NASA providing daily weather reports for Mars

Agencies
February 21, 2019

Washington, Feb 21: NASA's Jet Propulsion Laboratory will provide daily weather reports for Mars, thanks to the Red Planet's newest robotic resident, InSight, mission scientists announced Thursday.

"The InSight lander is close to the Martian equator -- just north of the equator -- so it is experiencing Martian winter," said Don Banfield, the mission's lead for the lander's Auxiliary Payload Subsystem (APSS).

APSS is a suite of meteorological sensors on the lander's deck that also helps with quake detection.

"For our mission, APSS will help us filter out noise in our data and know when we're seeing a Mars quake and when we aren't," said Banfield, a principal research scientist at Cornell University in the US.

"But by operating continuously, we'll also see a more detailed view of the weather than most surface missions, which usually collect data for just a few hours at a time," Banfield said in a statement.

Currently, Mars' northern hemisphere sits in winter -- the stormy season, researchers said.

"Since the lander is close to the equator, I did not think we would see any evidence of the storms that are 60-degrees north latitude, but we are already seeing evidence of the high and low pressure-signal waves that create weather on Mars," Banfield said.

"We can see those waves all the way down near the equator, as the waves are big enough that they have a signature. That was a surprise," he said in a statement.

The pressure signals oscillate every 2.5 sols (the name for days on Mars), and the waves are easier to predict as opposed to how pressure waves behave on Earth. One sol is about 24 hours, 39 minutes long.

"High and low pressure is indicative of the weather systems," Banfield said.

"Compared to Mars, Earth is pretty chaotic. Mars has a nearly perfect, smooth sinusoidal (up and down) waves -- it is a very regular seesaw guided by a metronome on Mars. On Earth, the pressure is guided by a hyperactive child," he said.

Mission scientists said the coldest temperatures -- as cold as minus 59 degrees Celsius -- occur at around 5 am local time. The warmest temperatures have been minus five degrees Celsius.

When the sun heats up the Martian surface, scientists have observed strong convective overturning.

"Think of a pot of water boiling -- the water is overturning vigorously. That happens on Mars, too," Banfield said.

"The atmosphere near the ground bubbles up like a buoyant plume of air. It happens on Earth, too, but you don't feel it as much. On Mars it happens with a lot more vigour," he said.

In another surprise, mission scientists are observing many "dust devils" -- those ghostly, low-pressure, tornado-like whirls of Martian soil.

"They spin at nearly 96 kilometres per hour. They do shake the lander, and we have seen a lot of that. They even tilt the ground, because we have such a sensitive seismometer," Banfield said.

"On Earth, the desert's dust devils would be likely 15 metres across and almost a kilometer tall. On Mars, they can be five to 10 kilometers tall. Big ones are 100 metres or more in diameter," he said.

The InSight craft landed on Mars in late November and is preparing to monitor the geologic interior of the planet.

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Agencies
March 10,2020

New Delhi, Mar 10: Crisis-hit Yes Bank on Tuesday said that it has enabled inward IMPS and NEFT services.

The move allows people to send money from other bank accounts to their Yes Bank account through IMPS (Immediate Payment Service) and NEFT (National Electronic Funds Transfer) mode.

In a tweet, the bank also said that Yes Bank customers can pay their credit card dues and loan obligations from other bank accounts.

"Inward IMPS/NEFT services have now been enabled. You can make payments towards YES BANK Credit Card dues and loan obligations from other bank accounts. Thank you for your co-operation. @RBIA @FinMinIndia," said tweet.

Last week Yes Bank was placed under moratorium and a withdrawal cap of Rs 50,000 was imposed till April 3.

The administrator of Yes Bank, Prashant Kumar and Rajnish Kumar, the Chairman of the State Bank of India are hopeful that moratorium would be lifted within a week.

As per the Reserve Bank of India (RBI) draft reconstruction scheme for the crisis-hit private lender, the SBI will take up 49 per cent in the bank by investing Rs 2,450 crore.

The new board of directors will stand constituted from the appointed date. It will comprise a CEO and MD, non-executive chairman and non-executive directors. The SBI will have nominee directors appointed on the board of the reconstructed bank.

The RBI may appoint additional directors to the board, who shall continue in office for one year, or until an alternate board is constituted by Yes Bank.

The SBI will not reduce its holding below 26 per cent before completion of three years from the date of infusion of the capital.

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Agencies
June 19,2020

Denser places, assumed by many to be more conducive to the spread of the coronavirus that causes COVID-19, are not linked to higher infection rates, say researchers.

The study, led by Johns Hopkins University, published in the Journal of the American Planning Association, also found that dense areas were associated with lower COVID-19 death rates.

