Sunday 25 November 2018

The Kilogram Is Dead. Meet the Kilogram 2.0

The NIST's replica of Le Grand K (front), the international weight that defines a kilogram which is stored in a vault in France. Physical objects will be replaced by Planck's constant as the definition of a kilogram.

For nearly 150 years, the official weight of a kilogram was determined by a shiny cylinder of platinum locked away in a French vault.

The kilogram, like the metre and the second, is one of the seven fundamental units of measurement (also known as the International System of Units or the metric system, the "SI" for short). These were first formalized in the 1875 Treaty of the Metre. Back then, the best way to agree on the weight of a kilogram was to forge a single hunk of metal and call it "Le Grand K." And for more than a century, all scientific scales were calibrated back to that one physical reference point (with copies stored in a dozen countries).

But even solid objects can change over time. When Le Grand K was weighed in the 1980s, it was a couple of micrograms lighter, meaning that all highly accurate scientific scales had to be recalibrated. That's what nerds call a real pain in the mass.

Luckily, teams of metrologists were already on the case (metrology is the science of weights and measures), searching for a universal constant that would generate a fixed value for the kilogram that's true now and a million years from now.

They had already found such a physics fix for the second, which was redefined in 1967 from 1/86,400th of a day to something much more confusing, but constant. It takes 9,192,631,770 oscillations of a special microwave beam to excite atoms of the isotope caesium-133 to a higher energy level. Since that number will never change (unlike the exact length of a day), that's your new second!

Same for the metre. Instead of being defined as the length of a single, meter-long metal pole forged back in 1889, it was redefined in 1983 as the distance light travels in a vacuum in 1/299,792,458th of a second.

It wasn't until 2017 that scientists working at the U.S. National Institute of Standards and Technology (NIST) and similar bodies worldwide finally agreed on a universal constant for the kilogram. The achievement required solving one of the thorniest physics problems of the last century, coming up with a numerical value for Planck's constant.

Without getting too technical, physicist Max Planck proved in 1900 that matter releases energy in discrete chunks called "quanta." His equation for measuring those packets of energy included a constant called h, hitherto known as Planck's constant. Thanks to Einstein, we know that energy and mass are mathematically related, so physicists figured out that Planck's constant (which is a fixed unit of energy) could yield the world's most accurate measurement of mass.

Calculating the exact value of Planck's constant took decades and some serious technological innovation (specifically a nifty device called a Kibble Balance), but now even distracted kindergarteners know that Planck's constant is 6.626070150 × 10^(-34) kg⋅m2/s.

In mid-November, at the annual meeting of the International Bureau of Weights and Measures (BIPM) in Versailles, France, representatives from more than 60 countries voted to approve a new and everlasting definition of the kilogram as calculated by the Planck constant. No more hunk of metal — the kilogram's mass is now tied to Planck's constant. New definitions were also announced for SI units the ampere (electrical current), the kelvin (temperature) and the mole (number of molecules or atoms in an element). These new definitions will take effect on May 20, 2019.

The original platinum kilogram prototype will remain in that underground French vault, while countless generations of scientists make life-changing discoveries using the kilogram 2.0.

Source - EarthSky.org

Why does a full moon look full?

Remember that half the moon is always illuminated by the sun. That lighted half is the moon’s day side.

Technically speaking, the moon is full at the instant it’s 180 degrees from the sun in ecliptic longitude. So why does a full moon look full? Remember that half the moon is always illuminated by the sun. That lighted half is the moon’s day side.

In order to appear full to us on Earth, we have to see the entire day side of the moon. That happens only when the moon is opposite the sun in our sky. So a full moon looks full because it’s opposite the sun.

That’s also why every full moon rises in the east around sunset – climbs highest up for the night midway between sunset and sunrise (around midnight) – and sets around sunrise. Stand outside tonight around sunset and look for the moon. Sun going down while the moon is coming up? That’s a full moon, or close to one.

Just be aware that the moon will look full for at least a couple of night around the instant of full moon.

A full moon is opposite the sun. We see all of its dayside.
If a full moon is opposite the sun, why doesn’t Earth’s shadow fall on the moon at every full moon? The reason is that the moon’s orbit is titled by 5.1 degrees with respect to Earth’s orbit around the sun. At every full moon, Earth’s shadow sweeps near the moon. But, in most months, there’s no eclipse.

A full moon normally passes above or below Earth’s shadow, with no eclipse.
Source - EarthSky.org

Saturday 24 November 2018

14 fascinating physics facts about flakes (of snow)

Every snowflake is a unique marvel of physics, thermodynamics, chemistry, and pure natural beauty. Try to remember that next time you’re shoveling the driveway.


Source - Perimeter Institute