing similar flapping motions to propel themselves through air as through water.
    “Through various theoretical, computational and experimental studies, we found that the mechanics of flapping propulsion are actually very similar in air and in water,” said Kevin Chen, a graduate student at the Harvard Microrobotics Lab at SEAS.
    The RoboBee, designed in postdoctoral fellow Robert J Wood’s lab, is a microrobot, smaller than a paperclip, that flies and hovers like an insect, flapping its tiny, nearly invisible wings 120 times per second.
    In order to make the transition from air to water, the team first had to solve the problem of surface tension.
    The RoboBee is so small and lightweight that it cannot break the surface tension of the water.
    To overcome this hurdle, the RoboBee hovers over the water at an angle, momentarily switches off its wings, and crashes unceremoniously into the water in order to sink.
    Next the team had to account for water’s increased density.
    “Water is almost 1,000 times denser than air and would snap the wing off the RoboBee if we didn’t adjust its flapping speed,” said graduate student Farrell Helbling, the paper’s second author.
    The team lowered the wing speed from 120 flaps per second to nine but kept the flapping mechanisms and hinge design the same.
    A swimming RoboBee changes its direction by adjusting the stroke angle of the wings, the same way it does in air. Like a flying version, it is still tethered to a power source.
    The team prevented the RoboBee from shorting by using deionised water and coating the electrical connections with glue.
    While this RoboBee can move seamlessly from air to water, it cannot yet transition from water to air because it can’t generate enough lift without snapping one of its wings.
    Solving that design challenge is the next phase of the research, according to Chen.

    Bacteria neutralises greenhouse gas

    A type of bacteria found at the bottom of the ocean could be used to neutralise large amounts of industrial carbon dioxide in the Earth’s atmosphere, researchers have found. Most atmospheric CO is produced from fossil fuel combustion.
    But converting the carbon dioxide into a harmless compound requires a durable, heat-tolerant enzyme. The bacterium, Thiomicrospira crunogena, studied by researchers from University of Florida, produces carbonic anhydrase, an enzyme that helps remove CO in organisms.
    The bacterium lives near hydrothermal vents, so the enzyme it produces is accustomed to high temperatures.
    That is exactly what is needed for the enzyme to work during the process of reducing industrial CO, said Robert McKenna at the University of Florida College of Medicine.
    The enzymecatalyses a chemical reaction between CO and water.
    The CO interacts with the enzyme, converting the greenhouse gas into bicarbonate. The bicarbonate can then be further processed into products such as baking soda and chalk.
    According to the UF researchers, which included graduate research assistants Brian Mahon and Avni Bhatt, in an industrial setting the carbonic anhydrase would be immobilised with solvent inside a reactor vessel that serves as a large purification column.
    Flue gas would be passed through the solvent, with the carbonic anhydrase converting the carbon dioxide into bicarbonate.