"These findings suggest that urban planners should continue to practice and advocate for compact places rather than sprawling ones, due to the myriad well-established benefits of the former, including health benefits," says study lead author Shima Hamidi from Johns Hopkins Bloomberg School of Public Health in the US.

For their analysis, the researchers examined SARS-CoV-2 infection rates and COVID-19 death rates in 913 metropolitan counties in the US.

When other factors such as race and education were taken into account, the authors found that county density was not significantly associated with county infection rate.

The findings also showed that denser counties, as compared to more sprawling ones, tended to have lower death rates--possibly because they enjoyed a higher level of development including better health care systems.

On the other hand, the research found that higher coronavirus infection and COVID-19 mortality rates in counties are more related to the larger context of metropolitan size in which counties are located.

Large metropolitan areas with a higher number of counties tightly linked together through economic, social, and commuting relationships are the most vulnerable to the pandemic outbreaks.

According to the researchers, recent polls suggest that many US citizens now consider an exodus from big cities likely, possibly due to the belief that more density equals more infection risk.

Some government officials have posited that urban density is linked to the transmissibility of the virus.

"The fact that density is unrelated to confirmed virus infection rates and inversely related to confirmed COVID-19 death rates is important, unexpected, and profound," said Hamidi.

"It counters a narrative that, absent data and analysis, would challenge the foundation of modern cities and could lead to a population shift from urban centres to suburban and exurban areas," Hamidi added.

The analysis found that after controlling for factors such as metropolitan size, education, race, and age, doubling the activity density was associated with an 11.3 per cent lower death rate.

The authors said that this is possibly due to faster and more widespread adoption of social distancing practices and better quality of health care in areas of denser population.

The researchers concluded that a higher county population, a higher proportion of people age 60 and up, a lower proportion of college-educated people, and a higher proportion of African Americans were all associated with a greater infection rate and mortality rate.

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Agencies
June 8,2020

Washington DC, Jun 8: Astronomers acting on a hunch have likely resolved a mystery about young, still-forming stars and regions rich in organic molecules closely surrounding some of them.

They used the National Science Foundation's Karl G Jansky Very Large Array (VLA) to reveal one such region that previously had eluded detection and that revelation answered a longstanding question.

The regions around the young protostars contain complex organic molecules which can further combine into prebiotic molecules that are the first steps on the road to life.

The regions, dubbed "hot corinos" by astronomers, are typically about the size of our solar system and are much warmer than their surroundings, though still quite cold by terrestrial standards.

The first hot corino was discovered in 2003 and only about a dozen have been found so far. Most of these are in binary systems, with two protostars forming simultaneously.

Astronomers have been puzzled by the fact that, in some of these binary systems, they found evidence for a hot corino around one of the protostars but not the other.

"Since the two stars are forming from the same molecular cloud and at the same time, it seemed strange that one would be surrounded by a dense region of complex organic molecules and the other wouldn't," said Cecilia Ceccarelli, of the Institute for Planetary Sciences and Astrophysics at the University of Grenoble (IPAG) in France.

The complex organic molecules were found by detecting specific radio frequencies, called spectral lines, emitted by the molecules. Those characteristic radio frequencies serve as "fingerprints" to identify the chemicals.

The astronomers noted that all the chemicals found in hot corinos had been found by detecting these "fingerprints" at radio frequencies corresponding to wavelengths of only a few millimetres.

"We know that dust blocks those wavelengths, so we decided to look for evidence of these chemicals at longer wavelengths that can easily pass through dust," said Claire Chandler of the National Radio Astronomy Observatory, and principal investigator on the project.

"It struck us that dust might be what was preventing us from detecting the molecules in one of the twin protostars," added Chandler.

The astronomers used the VLA to observe a pair of protostars called IRAS 4A, in a star-forming region about 1,000 light-years from Earth. They observed the pair at wavelengths of centimetres.

At those wavelengths, they sought radio emissions from methanol, CH3OH (wood alcohol, not for drinking). This was a pair in which one protostar clearly had a hot corino and the other did not, as seen using the much shorter wavelengths.

The result confirmed their hunch. "With the VLA, both protostars showed strong evidence of methanol surrounding them. This means that both protostars have hot corinos. The reason we did not see the one at shorter wavelengths was because of dust," said Marta de Simone, a graduate student at IPAG who led the data analysis for this object.

The astronomers cautioned that while both hot corinos now are known to contain methanol, there still may be some chemical differences between them. That, they said, can be settled by looking for other molecules at wavelengths not obscured by dust.

"This result tells us that using centimetre radio wavelengths is necessary to properly study hot corinos," Claudio Codella of Arcetri Astrophysical Observatory in Florence, Italy, said.

"In the future, planned new telescopes such as the next-generation VLA and SKA, will be very important to understanding these objects," added Codella.

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