Friday, 8 March 2019

Dinosaurs were thriving before asteroid strike that wiped them out

Artist's concept of asteroid striking Earth 
Dinosaurs were unaffected by long-term climate changes and flourished before their sudden demise by asteroid strike.
Scientists largely agree that an asteroid impact, possibly coupled with intense volcanic activity, wiped out the dinosaurs at the end of the Cretaceous period 66 million years ago.
However, there is debate about whether dinosaurs were flourishing before this, or whether they had been in decline due to long-term changes in climate over millions of years.
Previously, researchers used the fossil record and some mathematical predictions to suggest dinosaurs may have already been in decline, with the number and diversity of species falling before the asteroid impact.
Now, in a new analysis that models the changing environment and dinosaur species distribution in North America, researchers from Imperial College London, University College London and University of Bristol have shown that dinosaurs were likely not in decline before the meteorite.
Lead researcher Alessandro Chiarenza, a PhD student in the Department of Earth Science and Engineering at Imperial, said: "Dinosaurs were likely not doomed to extinction until the end of the Cretaceous, when the asteroid hit, declaring the end of their reign and leaving the planet to animals like mammals, lizards and a minor group of surviving dinosaurs: birds.
"The results of our study suggest that dinosaurs as a whole were adaptable animals, capable of coping with the environmental changes and climatic fluctuations that happened during the last few million years of the Late Cretaceous. Climate change over prolonged time scales did not cause a long-term decline of dinosaurs through the last stages of this period."
The study, published today in Nature Communications, shows how the changing conditions for fossilisation means previous analyses have underestimated the number of species at the end of the Cretaceous.
The team focused their study on North America, where many Late Cretaceous dinosaurs are preserved, such as Tyrannosaurus rex and Triceratops. During this period, the continent was split in two by a large inland sea.
In the western half there was a steady supply of sediment from the newly forming Rocky Mountains, which created perfect conditions for fossilising dinosaurs once they died. The eastern half of the continent was instead characterised by conditions far less suitable for fossilisation.
This means that far more dinosaur fossils are found in the western half, and it is this fossil record that is often used to suggest dinosaurs were in decline for the few million years before the asteroid strike.
Co-author Dr Philip Mannion, from University College London, commented: "Most of what we know about Late Cretaceous North American dinosaurs comes from an area smaller than one-third of the present-day continent, and yet we know that dinosaurs roamed all across North America, from Alaska to New Jersey and down to Mexico."
Instead of using this known record exclusively, the team employed 'ecological niche modelling'. This approach models which environmental conditions, such as temperature and rainfall, each species needs to survive.
The team then mapped where these conditions would occur both across the continent and over time. This allowed them to create a picture of where groups of dinosaur species could survive as conditions changed, rather than just where their fossils had been found.
The team found habitats that could support a range of dinosaur groups were actually more widespread at the end of the Cretaceous, but that these were in areas less likely to preserve fossils.
Furthermore, these potentially dinosaur-rich areas were smaller wherever they occurred, again reducing the likelihood of finding a fossil from each of these areas.

What does the Milky Way weigh? Hubble and Gaia investigate

This illustration shows the fundamental architecture of our island city of stars, the Milky Way galaxy: a spiral disk, central bulge, and diffuse halo of stars and globular star clusters. Not shown is the vast halo of dark matter surrounding our galaxy.
We can't put the whole Milky Way on a scale, but astronomers have been able to come up with one of the most accurate measurements yet of our galaxy's mass, using NASA's Hubble Space Telescope and the European Space Agency's Gaia satellite.
The Milky Way weighs in at about 1.5 trillion solar masses (one solar mass is the mass of our Sun), according to the latest measurements. Only a few percent of this is contributed by the approximately 200 billion stars in the Milky Way and includes a 4-million-solar-mass supermassive black hole at the center. Most of the rest of the mass is locked up in dark matter, an invisible and mysterious substance that acts like scaffolding throughout the universe and keeps the stars in their galaxies.
Earlier research dating back several decades used a variety of observational techniques that provided estimates for our galaxy's mass ranging between 500 billion to 3 trillion solar masses. The improved measurement is near the middle of this range.
"We want to know the mass of the Milky Way more accurately so that we can put it into a cosmological context and compare it to simulations of galaxies in the evolving universe," said Roeland van der Marel of the Space Telescope Science Institute (STScI) in Baltimore, Maryland. "Not knowing the precise mass of the Milky Way presents a problem for a lot of cosmological questions."
The new mass estimate puts our galaxy on the beefier side, compared to other galaxies in the universe. The lightest galaxies are around a billion solar masses, while the heaviest are 30 trillion, or 30,000 times more massive. The Milky Way's mass of 1.5 trillion solar masses is fairly normal for a galaxy of its brightness.
Astronomers used Hubble and Gaia to measure the three-dimensional movement of globular star clusters -- isolated spherical islands each containing hundreds of thousands of stars each that orbit the center of our galaxy.
Although we cannot see it, dark matter is the dominant form of matter in the universe, and it can be weighed through its influence on visible objects like the globular clusters. The more massive a galaxy, the faster its globular clusters move under the pull of gravity. Most previous measurements have been along the line of sight to globular clusters, so astronomers know the speed at which a globular cluster is approaching or receding from Earth. However, Hubble and Gaia record the sideways motion of the globular clusters, from which a more reliable speed (and therefore gravitational acceleration) can be calculated.
The Hubble and Gaia observations are complementary. Gaia was exclusively designed to create a precise three-dimensional map of astronomical objects throughout the Milky Way and track their motions. It made exacting all-sky measurements that include many globular clusters. Hubble has a smaller field of view, but it can measure fainter stars and therefore reach more distant clusters. The new study augmented Gaia measurements for 34 globular clusters out to 65,000 light-years, with Hubble measurements of 12 clusters out to 130,000 light-years that were obtained from images taken over a 10-year period.
When the Gaia and Hubble measurements are combined as anchor points, like pins on a map, astronomers can estimate the distribution of the Milky Way's mass out to nearly 1 million light-years from Earth.
"We know from cosmological simulations what the distribution of mass in the galaxies should look like, so we can calculate how accurate this extrapolation is for the Milky Way," said Laura Watkins of the European Southern Observatory in Garching, Germany, lead author of the combined Hubble and Gaia study, to be published in The Astrophysical Journal. These calculations based on the precise measurements of globular cluster motion from Gaia and Hubble enabled the researchers to pin down the mass of the entire Milky Way.
The earliest homesteaders of the Milky Way, globular clusters contain the oldest known stars, dating back to a few hundred million years after the big bang, the event that created the universe. They formed prior to the construction of the Milky Way's spiral disk, where our Sun and solar system reside.
"Because of their great distances, globular star clusters are some of the best tracers astronomers have to measure the mass of the vast envelope of dark matter surrounding our galaxy far beyond the spiral disk of stars," said Tony Sohn of STScI, who led the Hubble measurements.
The international team of astronomers in this study are Laura Watkins (European Southern Observatory, Garching, Germany), Roeland van der Marel (Space Telescope Science Institute, and Johns Hopkins University Center for Astrophysical Sciences, Baltimore, Maryland), Sangmo Tony Sohn (Space Telescope Science Institute, Baltimore, Maryland), and N. Wyn Evans (University of Cambridge, Cambridge, United Kingdom).
The Hubble Space Telescope is a project of international cooperation between NASA and ESA (European Space Agency). NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore, Maryland, conducts Hubble science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy in Washington, D.C.