    National leaders and the Medicine Nobel

    Several Latin American countries have been declared free of sleeping sickness

    What have national leaders like Ho Chi Min of Vietnam, Chairman Mao of China and Jimmy Carter of America to do with this year’s Nobel Prize in Physiology or Medicine? Reports have it that Ho Chi Min was greatly disturbed by the loss of thousands of soldiers (fighting the Americans in the Vietnam War) to malaria. He appealed to his ally, Chairman Mao, stating that a wild plant in rural Vietnam was claimed to cure malaria, and whether he could direct Chinese scientists to help isolate any active anti-malarial drug molecules from such a plant. Mao did so, and decades of work by Chinese scientists led to the drug artemisinin. The main player behind this was a lady scientist called Tu You You, who was honoured with the Nobel Prize in Medicine a few weeks ago. (Apparently when the Nobel Committee tried to call Tu You You (what a lyrical name!), they could not; she was away in the hinterlands, presumably working away).
    Former President of America, Mr. Jimmy Carter, after retirement, established the Jimmy and Rosalynn Carter Center in 1982 with the theme: “Waging Peace, Fighting Disease, Building Hope”. In the area of fighting disease, the Center collaborated with Emory University at Atlanta, GA, and the drug firm Merck. Together, they focused on the disease called Human African Trypanosomosis (also spelt as trypanosomiasis), which affects vision, leads to sleeping sickness, lymphatic swelling and elephantiasis, and overall lethargy. This disease was found to spread across 10 million square km in Sub-Saharan Africa (Sudan, Ethiopia, Uganda, Mali, Nigeria, Kenya, Gambia, Zimbabwe etc, particularly along river coasts (hence the name river blindness). It affects not only people but also livestock, where it leads to drop in milk and meat production, abortions and gradual weakness and wasting away. The Carter Center, in collaboration with Lions International, Merck Institute and in-house support, launched a programme to fight and end trypanosomosis in affected areas.
    The end results have been stunning and successful. The researchers, led by Dr William C Campbell of the Merck Center, obtained a natural product called Avermectin (sent to them by Dr. Satoshi Omura of Tokyo, Japan, who showed its effectiveness against parasitic infections), tweaked its chemical structure a bit to produce the drug called Ivermectin (Merck’s trade name for this is Mectizan). This drug cures this debilitating disease and also protects against latter day recurrence. One tablet a year (yes, just one per year) for 10 years is the dose; rather similar to how we administer vaccines! To date, thanks to the Carter Center’s request and participation, Merck has given away 270 million tablets of Ivermectin across not just Africa but also in parts of Latin America (Mexico, Guatemala, Ecuador, Venezuela, Colombia, Brazil) and in the Arab country Yemen. Several of these Latin American countries have been declared trypanosomosis-free.
    Why and how does trypanosomosis come about and how does it affect the body of the infected animals and humans? It is caused by a parasitic protozoan (a type of roundworm) that resides inside the fly called Tsetse (or Tzetze, also called tik tik; lyrical names again), which abound along river coasts across Sub-Saharan Africa and parts of Latin America. When the tsetse fly bites you, it delivers the villain parasite. This is what leads to the sleeping sickness, elephantiasis, lymphatic swelling and inflammation of the cornea of the eye, leading to loss of vision (river blindness or ‘onchocerciasis’ as the eye doctors call it).
    How was the solution found? It was in the 1970s that Dr. Satoshi Omura, working at the Kitasato University in Tokyo, identified some microbes called Streptomyces in the soil, and one form of it called S. avermitilis, which produces molecules that fight roundworms and other parasites. He isolated one of them, which he called avermectin and sent it to Merck in the US. William Campbell worked on it, modified it into a more effective molecule which he named Ivermectin (apparently named after a village in UK called Iver; Campbell is of Irish origin), and history was made. Campbell and Omura share half the prize amount, while Tu You You gets the other half. Incidentally, Jimmy Carter himself received the Nobel Peace Prize in 2002, for his humanitarian efforts.
    Does trypanosomosis through such a parasite occur in India? To date, thankfully enough, no; and even if it does, ivermectin will help take care of it. Thus, the sleeping sickness we see often in government offices has other origins.

    Why don't we see solar eclipse every month?

    SOLAR ECLIPSE
    Since the moon revolves around the Earth all the times, why don’t we see solar eclipse during every moon’s revolution around the Earth?

    Before the question is answered, we should know how solar eclipses do happen. Solar eclipse is nothing but obscuring of the Sun due to the Moon coming in between the Sun and the viewer on the Earth during the course of revolving of the Moon and the Earth. As we all know that the Earth revolves around the Sun in a near circular path completing one revolution in about 365 days. The plane in which the Earth moves around the Sun is known as the Ecliptic.
    At the same time the Moon also revolves around the Earth which is also a near circular path, completing on revolution in about 28 days, known as a lunar month. But the fact is that these two planes are inclined to each other at an angle.
    For the Solar eclipse to occur, the Sun, the Moon and the Earth must come not only in one straight line but also these three bodies should be in one plane.
    Although the Sun, the Moon and the Earth come in one line every two weeks, once on a new Moon night and second time on the full Moon night, they seldom come in one plane during these events. This occurs two to maximum of five times in a year. Similarly, the Moon eclipse occurs when the Earth’s shadow falls on the Moon, which happens when the Earth comes in between the Sun and the Moon exactly.
    This phenomenon takes place on a full Moon night and up to three times in a year. Generally the Sun eclipse and the Moon eclipse follow each other with a gap of 14 days. Another interesting fact about the Sun eclipse is that the events repeat each other after a time gap of 18.6 years, known as Saros cycle.