Friday, 1 March 2019

Some Facts

Depression is a possible manifestation of vitamin B12 deficiency and may be accompanied by anemia or dementia.

Stroke is a medical condition characterized by interruption of blood flow to the brain, causing a physical or mental handicap. Vitamin B12 deficiencey may increase the risk of stroke among young people who are not otherwise at risk of stroke. Whether or not there is a link is highly controversial, and the risk may result from excess homocysteine levels.

Myelopathy means disease of the spinal cord. Vitamin B12 deficiency causes a type of spine disease called subacute combined degeneration of the spinal cord, which is loss of the protective myelin of certain areas of the spinal cord that control moment, balance and sensation.

Symptoms of subacute combined degeneration of the spinal cord include:

Weakness
Numbness, tingling
Spasticity
Balance problems
Tongue swelling also results from vitamin B12 deficiency. Glossitis is the name used to describe a painful, unusually smooth tongue that can result from this nutritional deficiency.

Associated Conditions
Thyroid disease and multiple sclerosis (MS) are both conditions believed to be related to an autoimmune process. An autoimmune disease is a condition caused by the body attacking itself.

Intrinsic factor deficiency is an autoimmune disease that results from a ‘self’ attack on the region of the stomach that is involved in vitamin B12 absorption. Often, individuals who have thyroid disease or MS also have intrinsic factor deficiency and its associated vitamin B12 deficiency.

SEVEN FACTORS OF INTERNATIONAL HAPPINESS 😉



1. MIG 21 of 1970 vintage took out an F 16, so VLADIMIR PUTIN is very happy.

2. PAF Sherdil Sqn was not flying the Chinese aircraft, so XI JINPING is expressing great relief.

3.  Mirage 2000, the papa ji of Rafael stole the show, so EMANUEL MACRON is reported to be delighted.

4. The Israeli targeting pods 'AN / AAQ-28(V) Litening' on board Mirage worked very well, so BENJAMIN NETANYAHU is feeling overjoyed.

5.  IAF killed those 330 goddam terrorists and gave him a chance to finger General Bajwa and ISI,  so Imran Khan is having the good time of life.

6. Pak Armed Forces were caught pants down, ALI KHAMENEI of Iran and ASHRAF  GHANI of Afghanistan are  reported to be exuberantly cheering.

7. World attention was turned away from USA for 3 days, and no one was cursing its President for the time being, so TRUMP is  indeed delighted.

Therefore today, 1st of March, when Wg Cdr Abhinandan is returning home, the world leaders and PM MODI are proposing  at UN to declare it as INTERNATIONAL HAPPINESS DAY.

😄so my Indians, feel proud & be happy, Jai Hind

War joke






Long time ago Britain and France were at war. During one battle, the French captured an English colonel.
They took him to their headquarters h, and the French General began to question him.
Finally, as an afterthought, the French General asked, "Why do English Officers wear red coats? Don't you know the red material makes you easier targets for us to shoot at?"
In his bland English way, the officer informed the general that the reason British officers wear a red coats is that, if they are shot, the blood won't show, and the men they are leading won't panic."
And that is why, from that day to this, all Pakistani Army Officers wear yellowish brown pants...!!

Novel C. diff structures are required for infection, offer new therapeutic targets

  Iron storage "spheres" inside the bacterium C. diff -- the leading cause of hospital-acquired infections -- could offer new targ...