    NASA completes key milestone for most powerful rocket

    NASA’s Space Launch System (SLS), which will be the most powerful rocket ever built and the first vehicle designed to meet the challenges of the journey to Mars, has completed all steps needed to clear a critical design review.
    This is the first time in almost 40 years that a NASA human-rated rocket has cleared a critical design review (CDR).
    “We’ve nailed down the design of SLS, we’ve successfully completed the first round of testing of the rocket’s engines and boosters, and all the major components for the first flight are now in production,” said Bill Hill, deputy associate administrator of NASA’s Exploration Systems Development Division in US.
    “There have been challenges, and there will be more ahead, but this review gives us confidence that we are on the right track for the first flight of SLS and using it to extend permanent human presence into deep space,” Mr. Hill said.
    The CDR examined the first of three configurations planned for the rocket, referred to as SLS Block 1.
    The Block 1 configuration will have a minimum 70-metric-ton lift capability and be powered by twin boosters and four RS-25 engines.
    The next planned upgrade of SLS, Block 1B, would use a more powerful exploration upper stage for more ambitious missions with a 105-metric-ton lift capacity.
    Block 2 will add a pair of advanced solid or liquid propellant boosters to provide a 130-metric-ton lift capacity.
    In each configuration, SLS will continue to use the same core stage and four RS-25 engines.
    The SLS Programme completed the review in July, in conjunction with a separate review by the Standing Review Board, which is composed of seasoned experts from NASA and industry who are independent of the programme.
    Throughout the course of 11 weeks, 13 teams — made up of senior engineers and aerospace experts across the agency and industry — reviewed more than 1,000 SLS documents and more than 150 GB of data as part of the comprehensive assessment process at NASA’s Marshall Space Flight Centre, where SLS is managed for the agency.
    The Standing Review Board reviewed and assessed the programme’s readiness and confirmed the technical effort is on track to complete system development and meet performance requirements on budget and on schedule.
    The programme briefed the results of the review in October to the Agency Program Management Council, led by NASA Associate Administrator Robert Lightfoot, as the final step in the CDR process.
    This review is the last of four reviews that examine concepts and designs. The next step for the programme is design certification, which will take place in 2017 after manufacturing, integration and testing is complete.
    Critical design reviews for the individual SLS elements of the core stage, boosters and engines were completed successfully as part of this milestone.

    ASTROSAT spots Crab Nebula, the brightest X-ray source

    The sighting implies that the specific instrument can locate X-ray sources

    On October 9, ASTROSAT, the first Indian space observatory, spotted the Crab Nebula using the Cadmium Zinc Telluride Imager (CZTI) instrument. The Crab Nebula is the brightest hard X-ray (highest energy X-ray) source in the sky; researchers often use it as a reference to calibrate hard X-ray detectors.
    The sighting of the Crab is significant and implies that the specific instrument on board can locate X-ray sources. It would further view other celestial X-ray sources and aid Indian research on them.
    “This is only the beginning, with many more events to unfold”, ISRO said. The nebula was detected on October 9 [at the same time] by both the Mission Operation Centre at Peenya, Bengaluru, and the Payload Operation Centre, IUCAA, Pune.
    ASTROSAT also spotted and viewed Cygnus X-1, a black hole source, for two days.
    Nerve-wracking

    The sighting of the Crab Nebula was preceded by palpable tension and a “nerve wracking period which seemed like eternity but was only three days” before scientists at the Mission Operation Centre in Bengaluru detected the Crab Nebula at 2.03 pm on October 9. The Payload Operation Centre, IUCAA, Pune too detected it at almost the same time.
    “If we are not looking at the source, we would get some background photons. But the background photons were a lot more than anticipated,” said Dr. Varun Bhalerao, Post Doctoral Fellow at the Pune-based Inter-University Centre for Astronomy and Astrophysics (IUCAA). In fact, the background rate exceeded the anticipated rate by a factor of four.
    “When a cosmic ray hits any matter [in this case the telescope], it creates lots of photons locally due to cosmic ray interaction. What would be detected as one photon becomes 10 photons,” Dr. Bhalerao said. “Theoretically and observationally, it is known that when a high-energy cosmic ray hits any matter it can create a shower. Several parameters should be right to see this shower.”
    As a result, the signal from the Crab Nebula was swamped by noise (background photons) and hence the scientists could not spot the nebula in the very first orbit.
    Soon thereafter, the ASTROSAT passed through the South Atlantic Anomaly (SAA) region when the Crab was in the field of view. The South Atlantic Anomaly is Earth’s magnetic field anomaly region as a lot of charged particles are trapped there. So there is so much noise whenever a satellite passes through the SAA region. The region can also damage the instruments. Hence all instruments were switched off when ASTROSAT was passing through the South Atlantic Anomaly region.
    “Once outside the SAA region, the Crab Nebula was behind the Earth for most of the time,” Dr. Bhalerao said. “After a couple of orbits, we could finally see the Crab. The scientists by then were able to suppress the noise and detect the signal from the Crab Nebula. “On more analysis, we can now see the Crab from parts of all orbits. In hindsight, it becomes easier,” he said.
    The multi-wavelength ASTROSAT was launched on September 28 with its five scientific instruments.
    Other X-ray instruments would be made operational in the coming weeks. In about a month, all X-ray instruments will be ready to stare at interesting stars.

    Atom bomb: no excess cancer death among survivors’ kids

    This year we observed the 70th anniversary of A-bombing of Hiroshima and Nagasaki. In the 1950 Japanese national census, nearly 280,000 persons stated that they “had been exposed” in the two cities. The Radiation Effects Research Foundation (RERF)selected about 94,000 people to to study the health effects of radiation.

    One of the most notable among these projects is the study of the survivors’ children. Quite contrary to popular perception, this study recently revealed that the children born to exposed parents did not suffer from excess cancer mortality or non-cancer deaths (The Lancet Oncology, September 15, 2015).

    Dr Eric J Grant and co workers from the RERF looked at the birth records to identify children conceived after the atomic bombings and born in Hiroshima and Nagasaki. They also collected data from city offices which entertained applications from pregnant women.

    The study included 75,327 children of atomic bomb survivors in the two cities and unexposed controls, born between 1946 and 1984, and followed up to Dec 31, 2009. Researchers interviewed the parents directly or matched them to a master list of survivors to estimate the radiation exposure to their reproductive organs. This dose depended on distance of the individual from the hypocentre, shielding from such objects as buildings or hills and shielding from intervening tissues inside the body before radiation reached a particular organ.

    The study covered 16,869 children with one or both parents within 2 km of the hypocentres. The researchers compared them with 18,450 children born to one or both parents resident in the city before and after the bombing but neither parent closer than 2.5 km to the hypocentres and 16,738 children who had both parents outside of the cities at the time of the bombing. Researchers matched the comparison groups by year of birth, sex, and city.

    They cautioned that the study is still underpowered. Ninety per cent of the cohort is still alive. Further follow up will enhance the statistical power of the study.

    What is the importance of the study? In an accompanying comment, David Brenner, Center for Radiological Research, Columbia University Medical Center, U.S. noted that in the first decade or so after the explosions, scientists focussed most of the concerns about long-term health on potential heritable genetic effects in subsequent generations.

    They relied on Dr. Herman Mueller's 1927 study which showed that radiation could induce heritable genetic effects in fruit fly.

    “Since the 1950s, however, understanding of the relative importance of genetic and somatic radiation related effects has completely reversed: genetic effects are now considered only a small contributor to the overall detriment to health after radiation exposure”, Brenner clarified. The conclusions from the latest study are consistent with the recent thinking on the topic.

    . Long-term studies of the health impact of radiation on the progeny of A-bomb survivors have not shown any scientific evidence for heritable genetic effects.

    Scientists assume that persons exposed to radiation may suffer from genetic effects as a matter of abundant caution as studies on fruit flies and mouse have shown that radiation can cause genetic effects. Though it is only an assumption, members of the public consider genetic effects of radiation as gospel truth — a wrong public perception prevails over a robust scientific fact.

    While agreeing with Dr Brenner's view that “absence of evidence is not evidence of absence”, we need not lose sleep over the genetic effects of radiation as he rightly stated that “the risks must be small, otherwise they would have been observed in the children of survivors”.

    The writer is a former secretary, AERB

    Chinese chrysanthemum enters Guinness World Records

    A “full-standing multiflorous chrysanthemum” grafted in central China’s Henan province has earned its place in the Guinness World Records for containing the largest number of chrysanthemum species.
    The multiflorous chrysanthemum is 3.8 metres in diameter and composed of 641 different types of chrysanthemums grafted to southernwood. It was certified for the world record on Sunday in Kaifeng city of Henan province, Xinhua news agency reported.
    A representative of Guinness World Records made the announcement at a chrysanthemum festival in the city.
    It took about four years to cultivate the plant, which now has more than 1,500 flowers blossoming at one time.

    ABC conjecture: proved but still out of reach?


    The conjecture is key to solving several other important problems

    In August 2012, Shinichi Mochizuki, Japanese mathematician from Kyoto University’s Research Institute for Mathematical Sciences, posted four papers on his website that claimed to contain a proof of the important ABC conjecture. This was a potential bombshell, as the ABC conjecture holds the key to solving several other important problems.
    However, most mathematicians are still flummoxed by the proof which uses a new branch of the field too abstract even to them. It is not as though Mochizuki has made elaborate attempts to either publicise his work or render it more comprehensible by giving lectures about it around the world. His approach seems to be to quietly work for about a decade in near isolation, and then, equally quietly, to post the proof online!
    The ABC conjecture

    “The ABC conjecture says that an ‘additive condition’ on integers imposes strong restrictions on their ‘multiplicative structure’, that is, their prime factorization,” says mathematician Hector Pasten, of Harvard University, who works in number theory and mathematical logic, in an email to this correspondent.
    “For example, take the equation 128+81=209. On the left-hand side are 128 (which is factorised as the prime 2 repeated seven times) and 81 (which is factorised as the prime 3 repeated four times). The ABC conjecture says that we should not expect too many repetitions on the right-hand side because, on average, the primes should not be repeated too many times in an equation of the form A+B=C (after common primes are cancelled). And, in fact, 209=11x19 has no repeated prime factor!” he said.
    Dr Pasten remarks, “Believe or not, the content of the conjecture is not more complicated than what I just explained. A totally different story is trying to prove it!”
    There are many known uses to having a proof of the conjecture. These include its ability to solve many of the so-called Diophantine equations. Dr Pasten elaborates, “It would give much simpler new proofs to known very deep and complicated theorems in the area, such as Gerd Faltings’s theorem for curves (previously Mordell’s conjecture) and Fermat’s Last Theorem…It would give solutions to important open problems in number theory... It would establish new connections between the number theory and other areas of mathematics that might seem rather distant, such as complex analysis and mathematical logic...”
    Impenetrable
    Dr Pasten says, “The key notion in Mochizuki’s recent work is identifying arithmetic-geometric objects from their symmetries. However, this is not a new subject. In the technical sense required here, the idea was suggested by the great mathematician Alexander Grothendieck under the name of Anabelian Geometry … Mochizuki is a world expert in the subject of Anabelian Geometry and, in fact, he proved Grothendieck’s Anabelian conjecture in 1996, with all mathematical rigor. This experience makes people consider his work on ABC as a serious attempt, although we don’t currently understand it.”

    (It will be updated with more article from Sci tech section from October month.)